Researchers analyze cyclical changes in light spectrum emitted by Proxima Centauri and suggest the presence of a second planet. The candidate planet orbits every 5.2 years and may be a 'super-Earth', challenging current models of low-mass planet formation.
A team of researchers used a single star affected by the Milky Way-Gaia-Enceladus collision to determine its age and date the event to approximately 11.5 billion years ago. The study provides insights into the impact of galaxy collisions on their evolution.
The Transiting Exoplanet Survey Satellite (TESS) has discovered three new exoplanets, including one rocky planet in the habitable zone, which could potentially support liquid water and life. The newly found planets, TOI-270, are unique in that they occupy a 'missing link' between rocky Earth-like planets and gas-dominant mini-Neptunes.
The discovery of TOI-270 includes two sub-Neptunes that could be an intermediate size between Earth and Neptune, providing insights into planetary formation. Astronomers also found a rocky super-Earth with a three-day orbit, adding to the system's potential for studying exoplanet dynamics.
Researchers report the discovery of a methane hydrate phase in which water molecules surround and trap methane, remaining stable at pressures up to 150 gigapascals. This phase is similar to those found in the mantles of Uranus and Neptune.
Scientists from Tokyo Institute of Technology used computer simulations and observations of trans-Neptunian objects to understand how they may have formed. The study found that the size and orbit of satellite systems around large TNOs are best explained by impacts of molten progenitors.
Astronomers have measured the temperature of Uranus' rings for the first time, finding a cool 77 Kelvin. The new images also reveal differences in ring composition compared to Saturn's rings, including lower albedo and narrower widths.
Researchers investigate Haumea's ring, suggesting a degree of eccentricity is required for resonance to act on particles. They identify stable, circular orbits compatible with the ring, contradicting previous assumptions.
Scientists will study Uranus and Neptune's poorly understood regions with greater accuracy using a new, improved net flux radiometer. The instrument, developed for NASA's Planetary Concepts for the Advancement of Solar System Observations program, features thermopile sensors and seven infrared channels to measure heat.
Scientists from HZDR drove shock waves through plastics to simulate planetary conditions and observed crystalline structures at extreme pressures. The discovery may require revised models of Uranus and Neptune's interiors, suggesting less free hydrogen than previously thought.
A team of planetary scientists used Hubble images to track the growth of a new Great Dark Spot on Neptune, finding that dark spots originate deeper in the planet's atmosphere than previously thought. The study also revealed that these storms occur with a frequency of every four to six years and last up to six years.
Researchers have spotted two rings of dust around a young star, suggesting the formation of a planetary system similar to our own. The observations provide clear answers to previous models, with one ring at the asteroid belt location and the other at the Neptune orbit.
The Hubble Space Telescope has uncovered new insights into the weather patterns of Uranus and Neptune, revealing dynamic atmospheres with mysterious dark storms. The observations suggest that these storms form in a similar way to Jupiter's Great Red Spot and are driven by seasonal changes.
Scientists have discovered a new planet, HD 21749b, with the longest orbital period of three planets so far identified by TESS. The planet, about three times the size of Earth and 23 times as massive, is likely a dense, gaseous 'sub-Neptune' world.
Saturn's iconic rings are being pulled into the planet by gravity, draining an Olympic-sized swimming pool in half an hour. The research suggests the ring system will be gone in 300 million years, with some particles also falling onto Saturn's geysers from moon Enceladus.
A team of UNLV and international astronomers has conducted the first large-sample survey of protoplanetary disks using ALMA, yielding high-resolution images of 20 nearby disks. The results reveal a large population of young planets at wide-orbit similar to Neptune or Jupiter, which may be similar to our solar system
Research finds that gravity and unique shapes of small objects in our solar system create and maintain their own rings. Astronomers discovered that rings around Chariklo and Haumea are confined by the object's irregularities, contradicting previous assumptions about moon-dominated ring systems.
Researchers at Southwest Research Institute studied the Patroclus-Menoetius binary asteroid pair and found that its existence indicates an earlier dynamical instability. This instability pushed Uranus and Neptune outwards, scattering small bodies into the Kuiper Belt, where they formed the Trojan asteroids.
Researchers at Durham University found that a massive collision with an object twice the size of Earth likely tilted Uranus on its side. The impact may have trapped heat, explaining the planet's extremely cold temperature. Simulations also suggest this event could have formed Uranus' rings and moons.
Scientists at MIT have discovered nearly 80 new planetary candidates in the K2 dataset, including a likely planet that orbits HD 73344 every 15 days. The planet is estimated to be 2.5 times the size of Earth and 10 times as massive, with surface temperatures reaching 1,200-1,300 degrees Celsius.
