NASA has dated this image of the Earth to “sometime in 1969” on their Flickr page. What they do know for sure is that it was taken on the Apollo 11 mission – the excursion which sent men to the Moon. And the astronauts completed that goal, as evidenced by this photo clearly snapped from the lunar body.

30. Earth peeking out from behind the Moon

Today's Image of the Day from NASA features the spiral galaxy NGC 2566, which is located 76 million light-years away in the constellation Puppis. The image was captured by the NASA/ESA Hubble Space Telescope.



“A prominent bar of stars stretches across the center of this galaxy, and spiral arms emerge from each end of the bar. Because NGC 2566 appears tilted from our perspective, its disk takes on an almond shape, giving the galaxy the appearance of a cosmic eye,” said <a href="https://phys.org/news/2024-12-hubble-spies-spiral-galaxy-ngc.html" target="_blank" rel="noreferrer noopener">NASA</a>.



“As NGC 2566 appears to gaze at us, astronomers gaze right back, using Hubble to survey the galaxy's star clusters and star-forming regions.”



<h2 class="wp-block-heading" id="h-complex-appearance-of-ngc-2566">Complex appearance of NGC 2566</h2>



NGC 2566 lies at a considerable distance from Earth, making it a challenging object for amateur astronomers to observe in detail without powerful telescopes.&nbsp;



It can be seen in the Southern Hemisphere sky and is better observed from locations with minimal <a href="https://www.earth.com/news/how-light-pollution-influences-interest-in-astronomy/" target="_blank" rel="noreferrer noopener">light pollution</a>.&nbsp;



The galaxy's arms are populated with young, bright stars, regions of active star formation, and interstellar gas and dust - giving it a dynamic and complex appearance.



<h2 class="wp-block-heading" id="h-measuring-the-ages-of-stars">Measuring the ages of stars</h2>



According to NASA, data from Hubble is especially valuable for studying stars that are just a few million years old. “These stars are bright at the ultraviolet and visible wavelengths to which Hubble is sensitive.”



“Using these data, researchers can measure the ages of NGC 2566's stars, which helps piece together the timeline of the galaxy's star formation and the exchange of gas between star-forming clouds and the stars themselves.”



<h2 class="wp-block-heading" id="h-star-formation-in-galaxies">Star formation in galaxies</h2>



Star formation in <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">galaxies</a> is a fascinating and complex process that unfolds over millions of years. It begins in vast clouds of gas and dust, known as molecular clouds, which are often found in the spiral arms of galaxies or in regions of irregular or starburst galaxies.&nbsp;



These clouds provide the raw material for star formation, consisting primarily of hydrogen and helium, with trace amounts of heavier elements.



As the molecular clouds collapse under their own gravity, regions within them begin to condense and fragment, forming dense clumps. Within these clumps, protostars emerge. Their formation is driven by the gravitational pull drawing in surrounding gas.&nbsp;



During this process, the gas heats up due to increasing pressure, eventually igniting nuclear fusion in the core, signaling the birth of a new star.



<h2 class="wp-block-heading" id="h-rate-of-star-formation-nbsp-across-galaxies">Rate of star formation&nbsp;across galaxies</h2>



The rate of star formation varies across galaxies is influenced by numerous factors. In spiral galaxies like the Milky Way, star formation is most active in the spiral arms, where density waves compress gas and dust, triggering the collapse of molecular clouds.&nbsp;



Elliptical galaxies, which often have little cold gas and dust, typically exhibit low rates of star formation or none at all.



Starburst galaxies, on the other hand, experience episodes of exceptionally high star formation, often triggered by <a href="https://www.earth.com/news/webb-captures-a-galaxy-collision-with-a-radiant-smile/">galactic collisions</a> or interactions. 



These events can funnel large amounts of gas into central regions, leading to intense star-forming activity. However, such bursts are usually short-lived on cosmic timescales, exhausting the available gas quickly.



The environment within a galaxy also plays a significant role. Stellar winds and supernova explosions from existing stars can both inhibit and promote star formation. They may disperse gas, preventing further collapse, or compress nearby clouds, triggering new star formation.&nbsp;



Over time, as galaxies evolve, the availability of gas diminishes, leading to a gradual decline in star formation activity.



<h2 class="wp-block-heading" id="h-the-puppis-constellation-nbsp">The Puppis constellation&nbsp;</h2>



The Puppis constellation in the southern sky represents the stern of a ship. It was once part of a larger constellation known as Argo Navis, which depicted the mythical ship of Jason and the Argonauts.&nbsp;



However, Argo Navis was later divided into three separate constellations: Puppis, Carina (the keel), and Vela (the sails). Puppis is the largest of these three and contains many notable celestial objects.



This constellation is home to several bright stars, including Naos (Zeta Puppis), a hot, massive star that emits intense ultraviolet radiation. Puppis also hosts a wide variety of deep-sky objects, such as open <a href="https://www.earth.com/news/stunning-star-clusters-captured-in-the-extreme-outskirts-of-the-milky-way/" target="_blank" rel="noreferrer noopener">star clusters</a> and nebulae.&nbsp;



Among these, Messier 46 and Messier 47 stand out. Both are beautiful star clusters that are visible through binoculars or small telescopes. The region is dense with stars because it lies along the <a href="https://www.earth.com/news/milky-way-collision-may-change-everything-we-know-about-our-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>, making it a prime area for stargazing and astrophotography. 



Image Credit: NASA



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A cosmic eye in the Puppis constellation

Today's Image of the Day from NASA features the spiral...

Today's Image of the Day from NASA Earth Observatory features a satellite view of retreating glaciers in Alaska, where meltwater is rapidly expanding glacial lakes. 



“In parts of Alaska, water is replacing ice. As glaciers thin and <a href="https://www.earth.com/news/satellite-images-reveal-hidden-retreat-of-arctic-glaciers/" target="_blank" rel="noreferrer noopener">retreat</a>, meltwater collects at their fronts, forming proglacial lakes. According to an analysis by Mauri Pelto, a glaciologist at Nichols College, three such lakes in the southeastern part of the state have grown rapidly in recent decades,” said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



<h2 class="wp-block-heading" id="h-retreating-glaciers-in-alaska">Retreating glaciers in Alaska</h2>



“A trio of glaciers - Yakutat, Alsek, and Grand Plateau - descend from inland mountains and flow onto the coastal plain southeast of Yakutat borough, ending at Harlequin Lake, Alsek Lake, and Grand Plateau Lake,” noted NASA.&nbsp;



The retreat of the glaciers, as well as the growth of the lakes, are visible in the image. When compared to an <a href="https://eoimages.gsfc.nasa.gov/images/imagerecords/153000/153638/fastestlake_tm5_19840705_lrg.jpg" target="_blank" rel="noreferrer noopener">image</a> captured by Landsat 5 in the summer of 1984, the changes are even more evident.



NASA elaborated on the extent of the glacier retreat from 1984 to 2024. “During this period, Yakutat Glacier’s main arm retreated 4.3 miles, while Alsek Glacier’s northern and southern arms retreated 3.3 miles and 3.4 miles, respectively. Grand Plateau Glacier’s northern arm lost the most, retreating 4.8 miles.”



<h2 class="wp-block-heading" id="h-glacial-lakes-doubled-in-size-nbsp">Glacial lakes doubled in size&nbsp;</h2>



“Collectively, the three lakes more than doubled in size over 40 years. In 1984, they covered about 50 square miles. By 2024, they spanned 90 square miles. That’s an area larger than Seneca Lake (67 square miles) - one of the Finger Lakes in New York, which also have a glacial origin,” said NASA.



Pelto noted that the lakes forming in this region are immense - starting at the mountains and spreading toward the coast - making this a new lake district that is unique in our nation.



“Millions of other lakes, named and unnamed, dot the state. But this system has grown fast, so much so that Pelto thinks it might represent the fastest lake growth in the United States this century,” said NASA.



<h2 class="wp-block-heading" id="h-understanding-glacier-retreat-nbsp">Understanding glacier retreat&nbsp;</h2>



Glacier retreat is a significant phenomenon driven primarily by global warming the results from rising greenhouse gas <a href="https://www.earth.com/news/global-carbon-dioxide-emissions-hit-a-record-high-in-2023/" target="_blank" rel="noreferrer noopener">emissions</a>.&nbsp;



As temperatures rise, glaciers lose more ice during the summer melt than they can regain in winter snowfall, causing them to shrink over time. This process has profound implications for ecosystems, water resources, and global sea levels.



<h3 class="wp-block-heading" id="h-glacial-lakes">Glacial lakes</h3>



When glaciers retreat, they often leave behind depressions in the landscape that can fill with meltwater, forming glacial lakes. These lakes are typically bounded by natural dams made of rock, ice, or moraine - accumulations of debris left behind by the glacier's movement.&nbsp;



Over the past century, the number and size of glacial lakes worldwide have increased significantly due to the accelerating pace of <a href="https://www.earth.com/news/tropical-glaciers-offer-a-glimpse-of-our-harsh-climate-reality/" target="_blank" rel="noreferrer noopener">glacier</a> retreat. This trend is especially evident in high-altitude regions like the Himalayas, the Andes, and the Alps, as well as in polar areas such as Alaska and Greenland.



<h3 class="wp-block-heading" id="h-positive-and-negative-impacts-nbsp">Positive and negative impacts&nbsp;</h3>



Glacial lakes can have both positive and negative impacts. They provide critical water sources for downstream communities, support biodiversity, and sometimes offer opportunities for hydropower development or tourism.&nbsp;



However, they also pose serious risks. The dams holding back these lakes can fail suddenly, causing glacial lake outburst floods (GLOFs). These catastrophic events can devastate downstream areas, destroying infrastructure, agricultural lands, and habitats while endangering human lives.



<h3 class="wp-block-heading" id="h-monitoring-changes">Monitoring changes</h3>



Understanding glacier retreat and glacial lake formation requires a multidisciplinary approach, combining climate science, hydrology, and geology.&nbsp;



Monitoring these changes is essential to mitigate associated risks and adapt to the evolving landscape shaped by a <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fperu-has-lost-over-half-of-its-glaciers-in-six-decades%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">warming planet</a>.



<h2 class="wp-block-heading" id="h-glacier-retreat-worldwide">Glacier retreat worldwide</h2>



Studies and satellite observations show that most glaciers in almost all regions of the world are shrinking.&nbsp;



Melting glaciers contribute significantly to global <a href="https://www.earth.com/news/emergency-meeting-reveals-the-alarming-extent-of-antarcticas-ice-loss/" target="_blank" rel="noreferrer noopener">sea level rise</a>, which threatens coastal communities and ecosystems.



The retreat of glaciers is considered one of the clearest indicators of climate change.&nbsp;Some glaciers are retreating at unprecedented rates, indicating accelerating climate impacts.



The image was captured on August 4, 2024 by the Landsat 8 satellite.



Image Credit: NASA Earth Observatory



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Retreating glaciers and expanding meltwater lakes in Alaska

Today's Image of the Day from NASA Earth Observatory features...

Today's Image of the Day from NASA Earth Observatory features the Costa Atlántica Reserve stretching along the Atlantic coast in Argentina.



“At the far southern reaches of South America, a stretch of tidal flats, shoals, and beaches serves as a refuge for migratory shorebirds and copious aquatic life,” said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



“The Costa Atlántica Reserve in Argentina extends for 220 kilometers (140 miles) along the eastern shore of Tierra del Fuego. The area was designated a Ramsar site in 1995 and a provincial nature reserve in 1998." 



According to NASA, the reserve is the southernmost site both on the Ramsar list and in the Western Hemisphere Shorebird Reserve Network.



<h2 class="wp-block-heading" id="h-significance-of-the-costa-atlantica-reserve">Significance of the Costa Atlántica Reserve</h2>



The Costa Atlántica Reserve is an important conservation site that signifies Argentina's commitment to preserving its rich <a href="https://www.earth.com/news/human-induced-changes-in-ocean-salinity-threaten-biodiversity-and-marine-ecosystems/" target="_blank" rel="noreferrer noopener">coastal biodiversity</a>.&nbsp;



This vast expanse of protected area serves as a sanctuary for many species, ranging from migratory birds to marine mammals and diverse plant life.



