Articles tagged with Exoplanets
Researchers use Earth's geological record to identify vegetation signatures on exoplanets, which can indicate the presence of life. The study found that as plants evolved on Earth, their signature became stronger, making older exoplanets more promising targets for detecting vegetation.
TESS has shared its first science image, revealing a wealth of stars and other objects in the southern sky. The image captures systems previously known to have exoplanets, highlighting the mission's potential to discover new worlds.
Researchers used data from NASA's Kepler Space Telescope to discover Wolf 503b, an exoplanet with a radius near the 'Fulton gap', and is part of a class of 'super-Earths'. The discovery provides insights into the origin of this size gap and the nature of these planets.
Scientists have found that many exoplanets, especially those between two to four times the size of Earth, are likely to be water-rich. This suggests that water worlds may be common, with implications for the search for life in our Galaxy.
Researchers measured compositions of 18 planetary systems up to 456 light years away, finding similar proportions of elements to those on Earth. The study suggests that Earth-like planets may exist elsewhere in the galaxy.
Astronomers have detected iron and titanium vapors in the atmosphere of KELT-9b, an ultra-hot Jupiter, using spectroscopy. The high temperatures break apart molecules, making these atomic species visible.
Researchers have developed a reference catalog of light spectra and albedos for 19 solar system bodies. By comparing this catalog to exoplanet observations, scientists can characterize new worlds in reference to our own diverse planetary system. The catalog offers insights into the challenges of categorizing rocky and icy exoplanets.
TESS starts its search for planets, monitoring the nearest and brightest stars for periodic dips in their light, which suggest a planet may be passing in front of its star. The mission aims to discover thousands of exoplanets, some potentially supporting life.
Scientists have found a new exoplanet, 2MASS 0249 c, that is nearly identical to the well-studied gas-giant planet beta Pictoris b. The two planets share similar mass, brightness, and spectrum but differ in their formation environments, with one orbiting a bright star and the other a pair of faint brown dwarfs.
The James Webb Space Telescope will observe the atmospheres of gas giant exoplanets, including WASP-79b and WASP-43b, to detect water, carbon monoxide, and other molecules. The telescope aims to understand the physical processes responsible for these variations and their implications for potentially habitable planets.
Researchers have determined the detailed chemical abundances of Ross 128, a red dwarf star that hosts an exoplanet similar to our Solar System's Jupiter. This helps estimate the makeup of Ross 128 b, indicating it should be rocky with a temperate climate.
Scientists estimate that planets around almost every star in the galaxy may harbor life, prompting new research to identify biosignatures. Researchers propose solutions to detect gases and light signatures produced by life on exoplanets.
The UCR team's guidebook outlines three types of biosignatures that astrobiologists have proposed as markers for life on other planets. The review articles provide a comprehensive framework for scientists searching for signs of life, called biosignatures, in the data they collect from future telescope observations.
An international team of astronomers detected molecules on an exoplanet, allowing it to be visualized. The technique reveals the planet's surface composition and temperature, providing new insights into planetary atmospheres. Future spectrographs will enhance this method, enabling more accurate characterization of planets.
A team of astronomers has developed a new technique to find young extrasolar planets by analyzing the motion of gas in protoplanetary disks. The method successfully confirmed the existence of two Jupiter-mass planets around star HD 163296, providing insight into planet formation and the process that shaped our own solar system.
A Rutgers-led ENIGMA team will investigate the evolution of protein nanomachines, which may have arisen before life began, using a $6 million NASA grant. The team aims to understand the earliest processes that support life, including the movement of electrons and hydrogen atoms.
The Transiting Exoplanet Survey Satellite (TESS) has completed a lunar flyby, providing a gravity assist to help it reach its final working orbit. As part of camera commissioning, TESS snapped a two-second test exposure revealing over 200,000 stars in the southern constellation Centaurus.
Scientists discovered a new hot Jupiter exoplanet, KPS-1b, using data from an amateur astronomer. The exoplanet orbits a star similar to the Sun and has a mass and size close to that of Jupiter. Its proximity to its parent star results in extremely high temperatures in its atmosphere.