Astronomers have confirmed the presence of hydrogen sulfide in Uranus's cloud tops using sensitive spectroscopic observations. This discovery sheds light on questions about the planets' formation and history, particularly regarding the early Solar System's balance between nitrogen and sulfur.
Scientists from FAU, University of Leicester and University of Vigo have proven that the kinetic energy of particles in granular gases can increase temporarily due to surface adhesion. This effect contradicts Haff's law, which states that granular temperature decreases in closed systems.
Researchers have recreated superionic water, a state where oxygen remains fixed while protons flow freely, exhibiting properties of both solid and liquid. This discovery could lead to new materials with unique practical applications and provide insights into the physical properties of planets in our solar system.
Researchers have shed new light on the TRAPPIST-1 planetary system, revealing that all seven planets are mostly made of rock and contain up to 5% water. The study also found that five planets lack a hydrogen-dominated atmosphere, similar to Neptune or Uranus.
NASA has launched a fleet of missions to study the planets in our solar system, revealing unique features of each planet's magnetosphere. Earth's and other magnetospheres deflect charged particles away from the planet, but also trap energetic particles in radiation belts.
A team of scientists identified 68 exoplanets where observers can see the planets in our Solar System transit the Sun. Nine of these are ideally placed to observe Earth's transits, although none are habitable.
A new study suggests that hydrophobic molecules like oil can be forced to dissolve in water when subjected to high pressure. Researchers applied immense pressure to methane and water, gaining insights into their interaction. This finding has implications for replacing hazardous industrial solvents and modeling planetary bodies.
Scientists at Helmholtz-Zentrum Dresden-Rossendorf simulated the conditions inside Neptune and found diamonds forming in real time using an ultra-strong X-ray laser. The study provides insights into the planet's chemical makeup and has potential applications for electronic instruments, medical procedures, and industrial production.
Researchers created high-pressure conditions to simulate the interior of icy giant planets and observe the formation of solid diamonds. The team used X-ray pulses to measure the chemical reaction, providing unambiguous evidence of diamond rain in real-time for the first time.
Researchers at the University of Edinburgh used computer simulations to predict chemical compounds in Neptune's mantle, finding ammonia hemihydrate as a likely component. The discovery sheds light on the extreme conditions and chemistry of ice giants, influencing future studies.
The James Webb Space Telescope will observe a range of celestial objects, from the outer planets and Kuiper Belt to exoplanets and distant galaxies. The initial 2100 observations planned will address various science areas, including first light, galaxy assembly, and star and planet birth.
A team of astronomers advocates for a statistical comparative approach to find habitable planets and life beyond the solar system. By studying large numbers of exoplanets with less detailed measurements, they can estimate the frequency of habitable environments and life on those planets.
A NASA study using Hubble and Spitzer space telescopes reveals a primitive atmosphere around HAT-P-26b, composed mainly of hydrogen and helium. The planet's water signature suggests it formed closer to its star or later in the planetary system than similar planets.
A new study reveals that HAT-P-26b, a Neptune-sized planet, has a hydrogen and helium-dominated atmosphere with a strong water signature. The discovery challenges the long-held assumption that planets like Neptune formed in a region of icy debris, instead suggesting alternative formation mechanisms.
A team of international researchers has uncovered the primitive atmosphere surrounding a distant exoplanet called HAT-P-26b, also known as Warm Neptune. The study found that the planet's atmosphere is composed almost entirely of hydrogen and helium with no clouds present.
Astronomers have found clear signs of water in the atmosphere of HAT-P-26b, a Neptune-sized exoplanet. The presence of water suggests that the planet's gaseous envelope formed late in its formation process, with little to no pollution by impacting debris.
A new study in Space Weather suggests that aircrews may experience increased radiation exposure due to weak solar activity, which could impact flight safety and radiation exposure for frequent flyers. Researchers also found auroral activity on Uranus, providing fresh clues about its magnetosphere.
A team of researchers presented a new model for the origin of Saturn's rings based on computer simulations. The study found that Kuiper belt objects were destroyed by tidal forces when passing close to giant planets, forming icy ring systems. This process explains the compositional differences between Saturn and Uranus' rings.
Researchers at Ibaraki University used ALMA to observe the disk around TW Hydrae, finding multiple gaps that match theoretical predictions for planet formation. The team estimates a massive, icy giant planet similar in size to Neptune, with a mass likely more than that of Neptune.
