Today's Image of the Day from the European Space Agency features the barred spiral galaxy NGC 1559, located around 35 million light-years away in the little-observed southern constellation Reticulum. The image was captured by the James Webb Space Telescope.&nbsp;



<h2 class="wp-block-heading" id="h-fuel-for-star-formation">Fuel for star formation </h2>



"The data featured in this portrait make use of two of Webb’s instruments: the Mid-InfraRed Instrument (MIRI) and Near-InfraRed Camera (NIRCam)," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Here MIRI captures the glow of interstellar dust grains, which trace out the interstellar medium, the fuel for future star formation. NIRCam shows the light from stars, even young stars hidden behind prodigious amounts of dust. NIRCam also captures emission from ionised nebulae around young stars."



<h2 class="wp-block-heading" id="h-webb-reveals-galaxies-in-new-light">Webb reveals galaxies in new light</h2>



According to ESA, the data was collected by the <a href="https://sites.google.com/view/phangs/home">PHANGS team</a> as part of a program in which Webb will observe 55 <a href="https://www.earth.com/news/james-webb-captures-galaxies-that-are-too-old-to-exist/">galaxies</a> that have also been mapped by the Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope, the Hubble Space Telescope, and more.&nbsp;



"By combining Webb’s unprecedented view of the dust and stars with data from these other facilities, the team aims to obtain a new, highly detailed view of how stars are born, live, and die in galaxies across the Universe."



<h2 class="wp-block-heading" id="h-ngc-1559-a-loner-in-space">NGC 1559: A loner in space</h2>



Although NGC 1559 appears to sit close to one of our nearest neighbors in the sky - the Large Magellanic Cloud (LMC) - this is just a trick of perspective, noted ESA.



While it is part of the Reticulum constellation, NGC 1559 is not part of the Local Group of galaxies but instead resides in a more distant region of space.



"In reality, NGC 1559 is physically nowhere near the LMC in space; in fact it truly is a loner, lacking the company of any nearby galaxies or membership of any galaxy cluster."



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1559">Star formation in NGC 1559</h2>



NGC 1559 is notable for its active star formation and strong magnetic fields. It has also been the site of several <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernovae</a>, making it of particular interest to astronomers studying stellar evolution and the lifecycle of stars.



The structure of NGC 1559 includes well-defined spiral arms that are rich in young, hot stars and regions of ionized gas, indicative of ongoing <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">star formation</a>.



The galaxy’s central bar is believed to play a role in driving gas towards the core, fueling both the star formation and the activity around its nucleus.



<h2 class="wp-block-heading" id="h-an-extragalactic-wonder">An extragalactic wonder</h2>



Despite being relatively small compared to larger galaxies like the Milky Way, NGC 1559 is an important object for understanding how barred spiral galaxies evolve and the processes that trigger supernovae.



The galaxy’s remote location and active nature make it a fascinating subject of study in the field of extragalactic astronomy. The isolation of NGC 1559 allows for a clearer view of its structure without much interference from neighboring galaxies.



<h2 class="wp-block-heading" id="h-barred-spiral-galaxies">Barred spiral galaxies</h2>



Barred spiral galaxies are a type of spiral galaxy characterized by a central bar-shaped structure composed of stars. This bar extends out from the core and connects to the galaxy's spiral arms, which swirl outward in a graceful pattern.



Scientists believe that the bar plays a crucial role in the evolution of the galaxy, funneling gas towards the core and potentially triggering star formation or feeding a central black hole. 



The <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">Milky Way</a>, our own galaxy, is an example of a barred spiral. These galaxies are quite common in the universe, making up about two-thirds of all observed spiral galaxies.



The bar itself is thought to be a temporary feature, developing as the galaxy matures and possibly disappearing over time as the dynamics of the stars change. 



<h2 class="wp-block-heading" id="h-the-reticulum-constellation">The Reticulum constellation</h2>



The Reticulum constellation is a small, faint constellation in the southern sky. Its name means "the reticle" in Latin, which refers to the crosshairs in an eyepiece of a telescope. 



The constellation was named in the 18th century by the French astronomer Nicolas Louis de Lacaille to honor the reticle he used in his scientific instruments. It is one of the 88 modern constellations recognized by the International Astronomical Union.



Image Credit: ESA/Webb, NASA &amp; CSA, A. Leroy, J. Lee and the PHANGS Team



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Spiral galaxy NGC 1559 is a loner in outer space

Today's Image of the Day from the European Space Agency features the barred spiral galaxy NGC 1559, located around 35 million light-years away in the little-observed southern constellation Reticulum. The image was captured by the James Webb Space Telescope.&nbsp; Fuel for star formation "The data featured in this portrait make use of two of Webb’s instruments: the Mid-InfraRed Instrument (MIRI) and Near-InfraRed Camera (NIRCam)," noted ESA. "Here MIRI captures the glow of interstellar dust grains, which trace out the interstellar medium, the fuel...

Today's Image of the Day from the European Space Agency features NGC 1792, a spiral galaxy located in the constellation Columba, about 43 million light-years away from Earth.&nbsp;



This galaxy, discovered by British astronomer James Dunlop in 1826, is part of the larger NGC 1808 group of galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-intimate-view-of-ngc-1792">Intimate view of NGC 1792</h2>



“An orange glow radiates from the center of NGC 1792, the heart of this stellar forge. Captured by the NASA/ESA Hubble Space Telescope, this intimate view of NGC 1792 gives us some insight into this galactic powerhouse,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The vast swathes of tell-tale blue seen throughout the galaxy indicate areas that are full of young, hot stars, and it is in the shades of orange, seen nearer the center, that the older, cooler stars reside.”



<h2 class="wp-block-heading" id="h-vigorous-star-formation-nbsp">Vigorous star formation&nbsp;</h2>



NGC 1792 is notable for its vigorous star formation, classifying it as a starburst galaxy. This high rate of star formation is thought to be triggered by gravitational interactions with neighboring galaxies, though the exact cause is still under study.



“Nestled in the constellation of Columba (The Dove), NGC 1792 is both a spiral galaxy, and a starburst galaxy,” said ESA. “Within starburst galaxies, stars are forming at comparatively exorbitant rates. The rate of star formation can be more than 10 times faster in a starburst galaxy than in the Milky Way.”



<h2 class="wp-block-heading" id="h-fierce-bursts-of-star-formation">Fierce bursts of star formation</h2>



ESA noted that when galaxies have a large reservoir of gas, like NGC 1792, these short-lived starburst phases can be sparked by galactic events such as mergers and tidal interactions.&nbsp;



“One might think that these starburst galaxies would easily consume all of their gas in a large forming event. However, supernova explosions and intense stellar winds produced in these powerful starbursts can inject energy into the gas and disperse it.”&nbsp;



“This halts the star formation before it can completely deplete the galaxy of all its fuel. Scientists are actively working to understand this complex interplay between the dynamics that drive and quench these fierce bursts of star formation.”



