Researchers at Ohio State University found that carbon-rich planets could form with a core and mantle, but these cores would be very carbon-rich and mantles dominated by diamond. This means no geothermal energy, plate tectonics, or magnetic field on such planets.
A Caltech-led team of astronomers has discovered 18 new planets orbiting massive stars, with masses similar to Jupiter's. The findings provide valuable insights into planetary formation and support the theory that planets grow from seed particles accumulating gas and dust in a disk surrounding a newborn star.
Researchers propose that Jupiter may have 'jumped' out of its orbit to avoid disturbing the inner solar system. The 'jumping-Jupiter' theory suggests one planet was ejected from the solar system, leaving four giant planets behind.
A new theory suggests that high-speed collisions between planets and asteroids near supermassive black holes create microscopic dust clouds. This process blocks harmful radiation, creating a more hospitable environment for life in the galaxy's central region.
A team of astronomers has discovered three new planets and a mystery object orbiting giant, dying stars. The research provides insights into the evolution of planetary systems around these stars and how metal content influences their behavior.
Scientists have discovered thousands of Earth-oceans' worth of water within the planet-forming disk of TW Hydrae. This finding suggests that comets could deliver vast amounts of water to new planets through impacts. The detection was made using the Heterodyne Instrument for the Far-Infrared on the Hershel Space Observatory.
Astronomers have captured a new image of a star's disk, revealing spiral-arm-like structures that could indicate the presence of hidden planets. The Subaru Telescope's advanced imaging capabilities have revealed these dynamic features for the first time.
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.
The MESSENGER spacecraft has shown that Mercury's surface material composition differs significantly from other terrestrial planets, with higher abundances of sulfur and potassium. The planet's surface also features a unique magnetic field and extensive volcanic plains covering over 6% of its surface.
Astronomers at Yale University have discovered the first two potential exoplanets found by Planet Hunters users analyzing real scientific data from NASA's Kepler mission. The candidate planets orbit their host stars with periods ranging from 10 to 50 days and radii that range in size from two-and-a-half to eight times Earth's radius.
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.
Astronomers at Caltech have discovered that the dwarf planet 2007 OR10, or Snow White, is an icy world with about half its surface covered in water ice. The findings suggest that the red-tinged dwarf planet may be covered in a thin layer of methane, remnants of an atmosphere slowly being lost into space.
The Mid-Infrared Instrument (MIRI) has completed 2,000 individual tests at cryogenic temperatures, a milestone for the James Webb Space Telescope mission. Scientists will use MIRI to study young planets around distant stars and explore their habitability.
The Genesis mission analysis shows differences in oxygen and nitrogen isotopes between the sun and rocky inner planets, including Earth. These findings suggest that the solar system's formation was more complex than previously thought.
A University of Arizona planetary scientist has determined Neptune's rotation with high accuracy by tracking atmospheric features in its atmosphere. The discovery improves upon previous measurements and provides a better understanding of the planet's fundamental properties.
Researchers have found a method to measure a star's true age using its spin. Astronomer Soren Meibom presented his findings in a press conference, nearly doubling the age covered by previous studies of younger clusters. The technique involves measuring stellar rotation rates for stars in clusters with known ages.
Kepler's first four months of data reveal evidence for over 1,200 planetary candidates, with 408 residing in systems containing two or more planets. These multi-planet systems are characterized by flat orbits, tilted less than 1 degree, and lack Jupiter-sized gas giants.
A recent study using data collected between 2006 and 2007 found evidence for 10 free-floating planets roughly the mass of Jupiter, suggesting they are common. The discovery supports the 'ejection' scenario where planets are kicked out from their solar systems due to close gravitational encounters with other planets or stars.
Bennett's team found 10 free-floating planets roughly the mass of Jupiter, suggesting planetary systems often become unstable, ejecting planets from their orbits. The discovery confirms that free-floating planets exist and are quite common, estimated to be twice as many as stars.
Astronomers at UC Berkeley are using the Green Bank radio telescope to search for signals from advanced civilizations on 86 Earth-like planets identified by Kepler. The team aims to detect signals that could be indicative of life, scanning a range of frequencies including the water hole, a canonical place to look for intentional signals.
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.
Scientists suggest that bombardments of micro-meteorites on Earth and Mars four billion years ago led to catastrophic cooling effects, making it hard for early life to thrive. The influx of sulphur dioxide into the atmospheres of both planets could have plunged them into an Arctic winter, lasting millions of years.
A new paper suggests that potentially habitable planets orbiting white dwarfs could be much easier to find than other exoplanets. The study proposes a survey of the 20,000 closest white dwarfs, which could be detected using a 1-meter ground telescope.
Cardiff University astronomers propose that young stars' long naps could lead to the birth of smaller stars and planets. The researchers developed advanced computer models to simulate young star behavior, finding that disc fragmentation is possible in nature.
