Explanation: The center of the Lagoon Nebula is a whirlwind of spectacular star formation. Visible on the lower left, at least two long funnel-shaped clouds, each roughly half a light-year long, have been formed by extreme stellar winds and intense energetic starlight. The tremendously bright nearby star, Hershel 36, lights the area. Vast walls of dust hide and redden other hot young stars. As energy from these stars pours into the cool dust and gas, large temperature differences in adjoining regions can be created generating shearing winds which may cause the funnels. This picture, spanning about 5 light years, was taken in 1995 by the orbiting Hubble Space Telescope. The Lagoon Nebula, also known as M8, lies about 5000 light years distant toward the constellation of Sagittarius.

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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: M 8 - Lagoon Nebula - Tumannost' Laguna Publikacii so slovami: M 8 - Lagoon Nebula - Tumannost' Laguna
Sm. takzhe: Triplet v Strel'ce Glubokaya Laguna V centre tumannosti Laguna Tumannost' Laguna bez zvezd Ozhivlennyi centr tumannosti Laguna Yuzhnyi utes v Lagune Centr tumannosti Laguna v infrakrasnom svete Vse publikacii na tu zhe temu >>