Explanation: The Crab Nebula resulted from a star that exploded - a supernova. The outer layers of the star were thrown violently into space, while the inner core collapsed to form a neutron star. This neutron star is visible to us today as a pulsar - a rotating star at the center of the nebula that emits visible flashes of light. The Crab Pulsar flashes about 30 times every second. Although the stellar explosion that caused the Crab Nebula was seen over 900 years ago, the nebula itself still expands and shines. How the nebula obtains the energy needed to shine was a mystery eventually solved by noting that this energy could be released by the slowing of the pulsar's rotation.

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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: M 1 - Crab Nebula - ostatok Sverhnovoi - pul'sar v Krabe Publikacii so slovami: M 1 - Crab Nebula - ostatok Sverhnovoi - pul'sar v Krabe
Sm. takzhe: Ostatok sverhnovoi Kassiopeya A Bol'shoi i malen'kii ostatki sverhnovyh Ostatok sverhnovoi tumannost' Rusalka Ostatok sverhnovoi CTA 1 Krabovidnaya tumannost' ot vidimogo sveta do rentgenovskih luchei Volokna ostatka sverhnovoi v Parusah Neobychnaya tumannost' Pa 30 Vse publikacii na tu zhe temu >>