Today's Image of the Day from the European Space Agency features a Copernicus Sentinel-2 photograph of South Georgia, a remote and rugged island located in the southern Atlantic Ocean. 



"Linked with the South Sandwich Islands to form a British Overseas Territory, this southern Atlantic island is a haven for a vast array of wildlife," said <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Around five million seals call the islands home, as well as 65 million birds of 30 different species. Migrating whales and various fish species populate the surrounding waters and there is a large penguin population."



<h2 class="wp-block-heading" id="h-climate-and-wildlife-of-south-georgia">Climate and wildlife of South Georgia </h2>



The island is dominated by mountains, glaciers, and fjords. Its highest peak, Mount Paget, rises to 2,935 meters, making it one of the tallest in the region.



South Georgia’s location within the Antarctic Convergence gives it a cold, maritime climate. Although not part of the Antarctic Treaty System, its environment and <a href="https://www.earth.com/news/conservation-efforts-are-not-enough-to-save-antarctic-wildlife/" target="_blank" rel="noreferrer noopener">wildlife</a> are closely linked to Antarctica. 



The island is home to vast colonies of penguins, seals, and seabirds. The surrounding waters are rich with krill, providing an abundant food source for marine life.



<h2 class="wp-block-heading" id="h-penguins-adapted-to-harsh-environments">Penguins adapted to harsh environments </h2>



The most notable species found here are the king penguins, which are the second-largest penguin species in the world. South Georgia also hosts large populations of <a href="https://www.earth.com/news/what-makes-the-gentoo-penguin-the-worlds-fastest-swimming-bird/" target="_blank" rel="noreferrer noopener">gentoo</a> and macaroni penguins. 



The island's harsh climate, characterized by strong winds, snow, and cold temperatures, makes it a tough environment, but the penguins have adapted well. 



Their colonies - some of which number in the hundreds of thousands - can be found along the island's rugged coasts and beaches. 



The island’s isolation, combined with its plentiful food supply, makes it a critical breeding ground for these penguins.



<h2 class="wp-block-heading" id="h-history-of-south-georgia">History of South Georgia </h2>



The island has a history of exploration and exploitation. Captain James Cook first claimed South Georgia for Britain in 1775. 



During the late 19th and early 20th centuries, it became a hub for the <a href="https://www.earth.com/news/echoes-of-the-past-whalings-long-term-impact-on-genetic-diversity/" target="_blank" rel="noreferrer noopener">whaling</a> industry, with stations like Grytviken serving as operational centers. These stations have since been abandoned, and the island is now a haven for scientific research and ecotourism.



South Georgia is also notable for its role in Ernest Shackleton’s famed Endurance expedition. His crew reached the island in 1916 after an extraordinary open-boat journey from Elephant Island. Shackleton later died on South Georgia in 1922 and is buried in Grytviken.



<h2 class="wp-block-heading" id="h-pristine-nature-of-the-island">Pristine nature of the island</h2>



Today, South Georgia is a focus of conservation efforts. The eradication of invasive species, such as rats and reindeer, has been a significant success, allowing native wildlife to recover. 



Rats and mice were responsible for the decline of ground-nesting birds, including the South Georgia pipit, the island's only endemic bird. 



<a href="https://www.earth.com/news/reindeer-use-ultraviolet-vision-to-find-food-in-the-winter/" target="_blank" rel="noreferrer noopener">Reindeer</a>, which had been introduced for farming in the 19th century, caused extensive damage to the island’s vegetation, disrupting the habitat for native species.



South Georgia is uninhabited except for a small number of scientists and staff working at research stations and administrative facilities, emphasizing its role as a protected wilderness area and an essential site for understanding global environmental changes.



Its uninhabited status has helped preserve its pristine nature. Visitors to South Georgia must follow strict environmental guidelines to minimize human impact on this extraordinary island.



<h2 class="wp-block-heading" id="h-scientific-significance-of-remote-islands">Scientific significance of remote islands </h2>



Remote <a href="https://www.earth.com/news/plant-life-on-islands-loses-diversity-when-humans-arrive/" target="_blank" rel="noreferrer noopener">islands</a> are scientifically significant for several reasons. They often serve as unique ecosystems that can provide insights into evolutionary processes, biodiversity, and adaptation. 



Due to their isolation, species on remote islands may evolve differently from their mainland counterparts, resulting in the development of endemic species that exist nowhere else in the world. 



These islands also act as natural laboratories for studying the effects of climate change, human activity, and ecological interactions, as they are more vulnerable to disturbances. 



Moreover, remote islands can offer valuable information on the health of marine and terrestrial ecosystems, as their ecosystems are often less impacted by human-induced factors. This makes them ideal for studying natural processes in relatively undisturbed environments. 



The isolation of these islands can also help scientists study the patterns of species migration, colonization, and extinction.



Image Credit: ESA 



Like what you read? <a href="https://www.earth.com/subscribe/">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



—--



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

South Georgia: One of the most remote islands in the world

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

Today's Image of the Day from the European Space Agency features NGC 6744 - a large, barred spiral galaxy located approximately 30 million light-years away in the constellation Pavo.&nbsp;



The galaxy is often considered a close analog to the <a href="https://www.earth.com/news/uma3-u1-faintest-star-system-found-orbiting-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a> due to its similar structure and size, spanning about 175,000 light-years across.&nbsp;



<h2 class="wp-block-heading" id="h-euclid-space-mission-nbsp">Euclid space mission&nbsp;</h2>



The image was captured by the <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid</a> space telescope. NGC 6744 stands out as a prime example of the galaxies currently forming the majority of stars in the nearby universe, making it an ideal subject for study with the Euclid mission.&nbsp;



Euclid’s extensive field-of-view allows it to capture the entire galaxy, showcasing not only its large-scale spiral structure but also revealing intricate details on smaller scales across various wavelengths. These details include feather-like dust lanes, known as “spurs,” emerging from the spiral arms.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-6744">Star formation in NGC 6744</h2>



Euclid's observations enable scientists to count individual stars within NGC 6744, trace the distribution of stars and dust throughout the galaxy, and map the dust associated with the gas that fuels the development of new stars.&nbsp;



<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 a key process in the growth of galaxies, making these studies crucial for understanding galaxy evolution.



