Astronomers are using the James Webb Space Telescope and high-performance computers to study the atmospheres of seven planets beyond our solar system, gaining insights into planetary formation and evolution. The KRONOS program aims to understand how planets form, evolve, and potentially harbor life.
A study examined floating plants on ocean planets and found they display a pronounced red edge in their reflectance spectra, potentially detectable via satellite remote sensing. The characteristic seasonal variation in NDVI values suggests this method could be promising for detecting life on habitable exoplanets.
A new study found that hotter and colder regions on a star's surface can distort our interpretations of planets, particularly when looking at dips in starlight. This distortion can lead to misinterpretation of features such as planet size, temperature, and atmospheric composition.
The completion of NASA's Pandora spacecraft bus brings the exoplanet mission one step closer to launch, set to study at least 20 planets' atmospheres for hazes, clouds, and water. The mission will utilize a novel telescope design to capture stellar surfaces and cleanly separate star and planetary signals.
A new type of exoplanet, similar to 'Super-Venus', has been detected by the James Webb Space Telescope. The planet's atmosphere is characterized by high concentrations of carbon dioxide, unlike typical Earth-like rocky planets or Neptune-like icy worlds.
The discovery of two new planets in the WASP-132 system has overturned existing understanding of how 'hot Jupiter' planetary systems form and evolve. The planets' unique configurations challenge traditional migration theories and suggest a more stable, 'cool' migration path for hot Jupiters.
A UNIGE study has overturned the assumption that Hot Jupiters orbit alone, discovering a unique multi-planetary system with an inner Super-Earth and an outer massive giant planet. The WASP-132 system's unexpected architecture raises new questions about planet formation and evolution.
Researchers used NASA's James Webb Space Telescope to study stars in a nearby galaxy with limited heavy elements. They found that some star-forming disks persist longer than predicted, allowing planets to form and grow bigger.
Researchers analyzed TRAPPIST-1 b's mid-infrared data to determine if it has an atmosphere. The study used a global analysis of all available JWST data and compared the observations with surface and atmospheric models.
A recent study using radio astronomy observations has revealed that planets help form the next by concentrating dust grains into a narrow region at their orbits. This sequential formation process can explain how our Solar System formed, with each planet triggering the next like a line of falling dominos.
Hubble's OPAL program has observed the four giant outer planets since 2018, providing long-term baseline data on their atmospheric changes. The observations have led to remarkable discoveries, including the measurement of Jupiter's wind speeds and Saturn's ring system colors.
A team of astronomers has detected the smallest main-belt asteroids ever found, with 138 rocky bodies reported in the asteroid belt. The discovery provides insights into the formation of small objects in the solar system and their potential impact on Earth's planetary defense.
Astronomers have discovered a fourth planet in the unusual Kepler-51 system, which consists of three ultra-low density 'super-puff' planets. The new planet, Kepler-51e, has a mass similar to the other three and follows a circular orbit of approximately 264 days.
The discovery of planet IRAS 04125+2902 b challenges current understanding of planet formation, with a 3-million-year-old age that's roughly equivalent to a two-week-old baby. The research provides new insights into early planetary system formation and sets a new benchmark for young planets.
A University of Washington-led study suggests that rocky planets orbiting M-dwarf stars can maintain stable atmospheres over time, enhancing the chances of supporting life. The James Webb Space Telescope has observed hotter planets without significant atmospheres, but temperate planets in the 'Goldilocks zone' may have stable atmospheres.
Researchers have discovered a new area called the 'Neptunian Ridge', which separates a desert of rare, radiation-eroded planets from a more populated savannah. The ridge is thought to be the result of high-eccentricity tidal migration, shaping the geography of exoplanet landscapes.
Researchers at the University of Colorado Boulder created a type of organic sulfur compound, dimethyl sulfide, in a lab without organisms present. This finding challenges previous research on its potential as an indicator of life beyond Earth.
A research team at Lund University has discovered a small exoplanet, TOI-1408c, with an unusual orbital motion that deviates from predicted behavior. The planet's interactions with its star and other planets offer insights into the complexity of planetary system formation.
Drs Johanna Vos aims to better understand weather patterns on extrasolar worlds using the James Webb Space Telescope. Her Exo-PEA project will reveal dominant atmospheric processes governing giant world weather, expanding our understanding of planetary atmospheres.
