Astronomy Picture of the Day
    


Flame Nebula Close Up
<< Yesterday 25.11.2010 Tomorrow >>
Flame Nebula Close Up
Credit & Copyright: Adam Block, Mt. Lemmon SkyCenter, U. Arizona
Explanation: Of course, the Flame Nebula is not on fire. Also known as NGC 2024, the nebula's suggestive reddish color is due to the glow of hydrogen atoms at the edge of the giant Orion molecular cloud complex some 1,500 light-years away. The hydrogen atoms have been ionized, or stripped of their electrons, and glow as the atoms and electrons recombine. But what ionizes the hydrogen atoms? In this close-up view, the central dark lane of absorbing interstellar dust stands out in silhouette against the hydrogen glow and actually hides the true source of the Flame Nebula's energy from optical telescopes. Behind the dark lane lies a cluster of hot, young stars, seen at infrared wavelengths through the obscuring dust. A young, massive star in that cluster is the likely source of energetic ultraviolet radiation that ionizes the hydrogen gas in the Flame Nebula.

January
February
March
April
May
June
July
August
September
October
November
December
 < November 2010  >
Mo Tu We Th Fr Sa Su
1234567
891011121314
15161718192021
22232425262728
2930




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.

Based on Astronomy Picture Of the Day

Publications with keywords: Flame nebula
Publications with words: Flame nebula
See also:
All publications on this topic >>