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- Gould_Belt abstract "The Gould Belt is a partial ring of stars in the Milky Way galaxy, about 3000 light years across, tilted toward the galactic plane by about 16 to 20 degrees. It contains many O- and B-type stars, and may represent the local spiral arm to which the Sun belongs—currently the Sun is about 325 light years from the arm's center. The belt is thought to be from 30 to 50 million years old, and of unknown origin. It is named for Benjamin Gould, who identified it in 1879.The belt contains bright stars in many constellations including (in order going more or less eastward) Cepheus, Lacerta, Perseus, Orion, Canis Major, Puppis, Vela, Carina, Crux (the Southern Cross), Centaurus, Lupus, and Scorpius (including the Scorpius-Centaurus Association). The Milky Way also passes through most of these constellations, but a bit southeast of Lupus.A theory proposed around 2009 suggests that the Gould Belt formed about 30 million years ago when a blob of dark matter collided with the molecular cloud in our region. There is also evidence for similar Gould belts in other galaxies.".
- Gould_Belt thumbnail Infrared_Image_of_Dark_Cloud_in_Aquila.jpg?width=300.
- Gould_Belt wikiPageExternalLink gould.html.
- Gould_Belt wikiPageExternalLink index.html.
- Gould_Belt wikiPageExternalLink Perrot.pdf.
- Gould_Belt wikiPageID "6010685".
- Gould_Belt wikiPageRevisionID "602134794".
- Gould_Belt hasPhotoCollection Gould_Belt.
- Gould_Belt subject Category:Astronomical_objects_discovered_in_1879.
- Gould_Belt subject Category:Milky_Way_Galaxy.
- Gould_Belt subject Category:Objects_within_10_kly_of_Earth.
- Gould_Belt subject Category:Open_clusters.
- Gould_Belt subject Category:Orion–Cygnus_Arm.
- Gould_Belt type Abstraction100002137.
- Gould_Belt type Agglomeration107959269.
- Gould_Belt type Bunch107959943.
- Gould_Belt type Collection107951464.
- Gould_Belt type Group100031264.
- Gould_Belt type OpenClusters.
- Gould_Belt comment "The Gould Belt is a partial ring of stars in the Milky Way galaxy, about 3000 light years across, tilted toward the galactic plane by about 16 to 20 degrees. It contains many O- and B-type stars, and may represent the local spiral arm to which the Sun belongs—currently the Sun is about 325 light years from the arm's center. The belt is thought to be from 30 to 50 million years old, and of unknown origin.".
- Gould_Belt label "Ceinture de Gould".
- Gould_Belt label "Cintura di Gould".
- Gould_Belt label "Cinturão de Gould".
- Gould_Belt label "Cinturón de Gould".
- Gould_Belt label "Gould Belt".
- Gould_Belt label "Gouldscher Gürtel".
- Gould_Belt label "Pas Goulda".
- Gould_Belt label "Пояс Гулда".
- Gould_Belt label "グールド・ベルト".
- Gould_Belt label "古爾德帶".
- Gould_Belt sameAs Gouldscher_Gürtel.
- Gould_Belt sameAs Cinturón_de_Gould.
- Gould_Belt sameAs Ceinture_de_Gould.
- Gould_Belt sameAs Sabuk_Gould.
- Gould_Belt sameAs Cintura_di_Gould.
- Gould_Belt sameAs グールド・ベルト.
- Gould_Belt sameAs 굴드_대.
- Gould_Belt sameAs Pas_Goulda.
- Gould_Belt sameAs Cinturão_de_Gould.
- Gould_Belt sameAs m.0fkg52.
- Gould_Belt sameAs Q24469.
- Gould_Belt sameAs Q24469.
- Gould_Belt sameAs Gould_Belt.
- Gould_Belt wasDerivedFrom Gould_Belt?oldid=602134794.
- Gould_Belt depiction Infrared_Image_of_Dark_Cloud_in_Aquila.jpg.
- Gould_Belt isPrimaryTopicOf Gould_Belt.
