Articles tagged with Exoplanets
Astronomers have developed a new method to gauge exoplanet pressure by detecting dimer molecules. This technique may also help identify biosignatures of life in extraterrestrial atmospheres. The discovery could be made possible with future powerful telescopes like the James Webb Space Telescope.
Scientists have made the first detection of water in the atmosphere of a hot Jupiter, tau Boötis b, using a novel technique that expands on the radial velocity method. The study confirms the presence of water vapor and also reveals the planet's mass, which was previously difficult to determine.
A team of scientists at Penn State University has detected water vapor in the atmosphere of a hot-Jupiter exoplanet, tau Boötis b. This discovery could help researchers understand how many planets like Earth exist throughout the universe and provides new insights into the formation and evolution of exotic hot-Jupiter planets.
The PLATO mission aims to discover and characterize Earth-like planets in the Sun's neighborhood. With an array of telescopes, it will measure planetary sizes, masses, and ages to determine their habitability. By observing one million stars, PLATO is expected to find thousands of new exoplanets.
Despite recent advances, reliable information about exoplanet atmospheres is scarce due to flawed methods like photometric interpretations. New techniques like spectrometry hold promise for a more comprehensive understanding of exoplanets.
Astrobiology Journal suggests Alpha Centauri B's unique tidal heating could create environments favorable to life. This finding presents a promising target for extrasolar exploration and expands our search for extraterrestrial life.
Researchers found a new giant planet in the Pisces constellation using radial velocity technique, contradicting initial assumption that only single-star systems host planets. The discovery has significant implications for understanding how extrasolar planets are formed and could lead to further discoveries in multiple-star systems.
New measurements of mass reveal that planets smaller than Neptune have low density due to extensive gas coverage, while larger ones have higher density. This suggests these planets formed quickly after their star's birth, contrasting with Earth's late formation.
The Gemini Planet Imager has successfully captured its first light images of exoplanets, allowing scientists to study their atmospheres and characteristics in unprecedented detail. The instrument's advanced technology enables it to detect planets that are millions of times fainter than their parent stars.
The Gemini Planet Imager has captured its first light images, revolutionizing the field of exoplanet detection and study. The instrument's advanced adaptive optics system allows for direct imaging of faint planets, including those 1 million to 10 million times fainter than their host stars.
Astronomers have detected clear evidence of clouds in the atmosphere of GJ 1214b, a super-Earth exoplanet, using data from the Hubble Space Telescope. The findings suggest that high-altitude clouds blanket the planet, hiding information about its composition and behavior.
Two teams of scientists used NASA's Hubble Space Telescope to detect faint water signals in the atmospheres of five distant planets. The strengths of their water signatures varied, with some planets having stronger signals than expected.
Based on Kepler data, scientists found that one in five sun-like stars has an Earth-size planet in its habitable zone. The estimated number suggests that life-supporting planets may be more common than previously thought.
Researchers at MIT have discovered an exoplanet named Kepler 78b that is approximately 1.2 times the size of Earth and has a mass about 1.7 times that of our planet. The planet's density is also similar to Earth's, suggesting it may be composed mainly of rock and iron.
A new study led by UA graduate student Johanna Teske reexamines the composition of a potentially diamond-rich exoplanet, finding it may contain less carbon than previously thought. The analysis, based on revised star observations, suggests that the 'diamond planet' could be more rocky than initially proposed.
Astronomers have confirmed that nearby double star Fomalhaut is actually a triple star system. The discovery was made using precise movements and spectroscopic measurements of astrometric data, revealing a third smaller star in the vicinity. The stars are separated by 5.5 degrees, but their gravitational pull keeps them bound together.
Astronomers have developed a new technique to measure the surface gravity of distant stars, which is crucial for calculating their physical properties and evolutionary state. The technique has been shown to be more accurate than existing methods and can significantly improve estimates of exoplanet sizes.
The TESS mission will map the locations of over 500 transiting exoplanets, including small planets around bright stars. This is the first time NASA has studied a large number of small planets with advanced instruments.
A team of researchers has developed a new method to measure the internal properties of stars, enabling more accurate assessments of their orbiting planets. By using asteroseismology, they were able to determine the mass and rotation rate of a pulsating star, confirming the existence of an exoplanet in its orbit.
Researchers at the University of Montana are building Project Minerva, a dedicated observatory to detect Earth-like exoplanets. The project aims to identify planets in the habitable zone with suitable conditions for liquid water and life.
