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・ Psychagrapha
・ Psychai
・ PSR
・ PSR B0329+54
・ PSR B0943+10
・ PSR B0950+08
・ PSR B1257+12
・ PSR B1257+12 A
・ PSR B1257+12 B
・ PSR B1257+12 C
・ PSR B1259-63/LS 2883
・ PSR B1509-58
・ PSR B1620-26
・ PSR B1620-26 b
・ PSR B1828-11
PSR B1829−10
・ PSR B1913+16
・ PSR B1919+21
・ PSR B1937+21
・ PSR J0108-1431
・ PSR J0348+0432
・ PSR J0357+3205
・ PSR J0437-4715
・ PSR J0537-6910
・ PSR J0540-6919
・ PSR J0737-3039
・ PSR J0738-4042
・ PSR J0855-4644
・ PSR J1311–3430
・ PSR J1614–2230


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PSR B1829−10 : ウィキペディア英語版
PSR B1829−10


PSR B1829-10 (often shortened to PSR 1829-10) is a pulsar that is approximately 30,000 light-years away in the constellation of Scutum. This pulsar has been the target of interest, because of a mistaken identification of a planet around it. Andrew G. Lyne of the University of Manchester and Bailes claimed in July 1991 to have found "a planet orbiting the neutron star PSR1829-10" but in 1992 retracted. They had failed to correctly take into account the ellipticity of Earth's orbit, and had incorrectly concluded that a planet with an orbital period of half a year existed around the pulsar.
==See also==

* Extrasolar planet
* Hypothetical planet
* Pulsar
* Pulsar planet

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「PSR B1829−10」の詳細全文を読む



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