Researchers are utilizing Euclid’s data to explore the relationship between dust, gas, and star formation; to map the distribution of different stellar populations and identify regions of active star formation; and to investigate the underlying physics of spiral galaxy structures.&nbsp;



Spiral arms play a significant role in star formation by compressing gas, yet the precise mechanisms behind this process are still unclear. The presence of “spurs” along NGC 6744’s spiral arms offers valuable insights into the dynamics of star formation within these structures.



<h2 class="wp-block-heading" id="h-discovering-new-dwarf-galaxies-nbsp">Discovering new dwarf galaxies&nbsp;</h2>



Additionally, Euclid's dataset will help scientists identify clusters of old stars (globular clusters) and discover new dwarf galaxies around NGC 6744. 



Remarkably, Euclid has already identified a new dwarf satellite galaxy of NGC 6744 - a surprising discovery given that the galaxy has been studied extensively.



With Euclid’s detailed observations, scientists are gaining a deeper understanding of the processes shaping galaxies, providing essential clues to the evolution and appearance of the <a href="https://www.earth.com/news/universes-expansion-rate-hubble-tension-puzzles-astronomers/" target="_blank" rel="noreferrer noopener">universe</a>.



<h2 class="wp-block-heading" id="h-more-about-ngc-6744">More about NGC 6744</h2>



NGC 6744's disk is rich in star-forming regions and contains numerous young, bright blue stars. The galaxy's nucleus is slightly elongated and has a bar structure, which influences the motion of the stars and gas within it.&nbsp;



The spiral arms of NGC 6744 are well-defined and extend outward, wrapping around the central bar. 



Additionally, NGC 6744 has a smaller companion galaxy, NGC 6744A, which is interacting with it, adding to the complexity and interest of this distant system. 



<h2 class="wp-block-heading" id="h-types-of-spiral-galaxies">Types of spiral galaxies</h2>



<a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">Spiral galaxies</a> are one of the most common types of galaxies in the universe, characterized by their distinct, spiral-shaped structure.&nbsp;



The galaxies typically consist of a flat, rotating disk containing stars, gas, and dust, along with a central concentration of stars known as the bulge. This bulge is often surrounded by a halo of older stars.&nbsp;



The spiral arms, which extend from the central bulge, are regions of active star formation and are rich in young, hot stars, giving them a bright, bluish appearance.&nbsp;



These arms are also sites where interstellar gas and dust are concentrated, leading to the formation of new stars.&nbsp;



Spiral galaxies are classified into different types based on the tightness of their spirals and the size of their central bulge, with classifications ranging from tightly wound arms in Sa galaxies to more loosely wound arms in Sc galaxies. The <a href="https://www.earth.com/news/large-amount-of-dark-matter-may-be-missing-from-the-milky-way/" target="_blank" rel="noreferrer noopener">Milky Way</a>, our home galaxy, is a prime example of a spiral galaxy.



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



Pavo, which means "peacock" in Latin, is a constellation in the southern sky. It was named by the Dutch astronomer Petrus Plancius in the late 16th century, based on observations made during the Dutch explorations of the southern hemisphere. 



Pavo is one of the 12 constellations created by Plancius from the records of explorers Pieter Dirkszoon Keyser and Frederick de Houtman. 



The constellation is known for its distinctive shape, resembling a peacock with a long, curved tail. Pavo is not visible from most of the northern hemisphere, but it can be seen from the southern hemisphere, particularly during the winter months.



The constellation contains several interesting celestial objects, including the star Peacock, also known as Alpha Pavonis, which is the brightest star in the constellation. This star is a blue-white subgiant located about 179 light-years from Earth.



Image Credit: <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>/Euclid/Euclid Consortium/NASA&nbsp;



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Young stars illuminate a spiral galaxy in the constellation Pavo

Today's Image of the Day from the European Space Agency features the galaxy I Zwicky 18, which was captured in remarkable detail by the James Webb Space Telescope.



I Zwicky 18 is a blue compact dwarf <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">galaxy</a> located approximately 59 million light-years away in the constellation Ursa Major.&nbsp;



<h2 class="wp-block-heading" id="h-star-formation-in-i-zwicky-18">Star formation in I Zwicky 18</h2>



The galaxy is notable for its relatively young appearance and the fact that it contains very few heavy elements. These characteristics indicate that it has experienced little <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> compared to other galaxies of similar age.



“The galaxy was first identified by Swiss astronomer Fritz Zwicky in the 1930’s and resides roughly 59 million light-years from Earth,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>. “This galaxy has gone through several sudden bursts of star formation.”&nbsp;



According to ESA, I Zwicky 18 is typical of the kinds of galaxies that inhabited the early universe and is much smaller than our <a href="https://www.earth.com/news/runaway-star-j1249-36-spotted-trying-to-escape-our-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>.



<h2 class="wp-block-heading" id="h-webb-telescope-image-of-the-galaxy">Webb telescope image of the galaxy</h2>



“Two major starburst regions are embedded in the heart of the galaxy. The wispy brown filaments surrounding the central starburst region are bubbles of gas that have been heated by stellar winds and intense ultraviolet radiation unleashed by hot, young stars,” said ESA.