“Tidal habitats along the coast support some 135 species of birds, while crustaceans, mollusks, fish, and cetaceans feed in the productive coastal waters,” said NASA.&nbsp;



“The topography inland of Costa Atlántica, stretching into Chile to the west, is blanketed in shrubs and grassland vegetation adapted to dry conditions - part of a semiarid ecosystem known as the Fuegian steppe.”



<h2 class="wp-block-heading" id="h-maintaining-ecological-balance-nbsp">Maintaining ecological balance&nbsp;</h2>



Established to safeguard the delicate ecosystems of dunes, estuaries, and <a href="https://www.earth.com/news/coastal-lagoons-have-high-loads-of-microplastics/" target="_blank" rel="noreferrer noopener">coastal lagoons</a>, the reserve plays a crucial role in maintaining ecological balance.&nbsp;



The Costa Atlántica Reserve provides critical habitats for numerous threatened species, including the <a href="https://www.earth.com/news/southern-right-whales-have-shifted-their-foraging-grounds/">Southern Right Whale</a>, which finds refuge in these waters during its breeding season. 



The reserve’s sheltered bays and nutrient-rich waters create an ideal environment for mothers to nurse their calves before embarking on long migrations. 



In addition to whales, the reserve supports populations of sea lions and Magellanic penguins. Its protection is vital for the long-term survival of these species in the face of climate change and human activity.



<h2 class="wp-block-heading" id="h-costa-atlantica-reserve-a-living-laboratory-nbsp">Costa Atlántica Reserve: A living laboratory&nbsp;</h2>



The Costa Atlántica Reserve is not only a refuge for wildlife but also a living laboratory for scientific research. 



Conservationists and researchers work within its bounds to monitor ecosystems, study species behaviors, and develop strategies for sustainable management. 



This ongoing research is pivotal in understanding the impacts of climate change on <a href="https://www.earth.com/news/coastal-river-deltas-face-major-threats-beyond-climate-change/" target="_blank" rel="noreferrer noopener">coastal environments</a> and in devising measures to mitigate these effects.



Furthermore, the reserve illustrates the importance of community involvement in conservation efforts. Local communities are engaged in sustainable tourism and educational programs.&nbsp;



Through <a href="https://www.earth.com/news/how-bird-photographers-improve-nesting-success/" target="_blank" rel="noreferrer noopener">eco-tourism</a> initiatives, visitors can experience the natural beauty of the reserve while contributing to its preservation.



<h2 class="wp-block-heading" id="h-tierra-del-fuego-archipelago">Tierra del Fuego archipelago</h2>



According to NASA, the broader landscape of the Tierra del Fuego archipelago was shaped by glaciers.&nbsp;



“Ice advanced over the mountains and lowlands during cold climatic periods between the mid-Pleistocene, about 1 million years ago, and the Last Glacial Maximum, about 20,000 years ago. San Sebastián Bay formed in a tectonic depression that was deepened by glacial erosion," noted NASA.&nbsp;



“Further evidence of glaciation, including hummocky moraines and fields of glacial erratics, appears around the bay, though it is too small to be visible in this image.”



“Partially enclosed by a long, sandy peninsula, San Sebastián Bay attracts copious migratory birds, some of which shuttle seasonally between the Northern and Southern Hemispheres.”



“Large populations of the Hudsonian godwit, white-rumped sandpiper, and other long-distance flyers congregate in the vast intertidal zones. This part of the reserve, however, is vulnerable to the impact of oil and gas extraction from onshore and offshore deposits.”



The image was captured on February 20, 2024 by the <a href="https://landsat.gsfc.nasa.gov/satellites/landsat-9/landsat-9-instruments/oli-2-design/" target="_blank" rel="noreferrer noopener">OLI-2</a> (Operational Land Imager-2) on Landsat 9.



Image Credit: NASA Earth Observatory&nbsp;



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Costa Atlántica Reserve in Argentina

Today's Image of the Day from NASA Earth Observatory features an explosive eruption of Mount Etna, the most active volcano in Europe. The photo was captured on February 13 by the OLI (Operational Land Imager) on the Landsat 8 satellite.



<a href="https://earthobservatory.nasa.gov/images/153962/river-of-fire-on-mount-etna" target="_blank" rel="noreferrer noopener">NASA</a> noted that the natural-color scene is overlaid with an infrared signal to distinguish the lava’s heat signature on the mountain's snowy slopes.



<h2 class="wp-block-heading" id="h-signs-of-unrest">Signs of unrest</h2>



“On February 8, 2025, Italy’s National Institute of Geophysics and Volcanology (INGV) reported that Mount Etna had begun exhibiting ‘signs of unrest above its background level,’”&nbsp;said NASA.



“That’s unsurprising for the frequently unruly Sicilian peak, one of the most active stratovolcanoes in the world. But the fiery explosions, disruptive ash clouds, and long lava flows that ensued stood out as being unusually spectacular to many Etna watchers.”



<h2 class="wp-block-heading" id="h-intensifying-eruptions-on-mount-etna">Intensifying eruptions on Mount Etna </h2>



The activity intensified on February 10th, with lava flowing from the Bocca Nuova crater at an altitude of approximately 3,000 meters above sea level.&nbsp;



According to news reports, the eruption created a striking visual as molten lava traversed the snow-covered slopes, producing rivers of lava up to 3 kilometers long and emitting ash plumes visible from several kilometers away.



The <a href="https://www.earth.com/news/new-research-enhances-predictions-on-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">volcanic activity</a> attracted thousands of tourists eager to witness the spectacle. However, the influx of visitors led to traffic congestion, obstructing emergency services and prompting warnings from local authorities about the potential dangers of approaching the active volcano.



<h2 class="wp-block-heading" id="h-impacts-of-mount-etna-eruptions">Impacts of Mount Etna eruptions </h2>



Despite the dramatic displays, there were no reports of injuries or significant property damage, though experts continue to closely monitor the situation.



Satellite imagery has provided detailed views of the active lava flow cutting through the snow-covered slopes, with ash plumes dispersing from the summit.



“The presence of ash prompted authorities to raise the aviation color code to orange on February 13. On other days during this eruption, it was elevated to red, the highest level of concern. The airport in nearby Catania diverted flights amid hazardous conditions, according to news reports,” said NASA.



“Since Etna stirred to life this time around, crowds of hikers and even some skiers flocked to its slopes to witness the fiery displays and lava flows melting through snow. The eruption was ongoing as of February 18, with weak ash emissions and decreasing explosive activity.”



<h2 class="wp-block-heading" id="h-a-volcano-with-a-long-history">A volcano with a long history </h2>



Mount Etna has a history stretching back hundreds of thousands of years. Located on the east coast of Sicily, near Catania, the volcano has shaped the landscape and influenced human civilization.



The volcano’s activity dates back at least 500,000 years, with its earliest eruptions occurring beneath the sea before the landmass emerged. Over time, lava flows, <a href="https://www.earth.com/news/yellowstone-supervolcano-eruption-study-sparks-new-debate-on-where-and-when-it-will-erupt/" target="_blank" rel="noreferrer noopener">eruptions</a>, and collapses have sculpted the towering stratovolcano seen today.



Ancient civilizations were well aware of Etna’s power. Greek mythology depicted it as the forge of Hephaestus, the god of fire, while the poet Pindar described its violent eruptions. The philosopher Empedocles was even said to have perished in its fiery depths.&nbsp;



Etna’s eruptions were documented throughout Roman history, including a major event in 122 BC that devastated Catania.



During the Middle Ages and Renaissance periods, Etna continued its eruptions, frequently altering its landscape and affecting nearby settlements.&nbsp;



<h2 class="wp-block-heading" id="h-monitoring-the-activity-of-mount-etna">Monitoring the activity of Mount Etna </h2>



One of the most devastating eruptions occurred in 1669, when lava flows destroyed several villages and overwhelmed parts of Catania’s city walls. Despite these dangers, people continued to live and farm on Etna’s fertile slopes, taking advantage of its rich volcanic soil.



Scientific study of Mount Etna began in the 19th and 20th centuries, as researchers sought to understand its behavior and mitigate its risks. Advances in monitoring technology have since helped track its activity, though eruptions remain unpredictable.&nbsp;



In modern times, Etna continues to be one of the most closely watched <a href="https://www.earth.com/news/axial-seamount-large-underwater-volcano-off-us-coast-will-likely-erupt-in-2025/" target="_blank" rel="noreferrer noopener">volcanoes</a> in the world, with frequent eruptions, ash clouds, and lava flows affecting air travel and local communities.



Mount Etna was designated a UNESCO World Heritage Site in 2013 due to its geological significance and cultural history.&nbsp;



Today, the <a href="https://www.earth.com/news/earths-next-big-volcano-eruption-will-cause-global-chaos-climate-impact/" target="_blank" rel="noreferrer noopener">volcano</a> attracts tourists, scientists, and locals alike, serving as both a reminder of nature’s power and a source of economic and scientific interest.



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Fiery eruption of Mount Etna captured from space

Today's Image of the Day from the European Space Agency features NGC 1333, a reflection nebula located in the Perseus molecular cloud about 960 light-years away from Earth. The photo is a mosaic of images captured by the James Webb Space Telescope.



<h2 class="wp-block-heading" id="h-the-power-of-webb-nbsp-nbsp">The power of Webb&nbsp;&nbsp;</h2>



“Webb’s superb sensitivity allows astronomers to investigate young objects with extremely low masses. Some of the faintest ‘stars’ in the picture are in fact newly born free-floating brown dwarfs with masses comparable to those of giant planets,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



The same cluster was featured as the 33rd anniversary image of the Hubble Space Telescope in April 2023.&nbsp;



According to ESA, Hubble’s image just scratched the surface of this region, because clouds of dust obscure much of the star formation process. 



"Observing with larger aperture and in the infrared part of the spectrum, Webb is capable of peering through the dusty veil to reveal newborn stars, brown dwarfs and planetary mass objects."



<h2 class="wp-block-heading" id="h-webb-s-view-of-ngc-1333">Webb’s view of NGC 1333</h2>



ESA noted that the center of the image presents a deep peek into the heart of the NGC 1333 cloud. 



“Across the image we see large patches of orange, which represent gas glowing in the infrared. These so-called Herbig-Haro objects form when ionized material ejected from young stars collides with the surrounding cloud. They are hallmarks of a very active site of star formation."



The disks of gas and dust that surround the <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">stars</a> in this image may eventually produce planetary systems.&nbsp;



<h2 class="wp-block-heading" id="h-formation-of-the-sun">Formation of the Sun</h2>



“Similar to the young stars in this mosaic, our own Sun and planets formed inside a dusty molecular cloud, 4.6 billion years ago. Our Sun did not form in isolation but as part of a cluster, which was perhaps even more massive than NGC 1333,” explained ESA.



Over time, the stars in the Sun's birth cluster would have drifted apart due to gravitational interactions and the dispersion of gas in the region.



Astronomers have been studying certain clues, such as isotopic signatures in meteorites, that hint the Sun may have formed near massive stars. These stars likely produced supernovae, which could have influenced the early <a href="https://www.earth.com/news/mysterious-objects-spotted-in-the-outer-solar-system-beyond-pluto/" target="_blank" rel="noreferrer noopener">solar system</a> by injecting heavy elements like iron-60.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1333">Star formation in NGC 1333</h2>



NGC 1333 is a vibrant example of a stellar nursery, where active <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> is ongoing. It is known for its chaotic appearance, shaped by the interactions between newborn stars and the surrounding material.



Within NGC 1333, astronomers have observed a high level of turbulence, which makes the region dynamic and complex. 



These disturbances are caused by the outflows of young stars as they eject material into their surroundings, creating shock waves and influencing further star formation.&nbsp;



These outflows are often seen as jets, which are visible in multiple wavelengths of light, especially infrared, as the surrounding dust absorbs visible light.



