Researchers at CU-Boulder are developing a precise laser ruler to measure tiny changes in infrared light caused by the gravitational wobble of small, cool stars as they interact with rocky planets. The technique will allow them to detect Earth-like planets around M stars, which are much more common than larger stars.
New research suggests that dirty stars with a high abundance of elements like iron and oxygen are more likely to host planets. The study's findings support the idea that the composition of a star reflects its disk, leading to an increased number of exoplanets around such stars.
A team of international scientists captured a snapshot of Earth's chemical signature using a lunar eclipse, providing crucial information for identifying potentially habitable planets. The observation, published in Nature magazine, offers a unique opportunity to study planetary atmospheres and compositions.
Astronomers at the Science and Technology Facilities Council's William Herschel Telescope have confirmed an effective way to search the atmospheres of planets for signs of life. This method uses transmission spectra, which can reveal vital information about a planet's atmosphere, providing clues about potential biological processes.
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 use new calculations to redefine habitable zones, considering tidal forces that can impact planet's climate and life. The revised definition limits potential habitable environments, focusing searches on overlapping zones.
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.
A NASA/University team developed a method to indicate the presence of oceans on extrasolar Earth-like worlds by analyzing how Earth's light changes as it rotates. The technique relies on observing blue color changes caused by oceans, which appear bluer than continents.
Researchers at Harvard-Smithsonian Center for Astrophysics have created an 'astro-comb' to help detect lighter planets around distant stars. The technique sharpens spectroscopy, enabling more accurate pinpointing of planet locations and opening possibilities for detecting more Earth-like planets.
Astronomers have found evidence of planet destruction caused by a star's tides, with some planets falling into their parent stars. The research uses computer models and observations to show that the tidal forces can misshape the star's surface, leading to the planet's demise.
Kepler will observe a broad region of the summer-time sky using a photometer to measure the brightness of stars. The mission aims to determine the number of Earth-like planets in the galaxy by watching for tiny flickers in starlight that could indicate a planet passing in front.
A team of CU-Boulder students and professionals will operate the Kepler spacecraft from launch, monitoring onboard systems and uploading commands twice a week. The mission aims to identify small, rocky planets in habitable zones, fueling growing excitement among space scientists.
Researchers have found hundreds of new planets beyond our solar system, with evidence for all three classes of planets detected in extra-solar systems. Carnegie Institution scientists predict that many planets will be habitable, potentially inhabited by life.
Scientists will discuss new techniques to understand planetary formation, habitability, and potential for life. Experts will share insights on the probability of finding Earth-like planets within a few dozen light years of the sun.
New research demonstrates how laser-based techniques can create micron-sized light pathways in three dimensions, enabling the detection of faint light from extrasolar planets and galaxies. This technology has the potential to improve the sensitivity and precision of future telescopes, such as the planned European ELT.
The European team discovered the smallest transiting extrasolar planet, CoRoT-Exo-7b, orbiting a star slightly smaller than the Sun. The planet's radius is about twice that of Earth and orbits its host star in just 20 hours.
Scientists at Lawrence Livermore National Laboratory and the University of Illinois have determined the temperature at which helium becomes insoluble in dense metallic hydrogen. This finding has significant implications for models of the interior structure and evolution of Jovian planets, including Saturn and Jupiter.
Researchers built a novel device to study convection in rotational systems, providing new insights into how it controls planetary and stellar behavior. The findings show that fluid boundary layers control rotating convection systems, rather than Coriolis and buoyancy forces.
Two independent groups successfully detected the thermal emissions of exoplanets OGLE-TR-56b and TrES-3b using ground-based telescopes. The detections are significant because they will continue to study hot Jupiters beyond the capabilities of the soon-to-be-retired Spitzer telescope.
A new study found that gas giants like Jupiter must form extremely fast, in less than 5 million years, or they won't form at all. This rapid growth spurt is necessary because the material from which they formed probably disappeared within a few million years.
Researchers are exploring the possibility of life on giant, cold planets called Super-Earths that could harbor a liquid ocean beneath their icy surface. The team uses a novel approach involving gravitational microlensing to detect these potentially habitable worlds.
