Explanation: Comet Hale-Bopp has quite a tail to tell already. This remarkable comet was first discovered in 1995, even before Comet Hyakutake. Since then, this erupting snowball continues to fall into our inner Solar System and is starting to put on quite a show. Comets have been known throughout history to show tails that spread across the sky. In the above picture, the blue stream is the ion tail which consists of ions pushed away from the comet's head by the solar wind. The ion tail always points directly away from the Sun. Comet Hale-Bopp is now visible in the morning sky, moving a few degrees each day. Comet Hale-Bopp is expected to be at its best and brightest in late March and early April.

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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.

Publikacii s klyuchevymi slovami: tail - Comet Hale-Bopp - kometa Heila-Boppa - kometnye hvosty Publikacii so slovami: tail - Comet Hale-Bopp - kometa Heila-Boppa - kometnye hvosty
Sm. takzhe: Izmenyayushiisya ionnyi hvost komety Ponsa-Bruksa Ionnyi hvost komety Ponsa-Bruksa Hvosty komety ZTF Kometa Heila-Boppa: bol'shaya kometa 1997 goda Kometa Leonarda vilyaet hvostom Dlinnyi hvost komety Leonarda Kometa Heila-Boppa nad perevalom Val Parola Vse publikacii na tu zhe temu >>