Researchers found that equatorial regions on planets like Proxima b and TRAPPIST-1d might trap ozone, hiding signs of life from telescopic observations. This discovery highlights the challenges in detecting life beyond Earth, requiring a more nuanced strategy for searching for life.
Fast-moving space dust could collide with biological particles, enabling bacteria and organisms to travel to other planets. The study suggests that asteroid impacts are not the sole mechanism for transferring life between planets.
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.
Researchers aim to understand the evolution of our solar system by studying 'hot Jupiters', gas giants orbiting close to their parent stars. They will measure escaping gases and look for evidence of magnetic fields on these planets.
A giant gas giant planet, NGTS-1b, has been discovered orbiting a tiny star, defying conventional formation theories. The planet's proximity to its star and short orbital period pose significant challenges for understanding the origins of such massive worlds.
Researchers use Hubble Space Telescope to find 'sunscreen snow' on hot giant planet outside solar system, where titanium dioxide condenses into clouds. The discovery sheds light on exoplanet climates and may aid in gauging Earth-size planets' habitability.
Astronomers have discovered a new insight into how planets form, using high-powered telescopes to target the star V1247 Orionis. The team found a dust-trapping vortex that could protect sites of planet formation, allowing dust particles to clump together and grow.
Yale researchers Darryl Seligman and Greg Laughlin have created a new model for understanding how black holes, planets, and galaxies emerge from the vortex-rich environments of space. They found that vortices may shed Rossby waves as they spin and that the number of orbits between two vortices is different in their model.
Scientists from the University of Bristol have discovered evidence suggesting that massive collisions during planetary accretion resulted in significant mass loss, altering a planet's composition. This process, which occurred in the Earth and Mars formation, led to their distinctive volatile poor compositions.
New research from Oxford University sheds light on the formation of the Earth and its depletion of vital chemical elements. By simulating early Earth conditions, scientists found that melting and evaporation played a key role in shaping the planet's chemistry.
Scientists propose a new concept of terrestrial planet formation involving heat-pipes, which transport heat from interior to surface via mantle melting and magma ascent. This hypothesis resolves major outstanding problems across all planets, including the formation of volcanic terrains and lithospheres.
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.
Researchers demonstrated a region of very deep contrast between a simulated star and its planet, achieving an 18% bandpass. This milestone is crucial for future missions like WFIRST to detect and analyze the atmospheres of giant planets.
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.
Researchers found that the moon's magnetic field declined by about 90 percent over 3.56 billion years ago, with a 1-2.5 billion year time frame for its existence. This discovery has implications for habitability on other moons and planets, as well as the potential for life to respond to unstable environments.
The Transiting Exoplanet Survey Satellite (TESS) will identify over 20,000 extrasolar planets, including Earth-sized and 'super Earth' planets. The satellite's four cameras have been mounted onto the camera plate and successfully demonstrated operation with the flight computer.
A team of UA astronomers proposes a scenario that reconciles observed disk features and the population of planets in our galaxy. They simulated protoplanetary disks using synthetic observations to account for the formation of multiple gaps, challenging conventional theories.
Researchers at Yale University have discovered 60 new potential 'hot Jupiters,' gas giant planets that orbit extremely close to their stars. The discovery was made possible by a novel application of machine learning algorithms and the analysis of more than 140,000 star observations from NASA's Kepler mission.
Astronomers Dr Jane Greaves and Dr Wayne Holland propose a new model for forming planets in the aftermath of a supernova explosion. They suggest that material caught up in the bow-wave around a moving neutron star could provide raw materials for future planet formation. Further data from ALMA is needed to confirm this theory.
A new study has classified nearly 3,500 confirmed exoplanets into two distinct size groups: rocky Earth-like planets and larger mini-Neptunes. The researchers used data from NASA's Kepler mission and the W.M. Keck Observatory to make this discovery.
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 University of Oklahoma researcher has identified the possible compositions of seven planets in the TRAPPIST-1 system, finding six to be Earth-like. The exception, TRAPPIST-1f, has a high water content, suggesting TRAPPIST-1e as a potential candidate for habitability studies.
Two exoplanets, WASP-67 b and HAT-P-38 b, have distinct atmospheric compositions, with one being cloudier than the other. The team's findings suggest that their past formation histories may be responsible for these differences.
Researchers confirmed the orbit and temperature of TRAPPIST-1h, which orbits its star every 18.77 days and is frigidly cold. The discovery suggests that TRAPPIST-1h may have been habitable in the past, with a possible rotation period and activity level for its host star.
Researchers Simon Lock and Sarah Stewart propose a new type of planetary object called a synestia, which forms through giant impacts. Synestias could be responsible for moon formation, particularly in our solar system where Earth's moon is similar to its parent planet.
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.
Astrophysicists discovered that the TRAPPIST-1 system remains stable due to a 'resonant chain' configuration, where planets' orbital periods form simple ratios. This harmonic stability explains why the system has survived for millions of years.
A rocky super-earth, LHS 1140b, has been discovered orbiting an M-type star in the habitable zone, making it a promising candidate for atmospheric study and search for life. The planet's size and mass indicate a rocky composition, and its distance from the star allows for relatively cool temperatures.
The James Webb Space Telescope will analyze atmospheric components in TRAPPIST-1 exoplanets for potential biosignatures. Three promising planets, e, f and g, orbit within the habitable zone, with conditions suitable for supporting liquid water.
A UCL-led team found evidence of planetary debris surrounding a double sun system called SDSS 1557, which suggests the presence of terrestrial planets like Tatooine. The discovery is remarkable because it shows a high metal content, including silicon and magnesium, indicating rocky planet assembly via large asteroids that formed.
