Imaging Studies of Sodium Tails in Comets

Astronomy and Astrophysics – Astronomy

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Scientific paper

While the presence of sodium in comet tails has been known for decades, the recent application of imaging techniques to portray the Na component of comet Hale-Bopp added a new dimension to the study of sources and dynamics of cometary gases. In this paper, we report on preliminary results of a search for additional image sets showing sodium tails in comets. New observations made at the McDonald Observatory in January 1998 searched for Na components of two comets: Tempel-Tuttle (magnitude ~ 9.5) at a heliocentric distance of 1.1 AU (pre-perihelion) and geocentric distance of 0.4 AU, and Hartley-2 (magnitude ~ 8.5) at a heliocentric distance of 1.1 AU (post-perihelion) and a geocentric distance of 0.8 AU. In both cases, using the same techniques that detected Na in Hale-Bopp, we found no evidence for sodium above the detection threshold of 10 Rayleighs. Earlier observations of comet Hyakutake (magnitude ~ 1.5) at 0.9 AU from the sun (pre-perihelion), made from the site of the National Telescope Galileo (TNG) on La Palma in April 1996, revealed a well-formed sodium tail. The Hyakutake sodium tail had a peak brightness of ~ 100 Rayleighs near the coma, and a brightness of 20 Rayleighs at 2 million kilometers in the anti-sunward direction. Preliminary model studies suggest that the brightness pattern cannot be explained with a nucleus source alone; an extended sodium source in the tail region is indicated.

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