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List of top Physics Questions on Keplers Laws
The maximum and minimum distances of a satellite revolving in an elliptical orbit are in the ratio $3:1$. If the speed of the satellite at the nearest distance is $v$, then the speed at the farthest distance is
KEAM - 2026
KEAM
Physics
Keplers Laws
What is the ratio of escape velocity to orbital velocity?
MHT CET - 2026
MHT CET
Physics
Keplers Laws
The semi-major axis of the orbit of Saturn is approximately nine times that of Earth. The time period of revolution of Saturn is approximately equal to
KEAM - 2026
KEAM
Physics
Keplers Laws
The maximum and minimum distances of a planet from sun are $r_1$ and $r_2$ respectively. If minimum velocity is $V_1$ and minimum velocity is $V_2$, then the ration $V_1 : V_2$ is:
KEAM - 2026
KEAM
Physics
Keplers Laws
If T is the time period of satellite in an orbit of radius r, then the time period in an orbit of radius 3r is:
KEAM - 2026
KEAM
Physics
Keplers Laws
A satellite is orbiting the Earth and dissipates energy due to some resistive forces. Its initial total mechanical energy is \(E\) (negative). If the radius of its orbit becomes half of the original value, what is the new total mechanical energy of the satellite?
BITSAT - 2026
BITSAT
Physics
Keplers Laws
If a satellite of mass M is spinning about its own axis and revolves around the earth in a circular orbit, then it does not have
KEAM - 2025
KEAM
Physics
Keplers Laws
The line that joins any planet to the sun sweeps out equal areas in equal intervals of time. This statement is
KEAM - 2025
KEAM
Physics
Keplers Laws
The period of revolution of the planet A around the sun is 27 times that of another planet B. If the distance of A from the sun is \( X \) times greater than that of B from the sun, then the value of \( X \) is
KEAM - 2025
KEAM
Physics
Keplers Laws
If a satellite orbiting the Earth is 9 times closer to the Earth than the Moon, what is the time period of rotation of the satellite? Given rotational time period of Moon = 27 days and gravitational attraction between the satellite and the moon is neglected.
JEE Main - 2025
JEE Main
Physics
Keplers Laws
Applying the principle of homogeneity of dimensions, determine which one is correct. Where \( T \) is the time period, \( G \) is the gravitational constant, \( M \) is the mass, and \( r \) is the radius of the orbit.
JEE Main - 2024
JEE Main
Physics
Keplers Laws
Correct formula for height of a satellite from earths surface is :
JEE Main - 2024
JEE Main
Physics
Keplers Laws
If the distance of the Earth from the Sun is \( 1.5 \times 10^6 \, \text{km} \), then the distance of an imaginary planet from the Sun, if its period of revolution is \( 2.83 \, \text{years} \), is:
JEE Main - 2023
JEE Main
Physics
Keplers Laws
Every planet revolves around the sun in an elliptical orbit:-
A. The force acting on a planet is inversely proportional to square of distance from sun
B. Force acting on planet is inversely proportional to product of the masses of the planet and the sun
C. The Centripetal force acting on the planet is directed away from the sun
D. The square of time period of revolution of planet around sun is directly proportional to cube of semi-major axis of elliptical orbit
Choose the correct answer from the options given below:
JEE Main - 2023
JEE Main
Physics
Keplers Laws
The time period of a satellite of earth is 24 hours. If the separation between the earth and the satellite is decreased to one fourth of the previous value, then its new time period will become.
JEE Main - 2023
JEE Main
Physics
Keplers Laws
Kepler’s third law states that the square of period of revolution T of a planet around the sun is proportional to the cube of average distance r between sun and planet i.e. T² = Kr³, where K is constant. If the masses of sun and planet are M and m respectively and as per Newton’s law of gravitation the force of attraction between them is F=(GMm)/(r²), where G is gravitational constant, the relation between G and K is described as:
BITSAT - 2020
BITSAT
Physics
Keplers Laws
Kepler's third law states that the square of the period of revolution (T) of a planet around the sun is proportional to the third power of average distance r between sun and planet i.e. T² = Kr³, where K is a constant. If the masses of sun and planet are M and m respectively and as per Newton's law of gravitation the force of attraction between them is F=(GMm)/(r²), where G is the gravitational constant. The relation between G and K is described as:
BITSAT - 2016
BITSAT
Physics
Keplers Laws
Binary stars \(m_A, m_B\) move in circular orbits. Compare their time periods.
MET - 2014
MET
Physics
Keplers Laws
A geo-stationary satellite is one which:
BITSAT - 2011
BITSAT
Physics
Keplers Laws