Articles tagged with Protoplanets
A new study estimates that the asteroid that formed the Moon's Imbrium Basin was likely a protoplanet-sized object, two times larger in diameter and 10 times more massive than previous estimates. The research also sheds light on the geological features surrounding the basin, which help explain some of its puzzling characteristics.
Researchers found two gaps in the gas disk that overlap with dust gaps, suggesting infant planets carve out the gaps. The team estimates a planet mass 0.8 times Jupiter's at the inner gap, but the outer gap's origin remains unclear.
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 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.
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.
Researchers suggest that chondrules may have formed from high-pressure collisions between planetesimals, which would explain their composition and origin. This theory resolves a long-standing puzzle in cosmochemistry and provides a potential solution to the mystery of how these glassy spherules were embedded within meteorites.
Scientists find that impacting small asteroids delivered dark, carbonaceous material to the protoplanet Vesta. The material, found in craters and meteorites, suggests a link between giant impact basins and the delivery of essential building blocks for organic molecules.
Scientists found that carbon-rich asteroids have been splattering dark material on Vesta's surface over billions of years, creating a youthful appearance. The protoplanet's bright outer layer remains pristine, with tiny metallic particles absent, indicating minimal weathering.
A study published in Nature found that a cloud of dust circling a young star disappeared within three years, contradicting the commonly accepted timescale for dust removal. This sudden disappearance suggests that planet formation may be much faster or more efficient than previously thought.
A new doctoral dissertation published in Nature sheds light on the dynamics of the earth and crust formation before 3 billion years ago, revealing a significant shift in the Earth's dynamics. This new understanding has significant implications for future climate change.
Dr. William R. Ward has made fundamental contributions to understanding how planets and satellites form and dynamically evolve, including the giant impact theory of lunar formation and Mars' polar axis oscillations
A team of astronomers investigated six young brown dwarfs and found that dust particles in their circumstellar discs stuck together, forming larger clumps of olivine. This material is also found in comets and normal stars, suggesting a similar growth process in planet formation
Researchers have found a young planet that is smaller than expected and orbits its parent star at the same distance as our own Neptune. The discovery was made using NASA's Spitzer Space Telescope and challenges current understanding of planetary formation, leading to a re-examination of existing theories.
Astronomers used Hubble to search for faint Kuiper Belt objects, finding only three small objects in a 15-day period. The discovery suggests that smaller planetesimals may have been shattered into dust by colliding with each other, affecting the number of comets near Earth.
Astronomers using the Hubble Space Telescope have discovered a large crater on asteroid Vesta with an estimated diameter of 285 miles and 8 miles deep. The crater's impact debris is believed to be a source of special types of meteorites, including those found in Hawaii.