Astronomy Picture of the Day
    


The Dust and Ion Tails of Comet Hale Bopp
<< Yesterday 26.12.2000 Tomorrow >>
The Dust and Ion Tails of Comet Hale Bopp
Credit & Copyright: John Gleason (Celestial Images)
Explanation: In 1977, Comet Hale-Bopp's intrinsic brightness exceeded any comet since 1811. Since it peaked on the other side of the Earth's orbit, however, the comet appeared only brighter than any comet in two decades. Visible above are the two tails shed by Comet Hale-Bopp. The blue ion tail is composed of ionized gas molecules, of which carbon monoxide particularly glows blue when reacquiring electrons. This tail is created by the particles from the fast solar wind interacting with gas from the comet's head. The blue ion tail points directly away from the Sun. The white dust tail is created by bits of grit that have come off the comet's nucleus and are being pushed away by the pressure of light from the Sun. This tail points nearly away from the Sun. The above photograph was taken in March 1997.

January
February
March
April
May
June
July
August
September
October
November
December
 < December 2000  >
Mo Tu We Th Fr Sa Su




123
45678910
11121314151617
18192021222324
25262728293031
Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Based on Astronomy Picture Of the Day

Publications with keywords: comet - dust - tail - Comet Hale-Bopp
Publications with words: comet - dust - tail - Comet Hale-Bopp
See also:
All publications on this topic >>