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When is a comet not a comet?

Astronomers using the Hubble Space Telescope have observed a unique asteroid with six comet-like tails, challenging current understanding of asteroids and comets. The asteroid's rotation rate may have caused its surface to fly apart, ejecting dust into space.

SourceESA/Hubble Information Centre·JournalThe Astrophysical Journal Letters·DateNov 7, 2013

Team solves one of the moon's mysteries

A Purdue University-led team has mapped the location and development of mass concentrations, or mascons, on the lunar surface, resolving a decades-long mystery. The findings provide valuable insights into the moon's origin and evolution and will aid in navigating future lunar missions.

SourcePurdue University·JournalScience·DateMay 30, 2013

NASA's Hubble Space Telescope finds dead stars 'polluted with planet debris'

Researchers have found evidence of building blocks for Earth-sized planets in the atmospheres of two burned-out stars called white dwarfs. The silicon and low levels of carbon in these dead stars suggest that asteroid-like debris is falling onto them, potentially creating rocky planet assembly around stars.

SourceNASA/Goddard Space Flight Center·JournalMonthly Notices of the Royal Astronomical Society·DateMay 9, 2013

NASA sees leaping lunar dust

Researchers found a new class of dust motion on the moon, where charged particles swarm like bees around partially shaded regions. This phenomenon creates oscillations over 1-10 meter-sized shaded regions, with dust bouncing back and forth between sunlit areas.

SourceNASA/Goddard Space Flight Center·JournalAdvances in Space Research·DateMar 18, 2013

Asteroid searchers take the high ground

The University of Calgary has launched a satellite to track near-Earth asteroids, enabling researchers to study these rare and difficult-to-detect objects. The NEOSSat satellite will enable scientists to take hundreds of sensitive images daily to search for moving dots of light that represent asteroids.

Asteroid belt found around Vega

Researchers have found an asteroid belt surrounding Vega, a star similar to the Sun, and believe multiple planets are orbiting it. The discovery was made using Infrared Space Telescopes, which detected infrared light emitted by warm and cold dust in discrete regions around the stars.

Mass extinction study provides lessons for modern world

Researchers found that pre-Cretaceous ecosystem changes and environmental factors led to more fragile communities in late Cretaceous North America. The study's findings suggest that human-made changes to modern ecosystems could worsen their ability to withstand disturbances, emphasizing the importance of understanding ecological function.

SourceUniversity of Chicago·JournalProceedings of the National Academy of Sciences·DateOct 29, 2012

Asteroid's troughs suggest stunted planet

Researchers found that asteroid Vesta's extensive system of troughs is likely the result of faults formed by a large collision. The troughs' unique characteristics, such as flat floors and distinct walls, suggest a fault moving apart, rather than simple cracking on the surface.

SourceAmerican Geophysical Union·JournalGeophysical Research Letters·DateSep 26, 2012

Magnetic moon

A team of researchers from Harvard and MIT suggests that massive asteroid collision is responsible for the Moon's magnetic anomalies. The anomaly is found around the rim of a 2,400-kilometer-diameter crater known as South Pole-Aitken.

SourceHarvard University·JournalScience·DateMar 8, 2012

Jupiter's 'Trojans' on an atomic scale

Researchers successfully stabilized electron orbits using an electromagnetic field, mimicking Jupiter's gravitational influence on asteroids. The experiment verifies calculations made at Vienna University of Technology and holds promise for future studies on the quantum-world of tiny objects.

SourceVienna University of Technology·JournalPhysical Review Letters·DateJan 25, 2012

The Lutetia asteroid – a prehistoric relic

Researchers found that the Lutetia asteroid is a dense, intact relic dating back to the solar system's formation. The asteroid's density was calculated using a mathematical method developed by Professor Mikko Kaasalainen, revealing a large and metallic core surrounded by a more porous outer layer.

SourceAcademy of Finland·JournalScience·DateOct 28, 2011