Kepler qonuni - muammolar va yechimlar

1. The Earth’s masofa from the Sun is 149.6 x 106 km and period of Earth’s revolution is 1 year. Calculate T2 / r3

Ma'lum:

T = 1 year, r = 149.6 x 106 km

Wanted :T2 / r3 = … ?

qaror :

k = T2 / r3 = 12 / (149.6 x 106)3 = 1 / (3348071.9 x 1018) = 2.98 x 10-25 yil2/ km3

Shuningdek qarang  Kondensator zanjirlaridagi elektr energiyasi – muammolar va yechimlar

2. Universal doimiy (G) = 6.67 x 10-11 Nm2/kg2 and Sun’s 1.99 x 1030 kg.

Kepler's law – problems and solutions 1

Kepler's law – problems and solutions 2

Shuningdek qarang  Astronomik teleskoplar – muammolar va yechimlar

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?

Ma'lum:

r of Earth = 149.6 x 106 km

r of mercury = 57.9 x 106 km

T of Earth = 1 year

Kerakli: T of mercury?

yechim:

Kepler's law – problems and solutions 3

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