Researchers at UCR's Alternative Earths Astrobiology Center are developing a framework for dynamic biosignatures based on seasonal changes. They found that ozone could be a more easily measurable marker for seasonal variability in oxygen, which is produced by life. Observing atmospheric seasonality in exoplanets may help detect life.
Scientists have detected an exoplanet atmosphere free of clouds, marking a pivotal breakthrough in understanding planets beyond our solar system. The 'hot Saturn' WASP-96b's clear sodium signature is the result of its cloud-free atmosphere.
Astronomers have successfully detected helium in the atmosphere of WASP-107b, a super-Neptune exoplanet. The detection was made using the Hubble Space Telescope and reveals an abundance of helium in the upper atmosphere, extending tens of thousands of kilometres into space.
Researchers simulated conditions inside a planet three times larger than Earth using high-powered laser beams. The study revealed that the crystal structure of iron-silicon alloys changes with higher silicon content under extreme pressures, providing new insights into the nature of super-Earths and their cores.
The discovery of 51 Pegasi b marked a significant milestone in the search for exoplanets, with Michel Mayor and his colleague Queloz credited with the groundbreaking find. The development of better telescopes enabled this achievement, contributing to a new community of researchers exploring this field.
The Transiting Exoplanet Survey Satellite (TESS) will survey nearly the entire sky for signs of passing planets. The spacecraft aims to detect thousands of stars hosting transiting planets and measure the masses of at least 50 small planets less than four times that of Earth.
Researchers have developed chemical models from car engines to study the atmospheres of hot exoplanets. The results show deviations in these atmospheres due to extreme temperatures and pressures.
A team of MIT researchers has developed a machine-learning system that can automatically search for debris disks around stars, indicating the presence of exoplanets. The system achieved a 97% accuracy rate and identified 367 previously unexamined celestial objects as promising candidates for further study.
Scientists at Johns Hopkins University conducted the first laboratory simulations of exoplanet atmospheres to understand haze formation and its impact on habitability. The study found that certain gas combinations produce more haze particles, which can affect atmospheric temperature structures and potentially shield life.
Astronomers have discovered a trio of super-Earths around the star GJ 9827, with two of them having radii between 1.7 times and 2.5 times that of Earth, sparking debate about their composition. The study's findings provide insight into how these planets form and evolve, with implications for the search for life beyond our Solar System.
Scientists from NASA and universities are investigating exoplanets to determine their habitability, focusing on astrophysics, Earth science, heliophysics, and planetary science. Researchers use tools like DSCOVR's high-resolution images to simulate habitable planets and study the interaction between stars and planets.
The oversized planet WASP-18b is wrapped in a smothering stratosphere loaded with carbon monoxide and devoid of water. The formation of this atmosphere is attributed to 'sunscreen'-like molecules absorbing UV radiation and releasing heat, which is unusual compared to other gas giants.
Researchers have discovered two super-Earths around the red dwarf star K2-18, one of which could be a scaled-up version of our own planet. The newly found planet, K2-18c, is likely too hot to support life, but its companion, K2-18b, has potential for liquid surface water and might harbor conditions suitable for life.
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.
Researchers suggest hunting for cruder signatures of potentially habitable worlds, which would be easier to detect with current resources in less time. They look for atmospheres rich with water vapor and nitrogen, and oxygen, as these are basic molecules that are biologically friendly and have strong infrared emitting power.
A citizen scientist has discovered a comet's tail streaking past a distant star using data from the Kepler Space Telescope. The discovery marks the first time an object as small as a comet has been inferred by observing dips in a star's light.
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.
Researchers used a new model to simulate atmospheric conditions in three dimensions, revealing a key role for stellar radiation in creating moist greenhouse states on exoplanets. This process could make planets closer to their stars habitable despite intense radiation and tidal forces.
Astronomers have discovered an exoplanet, GJ 436b, with a huge gas cloud resembling a comet's tail, caused by intense stellar irradiation. The planet's atmosphere loses hydrogen due to the star's radiation, forming a massive cloud that absorbs UV radiation.