Researchers used a new technique to measure the precise size of WASP-10b, a planet thought to have an unusually large diameter. The team's use of the OPTIC camera resulted in a finding that the planet is one of the densest known, rather than bloated.
Astronomers have discovered carbon dioxide on a Jupiter-sized planet orbiting another star, HD 189733b. The detection is significant as it could be a sign of biological activity, and further studies will focus on characterizing the planet's atmosphere to determine its habitability.
Researchers discovered glycolaldehyde, a basic sugar molecule, towards a star-forming region where habitable planets may exist. The detection suggests that the production of this key ingredient for life could be common throughout the galaxy.
A team of astronomers discovered a new planet closely orbiting the giant star HD 102272, nearly six times the mass of Jupiter. The planet's location near the star raises questions about how aging stars influence nearby planets.
Gemini Observatory's groundbreaking discovery reveals two planets orbiting a young, massive star called HR 8799. The system consists of three planets, including the 'first family' member, which are still glowing from heat released as they contracted, and are about seven and ten times the mass of Jupiter.
A team of astronomers has discovered three planets in orbit around the young star HR 8799, using advanced computer processing techniques to separate them from the star's light. The planets are found to possess complex atmospheres with dusty clouds partially trapping and re-radiating escaping heat.
Researchers have captured the first-ever images of three giant planets orbiting the star HR 8799. The planets, each about ten times the mass of Jupiter, have complex atmospheres with dusty clouds that trap and re-radiate heat.
The new solar system orbits a dusty young star named HR8799, with three planets roughly 10 times the mass of Jupiter. The discovery allows scientists to study planets as individuals, providing insights into their atmospheres and composition.
Meteorites containing ancient magnetic records have provided new insights into the early history of planets. The study suggests that small bodies in the solar system were large enough to melt and form magnetic dynamos, overturning previous ideas about planet formation.
Research on the centre of planets provides deeper insight into controlled thermonuclear fusion and improves models of Jupiter and Saturn. The study reveals that extreme matter behaves like a charged liquid at smaller distances but acts more like a gas over larger lengths.
A new MIT study suggests that young, hot planets like Earth could stay hotter for millions of years, making them detectable by current telescopes. This extended molten surface would increase the brightness of the planet in infrared light, reducing the contrast with its star and allowing for easier detection.
Researchers used NASA's Thunderhead supercomputer to simulate dusty disks around sunlike stars, finding that planets as small as Mars can create detectable ring structures. The models provide a way to infer a planet's mass and orbital distance based on dust particle simulations.
Scientists use frequency comb to determine starlight color with high accuracy, allowing them to measure velocity changes of astronomical bodies with precision. This method could help search for Earth-like planets and test universe expansion acceleration.
The study reveals that the formation of planetary systems was full of violence and drama, but our solar system required conditions to be just right. The researchers ran over 100 simulations, showing that an average planetary system's origin was dramatic, with planets being flung into space or crowded together.
Researchers at UC Berkeley and University College London discovered that metallic helium is produced under extreme conditions found at the centers of Jupiter and Saturn, mixing with metal hydrogen to form a liquid metal alloy. This finding challenges previous theories about the energy source powering these planets.
A team of European astronomers has discovered a triple system of super-Earths around the star HD 40307 using the HARPS instrument. The planets have masses between 4.2 and 9.4 times that of Earth, and orbit the star with periods ranging from 4.3 to 20.4 days.
A team of astronomers led by David Bennett discovered a planet with a mass about three times that of Earth, orbiting a star with a mass 6% of the sun's, potentially hosting conditions suitable for life. The discovery was made using the gravitational microlensing method and confirms predictions made in 1996.
Scientists have developed a record-breaking ultrafast laser that can aid in the search for Earthlike planets. The new laser offers high speed, short pulses, and high average power, making it ideal for boosting the sensitivity of astronomical tools.
Astronomers are looking for Earth-like planets with liquid oceans in the habitable zone of their star. By monitoring the light curve of a distant planet as it spins on its axis, they can determine if the planet has water.
An international team of astronomers has found 10 new 'extra solar' planets using a robotic camera technique that will revolutionize scientific understanding of how planets form. The newly discovered planets have masses between half the size of Jupiter to eight times its size, including exotic worlds with extremely close orbits.
