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一衛星環繞一行星做橢圓軌道之運動,設此衛星至行星最遠距離與最近距離之速度大小比為1:2,則衛星至行星最遠距離與最近距離之向心加速度大小比為何? [前中]
[詳解]
Posted in 牛頓對克卜勒行星運動定律的解釋.
Tagged with 向心加速度, 橢圓, 行星運動.
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By admin – 2009 年 03 月 17 日
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