Due to its distance and brightness, NGC 1792 can be observed with medium-sized telescopes under favorable conditions.



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



Galaxy evolution refers to the process by which galaxies form and change over time. It begins in the early universe, shortly after the <a href="https://www.earth.com/news/new-observations-disprove-big-bang-theory-universe-began-tired-light-theory/" target="_blank" rel="noreferrer noopener">Big Bang</a>, when small density fluctuations in the primordial gas led to the collapse of matter into the first galaxies. 



<h3 class="wp-block-heading" id="h-galaxy-mergers">Galaxy mergers</h3>



These early galaxies were small and irregular, composed mostly of gas and dark matter. Over billions of years, galaxies grew larger by merging with one another and by accreting gas from the surrounding space.&nbsp;



These interactions often triggered bursts of star formation, and collisions between galaxies sometimes led to the creation of new, more massive galaxies.



<h3 class="wp-block-heading" id="h-structural-changes">Structural changes</h3>



As galaxies evolve, their morphology - their shape and structure - can change. Early galaxies were often irregular or disk-shaped, but over time, many galaxies formed into the elliptical or spiral shapes we see today.&nbsp;



<h3 class="wp-block-heading" id="h-star-formation">Star formation</h3>



Star formation is a key driver of galaxy evolution, but it gradually slows down as galaxies age. 



The gas that fuels <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">star formation</a> can be used up, or it can be heated and pushed out of galaxies by supernovae or black holes, reducing the galaxy's ability to form new stars.



<h3 class="wp-block-heading" id="h-galaxy-environment-nbsp">Galaxy environment&nbsp;</h3>



The environment in which a galaxy resides also plays a role in its evolution. Galaxies in dense clusters are more likely to interact with their neighbors, which can alter their shape or trigger bursts of star formation.&nbsp;



In contrast, galaxies in more isolated regions of space evolve more slowly and without as many dramatic interactions.



<h3 class="wp-block-heading" id="h-dark-matter">Dark matter</h3>



Dark matter also plays a crucial role in galaxy evolution. It provides the gravitational framework that holds galaxies together and influences their interactions with one another.&nbsp;



Supermassive <a href="https://www.earth.com/search-results/?search=Galaxies%20merge&amp;start=0" target="_blank" rel="noreferrer noopener">black holes</a>, found at the centers of most large galaxies, can also affect their evolution by releasing energy that impacts star formation and the movement of gas within the galaxy.



Overall, galaxy evolution is a complex and ongoing process driven by interactions between stars, gas, <a href="https://www.earth.com/news/study-dark-matter-does-not-exist-and-the-universe-is-27-billion-years-old/" target="_blank" rel="noreferrer noopener">dark matter</a>, and black holes, and shaped by both internal processes and external influences.



Image Credit: ESA/Hubble &amp; NASA, J. Lee



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NGC 1792: A galactic powerhouse 

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

Burlington, Iowa and the Mississippi River Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at Burlington, Iowa along the Mississippi River. 

The photo was taken by an astronaut on board the International Space Station.

Burlington sits atop high bluffs along the Mississippi, which narrows as the river approaches the city. <ins class="adsbygoogle" style="display: block; text-align: center;" data-ad-layout="in-article" data-ad-format="fluid" data-ad-client="ca-pub-2900029420000674" data-ad-slot="3505321548"></ins>

Additionally, a dam helps slow the flow of the river, which allows for two bridges to connect both sides. 

When major <a href="https://www.earth.com/image/peru-devastating-flooding/">flooding</a> occurs, the Mississippi spills its water into the low floodplain. The most severe flood ever recorded in the area happened in June 2008, which caused the water level to rise 25.73 feet.The Mississippi River is the <a title="List of longest rivers of the United States (by main stem)" href="https://en.wikipedia.org/wiki/List_of_longest_rivers_of_the_United_States_(by_main_stem)">second-longest river</a> and chief <a title="River" href="https://en.wikipedia.org/wiki/River">river</a> of the second-largest <a title="Drainage system (geomorphology)" href="https://en.wikipedia.org/wiki/Drainage_system_(geomorphology)">drainage system</a> on the North American continent, second only to the <a title="Hudson Bay" href="https://en.wikipedia.org/wiki/Hudson_Bay">Hudson Bay</a> drainage system. From its traditional source of <a title="Lake Itasca" href="https://en.wikipedia.org/wiki/Lake_Itasca">Lake Itasca</a> in northern <a title="Minnesota" href="https://en.wikipedia.org/wiki/Minnesota">Minnesota</a>, it flows generally south for 2,320 miles (3,730 km) to the <a title="Mississippi River Delta" href="https://en.wikipedia.org/wiki/Mississippi_River_Delta">Mississippi River Delta</a> in the <a title="Gulf of Mexico" href="https://en.wikipedia.org/wiki/Gulf_of_Mexico">Gulf of Mexico</a>. With its many <a title="Tributary" href="https://en.wikipedia.org/wiki/Tributary">tributaries</a>, the Mississippi's <a title="Drainage basin" href="https://en.wikipedia.org/wiki/Drainage_basin">watershed</a> drains all or parts of 32 <a title="U.S. state" href="https://en.wikipedia.org/wiki/U.S._state">U.S. states</a> and two <a title="Provinces and territories of Canada" href="https://en.wikipedia.org/wiki/Provinces_and_territories_of_Canada">Canadian provinces</a> between the <a title="Rocky Mountains" href="https://en.wikipedia.org/wiki/Rocky_Mountains">Rocky</a> and <a title="Appalachian Mountains" href="https://en.wikipedia.org/wiki/Appalachian_Mountains">Appalachian</a> mountains. The <a class="mw-redirect" title="Mainstem (hydrology)" href="https://en.wikipedia.org/wiki/Mainstem_(hydrology)">main stem</a> is entirely within the United States; the total <a title="Drainage basin" href="https://en.wikipedia.org/wiki/Drainage_basin">drainage basin</a> is 1,151,000 sq mi (2,980,000 km2), of which only about one percent is in Canada. The Mississippi ranks as the <a title="List of rivers by discharge" href="https://en.wikipedia.org/wiki/List_of_rivers_by_discharge">fifteenth-largest</a> river by discharge in the world. The river either borders or passes through the states of <a title="Minnesota" href="https://en.wikipedia.org/wiki/Minnesota">Minnesota</a>, <a title="Wisconsin" href="https://en.wikipedia.org/wiki/Wisconsin">Wisconsin</a>, <a title="Iowa" href="https://en.wikipedia.org/wiki/Iowa">Iowa</a>, <a title="Illinois" href="https://en.wikipedia.org/wiki/Illinois">Illinois</a>, <a title="Missouri" href="https://en.wikipedia.org/wiki/Missouri">Missouri</a>, <a title="Kentucky" href="https://en.wikipedia.org/wiki/Kentucky">Kentucky</a>, <a title="Tennessee" href="https://en.wikipedia.org/wiki/Tennessee">Tennessee</a>, <a title="Arkansas" href="https://en.wikipedia.org/wiki/Arkansas">Arkansas</a>, <a title="Mississippi" href="https://en.wikipedia.org/wiki/Mississippi">Mississippi</a>, and <a title="Louisiana" href="https://en.wikipedia.org/wiki/Louisiana">Louisiana</a>.