Researchers have found evidence of small, sandy particles orbiting a newborn solar system at a distance similar to the Earth's orbit around the sun. The discovery sheds light on how Earth-like planets may form and offers new opportunities for studying the chemical composition of these particles.
Researchers at the University of Rochester found that planets or low-mass stars orbiting dying stars create breathtaking objects in the sky. The study explores how these companions shape planetary nebulae through spiral waves and magnetic fields, producing striking shapes like the Dumbbell Nebula.
The Mars Express and Venus Express spacecraft reveal that the two planets' atmospheres are stripped away into space due to solar wind interactions. The similarity in magnetic field structure between the two planets suggests a shared ionosphere density at high altitudes.
NASA awards CU-Boulder $1 million to lead the study of a space observatory that will find Earth-like planets and detect biomarkers like methane, oxygen, and water. The project plans to launch a 4-meter telescope into an orbit roughly 1 million miles from Earth, with a giant starshade to block starlight.
Astronomers have discovered that many nearby sun-like stars may form rocky planets, with potential for life being more common than thought. The study suggests that at least 20 percent to 60 percent of stars similar to the sun are candidates for forming terrestrial worlds.
A new system of planets has been discovered with striking similarities to our Solar System, revealing giant planets that favour family groups over lone objects. The discovery uses a world-wide net of telescopes and challenges the single-life theory of gas-giant planets.
An international team of astronomers has discovered two planets resembling smaller versions of Jupiter and Saturn in a solar system nearly 5,000 light years away. The newly-discovered planets appear to be gaseous planets with masses similar to those of the giant planets in our own solar system.
Astronomers have discovered a solar system nearly 5,000 light years away with scaled-down versions of Jupiter and Saturn. The planets are similar in size to our own, suggesting that planetary systems like ours may be more common than previously thought.
Researchers have discovered a multi-planet system with two large planets similar to Jupiter and Saturn, suggesting that planetary systems like our own may be common in the Milky Way galaxy. This is the first discovery of its kind, using a new gravitational microlensing technique.
The Deep Impact spacecraft is using its flyby of Earth to calibrate its instruments for the EPOXI mission, which will study comet Hartley 2. The team made observations of the moon to test the spacecraft's pointing and commanding systems.
The EPOXI mission will use the Deep Impact spacecraft to search for Earth-sized planets around five stars and conduct an extended flyby of Comet Hartley 2, studying its surface and composition. This new mission aims to better understand how solar systems form and evolve.
Astronomers at the University of Illinois have discovered a stellar cradle where planets and moons are believed to form. Located 800 light-years away in the constellation Cepheus, the object is an enormous flow of shocked molecular hydrogen gas erupting from a young protostar's magnetic poles.
The discovery of a fifth planet around 55 Cancri is significant due to its habitable zone, where water could exist as a liquid. The planet's size and orbit suggest it may be rocky, with a potential for life.
Scientists have discovered a huge belt of warm dust swirling around the distant star, which is just slightly more massive than our sun. The conditions are suitable for forming rocky planets, and the material mix is reminiscent of lava flows on Earth.
Astronomers have discovered 'embryonic planets' forming in nearby star systems using new Hubble Space Telescope imagery. These small, Pluto-sized bodies are thought to be the first stage of planet formation and may hold the key to understanding how our own planet came to be.
A team of scientists from MIT, NASA, and Carnegie Institution created models for 14 different types of solid planets that might exist in our galaxy. The models predict a planet's diameter for a given composition and mass, revealing surprising similarities in how gravity compresses planets of varying materials.
TrES-4 is the largest known exoplanet, about 70% bigger than Jupiter but less massive, making it a planet of extremely low density. It orbits its host star in three and a half days and is very hot due to its close proximity.
The discovery of a planet orbiting a giant red star provides insight into the potential fate of our solar system as it evolves into a red-giant star. The planet, located 300 light years from Earth, circles its star every 360 days and offers astronomers a unique opportunity to study the effects of red-giant stars on planetary systems.
Astronomers used powerful telescopes to detect giant Jupiter-like planets in the outer regions of nearby solar systems, but found none beyond 5 astronomical units from their stars. The survey, which was conducted over three years, aimed to determine what the average planetary system looks like and whether ours is typical.