<h2 class="wp-block-heading" id="h-significance-of-ngc-1333">Significance of NGC 1333</h2>



NGC 1333 is also an area of interest for studying the early stages of star and <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planet formation</a>, as many of the stars within the cluster are in their infancy, still in the process of gathering material and developing protoplanetary disks.&nbsp;



In images, NGC 1333 is marked by bright patches of blue and red, representing reflection <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/" target="_blank" rel="noreferrer noopener">nebulae</a> and the ionized gas created by energetic young stars.&nbsp;



<h2 class="wp-block-heading" id="h-the-perseus-molecular-cloud-nbsp">The Perseus molecular cloud&nbsp;</h2>



The Perseus molecular cloud is a vast region of cold gas and dust located about 600 light-years away from Earth in the constellation <a href="https://www.earth.com/news/1500-billion-orphan-stars-discovered-in-the-perseus-galaxy-cluster/" target="_blank" rel="noreferrer noopener">Perseus</a>.&nbsp;



It is one of the most studied star-forming regions in our galaxy due to its relative proximity and the diversity of its young stellar objects. This cloud spans several hundred light-years and contains dense pockets of gas where new stars are actively forming.&nbsp;



These areas are often enshrouded in thick dust, which obscures them in visible light but allows astronomers to study them using infrared and radio wavelengths.



The Perseus molecular cloud is particularly interesting because of the chemistry taking place within it, including the formation of complex organic molecules that could be precursors to life.&nbsp;



Image Credit: ESA/Webb, NASA &amp; CSA



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Stellar nursery shines in the Perseus cloud

Today's Image of the Day from the European Space Agency...

Today's Image of the Day from NASA Earth Observatory features smoke streaming from Tasmania, where bushfires were ignited by dry lightning strikes earlier this month.&nbsp;



By February 5, more than a dozen fires were burning in the state's remote central and western regions.



<h2 class="wp-block-heading" id="h-bushfires-fueled-by-challenging-conditions">Bushfires fueled by challenging conditions </h2>



Communities such as Zeehan, Corinna, and Pieman Heads have been threatened, leading to evacuations and significant disruptions during the peak tourism season.



“In early February 2025, bushfires ignited in northwestern Tasmania, where they have continued to burn on the island for more than a week amid windy, warm, and dry conditions,” said <a href="https://earthobservatory.nasa.gov/images/153933/smoke-billows-from-bushfires-in-tasmania" target="_blank" rel="noreferrer noopener">NASA</a>.



“Smoke from the fires is visible in this image, acquired at about 4 p.m. local time on February 12, 2025, by the MODIS (Moderate Resolution Imaging Spectroradiometer) instrument on NASA’s Aqua satellite.”



<h2 class="wp-block-heading" id="h-impacts-of-the-tasmania-bushfires">Impacts of the Tasmania bushfires</h2>



The <a href="https://www.earth.com/news/wildfires-threaten-the-recovery-of-the-ozone-layer/" target="_blank" rel="noreferrer noopener">fires</a> have burned over 90,000 hectares, with a combined perimeter exceeding 1,200 kilometers.



The fires are expected to continue burning for several more weeks. Due to the region's remote and challenging terrain, authorities report that significant effort is still needed to gain control over the blazes.



“According to a heatwave warning from Australia’s Bureau of Meteorology (BoM), much of the state’s west coast saw severe heatwave conditions on several days during the week of February 10,” noted NASA.



“The region has also been exceptionally dry. For example, the past 12-month period has been the driest on record (since 1900) along the coastal areas near Sandy Cape.”



<h2 class="wp-block-heading" id="h-cultural-and-heritage-sites">Cultural and heritage sites</h2>



One significant area under threat is the takayna/Tarkine region in northwest Tasmania. This region is home to a grove of ancient Huon pine trees, including one estimated to be between 2,500 and 3,000 years old, making it the oldest known Huon pine.&nbsp;



The Yellowband Plain fire has burned perilously close to this grove, coming within meters of these irreplaceable trees.



Firefighters from Tasmania, interstate, and New Zealand are collaborating to control the blazes and help protect the Huon pine trees, as well as Indigenous heritage sites. 



Efforts to assess and mitigate the damage have been hampered by challenging weather conditions, including low cloud cover that restricts aerial surveys. Strong winds of up to 50 miles per hour have also complicated efforts to contain the bushfires.&nbsp;



<h2 class="wp-block-heading" id="h-climate-change-is-intensifying-bushfires-nbsp">Climate change is intensifying bushfires&nbsp;</h2>



Climate change and bushfires are deeply interconnected, with rising global temperatures intensifying the frequency and severity of wildfires in many regions.&nbsp;



Warmer temperatures lead to drier conditions, reducing moisture in vegetation and making it more susceptible to ignition. Prolonged droughts - which are becoming more common due to climate change - further dry out forests and grasslands, creating an abundance of flammable material.



Extreme heat waves increase the likelihood of fires starting and spreading rapidly. Higher temperatures also contribute to stronger winds, which can fan flames and carry embers over long distances, igniting new fires. 



Additionally, shifting <a href="https://www.earth.com/news/ultrafine-particles-in-wildfire-smoke-change-weather-patterns/" target="_blank" rel="noreferrer noopener">weather patterns</a> are altering fire seasons, making them longer and more unpredictable. Some areas that previously had clear fire seasons are now experiencing fires year-round.



<h2 class="wp-block-heading" id="h-shifting-behavior-of-wildfires-nbsp">Shifting behavior of wildfires&nbsp;</h2>



Climate change is also affecting the way bushfires behave. Many recent wildfires have been more intense, burning hotter and <a href="https://www.earth.com/news/fast-wildfires-are-gaining-even-more-speed/" target="_blank" rel="noreferrer noopener">spreading faster</a> than historical fires. This makes them harder to control and increases their impact on communities, ecosystems, and wildlife. 



The destruction of forests not only contributes to immediate carbon emissions but also reduces the planet’s ability to absorb carbon dioxide, creating a feedback loop that worsens climate change.



<h2 class="wp-block-heading" id="h-consequences-of-increased-fire-activity">Consequences of increased fire activity</h2>



Beyond the direct effects on landscapes and air quality, increased bushfire activity has severe consequences for <a href="https://www.earth.com/news/wildfire-smoke-is-an-underestimated-threat-to-public-health/" target="_blank" rel="noreferrer noopener">human health</a>, economies, and biodiversity. 



Smoke from large wildfires contains fine particles that can cause respiratory problems and other health issues, even for people far from the fire zones.&nbsp;



Wildlife struggles to escape or recover from habitat destruction, sometimes pushing species closer to extinction.



<h2 class="wp-block-heading" id="h-mitigating-the-risks">Mitigating the risks</h2>



Efforts to mitigate these risks include better fire management strategies, improved early <a href="https://www.earth.com/news/bushfires-are-detected-500-times-faster-with-ai-satellites/" target="_blank" rel="noreferrer noopener">warning systems</a>, and sustainable land-use practices. 



However, long-term solutions require addressing the root cause - reducing greenhouse gas emissions to slow down global warming.&nbsp;



Without significant action, climate change will continue to fuel more extreme and destructive bushfires, with devastating consequences for both nature and society.



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Tasmania bushfires: A growing crisis in an era of climate change

Today's Image of the Day from NASA Earth Observatory features an astronaut view of Mount Nemrut, a volcano located in eastern Turkey near Lake Van.



Mount Nemrut is notable for its immense caldera, which was formed through a series of <a href="https://www.earth.com/news/volcanic-eruptions-play-an-overlooked-role-in-earths-climate/" target="_blank" rel="noreferrer noopener">eruptions</a>. The caldera, one of the largest in the world, now contains several lakes such as Lake Nemrut.&nbsp;



"The eastern half of the caldera is partially filled by solidified lava flows from past eruptions. Snow cover present at the time of this photo accentuates pressure ridges that formed as the lava was flowing and cooling," noted <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



"These pressure ridges vary in size, thickness, and orientation due to the varying viscosity and flow direction of the lavas during eruptions."



<h2 class="wp-block-heading" id="h-formation-of-lake-nemrut">Formation of Lake Nemrut</h2>



"Lake Nemrut (Nemrut Gölü) occupies the western half of the caldera, creating a rough crescent shape that partially submerges the old lava flows," said NASA.



"This freshwater lake, reaching up to 176 meters deep, is accompanied by a smaller lake at the upper-center of the caldera."



The lake was formed after the collapse of the Nemrut volcano's summit. This collapse created a massive crater, which gradually filled with water over time, forming the <a href="https://www.earth.com/news/alarming-study-most-of-the-worlds-largest-lakes-are-quickly-losing-water/" target="_blank" rel="noreferrer noopener">lake</a>.



<h2 class="wp-block-heading" id="h-unesco-world-heritage-site">UNESCO World Heritage Site </h2>



Mount Nemrut and its surroundings are part of a protected UNESCO World Heritage Site due to their ecological and geological significance.



The site is home to diverse wildlife, including various bird species that use the lake as a stopover during migration. The caldera also contains smaller lakes and wetlands, adding to the area's biodiversity.



Lake Nemrut is a popular destination for tourists, hikers, and nature enthusiasts, offering stunning views of the volcanic landscape.



Despite its popularity, the lake remains relatively remote and unspoiled, contributing to its appeal as a natural wonder.



<h2 class="wp-block-heading" id="h-mount-nemrut-has-shaped-the-landscape">Mount Nemrut has shaped the landscape</h2>



Geologically, Mount Nemrut is interesting because its <a href="https://www.earth.com/news/new-research-enhances-predictions-on-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">eruptions</a> have played a key role in shaping the local landscape. 



Its last major eruption occurred around 1441 AD, which indicates that it's not currently active.



The area around Nemrut is known for its geothermal activity, including hot springs and fumaroles, suggesting that there is still significant heat beneath the surface.



<h2 class="wp-block-heading" id="h-tribute-to-a-king">Tribute to a king</h2>



Over thousands of years, various civilizations have inhabited the region around Nemrut, leaving behind a wealth of archaeological sites.



The summit of Mount Nemrut is dominated by a vast funerary mound constructed by King Antiochus I Theos, who ruled the Kingdom of Commagene in the 1st century BCE. 



The site was intended to serve as his tomb sanctuary and a place to commemorate the king's vision of divine kingship and unity between Eastern and Western cultures.



The mound, made of loose crushed stones, measures about 50 meters (164 feet) in height and spans a diameter of 150 meters (492 feet), creating an imposing feature visible from afar.



Surrounding the mound are terraces on the eastern, western, and northern sides, each adorned with colossal statues and reliefs. The statues, ranging in height from 8 to 10 meters (26 to 33 feet), represent various deities, including Zeus, Apollo, Hercules, and the goddess Tyche, alongside King Antiochus himself. 



The heads of the statues, many of which have toppled over due to <a href="https://www.earth.com/news/new-map-shows-75-percent-of-the-u-s-at-risk-of-damaging-earthquakes/" target="_blank" rel="noreferrer noopener">earthquakes</a> and erosion, lie scattered around the site.



<h2 class="wp-block-heading" id="h-spiritual-and-religious-practices">Spiritual and religious practices</h2>



In addition to the statues, inscriptions at Mount Nemrut provide valuable historical information about the kingdom, the king's lineage, and the religious practices of the time.



The site is not only a marvel of ancient engineering but also a spiritual and astronomical center. Scholars believe the terraces were aligned with celestial events, serving as an observatory for solstices and equinoxes.



In addition to its natural and historical significance, the Nemrut volcano has been the subject of scientific study, as researchers aim to understand more about <a href="https://www.earth.com/news/volcanic-eruptions-play-an-overlooked-role-in-earths-climate/" target="_blank" rel="noreferrer noopener">volcanic activity</a> in the region, the history of its eruptions, and the potential risks it may pose in the future.



Image Credit: NASA Earth Observatory



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Mount Nemrut: Ancient mysteries and natural marvels 

Today's Image of the Day from NASA Earth Observatory features La Niña, a global climate event that is expected to be short-lived.



The map represents sea surface height anomalies on January 13, 2025 across the central and eastern Pacific Ocean.&nbsp;



“Shades of blue indicate sea levels that were lower than average, while shades of red indicate areas where the ocean stood higher than normal. Normal sea level conditions appear in white,” noted <a href="https://earthobservatory.nasa.gov/images/153917/la-nina-is-here" target="_blank" rel="noreferrer noopener">NASA</a>.



<h2 class="wp-block-heading" id="h-the-onset-of-la-nina-nbsp">The onset of La Niña&nbsp;</h2>



According to the National Oceanic and Atmospheric Administration (NOAA), sea surface temperatures in the east-central equatorial Pacific dropped below average in December 2024, marking the onset of La Niña. This cooling pattern has persisted into early 2025.



NOAA's Climate Prediction Center indicates a 59% chance that La Niña conditions will continue through February-April 2025, with a likely transition to ENSO-neutral conditions during March-May 2025.



