Articles tagged with Exoplanets
Astronomers have detected powerful jetstream winds on the equator of WASP-127b, a giant gas planet located 500 light-years from Earth. The winds reach nearly six times the speed at which the planet rotates, making them the fastest wind ever measured in a jetstream.
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.
Researchers have discovered a mismatched composition of gases in the planet's atmosphere compared to gases within the disk. The study found that the ratio of carbon and oxygen gases in the planet is much lower than expected, suggesting that current models of planet formation may be too simplified.
A new study using the James Webb Space Telescope has reevaluated the atmospheric composition of Trappist-1 b, finding conditions that could support a thick CO2-rich atmosphere. Researchers propose that haze from hydrocarbon compounds in the upper atmosphere may explain this scenario.
A new detection method has been used to identify over 100 small asteroids in the main asteroid belt, ranging from bus-sized to stadium-wide. This breakthrough could aid in tracking potential asteroid impactors and provide insights into meteorite origins.
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.
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.
A team of astronomers from the University of Cambridge found that Venus' interior is too dry for liquid water to have existed on its surface. This conclusion challenges long-held theories and has implications for understanding Earth's uniqueness and searching for life elsewhere in the Solar System.
Researchers at Cornell University have developed a library of basalt-based spectral signatures to help identify the presence of water on exoplanets. By analyzing small spectral differences between basalt samples, scientists can determine if an exoplanet once had running surface water or water in its interior.
The discovery of K2-360 b, an ultra-short period planet with a density similar to lead, reveals clues about its formation. An outer companion, K2-360 c, may have played a crucial role in the system's development through high-eccentricity migration.
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.
Astronomers at Caltech have discovered that the well-studied brown dwarf Gliese 229B is actually a pair of tightly orbiting brown dwarfs weighing about 38 and 34 times the mass of Jupiter. This resolves the long-standing mystery about its dimness.
Astronomers used the combined perspective of Hubble and New Horizons to study the atmosphere of Uranus, a proxy for similar planets beyond our solar system. The results suggest that exoplanets may be dimmer than predicted at partial phases, offering new clues to their potential habitability.
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.
Astronomers have discovered an exoplanet orbiting Barnard's star, located six light-years away, which has at least half the mass of Venus and orbits its star in just over three Earth days. The discovery was made using ESO's VLT and confirms the existence of a new exoplanet candidate, while also hinting at the presence of three more.
Researchers from University of Texas at Arlington have identified 206 systems of interest for potential habitability, including one system where the planet is always situated in the HZ. The team analyzed data from NASA Exoplanet Archive and found F-type stars to be a promising case for life beyond Earth.
A team of astronomers discovered a planetary system that resembles the sun-Earth system, with an Earth-size companion in an orbit twice as large as Earth's today. The discovery provides insight into the evolution of main sequence stars and their impact on planets.
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 have observed a uniquely inflated and asymmetric exoplanet called WASP-107b using the James Webb Space Telescope. The exoplanet has an east-west asymmetry in its atmosphere, which may help scientists understand its climate and atmospheric dynamics.
Researchers have developed a method using physics-informed neural networks to model the complex light scattering in exoplanet atmospheres. This breakthrough enables more accurate analysis of exoplanet atmospheres, particularly with regard to cloud influence and chemical composition.
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.
The James Webb Space Telescope has identified six likely rogue worlds, including the lightest ever found with a dusty disk around it. These objects offer insights into how stars and planets form, suggesting that gas giants can form in disks around young stars.
Researchers found that as planet mass increases, water tends to integrate with the iron core, leading to a reevaluation of astronomical observation data and planetary habitability. This discovery has significant implications for the study of Super-Earths and the search for life beyond Earth.
The Ariel Data Challenge 2024 aims to extract faint exoplanetary signals from noisy space telescope observations, with a focus on overcoming noise sources like 'jitter noise'. The competition offers a unique chance for data scientists and AI enthusiasts to contribute to cutting-edge research in exoplanet atmospheres.
Astronomers have imaged the coldest exoplanet ever detected using JWST, which agrees with models of planet evolution and solar system ages. The exoplanet orbits a super-Jupiter in the Epsilon Indi triple star system and has a mass six times that of Jupiter.
Astronomers have directly imaged the coldest exoplanet, Epsilon Indi Ab, using NASA's James Webb Space Telescope. The planet is around 2 degrees Celsius colder than previously imaged planets, providing a rare opportunity to study its atmospheric composition.
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...
A team of astronomers has successfully detected evidence of water vapor in the atmosphere of a scorching hot Saturn, HD 149026 b. This finding is significant because it challenges the conventional wisdom that such extreme environments should not support liquid water.
The European Space Agency's PLATO mission aims to find nearby potentially habitable worlds around Sun-like stars. The space telescope will blast into orbit in December 2026 and study the stars using a range of techniques, including asteroseismology, to work out their masses, radii, and ages.
Astronomers at MIT and Penn State have discovered a new 'progenitor' of hot Jupiters, a highly eccentric planet with an orbit providing clues to its evolution. The planet, TIC 241249530 b, is expected to become a scorching hot Jupiter in about 1 billion years.