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By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="http://earth.com/staff">Earth.com</a> Staff Writer

Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90229&amp;eocn=home&amp;eoci=iotd_title">NASA Earth Observatory</a>
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Burlington, Iowa and the Mississippi River

Burlington, Iowa and the Mississippi River Today’s Image of the...

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at Iceland at night.

The graphic is a composite built using images taken by the <a href="https://jointmission.gsfc.nasa.gov/viirs.html">Visible Infrared Imaging Radiometer Suite</a> (VIIRS) on the <a href="https://jointmission.gsfc.nasa.gov/suomi.html">Suomi NPP</a> satellite. 

Night light images can be very helpful in illustrating population distribution. For example, Iceland’s interior center highlands are high in elevation, very cold, and sparsely vegetated. As a result, there is very little permanent human settlement there, especially compared to its coastal perimeter.  

The outer coast of Iceland, which includes its capital Reykjavik, has more hospitable conditions and easy access to ocean resources such as <a href="https://www.earth.com/news/rampant-overfishing-gulf-california/">fishing</a>.

--

By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="http://earth.com/staff">Earth.com</a>

Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=85177">NASA Earth Observatory</a>

Nighttime in Iceland

Today’s Image of the Day comes thanks to the NASA...

IDL TIFF file

Scorpion Reef in the Gulf of Mexico Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at Arrecife Alacranes, otherwise known as the Scorpion reef of the southern Gulf of Mexico.

This image was taken by the Operational Land Imager (OLI) on Landsat 8.

Scorpion Reef is located about 60 miles north of Progresso, Mexico and consists of five small islands. Together, however, they comprise the largest coral structure in the southern Gulf. 
In 2006, the reef was named an official UNESCO biosphere reserve.Scorpion Reef is a reef surrounding a small group of islands in the Gulf of Mexico off the northern coast of the state of Yucatán, Mexico. Designated a national park, the reef is part of the Campeche Bank archipelago and is the largest reef in the southern Gulf of Mexico. It contains the five main vegetated islands of Isla Pérez, Isla Desertora, Isla Pájaros, Isla Chica, and Isla Desterrada. Isla Pérez is the only inhabited island and includes a lighthouse. The reef, including its islets and surrounding waters, has been recognised as an Important Bird Area by BirdLife International because it supports a population of magnificent frigatebirds.

--

By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="http://earth.com/staff">Earth.com</a>

Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=85177">NASA Earth Observatory</a>

Scorpion Reef in the Gulf of Mexico

Scorpion Reef in the Gulf of Mexico Today’s Image of...

Mount Fuji in Japan Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look.

The photo was taken by an astronaut on the International Space Station using the most powerful lens to fully capture the three dimensions.
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Mount is situated on Honshu Island, and measures in at 12,389 feet in height, making it the tallest mountain in Japan. 

The mountain is located 60 miles southwest of <a href="https://www.earth.com/video/megacity-tokyo-bay-japan/">Tokyo</a> and is classified as a stratovolcano that last erupted in 1707.

Mount Fuji is also one of Japan’s “3 Holy Mountains,” along with Mount Tate and Mount Haku.Mount Fuji (富士山, Fujisan, IPA: , located on the island of <a title="Honshu" href="https://en.wikipedia.org/wiki/Honshu">Honshū</a>, is the <a title="List of mountains and hills of Japan by height" href="https://en.wikipedia.org/wiki/List_of_mountains_and_hills_of_Japan_by_height">highest mountain</a> in <a title="Japan" href="https://en.wikipedia.org/wiki/Japan">Japan</a>, standing 3,776.24 m (12,389.2 ft). It is the second-highest <a title="Volcano" href="https://en.wikipedia.org/wiki/Volcano">volcano</a> located on an island in Asia (after <a title="Mount Kerinci" href="https://en.wikipedia.org/wiki/Mount_Kerinci">Mount Kerinci</a> on the island of <a title="Sumatra" href="https://en.wikipedia.org/wiki/Sumatra">Sumatra</a>), and seventh-highest peak of an island on Earth. Mount Fuji is an <a class="mw-redirect" title="Active volcano" href="https://en.wikipedia.org/wiki/Active_volcano">active</a> <a title="Stratovolcano" href="https://en.wikipedia.org/wiki/Stratovolcano">stratovolcano</a> that last erupted from 1707 to 1708. The mountain stands about 100 km (62 mi) southwest of <a title="Tokyo" href="https://en.wikipedia.org/wiki/Tokyo">Tokyo</a> and is visible from there on clear days. Mount Fuji's exceptionally symmetrical cone, which is <a title="Snow field" href="https://en.wikipedia.org/wiki/Snow_field">snow-capped</a> for about five months of the year, is commonly used as a <a title="Cultural icon" href="https://en.wikipedia.org/wiki/Cultural_icon">cultural icon</a> of Japan and it is frequently depicted in art and photography, as well as visited by sightseers and climbers.

--

By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="http://earth.com/staff">Earth.com</a>

Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=87766">NASA Earth Observatory</a>
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Mount Fuji in Japan

Mount Fuji in Japan Today’s Image of the Day comes...

Monterrey, Mexico from the International Space Station Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at Monterrey, the capital of of the Mexican state of Nuevo Leon.

This photo was captured by an astronaut on board the International Space Station.

The area is perhaps most famous for Mount Silla, also known as Cerro De La Silla. <ins class="adsbygoogle" style="display: block; text-align: center;" data-ad-layout="in-article" data-ad-format="fluid" data-ad-client="ca-pub-2900029420000674" data-ad-slot="3505321548"></ins>

Mount Silla has also been nicknamed Saddle Hill, as the mountain’s <a href="https://www.earth.com/news/life-found-mariana-trench/">ridges</a> and peaks look very much like a saddle when viewed from the west. 