“After seven months of waiting, La Niña - the cooler sister of El Niño - finally showed up in the eastern Pacific Ocean in early December 2024. La Niña may not stick around long, though,” said NASA.



<h2 class="wp-block-heading" id="h-what-is-la-nina">What is La Niña?</h2>



La Niña is a phase of the El Niño-Southern Oscillation (ENSO) cycle that occurs when strengthened easterly trade winds enhance the upwelling of cooler water from the depths of the eastern tropical Pacific.&nbsp;



This process leads to a significant cooling of surface waters in the central and eastern Pacific near the equator. The intensified trade winds also drive warm equatorial waters westward toward Asia and Australia.&nbsp;



“This dramatic cooling of the ocean’s surface layers affects the atmosphere by modifying the moisture content across the Pacific,” explained NASA.



“In a report published on January 9, 2025, the NOAA Climate Prediction Center confirmed that La Niña conditions were present. They measured sea surface temperatures 0.7 degrees Celsius (1.3 degrees Fahrenheit) below average in an area of the tropical Pacific, from 170° to 120° West longitude, known as the Niño 3.4 region.”



“The signature of La Niña is also visible in the central and eastern Pacific Ocean as areas of lower-than-average water levels. That’s because cooler water contracts, lowering sea levels. (Conversely, warmer water expands, raising them).”&nbsp;



<h2 class="wp-block-heading" id="h-la-nina-forecast-nbsp">La Niña forecast&nbsp;</h2>



Josh Willis, an oceanographer and Sentinel-6 Michael Freilich project scientist at JPL, pointed out that although La Niña is here, it’s not a particularly strong one.



Willis noted that during an especially strong La Niña in 2010-2011, temperatures in the tropical Pacific were about 1.6°C (2.9°F) below average in January 2011, compared to just 0.7°C (1.3°F) below average in January 2025.&nbsp;



NOAA predicts that this La Niña will remain weak and is unlikely to drop below -1°C from the average - the threshold for a moderate-strength event. Neutral conditions are expected to return during the meteorological spring.



La Niña’s interaction between the ocean and atmosphere alters global atmospheric circulation, shifting mid-latitude jet streams in ways that can intensify rainfall in some regions and cause drought in others.&nbsp;



In the western Pacific, Indonesia and Australia may experience increased rainfall. The central and eastern Pacific is expected to experience reduced cloud cover and precipitation, leading to drier conditions in Brazil, Argentina, and other parts of South America. Meanwhile, Central America may see wetter conditions.&nbsp;



<h2 class="wp-block-heading" id="h-"></h2>



In North America, La Niña typically brings cooler, stormier weather to the Pacific Northwest, while the southern United States and northern Mexico tend to experience warmer, drier conditions.



<h2 class="wp-block-heading" id="h-natural-source-of-variability">Natural source of variability</h2>



“ENSO adds a natural source of year-to-year variability in global temperatures. Because such a wide swath of the Pacific is cold, La Niña tends to keep a lid on the average global surface temperature,” explained NASA.



“But even the cool water in the Pacific does not completely offset long-term warming trends; some of the hottest years on record have coincided with La Niña, such as in 2010 and 2020.”



The map is based on data that was acquired by the Sentinel-6 Michael Freilich satellite and processed by scientists at NASA’s Jet Propulsion Laboratory (JPL).&nbsp;



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La Niña has arrived - but it may not stay for long

The MODIS instrument, short for Moderate Resolution Imaging Spectroradiometer, is a key instrument aboard the Terra and Aqua satellites. MODIS is playing a vital role in the development of Earth ecosystem models, able to predict global changes, which then assist policy makers in making informed decisions about the protection of the global environment.

Heavy snow and cloud cover in the Alps are seen in this Image of the day&nbsp;from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at heavy snow and low clouds in the Alps. Wildlife such as ibex live in the higher peaks to elevations of 3,400 m (11,155 ft), and plants such as Edelweiss grow in rocky areas in lower elevations as well as in higher elevations.

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

Aqua is a NASA scientific research satellite that studies precipitation, evaporation, and water cycles. Terra and Aura make up the Earth Observing System. It's the second component of the system.

A frozen Lake Erie in February Today’s Image of the Day comes from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at a frozen <a href="https://www.earth.com/image/icy-lake-erie/">Lake Erie</a>, which is currently 93.3 percent iced over. A frozen Lake Erie in February
This false-color image was created using data from the Moderate Resolution Imaging Spectroradiometer (MODIS) on board the Aqua satellite to differentiate between snow, ice, and clouds.
Lake Erie /ˈɪəri/ (French: Lac Érié) is the fourth-largest lake (by surface area) of the five Great Lakes in North America, and the eleventh-largest globally if measured in terms of surface area.It is the southernmost, shallowest, and smallest by volume of the Great Lakes and therefore also has the shortest average water residence time. At its deepest point Lake Erie is 210 feet (64 metres) deep. 
Situated on the International Boundary between Canada and the United States, Lake Erie&#8217;s northern shore is the Canadian province of Ontario, specifically the Ontario Peninsula, with the U.S. states of Michigan, Ohio, Pennsylvania, and New York on its western, southern, and eastern shores. These jurisdictions divide the surface area of the lake with water boundaries. 
The lake was named by the Erie people, a Native American people who lived along its southern shore. The tribal name &#8220;erie&#8221; is a shortened form of the Iroquoian word erielhonan, meaning long tail
&#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Image Credit: <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>

A frozen Lake Erie in February

Aqua Earth Observing Satellite

This beautiful photo gallery contains 50 incredible images of Earth from Space. These images were taken by astronauts onboard the International Space Station, as well as by a multitude of NASA satellites orbiting the earth.

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a> and features a look at Super Typhoon Noru in the Pacific Ocean just south of <a href="https://www.earth.com/news/first-blue-chrysanthemums-created/">Japan</a>.
This image was captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite on July 31, 2017. 
At the time the photo was taken, Typhoon Noru was located just 250 kilometers south of Iwo Jima. Maximum sustained winds hit 150 miles per hour.
The storm briefly became a category 5 on July 30, before being downgraded to a category 4 one day later.
&#8211;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a>

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

Photos from the International Space Station are found in this awesome Earth.com image gallery. Flat-earthers won't agree, but these incredible photos of the Earth were taken by astronauts onboard the International Space Station. The International Space Station is a modular space station in low Earth orbit.

Northern Italy from the space station is seen here in this Image of the Day from the <a href="http://www.esa.int/">European Space Agency</a> (ESA). The view includes the top half of the Italian Peninsula, along with <a href="https://www.earth.com/image/wildfires-burn-northern-corsica/">Corsica</a> and Sardinia off the coast. This image was captured by ESA astronaut Paolo Nespoli on his third and final mission to the Space Station.

Northern Italy from the Space Station

Photos from the International Space Station

Fossils newly unearthed in southeastern Australia have upended long-held assumptions about dinosaur evolution, revealing the world’s oldest known megaraptorid and the first confirmed evidence of carcharodontosaurs on the continent.&nbsp;



These discoveries paint a vivid picture of an unusual predator hierarchy that once roamed the region during the Early Cretaceous, adding a crucial piece to the puzzle of dinosaur history.



The research was carried out by a team led by <a href="https://museumsvictoria.com.au/research-institute/">Museums Victoria Research Institute</a> and <a href="https://www.monash.edu/">Monash University</a> PhD student Jake Kotevski.&nbsp;



The study focused on five <a href="https://www.earth.com/news/large-theropod-dinosaurs-thrived-in-polar-environments/">theropod</a> fossils found along Victoria’s coastline. They were collected in the upper Strzelecki (Bass Coast, dating back roughly 121.4–118 million years) and the Eumeralla Formation (Otway Coast, about 113–108 million years old).



<h2 class="wp-block-heading" id="h-dinosaurs-thriving-in-australia-nbsp">Dinosaurs thriving in Australia&nbsp;</h2>



The newly studied remains suggest an unexpected arrangement of carnivorous dinosaurs. They indicate that large megaraptorids - measuring between six and seven meters long - coexisted alongside smaller carcharodontosaurs that reached only two to four meters in length, as well as the agile, meter-long unenlagiines (nicknamed “southern raptors”). 



This stands in stark contrast to better-known ecosystems where carcharodontosaurs typically surpassed other predatory dinosaurs in size.



“The discovery of carcharodontosaurs in Australia is groundbreaking,” Kotevski said. “It’s fascinating to see how Victoria’s predator hierarchy diverged from South America, where carcharodontosaurs reached <a href="https://www.earth.com/news/t-rex-was-about-70-percent-bigger-than-we-thought/">Tyrannosaurus rex</a>-like sizes up to 13 metres, towering over megaraptorids. Here, the roles were reversed, highlighting the uniqueness of Australia’s Cretaceous ecosystem.”



Two of the newly identified fossils rank among the earliest megaraptorids known worldwide, prompting experts to reconsider their evolutionary timeline.&nbsp;



Because these megaraptorids thrived in Australia at such an early date, they may have played a more pivotal role in Gondwanan <a href="https://www.earth.com/news/new-predatory-dinosaur-species-identified-in-lost-photos/">predator</a> communities than previously recognized.



<h2 class="wp-block-heading" id="h-new-clues-about-dinosaur-migration-nbsp">New clues about dinosaur migration&nbsp;</h2>



According to Dr. Thomas Rich, senior curator of vertebrate palaeontology at Museums Victoria Research Institute, the fossils also hint at broader patterns of dinosaur dispersal in the Southern Hemisphere.&nbsp;



He noted that the findings not only expand Australia’s theropod fossil record but offer compelling evidence of faunal interchange between Australia and South America through Antarctica during the Early Cretaceous.&nbsp;



“The findings also challenge previous assumptions about body-size hierarchies in Gondwanan predator ecosystems highlighting Victoria’s unique <a href="https://www.earth.com/news/extraordinary-dinosaur-fossils-discovered-from-the-end-of-cretaceous-era/">Cretaceous</a> fauna,” xplained Dr. Rich.



These links to other Gondwanan regions bolster the theory that dinosaurs and other animals migrated between connected landmasses before shifting continents isolated certain populations.&nbsp;



Over time, such isolation could have led to distinct paths of <a href="https://www.earth.com/news/dinosaurs-evolved-feathers-for-much-more-than-just-flying/">evolutionary development</a>, explaining why Australian megaraptorids, rather than carcharodontosaurs, occupied the apex predator niche.



<h2 class="wp-block-heading" id="h-significance-of-museum-collections">Significance of museum collections </h2>



Beyond revealing hidden chapters of Australia’s dinosaur history, the study demonstrates the significance of museum collections in fueling new scientific breakthroughs. 



Researchers often depend on carefully preserved fossils that can remain unclassified for decades, awaiting fresh analytical methods or new comparative specimens before their true importance is revealed.



“Museum collections are crucial to advancing our understanding of prehistoric life,” said Tim Ziegler, the vertebrate palaeontology collection manager at Museums Victoria Research Institute.&nbsp;



“Specimens preserved in the State Collection for decades - unidentifiable until now - are providing new insights into the evolution of dinosaur ecosystems.”



The project also illustrates a longstanding tradition of mentorship, continuity, and collaboration among palaeontologists. Senior curator Dr. Rich, at Museums Victoria since 1974, has worked with multiple generations of researchers.&nbsp;



These efforts culminate in cutting-edge studies like Kotevski’s PhD research, forming a chain of inquiry that steadily advances what we know about ancient life.



<h2 class="wp-block-heading" id="h-volunteers-in-the-field">Volunteers in the field</h2>



Three of the fossils in this study were first identified between 2022 and 2023 by a Museums Victoria volunteer, Melissa Lowery, demonstrating the critical role that community members play in paleontology.&nbsp;



With an eye for intriguing shapes and textures, volunteers often detect clues that lead to major discoveries.



Kotevski and his colleagues continue to search for additional remains at key sites, including the location where the large megaraptorid was found.&nbsp;



These expeditions form part of the long-running <a href="http://dinosaurdreaming.monash.edu/">Dinosaur Dreaming project</a>, responsible for uncovering over 10,000 fossils - from dinosaurs and birds to mammals and marine reptiles - since it began.&nbsp;



Each new bone or tooth refines scientists’ understanding of the richly varied ecosystems that existed on Australia’s ancient coastlines.



