Kepler's Third Law states that the ratio T/a³/2 is equal to a con- stant C for all planetary orbits around the sun, where T is the period (time for a complete orbit) and a is the semimajor axis. (a) Compute C in units of days and kilometers, given that the semi- major axis of the earth's orbit is 150 x 106 km. (b) Compute the period of Saturn's orbit, given that its semimajor axis is approximately 1.43 × 10º km.

Algebra & Trigonometry with Analytic Geometry
13th Edition
ISBN:9781133382119
Author:Swokowski
Publisher:Swokowski
Chapter11: Topics From Analytic Geometry
Section11.3: Hyperbolas
Problem 36E
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Kepler's Third Law states that the ratio T/a³/2 is equal to a con-
stant C for all planetary orbits around the sun, where T is the period
(time for a complete orbit) and a is the semimajor axis.
(a) Compute C in units of days and kilometers, given that the semi-
major axis of the earth's orbit is 150 x 106 km.
(b) Compute the period of Saturn's orbit, given that its semimajor axis
is approximately 1.43 × 10º km.
Transcribed Image Text:Kepler's Third Law states that the ratio T/a³/2 is equal to a con- stant C for all planetary orbits around the sun, where T is the period (time for a complete orbit) and a is the semimajor axis. (a) Compute C in units of days and kilometers, given that the semi- major axis of the earth's orbit is 150 x 106 km. (b) Compute the period of Saturn's orbit, given that its semimajor axis is approximately 1.43 × 10º km.
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