Media Information

 
 
 
Collection:
NASA Astronomy Picture of the Day Collection
Title:
At the Edge of the Crescent Nebula
Explanation:
The Crescent Nebula is a rapidly expanding shell of gas surrounding a dying star. In this recently released image [ http://oposite.stsc…] by the Hubble Space Telescope [ http://oposite.stsc…], a bright dynamic part of the nebula three light-years across is shown in representative color. The Crescent Nebula [ http://www.ne.jp/as…] began to form about 250,000 years ago as central Wolf-Rayet [ http://antwrp.gsfc.…] star WR 136 began to shed its outer envelope in a strong stellar wind [ http://www-istp.gsf…], expelling the equivalent of our Sun's mass every 10,000 years. This wind [ http://science.msfc…] has been impacting surrounding interstellar gas [ http://antwrp.gsfc.…], compacting it into a series of complex shells, and lighting it up. The Crescent Nebula [ http://www.astro.un…], also known as NGC 6888, lies about 4,700 light-years [ http://www.howstuff…] away in the constellation [ http://www.eagleque…] of Cygnus [ http://www.seds.org…] and can only be seen through a telescope. Star WR 136 [ http://adsabs.harva…] will probably undergo a supernova [ http://antwrp.gsfc.…] explosion sometime in the next million years.
Credit and Copyright:
Brian D. Moore [ mailto:brian.moore@a su.edu ] (ASU [ http://phy.asu.edu/]) et al., WFPC2, HST, NASA [ http://www.nasa.gov/]
keyword:
Wolf-Rayet
keyword:
NGC 6888
keyword:
Crescent Nebula
facet_where:
Goddard Space Flight Center (GSFC)
facet_where:
Marshall Space Flight Center (MSFC)
facet_what:
Sun
facet_what:
Cygnus
facet_what:
nebula
facet_what:
crescent
facet_what:
Hubble Space Telescope (HST)
original url:
UID:
SPD-APOD-ap000802

At the Edge of the Crescent Nebula