“A companion galaxy resides nearby to the dwarf galaxy, which can be seen at the bottom of the wider-field image. The companion may be interacting with the dwarf galaxy and may have triggered that galaxy's recent star formation.”&nbsp;



ESA explained that the “orange blobs” surrounding the galaxy are the dim glow from ancient fully formed galaxies at much larger distances.



<h2 class="wp-block-heading" id="h-key-characteristics-of-i-zwicky-18">Key characteristics of I Zwicky 18</h2>



As previously mentioned, the galaxy has a very low abundance of elements heavier than hydrogen and helium, suggesting that it has not undergone significant stellar processing.



<h3 class="wp-block-heading" id="h-young-stellar-population-nbsp">Young stellar population&nbsp;</h3>



Despite its old age, I Zwicky 18 contains many young, hot stars. This suggests that it might have experienced a burst of <a href="https://www.earth.com/news/hubble-detects-awe-inspiring-newborn-star/" target="_blank" rel="noreferrer noopener">star formation</a> relatively recently in its history.



<h3 class="wp-block-heading" id="h-interstellar-medium-nbsp">Interstellar medium&nbsp;</h3>



The galaxy has a high density of gas, which is a prime ingredient for star formation. This gas is mostly in the form of hydrogen.



<h3 class="wp-block-heading" id="h-unusual-characteristics">Unusual characteristics</h3>



Its characteristics are more typical of primordial galaxies found in the early universe, making it a valuable object of study for understanding galaxy formation and evolution.



Ultimately, I Zwicky 18 provides insights into the conditions and processes that might have been prevalent in the early universe.



<h3 class="wp-block-heading" id="h-life-cycles-of-stars-and-dust">Life cycles of stars and dust</h3>



The image was captured as part of a Webb program to study the life cycle of dust in I Zw 18.&nbsp;



“Scientists are now building off of previous research with Hubble obtained at optical wavelengths, studying individual dusty stars in detail with Webb’s equivalent spatial resolution and sensitivity at infrared wavelengths.”&nbsp;



ESA noted that this galaxy is of particular interest as its content of elements heavier than helium is one of the lowest of all known <a href="https://www.earth.com/news/early-galaxy-formation-occurred-much-faster-than-we-thought/" target="_blank" rel="noreferrer noopener">galaxies</a> in the local universe.&nbsp;



“Such conditions are thought to be similar to those in some of the first star-forming galaxies at high redshift, so the Webb study of I Zw 18 should shed light on the life-cycle of stars and dust in the early universe.”



<h2 class="wp-block-heading" id="h-the-constellation-ursa-major">The constellation Ursa Major </h2>



Ursa Major, also known as the Great Bear, is one of the most prominent and easily recognizable constellations in the northern sky. 



Its name, "Ursa Major," means "Great Bear" in Latin, and it has been a significant part of various mythologies and star lore across cultures for thousands of years. 



One of the most famous asterisms within Ursa Major is the Big Dipper, a group of seven bright stars that form a shape resembling a ladle or dipper. The Big Dipper is often used as a navigation tool because it points to Polaris, the North Star, located in the nearby constellation Ursa Minor.



Ursa Major is best viewed in the northern hemisphere and is circumpolar, meaning it is visible year-round for much of the Northern Hemisphere. Its position changes with the seasons, rotating around Polaris, the North Star.



Image Credit: NASA/ESA/CSA James Webb Space Telescope



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Dwarf galaxy provides a window into the early universe

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 southern constellation Reticulum. The image was captured by the James Webb Space Telescope. 



"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 ionized 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 who study stellar evolution and the life cycle of stars.



The structure of NGC 1559 includes well-defined spiral arms that contain 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>.



<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



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Spiral galaxy NGC 1559 is a loner in outer space

Today's Image of the Day from NASA Earth Observatory features smoke from wildfires across the southeastern region of South Korea.



NASA noted that dozens of <a href="https://www.earth.com/news/experts-have-identified-the-key-driver-of-severe-wildfires-in-canada/" target="_blank" rel="noreferrer noopener">wildland fires</a> broke out as dry winds swept across the country.



“Blazes began igniting on March 21, prompting evacuations as well as the deployment of thousands of personnel and more than 100 helicopters to combat the fires.”



<h2 class="wp-block-heading" id="h-smoke-from-wildfires-in-south-korea">Smoke from wildfires in South Korea </h2>



“Smoke from some of the larger fires is visible in this image, acquired by the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Aqua satellite on March 22,” said <a href="https://earthobservatory.nasa.gov/images/154083/outbreak-of-fire-across-south-korea" target="_blank" rel="noreferrer noopener">NASA</a>.



One of the plumes is streaming from a wildfire near Andong in Uiseong County, where hundreds of people were evacuated.&nbsp;



“To the south, another large smoke plume originated from rural Sancheong County,” noted NASA.



‘A large, fast-moving fire had burned over 500 hectares (2 square miles) by the evening of March 22, the Associated Press reported, and caused multiple injuries and deaths.”&nbsp;



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



The devastating wildfires in South Korea have caused significant loss of life and property. The fires have claimed at least 24 lives, including four firefighters and a helicopter pilot who crashed while assisting in the efforts. 



Approximately 27,000 residents have been forced to evacuate as the flames have burned more than 17,000 hectares of land.&nbsp;



The fires have caused extensive damage to infrastructure and cultural heritage sites. More than 200 structures, including historical structures such as a seventh century Buddhist temple, have been destroyed.



The wildfires have spread rapidly. Lee Byung-doo, a forest disaster expert at the National Institute of Forest Science, told The Guardian that the Uiseong fire spread with “unimaginable” <a href="https://www.earth.com/news/fast-wildfires-are-gaining-even-more-speed/" target="_blank" rel="noreferrer noopener">speed</a>.&nbsp;



Dry, windy conditions and record-high temperatures have made the fires difficult to contain.&nbsp;



The government has elevated the crisis alert to its highest level, deploying thousands of firefighters and over 130 helicopters to combat the blazes.



