Universe: Stars And Galaxies
Universe: Stars And Galaxies
6th Edition
ISBN: 9781319115098
Author: Roger Freedman, Robert Geller, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 1, Problem 29Q
To determine

(a)

To convert:

The distance from the earth to sun in light years.

To determine

(b)

The distance from the Earth to Sun in parsecs.

To determine

(c)

To discuss:

Whether light year or parsecs are useful units to express the distance between Earth and Sun.

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Be sure to answer all parts. Carry out the following conversions: (a) 1.25 light-years to miles (a light-year is an astronomical measure of the distance traveled by light in a year, or 365 days; the speed of light is 3.00 × 10° m/s) x 10 mi Enter your answer in scientific notation. (b) 27.3 yd to centimeters x 10 cm Enter your answer in scientific notation. (c) 2.7 × 1010 cm/s to ft/s X 10 ft/s Enter your answer in scientific notation.
(the complete question is in the picture) If the Newtonian constant has units G = [N · m2/kg2], the speed of light has units c = [m/s], the mass has units M = [kg] and the SI unit newtons is equivalentto N = [kg · m/s2], what are the units of the relation GM/c3?A. [kg · s]B. [kg · m2/s]C. [m2/s]D. [s]
I'm having trouble completing the problem I've attached a picture of below. I was able to find the the Earth's average speed in m/s relative to the sun by doing (2pi*(1.49x10^11))/31536000. But I am struggling to find the average velocity for the same thing over a period of one year in m/s. I was wondering how to calculate that? I've tried doing the (final velocity-initial velocity)/2 but the program doesn't accept my answer when using that approach.
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