Astronomers have detected water vapor in the atmosphere of HD 189733b, a gas giant 63 light-years away. The presence of water vapour suggests that the planet may have had liquid water on its surface at some point, increasing hopes for detecting life on other rocky planets.
Researchers at UCL have detected water vapor in the atmosphere of an extrasolar planet, HD 189733b. The discovery was made using NASA's Spitzer telescope and confirms that water might be more common than previously thought outside our Solar System.
Recent findings indicate a trend of increasing water content in the atmospheres of planets, from Jupiter (depleted) to Uranus and Neptune (water-rich). Computer models provide insights into planetary atmospheric chemistry, predicting the composition of Earth-like planets in other solar systems.
Researchers are studying various biosignatures to infer the composition of extrasolar planet atmospheres. They explore theories about what other worlds might be like, including different types of pigments for photosynthesis. One key clue is disequilibrium, where simultaneous presence of contradictory substances could indicate life.
Astronomers have discovered a young star with an elliptical ring that is likely caused by the presence of an undiscovered Neptune-sized planet. The ring is offset by 1.4 billion miles, more than 15 times the distance from Earth to the Sun.
Astronomers have discovered a massive transiting planet, TrES-3, with a 31-hour year, orbiting its parent star about 1,500 light-years away. The planet is twice the mass of Jupiter and one of the planets with the shortest known periods.
Researchers have found a massive exoplanet, XO-3b, which orbits its star in less than four days and is 13 times the mass of Jupiter. The planet's unusual characteristics, including its elliptical orbit and size, raise questions about its classification as a brown dwarf.
The California and Carnegie Planet Search team has reported 28 new exoplanets, increasing the total number of known exoplanets to 236. The new discoveries include seven confirmed brown dwarfs, which are failed stars that can be more massive than Jupiter-sized planets.
The University of Central Florida professor has made a groundbreaking discovery that the hottest known extrasolar planet, HD 149026b, is approaching temperatures of 3,700 degrees. This unprecedented finding indicates that the planet's surface must be incredibly black to absorb all the starlight it receives.
Researchers have developed a method to achieve pressures up to a billion atmospheres, recreating conditions expected in the cores of supergiant planets. This breakthrough allows for the study of extreme chemistry and material properties, shedding light on the composition of Earth's mantle and rocky core.
Researchers used Earth-based light data to identify dominant photosynthesis colors for extrasolar planets, narrowing the range of expected colors. This new approach will guide future space telescope designs to study habitable planets and detect alien life.
Scientists have obtained a spectrum of a planet orbiting another star, revealing the presence of silicate dust in its atmosphere. The discovery was made using NASA's Spitzer Space Telescope and represents a significant advance in extrasolar planetary science.
The study measures infrared light from three gas giant planets, detecting no temperature differences between their day and night sides. Temperatures appear to be uniform, around 925 degrees Celsius, due to strong winds that mix the atmosphere planetwide.
Researchers found that gas giants either form within the first 10 million years of a sun-like star's life or not at all. The study suggests that gas giant planets must form early in a star's history, offering insights into planet formation.
The Corot space mission is scheduled to launch on December 27, 2006, and will detect planets orbiting around other stars. The mission will also probe the secrets of stellar interiors, potentially discovering rocky worlds similar to Earth.
The film showcases various phenomena like hurricanes, satellite data collection, and ocean temperature changes. It also features special presentations about Earth's moon and Mars, offering an immersive experience of space exploration.
A team of astronomers has measured the temperature variation across the surface of a giant gas planet, Upsilon Andromeda b, for the first time. The study reveals that the planet's hot side reaches temperatures of 2,550 degrees Fahrenheit, while its dark side is frigid.
UCF, UCLA astronomers have made the first direct observation of distinct day and night temperatures on a planet orbiting another star. The team used NASA's Spitzer Space Telescope to measure infrared light emitted by the planet upsilon Andromedae b at five points around its orbit.
Astronomers confirm two exoplanets using ESO's Very Large Telescope and Hubble Space Telescope data. The discoveries provide strong evidence for at least 6 billion Jupiter-sized planets in the Milky Way, including five new ultra-short-period planet types.
Astronomers used VISIR instrument to map infrared disc around young, massive star HD 97048, finding it at least 12 times larger than Neptune's orbit. The disc is flared and contains a large amount of gas, potentially hosting planetary embryos.