The hardest hit regions have been designated as disaster areas to expedite recovery efforts.



<h2 class="wp-block-heading" id="h-climate-change-and-wildfire-dynamics-nbsp">Climate change and wildfire dynamics&nbsp;</h2>



<a href="https://www.earth.com/news/extreme-fire-risk-has-grown-exponentially-in-a-hotter-climate/" target="_blank" rel="noreferrer noopener">Climate change</a> is significantly influencing wildfire intensity by creating conditions that make fires more frequent, larger, and more severe.&nbsp;



Rising global temperatures lead to prolonged <a href="https://www.earth.com/news/climate-change-is-now-the-driving-force-behind-droughts/" target="_blank" rel="noreferrer noopener">droughts</a>, drier vegetation, and higher evaporation rates, all of which contribute to an increased likelihood of wildfires.&nbsp;



As heat waves become more extreme and prolonged, forests and grasslands become more susceptible to ignition, whether from natural sources like lightning or human activity.



Shifting precipitation patterns also play a role in wildfire dynamics. Some regions experience less frequent but more intense rainfall, leading to rapid vegetation growth that, once dried out, becomes highly flammable fuel for fires.&nbsp;



In other areas, persistent droughts reduce soil moisture and weaken plant health, making ecosystems more vulnerable to burning.



<h2 class="wp-block-heading" id="h-rapid-and-unpredictable-fires-nbsp">Rapid and unpredictable fires&nbsp;</h2>



The warming climate is also altering wind patterns, which can spread fires more rapidly and unpredictably. Stronger winds carry embers over long distances, igniting new fires far from the original source.&nbsp;



Additionally, changes in seasonal patterns, such as earlier snowmelt and delayed autumn rains, extend the wildfire season, allowing fires to burn longer and with greater intensity.



These intensifying wildfires have cascading effects on ecosystems and human communities. Increased fire severity can lead to soil degradation, loss of biodiversity, and long-term changes in forest composition.&nbsp;



In populated areas, wildfires pose serious threats to human life, property, and air quality, with smoke from large fires contributing to respiratory health issues and worsening climate change by releasing massive amounts of carbon dioxide into the atmosphere.



<h2 class="wp-block-heading" id="h-an-escalating-cycle-nbsp">An escalating cycle&nbsp;</h2>



Ultimately, climate change and wildfires form a dangerous feedback loop. As wildfires become more intense and widespread, they release more carbon, accelerating climate change and increasing future fire risks.&nbsp;



This escalating cycle highlights the urgent need for strategies to mitigate climate change and improve wildfire management through policies that address both emissions reductions and adaptive land-use practices.



Image Credit: NASA Earth Observatory&nbsp;



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



Check us out on <a href="https://www.earth.com/earthsnap/" target="_blank" rel="noreferrer noopener">EarthSnap</a>, a free app brought to you by <a href="https://www.linkedin.com/in/eric-ralls/" target="_blank" rel="noreferrer noopener">Eric Ralls</a> and Earth.com.



-----

Smoke and destruction: South Korea’s wildfire crisis

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

Space journeys that stretch far beyond home are on the horizon. Crews heading for Mars will face conditions quite different from those on Earth, and researchers have been working to figure out what might happen to the human body during these extended voyages. 



Kidneys have been a big question mark. Recent work reveals that these important organs could face more trouble than previously assumed, including a higher risk of stones and lasting damage.



Several studies have hinted at health concerns for astronauts ever since humans first ventured outside Earth’s protective zone, but the new findings shed light on why such problems arise in the kidneys. 



Dr. Keith Siew from the <a href="https://www.londontubularcentre.org/" target="_blank" rel="noreferrer noopener">London Tubular Centre</a>, based at the UCL Department of Renal Medicine, and his colleagues have pieced together a detailed picture of what happens when living beings - human and otherwise - experience space-like conditions for weeks to years.



<h2 class="wp-block-heading" id="h-space-missions-and-human-kidneys">Space missions and human kidneys</h2>



The latest study was conducted under a UCL-led initiative involving over 40 institutions on five continents.



The team considered data from 20 different research cohorts and samples linked to over 40 Low Earth orbit missions to the <a href="https://www.earth.com/news/nasa-says-the-international-space-station-is-too-clean-add-microbes/" target="_blank" rel="noreferrer noopener">International Space Station</a>, plus 11 simulations with mice and rats. 



The work is described as the largest analysis of kidney health in spaceflight so far and includes the first health dataset for commercial astronauts. 



It also involved seven simulations in which mice were exposed to radiation that mimicked up to 2.5 years of cosmic travel beyond <a href="https://www.earth.com/earthpedia-articles/earths-magnetic-field-origin-structure-and-impact-on-humanity/" target="_blank" rel="noreferrer noopener">Earth’s magnetic field</a>. 



Findings revealed that the structure and function of the kidneys are altered by spaceflight, with galactic radiation causing permanent damage that would jeopardize any long-distance mission.



<h2 class="wp-block-heading" id="h-kidneys-and-deep-space-radiation">Kidneys and deep space radiation</h2>



Astronauts in Low Earth orbit still benefit from partial shielding by our planet’s magnetic field. 



Only 24 people - the ones who went to the moon - have been exposed to the full brunt of Galactic Cosmic Radiation for short trips of about 6-12 days. 



Nobody has ventured on a years-long mission beyond the Earth’s magnetic boundary, so it was unclear how organs might hold up under <a href="https://www.earth.com/news/voyager-spacecraft-fighting-survival-cosmic-threats-outside-our-solar-system/" target="_blank" rel="noreferrer noopener">more extreme conditions</a>.



