Articles tagged with Solar System
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 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.
The BepiColombo mission has provided unprecedented measurements of Mercury's particle bombardment, revealing a wide area affected by highly energetic particles. The planet's magnetic field and atmosphere play a crucial role in protecting it from these particles, which generate X-ray radiation and provide insights into Mercury's evolution.
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...
Scientists found that a type of supernova explosion could create the necessary elements for planets, including water, around 100 million years after the Big Bang. This discovery suggests that planet formation may have occurred earlier than previously thought.
Dr. Olivier Mousis has been elected an Academician of the International Academy of Astronautics, a full member recognizing his distinguished contributions to space science and exploration. He leads research on the origin and evolution of the solar system at SwRI.
A new SwRI study provides the first evidence of recent liquid flows to Pluto's surface, suggesting that liquid nitrogen is rising from beneath the Sputnik Planitia glacier. This finding, based on data from NASA's New Horizons spacecraft, indicates a new kind of time-variable feature on Pluto.
Researchers discovered that the solar wind slows down by 13-15% as it approaches the outer boundary of the heliosphere, aligning with previous models. This slowdown is crucial for understanding the impact of interstellar material on long-term space travel.
The SETI Institute has awarded $1 million in STRIDE grants to support cutting-edge research in astrobiology, exoplanet science, and public engagement. The awards will fund projects that push the boundaries of life detection, planetary climate modeling, and innovative education initiatives.
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.
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.
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.
Researchers found our Sun joined a mass migration of similar stars 4-6 billion years ago, shedding light on galaxy evolution and the corotation barrier. The discovery reveals the time range over which the bar structure at the galactic center was formed.
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.
A new international study finds that Io and Europa's contrasting water makeup was established at birth, contradicting the idea that it evolved over time. The research suggests that Io formed from dry materials and Europa accreted from ice-rich building blocks.
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.
The UVS instrument collected data on the comet's composition, including oxygen, hydrogen, and dust-related features. The unique sunward viewpoint provided a downstream view of the comet's tails, allowing researchers to gain insights into its geometries.
The CoDICE instrument has successfully collected first-light data from IMAP, measuring energized particles from interstellar space, the solar wind, and solar energetic particles. This will provide a better understanding of our place in the universe by studying the interaction between the interstellar medium and the solar wind.
The PUNCH mission has made significant advancements in imaging the Sun's outer atmosphere and solar wind. The spacecraft has tracked enormous coronal mass ejections, providing a unique view of space weather events and their impact on our planet.
A SwRI-led study finds that quasi-periodic pulsations (QPPs) in solar flares are driven by dynamic oscillations in magnetic reconnection. This research could help refine traditional solar flare models, providing new insights into the mechanisms driving space weather.
Scientists have discovered olivine-bearing clasts from a lunar regolith sample, shedding light on the migration of Carbonaceous Ivuna-type chondrites to the Earth-Moon System. The findings provide new insights into the origin of water on the lunar surface.
Researchers have created a new model that shows how planet formation timing influences planetary composition and density. The study suggests that older, rocky planets are less dense than younger ones due to the varying lifetimes of stars.
Astronomers have discovered that the 1998 KY26 asteroid, targeted by Japan's Hayabusa2 mission, is only 11 meters wide and spins twice as fast as previously thought. This smaller size will make a touchdown manoeuvre more challenging for the spacecraft.
The Europlanet Science Congress 2025 will feature press briefings on the RAMSES mission to asteroid Apophis and recent discoveries with the Juno Mission. These events aim to improve our ability to defend Earth from potential asteroid threats.
Three planetary scientists have been awarded Europlanet Career Medals for their contributions to planetary science. Dr Tim Lichtenberg received the Early-Career Medal for his work on planetary formation and exoplanet evolution, while Dr Benoit Carry won the Mid-Career Medal for his research on asteroid structures and planetary defence.
The European Space Agency-led Solar Orbiter mission has split energetic particles into two groups, tracing them back to distinct solar outbursts. Researchers found that one type of particle is connected to intense solar flares and the other to larger coronal mass ejections.
A study of Bennu samples reveals the asteroid reflects light differently at red and blue wavelengths, offering insights into solar system evolution. The findings also enable future research on asteroid navigation and selection.
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.
The OSIRIS-REx sample return mission revealed asteroid Bennu's composition, history, and unique materials. Researchers found stardust from other stars and organic material formed in interstellar space, shedding light on the early solar system's formation.
Researchers find shared dusty layer of troilite on M- and K-type asteroids, suggesting they originated from similar large objects. Polarization studies reveal unique composition linking these distinct asteroid types.
A study by researchers at UC Santa Barbara, Yale University and others found that a third of young stars have misaligned rotational axes with their protoplanetary disks. This challenges centuries-old assumptions about the alignment of stars and planets in our solar system and suggests that some stars may be born tilted.
A new study from NYU Abu Dhabi found that high-energy particles from space, known as cosmic rays, could create energy needed to support life underground on planets and moons. This process, called radiolysis, can power life even in dark, cold environments with no sunlight.
Researchers used Japan's Himawari-8 and -9 meteorological satellites to track temporal changes in Venus' cloud-top temperature, finding variations in thermal tides and planetary-scale waves. The study provides a new avenue for long-term multiband monitoring of solar system bodies.
Dr. Robin Canup, a leading expert in planetary science, has received the 2025 AAS DDA Dirk Brouwer Career Award for her groundbreaking research on planet and satellite formation, including the Earth-Moon system's origins.
The study provides a new look at the galactic region surrounding our solar system, revealing a roughly uniform background Lyman alpha sky brightness. The findings suggest hot interstellar gas bubbles may be regions of enhanced hydrogen gas emissions at a wavelength called Lyman alpha.