Two new planets have been discovered by astronomers, both extremely close to their stars and estimated to be around 3,272 degrees Fahrenheit. The discovery is made possible by the transit method, which detects slight dimming of starlight as planets pass in front of their stars.
A recent study led by the University of Colorado at Boulder and Pennsylvania State University found that over one-third of giant planet systems could have Earth-like planets in habitable zones. These planets, formed through the migration of gas giants, may host oceans several miles deep and potentially support life.
The IAU defined a planet as a celestial body in orbit around the Sun with sufficient mass to assume hydrostatic equilibrium. The new definition includes our solar system's eight recognized planets and a distinct class of dwarf planets, including Pluto.
The IAU draft definition of a planet, which includes eight classical planets, three new 'plutons,' and Ceres, has been reached after two years of work. The definition states that a planet must be in orbit around a star and have sufficient mass to assume a hydrostatic equilibrium shape.
Researchers have found a nearby star system that could potentially host an Earth-like planet with the right conditions. The modelled system is expected to have a habitable zone where terrestrial planets can form, similar to our own solar system.
A University of Colorado study suggests using a gigantic, daisy-shaped space shield to block out light from parent stars and allow telescopes to image distant Earth-like planets. The concept enables astronomers to identify planetary features and detect biomarkers like methane and oxygen.
Astronomers propose that super-Earths can form around red dwarf stars via ultraviolet stripping, a process previously thought to only create gas giant planets. The new theory suggests that the mass of the central star determines whether a planet forms as a gas giant or a super-Earth.
New Jersey Institute of Technology physicists have used Earthshine observations to study changes in the earth's climate, with a focus on cloud cover and global warming. The research also has implications for the search for life on other planets, as evidenced by the detection of oxygen, water, and ozone in the Earth's spectrum.
Three tiny companions orbiting HD 69830 have been discovered by astronomers using the ESO's HARPS instrument. The newly found planets have minimum masses between 10 and 18 times the mass of Earth, with one located in the habitable zone.
A new model for the capture of planetary satellites involving a three-body gravitational encounter between a binary and a planet suggests that Triton was originally part of a binary pair orbiting the Sun. This mechanism introduces a new pathway for satellite capture by planets, which may be relevant to other objects in the solar system.
Margaret Turnbull has shortlisted five stars for radio signal detection and five for direct imaging of Earth-like planets. Her criteria include age, metallicity, and residency on the main sequence, favoring Sun-like stars with stable orbits.
Scientists simulated the cores of giant planets and exoplanets to understand how they formed and evolved. They found that extreme temperatures and pressures lead to the formation of metallic crystals, affecting a planet's magnetic field and surface activity.
Astronomers discovered dusty disks around two massive stars, suggesting that planets might form and survive in hostile environments. The discovery expands the range of known conditions for complex dust grain formation and potentially indicates that these stars are forming planets.
Astronomers discover an Earth-like planet with a solid core, orbiting a red dwarf star five times less massive than the sun. The discovery, made using microlensing technique, reveals thousands of potentially habitable planets in distant parts of the galaxy.
Astronomers have detected a rocky, icy planet about five-and-a-half times the mass of Earth, located over 20,000 light years away. The discovery was made possible by gravitational microlensing, which may lead to finding smaller planets in habitable zones around stars.
Astronomers have found a small planet with a mass about five times that of Earth, orbiting a small star near the center of the galaxy. The discovery suggests there are many other small planets in habitable zones, where temperatures are moderate enough for liquid water to appear on their surfaces.
Astronomers have discovered the first and only icy exoplanet that matches theoretical predictions for Solar System formation. OGLE-2005-BLG-390Lb orbits a small red star at an extremely close distance, with a surface temperature of -220°C, and is likely to resemble Pluto more than rocky planets like Earth.
The discovery of OGLE-2005-BLG-390Lb provides strong evidence that low-mass planets, potentially supporting life, are more common than Jupiter-like gas giants. Researchers hope the gravitational microlensing technique will reveal more habitable worlds in the Milky Way galaxy.
Researchers found that half of planetary collisions result in impactors bouncing off, leaving them significantly altered. These collisions can strip away atmospheres, crusts, and mantles, producing diverse asteroid populations.
Astronomers have discovered a planet orbiting a 600-million-year-old star using the Exoplanet Tracker, a faster and cheaper instrument. The new method allows for more efficient search of distant stars, potentially uncovering planets capable of supporting life.