<h2 class="wp-block-heading" id="h-dinosaurs-of-cretaceous-australia">Dinosaurs of Cretaceous Australia</h2>



Unusual for reversing the roles typically observed in other continents, Victoria’s predator lineage helps paleontologists envision a world where megaraptorids reigned supreme while smaller carcharodontosaurs prowled in their shadow.&nbsp;



By confirming that early megaraptorids inhabited the region and that carcharodontosaurs were present yet less dominant, these fossils challenge orthodox views on predator size hierarchies and evolutionary pathways within Gondwana.



As fieldwork continues, each new fragment of bone has the potential to reshape our perspective on how dinosaurs spread across the prehistoric southern supercontinent, adapted to different environments, and carved out ecological niches.&nbsp;



Together, the fossils detail a singular evolutionary story that sets Cretaceous Australia apart, forever changing how we see the era’s predatory power dynamics - and offering fresh directions for future discoveries.



Image Credit: Artwork by Jonathan Metzger. Source: Museums Victoria



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Fossils discovered in Australia rewrite dinosaur history

Fossils newly unearthed in southeastern Australia have upended long-held assumptions...

Male fruit flies buzzing around in a small, contained arena sounds like a pretty ordinary science experiment. Yet one group of researchers noticed something unusual about how some of them reacted to a spinning disk.



They observed that while many flies stayed away from the disk, a select few hopped onto it and stayed for surprising amounts of time. 



<a href="https://sciprofiles.com/profile/2253355" target="_blank" rel="noreferrer noopener">Dr. Wolf Huetteroth</a> from the <a href="https://www.uni-leipzig.de/en" target="_blank" rel="noreferrer noopener">University of Leipzig</a> notes that these findings could open new questions about how body awareness develops in living creatures.



<h2 class="wp-block-heading" id="h-flies-spin-with-purpose">Flies spin with purpose</h2>



Many people think of fruit flies as tiny <a href="https://www.earth.com/news/insects-fruit-flies-smell-well-as-humans-with-much-less-nose-neurons/" target="_blank" rel="noreferrer noopener">creatures</a> flitting around fruit bowls. Yet a recent study suggests that they might show optional behavior patterns that fit the definition of play. This observation challenges old assumptions about insects.



“Using several carousels, we generated and analyzed a total of around seven years of film data,” says Dr. <a href="https://www.researchgate.net/profile/Tilman-Triphan" target="_blank" rel="noreferrer noopener">Tilman Triphan</a>, the first author of the study. 



Researchers used several rotating platforms placed under a thin glass cover. Some flies dashed to the edge, but others returned to the carousel again and again.&nbsp;



<h2 class="wp-block-heading" id="h-individual-preferences">Individual preferences</h2>



A fraction of the <a href="https://www.earth.com/news/fruit-flies-on-treadmills-video-shows-how-insects-walk-and-balance/" target="_blank" rel="noreferrer noopener">flies</a> sought the disk and rode it in repeated sessions. Those individuals spent extended periods on the spinner, while their peers avoided it altogether. The behavior looked deliberate, rather than forced or random.



One aspect was the difference in how these seekers got onto the spinning surface. 



“However, we were able to distinguish whether the flies had deliberately walked onto the carousel or jumped onto it in an uncoordinated way. This allowed us to show that unplanned visits to the carousel were rather atypical for the playing flies,” says co-author <a href="https://www.northumbria.ac.uk/about-us/our-staff/f/clara-ferreira/" target="_blank" rel="noreferrer noopener">Dr. Clara H. Ferreira</a>, an assistant Professor at <a href="https://www.northumbria.ac.uk/" target="_blank" rel="noreferrer noopener">Northumbria University</a>.



<h2 class="wp-block-heading" id="h-possible-value-of-body-sense">Possible value of body sense</h2>



The repeated interaction with the moving disk seems to involve <a href="https://journals.physiology.org/doi/full/10.1152/physrev.00048.2011" target="_blank" rel="noreferrer noopener">proprioceptive feedback</a>, which refers to the body’s sense of position and motion.



If some flies are actively seeking the extra sensation, it might be fulfilling a hidden benefit. This is reminiscent of how certain mammals, like <a href="https://pubmed.ncbi.nlm.nih.gov/9861614/" target="_blank" rel="noreferrer noopener">rats</a>, engage in rough-and-tumble routines that refine their coordination.



Some insects ended up swapping mealtime for more spins on the carousel. That trade-off hints at a possible reward gained from the turning <a href="https://www.earth.com/news/dragonflies-develop-waxy-coating-to-withstand-warmer-climates/" target="_blank" rel="noreferrer noopener">motion</a>. 



The interesting part is that these insects showed no direct advantage other than what seems to be playful amusement.



<h2 class="wp-block-heading" id="h-flies-spin-by-choice-not-force">Flies spin by choice, not force</h2>



Natural curiosity is often observed in higher animals, but insects rarely get credit for it. 



Here, the setting was calm, with continuous observation over days to capture genuine conduct. There were no artificial triggers that forced the flies onto the disk.



The team set up the environment to ensure no threat forced the flies to remain. If the spinning platform caused anxiety, they could easily walk away. 



Instead, some made a personal choice to return. This self-directed action adds weight to the suggestion of a real <a href="https://www.earth.com/news/flies-are-more-vulnerable-to-climate-change-than-bees/" target="_blank" rel="noreferrer noopener">playful attitude</a>.



<h2 class="wp-block-heading" id="h-why-does-it-matter-for-humans">Why does it matter for humans?</h2>



“This could help us to find out how we humans also develop efficient self-awareness of our bodies,” says Huetteroth. 



The clue lies in how the spinning motion may sharpen the brain’s ability to map physical space. Because the flies appear to seek out extra movement, they might be training themselves to adapt and respond to unexpected motion.



Similar responses appear in many species that enjoy roller coasters or spinning rides. Researchers believe the <a href="https://www.earth.com/news/how-human-brain-connects-unrelated-concepts-through-reasoning/" target="_blank" rel="noreferrer noopener">brain learns</a> from these experiences, reinforcing internal models of balance and orientation.



If a small insect displays a version of this, it might show that the drive to engage in such activity evolved long ago.



<h2 class="wp-block-heading" id="h-flies-spin-despite-easy-alternatives">Flies spin despite easy alternatives</h2>



The flies had easy access to food and water. They also had corners to rest without interruption. Despite these calmer options, some crawled over for a spin. 



That behavior did not enhance survival, which points toward a motivational factor besides hunger or fear.



Scientists have used <a href="https://pubmed.ncbi.nlm.nih.gov/5787388/" target="_blank" rel="noreferrer noopener">open-field tests</a> to measure caution or stress in animals. 



Usually, creatures stay near edges when anxious. The carousel-seeking flies, however, went to the center and stayed. This breaks usual fear-driven patterns.



<h2 class="wp-block-heading" id="h-what-happens-next">What happens next?</h2>



So far, scientists have only glimpsed how fruit flies pick between exploration, feeding, and spinning. The genetic tools available in fruit <a href="https://www.earth.com/news/chemicals-are-changing-insects-in-subtle-yet-deadly-ways/" target="_blank" rel="noreferrer noopener">flies</a> might shine more light on the neural wiring behind this playful bent. 



Perhaps targeted genetic studies will uncover exactly which circuits reward them for spinning.



In time, deeper understanding could reveal ways that controlled motion shapes a creature’s internal map. 



That concept might prove relevant to other animals, including humans learning how to handle complex movement or interactive environments.



The study is published in <a href="https://www.cell.com/current-biology/fulltext/S0960-9822(25)00055-7?_returnURL=https%3A%2F%2Flinkinghub.elsevier.com%2Fretrieve%2Fpii%2FS0960982225000557%3Fshowall%3Dtrue" target="_blank" rel="noreferrer noopener">Current Biology</a>.



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Flies like to play and have fun like other animals, according to a fascinating new study

Male fruit flies buzzing around in a small, contained arena...

Scientists have devised an affordable way to permanently remove carbon dioxide from the atmosphere by converting common minerals into highly reactive substances that spontaneously lock away CO2. 



This breakthrough could play a critical role in curbing global warming by addressing one of its primary causes.



The new technique was developed by chemists at <a href="https://www.stanford.edu/">Stanford University</a> Matthew Kanan, a professor of chemistry and senior author of the paper, explained the motivation behind the carbon capture research.



“The Earth has an inexhaustible supply of <a href="https://www.earth.com/news/chinas-rare-earth-jackpot-1-15-million-tons-of-minerals-uncovered/">minerals</a> that are capable of removing CO2 from the atmosphere, but they just don’t react fast enough on their own to counteract human greenhouse gas emissions. Our work solves this problem in a way that we think is uniquely scalable.”



<h2 class="wp-block-heading" id="h-rapid-carbon-removal-with-new-chemistry">Rapid carbon removal with new chemistry </h2>



In nature, silicate minerals gradually bind with CO2 through <a href="https://www.earth.com/news/natural-rock-weathering-is-a-co2-source-comparable-to-volcanoes/">weathering</a>, forming stable carbonates over hundreds or thousands of years.&nbsp;



Researchers worldwide have long sought methods to accelerate this slow process, often referred to as enhanced weathering. 



Kanan and Stanford postdoctoral scholar Yuxuan Chen found a way to make silicates rapidly absorb carbon, thanks to what Chen describes as a “new chemistry.”



“We envisioned a new chemistry to activate the inert silicate minerals through a simple ion-exchange reaction,” said Chen, who led the lab work. “We didn’t expect that it would work as well as it does.”



By speeding up mineral reactions that would otherwise unfold over centuries, this approach has the potential to remove significant amounts of <a href="https://www.earth.com/news/how-carbon-dioxide-travels-in-the-atmosphere/">carbon dioxide</a> from the air in a fraction of the time.



<h2 class="wp-block-heading" id="h-more-efficient-mineral-transformation">More efficient mineral transformation</h2>



Existing carbon removal strategies - such as direct <a href="https://www.earth.com/news/capturing-carbon-directly-from-the-air-is-now-much-more-efficient-thanks-to-new-material/">air capture</a> - often rely on energy-intensive equipment, including large fans, chemicals, and other methods to filter out CO2. They can be both costly and difficult to scale. In contrast, the Stanford scientists point to the energy savings of their approach.



“Our process would require less than half the energy used by leading direct air capture technologies, and we think we can be very competitive from a cost point of view,” said Kanan, who is also a senior fellow at the <a href="https://energy.stanford.edu/" target="_blank" rel="noreferrer noopener">Precourt Institute for Energy</a> in the Stanford Doerr School of Sustainability.



In their experiments, the team heated limestone (calcium carbonate) in a kiln to produce calcium oxide, then combined this material with silicate minerals containing magnesium.&nbsp;



When the two substances were heated together, they exchanged ions and yielded magnesium oxide and calcium silicate - both of which readily take up carbon from the air.



“The process acts as a multiplier,” Kanan noted. “You take one reactive mineral, calcium oxide, and a magnesium silicate that is more or less inert, and you generate two reactive minerals.”



<h2 class="wp-block-heading" id="h-trapping-carbon-with-simple-chemistry">Trapping carbon with simple chemistry </h2>



<a href="https://www.earth.com/news/new-crack-resistant-cement-material-inspired-by-nature/">Cement</a> manufacturers have used kilns for centuries, processing limestone at high temperatures to create key ingredients for concrete. The Stanford method adapts this time-tested approach but substitutes part of the cement mixture with magnesium silicates.



When these newly formed minerals are exposed to water and carbon dioxide - even at the relatively low concentrations found in ambient air - they spontaneously convert CO2 into stable carbonates.&nbsp;



Laboratory tests showed that wet samples of magnesium oxide and calcium silicate could trap carbon in weeks to months, far outpacing natural weathering.



“You can imagine spreading magnesium oxide and calcium silicate over large land areas to remove CO2 from ambient air,” Kanan said.&nbsp;



“One exciting application that we’re testing now is adding them to agricultural soil. As they weather, the minerals transform into bicarbonates that can move through the soil and end up permanently stored in the ocean.”



