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Orion Nebula

   Also found in: Wikipedia, Hutchinson 0.01 sec.
Orion Nebula, bright diffuse nebula nebula (nĕb`ylə) [Lat.
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 in the constellation Orion; also known as the Great Nebula of Orion and cataloged as M42 or NGC 1976. It is located near the middle of the "sword" hanging from Orion's "belt" of stars. Its central bright region is about 1° in diameter and it has a total extension of 3°. It is about 1,000 light-years distant and as many as 60 light-years in diameter. The nebula is an enormous cloud of gas surrounding a cluster of very hot young stars. To the naked eye the nebula appears to be a faint star but becomes a vague patch of light when viewed through binoculars. The bright region is divided into two sections, the northeast portion being cataloged separately as M43 or NGC 1982. The Orion Nebula is the nearest major site to earth of massive star formation.

Orion Nebula

Bright nebula, faintly visible to the unaided eye in the sword of the hunter's figure in the constellation Orion. About 1,500 light-years from Earth, it contains hundreds of very hot young stars clustered about a group of four massive stars known as the Trapezium. Radiation primarily from these four stars excites the nebula to glow. Discovered in the early 17th century, it was the first nebula to be photographed (1880).


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To investigate, Luisa Rebull of the California Institute of Technology in Pasadena and her colleagues used the infrared Spitzer Space Telescope to study about 500 young stars in a densely packed stellar nursery, the Orion nebula.
The image is described as a stunning photograph of the famous Great Orion Nebula that shows the star birth cloud in unprecedented detail.
A good 7 X 35 pair of binoculars will show lots of details of the Moon, star dusters like the Pleiades, the Orion Nebula or the four moons of Jupiter," he said.
 
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