Articles tagged with Planets
Researchers at the University of Copenhagen have reconstructed the earliest stages of planet formation, revealing that Earth and Mars formed in different ways. The study's findings support the hybrid model, which suggests that both collision-based and pebble accretion mechanisms contributed to planetary formation.
A University of Washington study suggests the north pole of Mars contains less dust than previously estimated, with layers of cleaner ice stacked between dustier ice. This discovery could provide key details about Mars' climate thousands of years ago, and potentially shed light on the planet's habitability.
A new study suggests that Enceladus's icy vents may concentrate organic molecules and molecular biosignatures into individual grains, making them easier to detect. Researchers propose that the process could aid in the search for life on the moon.
A team of astronomers discovered water, methane, and ammonia in HATS-6 b's atmosphere, challenging our understanding of giant planet formation. The planet's unexpected temperature suggests cloud and haze may be responsible, raising questions about the reliability of atmospheric analysis.
A Purdue-led study published in Communications Earth & Environment reveals a complex history of water on Mars, with evidence of multiple water episodes and hydrothermal activity. The research found carbonate-rich ridges, groundwater, and lake water, shedding light on the possibility of life on Mars.
Venus, Earth's twin planet, lacks a rocky satellite due to its slow spin and gravity, which causes a moon to collapse and crash into the planet. The discovery sheds light on the planet's evolution and potential habitability.
Researchers used state-of-the-art computational techniques to reveal fundamental differences in moon formation from a Mars-sized object and Earth 4.5 billion years ago. Material strength of the two ancestral bodies matters in the process, changing how researchers think the planetary collision happened.
Researchers have estimated that the unknown absorber in Venus's clouds must absorb light very efficiently, occur at a high concentration, or both, with a required decadic absorption coefficient reaching approximately 1,278 cm-1 at 375 nm. This suggests that highly absorbing conjugated organic molecules could be the culprit, but the stu...
A team at the SETI Institute is developing a new method to identify resources in space using Raman spectroscopy, aiming to answer key questions such as what is there, how much is there, and where can it be found. This approach could potentially reduce costs and risks associated with space exploration and resource extraction.
A team of scientists, led by Wladimir Lyra at New Mexico State University, propose a new mechanism for forming massive planets around supermassive black holes. Computer simulations show how these planets can grow to sizes comparable to those of stars, potentially igniting nuclear fusion.
Astronomers discovered a cosmic river of gas that tilted the outer ring of GW Orionis, causing its orbital plane to deviate from its expected orientation. This finding suggests that streamers may play a significant role in shaping planetary systems.
Astronomers have detected an atmosphere on a rocky planet, LHS 1140 b, in the habitable zone of its host star, which is consistent with conditions for liquid water and potentially life. The discovery was made using the WINERED spectrograph on the Magellan Clay telescope and reveals helium escaping from the upper atmosphere.
A new study by University of Florida Assistant Professor Jason Dittmann reveals that the rocky exoplanet LHS 1140b may have its own atmosphere. The planet's age and atmospheric composition suggest a steady-state atmosphere with water, which could persist over time.
A team of researchers from Kyushu University and Max Planck Institute for Extraterrestrial Physics have detected ambipolar diffusion in a prestellar core, weakening magnetic support and leading to gravitational collapse. This finding provides insight into early star formation and the creation of stellar systems like our own.
Researchers have discovered two rare 'super-puff' planets with densities lower than candy floss, orbiting an F7-type dwarf star. The study provides a unique laboratory for understanding how these planets form and evolve, offering insights into their extremely low densities.
Researchers found that even small shifts between mirror segments can greatly affect the performance of image-processing techniques used to detect exoplanets. The study's findings highlight the importance of segment alignment stability for planet detection and provide valuable guidance for future instrument design.
New study by University of Southampton confirms the universe's expansion is still accelerating as previously found, debunking 2025 claims that the cosmos was slowing. The team re-evaluated data using Type Ia supernovae to calculate vast cosmic distances and found no error in their methods.
Astronomers have developed a novel method to estimate the masses of newborn planets using the properties of dust rings around stars. By analyzing the width, brightness peak location, and dust content of these ring structures, researchers can reconstruct planet masses even when those planets are too faint or embedded to observe directly.
Researchers have discovered daily cloud cycles on WASP-94A b, a Hot Jupiter planet, using data from the James Webb Space Telescope. The findings reveal different weather patterns on the morning and evening sides of the planet, with magnesium silicate clouds forming in the mornings and clearing up by nightfall. This breakthrough provide...
The Juice and Europa Clipper spacecraft captured simultaneous images of both hemispheres of the interstellar comet 3I/ATLAS. The observations revealed hydrogen, oxygen, and carbon emissions, providing insights into the comet's origin and composition.