Mount Silla has been officially declared a natural monument according to the <a href="https://www.iucn.org/theme/protected-areas/wcpa">World Commission on Protected Areas</a>.

--Monterrey is the capital and largest city of the northeastern state of Nuevo León, Mexico. The city is anchor to the Monterrey metropolitan area, the second most productive in Mexico with a GDP of US$123 billion, and the second largest metropolitan area in México with an estimated population of 5,341,171 people as of 2020. According to the 2020 census, the city itself has a population of 1,142,194. Monterrey is one of the most livable cities in Mexico, and a 2018 study found that suburb San Pedro Garza García is the city with the best quality of life in Mexico. It serves as a commercial center of northern Mexico and is the base of many significant international corporations. Its purchasing power parity-adjusted GDP per capita is considerably higher than the rest of Mexico's at around US$35,500, compared to the country'

By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="http://earth.com/staff">Earth.com</a>

Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90203&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a>
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Monterrey, Mexico from the International Space Station

Monterrey, Mexico from the International Space Station Today’s Image of...

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at the fiery red Lake Natron in Tanzania. 

Lake Natron is mostly inhospitable to life due to its salty, alkaline water. The lake gets its unique chemistry from the frequent <a href="https://www.earth.com/image/extinct-volcano-aden-yemen/">volcanic</a> activity in the area. 

Among the few species able to survive in these conditions are haloarchaea blooms, which are microorganisms that love salt and give off the vibrant pink and red colors seen in the image. 

This natural-color photo was captured by the Operational Land Imager (OLI) onboard the Landsat 8 satellite. 

--

By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="http://earth.com/staff">Earth.com</a>

Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90191&amp;eocn=home&amp;eoci=iotd_previous">NASA Earth Observatory</a>

Fiery red Lake Natron in Tanzania

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at a spring phytoplankton bloom in the Gulf of Alaska.

This photo was taken on April 12, 2017 by the Moderate Resolution Spectroradiometer (MODIS) onboard NASA’s Aqua satellite. 

This phenomenon occurs when bedrock that has been ground into dust by <a href="https://www.earth.com/image/long-island-carved-glaciers/">glaciers</a> seeps into the water and turns it a turquoise color. It also promotes the growth of phytoplankton that feed off its iron.

“We generally expect the blooms to start inshore and then propagate out to deeper water as stratification takes place,” said Scott Pegau, researcher at the Prince William Sound Science Center. Spring phytoplankton bloom in the Gulf of Alaska.

The Gulf shoreline is a rugged combination of forest, mountain and a number of tidewater glaciers. Alaska's largest glaciers, the Malaspina Glacier and Bering Glacier, spill out onto the coastal line along the Gulf of Alaska. The coast is heavily indented with Cook Inlet and Prince William Sound, the two largest connected bodies of water. It includes Yakutat Bay and Cross Sound. Lituya Bay (a fijord north of Cross Sound, and south of Mount Fairweather) is the site of the largest recorded tsunami in history. It serves as a sheltered anchorage for fishing boats.

--

By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="http://earth.com/staff">Earth.com</a>

Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90195&amp;eocn=image&amp;eoci=moreiotd">NASA Earth Observatory</a>

Spring phytoplankton bloom in the Gulf of Alaska

Cape Coral, Florida from the International Space Station Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at Cape Coral, Florida.

This photo was taken by an astronaut on board the International Space Station.
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Cape Coral is nicknamed the “Waterfront Wonderland” thanks to the meticulous city planning that went into maximizing the beautiful views of the water. It is located on the western coast of <a href="https://www.earth.com/plants/vicia-floridana-florida-vetch/">Florida</a> as a part of the Fort Myers metropolitan area.Cape Coral is a city located in Lee County, Florida, United States, on the Gulf of Mexico. Founded in 1957 and developed as a planned community, the city grew to a population of 154,305 by the year 2010. The city's population estimate was 194,495 for 2019. With an area of 120 square miles, Cape Coral is the largest city between Tampa and Miami. It is a principal city in the Cape Coral – Fort Myers, Florida Metropolitan Statistical Area. The population estimate for the statistical area was 679,513 for 2014. The city has over 400 mi of navigable waterways. 

--Cape Coral is a city located in Lee County, Florida, United States, on the Gulf of Mexico. Founded in 1957 and developed as a planned community, the city grew to a population of 154,305 by the year 2010. The city's population estimate was 165,831 for 2013 and 189,343 for 2018. With an area of 120 square miles , Cape Coral is the largest city between Tampa and Miami. It is a principal city in the Cape Coral – Fort Myers, Florida Metropolitan Statistical Area. The population estimate for the statistical area was 679,513 for 2014. The city is known as a Waterfront Wonderland; with over 400 mi of navigable waterways.

By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="http://earth.com/staff">Earth.com</a>

Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=88435">NASA Earth Observatory</a>
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Cape Coral, Florida from the International Space Station

Cape Coral, Florida from the International Space Station Today’s Image...

The devastating rainfall from Storm Boris, which caused severe flooding across Central and Eastern Europe, could have been nearly nine percent less intense without the current levels of global warming. This is the conclusion of a recent analysis from the Alfred Wegener Institute (AWI).



This finding was made possible by a novel modeling technique called “storylines,” which provides a new way to trace the fingerprints of climate change on <a href="https://www.earth.com/news/why-tens-of-millions-of-people-love-watching-videos-of-extreme-weather-events/" target="_blank" rel="noreferrer noopener">extreme weather events</a> in real time. 



This approach is described in the journal <a href="http://dx.doi.org/10.1038/s43247-024-01847-0" target="_blank" rel="noreferrer noopener">Communications Earth &amp; Environment</a> and is accessible via a new online tool developed by the <a href="https://www.awi.de/en/" target="_blank" rel="noreferrer noopener">Alfred Wegener Institute</a>.



<h2 class="wp-block-heading" id="h-the-impact-of-a-warmer-climate">The impact of a warmer climate</h2>



In mid-September, Storm Boris unleashed torrential rain across Poland, the Czech Republic, Austria, and Romania, resulting in catastrophic <a href="https://www.earth.com/news/can-we-outrun-the-flood-risks-of-climate-change/" target="_blank" rel="noreferrer noopener">flooding</a> and displacing countless families. 



Boris produced one of the highest rainfall totals ever recorded in several areas over a five-day period, and the floods claimed at least 27 lives. While cleanup is underway, public and media inquiries are focusing on whether global climate change played a role in this tragic event.



“For the past few years, science has been able to provide robust answers to this absolutely legitimate question,” said lead author Marylou Athanase, a climate physicist at AWI.&nbsp;



“As early as one or two weeks after a given event, so-called probabilistic attribution studies can be used to draw initial conclusions on how much more probable the event was, due to climate change.”



