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NGC 509 information


NGC 509
NGC 509 (SDSS)
Observation data (J2000.0 epoch)
ConstellationPisces
Right ascension01h 23m 24.10s [1]
Declination+09° 26′ 01.00″ [1]
Redshift0.007542 [1]
Heliocentric radial velocity2261 ± 5 km/s [1]
Distance87 Mly[1]
Apparent magnitude (V)13.70 [2]
Apparent magnitude (B)14.60 [2]
Characteristics
TypeS0? [1]
Apparent size (V)1.6 x 0.6 [1]
Other designations
UGC 932, MCG +01-04-045, PGC 5080

NGC 509 is a lenticular galaxy approximately 87 million light-years away from Earth in the constellation of Pisces.[1] It was discovered by German astronomer Albert Marth on October 1, 1864.[3]

NGC 509 and NGC 505 (SDSS)
  1. ^ a b c d e f g h Cite error: The named reference Database was invoked but never defined (see the help page).
  2. ^ a b Cite error: The named reference seds was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference astronomy-mall was invoked but never defined (see the help page).

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NGC 509

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NGC 509 is a lenticular galaxy approximately 87 million light-years away from Earth in the constellation of Pisces. It was discovered by German astronomer...

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NGC 505 is a lenticular galaxy approximately 234 million light-years away from Earth in the constellation of Pisces. It was discovered by German astronomer...

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Large Magellanic Cloud, Small Magellanic Cloud, M32, NGC 205, NGC 6822, NGC 185, IC 1613 and NGC 147. He also identified IC 10 as a possible part of the...

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1856; ApJ 276, S. 509-518 (1984) "NGC/IC Project". Archived from the original on 2013-01-15. Retrieved 2020-04-12. Media related to NGC 1856 at Wikimedia...

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Group galaxies M31 and M32, and a few galaxies beyond the Local Group, e.g. NGC 4395. In these galaxies, the mean square (or root mean square) velocities...

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stars – III. A detailed view of NGC 6905 and its central star". Monthly Notices of the Royal Astronomical Society. 509: 974–989. arXiv:2110.09551. doi:10...

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originally named the Andromeda Nebula and is cataloged as Messier 31, M31, and NGC 224. Andromeda has a D25 isophotal diameter of about 46.56 kiloparsecs (152...

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NGC 1600

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matter concentration of the galaxy group NGC 1600". Monthly Notices of the Royal Astronomical Society. 509 (2): 2647–2653. arXiv:2110.13931. doi:10.1093/mnras/stab3139...

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NGC 6445

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"Spectrophotometric studies 22 irregular ring nebulae NGC 6445". The Astrophysical Journal. 182: 509. doi:10.1086/152158. Perinotto, M. (June 1991). "Chemical...

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NGC 3593

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in the lenticular galaxy NGC 3593 reveal a supermassive black hole". Monthly Notices of the Royal Astronomical Society. 509 (2): 2920–2939. arXiv:2110...

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stars are only a few million years old. Lying 2 degrees southwest of NGC 2362 is NGC 2354 a fainter open cluster of magnitude 6.5, with around 15 member...

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Delphinus

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stars – III. A detailed view of NGC 6905 and its central star". Monthly Notices of the Royal Astronomical Society. 509: 974–989. arXiv:2110.09551. doi:10...

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NGC 2539

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Proplyd

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were discovered in the very young region NGC 2024, two of which have been photoevaporated by a B star. The NGC 2024 proplyds are significant because they...

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Supermassive black hole

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Possible examples include the black holes at the cores of TON 618, NGC 6166, ESO 444-46 and NGC 4889, which are among the most massive black holes known. Some...

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Hercules Cluster

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super-structure. The cluster's brightest member is the giant elliptical galaxy NGC 6041. Abell catalogue List of Abell clusters X-ray Astronomy NASA Astronomy...

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star-forming rate. NGC 253-dw2 (2016) is a dwarf spheroidal (dSph) galaxy candidate undergoing tidal disruption around the nearby galaxy NGC 253. The galaxy...

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