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| Name / Constellation | NGC 660 |
Other: UGC 1201, LEDA 6318, PGC 6318 | Pis |
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| Coordinates | AR: 01h 43m 02.4s, +13° 38′ 42″ | |||
| Optics | Officina Stellare 10" f8 Richtey-Cretien | |||
| Camera-Mount | PLAYERONE POSEIDON M-PRO - ZWO ASI 1600M (ONAG)- 10Micron GM2000 QCI Mount | |||
| Filters | Antlia V-Pro LRGB | |||
| Exposure |
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| Location / Date | Promiod (Valle D'Aosta-Italy) "TLP" Remote Observatory - Dic 2023/Jan 2025 | |||
| Seeing | 2.1" @ 1.17 arcosec/pixel binning 3 | |||
| Note | Drizzle 2X in postprocessing (Pixinsight)) | |||
| Acquisition | N.I.N.A. | |||
| Processing | Adobe Photoshop - |
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| Comment |
NGC 660 is a peculiar polar ring galaxy located in the constellation of Pisces, 45 million light-years away from Earth. It is part of the small galaxy group M74 and was probably formed about a billion years ago following a collision between two galaxies.[2] In late 2012, this galaxy experienced a huge explosion that was about ten times brighter than a supernova explosion. The cause is not yet fully understood, but this event appears to have been caused by a huge jet of material emanating from the central black hole located in the galactic nucleus.
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