<h2 class="wp-block-heading" id="h-connecting-climate-trends-and-weather-events">Connecting climate trends and weather events</h2>



Yet explaining these probabilities to the public has often proven challenging. Probabilistic studies, while valuable, may lack clarity when connecting global climate trends with specific weather events.&nbsp;



“That’s why we at the AWI have worked so hard to advance a totally new way - the ‘storyline’ approach,” explained co-lead author Antonio Sánchez-Benítez.&nbsp;



“Essentially, we apply the ‘what if?’ principle. What would a given catastrophe look like in a world without <a href="https://www.earth.com/news/climate-change-earth-energy-imbalance-temperature-rise/" target="_blank" rel="noreferrer noopener">climate change</a>? And what about in a climate that was even warmer?”



<h2 class="wp-block-heading" id="h-climate-impact-on-specific-storms">Climate impact on specific storms</h2>



Using the storm as a case study, AWI’s team illustrated the power of this approach. Their analysis showed that, if not for climate change, Storm Boris would have dropped about nine percent less rain.&nbsp;



On its journey from the eastern Mediterranean toward Central Europe, Boris intensified as it encountered water roughly two degrees Celsius warmer than preindustrial levels, which increased the water vapor in the atmosphere.&nbsp;



While nine percent may sound minimal, it can make a significant difference in areas where the additional water exceeds the capacity of rivers, dams, or drainage systems, leading to potentially devastating consequences.



<h2 class="wp-block-heading" id="h-climate-models-and-real-world-weather">Climate models and real-world weather</h2>



One of the key challenges was to accurately connect long-term climate modeling with the actual, observed conditions of specific weather events.&nbsp;



To address this, the team used a process called “nudging,” where actual wind data, including jet stream information, is fed into the model to align it more closely with real-world conditions.&nbsp;



“Climate models normally simulate a specific, quasi-random sequence of weather conditions,” explained Helge Gößling, a climate physicist and head of storyline research at AWI.&nbsp;



“With nudging, we provide the model with actually observed <a href="https://www.earth.com/news/strong-winds-make-it-difficult-for-albatrosses-to-feed/" target="_blank" rel="noreferrer noopener">wind</a> data, and we nudge the model a bit in the direction of the actually observed wind. In this way, we can accurately reproduce real weather in the real climate.”



<h2 class="wp-block-heading" id="h-quantifying-the-influence-of-global-warming-nbsp">Quantifying the influence of global warming&nbsp;</h2>



In their models, the researchers could simulate a pre-climate change world by reducing greenhouse gas levels and adjusting other variables.&nbsp;



By rerunning the scenario, they produced a side-by-side comparison of current and hypothetical climates. This approach allows scientists to quantify the influence of global warming on specific events, from extreme storms to more typical weather patterns.



<h2 class="wp-block-heading" id="h-advanced-climate-data-and-technology">Advanced climate data and technology</h2>



The researchers used the CMIP6 version of the AWI climate model, which contributed to the IPCC’s Sixth Assessment Report, incorporating real-time wind data from the <a href="https://www.ecmwf.int/" target="_blank" rel="noreferrer noopener">European Center for Medium-Range Weather Forecasts</a> (ECMWF). 



“We have since automated the system to the point where daily analyses on the current weather are run on the supercomputer at the <a href="https://www.dkrz.de/en/about-en/about-us" target="_blank" rel="noreferrer noopener">German Climate Computing Center</a> (DKRZ),” Athanase said



The results are then made available to the public on AWI’s online platform. This <a href="https://climate-storylines.awi.de/" target="_blank" rel="noreferrer noopener">tool</a>, updated with a three-day lag from real-time, provides users with access to maps and interactive timelines showing the “Climate Change Signal of the Day” for extreme and daily weather events worldwide.



<h2 class="wp-block-heading" id="h-climate-science-and-public-understanding-nbsp">Climate science and public understanding&nbsp;</h2>



By offering a visual and interactive way to examine climate change’s influence, AWI hopes to bridge the gap between complex climate science and public understanding.&nbsp;



For now, the tool tracks temperature and precipitation data starting from January 2024, allowing users to explore climate impacts on recent weather events.&nbsp;



“Our goal is to promote a better understanding of the connections between climate change and extreme weather events, and to supply concrete and timely answers that can also be used in media coverage of these events,” Athanase said.



The AWI’s storyline model and online tool represent an innovative step forward in climate science communication, helping researchers, decision-makers, and the public see, in real terms, how global warming affects <a href="https://www.earth.com/news/pollen-alters-cloud-formation-and-changes-weather-patterns/" target="_blank" rel="noreferrer noopener">weather patterns</a> and extreme events.



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How much does climate change influence extreme weather events?

The devastating rainfall from Storm Boris, which caused severe flooding...

Curiosity, the renowned Mars rover from NASA, is enriching our understanding of the Red Planet's mysterious landscapes and puzzling geological features.



Around the corner awaits a new expedition for Curiosity, this time to investigate a formation known as a boxwork. This intriguing network of patterns lies in a region at the foot of Mount Sharp and promises even more fascinating discoveries. 



<h2 class="wp-block-heading" id="h-curiosity-finds-yellow-sulfur-stones">Curiosity finds yellow sulfur stones</h2>



Before embarking on this new quest, Curiosity bids farewell to <a href="https://www.earth.com/news/nasas-curiosity-rover-explores-mars-ridge-with-intriguing-watery-past/" target="_blank" rel="noreferrer noopener">Gediz Vallis</a>, a channel that is shrouded in enigma.



Details of the formation of this channel during a period of transition to a drier climate continue to elude scientists. 



But it is not just the channel that piques their interest. Curiosity stumbled upon a strange field of yellow sulfur stones during the summer, literally crushing them with its wheels as it drove along. This adds another layer of mystery to the Martian puzzle.



Before moving out, Curiosity provided scientists with invaluable imagery. The rover captured 360-degree panoramas of the stones, along with channel features, making sure no detail was overlooked.



<div class="wp-block-sendtonews-playerselector">[sendtonews key="cczO1PejFp-4040684-12187" type="single"]</div>



<h2 class="wp-block-heading" id="h-the-quest-for-ancient-life">The quest for ancient life</h2>



A fundamental purpose of the rover's mission is probing <a href="https://www.earth.com/news/new-evidence-found-for-life-on-mars-where-ancient-rivers-once-flowed/" target="_blank" rel="noreferrer noopener">Mars' past</a>, with the hope of finding traces of ancient life.



Billions of years ago, Mars was flush with lakes and rivers, potentially creating conditions conducive to microbial life. 



