Gl 687
Encyclopedia : G : GL : GL6 : Gl 687
|- style="vertical-align: top;" | B-V color index | |- style="vertical-align: top;" | U-B color index | |- style="vertical-align: top;" | Variable type |
|- ! style="background-color: #FFFFC0;" colspan="2" | Other designations |- | colspan="2" |
This is one of the closest stars to the Sun and lies at an approximate distance of less than 15 light years. The star has a high proper motion across the sky, advancing 1.304 arc seconds per year. It has a net relative velocity of about 39 km/s.
GJ 687 is suspected of being a close binary star system.
See also
External links
From Wikipedia, the Free Encyclopedia. Original article here. Support Wikipedia by contributing or donating.
All text is available under the terms of the GNU Free Documentation License See Wikipedia Copyrights for details.