Researchers at Georgia State University have developed a new approach to finding life beyond Earth by focusing on the most abundant type of star in the universe: M dwarfs. With their vast resources and potential for habitable planets, M dwarfs offer the best chance for scientists to discover life-supporting exoplanets.
A team of researchers developed a new model that incorporates all necessary physical processes in planet formation, showing that annular perturbations can trigger the rapid formation of multiple gas giants. The results match latest observations and indicate more efficient and quick planet formation than previously thought.
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...
Research led by Heidelberg University reveals that small water-rich astronomical bodies in the early solar system supplied building materials for planets, including the Earth. These planetesimals brought water to Earth through their thermal evolution and point of origin.
Researchers detected hydrogen sulfide in HD 189733 b's atmosphere using the James Webb Space Telescope, shedding light on sulfur's role in planetary formation. The study also measured oxygen and carbon levels, providing insights into how planets form and evolve.
An international team has revealed that sub-Neptunes exist in two distinct populations: dense and less dense. The research suggests a physical link between resonance and density, with planets in resonant systems being less dense due to formation processes involving collisions and fusion.
The James Webb Space Telescope reveals the largest number of carbon-containing molecules in a disk around a young star. The findings have implications for the potential composition of planets that may form in such environments.
The James Webb Space Telescope has found a carbon-rich chemistry with 13 carbon-bearing molecules in the protoplanetary disk surrounding ISO-ChaI 147, a young 0.11-solar-mass star. This high carbon/oxygen ratio suggests radial transport of material within the disk, potentially affecting planet composition.
The MIRI Mid-INfrared Disk Survey (MINDS) discovered a large variety of carbon-rich gases in the disk surrounding a very low-mass star. This finding suggests that rocky planets with Earth-like characteristics may form more efficiently than Jupiter-like gas giants in such disks.
Researchers have discovered a new parameter controlling the main auroral structure of planets, explaining differences in aurora displays on Earth, Saturn and Jupiter. This study provides insights into planetary magnetic fields and solar wind interactions, enhancing our understanding of space environments.
A team of UH astronomers has discovered a diverse range of exotic exoplanets using the TESS-Keck Survey, which provides new insights into their properties and environments. The study reveals rare worlds with extreme environments and potentially habitable planets.
The NASA TESS-Keck Survey catalog features 126 exotic planets with detailed measurements allowing for comparisons with our solar system. Several planets stand out as touchstones for deepening astronomers' understanding of planetary formation and evolution.
A new study has revealed the mechanisms behind hydrodynamic escape in low-mass exoplanets, which is a process that can lead to significant changes in a planet's mass and climate. The research proposes a new classification method for understanding these escape processes and provides insights into the habitability of distant worlds.
The discovery of SPECULOOS-3 b is the second of its kind around an ultra-cool dwarf star and offers opportunities for life on orbiting planets to develop due to the star's long lifespan. The planet takes 17 hours to complete an orbit, making days and nights endless.
The study highlights the impact of volatile elements, convective mechanisms, liquid water, and carbon cycles on planetary habitability. Volatile elements affect atmospheric composition, while convection mechanisms shape surface conditions and regulate nutrient cycles.
A team of researchers using the James Webb Space Telescope has detected signs of an atmosphere around 55 Cancri e, a rocky exoplanet. The planet's surface is estimated to be molten, but the team believes it may have a secondary atmosphere that could provide insights into habitable planets.
A team of astronomers and citizen scientists has discovered a planet in the habitable zone of an unusual star system, including two stars and potentially another exoplanet. The newly discovered planet, TOI 4633 c, boasts the second-longest orbit of any planet discovered with TESS data.
A new study led by Durham University researchers proposes that strong stellar magnetic fields can dissipate gravitational tides, leading to the orbital decay of 'hot Jupiter' exoplanets. The findings suggest certain nearby stars may be good targets for searching additional hot Jupiter planets on decaying orbits.
Researchers introduce a new model that suggests dense stellar clusters can eject pairs of giant planets, which remain gravitationally bound to each other as they float through space. This discovery fills a critical gap in our understanding of planetary evolution and challenges prevailing theories of planet formation.
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.
Megan Reiter, assistant professor of physics and astronomy at Rice University, has received a $951,446 NSF grant to study the influence of neighboring stars on planet formation. Her research aims to clarify key forces shaping planet formation by exploring interplay between stars, planets, and environments.
