118401 LINEAR

'118401 LINEAR' (provisional designation ) is an asteroid and main-belt comet ('176P/LINEAR', also known as 'LINEAR 52') which was discovered by the Lincoln Near-Earth Asteroid Research (LINEAR) 1-metre telescopes in Socorro, New Mexico on September 7, 1999. (118401) LINEAR was discovered to be cometary on November 26, 2005, by Henry H. Hsieh and David C. Jewitt as part of the Hawaii Trails project using the Gemini North 8-m telescope on Mauna Kea and was confirmed by the University of Hawaii's 2.2-m (88-in) telescope on December 24-27, 2005, and Gemini on December 29, 2005. Based on an absolute magnitude (H) of 15.04, (118401) LINEAR is assumed to be smaller than 6 km in diameter.
The main-belt comets are unique in that they have flat, circular, asteroid-like orbits, and not the elongated, often tilted orbits characteristic of all other comets. Since (118401) LINEAR can generate a coma (produced by vapour boiled off the comet), it must be an icy asteroid. When a typical comet approaches the Sun, its ice heats up and sublimates (changes directly from ice to gas), venting gas and dust into space, creating a tail and giving the object a fuzzy appearance. Far from the Sun, sublimation stops, and the remaining ice stays frozen until the comet's next pass close to the Sun. In contrast, objects in the asteroid belt have essentially circular orbits and are expected to be mostly baked dry of ice by their confinement to the inner solar system.
It is suggested that these main-belt asteroid-comets are evidence of a recent impact exposing an icy interior to solar radiation. A good question is, "How long will current main-belt comets keep generating a coma?" It is estimated short period comets remain active for about 10,000 years before having most of their ice sublimated away and going dormant.

Contents

References

References

★ New Class of Comets

★ Main-Belt Comets

★ orbital simulation from JPL (Java)

★ 118401 on November 13th, 2011

★ LINEAR home page

★ Seiichi Yoshida's comet list