<h2 class="wp-block-heading" id="h-potential-benefits-for-farmers">Potential benefits for farmers</h2>



Soil treatments commonly include calcium carbonate (lime) to raise pH when it is too acidic. In principle, farmers could switch to these new reactive minerals instead of conventional lime.&nbsp;



“Adding our product would eliminate the need for liming, since both mineral components are alkaline,” Kanan explained.&nbsp;



“In addition, as calcium silicate weathers, it releases silicon to the soil in a form that the plants can take up, which can improve crop yields and resilience. Ideally, farmers would pay for these minerals because they’re beneficial to farm productivity and the health of the soil - and as a bonus, there’s the carbon removal.”



<h2 class="wp-block-heading" id="h-scaling-up-for-global-impact">Scaling up for global impact</h2>



According to Kanan’s team, ramping up production to a meaningful scale would require converting millions of tons of silicate minerals each year.&nbsp;



“Each year, more than 400 million tons of mine tailings with suitable silicates are generated worldwide, providing a potentially large source of raw material,” Chen said.&nbsp;



“It’s estimated that there are more than 100,000 gigatons of olivine and serpentine reserves on Earth, enough to permanently remove far more CO2 than humans have ever emitted.”



<h2 class="wp-block-heading" id="h-nature-s-carbon-solution">Nature's carbon solution</h2>



After factoring in emissions from heating kilns using natural gas or <a href="https://www.earth.com/news/biofuels-may-eliminate-90-of-black-smoke-emissions-from-cars/">biofuel</a>, the researchers estimate that each ton of their final material can remove one ton of CO2 from the atmosphere.&nbsp;



For context, fossil fuel emissions of carbon dioxide surpassed 37 billion tons in 2024, demonstrating the pressing need for large-scale solutions.



“Society has already figured out how to produce billions of tons of cement per year, and cement kilns run for decades,” Kanan said. “If we use those learnings and designs, there is a clear path for how to go from lab discovery to carbon removal on a meaningful scale.”



Work is also underway to develop electric-powered kilns in collaboration with electrical engineering associate professor Jonathan Fan. 



If successful, this innovation could reduce or eliminate the carbon footprint of the heating process, further boosting the climate benefits.



By combining well-established industrial methods with a novel chemical reaction, this approach could offer a promising and relatively low-cost way to draw down billions of tons of CO2 from the atmosphere - and help mitigate the accelerating effects of climate change.



The study is published in the journal <a href="http://dx.doi.org/10.1038/s41586-024-08499-2">Nature</a>.



Image Credit: Renhour48 via Wikimedia



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Common rocks turned into great carbon trappers with new technology

Scientists have devised an affordable way to permanently remove carbon...

Stars are born in dense clouds of gas and dust, but new evidence suggests that conditions in the early universe may have shaped their formation in surprising ways.&nbsp;



In a recent study, observations of the Small Magellanic Cloud (SMC) revealed that about 40% of the star-forming clouds in this distant dwarf galaxy exhibit a “fluffy” shape.&nbsp;



This discovery potentially alters our understanding of how many stars - similar to our own Sun - came into being.



<h2 class="wp-block-heading" id="h-star-formation-across-cosmic-history">Star formation across cosmic history </h2>



The research was led by Kazuki Tokuda, a postdoctoral fellow at <a href="https://www.kyushu-u.ac.jp/en/" target="_blank" rel="noreferrer noopener">Kyushu University</a>’s Faculty of Science. The findings may shed new light on the evolution of star formation across cosmic history.



In the <a href="https://www.earth.com/news/milky-ways-black-hole-unleashes-mysterious-flares/">Milky Way</a> today, stars generally form within elongated, filamentary molecular clouds.&nbsp;



Astronomers believe our own Solar System originated in such a structure, where a large filament broke apart into smaller cores - often called “stellar eggs.” 



Over hundreds of thousands of years, gravity pulled gas into each core to forge a new star.



<h2 class="wp-block-heading" id="h-conditions-of-the-early-universe">Conditions of the early universe</h2>



Tokuda noted that our understanding of star formation is still developing, and comprehending how <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/" target="_blank" rel="noreferrer noopener">stars formed</a> in the earlier universe is even more challenging. 



“The early universe was quite different from today, mostly populated by hydrogen and helium. Heavier elements formed later in high-mass stars," explained Tokuda.



"We can’t go back in time to study star formation in the early universe, but we can observe parts of the universe with environments similar to the early universe.”



The Small Magellanic Cloud meets these conditions. It lies about 20,000 light-years from Earth - very close by cosmic standards - and contains only one-fifth the <a href="https://www.earth.com/news/hungry-white-dwarf-stars-eat-heavy-metals/">heavy elements</a> (sometimes called “metals” by astronomers) found in the Milky Way.&nbsp;



This makes the SMC an excellent proxy for conditions that would have been prevalent around 10 billion years ago, when the universe itself contained fewer heavy elements.



<h2 class="wp-block-heading" id="h-observing-fluffy-molecular-clouds">Observing fluffy molecular clouds </h2>



Despite the SMC’s usefulness, it has proven challenging to gather high-resolution data on its star-forming regions. 



Astronomers need to distinguish whether filaments - like those that give rise to stars in the Milky Way - also exist in the SMC, or if some entirely different process might govern star formation there.



Fortunately, new observations from the ALMA radio telescope in Chile offered the resolution needed to analyze molecular clouds in the Small Magellanic Cloud. 



“In total, we collected and analyzed data from 17 molecular clouds. Each of these molecular clouds had growing baby stars 20 times the mass of our Sun,” Tokuda said.&nbsp;



“We found that about 60% of the molecular clouds we observed had a filamentary structure with a width of about 0.3 light-years, but the remaining 40% had a ‘fluffy’ shape. Furthermore, the temperature inside the filamentary molecular clouds was higher than that of the fluffy molecular clouds.”



Higher temperatures in the filamentary clouds appear to reflect a more recent formation. After their initial collisions, these clouds start off relatively hot, with weak turbulence.&nbsp;



As the gas cools, the incoming energy from further collisions creates increased turbulence, which can smooth out the filamentary structure - resulting in the “fluffy” clouds that Tokuda’s team observed.



<h2 class="wp-block-heading" id="h-colossal-star-forming-factories">Colossal star-forming factories</h2>



The shift from filamentary to fluffy shapes could have profound implications for the stars that eventually emerge. If the filaments remain intact, they tend to fragment along their lengths, producing many stars (some of them low-mass stars like the Sun).&nbsp;



On the other hand, if the clouds lose their structure too quickly and become fluffy, the formation of these stellar cores may be disrupted, potentially affecting how many Sun-like stars (and planetary systems) can form.



The difference in temperature between filamentary and fluffy clouds is likely linked to their age. Initially, all molecular clouds formed as filamentary structures with high temperatures, primarily due to the impact of cloud collisions. In this heated state, turbulence within the cloud remains weak.&nbsp;



However, as the cloud cools over time, the kinetic energy from incoming gas increases turbulence, gradually breaking down the filamentary structure and transforming it into a more diffuse, fluffy cloud.



Such differences highlight the importance of heavy elements in stabilizing molecular clouds - elements that play a key role in radiative cooling and help regulate the dynamics within these colossal star-forming factories.&nbsp;



“This study indicates that the environment, such as an adequate supply of heavy elements, is crucial for maintaining a filamentary structure and may play an important role in the formation of planetary systems,” Tokuda added.



<h2 class="wp-block-heading" id="h-mysteries-of-star-formation">Mysteries of star formation </h2>



Given that heavy elements were far scarcer in the <a href="https://www.earth.com/news/red-monsters-challenge-what-we-know-about-the-early-universe/">early universe</a>, these findings hint that many primordial stars might have formed under conditions more akin to the “fluffy” clouds in the SMC. That scenario could alter our perspective on the first generations of stars and the overall evolution of galaxies in the cosmos.



“In the future, it will be important to compare our results with observations of molecular clouds in heavy-element-rich environments, including the Milky Way galaxy. Such studies should provide new insights into the formation and temporal evolution of molecular clouds and the universe,” Tokuda said.



Whether filamentary or fluffy, molecular clouds remain at the heart of one of astronomy’s greatest questions: How, and under what circumstances, do stars emerge?&nbsp;



By studying the SMC and beyond, researchers aim to map out these stellar birthplaces more completely, revealing how different cosmic eras might have shaped the countless stars that fill our skies today.



The study is published in <a href="http://dx.doi.org/10.3847/1538-4357/ada5f8">The Astrophysical Journal</a>.



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‘Fluffy’ molecular clouds may change our understanding of star formation

Stars are born in dense clouds of gas and dust,...

Flowers that lose their initial charm often end up in the trash. This might seem normal when the petals wither, yet many of these blooms are still valuable.



Scientists are exploring opportunities to use edible varieties of these flowers. They are checking their nutrients, flavors, and possible effects on food quality and shelf life.



“Rose flowers are still going to be rose flowers on Valentine’s Day. But we are looking at what happens the day after Valentine’s Day to those flowers,” said Anand Mohan, associate professor in UGA’s College of Agricultural and Environmental Sciences.



Some flowers offer natural pigments that could replace synthetic colorants. Others contain antioxidants and proteins that might strengthen nutritional content in everyday meals.



Flowers with broad petals sometimes carry protective compounds that can guard meats, cereals, or even beverages against spoilage. These qualities are drawing attention in food science.



<h2 class="wp-block-heading" id="h-the-promise-of-ultrasound">The promise of ultrasound</h2>



Researchers highlight that ultrasound waves help process many foods with less time and resource use. They also see the potential for ultrasound to extend a flower’s <a href="https://www.earth.com/news/food-waste-crisis-why-u-s-goals-remain-out-of-reach/" target="_blank" rel="noreferrer noopener">usability</a> beyond a typical bouquet’s lifespan.



Ultrasound equipment works by sending waves into the material. Those waves move water away more efficiently and release beneficial compounds locked inside the petals.



When handled properly, this low-frequency technology can disrupt cell walls and let colorants, proteins, and vitamins flow into a solution. Once extracted, these compounds can be turned into powders or liquids.



Ultrasound may open up new <a href="https://www.earth.com/news/your-freezer-can-play-a-key-role-in-reducing-food-waste/" target="_blank" rel="noreferrer noopener">prospects</a> for turning leftover petals into color boosters or dietary enhancements. This shift could reduce waste and get more mileage out of every bloom.



<h2 class="wp-block-heading" id="h-flower-petals-as-food-ingredients">Flower petals as food ingredients</h2>



“We are trying to use edible flowers as a source of protein, food colorant and vitamins,” said Mohan. 



Some species of broccoli flowers have protein content that can be blended into cereals. Others, like hibiscus, yield a vibrant color that can replace artificial dyes.



Much of the effort involves pinpointing the right flower for the right purpose. Roses might suit meat preservation, while marigolds might fit as an ingredient in certain sauces.



Scientists also look at how different varieties thrive in changing climates. The goal is to identify flowers that stay strong and maintain a steady supply for the food <a href="https://www.earth.com/news/digital-labels-help-grocers-cut-food-waste/" target="_blank" rel="noreferrer noopener">market</a>.



<h2 class="wp-block-heading" id="h-balancing-flavor-and-shelf-life">Balancing flavor and shelf life</h2>



Edible flowers might shift taste profiles. Some bring a delicate note, while others contribute a mild bitterness or herbal kick.



Preserving these flowers isn’t always easy. Traditional drying can be slow and may destroy color and aroma.



Hot air drying often leads to a dimmer petal hue. Ultrasound pretreatment shortens drying time and cuts the browning that heat can trigger.



The result is a dried ingredient that can be crushed or powdered. This form is simple to ship and store, making it perfect for large-scale food production.



<h2 class="wp-block-heading" id="h-keeping-color-intact">Keeping color intact</h2>



Many edible flowers get their bright appearance from anthocyanins or other plant chemicals. Heat can degrade these compounds, turning a vibrant petal into a dull one.



Ultrasound can reduce this risk by aiding quick water removal and limiting direct high-heat exposure. It also stalls enzymes like polyphenol oxidase, which spark browning.



A mild ultrasound phase maintains crucial pigments. The finished product retains most of its original shade.



Manufacturers see this as a bonus since vibrant natural colors attract consumers who want fewer artificial additives.



<h2 class="wp-block-heading" id="h-extracting-beneficial-compounds">Extracting beneficial compounds</h2>



Beyond color, certain petal extracts carry valuable antioxidants that can guard against cell damage in the body. Ultrasound helps release these compounds into a friendly solvent.



