Explanation: Why is the sky near Antares and Rho Ophiuchi so colorful? The colors result from a mixture of objects and processes. Fine dust illuminated from the front by starlight produces blue reflection nebulae. Gaseous clouds whose atoms are excited by ultraviolet starlight produce reddish emission nebulae. Backlit dust clouds block starlight and so appear dark. Antares, a red supergiant and one of the brighter stars in the night sky, lights up the yellow-red clouds on the upper left. Rho Ophiuchi lies at the center of the blue nebula on the right. The distant globular cluster M4 is visible just below Antares, and to the left of the red cloud engulfing Sigma Scorpii. These star clouds are even more colorful than humans can see, emitting light across the electromagnetic spectrum.

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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: Antares - otrazhatel'nye tumannosti - emissionnaya tumannost' - krasnyi sverhgigant Publikacii so slovami: Antares - otrazhatel'nye tumannosti - emissionnaya tumannost' - krasnyi sverhgigant
Sm. takzhe: NGC 6188: drakony v Zhertvennike Ou4: tumannost' Gigantskii Kal'mar RCW 85 Raznocvetnye oblaka i zvezdy okolo ρ Zmeenosca Sh2-132: tumannost' Lev M78 ot kosmicheskogo teleskopa "Evklid" IC 1795: tumannost' Ryb'ya golova Vse publikacii na tu zhe temu >>