Articles tagged with Solar System Formation
A team led by Lucas Cieza has made the first resolved observations of a water snow line in a protoplanetary disc using ALMA's long baselines. The discovery pushes the water snow line out to a distance of around 40 au, significantly impacting our understanding of planetary formation models.
Astronomers may discover these 'diamond worlds' around rare carbon-enhanced metal-poor stars, which formed in the early universe. Carbon-based life is thought to be universal, supporting the possibility of life on these unusual planets.
The James Webb Space Telescope science instrument package was successfully installed into the telescope structure with precision engineering and teamwork. The team conducted rigorous training and testing before the critical mission operation, ensuring the instruments and mirrors are ready for launch.
Scientists at SwRI discovered two geologically young craters, one 16 million and the other between 75-420 million years old, in the Moon's darkest regions. The discovery was made possible by a new technique using the Lyman-Alpha Mapping Project instrument aboard the Lunar Reconnaissance Orbiter.
An international team of astronomers has detected icy comets and carbon monoxide gas around a nearby sun-like star using ALMA. The findings provide early insights into the properties of comet clouds in stellar systems just after their birth.
Researchers analyze the Kepler-223 star system, finding a unique orbital configuration similar to that of Jupiter, Saturn, and Uranus. The study suggests that the four planets may have migrated through a disk, getting stuck and maintaining their current orbits, which differs from the formation process of Earth's inner planets.
New research by astronomers at the Harvard-Smithsonian Center for Astrophysics examines scenarios for Planet Nine's formation and finds most have low probabilities. The simplest solution suggests the solar system created an extra gas giant, boosting Planet Nine into its wider orbit over time.
The James Webb Space Telescope's primary mirror is the largest yet sent into space, made of 18 beryllium segments coated with a thin layer of gold. The telescope will study the formation of solar systems capable of supporting life on planets similar to Earth, as well as the evolution of our own solar system.
Astronomers have captured unprecedented details of the TW Hydrae disk, which may host a super-Earth or an infant version of our home planet. The images show concentric dusty bright rings and dark gaps, including a tantalizing gap at Earth's distance from the star.
Scientists have found evidence of curium in a rare meteorite sample called 'Curious Marie', dating back to the solar system's formation. The discovery resolves a 35-year-old debate and helps reassess models of stellar evolution and element synthesis.
New Atacama Large Millimeter/submillimeter Array (ALMA) images provide detail on the binary star system HD 142527, revealing a broad ring of dust and ice. The system's formation is expected to yield insights into planetary systems around binary stars.
The James Webb Space Telescope will study planets, moons, comets and asteroids in our solar system to understand its formation and potential habitability. Scientists envision monitoring the water cycle on Mars, studying weather patterns on Saturn's moon Titan, and tracking comets to better comprehend our solar system's evolution.
The final primary mirror segment was installed on the telescope structure using a robotic arm, completing a decade-long design and manufacturing process. Once deployed, the 18 segments will form a single large 21.3-foot diameter mirror to study planetary atmospheres, star-forming regions, and the universe's beginnings.
A York University-led laser altimeter, OSIRIS-REx Laser Altimeter (OLA), will map the surface and create a 3D model of asteroid Bennu during a NASA mission. The instrument will help guide the spacecraft to a safe spot to grab a sample, providing Canadian scientists with their first direct access to a pristine asteroid sample.
Jason Dworkin, chief of NASA's Astrochemistry Laboratory, has made significant contributions to our understanding of the early solar system through his research on organic compounds in meteorites, comets, and asteroids. His work has identified amino acids and nucleobases that are precursors to essential biological molecules, shedding l...
A team from The Hebrew University of Jerusalem suggests that rare mergers of binary neutron stars are the origin of naturally occurring radioactive plutonium-244. This theory resolves the Galactic radioactive plutonium puzzle by explaining why only a small amount of plutonium has reached Earth in recent 100 million years.
Dr. William Bottke will present on a relatively tranquil time between two violent bombardment phases in the early solar system, exploring evidence from various sources including planet formation models and ancient samples.
The James Webb Space Telescope has received its first mirror installation, with 18 primary mirror segments scheduled to be installed by early next year. The mirrors are made of ultra-lightweight beryllium and must remain precisely aligned in space for successful science investigations.
Researchers from the University of Sydney and other institutions have directly observed a planet in formation for the first time. The planet, located 450 light years away, is surrounded by a vast disc of dust and gas, and its presence has been confirmed through images and spectral fingerprint analysis.
Comet Lovejoy released large amounts of ethyl alcohol and glycolaldehyde into space, adding to evidence that comets could be a source of complex organic molecules necessary for life. The discovery supports the idea that comets carried sophisticated chemistry to Earth during its early stages.
The Lucy mission aims to survey the diversity of Trojan asteroids, which are believed to be remnants from the formation of the outer gas giants. The spacecraft will use remote-sensing instruments to study geologic and physical properties of the asteroid targets.
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.
A Ph.D. student at the University of Houston is studying calcium-aluminum-rich inclusions from the Allende meteorite to understand when the solar system formed. By analyzing the age of these inclusions, he can gain insight into the timing and nature of early solar system processes.
Researchers reveal that Saturn's F ring and its shepherd satellites, Prometheus and Pandora, formed from the collision of small satellites with a dense core. This study sheds light on the formation process of satellite systems in our solar system and beyond.
The University of Texas at Arlington's Planetarium will debut the first active stereo 3-D show about NASA's SOFIA mission, exploring the study of Mars atmospheres and comets. The 3.5-minute film aims to inspire young scientists and engineers.
