NGC 1512 [SEP] constellation
NGC 1512
NGC 1512 is a barred spiral galaxy approximately 38 million light-years away from Earth in the constellation Horologium. The galaxy displays a double ring structure, with one ring around the galactic nucleus and another further out in the main disk. The galaxy hosts an extended UV disc with at least 200 clusters with recent star formation activity. NGC 1512 is a member of the Dorado Group.
Gravitational interaction with NGC 1510.
Gravitational tidal forces of NGC 1512 are influencing nearby dwarf lenticular galaxy NGC 1510. The
likely from a previously existing reserve.
Other resources.
Other resources See also.
- Spiral Galaxy NGC 1512
- NGC 7742, "a very similar galaxy in the same constellation"
External links.
- NGC 7217
- http://atlas.zevallos.com.br/