This dream-like
image from the NASA/ESA Hubble Space Telescope features the galaxy known as NGC
3156. It lies about 73 million light-years from Earth, in the minor equatorial
constellation Sextans.
NGC 3156 is a lenticular galaxy, with two
visible threads of dark reddish-brown dust crossing the galaxy’s disk. This
galaxy type is named for their lens-like appearance when viewed from the side
or edge-on. They fall somewhere between elliptical and spiral galaxies and have
properties of both. Like spirals, lenticulars have a central bulge of stars and
a large disk surrounding it. They often have dark dust lanes like spirals, but
no large-scale spiral arms. Like ellipticals, lenticular galaxies have mostly
older stars and little ongoing star formation.
Astronomers have studied NGC 3156 in many
ways – from its cohort of globular clusters (roughly spherical groups of stars
bound together by their gravitational attraction), to the stars being destroyed
by the supermassive black hole at its heart. Using Hubble data, they compared
stars near the galaxy’s core to those in galaxies with similarly sized black
holes. They found that NGC 3156 has a higher-than-average percentage of stars
gobbled up by its supermassive black hole when compared to its counterparts.
Text credit: European Space Agency (ESA)
Image credit:
ESA/Hubble & NASA, R. Sharples, S. Kaviraj, W. Keel
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