Researchers found carbonic acid, orthocarbonic acid, and clathrate compounds stable under high pressure conditions. The cores of Uranus and Neptune may consist of these exotic materials.
A team of Carnegie scientists has discovered three giant planets in a binary star system composed of stellar 'twins' that are also effectively siblings of our Sun. The findings may help explain the influence that giant planets like Jupiter have over a solar system's architecture.
Research from the University of Warwick suggests that Planet Nine's existence could lead to the elimination of a giant planet and its ejection into interstellar space. The hypothetical planet's presence could cause a 'pinball' effect, hurling planets out of the solar system as the sun dies in around seven billion years.
Researchers analyze the Kepler-223 star system, finding a unique orbital configuration similar to that of Jupiter, Saturn, and Uranus. The study suggests that the four planets may have migrated through a disk, getting stuck and maintaining their current orbits, which differs from the formation process of Earth's inner planets.
Astronomers have captured the most detailed image yet of a protoplanetary disc around the young star TW Hydrae, revealing concentric dusty bright rings and dark gaps. The new ALMA images show intriguing features that may indicate a planet with an Earth-like orbit is forming in the disc.
Astronomers have captured unprecedented details of the TW Hydrae disk, which may host a super-Earth or an infant version of our home planet. The images show concentric dusty bright rings and dark gaps, including a tantalizing gap at Earth's distance from the star.
Phobos will likely break apart and form a ring around Mars due to tidal forces. The debris from Phobos will continue to orbit Mars for millions of years before eventually colliding with the planet.
Researchers at Princeton University have predicted a new phase of superionic ice with unusual conductivity properties. The P21/c-SI phase occurs at high pressures beyond giant ice planets, offering insights into the material's behavior.
Researchers suggest planetary pebbles, icy objects about a foot in diameter, were the building blocks for Jupiter and Saturn. This new model improves solar system formation models, producing the observed structure of the solar system with two gas giants, two ice giants, and a pristine Kuiper belt.
Dr. Martin Duncan's new model proposes that gas giants like Jupiter and Saturn formed through the accumulation of small 'pebbles', allowing cores to form rapidly enough to capture their atmosphere. The successful model predicts the formation of one to four gas giant planets, consistent with the observed outer solar system configuration.
Astronomers using Gemini Observatory's new Planet Imager have probed a newly discovered world in unprecedented detail. The planet, 51 Eridani b, is about two times the mass of Jupiter and features a Solar System-like atmosphere with methane detection.
Astronomers confirm exoplanet orbiting far from its central star using gravitational microlensing, opening new discovery space for long-period orbits. The Uranus-sized planet is about 370 million miles from its parent star, with a host star about 70% as massive as our Sun.
A team of researchers has discovered that the presence of salty impurities in ice can push the formation of electrically conducting ice to occur at higher pressures, potentially explaining the magnetic fields of Uranus and Neptune. This finding challenges current assumptions about the physics of icy planetary bodies.
A new system devised by Dr. Ravit Helled measures Saturn's rotation period, offering a more accurate determination of the planet's internal structure, weather patterns, and formation process. The method applies to other gas planets in the solar system, including Uranus and Neptune.
Researchers used the Titius-Bode law to calculate planetary positions and found billions of stars with 1-3 planets in their habitable zone. This suggests that a significant number of these planets could have liquid water and support life.
A team of researchers from MIT has detected optical features around Chiron that may signal the presence of a ring system, jets, or a shell of dust. The findings are based on observations of a stellar occultation in 2011, which revealed symmetrical and sharp features near the start and end of the event.
Researchers found standard stars have about two habitable environments where liquid water can exist, providing conditions for life. However, the existence of intelligent civilizations remains uncertain due to unknown bottlenecks or self-destruction.
Astronomers found that tidal forces and atmospheric escape can transform mini-Neptune-like worlds into gas-free, potentially habitable planets. This process could provide a pathway to the formation of habitable worlds around M dwarf stars.
Researchers use laser-driven compression to study extreme conditions inside planets, revealing properties of silica that determine planet formation and evolution. The findings suggest large rocky planets may have long-lived oceans at depth and could explain the existence of planets like Neptune and Uranus.
A new study by McGill University and UCL finds that Mars experiences a transitional 'macroweather' regime between weather and climate. The sun plays a major role in determining macroweather on Mars, with temperature and wind fluctuations occurring over 1.8 Martian days.
A team of astronomers detected eight large storms on Uranus's northern hemisphere, including the brightest storm ever seen at 2.2 microns. The storms are thought to be caused by gases such as methane rising in the atmosphere and condensing into highly reflective clouds of methane ice.