In this article we are going to talk about NGC 1536, a topic that has captured the attention of people of all ages and interests. NGC 1536 is a topic that has generated a lot of debate and controversy in recent times, and it is important to analyze it from different perspectives. From its impact on society to its relevance in popular culture, NGC 1536 has proven to be a topic of general interest that deserves to be explored in depth. Throughout this article, we will analyze different aspects of NGC 1536, from its origin to its possible consequences in the future.
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 is a Type II Supernova in NGC 1536 discovered by Duília de Mello in 1997. 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.[5]