Researchers found amino acids are consistently more diverse and evenly distributed in biological samples than abiotic ones, while fatty acids show the opposite pattern. This fundamental principle of life may be detectable in data collected by space missions.
Researchers discovered a 'hydraulic jump' causing massive cloud waves on Venus, connected to the planet's superrotation and sulfuric acid vapor. This phenomenon may also impact future Mars missions, with potential implications for planetary exploration.
A Harvard study resolves a longstanding climate puzzle by proposing that the Sturtian glaciation could have lasted 56 million years due to oscillating 'snowball' and 'hothouse' conditions. The researchers suggest intense weathering of volcanoes triggered global glaciations, which warmed and retreated over repeated cycles.
Scientists have measured the atmosphere of the mini-Neptune, revealing a heavy composition with water vapor, carbon dioxide, and sulfur dioxide. The findings suggest that both planets formed far from their host star, then were drawn inward through a gradual process, preserving their atmospheres.
A team of astronomers using a new method to find planets has detected 27 potential circumbinary planet candidates in double star systems. The findings, published in the Monthly Notices of the Royal Astronomical Society, broaden our understanding of planet formation and evolution in complex environments.
Researchers propose an agnostic biosignature that detects life on a population level by analyzing patterns of planetary traits and spatial relationships. This method prioritizes reliability over completeness, minimizing false positives even if it misses some life-bearing planets.
Scientists at MIT have developed a new wave model called PlanetWaves that predicts how waves will behave on planetary bodies with different liquids, atmospheres, and gravity. The model reveals that gentle winds can create massive waves on Titan, while hurricane-force winds barely move the surface of lakes on exoplanet 55-Cancri e.
Researchers discover quasi-one-dimensional superionic state of carbon hydride under extreme pressures and temperatures found deep inside ice giant planets. This finding has implications for heat and electricity movement through planetary interiors and could influence magnetic-field generation.
A team of scientists using Curiosity rover images discovered ancient Martian ripple marks, indicating intense sandstorms swept through Gale crater around 3 billion years ago. The findings provide insight into the planet's atmosphere at that time, suggesting conditions were higher and closer to Earth's than they are currently.
Researchers have confirmed that giant planets like Saturn operate under a unique magnetospheric regime, with a shifted cusp location due to its rapid rotation. This discovery alters models of magnetic reconnection and high-energy particle acceleration, revealing new insights into Saturn's auroral activity.
A new AI pipeline called RAVEN has validated over 100 exoplanets, including 31 newly detected planets, using NASA's TESS data. The study found that around 9-10% of Sun-like stars host a close-in planet, and 'Neptunian desert' planets occur around just 0.08% of Sun-like stars.
A new class of molten planet has been discovered, with a permanent ocean of magma and a unique composition of heavy sulphur molecules. This exoplanet, L 98-59 d, is unlike any known planet in our Solar System and may be the first of its kind in the galaxy.
Researchers analyzed Ryugu asteroid samples to understand magnetic field evolution in early solar system. The study found that 23 of 28 samples exhibited stable NRM components, providing critical information on the spatiotemporal evolution of magnetic fields.
Astronomers at UCLA and UCSD have discovered hydrogen sulfide in the atmospheres of four distant gas giant planets orbiting HR 8799, confirming their planetary status. The detection uses a new data analysis technique that will improve the search for life on other planets.
A team of researchers used spectral data from the James Webb Space Telescope to study the HR 8799 star system, finding clear evidence of sulfur on three gas giant planets. This discovery suggests that these massive planets likely formed through core accretion, contradicting older models.
A team from the University of Trento has identified an empty subsurface lava tube beneath Venus' surface, estimated to be approximately one kilometer in diameter and 375 meters deep. The discovery was made possible by analyzing Magellan's radar images and provides new insights into Venus' volcanic processes and geology.
A new study from Tohoku University and other international researchers has found that an anomalous dust storm on Mars can drive the transport of water to the upper layers of the atmosphere, leading to significant water loss. This discovery opens a new path for understanding how Mars lost much of its water over time.
Researchers created the highest resolution map of dark matter, showing its interaction with normal matter through gravity. The new data from NASA's James Webb Space Telescope confirms previous research and provides new details about dark matter's influence on the Universe.
Scientists found that a planet's interior composition, specifically the 'softness' of its vortex base, determines the formation of polar vortices. The study suggests that Saturn may have a harder interior than Jupiter, leading to a single massive polar vortex, while Jupiter's softer interior gives rise to multiple smaller vortices.
Researchers from the University of Copenhagen have explained the mysterious 'red dots' seen in James Webb Space Telescope images as young black holes. The discovery provides insight into how the universe's first black holes were born and sheds light on their early development.