As part of the new study, researchers found that certain kidney tubules, which control delicate balances of salts and calcium, shrink after just a month in <a href="https://www.earth.com/news/microgravity-causes-big-problems-with-human-gene-expression/" target="_blank" rel="noreferrer noopener">microgravity</a>. 



The kidneys also process salts in a way that increases the likelihood of kidney stone formation. 



This new insight shifts the focus away from an older assumption that stones in space result mainly from bone loss causing elevated calcium in urine.



<h2 class="wp-block-heading" id="h-longer-distance-more-radiation">Longer distance, more radiation</h2>



The research highlighted that cosmic radiation cannot be fully blocked by typical shielding. When mice were given doses of simulated <a href="https://www.swpc.noaa.gov/phenomena/galactic-cosmic-rays" target="_blank" rel="noreferrer noopener">Galactic Cosmic Radiation</a> equal to a mission length of up to 2.5 years, the animals showed irreversible kidney damage. 



Some of the key observations point to changes in how the kidneys manage vital minerals, which impacts long-term health during space travel.



“We know what has happened to astronauts on the relatively short space missions conducted so far, in terms of an increase in health issues such as kidney stones,” explained Dr. Siew. 



“What we don’t know is why these issues occur, nor what is going to happen to astronauts on longer flights such as the proposed <a href="https://www.earth.com/news/mars-curiosity-rover-finds-sulfur-crystals-martian-rock-hints-at-possible-life/" target="_blank" rel="noreferrer noopener">mission to Mars</a>.”



If scientists don’t develop new ways to protect the kidneys, any astronaut that makes it to <a href="https://www.earth.com/news/largest-organic-molecules-ever-found-on-mars-confirm-life-forming-chemistry-is-possible/" target="_blank" rel="noreferrer noopener">Mars</a> will likely need dialysis on the way home or upon arrival.



"We know that the kidneys are late to show signs of radiation damage; by the time this becomes apparent it’s probably too late to prevent failure, which would be catastrophic for the mission’s chances of success," Dr. Siew concluded.



<h2 class="wp-block-heading" id="h-human-kidneys-and-future-space-travel">Human kidneys and future space travel</h2>



Space agencies have been aware since the 1970s that journeys outside our planet’s natural defenses lead to health concerns involving bones, eyes, and the <a href="https://www.earth.com/news/a-century-of-progress-in-the-fight-against-cardiovascular-disease/" target="_blank" rel="noreferrer noopener">cardiovascular system</a>. 



This new work puts fresh focus on the kidneys. It also highlights the importance of managing both microgravity and radiation, especially with more ambitious missions on the table.



“Our study highlights the fact that if you’re planning a space mission, kidneys really matter. You can’t protect them from galactic radiation using shielding," noted Professor Stephen B. Walsh from the London Tubular Centre, UCL Department of Renal Medicine.



"But as we learn more about renal biology it may be possible to develop technological or pharmaceutical measures to facilitate <a href="https://www.earth.com/news/space-travel-has-unexpected-effects-on-gut-health/" target="_blank" rel="noreferrer noopener">extended space travel</a>."



Any drugs developed for astronauts may also be beneficial here on Earth. For instance, by enabling cancer patients’ kidneys to tolerate higher doses of radiotherapy, which is currently an impediment to that form of treatment.



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



Though this work only outlines organ changes up to two and a half years, it stands as the most comprehensive data currently available for that timescale. 



Researchers say that pinpointing these risks is a vital first step before reliable solutions can be introduced. 



The study’s international collaboration suggests momentum is building to safeguard astronauts’ kidneys, and future innovations could reach beyond space missions to help patients on Earth.



Experts note that learning how to handle the combined effects of microgravity and cosmic radiation will be key to making ambitious missions safer. 



With evidence pointing to serious kidney challenges, careful planning will be needed to keep crews healthy on journeys that last far longer than any undertaken before.



The full study was published in the journal <a href="https://www.nature.com/articles/s41467-024-49212-1" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.



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



-----

Astronauts can survive a trip to Mars, but one critical internal organ will likely fail

Space journeys that stretch far beyond home are on the...

Wind and Earth’s spin keep the ocean’s surface currents constantly moving, and those currents are the main reason floating plastic and other debris travel so far. A prime example of this phenomenon is the Great Pacific Garbage Patch.



Two types of currents do most of the work: geostrophic currents, which form from the balance between gravity and Earth’s rotation, and Ekman currents, which wind drives directly. Together, they carry debris across vast stretches of the ocean.



As these currents swirl, they naturally pull trash toward the centers of the world’s five subtropical gyres - massive, slow-moving whirlpools in the ocean. Over time, these zones turn into plastic hotspots, where all kinds of floating junk gathers.



The North Pacific subtropical gyre is the most infamous of the bunch. That’s home to the Great Pacific Garbage Patch, the biggest and most studied plastic pile-up in the ocean. 



It’s drawn the attention of scientists, environmentalists, and the public alike. And not surprisingly, many of the first large-scale ocean cleanup projects have started right there.



<h2 class="wp-block-heading" id="h-understanding-the-great-pacific-garbage-patch">Understanding the Great Pacific Garbage Patch</h2>



The Great Pacific Garbage Patch is a massive collection of plastic debris, abandoned fishing gear, and other trash that accumulates in the North Pacific Ocean. 



These plastics can take hundreds of years to break down, and even when they do, they become tiny microplastics that enter marine food chains. 



This swirling soup of litter poses a big threat to marine life, seabirds, and even human health when contaminated seafood ends up on our plates.



You might picture the patch as a giant floating island of trash, but in reality, it’s more like a massive zone of scattered debris. 



This makes it difficult to clean up, as much of the garbage is tiny bits of plastic dispersed throughout the water. 



