Chapter 08, Problem 47 A planet orbits a star, in a year of length 4.83 x 10^7 s, in a nearly circular orbit of radius 2.25 x 10^11 m. With respect to the star, determine (a) the angular speed of the planet, (b) the tangential speed of the planet, and (c) the magnitude of the planet's centripetal acceleration.
Chapter 08, Problem 47 A planet orbits a star, in a year of length 4.83 x...
A planet orbits a star, in a year of length 4.39 x 107 s, in a nearly circular orbit of radius 1.77 x 1011 m. With respect to the star, determine (a) the angular speed of the planet, (b) the tangential speed of the planet, and (c) the magnitude of the planet's centripetal acceleration.
A planet orbits a star, in a year of length 2.88 x 107 s, in a nearly circular orbit of radius 3.80 x 1011 m. With respect to the star, determine (a) the angular speed of the planet, (b) the tangential speed of the planet, and (c) the magnitude of the planet's centripetal acceleration.
A planet orbits a star, in a year of length 4.22 x 107 s, in a nearly circular orbit of radius 2.69 x 1011 m. With respect to the star, determine (a) the angular speed of the planet, (b) the tangential speed of the planet, and (c) the magnitude of the planet's centripetal acceleration.
A planet orbits a star, in a year of length 2.23 x 107 s, in a nearly circular orbit of radius 2.89 x 1011 m. With respect to the star, determine (a) the angular speed of the planet, (b) the tangential speed of the planet, and (c) the magnitude of the planet's centripetal acceleration.
A planet orbits a star once every 2.90 x 10's in a nearly circular orbit of radius 1.43 x 1011 m. (a) With respect to the star, determine the angular speed of the planet. rad/s (b) With respect to the star, determine the tangential speed of the planet. m/s (C) With respect to the star, determine the magnitude and direction of the planet's centripetal acceleration. magnitude direction ---Select--- m/s2
please show work 7. 1.1/3.1 points Previous Answers CJ10 8.P.047. A planet orbits a star once every 3.29 x 10's in a nearly circular orbit of radius 1.53 x 1011 m. (a) With respect to the star, determine the angular speed of the planet. X rad/s (b) with respect to the star, determine the tangential speed of the planet. 29219.7 m/s (c) with respect to the star, determine the magnitude and direction of the planet's centripetal acceleration, magnitude m/s2 direction...
Problem 1 Planetary Orbits Consider the two-body problem for a planet-star system. The planet, of mass m, is initially in a circular orbit of radius r and angular speed w about the star, of mass M. (i) What is the gravitational potential energy of the system, U? What is the kinetic energy of the planet, K? What is the total energy of the system, E = K +U? (ii) The star suddenly loses half of its mass, M + M/2....
Chapter 08, Problem 51 Chalkboard Video A star has a mass of 2.10 x 1050 kg and is moving in a circular orbit about the center of its galaxy. The radius of the orbit is 2.5 x 104 light-years (1 light-year = 9.5 x 1015 m), and the angular speed of the star is 2.0 x 10-15 rad/s. (a) Determine the tangential speed of the star. (b) What is the magnitude of the net force that acts on the star...
(1) . A planet orbits a star in a circle. By Kepler's 2d aw of planetary motion the planet s speed is constant. If the radius of the orbit is 1.50x10 m and it takes s complete an orbit, what are the magnitude and direction of the acceleration o f the planeti? (2) A dangerously careless student ignores safety regulations and rotates a metal probe in a circular motion experiment far faster than the safety limit in his Ia breaks...
4. Consider a planet in orbit about a star of mass M. Let the x-y plane correspond to the plane of the orbit, with the star at the origin. In the limit in which the stellar mass greatly exceeds the planetary mass, the planet's radial equation of motion is GM h2 p2 + 73 where h = rė is the planet's constant angular momentum per unit mass, and G is the universal gravitational constant. Here, x = r cos @...