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・ Philip Cecil Crampton
・ Philip Cezar
・ Philip Champion
・ Philip Chan
・ Philip Charles Durham
・ Philip Charles Hardwick
・ Philip Charles Lithman AKA Snakefinger
・ Philip Charles MacKenzie
・ Philip Charles Wilkins
・ Philip Chen Nan-lok
・ Philip Cheng
・ Philip Chetwinde
・ Philip Chetwode, 1st Baron Chetwode
・ Philip Chevron
・ Philip Child
Philip Childs Keenan
・ Philip Choy
・ Philip Christison
・ Philip Christman House
・ Philip Christoph von Königsmarck
・ Philip Christophers
・ Philip Chute
・ Philip Ciaccio
・ Philip Claeys
・ Philip Clairmont
・ Philip Clark (cricketer)
・ Philip Clark (rugby union)
・ Philip Clarke
・ Philip Clarke (businessman)
・ Philip Clarke (politician)


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Philip Childs Keenan : ウィキペディア英語版
Philip Childs Keenan

Philip Childs Keenan (March 31, 1908 – April 20, 2000) was an American astronomer.
Keenan was an American spectroscopist who collaborated with William Wilson Morgan and Edith Kellman (1911–2007) to develop the MKK stellar spectral classification system between 1939 and 1943. This two-dimensional classification system (temperature & luminosity) was further revised by Morgan and Keenan in 1973. The MK system remains the standard stellar spectral classification system used by astronomers today.
During their long collaboration, Keenan tended to focus his research on stars cooler than the Sun, while Morgan emphasized the hotter stars. Keenan had a long and productive career, publishing his final scientific paper in 1999, seventy years after his first.
==Honors==
Named after him
*Asteroid 10030 Philkeenan

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