<h2 class="wp-block-heading" id="h-smarter-alternative-hiding-in-plain-sight">Smarter alternative hiding in plain sight</h2>



Instead of chasing the trash, scientists now suggest using the ocean’s own natural flow to do the work. A new study has mapped out zones where water tends to converge and pull debris into tight pockets.



“Instead of boats slowly trawling and burning fuel, they can hold their position and keep the nets steady at a location where currents funnel and aggregate drifting objects,” said <a href="https://www.psi.edu/staff/profile/rodrigo-duran/" target="_blank" rel="noreferrer noopener">Rodrigo Duran</a>, a research scientist at the <a href="https://www.psi.edu/" target="_blank" rel="noreferrer noopener">Planetary Science Institute</a>, and co-author of the study.



<h2 class="wp-block-heading" id="h-ocean-patterns-pull-trash-into-zones">Ocean patterns pull trash into zones</h2>



The team, led by <a href="https://www.researchgate.net/profile/Luca_Kunz" target="_blank" rel="noreferrer noopener">Luca Kunz</a> from the University of Hamburg, used over 20 years of satellite and drifter data to spot high-traffic areas for floating <a href="https://www.earth.com/news/ocean-currents-may-soon-clean-up-waste-thanks-to-space-tech/" target="_blank" rel="noreferrer noopener">debris</a>. 



These zones, called Transient Attracting Profiles (<a href="https://ui.adsabs.harvard.edu/abs/2024OcSci..20.1611K/abstract" target="_blank" rel="noreferrer noopener">TRAPs</a>), are temporary regions where swirling currents push trash together.



TRAPs form when four eddies - circular currents - spin in just the right pattern. About 60% of the time, this <a href="https://www.earth.com/news/critical-ocean-current-may-be-more-stable-than-previously-thought/" target="_blank" rel="noreferrer noopener">pattern</a> pulls debris into a stable zone roughly 60 miles (96 kilometers) wide. Most of these zones stick around for about six days.



<h2 class="wp-block-heading" id="h-why-this-changes-cleanup-strategy">Why this changes cleanup strategy</h2>



Instead of moving across hundreds of miles, crews could now wait at known TRAP locations. When positioned right, nets could skim off trash that is funneled in by the current.



That saves fuel, time, and effort - and reduces the environmental cost of sweeping up the <a href="https://www.earth.com/news/earths-oceans-are-rapidly-changing-colors-matching-climate-predictions/" target="_blank" rel="noreferrer noopener">ocean</a>.



<h2 class="wp-block-heading" id="h-more-than-just-ocean-trash">More than just ocean trash</h2>



While TRAPs are useful for plastic cleanup, Duran says they could also be used for search and rescue, cargo loss, oil spill containment, or tracking volcanic ash and wildfire smoke as it drifts across the <a href="https://www.earth.com/news/climate-change-is-draining-nutrients-from-the-oceans-surface/" target="_blank" rel="noreferrer noopener">ocean</a> and air.



“This can even be used for atmospheric data,” Duran said, pointing to how the technique can predict movement across multiple systems.



<h2 class="wp-block-heading" id="h-why-past-predictions-fell-short">Why past predictions fell short</h2>



Previous models tried to guess where trash was heading based on <a href="https://www.sciencedirect.com/science/article/abs/pii/030193229090034G" target="_blank" rel="noreferrer noopener">Lagrangian simulations</a>, which track particles drifting on oceans over time. But at the smaller scale - about 1 to 10 miles (1.6 to 16 kilometers) - those methods break down.



TRAPs flip the question. Instead of asking where an object will go, they ask: where will things gather? That shift makes all the difference.



<h2 class="wp-block-heading" id="h-testing-the-patterns">Testing the patterns</h2>



To verify these zones, the team analyzed how drifters (floating sensors that move with surface currents) behaved around TRAPs. Most stayed near a TRAP for an average of six days. A few stuck around for over a month.



Researchers also noticed that drifters weren’t just spinning in circles. They were pulled straight into a TRAP, then funneled along its length - like getting sucked into a current and pushed out the other side.



<h2 class="wp-block-heading" id="h-how-this-can-change-everything">How this can change everything</h2>



The most effective TRAPs form in clusters of four eddies with alternating spin directions. These structures appear often in areas of high turbulence, like near <a href="https://www.fisheries.noaa.gov/west-coast/science-data/oceanography-northern-california-current-study-area" target="_blank" rel="noreferrer noopener">California’s upwelling zone</a> or around the <a href="https://hilo.hawaii.edu/~kenhon/GEOL205/Chain/default.htm" target="_blank" rel="noreferrer noopener">Hawaiian Ridge</a>.



Tracking them in real time could help cleanup crews navigate better and use far fewer resources. Long-lasting TRAPs, in particular, offer a clear target: the longer they exist, the more plastic they tend to gather.



<h2 class="wp-block-heading" id="h-what-s-coming-for-ocean-trash-cleanup">What’s coming for ocean trash cleanup</h2>



This technique isn’t just theory. It’s backed by decades of observations and tested with real ocean data. Cleanup crews could start using TRAP tracking to guide where and when they deploy nets.



As satellite monitoring improves and new missions deliver higher-resolution data, smaller TRAPs near coastlines may also be tracked more easily.



“It’s a very exciting time,” Duran remarked. The scale of the garbage patch is overwhelming, but knowing where and when debris gathers gives crews a fighting chance.&nbsp;



If cleanup systems can act more like filters than drag nets, sitting still while the ocean delivers the trash, then this could mark a shift in how we tackle plastic pollution at sea.



The study is published in <a href="https://www.nature.com/articles/s41598-018-22939-w" target="_blank" rel="noreferrer noopener">Ocean Science</a>.



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



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



-----

New ideas on how to cleanup the 'Great Pacific Garbage Patch'

Wind and Earth’s spin keep the ocean’s surface currents constantly...

