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| | + | {{Night Sky |
| | + | | image =Leo constellation map.JPG |
| | + | | designation =Wolf 359<br/>CN Leonis |
| | + | | rightascension =10<sup>h</sup> 56<sup>m</sup> 28.99<sup>s</sup> |
| | + | | declination =+07<sup>o</sup> 00′ 52.0″ |
| | + | | distance =7.78 ly |
| | + | | constellation =[[Leo]] |
| | + | | type =[[Star]] |
| | + | | dimensions = |
| | + | | magnitude =Apparent Mag: 13.54<br/>Absolute Mag: 16.64 |
| | + | | redshift = |
| | + | | radvelocity =19±1 km/s |
| | + | | propmotion =RA: -3842 mas/yr<br/>Dec.: -2725 mas/yr |
| | + | | parallax =419.10 ± 2.10 mas |
| | + | }} |
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| | Wolf 359 is the fourth closest star at only 7.7 light years; only [[Proxima Centauri]], [[Alpha Centauri]] and [[Barnard's Star]] being closer. The star can be found in the constellation of [[Leo]]. One of the faintest known stars, it cannot be seen by the unaided eye and has a visual magnitude of only 13.54. | | Wolf 359 is the fourth closest star at only 7.7 light years; only [[Proxima Centauri]], [[Alpha Centauri]] and [[Barnard's Star]] being closer. The star can be found in the constellation of [[Leo]]. One of the faintest known stars, it cannot be seen by the unaided eye and has a visual magnitude of only 13.54. |
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| − | Discovered in 1918 by German astronomer Max Wolf, whom the star is named after, Wolf 359 is a dim [[red dwarf]] with a [[spectral class]] of M6.5. The star's mass is between 9 and 13 percent of Sol's, and has a diameter of approximately 16 to 19 of Sol's. The luminosity is a mere .002% of our own star, so dim if Wolf 359 replaced our sun, it would appear only 10 times brighter then the moon from our world. Like many [[red dwarf|red dwarfs]], Wolf 359 is a [[flare star]] and can violently flare and brighten on occasion<ref>http://www.solstation.com/stars/wolf359.htm</ref>. | + | Discovered in 1918 by German astronomer Max Wolf, whom the star is named after, Wolf 359 is a dim [[red dwarf]] with a [[Star#Spectral_Type|spectral class]] of M5.8Ve. The star's mass is between 9 and 13 percent of Sol's, and has a diameter of approximately 16 to 19 of Sol's. The luminosity is a mere .002% of our own star, so dim if Wolf 359 replaced our sun, it would appear only 10 times brighter then the moon from our world. Like many [[red dwarf|red dwarfs]], Wolf 359 is a [[flare star]] and can violently flare and brighten on occasion, however these flares are not as intense and are lease frequent then on well known flare stars such as [[Luyten 726-8|UV Ceti]] or [[Proxima Centauri]]<ref>http://adsabs.harvard.edu/abs/1983Ap%26SS..95..235G</ref><ref>http://www.solstation.com/stars/wolf359.htm</ref>. |
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| | At present there are no known companion bodies orbiting Wolf 359<ref>http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2000AJ....119..906S&db_key=AST&high=38e0b7728707947</ref>. For an Earth like world to have liquid water on its surface (within the [[habitable zone]]), it would have to be only .0042 AU from its parent star. Such a world would be tidally locked to Wolf 359, and be repeatedly exposed to intense radiation from the occasional flares. | | At present there are no known companion bodies orbiting Wolf 359<ref>http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2000AJ....119..906S&db_key=AST&high=38e0b7728707947</ref>. For an Earth like world to have liquid water on its surface (within the [[habitable zone]]), it would have to be only .0042 AU from its parent star. Such a world would be tidally locked to Wolf 359, and be repeatedly exposed to intense radiation from the occasional flares. |