The European Space Agency has approved a £400 million mission to study extra-solar planets, led by UCL, to look for signs of life in nearby star systems. The Exoplanet Characterisation Observatory (EChO) will use a 1.2 meter telescope to analyze the atmospheres of habitable planets and search for biomarkers.
Two new observations reveal detailed structures in protoplanetary disks of two young stars, including a large gap similar to our solar system's. The images suggest the presence of one or more massive planets sweeping up material from the disk, potentially forming an entire planetary system.
A NASA team led by University of Florida astronomers has discovered six new planets in a distant solar system resembling our own. The planets, orbiting Kepler-11, are rocky or ice-combined and have densities lower than water but higher than Earth.
The Kepler-11 system features five inner planets with masses between 2.3 and 13.5 times that of Earth, orbiting within 50 days, and a sixth planet with an orbital period of 118 days. The planets' densities suggest they may be mostly water or hydrogen-helium gases, defying expectations for small hot planets.
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.
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.
Astronomers have discovered a fourth giant planet in the HR8799 system, which is approximately seven times the mass of Jupiter. The system, consisting of four giant planets and two asteroid belts, is young compared to our solar system and may be on the verge of falling apart due to gravitational interactions.
Saturn's southern hemisphere emits more energy than its northern one, with variations seen in the planet's seasons and years. The Cassini CIRS instrument reveals Saturn is not losing power evenly, providing a new understanding of the planet's internal heat source.
According to a University of California, Berkeley study, nearly one in four sun-like stars could have Earth-size planets. The researchers found increasing numbers of smaller planets, down to super-Earths, about three times the mass of Earth.
A new way to weigh planets has been developed using radio signals from small spinning stars called pulsars, providing an independent check on previous results. The measurements of planet masses made this new way could feed into data needed for future space missions.
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.
New supercomputer simulations show what the solar system might look like to alien astronomers searching for planets. The models also provide a glimpse of how this view might have changed as our planetary system matured.
Researchers have found potassium in the atmosphere of a giant planet, HD 80606 b, using narrow-band transit spectrophotometry. The discovery supports previous computer models and demonstrates the value of this observational technique for characterizing planets that might support life.
The discovery of two planets, Kepler 9b and 9c, confirms the first planetary system with more than one planet transiting the same star. The planets, both Saturn-sized gas giants, exhibit orbital resonance and gravitational interaction.
A team of astronomers from the University of Florida has discovered two Saturn-sized planets and a possible third planet with an Earth-like size orbiting a distant star. The discovery was made using a new method of confirming planets called transit timing variation, which allows for more efficient confirmation of planetary systems.
UCF physicists analyze space dust using far IR spectroscopy to identify minerals and provide clues about solar system formation and life emergence. The findings will be published in the Monthly Notices of the Royal Astronomical Society journal.
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 New York Center for Astrobiology will expand its research with a new NASA grant, searching for the building blocks of life beyond Earth. Researchers study the chemical and physical conditions on Earth that gave birth to life and apply this information to search for similar conditions elsewhere in our solar system.
Computer modeling reveals that planets in habitable zones can fluctuate between life-supporting conditions and inhospitable temperatures due to giant neighbor's gravitational pull. This can cause drastic changes in a planet's orbit, potentially altering its geological properties over long timescales.
Scientists found 7,000 times less methane and plenty of carbon monoxide on GJ 436b, challenging standard chemistry theories about planetary atmospheres. The discovery suggests that scientists should be more flexible in their theories about similar planets.
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.
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.
The 2009 AAAS Newcomb Cleveland Prize was awarded to Christian Marois and colleagues for their direct imaging of multiple planets orbiting HR 8799, a distant star. The discovery, made using the Keck and Gemini North telescopes, reveals a system resembling our solar system's outer portion.
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...
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.
A new simulation by researchers at the American Museum of Natural History and University of Cambridge shows that regions of outward and inward migration in a protoplanetary disk can safely trap planets on orbits. This helps explain how Earth formed without falling into the Sun.
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.
CoRoT-7 b is a rocky planet circling a star 480 light years from Earth, with temperatures above 4,000 degrees F on its surface and potentially hosting multiple volcanoes due to its close orbit. Its extreme volcanic activity makes it unlikely to harbor 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.
Researchers found two brown dwarf-sized masses around an ordinary star, which is extremely rare. The discovery suggests that planets may assemble around stars more quickly and efficiently than thought possible.
Researchers have discovered two new planetary systems with low-mass 'super-Earths' orbiting nearby sun-like stars. The planets are smaller than previously discovered worlds and may be habitable.
An international team of astronomers has discovered six low-mass planets, including two super-Earths, around two nearby Sun-like stars. The discovery indicates that low-mass planets are common and potentially habitable worlds may be found within a few years.
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.
Astronomers have discovered that Sun-like stars with planetary systems tend to have lower levels of lithium than those without planets. The study, which analyzed 500 stars, found that planet-bearing stars had less than 1% of the lithium present in other similar stars.