Astronomers have analyzed eight 'hot Jupiter' exoplanets using the Hubble Space Telescope, revealing a diverse range of puzzling properties. The team found that winds and clouds play a crucial role in shaping the atmospheric composition of these exotic planets.
Astronomer Diana Dragomir reveals the hidden identity of super-Earth HD 97658b, measuring its size and mass for the first time. The exoplanet's density suggests a thick atmosphere, but it orbits too close to its star to support liquid water oceans.
Researchers have found evidence of an exoplanet forming at a distance of about 80 astronomical units (AU) from its star, TW Hydrae. The discovery is surprising as planets typically form closer to the central star.
A team led by University of Louisville doctoral student Karen Collins discovered KELT-6b, a hot Saturn-like planet with an orbit that transits its star every 7.8 days, in the constellation Coma Berenices near Leo.
The study of HR 8799c's atmosphere suggests a core accretion process led to its formation, similar to our Solar System's formation. The exoplanet's composition reveals an elevated carbon-to-oxygen ratio, indicating water ice grains condensed and formed the planet's solid core.
A team of scientists has observed the most detailed spectrum yet of an extrasolar planet, revealing a cloudy atmosphere containing water vapor and carbon monoxide. The findings provide clues to the planet's formation and offer insights into how planets form in other solar systems.
A team of astronomers has made the most detailed examination yet of a Jupiter-like planet beyond our Solar System, discovering a cloudy atmosphere containing carbon monoxide and water vapour. The findings suggest that the system is like a scaled-up Solar System, with gas giants forming at great distances from their parent star
Researchers collected the first chemical fingerprints of a distant solar system's four red exoplanets, revealing unique spectra and peculiar characteristics. The findings suggest that the planets are too toxic and hot to sustain life as we know it.
A team of UChicago astronomers, led by Jacob Bean, is utilizing new methods to analyze the atmospheres of exoplanets, with a focus on distinguishing between gas giants and water worlds. The search for exoplanets has revealed an estimated 17 billion Earth-sized planets in the Milky Way galaxy, potentially harboring life-sustaining worlds.
Astronomers have directly imaged a massive exoplanet, Kappa And b, orbiting the 2.5-solar-mass star Kappa Andromedae. The 'super-Jupiter' has a mass at least 13 times that of Jupiter and is bound to the star.
Astronomers have discovered a super-Jupiter orbiting the star Kappa Andromedae, with a mass about 12.8 times greater than Jupiter's. The object's ambiguity between being a planet or brown dwarf allows researchers to explore theoretical limits of planetary formation.
The Las Cumbres Observatory's Network of Robotic Echelle Spectrograph (NRES) prototype has achieved its first light, primarily designed to support the study of exoplanets. The NRES will extend the capabilities of the LCOGT 1-meter network with six high-resolution spectrographs.
Researchers at Uppsala University will analyze atmospheres of earth-like exoplanets using the CRIRES+ instrument. The project seeks to determine if these planets can support life.
Astronomers at the Gemini Observatory have produced exceptionally high-resolution images of Pluto and its largest companion Charon using a method called reconstructive speckle imaging. The resulting images hint at the exoplanet verification power of large state-of-the-art telescopes combined with speckle imaging techniques.
Researchers at the University of Texas at Austin have developed a simulation model to study how planets form from protostellar disks. The models simulate key factors such as turbulence and temperature, which affect planet formation, providing insights into the conditions most favorable for planetary birth.
The James Webb Space Telescope's NIRISS and FGS instruments, developed by University of Montreal's Professor René Doyon, will study the universe from a record-breaking distance. These Canadian-made instruments will analyze stars and galaxies dating back to the Big Bang and search for life-supporting planetary systems.
Researchers use CRIRES instrument on VLT to study Tau Bootis b's atmosphere, measuring mass and carbon monoxide levels. The new technique allows for the detection of non-transiting exoplanets' atmospheres, enabling scientists to learn more about their atmospheric conditions.
A new method has been developed to measure the mass of non-transiting planets using carbon monoxide signatures in their atmospheres. This breakthrough technique allows for precise mass determination, opening a new path to study exoplanet properties and potentially detect molecules associated with life.
Researchers have successfully measured the motion of exoplanet Tau Bootis b, revealing its mass to be six times that of Jupiter. The team used an innovative technique to unravel direct light from the planet itself, overcoming previous attempts to measure its atmosphere.
The KELT telescope has discovered two unusual planets, including a massive, puffed-up planet dubbed KELT-1b that may challenge our understanding of solar system evolution. The other planet, KELT-2Ab, is a Jupiter-like world with a bright star that will allow astronomers to study its atmosphere.
