A brand new photograph from the Hubble House Telescope reveals the gorgeous construction of a distant spiral galaxy.
The galaxy, known as NGC 1961, is classed as an intermediate spiral galaxy with an lively galactic nucleus (AGN). It’s situated about 180 million light-years away within the constellation Camelopardalis.
“The galaxy NGC 1961 unfurls its attractive spiral arms on this newly launched picture from NASA’s Hubble Space Telescope,” in keeping with a statement (opens in new tab) from the space company. “Glittering, blue areas of vivid younger stars dot the dusty spiral arms winding across the galaxy’s glowing middle.”
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AGN galaxies have very vivid facilities that may outshine the remainder of the galaxy as a result of presence of a supermassive black hole at its core. The supermassive black hole pulls in materials from its environment and releases huge quantities of radiation within the type of vivid jets and winds, which gas the galaxy’s lively nucleus.
The current Hubble observations counsel NGC 1961 is a reasonably frequent kind of AGN that emits low-energy-charged particles, NASA officers wrote within the assertion.
Categorised as an intermediate spiral galaxy, NGC 1961 lacks a well-defined central bar-shaped construction manufactured from stars, which usually acts like a funnel, pulling matter into the galaxy’s core from the encompassing accretion disk. With a medium-sized nucleus, NGC 1961 falls between an unbarred and barred spiral galaxy.
NASA shared the brand new photograph of NGC 1961 on Sept. 14. The Hubble information used to create the picture was collected as a part of different work on Arp galaxies and supernovas, in keeping with the assertion.
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