Explanation: Light-years across, this suggestive shape known as the Seahorse Nebula appears in silhouette against a rich, luminous background of stars. Seen toward the royal northern constellation of Cepheus, the dusty, obscuring clouds are part of a Milky Way molecular cloud some 1,200 light-years distant. It is also listed as Barnard 150 (B150), one of 182 dark markings of the sky cataloged in the early 20th century by astronomer E. E. Barnard. Packs of low mass stars are forming within from collapsing cores only visible at long infrared wavelengths. Still, colorful stars in Cepheus add to the pretty, galactic skyscape.

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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: dust - molecular cloud - pyl' - Molekulyarnye oblaka Publikacii so slovami: dust - molecular cloud - pyl' - Molekulyarnye oblaka
Sm. takzhe: Ruka pomoshi v Kassiopee Sem' Sester v pyli Temnyi Morskoi konek v Cefee IC 5146: tumannost' Kokon NGC 7023: tumannost' Iris Tumannost' "Temnaya shtuchka" Temnaya tumannost' Lindsa LDN 1251 Vse publikacii na tu zhe temu >>