NGC 4485
NGC 4485 is an irregular galaxy located in the constellation of Canes Venatici. It is interacting with the spiral galaxy NGC 4490 and as a result both galaxies are distorted and are undergoing intense star formation.
NGC 4485 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Canes Venatici[1] |
Right ascension | 12h 30m 31.113s[2] |
Declination | +41° 42′ 04.22″[2] |
Redshift | 0.0016[2] |
Distance | 25 million ly[1] |
Apparent magnitude (V) | 11.93[2] |
Apparent magnitude (B) | 12.32[2] |
Other designations | |
KPG 341a, MCG+07-26-013, UGC 7648, PGC 41326, UZC J123031.4+414201, 2MASX J12303111+4142042, VV 30b |
Gallery
- NGC 4485 and NGC 4490.
- Interaction between them created a stream of material about 25 000 light-years long.[3]
gollark: This is of course 22 heresy units of heresy.
gollark: Sadly, helloboi, their screenshot says windows, yes.
gollark: Satanic ubuntu?
gollark: I didn't say I was.
gollark: Thus, sinthorion did NOT write code?!
References
- "Starbursts in the wake of a fleeting romance". ESA/Hubble Picture of the Week. Retrieved 13 May 2014.
- "Search Results for NGC 4485". Astronomical Database. SIMBAD. Retrieved 13 May 2014.
- "Hubble Observes Creative Destruction as Galaxies Collide". www.spacetelescope.org. Retrieved 16 May 2019.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.