Explanation: One day our Sun may look like this. The Helix Nebula is the closest example of a planetary nebula created at the end of the life of a Sun-like star. The outer gasses of the star expelled into space appear from our vantage point as if we are looking down a helix. The remnant central stellar core, destined to become a white dwarf star, glows in light so energetic it causes the previously expelled gas to fluoresce. The Helix Nebula, given a technical designation of NGC 7293, lies 450 light-years away towards the constellation of Aquarius and spans 1.5 light-years. The above image was taken with the Canada-France-Hawaii Telescope (CFHT) located atop a dormant volcano in Hawaii, USA. A close-up of the inner edge of the Helix Nebula shows unusual gas knots of unknown origin.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: nebula - planetary nebula - Helix Nebula - CFHT Telescope - Tumannost' Ulitka Publikacii so slovami: nebula - planetary nebula - Helix Nebula - CFHT Telescope - Tumannost' Ulitka
Sm. takzhe: Tumannost' Meduza NGC 7293: tumannost' Ulitka Dzhons-Emberson-1 Raznocvetnye oblaka i zvezdy okolo ρ Zmeenosca HFG1 i Eibell 6: planetarnye tumannosti Tumannosti: ot Chaiki do Kalifornii NGC 2440: kokon novogo belogo karlika Vse publikacii na tu zhe temu >>