NGC 1536 | |
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![]() A Legacy Survey DR10 image of NGC 1536 | |
Observation data (J2000 epoch) | |
Constellation | Reticulum |
Right ascension | 04h 11m 00.90s [1] |
Declination | −56° 29′ 13.0″ [1] |
Redshift | 0.004059 ± 4.30e-5 [1] |
Distance | 57 Mly (17.71 Mpc) [1] |
Apparent magnitude (V) | 12.5 [2] |
Characteristics | |
Type | SB(s)c pec? [1] |
Size | 42,000 ly [1] |
Apparent size (V) | 1.905′ × 1.259′ [2] |
Notable features | N/A |
Other designations | |
ESO 157-IG 005, [1] ESO 040957-5636.9, [1] AM 0409-563, [1] WISEA J041059.94-562850.6 [1] |
NGC 1536 is a peculiar barred spiral galaxy located around 57 million light-years away in the constellation Reticulum. [1] [2] [3] It was discovered on December 4th, 1834 by the English astronomer John Herschel, and it has a diameter around 42,000 light-years. [1] [2] [4] NGC 1536 is not known to have much star-formation, and it is not known to have an active galactic nucleus. [1] [2]
SN 1997D was a Type II Supernova in NGC 1536 discovered by Duília de Mello on 14 January 1997. [5] SN 1997D had a low expansion velocity, and it is believed that the explosion produced a stellar mass black hole, instead of a neutron star. SN 1997D was located in the southernmost part of NGC 1536. [6]
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