NGC 7318 (also known as UGC 12099/UGC 12100 or HCG 92d/b) is a pair of colliding galaxies about 280 million light-years from Earth. [1] . They appear in the Constellation Pegasus and are members of Stephan's Quintet. [3] . They were discovered on 27 September 1873 by French astronomer Édouard Stephan. [4]

Space telescopes have provided new insight into the nature of the filament, which is now believed to be a shock-wave in the intergalactic gas, caused by one galaxy (NGC 7318B) falling into the center of the group at several million kilometres per hour.

NGC7318 A and B are two galaxies in the compact group and The image of the galaxies shows the strong interaction between the two including tidal tails and substantial disruption of regular spiral structures. There are shock waves present and …

Jul 29, 2022 · Stephan’s Quintet is a group of four interacting galaxies – NGC 7317, NGC 7318A, NGC 7318B and NGC 7319 – and a visual companion, the spiral galaxy NGC 7320. They were among the first targets of NASA's James Webb Space Telescope (JWST).

It was the first such compact group discovered and is also called Hickson Compact Group 92. 4 galaxies are physically connected and interacting: NGC 7318 A and B, NGC7319, and NGC7317 (and possibly NGC7320c).

In what might be dubbed as a semi-final round in a galactic elimination tournament, the two spirals of NGC 7318 are colliding. The featured picture was created from images taken by the Hubble Space Telescope.

NGC 7318 is a Spiral Galaxy located in the constellation of Pegasus in the northern hemisphere. NGC 7318 is called NGC 7318 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to …

NGC 7318 is a pair of colliding galaxies about 280 million light-years from Earth. They appear in the Constellation Pegasus and are members of Stephan's Quintet.

NGC 7318 is a Galaxy Pair in the Pegasus constellation. NGC 7318 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. The image below is a photograph of NGC 7318 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in ...

Oct 1, 2012 · NGC7317-7320C technical data / Telescope: Newtonian (d=443mm, f=2048mm) / Location: Emberger Alm, Kaernten, Austria / Camera: SBIG ST-10XME with AO-8 and CFW-9 / Exposure: 12 hours (luminance 72x5 min...

NGC 7318 (also known as UGC 12099/UGC 12100 or HCG 92d/b) is a pair of colliding galaxies about 280 million light-years from Earth. [1] They appear in the Constellation Pegasus and are members of Stephan's Quintet. [3] They were discovered on 27 September 1873 by French astronomer Édouard Stephan. [4]

NGC 7318B is a Barred Spiral Galaxy in the Pegasus constellation. NGC 7318B is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.06, NGC 7318B is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

Object: NGC 7318 Stephan's Quintet - Constellation Pegasus Distance: 280 million light years Date Imaged: Sept 17 through Oct 23, 2020 Date Image Processed: Feb 2021 Telescope: 16 inch Ritchey Chretian Telescope Image Train: FLI PDF Focuser, Optec Pyxis …

As NGC 7318B collides with gas in the group, a huge shock wave bigger than the Milky Way spreads throughout the medium between the galaxies, heating some of the gas to temperatures of millions of degrees.

Feb 22, 2024 · NGC 7318 is a galaxy located in the constellation Pegasus, approximately 300 million light-years away from Earth. It is part of the Stephan's Quintet, a group of five galaxies that are interacting with each other through gravitational forces.

From Redmond , NGC7318 will become visible at around 18:29 (PST), 35° above your western horizon, as dusk fades to darkness. It will then sink towards the horizon, setting at 23:00. "Uppsala General Catalogue of Galaxies", P. Nilson, 1973. All …

===== NGC 7318 is one of four galaxies in the famous "Stephan's Quintet" found by Stephan on the night of 23 Sept 1876. I've been curious as to which of the interacting pair that forms what we now call "NGC 7318" he actually saw.

NGC 7318A is a Elliptical Galaxy in the Pegasus constellation. NGC 7318A is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.4, NGC 7318A is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

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