This does not compute.Since NGC 4921 is a member of the Coma Cluster of Galaxies, refining its distance would also allow a better distance determination to one of the largest NGC 4921 has been informally dubbed anemic because of its low rate of star formation and low surface brightness.
APOD: Anemic Galaxy NGC 4921 at the Edge (2009 Feb 09)
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- Asternaut
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APOD: Anemic Galaxy NGC 4921 at the Edge (2009 Feb 09)
Is there something missing from the explanatory text?
Re: Anemic Galaxy NGC 4921 (2009 Feb 09)
Okay - not real scientific, more whimsical. BUT, did anyone else catch the space "snake" or "dragon" in this awesome shot? It's at XY:(325,1150) - zoom attached.
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Re: Anemic Galaxy NGC 4921 (2009 Feb 09)
Snake? A Hooded COBE, no doubt.
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Re: Anemic Galaxy NGC 4921 (2009 Feb 09)
That was exactly my thought, when reading the description. Hopefully TPTB will see it and fix it. For posterity, if not for clarity!Bill Melater wrote:Is there something missing from the explanatory text?
![Laughing :lol:](./images/smilies/icon_lol.gif)
Forget the box, just get outside.
Re: Anemic Galaxy NGC 4921 (2009 Feb 09)
I agree. It probably should read something like:Bill Melater wrote:Is there something missing from the explanatory text?
Since NGC 4921 is a member of the Coma Cluster of Galaxies, refining its distance would also allow a better distance determination to one of the largest galaxy clusters. NGC 4921 has been informally dubbed anemic because of its low rate of star formation and low surface brightness.
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Re: Anemic Galaxy NGC 4921 (2009 Feb 09)
http://apod.nasa.gov/apod/ap090209.html
<<Since NGC 4921 is a member of the *COMA* Cluster of Galaxies, refining its distance would also allow a better distance determination to one of the largest nearby clusters in the local universe. The magnificent spiral NGC 4921 has been informally dubbed anemic because of its low rate of star formation and low surface brightness.>>
. *COMA* (1978)
.......................................
Dr. Susan Wheeler: You did it. [Put people in irreversible COMAS]
.
Dr. George A. Harris (Richard Widmark): No decision is easy, Sue.
. It only looks that way when you're young.
. When you're older, everything is complicated.
. *There is no black and white, only GRAY*.
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<<Since NGC 4921 is a member of the *COMA* Cluster of Galaxies, refining its distance would also allow a better distance determination to one of the largest nearby clusters in the local universe. The magnificent spiral NGC 4921 has been informally dubbed anemic because of its low rate of star formation and low surface brightness.>>
-----------------------------<<In medicine, a *COMA* (from the Greek κῶμα koma, meaning deep sleep) is a profound state of unconsciousness. A COMAtose person cannot be awakened, fails to respond normally to pain or light, does not have sleep-wake cycles, and does not take voluntary actions. *COMA* may result from hypoxia in which the body as a whole (generalized hypoxia) or a region of the body (tissue hypoxia) is deprived of adequate oxygen supply. Hypoxia in which there is complete deprivation of oxygen supply is referred to as anoxia.>>
. *COMA* (1978)
.......................................
Dr. Susan Wheeler: You did it. [Put people in irreversible COMAS]
.
Dr. George A. Harris (Richard Widmark): No decision is easy, Sue.
. It only looks that way when you're young.
. When you're older, everything is complicated.
. *There is no black and white, only GRAY*.
-----------------------------
Art Neuendorffer
NASA: NGC 4921: Galaxy at the Edge
NGC 4921: Galaxy at the Edge
NASA Image of the Day | 30 Aug 2010
NASA Image of the Day | 30 Aug 2010
NGC 4921: Galaxy at the Edge
Spiral galaxy NGC 4921 presently is estimated to be 320 million light years distant. This image, taken by the Hubble Space Telescope, is being used to identify key stellar distance markers known as Cepheid variable stars. The magnificent spiral NGC 4921 has been informally dubbed anemic because of its low rate of star formation and low surface brightness. Visible in the image are, from the center, a bright nucleus, a bright central bar, a prominent ring of dark dust, blue clusters of recently formed stars, several smaller companion galaxies, unrelated galaxies in the far distant universe, and unrelated stars in our Milky Way Galaxy.
Credit: NASA, ESA, K. Cook (LLNL)