Nestled in the foothills of Mount Sharp, which is a towering mountain, Gediz Vallis might hold the key to understanding <a href="https://www.earth.com/news/how-mars-became-uninhabitable-after-being-life-supporting-ocean-world/" target="_blank" rel="noreferrer noopener">how Mars looked</a> as water dwindled on its surface.



Scientists aren't just interested in understanding the climate shift. The team is also investigating different features within the channel, including a debris mound aptly nicknamed “Pinnacle Ridge.”



Evidence suggests that rivers, wet debris flows, and dry avalanches have all left their signatures on this formation.



Intriguingly, the process of constructing a timeline of these events is well underway.



<h2 class="wp-block-heading" id="h-sulfur-stones-the-latest-martian-mystery">Sulfur stones: The latest Martian mystery</h2>



The sprawling field of sulfur stones, originally appearing as an unremarkable patch of light-colored terrain in images from NASA’s <a href="https://www.earth.com/news/stunning-photo-of-martian-space-potato-moon-phobos/" target="_blank" rel="noreferrer noopener">Mars Reconnaissance Orbiter</a>, has sprung a pleasant surprise.



A close inspection by Curiosity revealed that these sulfur stones were teeming with yellow crystals, a find unlike anything seen on Mars before.



The rover's instruments confirmed that the stones were pure sulfur - an unusual occurrence that raises more questions than it answers.



On our home planet, sulfur is usually linked with the presence of <a href="https://www.earth.com/news/water-frost-detected-on-mars-enormous-volcanoes/" target="_blank" rel="noreferrer noopener">volcanoes</a> and hot springs. Yet, no evidence on Mount Sharp suggests these phenomena as likely candidates.



Ashwin Vasavada is a Curiosity project scientist at NASA’s <a href="https://search.app?link=https%3A%2F%2Fwww.jpl.nasa.gov%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">Jet Propulsion Laboratory</a> in Southern California.



“We looked at the sulfur field from every angle - from the top and the side - and looked for anything mixed with the sulfur that might give us clues as to how it formed. We’ve gathered a ton of data, and now we have a fun puzzle to solve," said Vasavada.



<h2 class="wp-block-heading" id="h-treading-on-martian-spiderwebs">Treading on Martian "spiderwebs"</h2>



Having completed a thorough survey of the Gediz Vallis, Curiosity is all set to traverse the edge of the channel, capturing a few more panoramas before making its way to the boxwork region.



This formation of ridges, likened to spiderwebs sprawling across the surface, is believed to be linked to minerals settling into rock crevices and hardening over time. They have been left behind as the surrounding rock eroded.



“These ridges will include minerals that crystallized underground, where it would have been warmer, with salty liquid water flowing through. Early Earth microbes could have survived in a similar environment. That makes this an exciting place to explore,” said Kirsten Siebach, a Curiosity scientist from <a href="https://www.rice.edu/" target="_blank" rel="noreferrer noopener">Rice University</a> in Houston.



<h2 class="wp-block-heading" id="h-the-curious-legacy-of-curiosity">The curious legacy of Curiosity</h2>



Curiosity, a brainchild of NASA’s Jet Propulsion Laboratory managed by Caltech, continues to be a cornerstone of Martian exploration for NASA’s Science Mission Directorate. 



The Mars Reconnaissance Orbiter Project, under the management of the <a href="https://www.arizona.edu/" target="_blank" rel="noreferrer noopener">University of Arizona</a>, and its High-Resolution Imaging Science Experiment (HiRISE) instrument, constructed by BAE Systems, also play significant roles in taking our understanding of Mars to new heights.



Video Credit: NASA/JPL-Caltech/MSSS



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Sulfur stones and spiderwebs: Curiosity's latest discoveries on Mars

Curiosity, the renowned Mars rover from NASA, is enriching our...

A new study suggests that individual cells might be capable of learning - a behavior once thought exclusive to organisms with brains and complex nervous systems. 



The research, led by scientists at the <a href="https://www.crg.eu/" target="_blank" rel="noreferrer noopener">Center for Genomic Regulation</a> (CRG) in Barcelona and <a href="https://hms.harvard.edu/" target="_blank" rel="noreferrer noopener">Harvard Medical School</a> in Boston, challenges long-standing assumptions about the fundamental capabilities of cells.



“Rather than following pre-programmed genetic instructions, <a href="https://www.earth.com/news/animal-cells-capable-of-photosynthesis-created-for-the-first-time/" target="_blank" rel="noreferrer noopener">cells</a> are elevated to entities equipped with a very basic form of decision making based on learning from their environments,” explained study co-author Jeremy Gunawardena, an associate professor of systems biology at Harvard Medical School. 



The findings, published in <a href="http://dx.doi.org/10.1016/j.cub.2024.10.041" target="_blank" rel="noreferrer noopener">Current Biology</a>, could transform our understanding of life at its most basic level.



<h2 class="wp-block-heading" id="h-habituation-learning-without-a-brain">Habituation: Learning without a brain</h2>



The researchers focused on habituation, a simple form of learning where an organism gradually stops responding to a repeated stimulus - like how humans tune out the ticking of a clock or flashing lights.&nbsp;



While habituation has been extensively studied in animals with <a href="https://www.earth.com/news/how-black-widow-venom-attacks-the-nervous-system/" target="_blank" rel="noreferrer noopener">nervous systems</a>, whether similar behavior exists at the cellular level has been a contentious question.



Early experiments in the 20th century observed behavior resembling learning in the single-celled ciliate Stentor roeselii, but the findings were largely dismissed. In the 1970s and 1980s, more evidence of habituation emerged in other ciliates, and modern experiments have continued to build on these insights.



“These creatures are so different from animals with brains,” said Rosa Martinez, a co-author of the study and researcher at the CRG.



“To learn would mean they use internal molecular networks that somehow perform functions similar to those carried out by networks of neurons in brains. Nobody knows how they are able to do this, so we thought it is a question that needed to be explored.”&nbsp;



<h2 class="wp-block-heading" id="h-using-simulations-to-decode-cellular-learning">Using simulations to decode cellular “learning”</h2>



Instead of working with cells directly in the lab, the researchers turned to computer simulations to track the biochemical reactions that cells rely on to process information.&nbsp;



By simulating how molecular interactions change when exposed to repeated stimuli, the team uncovered evidence of <a href="https://www.earth.com/news/secrets-of-learning-how-our-brains-neurons-make-and-retrieve-memories/" target="_blank" rel="noreferrer noopener">learning</a>-like behavior.



The study focused on two common molecular circuits: negative feedback loops and incoherent feedforward loops.&nbsp;



Negative feedback is like a thermostat - it regulates processes by turning them off when a certain threshold is reached.&nbsp;



Incoherent feedforward loops act like a motion-activated light with a timer, triggering a process and its inhibitor simultaneously.



