This image from the NASA/ESA Hubble Space Telescope features the barred spiral galaxy NGC 3783. ESA/Hubble & NASA, M. C. Bentz, D. J. V. Rosario
This image from the NASA/ESA Hubble
Space Telescope features NGC 3783, a bright barred spiral galaxy about 130
million light-years from Earth that also lends its name to the eponymous NGC
3783 galaxy group. Like galaxy clusters, galaxy groups are aggregates of
gravitationally bound galaxies. Galaxy groups, however, are less massive
and contain fewer members than galaxy clusters do: whereas galaxy clusters can
contain hundreds or even thousands of constituent galaxies, galaxy groups do
not typically include more than 50. The Milky Way is actually part of a galaxy
group, known as the Local Group, which also holds two other large galaxies
(Andromeda and the Triangulum galaxy), as well as several dozen satellite
and dwarf galaxies. The NGC 3783 galaxy group contains 47 galaxies. It
also seems to be at a fairly early stage of its evolution, making it an
interesting object to study.
While the focus of this image is
the spiral galaxy NGC 3783, the eye is equally drawn to the very bright object
in the lower right part of this image. This is the star HD 101274. The
perspective in this image makes the star and the galaxy look like close
companions, but this is an illusion. HD 101274 lies only about 1,530
light-years from Earth, it is about 85,000 times closer than NGC 3783. This
explains how a single star can appear to outshine an entire galaxy!
NGC 3783 is a type-1 Seyfert
galaxy, which is a galaxy with a bright central region. Hubble captures it
in incredible detail, from its glowing central bar to its narrow, winding arms
and the dust threaded through them, thanks to five separate images taken in
different wavelengths of light. In fact, the galactic center is so bright that
it exhibits diffraction spikes, normally only seen on stars such as HD
101274.
Text credit: European Space Agency
(ESA)
Source: Hubble Captures a Bright Galactic and Stellar Duo - NASA Science
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