A team of astronomers has discovered an exoplanet with an elongated and backwards orbit, which holds clues to the formation history and future trajectories of high-mass gas giants. The exoplanet, named TIC 241249530 b, is approximately five times more massive than Jupiter and orbits its host star in a highly eccentric path.
Researchers discovered a highly eccentric exoplanet named TIC 241249530 with an orbital eccentricity of 0.94, causing extreme temperature variations. The planet's unusual backward-orbiting motion provides insight into the formation history and future trajectories of hot Jupiters.
Researchers detected distinct 'morning' and 'evening' sides on the exoplanet WASP-39b using James Webb Space Telescope data. The study found that the morning side was significantly cooler (600°C) compared to the evening side (800°C), with cloudier conditions also prevalent in the morning.
Researchers using NASA's James Webb Space Telescope have confirmed a significant temperature difference between the morning and evening atmosphere of WASP-39b, with the evening appearing hotter by roughly 300°F (200°C). The planet is tidally locked, resulting in constant dayside and nightside conditions.
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.
A study by University of Texas at Dallas geoscientist Dr. Robert Stern and colleague Taras Gerya suggests that plate tectonics, oceans, and continents are necessary for the evolution of intelligent civilizations. The researchers propose refining the Drake equation factor to account for these requirements, which could explain the Fermi ...
The 2024 Kavli Prize Laureates have made significant contributions to our understanding of exoplanet atmospheres, nanoscale materials for biomedical applications, and the localization of brain areas specialized for face recognition. Their work has broadened our knowledge of planetary life beyond Earth.
Researchers used high-energy laser experiments to study magnesium oxide's melting point and phase transitions under ultra-high pressures. The findings suggest the mineral could be the earliest solid to crystallize in forming super-Earths.
The James Webb Space Telescope has captured evidence of a cataclysmic asteroid collision in the Beta Pictoris star system, which is thought to be similar to our own solar system's early stages. The collision is believed to have occurred about 20 years ago and pulverized the asteroids into fine dust particles.
Astronomers have discovered a sulfurous atmosphere on the smallest and coldest exoplanet known, providing clues to its formation process. The planet's unique orbit and composition offer insights into how planets are created.
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.
The newly discovered exoplanet, nicknamed Phoenix, has a surprisingly large and dense atmosphere, challenging current understanding of planetary evolution in extreme environments. Scientists estimate that the planet will survive for only 100 million years before dying due to its proximity to the star.
Researchers used the TESS-Keck Survey to detect and characterize 126 exoplanets, including 15 new ones. The study utilized both the transit method and radial velocity technique to determine the planets' masses. This collaboration provides new insights into the makeup of exoplanet systems and their host stars.
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.
Astronomers have discovered an Earth-like exoplanet 40 light-years away with a surface temperature of 42°C (107°F), making it potentially habitable. The discovery of Gliese 12 b offers insights into the evolution of habitability on planets across our galaxy.
The James Webb Space Telescope has provided the first measurements of an exoplanet's core mass, with WASP-107 b showing a thousand times less methane than expected. The planet's super-sized core and turbulent atmosphere are being studied to better understand how planetary atmospheres behave in extreme conditions.
The James Webb Space Telescope has provided new insights into the mysterious case of WASP-107 b, an exoplanet that defies explanation due to its inflated size. Data collected by Webb shows surprisingly little methane in the planet's atmosphere, indicating a significantly hotter interior and core mass than previously estimated.
The SPECULOOS project has discovered an Earth-sized exoplanet around SPECULOOS-3, a nearby ultra-cool dwarf star. The planet, named SPECULOOS-3 b, is similar in size to our own planet and orbits the star in just 17 hours, resulting in constant day and night conditions.
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 newly discovered SPECULOOS-3b is an Earth-sized, likely airless planet orbiting a nearby ultracool dwarf star. The planet's extremely close proximity to its star has likely vaporized any atmosphere, allowing scientists to study its surface composition and history in unprecedented detail.
Scientists have discovered a new planet called WASP-193b that is 50% bigger than Jupiter yet has a density comparable to cotton candy. The planet's low density makes it an outlier among the over 5,400 planets discovered so far.
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 new rocky planet, TOI-6713.01, has been found to be covered with active volcanoes, making it glow with a fiery, glowing-red hue. The planet's surface temperature reaches 2,600 degrees Kelvin due to gravitational forces that cause it to experience tidal energy.
A recent study suggests that 55 Cancri e's atmosphere may be composed of carbon-rich vapor, contradicting its initial uninhabitable status. The discovery was made possible by the James Webb Space Telescope and demonstrates the potential for future telescopes to study distant rocky planets in detail.
A new study led by Dr. Assaf Hochman uncovers ozone's impact on atmospheric stability and temperature distribution on Proxima Centauri b, a habitable exoplanet tantalizingly close to Earth's solar system. The research highlights the importance of considering interactive ozone in understanding Earth-like exoplanets.