Question: A very early, simple satellite consisted of an inflated spherical aluminum balloon 30m in diameter and of mass 20 kg . Suppose a meteor having a mass of 7.0 kg passes within3.0 mof the surface of the satellite. What is the magnitude of the gravitational force on the meteor from the satellite at the closest approach?

Short Answer

Expert verified

Answer:

The magnitude of the gravitational force on the meteor from the satellite isF=2.9×10-11N

Step by step solution

01

Identification of given data

The mass of the spherical aluminum balloon is M = 20 kg

The mass of the meteor is m = 7.0kg

The diameter of the spherical aluminum balloon is d = 30 m

The distance between the meteor and the surface of a satellite is x = 3.0 m

02

Significance of Newton’s law of universal gravitation

Every particle in the universe is attracted to every other particle with a force that is directly proportional to the product of the masses and inversely proportional to the square of the distance, according to Newton's Law of Universal Gravitation.

Formula:

F=GMmr2

Where, is the gravitational constant ( 6.67×10-11N.m2kg2)

03

Determining the magnitude of the gravitational force on the meteor from the satellite at the closest approach

The radius of the spherical aluminum balloon is

R=d2=30m2

R = 15

The distance betweenthecenter ofthesatellite and the center ofthemeteor is

r=R+x

According to the Newton’s law of gravitation, the force of attraction is

r=15m+3.0mr=18m

The magnitude of the gravitational force on the meteor from the satellite is

F=GMmr2F=6.67×10-11N.m2kg2×20kg×7.0kg18m2F=2.9×10-11N

.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

We watch two identical astronomical bodies Aand B, each of mass m, fall toward each other from rest because of the gravitational force on each from the other. Their initial center-to-center separation isRi. Assume that we are in an inertial reference frame that is stationary with respect to the center of mass of this two body system. Use the principle of conservation of mechanical energy (Kf+ Uf=Ki +Ui ) to find the following when the center-to-center separation is 0.5Ri:

(a) the total kinetic energy of the system,

(b) the kinetic energy of each body,

(c) the speed of each body relative to us, and

(d) the speed of body Brelative to body A. Next assume that we are in a reference frame attached to body A(we ride on the body). Now we see body Bfall from rest toward us. From this reference frame, again useKf+Uf=Ki+Uito find the following when the center-to-center separation is0.5Ri:

(e) the kinetic energy of body Band

(f) the speed of body Brelative to body A.

(g) Why are the answers to (d) and (f) different? Which answer is correct?

Two neutron stars are separated by a distance of1.0×1010m. They each have a mass of 1.0×1030kgand a radiusof1.0×105m . They are initially at rest with respect to each other.As measured from that rest frame, how fast are they moving when(a) their separation has decreased to one-half its initial value and(b) they are about to collide?

z Assume a planet is a uniform sphere of radiusRthat (somehow) has a narrow radial tunnel through its center. Also assume we can position an apple any where a long the tunnel or outside the sphere. LetFRbe the magnitude of the gravitational force on the apple when it is located at the planet’s surface. How far from the surface is there a point where the magnitude isrole="math" localid="1657195577959" FRif we move the apple (a) away from the planet and (b) into the tunnel?

Two20Kgspheres are fixed in place on a yaxis, one aty=0.40mand the other aty=0.40m. A 10 kg ball is then released from rest at a point on the xaxis that is at a great distance (effectively infinite) from the spheres. If the only forces acting on the ball are the gravitational forces from the spheres, then when the ball reaches the (x, y) point(0.30m,0),,what are (a) its kinetic energy and (b) the net force on it from the spheres, in unit-vector notation?

The mean diameters of Mars and Earth are6.9×103km and1.3×104km , respectively. The mass of Mars is0.11 timesEarth’s mass. (a) What is the ratio of the mean density (mass perunit volume) of Mars to that of Earth? (b) What is the value of thegravitational acceleration on Mars? (c) What is the escape speedon Mars?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free