In this article we are going to explore the exciting world of NGC 1175. From its origins to its impact today, NGC 1175 has generated continued interest and has become a topic of discussion and debate in various areas. Throughout these pages, we will analyze the different aspects related to NGC 1175, from its importance in modern society to its influence on popular culture. Additionally, we will examine how NGC 1175 has evolved over time and how it continues to set trends today. Be prepared to embark on an exciting journey through the ins and outs of NGC 1175 and discover everything this theme has to offer.
Peanut Galaxy | |
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![]() The galaxy, as captured by the Hubble Space Telescope during the Gems of the Galaxy Zoos project | |
Observation data (J2000 epoch) | |
Constellation | Perseus |
Right ascension | 03h 04m 32s |
Declination | +42° 20′ 21″ |
Apparent magnitude (B) | 13.8 |
Surface brightness | 23.71 mag/arcsec^2 |
Characteristics | |
Type | S0A-S0B-SABa |
Other designations | |
NGC 1175,
PGC 11578, MCG 7-7-19, UGC 2515,CGCG 540-32 |
NGC 1175,[1] also known as the Peanut Galaxy,[2] is a large lenticular galaxy located in the constellation Perseus. Its speed relative to the cosmic microwave background is 5,349 ± 19 km/s, which corresponds to a Hubble distance of 78.9 ± 5.5 Mpc (~257 million ly).[3] It was discovered by the German-British astronomer William Herschel in 1786.[4]
NGC 1175 is about the same distance from the Milky Way as NGC 1177. These two galaxies form a gravitationally interacting pair.[3]
To date, a non-redshift measurement gives a distance of approximately 44,900 Mpc (~146 million ly).[5] This value is far outside the Hubble distance values. Note that it is with the average value of independent measurements, when they exist, that the NASA/IPAC database calculates the diameter of a galaxy.[3]