NASA’s Curiosity rover has made another remarkable discovery on Mars - the largest organic compounds ever detected on the Red Planet. 



These <a href="https://www.youtube.com/watch?v=wektNJExGks" target="_blank" rel="noreferrer noopener">molecules</a>, discovered in a rock sample drilled in 2013, offer fresh insights into the potential of Mars to support life.



The findings suggest that <a href="https://www.earth.com/news/mars-curiosity-rover-finds-sulfur-crystals-martian-rock-hints-at-possible-life/" target="_blank" rel="noreferrer noopener">Mars</a> might have hosted more advanced prebiotic chemistry than scientists had assumed.



Inside Curiosity’s onboard mini-lab called SAM, scientists identified three organic molecules: decane, undecane, and dodecane. 



These compounds contain 10, 11, and 12 carbon atoms, respectively. The researchers believe they are remnants of fatty acids.



<h2 class="wp-block-heading" id="h-understanding-fatty-acids-the-basics">Understanding fatty acids - the basics</h2>



On Earth, fatty acids play a big role in the foundation of life - they’re key players in what makes cells work. Alongside proteins, carbohydrates, and nucleic acids, fatty acids help build and maintain living organisms. 



One of their main jobs is forming <a href="https://www.earth.com/news/how-did-the-first-cells-life-form-on-earth-scientists-think-they-finally-figured-it-out/" target="_blank" rel="noreferrer noopener">cell membranes</a>. They link up with other molecules to create phospholipids, which act like a flexible, protective skin around every cell. 



Without fatty acids, cells wouldn’t have that structure or protection, and life as we know it would fall apart - literally.



They also help cells communicate and stay energized. Fatty acids store energy more efficiently than carbs or proteins, so your body taps into them when it needs a long-lasting fuel source. 



Plus, they help make signaling molecules that tell your cells how to grow, heal, and respond to their environment. 



So while they might not get as much attention as DNA or proteins, fatty acids quietly keep the whole operation running behind the scenes.



Detecting these molecules on Mars is a thrilling step. It shows that <a href="https://www.earth.com/news/did-mars-once-host-life-we-finally-know-where-to-look/" target="_blank" rel="noreferrer noopener">complex chemistry</a> did occur there.



<h2 class="wp-block-heading" id="h-long-awaited-sample-yields-new-surprises">Long-awaited sample yields new surprises</h2>



<a href="https://science.nasa.gov/mission/msl-curiosity/" target="_blank" rel="noreferrer noopener">Curiosity</a> drilled into the rock target “Cumberland” on May 19, 2013. The sample came from a location called Yellowknife Bay inside Gale Crater. 



At the time, scientists believed the area resembled an ancient lakebed. That guess turned out to be correct.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/Mars-Curiosity_Cumberland-rock_sample-drilling_organic-molecules_NASA_1big-1.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/Mars-Curiosity_Cumberland-rock_sample-drilling_organic-molecules_NASA_1s.webp" alt="NASA's Curiosity rover drilled into this rock target, &quot;Cumberland,&quot; and collected a powdered sample of material from the rock's interior. Curiosity used the Mars Hand Lens Imager camera on the rover’s arm to capture this view of the hole in Cumberland on the same sol as the hole was drilled. The diameter of the hole is about 0.6 inches. The depth of the hole is about 2.6 inches. Credit: NASA/JPL-Caltech/MSSS" class="wp-image-1963755"/></a><figcaption class="wp-element-caption">NASA's Curiosity rover drilled into this rock target, "Cumberland," and collected a powdered sample of material from the rock's interior. Curiosity used the Mars Hand Lens Imager camera on the rover’s arm to capture this view of the hole in Cumberland on the same sol as the hole was drilled. The diameter of the hole is about 0.6 inches. The depth of the hole is about 2.6 inches. Click to enlarge. Credit: NASA/JPL-Caltech/MSSS</figcaption></figure>



The rock was rich in clay, sulfur, and nitrates. All three materials help preserve organic compounds. Also present was methane with a carbon signature that, on Earth, often points to the presence of <a href="https://www.earth.com/news/detecting-life-on-mars-a-breakthrough-in-space-research/" target="_blank" rel="noreferrer noopener">life</a>.



“There is evidence that <a href="https://www.earth.com/news/mars-water-reservoir-discovered-medusae-fossae-formation-two-miles-deep/" target="_blank" rel="noreferrer noopener">liquid water existed</a> in Gale Crater for millions of years and probably much longer, which means there was enough time for life-forming chemistry to happen in these crater-lake environments on Mars,” said Daniel Glavin, senior scientist at NASA’s <a href="https://www.nasa.gov/goddard/" target="_blank" rel="noreferrer noopener">Goddard Space Flight Center</a>.



<h2 class="wp-block-heading" id="h-serendipitous-discovery-of-molecules">Serendipitous discovery of molecules</h2>



The discovery came during an unrelated experiment. Scientists were searching for amino acids in the Cumberland sample. They heated the sample and measured released gases. 



No amino acids were present. But instead, the experts found small amounts of decane, undecane, and dodecane.



These molecules could have broken off from longer ones during heating. Scientists traced them back to possible parent compounds: undecanoic acid, dodecanoic acid, and tridecanoic acid.



To confirm their findings, the researchers recreated the process in labs on Earth. They added undecanoic acid to Mars-like clay and heated it. It released decane, just like the <a href="https://www.earth.com/news/wave-ripples-discovered-mars-surface-indicate-liquid-water-present-4-billion-years-ago/" target="_blank" rel="noreferrer noopener">Martian sample</a> had.



<h2 class="wp-block-heading" id="h-martian-molecules-may-hint-at-past-life">Martian molecules may hint at past life</h2>



One interesting detail emerged. The detected fatty acids seem longer than those usually formed by geological activity. Non-biological processes tend to produce shorter chains - usually with fewer than 12 carbon atoms.