The National Institute of Polar Research's collection offers invaluable insights into the early solar system and planetary bodies. With over 13,000 classified meteorites, it advances global research on planetary evolution and solar system history.
Scientists have identified flickering loops in the solar atmosphere that signal impending solar flares. The loops' brightness variability can be measured to predict flares with up to 80% accuracy, potentially providing 2-6 hours of warning time for astronauts and technology.
Researchers used rare data from a 2012 Venus solar transit to validate techniques for studying small exoplanets' atmospheres, similar to that of Venus. The study reveals signs of carbon dioxide in the Venusian atmosphere, which can be used to differentiate it from Earth's atmosphere.
A team of astronomers discovered new insights into the forces that shape protoplanetary disks using the James Webb Space Telescope. They traced disk winds in unprecedented detail, revealing an intricate structure and a pronounced central hole inside each cone-shaped envelope of winds.
A new study by Rice University's David Alexander and Anthony Atkinson extends the definition of a habitable zone for planets to include their star's magnetic field. Only two exoplanets, K2-3 d and Kepler-186 f, meet all conditions for potential habitability, suggesting that stellar magnetism is a crucial factor in determining planetary...
Astrophysicists calculate that two million years ago, the solar system encountered a cold, harsh interstellar cloud, which may have interfered with the sun's solar wind and affected Earth's climate. The heliosphere, a protective plasma shield, was compressed in such a way that it briefly placed Earth outside its influence.
A University of Leicester-led study suggests that the orbital instability of the giant planets in our Solar System occurred between 60-100 million years after its beginning, based on analysis of enstatite meteorites. This instability is believed to have led to the formation of the Moon and may have impacted the habitability of Earth.
The Juno spacecraft has directly measured charged oxygen and hydrogen molecules from Europa's atmosphere, providing key constraints on the potential oxygenation of its subsurface ocean. The findings suggest that oxygen is continuously produced in the surface ice shell, with an estimated 12 kg per second, which could support habitability.
Researchers have discovered a multi-planet system that provides a rare glimpse into the formation of planets around a young star. The system consists of six confirmed planets and potentially a seventh, all forming under similar conditions at an age of just 700 million years.
Researchers at UTSA's Department of Physics and Astronomy have used deconvolution algorithms to enhance images of galaxy NGC 5728 obtained by the James Webb Space Telescope. The study reveals a faint extended feature that could be part of an outflow from a supermassive black hole interacting with the host galaxy.
A team of space physicists used NASA's Parker Solar Probe to analyze whistler waves, finding they originated from disturbances in Venus' weak magnetic fields. The results support a previous study that failed to detect radio waves generated by lightning strikes on the planet.
Researchers have found high levels of phosphates in the water on Saturn's moon Enceladus, a key component of DNA and cell membranes. The discovery increases the chances of finding habitable worlds across the galaxy, as Enceladus can support life over a wider range of distances from its star.
Astronomers have discovered an Earth-sized planet, LP 791-18d, with active volcanoes that could sustain an atmosphere, potentially allowing for liquid water and life. The planet's unique tidal locking creates a permanent day and night side, with the night side possibly experiencing condensation of water vapor.
Researchers propose that early interactions between the magma ocean and a molecular hydrogen proto-atmosphere could have given rise to Earth's signature features, including its abundant water. The study suggests that even dry rocky material collisions would generate large quantities of water through these atmospheric-magma interactions.
Astronomers have observed an extremely rare and aspherical Fast Blue Optical Transient (FBOT) explosion 180 million light years away. The explosion, similar to a flat disc shape, challenges scientists' current understanding of stellar explosions.
The ESO VLT observed the aftermath of the DART impact, showing that the ejected cloud was bluer than the asteroid itself, indicating fine particles. The team found no signs of ice or DART spacecraft propellant, but detected changes in light polarization suggesting altered surface composition.
A recent experiment by UC Riverside astrophysicist Stephen Kane demonstrates that a terrestrial planet in this location would have disastrous effects on the solar system. The simulation found that such a planet could destabilize Earth's orbit, making it far less habitable and potentially ejecting Mercury and Venus from the solar system.
Researchers have discovered that primitive meteorites contain a different mix of potassium isotopes than those found in other, more-chemically processed meteorites. This suggests that the Solar System was formed from a 'poorly mixed cake batter' of materials, with some planets receiving a unique blend of elements from distant sources.
Astronomers using Hubble Space Telescope data found a small but significant excess of light in the sky, equivalent to the glow of 10 fireflies. This residual glow could be caused by a tenuous sphere of dust from comets falling into the solar system, adding a new component to the known architecture of the solar system.
The Europlanet Prize for Public Engagement 2022 was awarded to Dr. Kosmas Gazeas and the team behind 'Planets In Your Hand', an interactive tactile exhibition that provides a multisensory experience of planetary surfaces. The exhibition has been traveling to schools, universities, and organizations, reaching thousands of visitors.
The analysis of particles from asteroid Ryugu has revealed a high carbon content, similar to the Sun, and the presence of rare earth metals in concentrations 100 times higher than elsewhere in the solar system. The findings suggest that Ryugu originated from a parent asteroid formed in the outer solar nebula.
Asteroids like Bennu and Ryugu appear rough due to the loss of fine-grained regolith caused by tiny space dust grains hopping around on their surfaces. This process may help small asteroids migrate faster through space, affecting their orbits.
The study suggests that Venus' atmosphere plays a crucial role in determining its rotation speed, with fast winds dragging along the surface and slowing it down. This has significant consequences for the sweltering Venusian climate, with average temperatures of up to 900 degrees Fahrenheit.