UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
11th Edition
ISBN: 9781319278670
Author: Freedman
Publisher: MAC HIGHER
bartleby

Videos

Question
Book Icon
Chapter 4, Problem 36Q
To determine

The gravitational force exerted by Sun on Saturn in comparison to the gravitational force exerted by Sun on Earth. Also compare the acceleration of Saturn and Earth when the mass of Saturn is 100 times that of Earth and the semi major axis of Saturn is 10 au.

Expert Solution & Answer
Check Mark

Answer to Problem 36Q

Solution:

Gravitational forces are equal and acceleration of Saturn is 100 times less than that of Earth.

Explanation of Solution

Given data:

Mass of Saturn is 100 times the mass of Earth.

Distance of Saturn from the Sun is 10 au and distance of Earth from Sun is 1 au.

Formula used:

Newton’s law of universal gravitation is stated by an equation as,

F= G(m1m2r2)

Here, m1 is the mass of first object, m2 is the mass of second object, r is the distance between the objects, and G is the universal constant of gravitation with a value of 6.67×1011 Nm2/kg2

Explanation:

From Newton’s law of universal gravitation, the gravitational force F is proportional to the mass and inversely proportional to the square of the distance r.

Use Newton’s equation and write the expression for the gravitational force of the Sun on the Earth,

FSunearth=G(Mmr2)

Here, M is the mass of the Sun, m is the mass of the Earth, and r is the distance between Sun and Earth.

Substitute 1 au for r,

FSunearth=G(Mm(1 au)2) …… (1)

Similarly, write the equation for gravitational force of the Sun on Saturn.

FSunSaturn=G(Mmsaturnr2)

Here, msaturn is the mass of Saturn and r is the distance of Saturn from the Sun.

Substitute 100m for msaturn (as mass of Saturn is 100 times the mass of Earth) and 10 au for r.

FSunSaturn=G(M(100m)(10 au)2)=G(Mm(1 au)2) …… (2)

Observe from equations 1 and 2 that the ratio of the gravitational forces between Sun and Earth and Sun and Saturn is 1.

FSunSaturnFSunearth=1

Newton’s law of universal gravitation is stated by an equation as,

F= G(m1m2r2)

Consider that mass m1 is considerably greater in size. So, the gravitational force of m1 will accelerate the mass m2 with an acceleration a2.

Using Newton’s second law which states that the external force is the product of mass of the object and the acceleration of the object, the above equation can be written as,

m2a2= G(m1m2r2)a2= G(m1r2)

So, the above expression can be written as,

a2 m1r2 …… (3)

Use the relation derived in equation (3) to write the expression for the acceleration of the Earth due to gravitational pull on the Sun of mass M.

aEarth Mr2

Use the relation derived in equation (3) to write the expression for the acceleration of Saturn due to gravitational pull on the Sun of mass M.

aSaturn Mr2

Determine the ratio of aEarth and aSaturn.

aEarthaSaturn= r2MMr2aEarthaSaturn=(rr)2

Substitute 1 au for r and 10 au for r,

aEarthaSaturn=(10 au1 au)2aEarth=100aSaturn

Conclusion:

From Newton’s law of gravity, the gravitational force is proportional to the mass and inversely proportional to the square of the distance between the planet and the Sun. So, for both Earth and Saturn, the gravitational force of the Sun on them are equal. However, since the acceleration of a planet does not depend on the planet’s mass, but only on the Sun’s mass and the distance between them, the acceleration is 100 times less for Saturn than it is for Earth.

Want to see more full solutions like this?

Subscribe now to access step-by-step solutions to millions of textbook problems written by subject matter experts!
Students have asked these similar questions
The Magellan orbiter orbits Venus with a period of 3.26 hours. How far (in km) above the surface of the planet is it? (The mass of Venus is 4.87 ✕ 1024 kg, and the radius of Venus is 6.05 ✕ 103 km.)
What is the difference in orbital velocity between Saturn's two coorbital satellites if the semimajor axes of their orbits are 151,400 km and 151,500 km?
There is a planet X that has a mass that is 24 times that of the earth and 4 times the earth's raidus. It orbits a star Y at a distance of 12 AU. (1 AU is the earth sun distance). Star Y has a mass 3 times that of our sun.What is the orbital period of Planet X in years?If an person has an earth weight of 140 lbs, what is it's weight on the surface of planet X?

Chapter 4 Solutions

UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER

Knowledge Booster
Background pattern image
Physics
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.
Similar questions
SEE MORE QUESTIONS
Recommended textbooks for you
Text book image
College Physics
Physics
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Cengage Learning
Text book image
University Physics (14th Edition)
Physics
ISBN:9780133969290
Author:Hugh D. Young, Roger A. Freedman
Publisher:PEARSON
Text book image
Introduction To Quantum Mechanics
Physics
ISBN:9781107189638
Author:Griffiths, David J., Schroeter, Darrell F.
Publisher:Cambridge University Press
Text book image
Physics for Scientists and Engineers
Physics
ISBN:9781337553278
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Lecture- Tutorials for Introductory Astronomy
Physics
ISBN:9780321820464
Author:Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina Brissenden
Publisher:Addison-Wesley
Text book image
College Physics: A Strategic Approach (4th Editio...
Physics
ISBN:9780134609034
Author:Randall D. Knight (Professor Emeritus), Brian Jones, Stuart Field
Publisher:PEARSON
Kepler's Three Laws Explained; Author: PhysicsHigh;https://www.youtube.com/watch?v=kyR6EO_RMKE;License: Standard YouTube License, CC-BY