Explanation: Comet Hale-Bopp continues its slow trek across the night sky, and can now be seen superposed near the bright globular cluster M14. Will Comet Hale-Bopp become as bright in early 1997 as Comet Hyakutake did in early 1996? It is still too early to tell. Currently Hale-Bopp is curiously holding at about 5^th magnitude - just barely bright enough to see without binoculars from a dark location. Because of the size of coma, some speculate that the nucleus of Hale-Bopp is unusually large. The actual nucleus is obscured, however, and recent speculation includes that the nucleus is comparable in size to Comet Halley - about 10-15 km across.

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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 - Sharovoe skoplenie - koma - kometa Heila-Boppa Publikacii so slovami: Comet Hale-Bopp - Sharovoe skoplenie - koma - kometa Heila-Boppa
Sm. takzhe: Milliony zvezd v ω Centavra Sharovoe zvezdnoe skoplenie 47 Tukana Ogromnoe sharovoe skoplenie v Gerkulese M15: plotnoe sharovoe zvezdnoe skoplenie NGC 2419: mezhgalakticheskii strannik NGC 4372 i tumannost' Temnaya shtuchka NGC 1850: v Mlechnom Puti takih net Vse publikacii na tu zhe temu >>