2013 November 25
Anemic Spiral NGC 4921 from Hubble
Image Credit: Data - Hubble Legacy Archive, ESA, NASA; Processing - Roberto Colombari
Explanation: How far away is spiral galaxy NGC 4921? Although presently estimated to be about 310 million
light years distant, a more precise determination could be coupled with its known
recession speed to help humanity better calibrate the
expansion rate of the entire visible universe. Toward
this goal, several
images were taken by the
Hubble Space Telescope in order to help identify key stellar distance markers known as
Cepheid variable stars. 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.
Visible in
the above 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.
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