Hubble House Telescope picture of galaxy NGC 7814, often known as the “Little Sombrero.” Credit score: NASA, ESA, and R. de Jong (Leibniz-Institut fur Astrophysik Potsdam); Picture processing: G. Kober (NASA Goddard/Catholic College of America)
NASA’s Hubble House Telescope has allowed astronomers to view galaxies of all sizes and shapes from practically each angle. When a galaxy is seen edge-on, the mesmerizing perspective reveals a blinding slice of the universe. The “Little Sombrero,” also referred to as NGC 7814 or Caldwell 43, is one such galaxy.
Set towards a speckled backdrop of extra distant galaxies, the Little Sombrero incorporates a vivid central bulge, a skinny disk filled with mud, and a glowing halo of gasoline and stars that sprawls out into area. It's situated roughly 40 million light-years from Earth, stretches 80,000 mild years broad, and is billions of years outdated.
NASA’s Hubble House Telescope has skilled its razor-sharp eye on one of many universe’s most stately and photogenic galaxies, the Sombrero galaxy, Messier 104 (M104). The galaxy’s hallmark is a superb white, bulbous core encircled by the thick mud lanes comprising the spiral construction of the galaxy. As seen from Earth, the galaxy is tilted practically edge-on. We view it from simply six levels north of its equatorial airplane. This good galaxy was named the Sombrero due to its resemblance to the broad rim and high-topped Mexican hat. Credit score: NASA and The Hubble Heritage Workforce (STScI/AURA)
The dusty spiral is known as after the grander-appearing Sombrero galaxy (picture above), which resembles a broad-brimmed Mexican hat. Additionally considered from its edge, the Sombrero galaxy is situated simply 28 million light-years away and appears bigger than the Little Sombrero. In actuality, they're practically the identical dimension, however the Sombrero seems greater as a result of it's nearer.
This picture of the Little Sombrero is a mixture of seen and infrared observations captured by Hubble’s Superior Digicam for Surveys in 2006. The observations had been taken to help astronomers in learning the galaxy’s stellar populations, and to assist make clear the evolution of this galaxy and others prefer it.
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