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UGC 3478 is a spiral galaxy, located in the constellation of Camelopardalis. [ 3 ] [ 4 ] Is is located at 128 million light-years from Earth. [ 5 ] It features a growing supermassive black hole (AGN) at its center.
NGC 2008 is a distant spiral galaxy located in the constellation Pictor. Its speed relative to the cosmic microwave background is 10,367 ± 11 km/s, which corresponds to a Hubble distance of 153 ± 11 Mpc (~499 million ly). [1] NGC 2008 was discovered by British astronomer John Herschel in 1834. [2]
NASA’s Hubble Space Telescope recently captured a breathtaking image of the spiral galaxy NGC 2566. Astronomers use detailed Hubble images to study star clusters and active star-forming regions.
NGC 3290 (also known as Arp 53) is a large and relatively distant intermediate spiral galaxy located in the constellation Hydra.Its speed relative to the cosmic microwave background is 10,937 ± 27 km/s, [1] which corresponds to a Hubble distance of 161 ± 11 Mpc (~525 million ly). [1]
NGC 4414 is a flocculent spiral galaxy, with short segments of spiral structure but without the dramatic well-defined spiral arms of a grand design spiral. The galaxy was imaged by the Hubble Space Telescope in 1995, as part of the HST's main mission to determine the distance to galaxies, and again in 1999 as part of the Hubble Heritage project .
NGC 7496 is a member of the NGC 7582 galaxy group. [8] Other members of the group include NGC 7552, NGC 7582, NGC 7590, and NGC 7599, which are also known as the Grus Quartet, [9] NGC 7531, NGC 7632, and IC 5325. [8] This group, along with the group centred around IC 1459 form the Grus cloud, a
NGC 1512 is a barred spiral galaxy approximately 38 million light-years away from Earth [2] in the constellation Horologium.The galaxy displays a double ring structure, with a (nuclear) ring around the galactic nucleus and an (inner) further out in the main disk.