Chi1 Orionis
Encyclopedia : C : CH : CHI : Chi1 Orionis
|- 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" | Details |- |style="vertical-align: baseline;" | Mass | M☉ |- |style="vertical-align: baseline;" | Radius | R☉ |- |style="vertical-align: baseline;" | Luminosity | L☉ |- |style="vertical-align: baseline;" | Temperature | K |- |style="vertical-align: baseline;" | Metallicity | |- |style="vertical-align: baseline;" | Rotation | |- |style="vertical-align: baseline;" | Age | })<()or(}})=()and(}})<())}}} years
|- ! style="background-color: #FFFFC0;" colspan="2" | Other designations |- | colspan="2" |
|} Chi1 Orionis (χ1 Ori / χ1 Orionis) is a star about 32 light years away from Earth. It is in the constellation Orion.χ1 Ori is a main sequence dwarf star of spectral type G0 V. It has a faint companion with an estimated mass of about 15% of the Sun, an orbital period of 14.1 years, and an estimated a stellar class of M6. The companion orbits an average distance of 6.1 AU from the primary and has a fairly high orbital eccentricity.
χ1 Ori is believed to be a stream star member of the Ursa Major Moving Group.
External links
- [Chi-1 Orionis] by Professor Jim Kaler.
- [Chi1 Orionis 2] at SolStation.
- [Alcyone] emphemeris.
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.
