Explanation: Glowing in the red light emitted by hydrogen atoms, the planetary nebula NGC 4361 is pictured above. The nebula itself is formed by the outer layers of gas shrugged off by the central star visible in the image. The star's nuclear fuel almost exhausted, it is cooling and shrinking - entering the white dwarf phase of its life. The curved tendrils of emission reaching out from the body of the nebula have a shape reminiscent of the arms of of a spiral galaxy.

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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: planetary nebula - Planetarnaya tumannost' - belyi karlik Publikacii so slovami: planetary nebula - Planetarnaya tumannost' - belyi karlik
Sm. takzhe: HFG1 i Eibell 6: planetarnye tumannosti NGC 2440: kokon novogo belogo karlika MyCn 18: planetarnaya tumannost' Pesochnye Chasy Tumannost' Kol'co ot teleskopa "Dzheims Vebb" NGC 1360: tumannost' Yaico drozda M2-9: kryl'ya tumannosti Babochka M57: tumannost' Kol'co Vse publikacii na tu zhe temu >>