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VREME

Vreme po Sloveniji ob 12 uri
CE
14°
NM
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MB
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KP
23°
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13°
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15°
NM
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HUBBLOVE NOVICE:

New Hubble Observations of Supernova 1987A Trace Shock Wave

02. 09. 2010

An international team of astronomers using the Hubble Space Telescope reports a significant...


First Use of Cosmic Lens to Probe Dark Energy

19. 08. 2010

An international team of astronomers using NASA's Hubble Space Telescope has devised a new method...


An "Island Universe" in the Coma Cluster

10. 08. 2010

A long-exposure Hubble Space Telescope image shows a majestic face-on spiral galaxy located deep...


02. 02. 2010 00:00

Suspected Asteroid Collision Leaves Odd X-Pattern of Trailing Debris

 

Something awfully curious is happening 100 million miles from Earth in the asteroid belt. There's a newly discovered object that superficially...


February 2, 2010: Something awfully curious is happening 100 million miles from Earth in the asteroid belt. There's a newly discovered object that superficially looks like a comet but lives among the asteroids. The distinction? Comets swoop along elliptical orbits close in to the Sun and grow long gaseous and dusty tails, as ices near the surface turn into vapor and release dust. But asteroids are mostly in circular orbits in the asteroid belt and are not normally expected to be "volatile."

The mystery object was discovered on January 6, 2010, by the Lincoln Near-Earth Asteroid Research (LINEAR) sky survey. The object appears so unusual in ground-based telescopic images that discretionary time on NASA's Hubble Space Telescope was used to take a close-up look. The observations show a bizarre X-pattern of filamentary structures near the point-like nucleus of the object and trailing streamers of dust. This complex structure suggests the object is not a comet but instead the product of a head-on collision between two asteroids traveling five times faster than a rifle bullet. Astronomers have long thought that the asteroid belt is being ground down through collisions, but such a smashup has never before been seen.

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