Mars plays a measurable role in shaping Earth's long-term climate patterns, including ice ages, through its gravitational influence and orbital cycles. The study suggests that Mars' presence is necessary for the existence of major climate cycles, which have driven evolutionary changes on Earth.
Astronomers have created a naturally occurring space weather station around complex periodic variable M dwarf stars to study the environment of planets. This discovery sheds new light on how stars affect their planets' makeup and might provide clues about the habitability of distant worlds.
An international team of astrophysicists observed four baby planets in the V1298 Tau system forming into super-Earths and sub-Neptunes. The planets' low densities, comparable to Styrofoam, were measured for the first time, providing observational proof.
A team of astronomers used NASA's JWST to reveal an alien atmosphere in the ancient, ultra-hot super-Earth TOI-561 b. The planet's thick atmosphere is upending conventional wisdom about ultra-short-period planets, and its composition could be representative of planets that formed when the universe was relatively young.
Researchers detect strong evidence for an atmosphere on ultra-hot super-Earth TOI-561 b, challenging the idea that small planets can't sustain atmospheres. The planet's unusually low density is explained by a thick volatile-rich atmosphere that circulates heat and cools the nightside.
A new study by the University of Zurich suggests that Uranus and Neptune may be more rocky than icy, challenging their classification as ice giants. The researchers developed a unique simulation process to model the planets' interiors, which found that the two planets could have either water-rich or rock-rich compositions.
Recent observations of TRAPPIST-1e, an Earth-sized exoplanet in the habitable zone, reveal hints of methane but raise questions about its atmosphere's existence. Researchers caution that more rigorous studies are needed to determine if the methane is a sign of an atmosphere or stellar contamination.
Astronomers have discovered a stellar companion near a star with hot dust, offering a complex laboratory to understand the origin and composition of this phenomenon. This breakthrough builds on decades of technological leadership in interferometry, enabling scientists to study the interaction between the companion and the dust.
Experts reach consensus on using the Global One Health Index to address complex global challenges and achieve Sustainable Development Goal 3. The index enables policy coordination across human, animal, and environmental health through globally standardized metrics.
Astronomers have confirmed the first sighting of a giant explosion on a nearby star using XMM-Newton and LOFAR telescopes. The coronal mass ejection (CME) was detected in a star with a magnetic field 300 times more powerful than our Sun, capable of stripping away the atmospheres of planets in its path.
Experimental tests demonstrate that interactions between magma oceans and primitive atmospheres during early years can produce significant amounts of water. This process has major implications for the physical and chemical properties of planets' interiors, with potential effects on core development and atmospheric composition.
A young rogue planet has displayed a record-breaking 'growth spurt', consuming 6 billion tons of gas and dust every second over several months. The observations provide insight into the turbulent infancy of such celestial bodies, revealing a tumultuous growth process similar to that of stars like our Sun.
A team of scientists from Princeton University and PPPL successfully recreated the star formation mechanism in a laboratory setting, validating astrophysical theory. The achievement marks over two decades of persistent effort and combines experimental ingenuity, theoretical insight, and advanced computational modeling.
Researchers have discovered a new type of tektite exclusively found in South Australia, recording an ancient asteroid impact event approximately 11 million years ago. The unique glasses provide valuable insights into the destructive power of past impacts and their importance for planetary defense.
Xinting Yu, an assistant professor at UT San Antonio, has been awarded the 2025 Harold C. Urey Prize for her contributions to planetary science. Her research focuses on understanding how planetary surfaces and atmospheres interact and evolve, with applications in exoplanet characterization and habitability studies.
A new study has revealed chemical signatures of ancient Martian microbial life in the Bright Angel formation, a region of Jezero Crater known for its fine-grained mudstones rich in oxidized iron and organic carbon. The findings suggest that early microorganisms may have played a role in shaping these rocks through redox reactions.
Astronomers have detected a growing planet outside our solar system in a cleared gap of a multi-ringed disk of dust and gas. The discovery provides the first direct evidence that protoplanets can create these gaps, resolving a long-standing debate in the scientific community.
Researchers at Nagoya University and the Italian National Institute for Astrophysics have determined how molten rock droplets formed in Jupiter's early days. Their study shows that chondrule characteristics are influenced by the water content of impacting planetesimals, providing a clearer picture of solar system formation.
Astronomers have devised a method to map the spottiness of distant stars using observations from NASA missions, improving understanding of planetary atmospheres and potential habitability. The new model, called StarryStarryProcess, can help discover more about exoplanet properties.
Researchers propose that Jupiter-sized exoplanets may accumulate and collapse into detectable black holes due to dark matter. This process could potentially generate multiple black holes in a single exoplanet's lifetime, making exoplanet surveys a promising method for hunting superheavy dark matter particles.