<h2 class="wp-block-heading" id="h-memories-formed-at-the-cellular-level">Memories formed at the cellular level</h2>



Simulations revealed that cells use these circuits to fine-tune their responses to repeated stimuli, replicating hallmark features of habituation seen in animals.&nbsp;



A critical discovery was the role of “timescale separation,” where some biochemical reactions occur much faster than others.



“We think this could be a type of ‘memory’ at the cellular level, enabling cells to both react immediately and influence a future response,” Martinez explained.



<h2 class="wp-block-heading" id="h-bridging-neuroscience-and-cognitive-science">Bridging neuroscience and cognitive science</h2>



The findings also offer new insights into a long-standing debate between neuroscientists and cognitive researchers about habituation.&nbsp;



Neuroscientists argue that stronger habituation occurs with more frequent or less intense stimuli, while cognitive scientists emphasize internal changes, finding habituation stronger with less frequent or more intense stimuli.



The study showed that both perspectives are valid. During habituation, cells respond less to frequent or weak stimuli, but after habituation, their response to similar stimuli is stronger.&nbsp;



“Neuroscientists and cognitive scientists have been studying processes which are basically two sides of the same coin,” Gunawardena said. “We believe that single cells could emerge as a powerful tool to study the fundamentals of learning.”



<h2 class="wp-block-heading" id="h-the-ability-of-cells-to-learn-and-remember-nbsp">The ability of cells to learn and remember&nbsp;</h2>



If confirmed through real-world experiments, these findings could have profound implications.&nbsp;



The ability of cells to “remember” might explain phenomena like cancer cells developing resistance to chemotherapy or <a href="https://www.earth.com/news/antibiotic-resistant-bacteria-have-been-found-in-clouds/" target="_blank" rel="noreferrer noopener">bacteria</a> becoming resistant to antibiotics. Both involve cells appearing to “learn” from their environment to survive.



The researchers used mathematical models to test various scenarios quickly, identifying those worth exploring in laboratory settings. This approach could save time and resources while accelerating discoveries.



<h2 class="wp-block-heading" id="h-a-computational-approach-to-biology">A computational approach to biology</h2>



“The moonshot in computational biology is to make life as programmable as a computer, but lab experiments can be costly and time-consuming,” Martinez said.&nbsp;



Her team works at the <a href="https://barcelonacollaboratorium.com/" target="_blank" rel="noreferrer noopener">Barcelona Collaboratorium</a>, a joint initiative designed to use mathematical modeling to tackle big biological questions.



“Our approach can help us prioritize which experiments are most likely to yield valuable results, saving time and resources and leading to new breakthroughs,” noted Martinez. “We think it can be useful to address many other fundamental questions.”



This research marks a significant step toward understanding learning and memory at the cellular level, potentially reshaping our view of what individual cells are capable of and opening new doors for medical and scientific exploration.



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Biological breakthrough: Cells can ‘learn’ like brains

A new study suggests that individual cells might be capable...

Bad habits are repetitive behaviors or patterns that may have negative consequences on physical health, mental well-being, relationships, or productivity. 



They often develop unconsciously and can be challenging to break because they are reinforced by habit loops, which consist of a cue, a routine, and a reward.



But what if you could easily change your habits? What if you had the power to take control of your brain's habit-making mechanism and use it to your advantage?



Enter cognitive neuroscience, a field that offers fresh insights into how our brains form habits. In a recent study, scientists at Trinity College Dublin have proposed a new approach to changing habits that promise lasting results.



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



Led by Dr. Eike Buabang, postdoctoral research fellow in the lab of Professor Claire Gillan, the study explores how habits drive our daily lives.



"Habits play a central role in our daily lives, from making that first cup of coffee in the morning to the route we take to work, and the routine we follow to prepare for bed," said Dr. Buabang.



"Our research reveals why these <a href="https://www.earth.com/news/happiness-influences-online-shopping-habits/" target="_blank" rel="noreferrer noopener">automatic behaviors</a> are so powerful - and how we can harness our brain's mechanisms to change them."



<h2 class="wp-block-heading" id="h-two-brain-systems">Two brain systems</h2>



Our habits are driven by two brain systems. One triggers automatic responses to familiar cues, while the other enables goal-directed control.



Take, for instance, the habit of scrolling through social media when you're bored - this is the result of an automatic response system. But when you put your phone away to focus on work - that's the goal-directed brain control system at work.



When these two systems are imbalanced, it can lead to action slips like entering an old password instead of the new one. 



In more severe cases, it can contribute to compulsive behaviors seen in conditions such as obsessive-compulsive disorder, substance-use disorders, and eating disorders.



<h2 class="wp-block-heading" id="h-switching-from-bad-habits-to-good-ones">Switching from bad habits to good ones</h2>



Understanding the interplay between these two systems can pave the way for personal development and clinical treatment of compulsive disorders. 



"Good and bad habits are two sides of the same coin - both arise when automatic responses overpower goal-directed control. By understanding this dynamic, we can start to use it to our own advantage, to both make and break habits," noted Dr. Buabang.



<h2 class="wp-block-heading" id="h-factors-involved-in-habit-change">Factors involved in habit change</h2>



Dr. Buabang's research provides a playbook for behavior change, bridging brain science with practical applications. The framework describes several factors crucial for influencing the balance between automatic responses and <a href="https://www.earth.com/news/how-to-set-realistic-goals-and-achieve-them-in-2024/" target="_blank" rel="noreferrer noopener">goal-directed control</a>.



<h3 class="wp-block-heading" id="h-repetition-and-reinforcement">Repetition and reinforcement</h3>



Repeating a behavior builds strong associations between cues and responses, while rewarding the behavior makes it more likely to be repeated. 



The same mechanism can be leveraged to break habits, by replacing old behaviors with new ones to create competing automatic responses.



<h3 class="wp-block-heading" id="h-environment">Environment</h3>



Your surroundings play a significant role in habit change. Tweaking your environment to make desired behaviors easier to access encourages good habits, while removing cues that trigger unwanted behavior disrupts the bad ones.



<h3 class="wp-block-heading" id="h-goal-directed-system">Goal-directed system</h3>



Knowing how to engage your goal-directed system can help strengthen and weaken habits. 



However, stress, time pressure, and fatigue can trigger a return to old patterns, so staying mindful and intentional is crucial when trying to break them.



<h2 class="wp-block-heading" id="h-from-theory-to-real-world-applications">From theory to real-world applications</h2>



The theory doesn't stop at habit change; it also opens the door to personalizing treatments based on how different people <a href="https://www.earth.com/news/how-long-does-it-take-to-form-a-habit/" target="_blank" rel="noreferrer noopener">form</a> and break habits.



