Answer: Why must the Sun be eclipsed to measure the | StudySoup

Textbook Solutions for Conceptual Physics

Chapter 36 Problem 5RQ

Question

Why must the Sun be eclipsed to measure the deflection of starlight passing near the Sun?

Solution

Solution  

Step 1 of 2

  • The bending of the path of the light by gravitational field of sun,

Light consists of a large number of energy qantas which are known as photons. The phenomenon of bending of photon or the light ray path due to the gravitational field of sun, is referred as gravitational lensing.

If we observe a star location during day time, the rays from the star will be bent due to the gravitational field of sun and hence the star will appear at apparent location. As in the figure,

gravitational lensing.jpg

Whereas if we observe the same when the sun is eclipsed or blocked(during night time),as the light rays will not be bent by the sun; the location of the star will be at actual position. As in the figure,

gravitational lensing.jpg

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Title Conceptual Physics 11 
Author Paul G. Hewitt
ISBN 9780321568090

Answer: Why must the Sun be eclipsed to measure the

Chapter 36 textbook questions

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