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Alpha Fornacis
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Alpha Fornacis : ウィキペディア英語版
Alpha Fornacis


Alpha Fornacis (α Fornacis, α For) is the brightest star in the constellation Fornax. It is the only star brighter than magnitude 4.0 in the constellation. It has the proper names Dalim (in Piazzi's ''Palermo Catalogue'') and Fornacis (in Burritt's ''Atlas'').〔 plate III.〕 This star was formally identical with 12 Eridani.
The stellar classification of Alpha Fornacis is F8IV, where the luminosity class IV indicates this is a subgiant star that has just evolved off the main sequence.〔 It has 33% more mass than the Sun and is an estimated 2.9 billion years old.〔〔 Alpha Fornacis is a binary star〔 and has a high proper motion.〔 This system displays an excess of infrared emission, which may indicate the presence of circumstellar material such as a debris disk.〔
The space velocity components of this star are (U, V, W) = (–35, +20, +30) km/s.〔 Approximately 350,000 years ago, Alpha Fornacis experienced a close encounter with the A-type main sequence star HD 17848. The two came within an estimated of each other.〔
==References==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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