21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 3, Problem 22QP
To determine

Compare the Earth’s eccentricity value with Moon’s eccentricity value and how does this tells the solar eclipses.

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Suppose you're in a circular orbit around Saturn (M = 5.683 x 1026 kg) with a semi-major axis of a = 237,948 km. a. What is your orbital velocity? b. Using the "Vis-viva" equation (which can be derived from the total energy) v = GM What is the delta-V you would need to get from your current orbit, into an elliptical orbit that has an apoapsis near Titan (a = 1,221,870 km)?
How does the rotation of Earth affect the apparent weight of a 1 kg mass at the equator? Does this effect on the apparent weight happen everywhere on Earth's surface? Justify your answers.
A newly discovered planet orbits a distant star with the same mass as the Sun at an average distance of 122 million kilometers. Its orbital eccentricity is 0.6. Find the planet's orbital period. Express your answer in years to three significant figures. Find the planet's nearest and farthest orbital distances from its star. Express your answers in millions of kilometers to three significant figures separated by a comma.
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