Astronomers discovered large discs of dust around two young red dwarf stars near our solar system, hinting at potential new planetary systems forming. The discovery challenges current theories on planet formation and suggests a longer lifespan for such discs.
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.
Scientists have discovered a Jupiter-like planet, 51 Eridani b, in a young star system that could help understand how planets formed around our sun. The exoplanet features the strongest methane signature ever detected and is roughly twice the mass of Jupiter.
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.
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.
A team of UCLA scientists discovers a Jupiter-like planet, 51 Eridani b, which orbits a nearby star at a distance similar to Saturn's orbit. The planet has the strongest concentration of methane ever detected on a planet outside the Milky Way and is roughly twice the mass of Jupiter.
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.
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 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 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.
Astronomers at SDSU announce the discovery of Kepler-453 b, the 10th known 'circumbinary' planet. The new planet orbits two stars and has a surprisingly tilted orbit, making transits visible only 9% of the time.
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.
A new study published in Nature Geoscience suggests that Earth's first crust was torn from the planet and lost to space due to asteroid bombardment, leading to the evolution of its plate tectonics, magnetic field and climate. This phenomenon, known as impact erosion, helps explain why Earth is habitable while Venus is not.
A new theory proposes that a planet's bulk composition, specifically the abundance of uranium, thorium, and potassium, dictates whether plate tectonics can occur. This affects the planet's internal heating, volcanism, and climate. The Earth's unique composition allows for current plate tectonics to operate.
A Brazilian-led team has discovered a planet with a mass similar to Jupiter's, orbiting a Sun-like star at almost the same distance. The planet's host, HIP 11915, is also similar in mass and age to our Sun, with a composition that hints at possible rocky planets.
A new NASA supercomputer simulation of the planet and debris disk around Beta Pictoris reveals that the planet's motion drives spiral waves throughout the disk, causing collisions among orbiting debris. The patterns in these collisions account for many observed features that previous research has struggled to explain.
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.
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 discovered a colossal cloud of hydrogen dispersing from the warm, Neptune-sized planet Gliese 436b. The enormous gaseous tail is about 50 times the size of its parent star and may offer clues on how hot super-Earths form around other stars.
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.
Scientists have discovered that Mercury's magnetic field is almost 4 billion years old, providing a new understanding of the planet's history. The discovery was made possible by data from NASA's MESSENGER spacecraft, which orbited Mercury between 2011 and 2015.
Scientists have discovered a magnetization signal emanating from an ancient region of Mercury's crust, indicating the presence of a dynamo-driven magnetic field 3.8 billion years ago. This finding suggests that Mercury's core dynamo has persisted for billions of years.
The MESSENGER spacecraft is using its altimeter instrument to help with navigation during close approaches to Mercury's surface. The team is using the altimeter's precise measurements of distance from the spacecraft to the surface to assess the accuracy of their orbit predictions.
A NASA study found that small solar eruptions, like a slow-moving CME, can cause significant atmospheric loss in planets without magnetic shields. This research has implications for understanding habitability and the potential effects of solar storms on other planets.
Researchers reveal 'juvenile' continental crust has been produced throughout Earth's history, contradicting the long-held theory that all continental crust was generated during the Archaean Eon. The study provides new understanding of the formation of the Earth's continental crust and its impact on the planet's life and climate.
New observations show that Jupiter's auroral glow sometimes flares up due to a process unrelated to the Sun. The giant planet's polar auroras are powered by a separate interaction between Jupiter and its moon Io, causing intense electric fields at Jupiter's poles.
Researchers from Queen Mary University of London and University of Hertfordshire re-evaluate data and find signal of GJ 581d to be real. The method used in the initial study was inadequate for detecting small planets, leading to a possible misidentification.
Astronomers have used NASA's Hubble Space Telescope to capture the most detailed edge-on picture yet of a large disk of gas and dust encircling Beta Pictoris. The disk is distorted by the gravitational pull of an embedded giant planet, allowing scientists to study the effects of planetary formation on young star systems.
Researchers have detected a mysterious high plume on Mars, extending horizontally about 500 km and reaching an exceptional altitude of 200-250 km above the planet's surface. The team used images from amateur astronomers and spacecraft to analyze the phenomenon, exploring possible scenarios such as cloud or auroral emission.
Researchers have discovered a distinct inner-inner core with different iron crystal alignment and behavior compared to the outer layer. This finding could reveal information about the planet's formation and evolution
Researchers use laser-driven compression to study extreme conditions inside planets, revealing properties of silica that determine planet formation and evolution. The findings suggest large rocky planets may have long-lived oceans at depth and could explain the existence of planets like Neptune and Uranus.
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.