Research suggests hundreds of billions of free-floating, Earth-sized life-bearing planets exist between stars in the Milky Way. These 'missing mass' planets could mix cosmic primordial life on a galaxy-wide scale.
Computer simulations reveal that giant gas planets prefer certain orbits over others, resulting in 'planet pile-ups' and 'planet deserts'. High-energy radiation from baby stars carves gaps in protoplanetary disks, corralling planets into specific orbits.
Researchers at Lawrence Livermore National Laboratory found a phase change in molten magnesium silicate that transforms to a more dense liquid with increasing pressure. This discovery provides insight into planet formation and suggests that extra-solar 'Super-Earth' planets may have different structures than Earth.
Two new planets, Kepler-34 and Kepler-35, have been discovered orbiting binary suns in the Cygnus constellation. The discovery indicates that planets can revolve around double stars, challenging our understanding of solar systems.
A recent study found that a large fraction of planets have orbital distances between 0.5 and 10 sun-Earth distances, challenging the previous assumption that most extrasolar planets were gas giants closer to their stars.
Astronomers at Vanderbilt University and Caltech discovered three smallest planets yet orbiting a distant star, KOI-961, connected to Barnard's star. The planets range in size from Mars to three-quarters the size of Earth, with short orbits making liquid water impossible.
The Habitable Exoplanets Catalog ranks planets according to various habitability indices, such as the Earth Similarity Index and Habitable Zones Distance. The catalog lists 15 exoplanets and 30 exomoons as potential habitable candidates, with only two confirmed exoplanets matching the criteria so far.
A new system for classifying exoplanets could catalogue newly discovered worlds with potential for life. The methodology uses two indices to describe a planet's Earth-like features and chemical/physical parameters conducive to life.
Researchers have achieved a record pressure of 50 megabars in a diamond experiment at the National Ignition Facility, replicating conditions believed to exist in super-Earths. The use of ramp-compression technique allowed for higher pressures than standard near-instantaneous shock-physics experiments.
Researchers have found visual evidence for two extrasolar planets in archival Hubble data from 1998, using a novel approach to detect faint planet signals. The discovery allows for the tracking of planetary orbits and provides insight into system stability, mass, and eccentricity.
Astronomers have detected stardust in debris discs of extra-solar planetary systems, providing insights into the planet formation process. The Jena research team found two systems with transiting planets, using photometric analysis to identify irregularities in the infrared range.
A University of Toronto-led team has observed extreme brightness changes on a nearby brown dwarf, suggesting the presence of a gigantic storm. The researchers used an infrared camera to capture repeated images of the brown dwarf over several hours, revealing the largest variations in brightness ever seen.
TrES-2b's extremely dark surface is attributed to its high temperature and the presence of light-absorbing chemicals. The planet emits a faint red glow due to its heat, revealing it's not pitch black despite its low reflectivity.
The EPOXI mission discovered that Hartley 2's strong activity in water release and carbon dioxide-powered jets occurred mainly at the ends of the comet, with most occurring at the small end. The study suggests that material in the waist region is likely redeposited material from the ends.
Astronomers at Northwestern University have developed a computer simulation that explains how hot Jupiters form with flipped orbits around their stars. The study, published in Nature, suggests that gravitational perturbations from other planets in the system can cause the inner planet to lose energy and orbit closer to its star.
Researchers have discovered that some extrasolar planets, known as hot Jupiters, can orbit in the opposite direction of their star's spin. This occurs due to gravitational interactions with nearby planets, which perturb the inner planet's orbit and cause it to lose energy via strong tides.
At the AAAS annual meeting, NASA researchers presented several key findings, including a new tool to manage protected areas using remote-sensing data from satellites and aircraft. Scientists also discussed the impact of regional nuclear war on global climate and presented discoveries in zero-gravity environments. Additionally, research...
Researchers discovered a carbon-rich atmosphere in WASP-12b, suggesting rocky exoplanets could be composed of pure carbon rocks like diamond or graphite. This finding introduces an entirely new class of exotic exoplanets to explore, with implications for the possibility of life on these planets.
The newly discovered fourth planet (HR 8799e) orbits a bright star called HR 8799, which lies some 129 light years from Earth and is faintly visible to the naked eye. The mass of the HR 8799 planetary system is much greater than our own.
The discovery of the fourth giant planet in the HR 8799 system strengthens the resemblance between this exoplanetary system and our own, with all four planets being similar in size. Detailed study of HR 8799e will be challenging due to its relative faintness and proximity to its star.