Scientists discover the first Earth-size planet in the habitable zone of a different star, confirming that planets like Earth exist elsewhere. The newly discovered planet, Kepler-186f, is 10% larger than Earth and located comfortably in its star's habitable zone, where liquid water could potentially exist on its surface.
The study confirms the existence of an Earth-sized planet orbiting Kepler-186, a temperate region where water could exist in liquid form. The team employed speckle imaging and adaptive optics to rule out background stars and stellar companions, allowing for the detection of Kepler-186f.
Researchers at San Francisco State University have discovered a new rocky planet, Kepler-186f, which may have liquid water on its surface. The planet's size and distance from its star suggest it could have a rocky surface similar to Earth.
Researchers found that pivoting planets with wobbling axes of rotation might maintain favorable conditions for life despite being far from their stars. This expands the idea of a habitable planet and where they might be found, particularly in systems with multiple gas giants.
Researchers studied Saturn's northern polar region and confirmed the hexagon's stability and unchanged jet stream. They suggest it's a manifestation of a Rossby wave similar to those on Earth, with implications for understanding Saturn's atmosphere.
A new analysis of Mercury's surface suggests that the planet experienced extended periods of volcanic explosions in its history. The study, led by researchers at Brown University, used MESSENGER data to determine that the eruptions did not occur all at once but rather over an appreciable period of Mercury's history.
The APF facility consists of a 2.4-meter telescope and the Levy Spectrometer, which Vogt designed and optimized specifically for planet hunting. Repeated measurement of a star's spectrum enables astronomers to detect the tiny wobble induced in a star by the gravitational tug of an orbiting planet.
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.
Scientists used MESSENGER spacecraft images and topographic data to build a comprehensive map of tectonic features on Mercury's surface. The findings indicate the planet has contracted between 4.6 and 7 kilometers in radius over its lifetime.
Researchers have discovered that Mercury has contracted by as much as 4.4 miles due to cooling, exceeding previous estimates of ½ to 2 miles. This finding is consistent with thermal models and resolves a decades-old paradox in understanding the planet's history.
Researchers discovered a compact cloud of poisonous gas formed by ongoing collisions among a swarm of icy bodies, suggesting an unseen planet with Saturn-like mass. The study suggests that the comet swarm could be the remnant of a crash between two Mars-sized icy planets or frozen debris trapped by the gravity of the hypothetical planet.
Scientists have made the first detection of water in the atmosphere of a hot Jupiter, tau Boötis b, using a novel technique that expands on the radial velocity method. The study confirms the presence of water vapor and also reveals the planet's mass, which was previously difficult to determine.
A team of scientists at Penn State University has detected water vapor in the atmosphere of a hot-Jupiter exoplanet, tau Boötis b. This discovery could help researchers understand how many planets like Earth exist throughout the universe and provides new insights into the formation and evolution of exotic hot-Jupiter planets.
Giant hot flow anomalies can swallow Venus whole due to its magnetic field absence, posing a significant threat to the planet's surface. Observations from European Space Agency's Venus Express reveal frequent and large-scale space weather events at Venus.
Circumbinary planets are thought to have formed far from their binary star systems before migrating to their current location. Researchers used computer simulations to model the early stages of planet formation around Kepler-34(AB)b and found that the majority must have formed much further away.
Researchers found a new giant planet in the Pisces constellation using radial velocity technique, contradicting initial assumption that only single-star systems host planets. The discovery has significant implications for understanding how extrasolar planets are formed and could lead to further discoveries in multiple-star systems.
New measurements of mass reveal that planets smaller than Neptune have low density due to extensive gas coverage, while larger ones have higher density. This suggests these planets formed quickly after their star's birth, contrasting with Earth's late formation.
A newly discovered celestial object, ROXs 42Bb, located nine times the mass of Jupiter and 30 times further away from its star than Jupiter, defies easy categorization as a planet or brown dwarf. This finding blurs the distinction between planets and brown dwarfs, prompting researchers to re-examine formation theories.
The Gemini Planet Imager has successfully captured its first light images of exoplanets, allowing scientists to study their atmospheres and characteristics in unprecedented detail. The instrument's advanced technology enables it to detect planets that are millions of times fainter than their parent stars.
The Gemini Planet Imager has captured its first light images, revolutionizing the field of exoplanet detection and study. The instrument's advanced adaptive optics system allows for direct imaging of faint planets, including those 1 million to 10 million times fainter than their host stars.
