In Fig. 13-24, two particles of masses, mand 2m, are fixed in place on an axis. (a) Where on the axis can a third particle of mass 3m be placed (other than at infinity) so that the net gravitational force on it from the first two particles is zero: to the left of the first two particles, to their right, between them but closer to the more massive particle, or between them but closer to the less massive particle? (b) Does the answer change if the third particle has, instead, a mass of 16m ? (c) Is there a point off the axis (other than infinity) at which the net force on the third particle would be zero?

Short Answer

Expert verified

1. The particle of mass 3m should be placed in between the particles of masses m and 2m near the less massive particle.

2. The location of the third particle does not change if its mass is 16m.

3.There is no such a point off the axis at which the net force on the third particle would be zero.

Step by step solution

01

The given data

The masses of the particles are m, 2m and 3m.

02

Understanding the concept of the gravitational force

The force of attraction between any two bodies is directly proportional to the product of their masses and is inversely proportional to the square of the distance between them, according to Newton's universal law of gravitation. Using the concept of gravitational force, we can observe in the figure which of the forces gets canceled out. Thus, the remaining force will be the net force acting on the central particle M.

Formula:

The Gravitational force of attraction between two bodies of masses M and m separated by distance R is, F=GMmR2 …(i)

03

(a) Calculation of the position of the third particle

If the third particle of mass 3m is placed on the left side of both particles of mass m and 2m, the forces acting on it due to these two masses would be towards right and the net force will be the addition of these two forces, and they will not get canceled with each other to give the net force equal to zero.

If the particle is placed at the right side of the two masses m and 2m , the net force will be towards the left and will be non-zero.

So, the particle of mass 3m should be placed in between the particles of masses and as the gravitational force is directly proportional to the masses and inversely proportional to the square of the distance between them. The forces due to m and 2m will be equal and opposite when the third particle is placed near the less massive particle ( m ) to balance the lower mass in the numerator with the lower value of r2in the denominator.

04

(b) Calculation of the location of the third particle if mass is 16m

The location of the third particle will be the same if its mass is 16 m instead of 3m as it will be the same in the numerator of the gravitational force acting on it due to the other two particles. So, the gravitational force will depend only on the masses of the other two particles and r.

For, we can write the force equation using equation (i):

G×m×3mr2=G×2m×3m(d-r)2

In the above equation, d is the distance between m and 2m. The distance between m and 3m is r.

For 16m, we can write the force equation using equation (i):

G×m×16mr2=G×2m×16m(d-r)2

From the above two equations, we can see that 3m is on both sides of the first equation and 16m is on both sides of the second equation. So, the mass of the 3rd particle will be canceled in both equations.

Hence, the position where the 3rd particle is placed would be independent of the mass of the 3rd particle.

05

(c) Calculation to check whether there is a position where the net force is zero

If the third particle of mass 3m is placed off the axis, the component of the force by particle m on particle 3m and the component of the force by particle 2m on particle 3m would be in the same direction and hence they would be added. So, the net force acting on it would not be zero.

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

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?

Question: The radius Rh of a black hole is the radius of a mathematical sphere, called the event horizon that is centered on the black hole. Information from events inside the event horizon cannot reach the outside world. According to Einstein’s general theory of relativity,Rh=2GM/c2 , where Mis the mass of the black hole and cis the speed of light.

Suppose that you wish to study a black hole near it, at a radial distance of 50Rh. However, you do not want the difference in gravitational acceleration between your feet and your head to exceed 10 m/s2 when you are feet down (or head down) toward the black hole. (a) As a multiple of our Sun’s mass Ms , approximately what is the limit to the mass of the black hole you can tolerate at the given radial distance? (You need to estimate your height.) (b) Is the limit an upper limit (you can tolerate smaller masses) or a lower limit (you can tolerate larger masses)?

In his 1865 science fiction novelFrom the Earth to the Moon,Jules Verne described how three astronauts are shot to the Moonby means of a huge gun. According to Verne, the aluminum capsule containing the astronauts is accelerated by ignition of nitrocellulose to a speed of11km/salong the gun barrel’s length of 220m.

(a) In gunits, what is the average acceleration of the capsule and astronauts in the gun barrel?

(b) Is that acceleration tolerable

Or deadly to the astronauts?

A modern version of such gun-launched spacecraft (although without passengers) has been proposed. In this modern version,

called the SHARP (Super High Altitude Research Project) gun, ignition of methane and air shoves a piston along the gun’s tube, compressing hydrogen gas that then launches a rocket. During this launch, the rocket moves3.5km and reaches a speed of 7.0km/s. Once launched, the rocket can be fired to gain additional speed.

(c) In gunits, what would be the average acceleration of the rocket within the launcher?

(d) How much additional speed is needed (via the rocket engine) if the rocket is to orbit Earth at an altitude of 700km?

The figure shows not to scale, a cross section through theinterior of Earth. Rather than being uniform throughout, Earth isdivided into three zones: an outercrust,amantle,and an innercore.The dimensions of these zones and the masses contained within them are shown on the figure. Earth has a total mass of5.98×1024kgand a radius of6370km. Ignore rotation and assumethat Earth is spherical. (a) Calculateat the surface. (b) Suppose that a bore hole (theMohole) is driven to the crust–mantle interface at a depth of25.0km; what would be the value ofat the bottom of the hole? (c) Suppose that Earth were a uniform spherewith the same total mass and size. What would be the value ofat a depth of25.0km? (Precise measurements ofare sensitive probes of the interior structure of Earth, although results can be becloud by local variations in mass distribution.)

The mean distance of Mars from the Sun is1.52times that of Earth from the Sun. From Kepler’s law of periods, calculate the number of years required for Mars to make one revolution around the Sun; compare your answer with the value given in Appendix C.

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