Astronomers conducted the first search for forming planets using the James Webb Space Telescope, combining it with prior observations. The team found a potential planet candidate, but its existence is uncertain due to unknown factors.
A new study using the James Webb Space Telescope has captured the first-ever image of a planet-forming disk's gas dispersal, providing insights into how planets form in our solar system. The observations reveal that the inner disk of T Cha is evolving on very short timescales, differing from earlier spectra detected by Spitzer.
Researchers discovered that twin stars differ in composition due to one star devouring planets or planetary material. The study used high-precision analysis and found the phenomenon in about eight percent of 91 pairs of twin stars, shedding light on planet evolution theorists.
A team of astronomers has shed new light on the process of planet formation through a groundbreaking survey of over 80 young stars. The research provides a wealth of data and unique insights into how planets arise in different regions of our galaxy, revealing diverse patterns of planet-forming discs.
A team of international astronomers has captured stunning images of over 80 young stars and planetary discs using the ESO's VLT. The research provides a wealth of data on planet formation, revealing diverse populations of planets and planetary nurseries across three star-forming regions in the Milky Way galaxy.
Researchers applied Bayesian network analysis to a corpus of 142 science fiction works, investigating the representation of extrasolar planets. They found that after the discovery of real exoplanets in 1995, fictional exoplanets became less Earth-like, reflecting the scientific reality of vast numbers of diverse exoplanet types.
Astronomers have discovered an extreme Earth-like planet with lava oceans that orbits its sun-like star every four days. The young planet, just 500 million years old, is the nearest Earth-sized planet found so far and could provide valuable insights into the evolution of planets similar to our own.
Researchers found nine out of 40 studied systems have perfect alignment, suggesting planetary systems may prefer an orderly configuration. This could be beneficial for life forming in those systems, as misaligned stellar companions can disrupt planetary stability.
Research suggests that planetary migration is the key to explaining the mysterious gap in the size distribution of super-Earths. Simulations show that sub-Neptunes' evolution contributes to the observed radius valley, while rocky planets 'shrink' by losing their atmosphere.
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 have devised a new method to identify habitable planets and potentially inhabited planets by comparing atmospheric CO2 levels, which suggests the presence of liquid water. This signature can be detected with current telescopes, providing a path to identify life on exoplanets.
Scientists propose searching for depleted carbon dioxide in planetary atmospheres as a sign of liquid water and potentially life on other planets. A study suggests that low carbon abundance relative to neighboring planets could indicate habitability.
Researchers uncover six transiting planets around HD110067, a bright star with a chain of resonances spanning five pairs. The precise gravitational dance enabled the team to solve the previously unsolvable puzzle of the system's arrangement, revealing planetary orbits and orbital periods.
Astronomers have discovered a rare six-planet system, HD110067, that exhibits an orbital resonance pattern, repeating every three and four orbits. This unique configuration provides valuable information on how sub-Neptunes form, evolve, and potentially support liquid water on their surfaces.
Researchers created lab-made haze to understand how it affects observations of distant planets, which could lead to misinterpretations of global temperatures and biological activity. The new data offers a better understanding of exoplanet atmospheres, helping scientists focus on specific planets and improve their search for life.
New studies show that giant gas planets in nearby star systems can prevent life on smaller, rocky planet neighbors by kicking them out of orbit and wreaking havoc on their climates. Researchers found that four giant planets in the HD 141399 system are likely to destroy the chances for life on Earth-like planets.
University of Leicester astronomers confirm the existence of an infrared aurora on Uranus, offering clues to its magnetic fields and potential for life. The discovery may also help identify other habitable planets with similar characteristics.
The James Webb Space Telescope detected no significant atmosphere around TRAPPIST-1 b, a planet in the habitable zone of its cool star. The study highlights the impact of stellar activity on observations of exoplanets, which can create 'ghost signals' that affect data interpretation.
A new study reveals that magma oceans on rocky exoplanets can affect their size, evolutionary path, and mantle structure. The research found that these ocean's compressible nature can make lava-rich planets denser than solid planets of similar size.
Scientists have discovered a simple test for signs of past or present life on other planets, using artificial intelligence to distinguish between biological and abiotic samples with high accuracy. The method has the potential to revolutionize the search for extraterrestrial life and deepen our understanding of Earth's earliest life.