Cumberland’s molecules had 11 to 13 carbon atoms. That suggests either a unique chemical process or possible signs of past biology. However, SAM’s tools cannot detect the longest chains reliably.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/Mars-Curiosity_Cumberland-rock_Hydrocarbons_organic-molecules-discovery_NASA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/Mars-Hydrocarbons_discovery_Curiosity-Rover_Cumberland-rock_illustration_NASA_1s-1.webp" alt="The long-chain organic molecules decane, undecane, and dodecane. These are the largest organic molecules discovered on Mars to date. They were detected in a drilled rock sample called &quot;Cumberland&quot; that was analyzed by the Sample Analysis at Mars lab inside the belly of NASA's Curiosity rover. The rover, whose selfie is on the right side of the image, has been exploring Gale Crater since 2012. An image of the Cumberland drill hole is faintly visible in the background of the molecule chains. Credit: NASA/Dan Gallagher" class="wp-image-1963756"/></a><figcaption class="wp-element-caption">The long-chain organic molecules decane, undecane, and dodecane. These are the largest organic molecules discovered on Mars to date. They were detected in a drilled rock sample called "Cumberland" that was analyzed by the Sample Analysis at Mars lab inside the belly of NASA's Curiosity rover. The rover, whose selfie is on the right side of the image, has been exploring Gale Crater since 2012. An image of the Cumberland drill hole is faintly visible in the background of the molecule chains. Click to enlarge. Credit: NASA/Dan Gallagher</figcaption></figure>



“Our study proves that, even today, by analyzing Mars samples we could detect chemical signatures of past life, if it ever existed on Mars,” said Caroline Freissinet, the study’s lead author.



<h2 class="wp-block-heading" id="h-why-this-matters-for-future-missions">Why this matters for future missions</h2>



The research supports the idea that organic molecules can survive Mars’s harsh conditions. <a href="https://www.earth.com/news/astronauts-can-survive-mars-space-journey-but-their-kidneys-will-be-permanently-damaged/" target="_blank" rel="noreferrer noopener">Radiation and oxidation</a> often destroy organic molecules over time. 



The preservation in Cumberland gives scientists hope for future discoveries.



Curiosity’s instruments can only do so much. That’s why scientists are eager to return Mars samples to Earth.



“We are ready to take the next big step and bring <a href="https://www.earth.com/news/astonishing-discovery-of-minerals-on-mars-hints-at-a-habitable-past/" target="_blank" rel="noreferrer noopener">Mars</a> samples home to our labs to settle the debate about life on Mars,” stated Glavin.



<h2 class="wp-block-heading" id="h-search-for-life-linked-molecules">Search for life-linked molecules</h2>



​NASA's Curiosity rover continues its mission inside <a href="https://science.nasa.gov/resource/a-guide-to-gale-crater/" target="_blank" rel="noreferrer noopener">Gale Crater</a>, exploring rock layers to better understand Mars’s ancient environments. 



The Sample Analysis at Mars (<a href="https://ssed.gsfc.nasa.gov/sam/" target="_blank" rel="noreferrer noopener">SAM</a>) tool remains key to these investigations. Every new sample adds another clue to a much larger puzzle.



With each discovery, scientists move one step closer to exploring one of the oldest and most profound questions we’ve ever asked: Did life ever exist on Mars, and if so, what traces of it remain locked beneath the planet’s surface?



<a href="https://youtu.be/wektNJExGks" target="_blank" rel="noreferrer noopener">Watch NASA's video about this discovery here...</a>



-----



This research was supported by NASA’s&nbsp;<a href="https://mars.nasa.gov/" target="_blank" rel="noreferrer noopener">Mars Exploration Program</a>.&nbsp;Curiosity is managed by NASA’s&nbsp;Jet Propulsion Laboratory (<a href="https://www.jpl.nasa.gov/missions/mars-science-laboratory-curiosity-rover-msl/" target="_blank" rel="noreferrer noopener">JPL</a>)&nbsp;in Southern California.&nbsp;The&nbsp;Centre National d'Études Spatiales (<a href="https://cnes.fr/en" target="_blank" rel="noreferrer noopener">CNES</a>), the French Space Agency, contributed to SAM’s gas chromatograph system.​



The study is published in the journal <a href="https://www.pnas.org/doi/abs/10.1073/pnas.2420580122" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



-----



Like what you read? <a href="https://www.earth.com/subscribe/" target="_blank" rel="noreferrer noopener">Subscribe to our newsletter</a> for engaging articles, exclusive content, and the latest updates.&nbsp;



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



-----

Mars rover makes the most significant find yet in the search for alien life

NASA’s Curiosity rover has made another remarkable discovery on Mars...

<div class="vdb_player vdb_58e3ebce955a315103d39bd158d96b98cd4fed198a0d2a49" vdb_params="m.embeded=cms_video_plugin_www.earth.com" data-placeholder="//img.vidible.tv/prod/2017-06/27/5952df10b90afb54eb343695/5952df1d7d768826006c11ea_o_A_v2.jpg?w=1440&#038;h=900">	<script type="text/javascript" src="//delivery.vidible.tv/jsonp/pid=58e3ebce955a315103d39bd1/vid=5952df10b90afb54eb343695/58d96b98cd4fed198a0d2a49.js?m.embeded=cms_video_plugin_www.earth.com"></script></div>
 
Today’s Video of the Day comes thanks to <a href="https://www.nasa.gov/">NASA</a> and features a look at all you need to know about the upcoming August 21st solar eclipse.
&#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a>
Source: <a href="https://www.nasa.gov/multimedia/videogallery/index.html">NASA</a>

Getting ready for the August 21st solar eclipse

News coming your way