KFU astronomers have made a groundbreaking discovery of an exoplanet orbiting a red giant star HD208897, located 210 light years away from Earth. The planet has a mass of 1.4 Jupiter masses and an orbital period of 353 days, marking the first time in Russian astronomy such a discovery was made using spectroscopic methods.
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 at the University of Texas at Arlington predicted an additional Earth-like planet in the Gliese 832 system, with stable orbital configuration and mass range of 1-15 Earth masses. The team analyzed simulated data using injected Earth-mass planet to find a habitable zone for potential new world.
Astronomer Rory Barnes finds that tidal locking is a major factor in the evolution of potentially habitable exoplanets, suggesting they may be more common than previously thought. The research suggests that even Earth's 'twin' could be tidally locked.
TESS will survey stars up to 100 times brighter than Kepler, finding thousands of new exoplanets around bright nearby stars. The mission will provide ideal targets for follow-up observations with the James Webb Space Telescope.
Researchers have found compelling evidence for a stratosphere on the enormous planet WASP-121b, hot enough to boil iron. The discovery was made using NASA's Hubble Space Telescope and indicates a strong stratosphere on this gas giant exoplanet.
Scientists have found a stratosphere on an enormous gas giant exoplanet WASP-121b with an atmosphere hot enough to boil iron. The discovery was made using spectroscopy to analyze the planet's brightness at different wavelengths of light, revealing glowing water molecules.
The Planetary Spectrum Generator (PSG) is being enhanced with additional databases to provide more accurate predictions of instrument performance. This will enable scientists to design and plan future missions more efficiently, reducing costs and resources.
A computer model suggests that Proxima b's atmosphere could be lost 10,000 times faster than Earth's due to extreme ultraviolet radiation from its host star. The study considers factors like thermosphere temperature and magnetic field orientation to understand the impact of stellar physics on habitability.
Astronomers have discovered an exoplanet, HIP65426b, using the SPHERE/VLT instrument for the first time. The planet is located at three times the Earth-Neptune distance from its star and has a mass 6 to 12 times higher than Jupiter.
Research suggests that exoplanets near cool, low-mass stars require strong magnetic fields to shield their atmospheres from harmful X-rays and extreme pressure. The study models CMEs in a cool star system and finds that most CMEs are trapped by the star's surface, posing a significant threat to planetary habitability.
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.
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.
Scientists have discovered an exoplanet, KELT-9b, hotter than most stars, with a day-side temperature of 4,600 Kelvin. The planet's atmosphere is being evaporated due to intense ultraviolet radiation from its host star.
Researchers used the Met Office Unified Model to simulate Proxima B's climate, finding it could have a habitable atmosphere and stable climate regime. The team also explored different atmospheric compositions and orbital configurations, suggesting the planet could support life.
Astronomers have found clear signs of water in the atmosphere of HAT-P-26b, a Neptune-sized exoplanet. The presence of water suggests that the planet's gaseous envelope formed late in its formation process, with little to no pollution by impacting debris.
Astronomers predict that combining NIRISS and NIRSpec on James Webb Space Telescope will maximize information content about exoplanet atmospheres. This combination allows for the observation of key chemical compounds such as water, methane, and carbon dioxide.
A team of researchers discovered that SIMP J013656.5+093347 is a planetary mass object, rather than a brown dwarf, due to its mass being at the boundary between brown dwarf-like and planet-like properties. This finding offers new insights into the atmospheres of gas giant exoplanets.
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.
Astronomers have discovered a super-Earth orbiting a quiet red dwarf star, LHS 1140, in the habitable zone where liquid water can exist. The exoplanet's large size and dense iron core suggest it may have retained an atmosphere long after its star calmed down.
The DFG is funding six new research units and two humanities centers focusing on topics such as plant morphodynamics, Russian lyric poetry, and trace element interactions. These initiatives aim to advance knowledge in various fields and tackle pressing issues.
A team of scientists led by Jonathan Gagné has found evidence of undetected giant exoplanets in the TW Hya star association, approximately 100 light years from Earth. The researchers used an initial mass function to calculate the distribution of mass in the group and predict the number of undiscovered objects.
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.