Astronomy Today (9th Edition)
9th Edition
ISBN: 9780134450278
Author: Eric Chaisson, Steve McMillan
Publisher: PEARSON
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Question
Chapter 2, Problem 8P
To determine
The force between a person and Earth using Newton's law of gravity, in both Newtons and Pounds.
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The sun is 93 million miles from earth. a) Convert 93 million miles to meters and use scientific notation and round your leading coefficient in your answer to the nearest tenth. (Show step by step conversion factors). EARTH has a mass of 6 x 10^24 kg and the Sun's mass is 1.9 x 10^30 kg. b). Use Newton’s law of universal gravitation to determine the gravitational force (N) between the earth and the sun.
You may attempt this question 3 more times for credit.
In this problem, we will directly calculate the surface gravity and your weight on another planet. In metric, your weight is measured in "Newtons", and 1
Newton = 1 kg m / s². Newton's constant G = 6.67 x 10-11 m³/(kg s²).
Earth has a mass = 5.97 x 1024 kg and a radius of 6378 km. You should be able to verify that g = 9.8 m/s² on Earth using the formula for surface gravity.
If your mass is 64 kg, you should also be able to verify you should weigh 626 Newtons. If you can do that you should be OK for what's next.
The mass of Venus is 4.87E+24 kg, and it's radius is 6.05E+3 km.
What is the surface gravity of this planet? (Watch your units!).
m/s²
If your mass is 64 kg, what would you weigh on Venus?
Newtons.
Note: Remember if your answer requires scientific notation to use the "e" notation: "1.1 x 105" is "1.1e5" to OWL.
Two 700-kg masses (1543 lb) are separated by a distance of 76 m. Using Newton's law of gravitation, find the magnitude of the
gravitational force exerted by one mass on the other. (Use G = 6.67 x 10-11 N-m²/kg2.)
Newton's Law of Gravitation
The gravitational force between two objects is proportional to the mass of each
object and inversely proportional to the square of the distance between the
centers of the masses:
Gm
F=
where G is a constant. The direction of the force is attractive and lies along the
line joining the centers of the two masses (fig. 5.19).
F,
0:00/5:04
m₂
figure 5.19 The gravitational force is attractive and acts along the line joining
the center of the two masses. It obeys Newton's third law of motion (F, =-F,).
480p
The magnitude of the gravitational force exerted by one mass on the other is
x 10-9 N.
Chapter 2 Solutions
Astronomy Today (9th Edition)
Ch. 2 - Prob. 1DCh. 2 - Prob. 2DCh. 2 - Prob. 3DCh. 2 - Prob. 4DCh. 2 - Prob. 5DCh. 2 - Prob. 6DCh. 2 - Prob. 7DCh. 2 - Prob. 8DCh. 2 - Prob. 9DCh. 2 - Prob. 10D
Ch. 2 - Prob. 11DCh. 2 - Prob. 12DCh. 2 - Prob. 13DCh. 2 - Prob. 14DCh. 2 - Prob. 15DCh. 2 - Prob. 1MCCh. 2 - Prob. 2MCCh. 2 - Prob. 3MCCh. 2 - Prob. 4MCCh. 2 - Prob. 5MCCh. 2 - Prob. 6MCCh. 2 - Prob. 7MCCh. 2 - Prob. 8MCCh. 2 - Prob. 9MCCh. 2 - Prob. 10MCCh. 2 - Prob. 1PCh. 2 - Prob. 2PCh. 2 - Prob. 3PCh. 2 - Prob. 4PCh. 2 - Prob. 5PCh. 2 - Prob. 6PCh. 2 - Prob. 7PCh. 2 - Prob. 8P
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