"We are all different; depending on your neurobiology, it might make more sense to focus on avoiding cues than reducing stress or allowing yourself more time for your daily routine," said Professor Gillan.



These insights have far-reaching implications. They could reshape public health strategies and help policymakers design more effective health campaigns. 



"By working with - rather than against - how our brains naturally form habits, we can create strategies that make healthier choices more automatic at both <a href="https://www.earth.com/news/shopping-habits-have-remained-consistent-for-3500-years/" target="_blank" rel="noreferrer noopener">individual</a> and societal levels," noted Professor Gillan.



In conclusion, this new approach to habit change has the potential to revolutionize both personal development and the treatment of compulsive disorders. 



The exciting findings from the <a href="https://www.tcd.ie" target="_blank" rel="noreferrer noopener">Trinity College Dublin</a> team have provided a new avenue for tapping into our brain's potential, making habit change achievable and lasting.



The study is published in the journal <a href="https://www.cell.com/trends/cognitive-sciences/fulltext/S1364-6613(24)00266-3?_returnURL=https%3A%2F%2Flinkinghub.elsevier.com%2Fretrieve%2Fpii%2FS1364661324002663%3Fshowall%3Dtrue" target="_blank" rel="noreferrer noopener">Trends in Cognitive Sciences</a>.



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Brain science: A new approach to breaking bad habits

Bad habits are repetitive behaviors or patterns that may have...

There is a green deficit in our cities, and it's more serious than you think. A new study led by RMIT University in Australia highlights this glaring issue. The study measured access to nature in eight global cities and found most of them to be grossly deficient in canopy cover.



This is despite these cities having a significant number of <a href="https://www.earth.com/news/trees-have-an-amazing-ability-to-adapt-to-new-climates/" target="_blank" rel="noreferrer noopener">trees</a> in sight. The discrepancy lies in the lack of adequate "canopy cover" - the overhead layer of branches and leaves that provide shade, reducing temperatures and increasing green cover.



<h2 class="wp-block-heading" id="h-troubling-tree-deficit">Troubling tree deficit</h2>



Less than 30 percent of buildings in cities such as New York City, Amsterdam, Buenos Aires, and Denver were found to be in neighborhoods with adequate canopy cover.



New York and Amsterdam scored almost 0% for canopy cover, while a whopping 92 and 50 percent of their buildings, respectively, had views of at least three <a href="https://www.earth.com/news/resilient-trees-can-help-safeguard-cities-from-climate-change/" target="_blank" rel="noreferrer noopener">trees</a>.



This research, a collaborative effort with the Technical University of Munich, studied over 2.5 million buildings across eight cities using the "3-30-300" rule, an emerging sustainable cities measure.



This innovative rule states that every home, school, and workplace should have a view of at least three <a href="https://www.earth.com/news/more-than-one-third-of-the-worlds-trees-face-extinction/" target="_blank" rel="noreferrer noopener">trees</a>, be located in a neighborhood with at least 30% canopy cover, and be within 300 meters of a park.



<h2 class="wp-block-heading" id="h-canopy-cover-champions">Canopy cover champions</h2>



Among the cities studied, only Seattle and Singapore could pass the 30% canopy benchmark. In these cities, 45% and 75% of buildings, respectively, have the luxury of enjoying adequate shading.



But the access to parks is not consistent. Singapore and Amsterdam scored high, while Buenos Aires and New York City trailed behind.



<h2 class="wp-block-heading" id="h-need-for-more-canopy-cover">Need for more canopy cover</h2>



Dr. Thami Croeser, a lead researcher and an <a href="https://www.rmit.edu.au" target="_blank" rel="noreferrer noopener">RMIT University</a> research fellow, found it alarming that a majority of the buildings studied failed the 30% tree canopy test.



Considering that 2023 was the hottest year on record and 25% of the global population experienced dangerous levels of extreme heat, canopy cover is an urgent requirement to cool down our cities, noted Dr. Croeser.



<h2 class="wp-block-heading" id="h-benefits-of-tree-cover-in-cities">Benefits of tree cover in cities</h2>



"Previous research has shown depression, anxiety, obesity and heatstroke are more prevalent in urban areas that lack access to shady <a href="https://www.earth.com/news/planting-trees-is-important-but-reforestation-can-help-too/" target="_blank" rel="noreferrer noopener">tree</a> canopy and green open spaces," said Dr. Croeser.



Environmentally, urban trees play a critical role in improving air quality by absorbing pollutants such as carbon dioxide, nitrogen dioxide, and sulfur dioxide, while also filtering harmful particulate matter. 



Additionally, trees are essential for stormwater management, as their roots absorb rainfall and reduce the risk of flooding.



By storing carbon, urban forests help offset greenhouse gas emissions. They also provide vital habitats for birds, insects, and other wildlife, enhancing urban biodiversity.



<h2 class="wp-block-heading" id="h-insufficiency-of-current-practices">Insufficiency of current practices</h2>



Dr. Croeser is critical of current methods of street design or retrofitting, which tend to prioritize infrastructure like cabling and pipelines over tree growth.



He advocates for a change in our practice, to prioritize green infrastructure and incorporate trees into early stages of design.



<h2 class="wp-block-heading" id="h-struggles-of-urban-trees">Struggles of urban trees</h2>



Urban trees face a tough life. They are planted in compacted soil, covered with asphalt and lack proper water access.



Dr. Croeser argues that improving these conditions can greatly enhance the growth and longevity of urban trees, thus increasing canopy cover. The "3-30-300" rule might be relatively new, but it is rapidly gaining global acceptance.



This benchmark was devised by Dutch urban forestry expert Professor Cecil Konijnendijk.to set a definitive, evidence-based minimum for nature in cities.



<h2 class="wp-block-heading" id="h-future-research-directions">Future research directions</h2>



Professor Wolfgang Weisser from the <a href="https://www.tum.de/en/" target="_blank" rel="noreferrer noopener">Technical University of Munich</a> and Dirk Voets, Senior Advisor Geospatial at Cobra Groeninzicht, have expressed support of the "3-30-300" rule and are optimistic about its potential.



The study is a clarion call for us to reassess our urban designs. The findings reach out to a global audience to advocate for more harmonious co-existence with nature in our urban spaces.



The research may ultimately be a catalyst for significant change, leading us to build more sustainable, liveable, and delightful cities.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-024-53402-2" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Most cities lack sufficient canopy cover, despite visible trees

There is a green deficit in our cities, and it's...

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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



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.

Flu viruses are more flexible than expected

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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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