Articles tagged with Exoplanets
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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.
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.
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.
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.
The UMD-led EPOXI spacecraft flew by comet Hartley 2 at a distance of 435 miles, collecting never-before-seen images that will help scientists understand the composition and diversity of comets. The mission aims to learn more about the origin and history of our solar system by studying the material from comets.
Using new optics technology developed at the University of Arizona's Steward Observatory, astronomers have obtained images of a planet on a closer orbit around its parent star than any other extrasolar planet previously found. The discovery enables scientists to search for planets closer to the star than has been previously possible.
Astronomer Joel Kastner finds evidence that a variable star in the Pisces constellation is a one billion-year-old red giant that has swallowed a companion star, forming an orbiting disk that may contain second-generation planets. The star's extreme properties and X-ray production rate point to its advanced age.
Rochester Institute of Technology scientist Don Figer is developing a new detector technology that can directly image and characterize exoplanets, potentially finding smaller, rocky planets like Earth. This technology could reduce detection time by one-third and overcome current limitations.
The discovery of exoplanet Beta Pictoris b, located 60 light-years from Earth, confirms that giant planets can form in time-spans as short as a few million years. The planet has a massive nine-Jupiter-mass orbit, challenging previous theories on planetary formation.
Astronomers discover six exoplanets orbiting their stars in the opposite direction to the star's rotation, contradicting conventional wisdom. This finding sparks alternative migration theories, suggesting that hot Jupiters may form far from their stars and migrate inward due to gravitational interactions with distant companions.
An international team of scientists has discovered a new planet called CoRoT-9b, similar in size to Jupiter. Located 1500 light-years from Earth, the planet orbits a star similar to our sun and is considered temperate.
Astronomers have discovered a temperate exoplanet, Corot-9b, with a mass about 80% that of Jupiter and an orbit similar to Mercury's. The planet is thought to have a temperature range of -20°C to 160°C, making it a significant finding in the study of exoplanets.
The University of California, Berkeley team's paper published in Science won the 2009 Newcomb Cleveland Prize for outstanding contributions to the field. The award recognizes the first visible-light picture of an extrasolar planet and its potential to change our view of how planets originate.
Astronomers from Caltech and other institutions have detected an extrasolar planet, HD 156668b, with a mass just four times that of Earth. The discovery highlights the potential for finding Earth-mass planets in the habitable zone, making it a promising lead in the search for life beyond our solar system.
Drake Deming, a Senior Scientist at NASA's Goddard Space Flight Center, has won the prestigious Beatrice M. Tinsley Prize for his pioneering work detecting thermal infrared emission from transiting extrasolar planets using the Spitzer Space Telescope. The prize recognizes Deming's outstanding research contribution to astronomy and astr...
The NASA Deep Impact spacecraft has captured videos of sun glints from space, indicating the presence of large bodies of water on Earth. The observations provide a way to detect planets beyond our solar system that are likely to have expanses of liquid, increasing the chances of finding life.
Astronomers found that only 10 percent of stars host planetary systems similar to our own, with several gas giant planets in the outer part of the system. The discovery was made using gravitational microlensing and is based on 10 years' worth of data from the MicroFUN survey.
Astronomers have directly imaged a faint celestial body orbiting the star GJ 758, estimated to be between 10 and 40 Jupiter masses. The discovered planet, GJ 758 B, has a temperature of around 330 degrees Celsius, making it the coldest companion of a Sun-like star ever imaged.
An international team of scientists has made the first direct observation of a planet-like object orbiting a star similar to the sun. The object, GJ 758 B, is estimated to be 10-40 times as massive as Jupiter and orbits its star at a distance of approximately 300 trillion miles.
The study uses radio telescope images to confirm the presence of a rotating molecular disk orbiting the young binary star system V4046 Sagittarii. The discovery expands the number of places to look for extrasolar planets, suggesting that planet formation may occur around double stars as easily as single stars.
Astronomers have devised a technique to identify liquid water on exoplanets similar to Earth, which could indicate potential for life. The method uses observations of light intensity from Earth in visible light bands, revealing dominant colors that suggest land masses and oceans.