Dr. Martin Duncan's new model proposes that gas giants like Jupiter and Saturn formed through the accumulation of small 'pebbles', allowing cores to form rapidly enough to capture their atmosphere. The successful model predicts the formation of one to four gas giant planets, consistent with the observed outer solar system configuration.
Researchers suggest planetary pebbles, icy objects about a foot in diameter, were the building blocks for Jupiter and Saturn. This new model improves solar system formation models, producing the observed structure of the solar system with two gas giants, two ice giants, and a pristine Kuiper belt.
A study by Carnegie's Alan Boss and Sandra Keiser suggests that a shock wave from a supernova may have induced the spin of our Solar System, enabling the formation of a disk around our proto-Sun. This finding challenges previous theories and provides new insights into the earliest phases of planet formation.
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.
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.
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.
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.
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.
Researchers have discovered a young planetary system with a ring-like disk of debris surrounding a Sun-like star, sharing similarities with the formation of our own early solar system. The disk is roughly the same size as our solar system's Kuiper Belt and may contain dust and icy particles.
An international team of astronomers has identified a young planetary system, located 360 light years away, with a disc-shaped bright ring of dust around a star similar to the sun. The disc's brightness and composition are consistent with the Kuiper Belt in our solar system.
Dr. Bill Ward, a renowned planetary scientist, was elected to the National Academy of Sciences for his groundbreaking research on the origin and evolution of the Moon and other celestial bodies. His work has significantly contributed to our understanding of planetary science and the formation of our solar system.
A NASA-funded SwRI-led research team independently estimated the Moon's age as 4.47 billion years based on shock signatures found in stony meteorites originating from the Main Asteroid Belt. This study provides insights into the last stages of planet formation in the inner solar system.
Scientists discover complex organic molecules in a protoplanetary disk surrounding a young star, hinting at the universality of prebiotic chemistry. The presence of these molecules, particularly methyl cyanide, suggests that protoplanetary disks are efficient factories for forming complex organic compounds.
Astronomers have detected large amounts of complex organic molecules, including methyl cyanide, in the protoplanetary disc surrounding young star MWC 480. This discovery suggests that these molecules are common in the universe and may be delivered to environments nurturing life.
Researchers propose that a second generation of planets, including super-Earths, existed in the inner solar system before being destroyed by Jupiter's massive migration. This scenario helps explain why Earth and other terrestrial planets have relatively low masses compared to exoplanets orbiting other sun-like stars.
The study explains why our solar system has a gap between Mercury and the outer planets. Jupiter's inward migration destroyed any newly-formed super-Earths, leaving behind rocky inner planets like Earth with thinner atmospheres.
A research team at the University of Arizona has discovered sulfide chondrules in meteorites, providing evidence for a new type of environment in the early solar system. The discovery sheds light on the formation of elements essential for life, such as carbon and oxygen.
Researchers found that iron vaporizes at lower impact speeds than previously thought, leading to a shift in understanding of Earth's core formation process. This change affects estimates of the timing of Earth's core formation, with new information suggesting a more rapid process.
International team of astronomers observes multiple-star system forming in Perseus constellation, revealing how stars are separated during early stages of formation. The discovery advances understanding of conditions governing the type of star systems to develop.
The comet's coma composition changes in response to temperature and seasonal variations, suggesting a complex nucleus-nucleus relationship. This finding challenges the long-held assumption that comets are made mostly of water ice.
Research suggests asteroid material originated from impacts between embryo planets, resolving long-standing mystery of chondrule formation. Chondrules are abundant in meteorites and similar to spherules formed by impact on Earth and moon.
Scientists mapped magnetic fields in a primitive meteorite, tracing back to the earliest steps of the solar system's formation. The findings point to shock waves traveling through the cloud of dusty gas around the newborn Sun as a major factor.
A team of researchers has provided evidence that the early solar system's protoplanetary disk was shaped by an intense magnetic field, driving gas toward the sun at a rapid rate. The study analyzed a meteorite sample, extracting individual grains and measuring their magnetic orientations to determine the original magnetic field.
Researchers have discovered two young stars with analogues to our solar system's asteroid and Kuiper belts, surrounded by a large dust halo. These findings suggest a common model for planetary formation and evolution, providing insight into the early stages of star formation and planet creation.
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.
Jacob Bean, an assistant professor at UChicago, has received a 2014 Packard Fellowship to study exoplanets and their atmospheres. He aims to gain a deeper understanding of planetary formation, chemistry, and habitability.
A UCSB geochemist used lead and helium isotope measurements to analyze Samoan volcanoes, finding evidence of a primordial component within the deep interior. The study revealed distinct chemical configurations and mixing relationships among four endmembers, providing new insights into Earth's mantle plume structure.
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.
A new study has shown that the water found on Earth originated before the Sun formed, suggesting that many exoplanets may also have access to abundant water. This discovery has important implications for the potential for life elsewhere in the galaxy.
A team of scientists found that much of Earth's water originated as ices in interstellar space, predating the Sun's birth. This discovery has implications for the potential emergence of life elsewhere in the universe.
Researchers have dated the final addition of heavy elements like gold and platinum to the solar system 100 million years before the sun's birth. This discovery has shed light on the sun's prehistory, including the duration of an 'incubation' period that preceded its formation.
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.
Researchers Guillaume Avice and Bernard Marty found the Earth is approximately 60 million years older than previously thought. The team analyzed xenon gas sealed in quartz samples to refine dating techniques and estimate the Moon-forming impact timing, now believed to be around 40 million years after solar system formation.
Scientists discovered a relationship between the time of the Moon-forming event and material added to Earth, forming a 'clock' to date the Moon. The new method estimates the Moon's age to be 95 ±32 million years after the beginning of the solar system.