Chapter 7: Problem 4
The orbital speed of Jupiter is (A) greater than the orbital speed of earth. (B) lesser than the orbital speed of earth. (C) equal to the orbital speed of earth. (D) Zero.
/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none}
Learning Materials
Features
Discover
Chapter 7: Problem 4
The orbital speed of Jupiter is (A) greater than the orbital speed of earth. (B) lesser than the orbital speed of earth. (C) equal to the orbital speed of earth. (D) Zero.
All the tools & learning materials you need for study success - in one app.
Get started for free
In 1783, John Mitchell noted that if a body having same density as that of the sun but radius 500 times that of the sun, magnitude of its escape velocity will be greater than \(c\), the speed of light. All the light emitted by such a body will return to it. He, thus, suggested the existence of a black hole. \(v=c=\sqrt{\frac{2 G M}{R}}\) suggests that a body of mass \(M\) will act as a black hole if its radius \(R\) is less than or equal to a certain critical radius. Karl Schwarzchild, in 1926 , derived the expression for the critical radius \(R_{S}\) called Schwarzchild radius. The surface of the sphere with radius \(R_{S}\) surrounding a black hole is called event horizon. Density of the sun is (A) \(14.1 \mathrm{~kg} \mathrm{~m}^{-3}\) (B) \(141.1 \mathrm{~kg} \mathrm{~m}^{-3}\) (C) \(1410 \mathrm{~kg} \mathrm{~m}^{-3}\) (D) None of these
The period of a satellite in a circular orbit around a planet is independent of, (A) the mass of the planet. (B) the radius of the planet. (C) the mass of the satellite. (D) all of three parameters \(a, b\) and \(c\).
The Fig. \(7.9\) shows a planet in elliptical orbit around the sun \(S\). Where is the kinetic energy of the planet maximum? (A) \(P_{1}\) (B) \(P_{2}\) (C) \(P_{3}\) (D) \(P_{4}\)
Two particle of equal mass \(m\) go around a circle of radius \(R\) under the action of their mutual gravitational attraction. The speed of each particle with respect to their centre of mass is (A) \(\sqrt{\frac{G m}{R}}\) (B) \(\sqrt{\frac{G m}{4 R}}\) (C) \(\sqrt{\frac{G M}{3 R}}\) (D) \(\sqrt{\frac{G m}{2 R}}\)
A particle is projected vertically upwards from the surface of the earth with a kinetic energy equal to \(\frac{1}{3}\) times the minimum kinetic energy needed to escape. If radius of the earth is \(6400 \mathrm{~km}\), the maximum height attained by the particle (in \(\mathrm{km}\) ) from the surface of the earth is \(\frac{n R}{2}\) then the value of \(n\) is.
What do you think about this solution?
We value your feedback to improve our textbook solutions.