Galactocentric distance
Galactocentric distance is a star's distance from the center of a galaxy. For example, our Sun is about 27 kly (8kpc) from the center of the Milky Way. Galactocentric distance may also refer to a galaxy's distance from another galaxy.
External links
- The Distance to the Galactic Center on astrophys-assist.com.
This article is issued from
Wikipedia.
The text is licensed under Creative Commons - Attribution - Sharealike.
Additional terms may apply for the media files.