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Newton's law of universal gravitation

Physics • Circular Motion & Gravitation • Transitional Reasoning • 10 questions

Newton's law of universal gravitation Transitional Reasoning Download PDF

Physics · Forces & Newton's Laws · Physics · Circular Motion & Gravitation

10 Physics practice questions on Newton's law of universal gravitation. Questions that build towards applied reasoning.

Questions

  1. 1.

    Two identical scientific satellites, Alpha and Beta, travel in stable circular orbits around a uniform spherical planet. Satellite Alpha moves at an orbital speed vv and experiences a gravitational force of magnitude FF from the planet. If Satellite Beta moves at an orbital speed of 2v2v, what is the magnitude of the gravitational force exerted by the planet on Satellite Beta in terms of FF?

    • A) 2F2F
    • B) 4F4F
    • C) 8F8F
    • D) 16F16F
  2. 2.

    Two orbital research satellites, Satellite 1 and Satellite 2, travel in concentric circular orbits around a uniform spherical planet of mass MM. Satellite 1 orbits at a distance rr from the planet's center, while Satellite 2 orbits at a distance of 2r2r. Assuming gravity is the only force acting on the satellites, what is the ratio of the centripetal acceleration of Satellite 1 to that of Satellite 2, a1/a2a_1 / a_2?

    • A) 2
    • B) 4
    • C) 1/2
    • D) 1/4
  3. 3.

    An astronomical survey team discovers two exoplanets, Planet 1 and Planet 2, in stable circular orbits around a star of mass MM. Planet 1 orbits at a distance rr with an orbital period TT, while Planet 2 orbits at a distance of 4r4r. Assuming that the gravitational attraction of the central star provides the necessary centripetal force and that interplanetary gravitational forces are negligible, what is the orbital period of Planet 2 in terms of TT?

    • A) 2T2T
    • B) 4T4T
    • C) 8T8T
    • D) 16T16T
  4. 4.

    An astronomical survey detects an isolated binary star system consisting of two identical stars, each of mass MM, separated by a constant center-to-center distance dd. Under the sole influence of their mutual gravitational attraction, the two stars travel in circular orbits around their common center of mass. Based on Newton's law of universal gravitation and circular motion principles, what is the orbital speed vv of each star?

    • A) v=2GMdv = \sqrt{\frac{2GM}{d}}
    • B) v=GMdv = \sqrt{\frac{GM}{d}}
    • C) v=GM4dv = \sqrt{\frac{GM}{4d}}
    • D) v=GM2dv = \sqrt{\frac{GM}{2d}}
  5. 5.

    A deep-space observatory deploys a formation of three identical spherical scientific probes, each of mass mm, stationed at the vertices of an equilateral triangle with side length LL. The mutual gravitational force between any pair of isolated probes has a magnitude of FF. Under the influence of only their mutual gravitational attractions, what is the magnitude of the net gravitational force exerted on any one of the probes by the other two probes?

    • A) FF
    • B) 3F\sqrt{3}F
    • C) 2F2F
    • D) 2F\sqrt{2}F
  6. 6.

    Two isolated spherical asteroids in deep space, Asteroid X of mass MM and Asteroid Y of mass 3M3M, interact solely through their mutual gravitational attraction when separated by a center-to-center distance dd. If both asteroids are released from rest in an inertial reference frame, how does the magnitude of the gravitational force exerted by Asteroid Y on Asteroid X compare to that exerted by Asteroid X on Asteroid Y, and what is the ratio of their initial accelerations, aX/aYa_X / a_Y?

    • A) FY on X=3FX on YF_{\text{Y on X}} = 3 F_{\text{X on Y}}, and aX/aY=3a_X / a_Y = 3
    • B) FY on X=3FX on YF_{\text{Y on X}} = 3 F_{\text{X on Y}}, and aX/aY=13a_X / a_Y = \frac{1}{3}
    • C) FY on X=FX on YF_{\text{Y on X}} = F_{\text{X on Y}}, and aX/aY=3a_X / a_Y = 3
    • D) FY on X=FX on YF_{\text{Y on X}} = F_{\text{X on Y}}, and aX/aY=1a_X / a_Y = 1
  7. 7.

    An autonomous exploration lander of mass mm is designed to operate on two newly surveyed, uniform spherical exoplanets, Kepler-Alpha and Kepler-Beta. Planetary data reveals that Kepler-Alpha has twice the radius of Kepler-Beta, yet both exoplanets share the exact same average mass density. If the magnitude of the gravitational force exerted by Kepler-Beta on the lander at its surface is FF, what is the magnitude of the gravitational force exerted by Kepler-Alpha on the same lander at its surface?

    • A) 0.25F0.25F
    • B) 0.50F0.50F
    • C) 1.00F1.00F
    • D) 2.00F2.00F
  8. 8.

    A communications satellite of mass mm orbits a uniform spherical planet of radius RR at an altitude equal to RR above the planet's surface, experiencing a gravitational force of magnitude FF. Flight controllers activate thrusters to move the satellite into a higher circular orbit at an altitude equal to 3R3R above the surface. What is the magnitude of the gravitational force exerted by the planet on the satellite in this new orbit?

    • A) 19F\frac{1}{9}F
    • B) 13F\frac{1}{3}F
    • C) 14F\frac{1}{4}F
    • D) 116F\frac{1}{16}F
  9. 9.

    An uncrewed scientific probe is positioned along the line directly connecting a dwarf planet of mass MM and its moon of mass mm, where M=9mM = 9m. The center-to-center distance between the dwarf planet and the moon is fixed at LL. At what distance from the center of the dwarf planet is the net gravitational force exerted on the probe by these two bodies equal to zero?

    • A) 14L\frac{1}{4}L
    • B) 110L\frac{1}{10}L
    • C) 910L\frac{9}{10}L
    • D) 34L\frac{3}{4}L
  10. 10.

    A team of aerospace engineers measures a mutual gravitational attraction of magnitude FF between two spherical autonomous exploration modules separated by a center-to-center distance rr. During a surface deployment, the mass of one module is quadrupled by loading rock core samples while the mass of the other remains unchanged, and their center-to-center distance is adjusted to 2r2r. Assuming both modules behave as uniform spherical masses, what is the magnitude of the new gravitational force between them in terms of FF?

    • A) FF
    • B) 2F2F
    • C) F/2F/2
    • D) 4F4F