Question

определите силу тяготения между Землей и Солнцем, если их массы 6*10^24кг и 2*10^30 кг соответственно и расстояние между ними 1,5*10^11 м.

Answer 1

G* (M1*M2)/R^2 

G- гравитационная постоянная G=6,67*10^-11 
M1, M2 - массы первого и второго тела 
R - расстояние между телами 

F=6*10^24*2*10^30*6,67*10^-11/(1,5*10^11)^2=3.557*10^22 Н

Answer 2

Calculating Gravitational Force Between Earth and Sun

To calculate the gravitational force (F) between the Earth and the Sun, we can use the formula:

F = G * (m1 * m2) / R^2

Where: - G is the gravitational constant, approximately 6.67 x 10^-11 N m^2/kg^2 - m1 and m2 are the masses of the two objects - R is the distance between the centers of the two objects

Given: - Mass of the Earth (m1) = 6 * 10^24 kg - Mass of the Sun (m2) = 2 * 10^30 kg - Distance between them (R) = 1.5 * 10^11 m

Using the above values, we can calculate the gravitational force (F) between the Earth and the Sun:

F = (6.67 * 10^-11) * (6 * 10^24) * (2 * 10^30) / (1.5 * 10^11)^2

F ≈ 1.95 * 10^21 N [[1]](https://uchi.ru/otvety/questions/opredelit-silu-vzaimnogo-prityazheniya-mezhdu-zemley-i-lunoy-esli-massa-zemli-597-10-24-k).