The discovery of KOI-314c reveals a planet weighing as much as Earth but 60% larger in diameter, indicating a thick, gaseous atmosphere. The planet's mass was measured using transit timing variations (TTV), a young method for studying low-mass planets.
Astronomers have detected clear evidence of clouds in the atmosphere of GJ 1214b, a super-Earth exoplanet, using data from the Hubble Space Telescope. The findings suggest that high-altitude clouds blanket the planet, hiding information about its composition and behavior.
The discovery of HD 106906 b, a giant planet orbiting its star at 650 times the average Earth-Sun distance, has puzzled astronomers. The planet's unusual orbit and mass throw doubt on existing planet formation theories, leaving scientists searching for alternative explanations.
The Solar Wind Electron Analyzer (SWEA) will track how charged particles, such as planetary oxygen ions, escape the planet's atmosphere. By identifying electrons in the solar wind and Martian ionosphere, SWEA can determine where the boundary layer between the two regions is located.
Researchers created a timeline of planet and atmosphere formation by studying liquid basalt under extreme pressures and temperatures. They discovered molten magma once formed an ocean within the Earth's mantle.
Based on Kepler data, scientists found that one in five sun-like stars has an Earth-size planet in its habitable zone. The estimated number suggests that life-supporting planets may be more common than previously thought.
Kepler-78b is the first known Earth-sized planet with an Earth-like density, posing a challenge to theorists due to its extremely tight orbit. The planet's mass measurement confirms it as the poster child for a new class of small, hot planets.
Researchers at MIT have discovered an exoplanet named Kepler 78b that is approximately 1.2 times the size of Earth and has a mass about 1.7 times that of our planet. The planet's density is also similar to Earth's, suggesting it may be composed mainly of rock and iron.
A new study led by UA graduate student Johanna Teske reexamines the composition of a potentially diamond-rich exoplanet, finding it may contain less carbon than previously thought. The analysis, based on revised star observations, suggests that the 'diamond planet' could be more rocky than initially proposed.
Researchers estimate Earth's habitable lifetime to be between 1.75 and 3.25 billion years, after which temperatures will become too high to support liquid water. This timeline suggests that complex life like humans may only emerge within a fraction of the planet's total habitable time.
The discovery of GJ 504b challenges traditional planet-formation theories, suggesting alternative formation methods may be needed. The exoplanet orbits its star at nearly 9 times the distance of Jupiter from the sun.
The Neutral Gas and Ion Mass Spectrometer (NGIMS) instrument on the MAVEN spacecraft will collect data on charged gas particles in Mars' upper atmosphere, helping scientists understand how the planet lost its majority of atmosphere. The data will also be used to build models of the Martian atmosphere billions of years ago.
Research led by Aomawa Shields found that planets orbiting cool stars absorb near-infrared light, warming the planet. In contrast, hotter stars' visible light is reflected by ice, cooling the planet. This interaction affects planetary habitability and may prioritize planets around cooler stars for life detection.
A new study estimates that global sea levels will rise 2.3 meters over the next several thousand years for every degree Celsius the planet warms. The four major contributors to sea-level rise on a global scale are melting of glaciers, Greenland ice sheet, Antarctic ice sheet, and ocean expansion as it warms.
The NASA Hubble Space Telescope has confirmed the presence of a true blue planet, HD 189733b, by detecting changes in light color as it passes behind its star. The observations indicate a deep blue color due to a hazy atmosphere with high clouds containing silicate particles.
For the first time, Hubble has measured the visible color of an exoplanet, revealing HD 189733b to be a deep azure blue due to its hazy and turbulent atmosphere. The planet's atmosphere is scorching with temperatures over 1000 degrees Celsius and features glass rain.
Astronomers have analyzed eight 'hot Jupiter' exoplanets using the Hubble Space Telescope, revealing a diverse range of puzzling properties. The team found that winds and clouds play a crucial role in shaping the atmospheric composition of these exotic planets.
Scientists have concluded that the oldest visible terrains on Mercury date back to 4 billion to 4.1 billion years ago, with volcanic activity resurfacing the planet's surface during this time period. The findings suggest a global resurfacing event due to volcanism and may indicate that large projectiles enhanced the observed resurfacing.
Astronomer Diana Dragomir reveals the hidden identity of super-Earth HD 97658b, measuring its size and mass for the first time. The exoplanet's density suggests a thick atmosphere, but it orbits too close to its star to support liquid water oceans.
Researchers have found evidence of an exoplanet forming at a distance of about 80 astronomical units (AU) from its star, TW Hydrae. The discovery is surprising as planets typically form closer to the central star.
