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Collection:
NASA Astronomy Picture of the Day Collection
Collection
NASA Astronomy Picture of the Day Collection
Collection
Title:
Reflections on NGC 6188
Title
Reflections on NGC 6188
Title
Explanation:
NGC 6188 is an interstellar carnival of young blue stars [
http://antwrp.gsfc.
], hot red gas [
http://antwrp.gsfc.
], and cool dark dust [
http://antwrp.gsfc.
]. Located 4000 light years away in the disk [
http://antwrp.gsfc.
] of our Galaxy, NGC 6188 [
http://www.aao.gov.
] is home to the Ara OB1 association [
http://adsbit.harva
], a group of bright young stars whose nucleus forms the open cluster NGC 6193 [
http://adsbit.harva
]. These stars are so bright that some of their blue light reflects off of interstellar dust [
http://antwrp.gsfc.
] forming the diffuse blue glow in the center of the above photograph [
http://www.aao.gov.
]. Open cluster [
http://www.seds.org
] NGC 6193 formed about three million years ago from the surrounding gas, and appears unusually rich in close binary stars. The red glow visible throughout the photograph arises from hydrogen [
http://www.chemical
] gas heated by the bright stars in Ara OB1. The dark dust [
http://www.pha.jhu.
] that blocks much of NGC 6188 [
http://www.geocitie
]'s light was likely formed in the outer atmospheres of cooler stars [
http://antwrp.gsfc.
] and in supernovae ejecta [
http://antwrp.gsfc.
].
Explanation
NGC 6188 is an interstellar carnival of young blue stars [
http://antwrp.gsfc.
], hot red gas [
http://antwrp.gsfc.
], and cool dark dust [
http://antwrp.gsfc.
]. Located 4000 light years away in the disk [
http://antwrp.gsfc.
] of our Galaxy, NGC 6188 [
http://www.aao.gov.
] is home to the Ara OB1 association [
http://adsbit.harva
], a group of bright young stars whose nucleus forms the open cluster NGC 6193 [
http://adsbit.harva
]. These stars are so bright that some of their blue light reflects off of interstellar dust [
http://antwrp.gsfc.
] forming the diffuse blue glow in the center of the above photograph [
http://www.aao.gov.
]. Open cluster [
http://www.seds.org
] NGC 6193 formed about three million years ago from the surrounding gas, and appears unusually rich in close binary stars. The red glow visible throughout the photograph arises from hydrogen [
http://www.chemical
] gas heated by the bright stars in Ara OB1. The dark dust [
http://www.pha.jhu.
] that blocks much of NGC 6188 [
http://www.geocitie
]'s light was likely formed in the outer atmospheres of cooler stars [
http://antwrp.gsfc.
] and in supernovae ejecta [
http://antwrp.gsfc.
].
Explanation
Credit and Copyright:
David Malin (AAO [
http://www.aao.gov.
]), AATB [
http://www.aao.gov.
]
Credit_and_Copyright
David Malin (AAO [
http://www.aao.gov.
]), AATB [
http://www.aao.gov.
]
Credit and Copyright
keyword:
emission nebula
keyword
emission nebula
keyword
keyword:
reflection nebula
keyword
reflection nebula
keyword
keyword:
absorption nebula
keyword
absorption nebula
keyword
facet_where:
Goddard Space Flight Center (GSFC)
facet_where
Goddard Space Flight Center (GSFC)
facet_where
facet_what:
Ara
facet_what
Ara
facet_what
facet_what:
New General Catalogue (NGC)
facet_what
New General Catalogue (NGC)
facet_what
original url:
http://antwrp.gsfc.
original_url
http://antwrp.gsfc.
original url
UID:
SPD-APOD-ap990825
UID
SPD-APOD-ap990825
UID
Reflections on NGC 6188
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