Explanation: Rippling dust and gas lanes give the Flaming Star Nebula its name. The red and purple colors of the nebula are present in different regions and are created by different processes. The bright star AE Aurigae, visible toward the image right, is so hot it is blue, emitting light so energetic it knocks electrons away from surrounding gas. When a proton recaptures an electron, red light is frequently emitted. The purple region's color is a mix of this red light and blue light emitted by AE Aurigae but reflected to us by surrounding dust. The two regions are referred to as emission nebula and reflection nebula, respectively. Pictured above, the Flaming Star Nebula, officially known as IC 405, lies about 1500 light years distant, spans about 5 light years, and is visible with a small telescope toward the constellation of Auriga.

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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: Flame nebula - Pylevaya tumannost' Publikacii so slovami: Flame nebula - Pylevaya tumannost'
Sm. takzhe: IC 348 i Barnard 3 Temnaya tumannost' Lindsa LDN 1251 Zvezdnaya pyl' v Persee Konskaya Golova i Plamya Neobychnaya globula v IC 1396 Zvezdnaya pyl' i hvosty komety Volokno v Edinoroge Vse publikacii na tu zhe temu >>