Explanation: Comets become fountains of gas and dust as they get near the Sun. Solar heat vaporizes the outer layers of these spectacular orbiting icebergs, exposing caverns of pressurized gas that erupt into jets. The above digitally enhanced image of Comet Hale-Bopp was taken on January 29^th and highlights several of these dust jets. Here, background stars appear as faint raised streaks. Comet Hale-Bopp is currently brighter than most stars, and is visible in the morning sky. Comet Hale-Bopp will continue to brighten and develop an extended tail until 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: Comet Hale-Bopp - kometa Heila-Boppa - dzhet Publikacii so slovami: Comet Hale-Bopp - kometa Heila-Boppa - dzhet
Sm. takzhe: Porfirion: samyi dlinnyi dzhet ot chernoi dyry Galaktika, dzhet i znamenitaya chernaya dyra Akkreciruyushaya chernaya dyra s dzhetom HH 211: dzhety ot formiruyusheisya zvezdy Zvezdy, pyl', stolby i strui v tumannosti Pelikan Kometa Heila-Boppa: bol'shaya kometa 1997 goda Dzhet ot molodoi zvezdy MHO 2147 Vse publikacii na tu zhe temu >>