Kepler txoj cai - teeb meem thiab kev daws teeb meem

1. The Earth’s deb from the Sun is 149.6 x 106 km and period of Earth’s revolution is 1 year. Calculate T2 / r ib3

Paub:

T = 1 year, r = 149.6 x 106 km

xav : Twm2 / r ib3 = … ?

tshuaj :

k = T2 / r ib3 = 12 / (149.6 x 106)3 = 1 / (3348071.9 x 1018) = 2.98 x 10-25 xyoo2/km3

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2. Qhov tsis hloov pauv thoob ntiaj teb (G) = 6.67 x 10-11 Nm2/ kg2 and Sun’s 1.99 x 1030 kg ua.

Kepler's law – problems and solutions 1

Kepler's law – problems and solutions 2

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3. The mean distance of Earth from the Sun is 149.6 x 106 km and the mean distance of Mercury from the Sun is 57.9 x 106 km. The period of Earth’s revolutions is 1 year, what is the period of Mercury’s revolution?

Paub:

r of Earth = 149.6 x 106 km

r of mercury = 57.9 x 106 km

T of Earth = 1 year

SE pob: T of mercury?

Tshuaj:

Kepler's law – problems and solutions 3

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