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Media Information
Collection:
NASA Astronomy Picture of the Day Collection
Collection
NASA Astronomy Picture of the Day Collection
Collection
Title:
NGC 5882: A Small Planetary Nebula
Title
NGC 5882: A Small Planetary Nebula
Title
Explanation:
Will most stars one day look like this? Pictured above is the planetary nebula [
http://antwrp.gsfc.
] NGC 5882, captured [
http://scivax.stsci
] by the Hubble Space Telescope [
http://antwrp.gsfc.
]. Although planetary nebulae [
http://zebu.uoregon
] can appear similar to planets like Uranus [
http://antwrp.gsfc.
] and Neptune [
http://antwrp.gsfc.
], they are actually gas [
http://antwrp.gsfc.
] clouds surrounding stars typically hundreds of light years away. Planetary nebula [
http://home.cc.uman
] form when a typical star [
http://antwrp.gsfc.
] completes fusion [
http://fusedweb.ppp
] in its core and ejects an outer envelope of gas - usually about 10 percent of the star's initial mass. This gas shell dims in about 50,000 years - short compared to the lifetimes of stars [
http://xalph.ast.ca
]. Therefore, although only about 1000 planetary nebula [
http://wonka.physic
] are known in our Galaxy [
http://antwrp.gsfc.
], it is thought that most stars go through this phase. Green light is emitted when oxygen [
http://web.cetlink.
] ions acquire electrons from the surrounding gas.
Explanation
Will most stars one day look like this? Pictured above is the planetary nebula [
http://antwrp.gsfc.
] NGC 5882, captured [
http://scivax.stsci
] by the Hubble Space Telescope [
http://antwrp.gsfc.
]. Although planetary nebulae [
http://zebu.uoregon
] can appear similar to planets like Uranus [
http://antwrp.gsfc.
] and Neptune [
http://antwrp.gsfc.
], they are actually gas [
http://antwrp.gsfc.
] clouds surrounding stars typically hundreds of light years away. Planetary nebula [
http://home.cc.uman
] form when a typical star [
http://antwrp.gsfc.
] completes fusion [
http://fusedweb.ppp
] in its core and ejects an outer envelope of gas - usually about 10 percent of the star's initial mass. This gas shell dims in about 50,000 years - short compared to the lifetimes of stars [
http://xalph.ast.ca
]. Therefore, although only about 1000 planetary nebula [
http://wonka.physic
] are known in our Galaxy [
http://antwrp.gsfc.
], it is thought that most stars go through this phase. Green light is emitted when oxygen [
http://web.cetlink.
] ions acquire electrons from the surrounding gas.
Explanation
Credit and Copyright:
H. Bond, HST, STSci [
http://www.stsci.ed
], NASA [
http://www.nasa.gov/
]
Credit_and_Copyright
H. Bond, HST, STSci [
http://www.stsci.ed
], NASA [
http://www.nasa.gov/
]
Credit and Copyright
facet_where:
Uranus
facet_where
Uranus
facet_where
facet_where:
Hamilton
facet_where
Hamilton
facet_where
facet_where:
Goddard Space Flight Center (GSFC)
facet_where
Goddard Space Flight Center (GSFC)
facet_where
facet_what:
Neptune
facet_what
Neptune
facet_what
facet_what:
Uranus
facet_what
Uranus
facet_what
facet_what:
nebula
facet_what
nebula
facet_what
facet_what:
planetary nebula
facet_what
planetary nebula
facet_what
facet_what:
Hubble Space Telescope (HST)
facet_what
Hubble Space Telescope (HST)
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-ap960828
UID
SPD-APOD-ap960828
UID
NGC 5882: A Small Planetary Nebula
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