The kinetic energies of a planet in an elliptical orbit about the Sun, at positions A, B and C are KA, KB and KC, respectively. AC is the major axis and SB is perpendicular to AC at the position of the Sun S as shown in the figure. Then
According to Kepler’s 2nd Law of planetary motion, a line segment joining the sun and planet sweeps out equal areas during equal intervals of time.
KB > KA > KC
KA < KB < KC
KB < KA < KC
KA > KB > KC
To solve this problem, we need to consider the properties of elliptical orbits, specifically that of a planet orbiting the Sun. According to Kepler's laws and the conservation of angular momentum, the kinetic energy of a planet in an elliptical orbit varies with its position.
Concepts Involved:
Analysis of Positions A, B, and C:
Conclusion:
Based on the above analysis, the relative order of kinetic energies should be:
Therefore, the correct order is K_A \gt K_B \gt K_C.
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)