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1 See also  





2 External links  














Wolf 359






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From Wikipedia, the free encyclopedia
 


This is an old revision of this page, as edited by Patricknoddy (talk | contribs)at21:11, 27 April 2007. The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
(diff)  Previous revision | Latest revision (diff) | Newer revision  (diff)

Wolf 359


Wolf 359 in Celestia

Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 10h 56m 29.2s
Declination +07° 00' 53"
Apparent magnitude (V) 13.53
Characteristics
Spectral type M6 V
U−B color index 1.34
B−V color index 2.01
Variable type Flare star
Astrometry
Radial velocity (Rv)+14.9 km/s
Proper motion (μ) RA: -3828 mas/yr
Dec.: -2720 mas/yr
Parallax (π)419.10 ± 2.10 mas
Distance7.78 ± 0.04 ly
(2.39 ± 0.01 pc)
Absolute magnitude (MV)16.64
Details
Mass0.09-0.13 M
Radius0.16-0.19 R
Luminosity0.00002 L
Temperature3,500 K
Age<1.0 ×1010 years
Other designations

CN Leonis, GCTP 2553, GJ 406, G 045-020, LTT 12923, LFT 750, LHS 36.

Wolf 359 is a star located approximately 2.4 parsecs or 7.80 light years from Earth's solar system. It is one of the nearest stars to the Sun; only the Alpha Centauri system and Barnard's star are known to be closer. Its celestial position is in the constellation Leo, near the ecliptic. It is an extremely faint red dwarf, too dim to be visible to the naked eye, and it is a flare star.

The star was discovered using astrophotography by German astronomer Max Wolfin1918. Its closest neighbor is Ross 128, 1.16 pc or 3.79 ly away.

See also

External links


Retrieved from "https://en.wikipedia.org/w/index.php?title=Wolf_359&oldid=126481177"

Categories: 
Leo constellation
Red dwarfs
Flare stars
Wolf objects
 



This page was last edited on 27 April 2007, at 21:11 (UTC).

This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



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