Researchers create an optical vortex mask that eliminates starlight, allowing for direct observation of nearby planets. The device successfully images Saturn and its rings, paving the way for future exoplanet detection projects like the Terrestrial Planet Finder.
The $400,000 award will fund a starshade-shaped 'New Worlds Observer' that blocks parent star light and captures planet images. Scientists can map planetary systems, detect biomarkers and study features like oceans and continents.
Astronomers have found two young stars with 'gaps' in their disks that resemble the gaps between Jupiter and Uranus in our solar system. The discovery challenges existing theories of giant-planet formation and provides a unique window into how our own solar system came to be.
Astronomers discover a perturbed dusty belt around Fomalhaut, indicating the presence of a planet. The discovery provides valuable insights into debris disks and planetary formation.
Researchers argue that oxygen-rich atmospheres are essential for complex life to exist. However, since levels of oxygen won't have had time to develop sufficiently before a sun dies, life may not be able to evolve on planets orbiting short-lived suns.
The newly discovered planet, orbiting Gliese 876, is the smallest and first rocky terrestrial planet found around a normal star. Its surface temperature may be too hot for life as we know it due to its close proximity to the star.
Researchers explain violent origins of extrasolar planetary behavior, citing planet-planet scattering as key factor. The study's findings suggest that strong instabilities led to the formation of highly eccentric orbits in multiple systems.
Researchers have directly measured light from two confirmed extrasolar planets, HD 209458b and TrES-1, using NASA's Spitzer Space Telescope. The gas giants, similar to Jupiter, orbit close to their stars and radiate strongly in the infrared, with temperatures reaching up to 1,574 degrees Fahrenheit.
Astronomers have discovered the smallest extra-solar planet to date, orbiting a pulsar in a planetary system resembling our own inner solar system. The new planet is estimated to be one-fifth the mass of Pluto and has an orbit approximately six times larger than its third planet.
Researchers found a young, faint companion to a star, measuring its mass for the first time. The object is 93 times as massive as Jupiter, contradicting theoretical predictions.
Researchers found that strong stellar winds around young red dwarfs may be responsible for removing dust and debris disks. The discovery provides a potential explanation for the rare occurrence of debris disks among red dwarfs, but further observations are needed to confirm this hypothesis.
Researchers have discovered two candidate planets orbiting white dwarfs, which are the remnants of dead stars. The team used a combination of telescopes to detect these planets, which could provide clues about the solar system's formation and the presence of life in the galaxy.
Astronomers have discovered a candidate planetary companion to a relatively bright young brown dwarf star located 225 light-years away in the southern constellation Hydra. The object, detected by NASA's Hubble Space Telescope, is estimated to be about five times the mass of Jupiter and orbits its host at a 99% confidence level.
Astronomers use Hubble's Near Infrared Camera and Multi-Object Spectrometer to observe a faint companion object orbiting a relatively bright young brown dwarf star. The observations provide strong evidence for the existence of an extrasolar planet, which is estimated to be about five times the mass of Jupiter.
Researchers used VLT interferometer observations to study infrared spectra of dusty discs around three young stars, finding abundant crystalline silicate grains and processed dust near the star. This suggests that building blocks for Earth-like planets are present in circumstellar discs from the start.
The University of Colorado at Boulder has proposed a system to map planetary systems around other stars and detect exo-solar planets as small as Earth's moon. The New Worlds Imager concept uses a giant 'pinhole camera' in space to capture images of distant planets, including their oceans, continents, and atmospheres.
Astronomers have discovered a Jupiter-sized gas giant orbiting a star located 500 light-years from Earth. The newly found world circles its star every 3.03 days at a distance of only 4 million miles, much closer and faster than Mercury in our solar system.
Scientists have discovered a distant planet using the transit technique and spectroscopy, revealing key findings about TrES-1's atmosphere and orbit. The discovery marks the first extrasolar planet found by a dedicated survey of thousands of relatively bright stars.
Scientists used computer models to analyze the internal structures of Jupiter and Saturn, finding that heavy elements like iron are concentrated in Saturn's core. The research uses data from shock compression experiments and helps improve models of the planets' formation.
A team of astronomers using a novel camera will hunt for planets orbiting other stars, aiming to directly image faint gas-giants. The SDI camera has already made stunning images of Saturn's moon Titan and discovered an object near Jupiter in solar systems beyond our own.