Research suggests that super-Earths can maintain oceans for at least 10 billion years due to a planet-wide recycling process. This finding implies that older super-Earths are more suitable for searching for complex life.
A University of Texas at Arlington astrophysicist has created a new online tool called BinHab that can calculate the regions of binary systems favorable for life. The tool uses a comprehensive mathematical approach to consider both stellar radiation and gravitational influence, directly relevant to NASA's Kepler mission.
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.
A team of astronomers detected eight large storms on Uranus's northern hemisphere, including the brightest storm ever seen at 2.2 microns. The storms are thought to be caused by gases such as methane rising in the atmosphere and condensing into highly reflective clouds of methane ice.
A new study from the University of Washington and MIT reveals that global warming is not solely caused by carbon dioxide's 'blanket' effect, but also involves shortwave radiation. The research shows how CO2 initially traps heat, but as the planet warms, it absorbs more solar radiation, leading to continued warming.
Scientists at Woods Hole Oceanographic Institution discover evidence of water on Earth dating back to the planet's formation. The findings suggest that Earth formed as a wet planet with water on its surface.
The MAVEN spacecraft successfully navigated a close pass by comet C/2013 A1 Siding Spring, providing valuable insights into the Red Planet's upper atmosphere and interaction with the solar wind. The mission will continue to study Mars' atmosphere and its effects on the planet's geology.
Astronomers have discovered a Uranus-like planet 25,000 light-years away, which orbits one star in a binary system. The planet's composition remains unknown due to its immense distance from the star.
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 NASA's Hubble Space Telescope to create a detailed map of the atmosphere of WASP-43b, an extremely hot and gaseous planet. The findings reveal that the planet has extreme temperature fluctuations between day and night, with winds howling at supersonic speeds.
Astronomers have mapped the temperature and water vapor on WASP-43b, a hot exoplanet with turbulent conditions. The findings provide insights into atmospheric dynamics and how giant planets like Jupiter are formed.
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.
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.
Astronomers have detected water vapour and other molecules on HAT-P-11b, the smallest exoplanet known to harbor these compounds. The discovery is significant for its potential implications on understanding the atmospheres of smaller planets.
New observations from NASA's Venus Express mission show giant holes in Venus' ionosphere, suggesting a more complex magnetic environment. The findings provide additional clues to understanding Venus' atmosphere and its interactions with the solar wind.
Researchers developed parameters to distinguish Venus-like planets from Earth-like ones based on distance from stars. The study identified 43 potential Venus-like planets with characteristics like size and orbit, but atmospheric conditions remain unknown.
Astronomers have pinpointed the 'Venus Zone' as a critical area around stars where planets are likely to exhibit unlivable conditions. This definition will help Kepler researchers distinguish between habitable and uninhabitable planets, enabling better understanding of Earth's atmospheric evolution.
Researchers at Florida State University analyzed an ancient Martian meteorite to determine the Red Planet's climate history. The team found evidence of a dramatic climate shift dating back 4.4 billion years, suggesting Mars has been cold and dry for at least 1.7 billion years.
Researchers found that an outer companion planet's gravitational pull can generate tidal heating, extending the habitable zone and potentially allowing older Earth-sized planets to host life. The study suggests that discovering such planets may lead to finding inner companion worlds, increasing their chance at hosting life.
Researchers found water vapour abundance to be between ten and a thousand times less than predicted models, raising questions about the chemical processes involved in planet formation. The discovery has implications for searching for life on exoplanets capable of supporting it.
Astronomers using NASA's Hubble Space Telescope found three 'hot Jupiters' with significantly lower than expected water vapor levels, challenging current theories on planet formation and migration. The discovery may require instruments to be designed with higher sensitivity for future space telescopes searching for water in potentially...
Researchers at University of East Anglia have developed a new model that takes into account the impact of oceans on climate, finding they play a vital role in moderating temperatures and habitability. This breakthrough helps answer whether other planets could sustain alien life.
Researchers have redefined the asteroid Vesta's internal structure based on Dawn data and simulations, questioning previous models of rocky planet formation. The study found that Vesta's crust is 3 times thicker than expected and lacks olivine, a mineral common in planetary mantles.
Computer modeling by NASA scientists shows that friction could be key to survival for distant Earth-sized planets in dangerous orbits. Some planets may move into safer orbits faster than expected due to tidal stress-induced friction.
A study suggests that Planet Mercury's unusual metal-rich composition is a result of early hit-and-run collisions with larger planets. This process could have stripped away Mercury's mantle without intense shock, leaving behind a mostly-iron body.
Astronomers have discovered an Earth-like planet in a binary star system, expanding the search for habitable planets. The planet orbits one of the stars at almost exactly the same distance from which Earth orbits the sun, but is much colder due to its host star's dimmer light.