A planet orbits a star, in a year of length 3.98 x 107 s, in a nearly circular orbit of radius 2.14 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.

Principles of Physics: A Calculus-Based Text
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Chapter3: Motion In Two Dimensions
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A planet orbits a star, in a year of length 3.98 x 107 s, in a nearly circular orbit of radius 2.14 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) Number i
(b) Number i
(c) Number
i
Units
Units
Units
Transcribed Image Text:A planet orbits a star, in a year of length 3.98 x 107 s, in a nearly circular orbit of radius 2.14 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) Number i (b) Number i (c) Number i Units Units Units
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(a) Number
(b) Number
1.58E-7
i 3.38E-3
(c) Number 5.33E-3
Units rad/s
Units m/s
Units
m/s^2
V
Transcribed Image Text:(a) Number (b) Number 1.58E-7 i 3.38E-3 (c) Number 5.33E-3 Units rad/s Units m/s Units m/s^2 V
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