21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 3.2, Problem 3.2CYU
To determine

Order the following from largest to smallest semi major axis.

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The planet Earth has a semi-major axis of a = 1.00 AU and an orbital period of P= 1 sidereal year = 365.25 days = 3.156 x 10^7 s. Compute the orbital periods of bodies orbiting the Sun with each of the following semi-major axes. a) a = 0.1 AU b) a = 10 AU c) a = 100 AU d) a = 1000 AU e) a = 10,000 AU 1 AU = 1.496 x 10^8 km = 1.496 x 10^11 m = 1.496 x 10^13 cm. GM(sun) = 1.327 x 10^20 m^3/s^2 = (Newton's Constant) x (Mass of Sun) %3D %3D
You land on Mars and observe that one of its moons (Phobos) has an orbital period of 7.66 hours. If the Phobos were farther from Mars than it is now, it’s period would be a) less than 7.66 hrs.           b) about 7.66 hrs.           c) more than 7.66 hrs.    d) difficult to predict without more information.
Directions: Complete the given table by finding the ratio of the planet’s time of the revolution to its radius. Planet Average Radius of Orbit Times of Revolution     R3     T2     T2 /R3   Mercury 5.7869 × 1010 7.605 ×106       Venus 1.081 × 1011 1.941 ×107       Earth 1.496 × 1011 3.156 ×107       What pattern do you observe in the last column of data? Which law of Kepler's does this seem to support?
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