Articles tagged with Exoplanets
A new approach aims to identify planets orbiting nearby stars that support life by focusing on creating a comprehensive list of molecules in their atmospheres. Researchers have searched for thousands of potentially biogenic gas molecules, sparking new research into identifying larger molecules and their potential as signs of life.
A new optical technology developed by Russian physicists can significantly improve the detection of exoplanets, allowing for direct observation of their images. The 'smoothed' light technique uses adaptive optics to remove atmospheric distortions, enabling telescopes to resolve the faint signals of Earth-type planets.
A Penn State-led research group has been selected by NASA to build a new instrument to detect planets orbiting stars outside our solar system. The NEID instrument will use the tiny gravitational tug of planets on their stars to discover and measure the orbits of rocky planets with liquid water.
Scientists have observed an exoplanet named HD 80606 b that orbits its star at incredible distances, experiencing scorching temperatures and then plummeting to extremely cold temperatures as it moves away. This unique system challenges existing theories on the formation of hot Jupiters and may require alternative explanations.
Astronomers have measured the rotation rate of a massive exoplanet using NASA's Hubble Space Telescope, revealing patchy and colorless cloud layers. The super-Jupiter completes one rotation every 10 hours, similar to Jupiter, with temperatures reaching 2,200-2,600 degrees Fahrenheit.
Astronomers at the University of Arizona have taken the first direct, time-resolved images of an exoplanet using NASA's Hubble Space Telescope. The young exoplanet, 2M1207b, has a patchy cloud pattern and rotates twice as fast as Earth.
The Wide Field Infrared Survey Telescope (WFIRST) will aid researchers in unraveling the secrets of the universe by studying dark energy and dark matter. The observatory will discover new worlds outside our solar system and advance the search for life-suitable planets.
Astronomers have studied ten hot Jupiter-sized exoplanets in detail using Hubble and Spitzer telescopes. The results show that planetary atmospheres are more diverse than expected, with some planets containing clouds and haze that hide water from view. This solves the mystery of why some exoplanets appear to have less water than expected.
Scientists have finally shed light on the atmospheres of a group of planets orbiting stars outside our solar system. A team of experts analyzed observations from NASA and ESA telescopes, revealing that water was hidden by haze and cloud on some hot-Jupiter exoplanets.
A newly discovered exoplanet, HD 106906 b, may have been violently ejected from its birthplace close to its star due to a recent gravitational disturbance. The planet is surrounded by a large dust ring or shroud, which could be evidence of the violent episode.
The Visible Nulling Coronagraph (VNC) technology has demonstrated improved sensitivity over a broader spectral range, making it a stronger contender for a future astrophysics mission. The instrument will enable spectroscopy to study exoplanet atmospheres and identify signs of life.
Researchers found that a fractal hydrocarbon haze on early Earth could have resulted in a moderate, possibly habitable average global temperature. The haze also would have absorbed ultraviolet light, shielding the planet from deadly radiation.
The discovery of GJ 1132b, an Earth-size exoplanet located just 39 light-years away from our Solar System, is a significant milestone in the search for alien life. The planet's proximity to its star and size make it an ideal laboratory for studying small, potentially livable worlds.
Scientists have discovered a new exoplanet, GJ 1132b, that is rocky and Earth-sized, orbiting a small star just 39 light-years from Earth. The planet's surface temperature is estimated to be around 500 degrees Fahrenheit, making it uninhabitable for life as we know it.
Scientists have simulated 3D exotic clouds on GJ1214b, an exoplanet with a flat spectrum that indicates high-altitude clouds or haze in its atmosphere. The clouds could be of salt and are thought to form deep in the atmosphere before rising into the upper atmosphere.
Scientists from KU Leuven discovered that two of three possible climates on rocky exoplanets are potentially habitable. The 'air conditioning system' keeps surface temperatures within the habitable range, despite permanent day and night sides. This finding provides valuable input for future space missions.
Research suggests oxygen in atmospheres of habitable extrasolar planets might not necessarily come from biological processes, potentially expanding the search for life. Scientists have proposed alternative explanations for oxygen formation, including abiotic reactions on planetary surfaces.
Astronomers have discovered a young, Jupiter-like exoplanet that provides insights into planetary origins. The Gemini Planet Imager revealed 51 Eridani b, which is still warm and luminous from its formation, with conditions that depend on whether it formed slowly or suddenly.
Astronomers using Gemini Observatory's new Planet Imager have probed a newly discovered world in unprecedented detail. The planet, 51 Eridani b, is about two times the mass of Jupiter and features a Solar System-like atmosphere with methane detection.
The Gemini Planet Imager has made its first exoplanet discovery, revealing a planet that may be the lowest-mass exoplanet ever directly imaged. Weighing twice as much as Jupiter, this finding provides insights into how our solar system was formed and paves the way for further research.