A new study suggests that volcanic hydrogen can warm planets, making them more likely to harbor life. With this discovery, distant stars could expand their habitable zones by 30-60%, adding many previously icy worlds to the list of potential candidates for hosting life.
Researchers propose that dust traps, high-pressure regions where dust grains accumulate and avoid fragmentation, play a key role in planet formation. These spontaneous traps concentrate grains from outer disk regions, helping to form planets and addressing the long-standing problem of how pebbles join together to create planetary cores.
Astronomers have confirmed the existence of seven small planets orbiting TRAPPIST-1, with sizes similar to Earth and temperatures comparable to those of Venus, Earth, and Mars. The inner six planets are likely rocky in composition and potentially harbor liquid water.
Researchers suggest an unseen population of gas giant planets may exist at distances similar to Jupiter and Saturn, resolving a long-standing debate about their formation. The predicted planets could be found using NASA's Wide Field Infrared Survey Telescope.
Scientists studied iron isotope ratios to understand Earth's differentiation event and how it differed from other planets. Nickel played a key role in shaping the ratios, with different elements forming under various planetary formation conditions.
The international team released a large dataset of exoplanet-detecting observations using the radial velocity method, identifying over 100 potential planets, including one orbiting the fourth-closest star to our Solar System. The data will enable astronomers around the globe to search for new planets and follow up on existing signals.
The Wolf 1061 system is a promising target in the search for extraterrestrial life due to its proximity to Earth and the presence of a habitable zone. The team's findings suggest that one of the planets, Wolf 1061c, may have an atmosphere similar to Venus, which could lead to a runaway greenhouse effect.
Astronomers have discovered three young star systems with doomed comets, suggesting a common mechanism for exocomet destruction. The study provides new insights into the past and present activity of comets in our solar system, potentially making life possible on terrestrial planets.
Researchers at Yale University developed a novel approach to detect exoplanets by analyzing signal fluctuations in star spectral intensity. By studying all signal information together, they can refine the search for Earth-like planets and improve traditional methods.
Researchers found that Neptune-mass worlds are likely the most common type of planet to form in icy outer realms. The study provides insight into the types of planets waiting to be found far from a host star, where scientists suspect planets form most efficiently.
Researchers have discovered a star that ingested some of its planets, revealing a violent history for the planetary system. The star's composition suggests it devoured four planets, preserving lithium and other elements in its atmosphere.
Astronomers have found compelling evidence for the existence of two infant planets orbiting a young star called HD 163296. The planets are estimated to be around the same mass as Saturn and are situated in the disk's outer regions, suggesting they are not yet fully formed.
Researchers have mapped gases in three dark rings around a distant star, indicating the presence of planets that are clearing dust and gas from the outer rings. However, one inner ring remains mysterious, with more carbon monoxide than expected, leaving scientists to investigate alternative explanations for its formation.
A new optical chip enables astronomers to capture clear images of exoplanets near their host sun, overcoming the challenge of intense solar brightness. This breakthrough technology uses an interferometer to cancel out sunlight and detect fainter planet light, paving the way for discovering planets with conditions suitable for life.
Scientists successfully measured the orbital period of K2-3d with high precision, enabling precise predictions of future transits. This improved forecast accuracy paves the way for searching for extraterrestrial life in the atmosphere of the planet.
Researchers have discovered complex systems of concentric rings surrounding young stars, formed by the interaction between protoplanetary discs and growing planets. These findings provide new insights into planet formation, shedding light on the dynamics of innermost disc regions.
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.
Research found that circumbinary planets can survive the late stages of their binary star's life by moving to wider orbits. Many such planets are likely to escape destruction and potentially become habitable for a short period.
Researchers from UNH captured unique measurements of the Van Allen radiation belts during a rare solar wind event. The findings provide valuable information for protecting orbiting satellites and exploring conditions on other Earth-like planets.
A team of researchers has shed light on the origin of centaur rings, revealing a scenario where tidal disruptions lead to disc formation and ring creation. The study suggests that rings around centaurs are more common than previously thought, with many awaiting discovery.
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.
A new study by Yale University researcher Jun Korenaga suggests that planets like Earth form through multiple giant impacts, leading to diverse sizes and internal temperatures. This lack of self-regulating mantle convection has significant implications for planetary habitability.
New research on brown dwarfs has found that atmospheric properties may be behind their incredible variation in size, temperature, chemistry, and more. The discovery may also apply to planets outside the solar system, making brown dwarfs a valuable tool for studying exoplanet evolution.
Researchers create high-pressure conditions to study the melting of forsterite, a mineral that makes up Earth's mantle. The experiments provide insight into how impact-generated magmas evolve and allow for modeling of Earth-type planets' inner structures.
Researchers from MIT and the University of Liège announce a new study on the TRAPPIST-1 planetary system, which hosts three potentially habitable, Earth-sized worlds. The team discovers that two innermost planets have compact atmospheres similar to those of rocky planets like Earth, Venus, and Mars.
Astronomers confirm 104 exoplanets outside our solar system using NASA's Kepler spacecraft on its K2 mission. The discoveries include a planetary system with four promising rocky planets orbiting the M dwarf star K2-72.
Researchers from KU Leuven show that surface composition and atmosphere interaction on exoplanets affect their temperature and habitability. A well-functioning 'air conditioning' system can make even planets with permanent day and night sides potentially habitable.
Researchers suggest minor evolutionary changes could have altered the fates of Earth and Venus, potentially leading to life on Venus and none on Earth. The study expands the notion of habitable zones and questions the role of plate tectonics in supporting life.