Astronomers have discovered a crescent-shaped structure, known as a dust trap, around a young solar system in the constellation Ophiuchus. The researchers speculate that this feature enables dust particles to cling together, setting the stage for the formation of larger objects.
A team led by University of Louisville doctoral student Karen Collins discovered KELT-6b, a hot Saturn-like planet with an orbit that transits its star every 7.8 days, in the constellation Coma Berenices near Leo.
Researchers using NASA's HiRISE camera have identified almost 250 fresh impact craters on Mars each year, providing a more accurate measure of surface processes on the Red Planet. The cratering rate is estimated at an average of one per area roughly the size of Texas, offering insights into climate change and the planet's activity.
New research published in Nature Geoscience reveals how Saturn keeps itself looking young and hot due to gas layers preventing heat from escaping. This unique layering effectively insulates the planet, preventing heat radiating out efficiently.
Researchers have identified five planets within the habitable zone of a Sun-like star, including two planets similar in size to Earth. The discovery was made using data from the Kepler spacecraft and validated by high statistical confidence.
Two new super-Earths and a Mars-sized planet have been found in the habitable zone of Kepler-62, a star similar to our Sun. These planets are thought to be solid and rocky or rocky with frozen water, making them potentially hospitable to life.
The MAVEN magnetometer will study the planet's magnetic field to infer how the atmosphere evolved, helping answer why Mars became a frozen desert. By measuring sections of the planet's magnetic field, scientists can create a bigger picture of the overall atmosphere and understand its interactions with solar wind.
A team of scientists has observed the most detailed spectrum yet of an extrasolar planet, revealing a cloudy atmosphere containing water vapor and carbon monoxide. The findings provide clues to the planet's formation and offer insights into how planets form in other solar systems.
A team of astronomers has made the most detailed examination yet of a Jupiter-like planet beyond our Solar System, discovering a cloudy atmosphere containing carbon monoxide and water vapour. The findings suggest that the system is like a scaled-up Solar System, with gas giants forming at great distances from their parent star
An international team led by Sascha Quanz has studied the disc of gas and dust around young star HD 100546, spotting a candidate protoplanet that could be a giant similar to Jupiter. The discovery provides an unique laboratory for studying the formation process of a new planetary system.
A new study suggests that future evidence for extraterrestrial life might come from dying stars, specifically from planets orbiting white dwarfs. Detectable oxygen in the atmosphere of these planets could indicate the presence of life, and a recent simulation indicates JWST can detect this with only a few hours of observation time.
Astronomers used Kepler spacecraft data to discover a planet smaller than Mercury, about the size of Earth's moon, in the Cygnus-Lyra region of the Milky Way. The planet, Kepler-37b, is likely a rocky world with no atmosphere or water.
Astronomers discovered a mysterious planet circling the nearby star Fomalhaut with an unusual elliptical orbit. The team hypothesizes that another undetected planet may have gravitationally ejected Fomalhaut B, sending it on a collision course with a vast dust ring.
Researchers using NASA's Kepler spacecraft have found that about 17% of stars have an Earth-sized planet in an orbit closer than Mercury. This means there are at least 17 billion possible Earth-like planets in the Milky Way, with 50% of stars having a planet of Earth-size or larger in a close orbit.
A six-year observation by ESA's Venus Express reveals significant changes in the planet's atmosphere, suggesting recent volcanic eruptions. The thick atmosphere contains over a million times more sulphur dioxide than Earth's, which is mostly generated by volcanic activity.
New research suggests that planets orbiting white or brown dwarfs are unlikely to support life due to the cooling and shrinking of their habitable zones. The study's findings indicate that such planets would have had to undergo a 'sterilization phase' in the past, making them dead for hosting life.
Astronomers have discovered that dwarf planet Makemake lacks a significant atmosphere, revealing new insights into its composition. The study used observations of Makemake passing in front of a star to determine its size, density, and albedo, with findings comparable to dirty snow.
Asteroid belts may play a key role in the evolution of complex life. According to a NASA study, only a tiny fraction of planetary systems seem to have giant planets in the right location to produce an asteroid belt of the appropriate size. This suggests that our solar system may be special.
A new analysis of Hubble observations suggests Fomalhaut b is a rare, uniquely massive planet shrouded by dust. The team found the planet remained at constant brightness, contradicting earlier interpretations of it as a transient dust cloud.
Astronomers detect the lightest exoplanet ever found around a Sun-like star, orbiting about six million kilometers away from the star. The newly discovered planet has a mass similar to Earth and orbits Alpha Centauri B every 3.2 days.