If the distance of the earth from Sun is $15 \times 10^6 km$ Then the distance of an imaginary planet from Sun, if its period of revolution is $2.83$ years is :
The portion of the line \( 4x + 5y = 20 \) in the first quadrant is trisected by the lines \( L_1 \) and \( L_2 \) passing through the origin. The tangent of an angle between the lines \( L_1 \) and \( L_2 \) is:
Kepler’s laws of planetary motion are three laws describing the motion of planets around the sun.
All the planets revolve around the sun in elliptical orbits having the sun at one of the foci.
It states that the radius vector drawn from the sun to the planet sweeps out equal areas in equal intervals of time.
It states that the square of the time period of revolution of a planet is directly proportional to the cube of its semi-major axis.
T2 ∝ a3