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The James Webb Space Telescope captured images of 19 spiral galaxies in near- and mid-infrared light. - NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), PHANGS Team
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. [6]
The Andromeda Galaxy is the closest spiral galaxy to the Milky Way but is still about 2.5 million light years away. It is the only spiral galaxy you can see with the naked eye. Irregular galaxies ...
UGC 2885 (Rubin's Galaxy, [10] nicknamed "Godzilla galaxy" [11]) is a large barred spiral galaxy of type SA(rs)c in the constellation Perseus.It is 232 million light-years (71 Mpc) from Earth and measures 463,000 ly (142,000 pc) across, making it one of the largest known spiral galaxies.
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 1055 is an edge-on spiral galaxy located in the constellation Cetus.The galaxy has a prominent nuclear bulge crossed by a wide, knotty, dark lane of dust and gas. The spiral arm structure appears to be elevated above the galaxy's plane and obscures the upper half of the bulge.
NGC 959 is a spiral galaxy in the northern constellation of Triangulum. [10] It was discovered on 9 November 1876 by French astronomer Édouard Stephan. [9] This galaxy is located at a distance of 36 million light years and is receding with a heliocentric radial velocity of 596 km/s. [2]
NGC 4565 is a giant spiral galaxy more luminous than the Andromeda Galaxy. [6] Much speculation exists in literature as to the nature of the central bulge. In the absence of clear-cut dynamical data on the motions of stars in the bulge, the photometric data alone cannot adjudge among various options put forth.
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