Shorter extraction times mean less chance of thermal stress. This helps safeguard delicate vitamins or volatile oils.



Blue butterfly pea flower is one example. Studies show ultrasound extraction can bolster its antioxidant content while preserving its bright blue color.



Manufacturers can incorporate these concentrates into teas or juices. They gain both natural coloring and potential health perks in one go.



<h2 class="wp-block-heading" id="h-other-advanced-techniques">Other advanced techniques</h2>



Microwave drying is another approach that rapidly heats petals. While quick, it can cause uneven heat distribution that may damage fragile flowers.



Infrared drying works at lower temperatures and keeps more nutrients intact. Its reach is shallower, so thicker petals might need extra time.



Ionizing radiation shows promise for sterilizing edible flowers. Yet consumer perception around radiation remains skeptical.



Ultrasound stands out for its mild thermal impact, which protects fragile compounds and saves energy. It has its own set of hurdles, but the results are enticing enough to keep it in the spotlight.



<h2 class="wp-block-heading" id="h-safe-consistent-results">Safe, consistent results</h2>



Ultrasound tools can be loud. The process involves intense vibrations that could affect hearing if workers aren’t shielded or if machines aren’t set up properly.



High-powered waves might also damage petal tissues if misused. Researchers must find the ideal treatment for each flower type.



The scale of production equipment is another factor. Small labs produce small batches, but bigger systems must ensure even coverage. Careful regulation of wave intensity and duration is essential for safe, consistent results.



<h2 class="wp-block-heading" id="h-turning-flowers-into-food-products">Turning flowers into food products</h2>



Companies in the beverage sector can look into floral extracts that add aroma or color. Start-ups might explore using leftover wedding or holiday flowers as raw material.



Supermarkets that toss out unsold blooms could partner with local facilities to transform them into new products. This idea saves money and reduces <a href="https://www.earth.com/news/what-age-group-is-responsible-for-the-most-food-waste/" target="_blank" rel="noreferrer noopener">trash</a>.



Shoppers might soon see ready-to-use flower powders or meal-ready petals in store aisles. The next step involves marketing that resonates with people looking for color and flavor without synthetic additives.



Many chefs are already known for edible petals on plates. Scaling this practice for everyday consumers is the bigger challenge.



<h2 class="wp-block-heading" id="h-edible-flowers-can-reduce-waste">Edible flowers can reduce waste</h2>



Flowers are grown year-round and shipped worldwide, but not all get purchased. Food scientists are pointing to these extras as a wasted resource.



Turning unsold flowers into extracts or powders addresses sustainability goals. It also recovers part of the cost that might otherwise vanish.



This loop of repurposing reduces the carbon footprint of the floral industry. People who want environmentally friendly options appreciate any step that rescues edible raw materials. Ultrasound-based processing could be a central tool in achieving that.



<h2 class="wp-block-heading" id="h-flowers-in-food-and-skincare">Flowers in food and skincare</h2>



Scientists are testing how flower-derived proteins boost nutritional value in everyday items like bars, cereals, or wraps. Others are exploring their potential in functional drinks or skincare lines.



The synergy between vitamins in certain petals and antioxidants in others might produce new solutions to common nutritional gaps. Such breakthroughs hinge on fine-tuning extraction and drying methods.



As more labs share positive data, companies could invest in research for large-scale production. This shift might reshape how we treat floral byproducts across multiple industries. 



Consumers might not see the behind-the-scenes processes, but they’ll notice new labels highlighting real flower extracts.



<h2 class="wp-block-heading" id="h-the-future-of-edible-flowers">The future of edible flowers</h2>



Some researchers see a future where local florists have partnerships with local food processors. The idea might grow as the data becomes more widely circulated.



Regulatory bodies need to establish clear guidelines for these new ingredients. Safety checks and labeling rules must be in place so that shoppers can trust the products.



Ultrasound might remain popular because of its non-destructive nature. Expanding beyond flowers, it might someday help reclaim other items that go to waste. For now, the excitement around edible flowers keeps building.



The study is published in the <a href="https://onlinelibrary.wiley.com/doi/10.1111/jfpe.70012" target="_blank" rel="noreferrer noopener">Journal of Food Process Engineering</a>.



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Flowers as food: How ultrasound makes it possible

Flowers that lose their initial charm often end up in...

iron ore deposit - 1

Far away, on a remote island in the northwestern Pacific, stands a volcano that many people have never heard of. It quietly shaped global events nearly two centuries ago by sending clouds of ash high into the atmosphere.



This imposing feature is known as Zavaritzki, a caldera that rests within the <a href="https://www.britannica.com/place/Kuril-Islands" target="_blank" rel="noreferrer noopener">Kuril Islands</a>. Once overlooked by explorers and mapmakers, it recently drew attention when scientists linked it to a mysterious weather shift in the early 1800s.



<a href="https://www.st-andrews.ac.uk/earth-sciences/people/wh39/" target="_blank" rel="noreferrer noopener">William Hutchison</a>, a volcanologist at the <a href="https://www.st-andrews.ac.uk/" target="_blank" rel="noreferrer noopener">University of St. Andrews</a>, matched sulfur-laden ice core samples with the distinct rock chemistry found on Zavaritzki’s slopes.



<h2 class="wp-block-heading" id="h-unraveling-the-zavaritzki-puzzle">Unraveling the Zavaritzki puzzle</h2>



Ice cores preserve chemical and mineral traces that help researchers identify old volcanic explosions. For decades, one major blast from 1831 baffled experts because they could not figure out <a href="https://volcano.si.edu/volcano.cfm?vn=290180" target="_blank" rel="noreferrer noopener">which volcano</a> triggered such dramatic cooling.



Historical journals from that year described unusual hues in the sky, including a Sun that took on a greenish cast. 



Many reports also noted a stark drop in temperature, which pointed to a significant injection of volcanic material into the air. 



Scientists suspected that <a href="https://www.earth.com/news/faster-global-warming-linked-to-fewer-aerosols-in-ship-pollution/">sulfur aerosols</a> had reflected sunlight, but pinpointing the exact source to Zavaritzki proved challenging.



<h2 class="wp-block-heading" id="h-potassium-poor-ash-as-the-key">Potassium-poor ash as the key</h2>



Clues emerged when geologists examined tiny shards of minerals, from the cores, under powerful microscopes. 



Tests showed these particles were low in potassium, which indicated a composition unlike many of the well-known volcanoes in Iceland or Alaska.



The discovery led researchers toward the Kurils, a remote chain of islands bridging northern Japan and Russia’s Kamchatka Peninsula. 



Additional analysis revealed that these shards mirrored fresh samples from the slopes of the Zavaritzki caldera, which led to a breakthrough.



<h2 class="wp-block-heading" id="h-cinder-cones-from-the-zavaritzki-caldera">Cinder cones from the Zavaritzki caldera</h2>



Zavaritzki’s complex includes several <a href="https://www.nps.gov/articles/000/cinder-cones.htm" target="_blank" rel="noreferrer noopener">cinder cones</a>, which arise when gas-charged lava splatters and cools in steep mounds. These clusters often form around larger vents, adding layers of material each time an eruption occurs.



Cinders and ash accumulate at angles that can reach around 30 degrees, sometimes forming cones a few hundred feet tall. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/02/Zavaritski-Caldera_volcanic-eruption-1800s_nasa_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/02/Zavaritski-Caldera_volcanic-eruption-1800s_nasa_1s.webp" alt="The Zavaritskogo volcano (also called Zavaritskii) is a striking feature on Simushir Island, in the middle of the archipelago. It is made up of nested, steep-walled calderas surrounding a central lake. The OLI (Operational Land Imager) on Landsat 8 captured these images of Zavaritskogo and its complex edifice on September 12, 2024. Credit: NASA" class="wp-image-1960590"/></a><figcaption class="wp-element-caption">The Zavaritskogo volcano (also called Zavaritskii) is a striking feature on Simushir Island, in the middle of the archipelago. It is made up of nested, steep-walled calderas surrounding a central lake. The OLI (Operational Land Imager) on Landsat 8 captured these images of Zavaritskogo and its complex edifice on September 12, 2024. Credit: NASA</figcaption></figure>



These structures can collapse inward if lava flows breach the sides, creating a patchwork of vents and channels.



<a href="https://www.nps.gov/articles/000/monogenetic-volcanic-fields.htm" target="_blank" rel="noreferrer noopener">Monogenetic cones</a> typically appear during a single eruptive phase, but multiple cones can punctuate the same region. 



The presence of these features in Zavaritzki’s caldera indicates a history of intermittent volcanic episodes.



<h2 class="wp-block-heading" id="h-tracing-the-eruption-s-impact">Tracing the eruption’s impact</h2>



<a href="https://www.earth.com/news/ancient-volcanoes-chaos-poisoned-ferns-for-millions-of-years/">Volcanoes</a> that push sulfur aerosols into the stratosphere can affect temperatures far from their origin. In 1831, the fallout is believed to have caused widespread weather anomalies and a notable chill.



Diarists in Europe described summer storms and hail that damaged crops, while some regions reported an early onset of colder spells. 



These conditions aligned with the timeline suggested by scientists from their ice core studies.



Radiocarbon analysis offered further confirmation that a major event happened around that date. By matching carbon signatures in volcanic deposits with those in dated materials, experts pieced together a more accurate chronology.



<h2 class="wp-block-heading" id="h-invisible-threats-and-modern-lessons">Invisible threats and modern lessons</h2>



Remote volcanoes can create havoc when they erupt, as they often remain off the usual monitoring grids. 



William Hutchison pointed out that blasts in higher latitudes can still impact worldwide climate by spreading sulfate aerosols.



Historic examples, like the 1991 <a href="https://earthobservatory.nasa.gov/images/1510/pinatubo-erupts" target="_blank" rel="noreferrer noopener">Pinatubo eruption</a> in the Philippines, illustrate how a single volcano can lower global temperatures for months or years. 



Even with modern satellite data, it is easy to overlook the activities of lesser-known peaks.



Scientists now prioritize collaborative efforts to expand surveillance networks. Improving early detection could reduce the toll of such eruptions on agriculture, infrastructure, and public health.



<h2 class="wp-block-heading" id="h-peering-beneath-the-waves">Peering beneath the waves</h2>



Some Kuril volcanoes lie partially submerged, forming flooded calderas where the ocean flows in. Others have steep-walled basins dotted with cinder cones and small lakes, as seen in Zavaritzki’s terrain.



During the Cold War, parts of this archipelago hosted submarines and hidden bases. Today, geologists map remnants of older eruptions to better grasp how these islands evolved over time.



<h2 class="wp-block-heading" id="h-why-the-zavaritzki-eruption-matters">Why the Zavaritzki eruption matters</h2>



Powerful <a href="https://www.earth.com/news/new-research-enhances-predictions-on-volcanic-eruptions/">volcanic eruptions</a> can leave behind evidence in ice cores, tree rings, and written accounts. These clues reveal how the planet responds to sudden injections of ash and gases.



Distant events can disrupt harvests, freeze waterways, and shift weather patterns, reminding us that we share a connected atmosphere. 



Understanding these processes helps us plan for future episodes that might catch us unprepared.



Zavaritzki highlights the importance of watching every corner of our planet, no matter how remote, in order to avoid the disasters associated with surprise volcanic eruptions. 



The study is published in <a href="https://www.pnas.org/doi/10.1073/pnas.2416699122" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Volcanic eruption that cooled the Earth and turned the Sun green

Far away, on a remote island in the northwestern Pacific,...

For years, scientists have been eager to tune in to the subtle vibrations sent across the universe by cataclysmic events. Gravitational-wave observatories provide that opportunity, but capturing the weakest signals demands innovative advancements.



A newly developed optical system offers a possible route to higher laser power levels, which is crucial for capturing more distant <a href="https://www.earth.com/news/quantum-particles-solution-gravitational-wave-mystery-bose-einstein-condensate/" target="_blank" rel="noreferrer noopener">events</a>.



Jonathan Richardson, an assistant professor at <a href="https://www.ucr.edu/" target="_blank" rel="noreferrer noopener">UC Riverside</a>, noted that the research represents a leap forward in our ability to control the heat-related distortions that hamper current detectors.