The team discovered a Jupiter-like planet, called 51 Eridani b, about twice the size of Jupiter and featuring the strongest methane signature ever detected on an alien planet. The discovery sheds light on how planets formed around our sun and could unlock secrets of gas giants' planetary systems.
A team of researchers has discovered a Jupiter-like planet, 51 Eridani b, within a young system that could provide new understanding of how planets formed around our sun. The planet shows the strongest methane signature ever detected on an alien planet, yielding clues about its formation.
Scientists have discovered a Jupiter-like planet in the young system 51 Eridani b, featuring the strongest atmospheric methane signal ever detected. The exoplanet's unique characteristics hint at its rapid formation process, offering insights into solar system evolution.
A team of astronomers has discovered a Jupiter-like exoplanet called 51 Eridani b, which shows the strongest methane signature ever detected on an alien planet. The new planet is the faintest exoplanet on record and provides clues about how planets formed around the sun.
Scientists have discovered a young Jupiter-like exoplanet, 51 Eridani b, with the strongest methane signature ever detected in an alien planet's atmosphere. The exoplanet is roughly twice the mass of Jupiter and offers insights into planet formation and the early stages of star development.
The newly discovered exoplanet, 51 Eridani b, is a young Jupiter-like planet with the strongest methane signature ever detected on an alien planet. Its mass and atmospheric composition suggest that it formed in a similar way to Jupiter in its infancy.
Astronomers confirm exoplanet orbiting far from its central star using gravitational microlensing, opening new discovery space for long-period orbits. The Uranus-sized planet is about 370 million miles from its parent star, with a host star about 70% as massive as our Sun.
Astronomers have discovered a powerful aurora on a brown dwarf, 10,000 times more powerful than any seen before. The discovery reveals a major difference in magnetic activity between low-mass stars and planets.
A new study has precisely measured the ages of 33 Kepler stars with solar-like oscillations, revealing that even stars older than 11 billion years have Earth-like planets. The research uses asteroseismology to analyze tiny variations in starlight and provides a large sample for studying galactic archeology.
Astronomers have discovered a massive cloud of hydrogen, dubbed 'The Behemoth,' evaporating from a warm Neptune-sized planet orbiting a nearby star. The phenomenon may help explain the existence of Hot Super-Earths and provide insights into how planets lose their outer layers.
Researchers discover a giant cloud of hydrogen gas being burnt off from the atmosphere of GJ 436b, an exoplanet orbiting a warm red dwarf star. The cloud forms a comet-like tail as ultraviolet light pushes hydrogen into spiral motion, with 1000 metric tonnes being lost every second.
A team of scientists has discovered a massive cloud of hydrogen escaping from the atmosphere of GJ436b, a Neptune-sized exoplanet located 33 light years away. This phenomenon may help explain the formation of hot and rocky 'super-earths' and potentially detect extrasolar oceans.
Astronomers have successfully commissioned a new type of optic that can reveal the image of an exoplanet next to its parent star. The vector-APP coronagraph uses advanced liquid crystal technology to cancel out starlight, allowing fainter planets to be imaged.
The discovery of a stratosphere on WASP-33b offers insights into the planet's composition and formation. The presence of titanium oxide in the atmosphere indicates temperature inversion, similar to Earth's ozone layer.
A team of UW graduate students has found a way to detect volcanic activity in the atmospheres of exoplanets during their transits. This could help choose worlds to study for possible life and determine if they are habitable. Volcanism regulates planetary temperatures, making it a key element in habitability.
A team of astronomers found that 74 Earth-sized exoplanets orbit their stars in circular patterns, contrary to expectations. This discovery suggests that small planets may maintain stable climates year-round, making them more hospitable to life.
Researchers discovered daily weather cycles on six exoplanets, with cloudy mornings and hot afternoons, using sensitive Kepler observations. The study found that winds transport clouds to the day side, heating them up and dissipating them, resulting in clear skies during the afternoon.
The LEECH exoplanets survey has obtained new images of HR 8799, a 30-million-year-old star with four known giant planets. The team found that the system likely consists of multiple double resonances, indicating gravitational interactions between the planets.
A team of international scientists has created a colorful catalog of reflection signatures from various Earth life forms to aid in the search for extraterrestrial life. The database features 137 diverse life forms, including extremophiles from extreme environments, which can help astronomers spot potential biosignatures on exoplanets.
Astronomers have discovered a star that is 11.2 billion years old and has at least five Earth-size planets, revealing that planetary formation occurred throughout the universe's history. The system, Kepler-444, consists of five planets with sizes between Mercury and Venus, orbiting a smaller star than our sun.
