Explanation: These wisps of gas are all that remain visible of a Milky Way star. Many thousands of years ago that star exploded in a supernova leaving the Veil Nebula, pictured above. At the time, the expanding cloud was likely as bright as a crescent Moon toward the constellation of Cygnus, visible for weeks to people living at the dawn of recorded history. The remaining supernova remnant lies about 1400 light-years away and covers over five times the size of the full Moon. The bright wisp on the right is known as the Witch's Broom Nebula and can be seen with a small telescope. The Veil Nebula is also known as the Cygnus Loop.

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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: Veil Nebula - tumannost' Vual' - ostatok Sverhnovoi Publikacii so slovami: Veil Nebula - tumannost' Vual' - ostatok Sverhnovoi
Sm. takzhe: Ostatok sverhnovoi tumannost' Rusalka NGC 6995: tumannost' Letuchaya Mysh' Ostatok sverhnovoi CTA 1 Volokna ostatka sverhnovoi v Parusah Neobychnaya tumannost' Pa 30 Ozvuchennyi ostatok sverhnovoi tumannost' Meduza Ostatok sverhnovoi Simeiz 147 Vse publikacii na tu zhe temu >>