<h2 class="wp-block-heading" id="h-ring-like-targeted-heating">Ring-like targeted heating</h2>



The new system directs infrared radiation onto mirrored surfaces with carefully shaped patterns. The ring-like approach corrects the warping that arises from intense laser power.



Each main mirror weighs about 88 pounds, so minimizing distortions is not easy. With precisely controlled heating zones, the system keeps the reflections crisp and stable, which is a major benefit for detecting faint <a href="https://www.earth.com/news/gravitational-waves-dark-matter-big-bang-breakthrough/" target="_blank" rel="noreferrer noopener">signals</a>.



Conventional adaptive optics in astronomy often corrects atmospheric blurring, but controlling thermal effects on a massive mirror is a different challenge. 



Engineers must ensure that the heating pattern doesn't add noise or degrade the device's sensitivity.



By shaping the heat precisely, the technique preserves the optical path. This safeguard is essential for measuring tiny disturbances in spacetime without spurious signals creeping in.



<h2 class="wp-block-heading" id="h-detecting-faint-gravitational-wave-signals">Detecting faint gravitational wave signals</h2>



The Laser Interferometer Gravitational-Wave Observatory (<a href="https://www.ligo.caltech.edu/" target="_blank" rel="noreferrer noopener">LIGO</a>) has already recorded events involving black holes and neutron stars, broadening our knowledge of cosmic collisions. 



The path to even fainter signals involves pushing laser power beyond 1 megawatt inside the detectors.



"We expect this technology, and future versions of it, will be able to achieve more power in the interferometer," said Professor Richardson. This boost brings greater heat, which introduces more distortion.&nbsp;



Quantum noise presents another obstacle, since gravitational-wave detectors rely on laser beams that exhibit quantum fluctuations. 



Researchers use techniques like light squeezing to reduce these uncertainties and gain clearer measurements.



Larger laser power amplifies the <a href="https://www.earth.com/news/rare-cosmic-object-detected-gravitational-wave-signal/" target="_blank" rel="noreferrer noopener">quantum effects</a>, making it vital to have stable mirrors. The new ring-like heating control is expected to help maintain mirror quality in those high-power conditions.



<h2 class="wp-block-heading" id="h-a-vision-for-tomorrow">A vision for tomorrow</h2>



Moving beyond current facilities, the proposed <a href="https://cosmicexplorer.org/" target="_blank" rel="noreferrer noopener">Cosmic Explorer</a> aims for arms about 25 miles in length. That vast distance should help capture gravitational ripples from earlier chapters in the universe.



Researchers predict that such a facility could show us signals when the cosmos was a small fraction of its present age. 



This might clarify puzzling details about the <a href="https://arxiv.org/pdf/2302.05709" target="_blank" rel="noreferrer noopener">expansion rate</a> of the universe, which has two conflicting measurements right now.



Cosmic Explorer's design is guided by lessons learned from LIGO's upgrades. Each expansion in size and power requires solutions that can handle more severe thermal and quantum effects.



Scientists are also evaluating materials that can endure higher energy levels without warping. Selecting the right substrates and coatings can make or break the performance of next-generation observatories.



<h2 class="wp-block-heading" id="h-secrets-unlocked-with-gravitational-waves">Secrets unlocked with gravitational waves </h2>



Accurate gravitational-wave observations might offer new insights into how general relativity works under extreme conditions. 



Researchers also see a chance to confirm or challenge alternative <a href="https://www.earth.com/news/black-hole-draco-1es-1927-654-just-awoke-is-spewing-material-at-incredible-speeds/" target="_blank" rel="noreferrer noopener">theories</a>, especially near the boundaries of a black hole.



"If you look at the history of astronomy, every time we’ve developed electromagnetic telescopes that can observe a different wavelength, we have discovered new objects," said Professor Richardson, who hopes gravitational waves will reveal something equally unanticipated.



By detecting more subtle signals, researchers can gather data on the evolution of black holes, including their spins and possible interactions with nearby objects. This might reveal patterns that haven't been visible with current methods.



Gravitational waves can also function as a different kind of cosmic ruler. When combined with traditional light-based observations, they could refine distance measurements to far-off galaxies.



<h2 class="wp-block-heading" id="h-new-era-of-gravitational-wave-detection">New era of gravitational wave detection</h2>



Experts plan to pair advanced optical systems with quantum-enhanced lasers to open new frontiers in detection. 



Studies show that combining these methods can lower noise across multiple frequency bands, allowing for the detection of weaker signals.



This work highlights the value of practical engineering in exploring cosmic mysteries. It also strengthens the case for building next-generation observatories that demand intense laser power and precise mirror control.



Ongoing experiments aim to integrate adaptive heating with other sensor improvements. Scientists are testing prototypes that can switch heating patterns in real time for different operating <a href="https://www.earth.com/news/detecting-warp-drives-extraterrestrial-spacecraft-using-gravitational-waves-experiment/" target="_blank" rel="noreferrer noopener">conditions</a>.



A coordinated global network of detectors might share insights on mirror shaping techniques, so the entire community benefits from every development. This synergy could accelerate our progress toward capturing signals from even more distant events.



<h2 class="wp-block-heading" id="h-creating-a-worldwide-network">Creating a worldwide network </h2>



Other projects, like Europe's proposed <a href="https://www.et-gw.eu/" target="_blank" rel="noreferrer noopener">Einstein Telescope</a>, aim to use underground tunnels arranged in a triangular shape to reduce seismic noise. 



This approach could complement what Cosmic Explorer attempts on a larger scale, creating a worldwide network.



Such coordination increases the odds of catching elusive signals and pinning down their sources. By comparing data across different detectors, scientists can refine their estimates of where in the sky a gravitational wave originated.



Collaborative data analysis is crucial, as it confirms detections and further refines estimates of each signal's origin.



Upgrades to existing facilities are already showing how small engineering tweaks can sharpen our vision of the cosmos. The adaptive heating approach is one such tweak, but it sets the stage for more ambitious changes.



Each incremental improvement broadens our view of gravitational-wave sources, whether they lurk billions of light-years away or hide in our local cosmic neighborhood. 



As these technologies advance, new mysteries might emerge that redefine our understanding of space and time.



The study is published in <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.116.061102" target="_blank" rel="noreferrer noopener">Physical Review Letters</a>.



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New technology dramatically boosts gravitational wave detection

For years, scientists have been eager to tune in to...

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Nushagak Bay, a large estuary in southwest Alaska. Nushagak runs mainly north to south and exits in Bristol Bay, a large body of water in the Bering Sea.



"The bay is primarily fed by the Nushagak River, which begins in the Alaska Range and flows southwest approximately 450 km. The bay is also fed by several additional rivers including the Wood, Igushik, Snake and Weary rivers," says ESA.



"The dark colors of the Nushagak River are most likely due to tannins or lignins (chemical substances found in plants). Tannins and lignins from roots, leaves, seeds, bark and soil can leach into the water and give it a brown or even black colour. The sediments then flow southwards where it is mixed with the bluer waters of the bay."



Video/ Image Credit: ESA



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By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Nushagak Bay in southwest Alaska

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Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> (ACS) reveals that proteins on flu viruses are actually flexible, tilting and waving in a “breath-like” motion. According to the experts, these proteins could be used to better defend against the flu.



"The main antigenic targets of influenza virus are two surface glycoproteins, hemagglutinin (HA) and neuraminidase (NA). Whereas the structural and dynamical properties of both glycoproteins have been studied previously, the understanding of their plasticity in the whole-virion context is fragmented," wrote the researchers.



To investigate, the team conducted detailed simulations of the influenza A H1N1 virion, or the swine flu. The experts concluded that the visualizations show many new vulnerable states of flu viruses, which could improve future vaccines and antiviral drugs.



Video/ Image Credit: American Chemical Society&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



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Flu viruses are more flexible than expected

[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"] Today's Video of the Day from the...

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Lake Trasimeno, which is located west of Perugia in central Italy. It is the fourth largest lake in the country. While Trasimeno’s water level varies, it has a maximum depth of approximately six meters.&nbsp;



"In this Copernicus Sentinel-2 image, captured on 6 August 2022, the lake’s emerald green colour is likely due to the presence of phytoplankton. Streaks in the water, particularly visible in the west, indicate the presence of soil and sediments which have been stirred up by winds. Dark colored waters in the southern part of the lake indicate a presence of submerged and floating macrophytes (aquatic plants) as well as algae," says ESA.



"Surrounded by hills on three sides, Trasimeno is subject to heavy storms created by winds, especially from the north and west. There are three islets in the lake: Maggiore, Minore and Polvese (the largest). The lake’s shores are sparsely inhabited with only two popular villages: Castiglione del Lago and Passignano sul Trasimeno."



"Italy is experiencing its worst drought in 70 years which has affected drinking water supplies, hydroelectric power and agricultural production. High temperatures, hot winds and lack of rainfall are the main causes of drought in the Umbrian region which saw Lake Trasimeno’s drop 1.3 m, reaching the limit of the hydrometric zero in July 2022."



Video/Image Credit: ESA&nbsp;



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By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Lake Trasimeno in Central Italy

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Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> describes a new self-powered nanosensor that can instantly detect mercury contamination with the tap of a finger.&nbsp;



The oxidized form of mercury can be harmful when it is ingested through contaminated water or food. This makes it necessary for experts to develop sensors that can quickly and accurately detect the presence of mercury.&nbsp;



Zong-Hong Lin and colleagues have now created a triboelectric nanosensor (TENS) that can detect mercury by simply by touching a sample. According to the researchers, their TENS could serve as the basis for similar devices to safely and remotely monitor other pollutants.



Video Credit: American Chemical Society&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



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Detecting mercury contamination with the tap of a finger

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Kainji Lake, a reservoir on the Niger River.



In 1968, Kainji Lake was created by the construction of the Kainji Dam. The Niger River, the third longest in Africa, enters the lake in the north.&nbsp;



According to <a href="https://www.earth.com/news/rivers-in-the-american-west-are-a-lifesaving-resource-for-birds/">ESA</a>, the creation of the lake submerged Foge Island and the town of Bussa and permanently flooded other riverine settlements, leaving around 50,000 people displaced.&nbsp;



Large parts of Foge Island are temporarily exposed during low water tides, and the land is often used by migrating fishermen. Kainji Dam is a dam across the Niger River in Niger State of Central Nigeria. 



Wild mammals occur at relatively low densities due to illegal hunting. Lake Kainji has suffered a dramatic decline as a fishery due to the high numbers of artisanal and subsistence fisherfolk using the lake. It has been suggested that a period of closure, together with controlled fishing rights may help improve fish stocks.



Kainji Lake National Park is the oldest of its kind in Nigeria. The park contains three distinct areas: a part of the Kainji Lake, the Borgu Game Reserve to the west of the lake, and the Zugurma Game Reserve to the southeast. The park is home to around 65 mammal species, 350 bird species, and 30 species of reptiles and amphibians. 



Video/ Image Credit: European Space Agency&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



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Kainji Lake in north central Nigeria

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Today’s Video of the Day from <a href="https://www.igb.illinois.edu/">Carl R. Woese Institute for Genomic Biology</a> reveals how scientists can modify common crops like soybean, rice, and wheat to protect them from heat stress.



“We need to double crop production by 2050 to feed a growing global population, and not only are we not on track to do that, but climate change is further complicating things,” said Amanda Cavanagh, a lecturer at the University of Essex. 



The study is part of Realizing Increased Photosynthetic Efficiency (RIPE), an international research project that aims to develop food crops that turn the sun’s energy into food more efficiently.



“Using an engineering approach we designed multiple alternative metabolic pathways to photorespiration. Testing them in the field showed increases in productivity which led Amanda to significantly move the project forward by showing our engineered plants can withstand pretty extreme temperature stress,” said study co-author and RIPE researcher Paul South.&nbsp;



“As the climate changes and temperature stresses increase the pressure on our global food supply, farmers will need every tool available including engineering approaches like the synthetic biology used here to maintain safe and productive harvests.”



The experts tested plants modified to have more efficient photorespiration to see if they were better adapted to warmer temperatures.&nbsp;



The team found that the engineered plants produced 26 percent more biomass than the wild-type plants exposed to the same temperatures, and had 15 percent less yield loss under the higher temperatures.



Video Credit: Amanda Nguyen/University of Illinois



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Designing crops that can beat the heat

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