Astronomers have discovered a star with three planets only slightly larger than Earth, one of which orbits in the habitable zone where surface temperatures could be moderate enough for liquid water and life to exist. The study found that these planets are about 2.1, 1.7, and 1.5 times the size of Earth.
A study suggests that exoplanets are more likely to have liquid water and be habitable due to their rotation speed, which can create a day-night cycle. This finding challenges the traditional assumption that all exoplanets exhibit synchronous rotation, potentially increasing their ability to develop life.
The Gemini Planet Imager (GPI) has produced high-quality exoplanet images and spectra from its first year of science operations. The instrument's advanced imaging capabilities have revealed significant differences in the colors of two planets in the HR 8799 system, suggesting unique atmospheric compositions.
Astronomers have found evidence that the recipe for Earth applies to terrestrial exoplanets orbiting distant stars. The HARPS-North instrument measured the masses of small, Earth-sized worlds and found a tight relationship between mass and size, suggesting rocky compositions similar to those of Venus and Earth.
Researchers at Lomonosov Moscow State University developed a new method to estimate the magnetic field of an exoplanet. They successfully estimated the magnetic moment of the hot Jupiter HD 209458b, which is relatively small compared to Earth's magnetic field.
The European satellite Gaia is expected to detect tens of thousands of new planets within its five-year mission, revealing unique details about each planet's properties. The satellite's instruments will also capture the motion, physical characteristics, and distance of roughly 1 billion objects in the Milky Way galaxy.
Astronomers develop a new laser-based technology called the green astro-comb to detect tiny Doppler shifts, helping identify habitable zone planets. The device will enable precise measurements of exoplanet gravity, allowing for better detection of rocky worlds like Earth.
A team of scientists used the Hubble Space Telescope to create a detailed weather map of WASP-43b, tracing the planet's temperature and water vapor content. The study found that the exoplanet has winds that can reach up to 1500 degrees Celsius, with temperatures on the day side hot enough to melt iron.
A new study has shown that the water found on Earth originated before the Sun formed, suggesting that many exoplanets may also have access to abundant water. This discovery has important implications for the potential for life elsewhere in the galaxy.
Researchers have detected water vapor and hydrogen on the exoplanet HAT P-11b, a planet about four times bigger than Earth. This discovery supports astronomers' ideas about planetary formation and suggests that small planets may be rich in heavy elements like oxygen.
Physicists from UT Arlington believe following a trail of radio wave emissions may lead them to the discovery of an exomoon. They suggest using detailed calculations about the Jupiter/Io dynamic to look for radio emissions that could indicate moons orbiting an exoplanet.
A team of astronomers using NASA's Hubble Space Telescope measured water vapour in the atmospheres of three gas giants, finding levels one-tenth to one-thousandth that predicted by standard theory. This discovery raises questions about exoplanet formation and highlights challenges in searching for water on Earth-like planets.
Research by Penn State scientists has debunked the existence of two controversial planets around dwarf star Gliese 581, which were believed to be prime targets in the search for extraterrestrial life. The study confirms that signals from the stars' magnetic activity, not the planets themselves, caused the initial findings.
Researchers found that planets between 1.7 and 3.9 times the size of Earth are dubbed 'gas dwarfs' with thick atmospheres of hydrogen and helium. The study also revealed that metallicity plays a crucial role in determining planetary composition, with stars hosting gas giants containing about 50% more metals than our Sun.
A team using the Gemini Planet Imager's next-generation adaptive optics system tracked the orbit of Beta Pictoris b, a planet with an estimated mass at least four times that of Jupiter. The team refined the estimate by analyzing images and debris discs around the star.
Researchers have discovered a gas giant exoplanet, GU Psc b, located 2,000 times closer to its star than Earth is to the Sun. The planet's massive size and distance from its star make it an ideal object for studying giant exoplanets.
Astronomers from Leiden University and SRON have measured the spin of Beta Pictoris b, an exoplanet orbiting a naked-eye star 63 light-years from Earth. The planet's day length is just 8 hours, despite being over 16 times larger and 3000 times more massive than Earth.
A new study suggests that detecting life on exoplanets is more difficult than previously thought, as a lifeless planet can mimic the same results as one with a biosignature. The resolution needed to distinguish between genuine and false positives is impossible with current telescopes.
Scientists at NRL detected water vapor in the atmosphere of tau Boo b, a hot Jupiter outside our solar system. The team measured the motion of the planet to establish its presence and determined it's six times more massive than Jupiter.
Researchers have found a mysterious 'shepherd' exoplanet in the Beta Pictoris system, which suggests that the system may be capable of supporting life. The planet is believed to be about the size of Saturn and is thought to be responsible for corraling a swarm of icy comets.