Why is Newton's version of Kepler's third law so useful toastronomers?It is the only way to determine the masses of many distant objects.O It tells us how rapidly a planet spins on its axis.O It explains why objects spin faster when they shrink in size.O It tells us that more-distant planets orbit the Sun more rapidly.

Given, Newton's version of Kepler third law

Why is Newton's version of Kepler's third law so useful to astronomers? It is the only way to determine the masses of many distant objects. It tells us how rapidly a planet spins on its axis. O It explains why objects spin faster when they shrink in size. O It tells us that more-distant planets orbit the Sun more rapidly.

Why is Newton's version of Kepler's third law so useful to astronomers? It is the only way to determine the masses of many distant objects. It tells us how rapidly a planet spins on its axis. O It explains why objects spin faster when they shrink in size. O It tells us that more-distant planets orbit the Sun more rapidly.

College Physics

11th Edition

ISBN:9781305952300

Author:Raymond A. Serway, Chris Vuille

Publisher:Raymond A. Serway, Chris Vuille

Chapter1: Units, Trigonometry. And Vectors

Section: Chapter Questions

Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...

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Special Relativity

The theory of special relativity discusses how space and time are related to objects traveling along a straight line at a constant speed. Simply stated, as an object reaches the speed of light, its mass becomes infinite and it is unable to move faster than light. This interstellar speed limit has been the topic of much debate in astronomy, and also in science fiction when people consider how to fly over large distances.

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Why is Newton's version of Kepler's third law so useful to
astronomers?
It is the only way to determine the masses of many distant objects.
O It tells us how rapidly a planet spins on its axis.
O It explains why objects spin faster when they shrink in size.
O It tells us that more-distant planets orbit the Sun more rapidly.

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