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The Sombrero Galaxy is an oblong, pale white disk with a glowing core. It appears nearly edge-on but slants slightly in the front, presenting a slight top-down view of the inner region of the galaxy and its bright core. The outer disk is darker with shades of brown and black. Different colored distant galaxies and various stars are speckled among the black background of space surrounding the galaxy.

Sombrero Galaxy

Located around 30 million light-years away in the constellation Virgo, the Sombrero Galaxy is instantly recognizable. Viewed nearly edge on, the galaxy’s softly luminous bulge and sharply outlined disk resemble the rounded crown and broad brim of the Mexican hat from which the galaxy gets its name. Though packed with stars, the Sombrero Galaxy is surprisingly not a hotbed of star formation. Less than one solar mass of gas is converted into stars within the knotted, dusty disk of the galaxy each year. Even the galaxy’s central supermassive black hole, which at nine billion solar masses is more than 2,000 times more massive than the Milky Way’s central black hole, is fairly calm. The galaxy is too faint to spot with unaided eye, but it is readily viewable with a modest amateur telescope. Seen from Earth, the galaxy spans a distance equivalent to roughly one-third the diameter of the full Moon. The galaxy’s size on the sky is too large to fit within Hubble’s narrow field of view, so this image is actually a mosaic of several images stitched together.

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