Question

Two particles moving under the influence of their mutual gravitational force describe circular orbits about one another with

0 0
Add a comment Improve this question Transcribed image text
Answer #1

8 m,am Let massm, and my are moving Under the mutual attraction from Centre of urdhero/2) . Let the speed of particle is v. 1③ Total Energy of two body gruenby = - Grimer F ) when distonde between them d= rol force between them, fg: Gooying * : 4 , 4In section C, by substituting the value T = 70/2, V = GM/ro(3/ro - 1) here view is radial velocity.

Add a comment
Know the answer?
Add Answer to:
Two particles moving under the influence of their mutual gravitational force describe circular orbits about one...
Your Answer:

Post as a guest

Your Name:

What's your source?

Earn Coins

Coins can be redeemed for fabulous gifts.

Not the answer you're looking for? Ask your own homework help question. Our experts will answer your question WITHIN MINUTES for Free.
Similar Homework Help Questions
  • Classical Mechanics Two particles move about each other in circular orbits under the influence of gravitational...

    Classical Mechanics Two particles move about each other in circular orbits under the influence of gravitational forces, with a period T_0. Their motion is suddenly stopped and then allowed to fall into each other. They collide after a time T_1. Calculate the ratio T_1/T_0.

  • 6 of 13 Properties of Circular Orbits Constants Find the orbital speed of a satelite in...

    6 of 13 Properties of Circular Orbits Constants Find the orbital speed of a satelite in a circular orbit of radius R around a planet of mass M. Express the orbital speed in terms of G, M, and R. View Available Hint(s) Learning Goal: To find some of the parameters characterizing an object moving in a circular orbit. The motivation for Isaac Newton to discover his laws of motion was to explain the properties of planetary orbits that were observed...

  • two satellites, one lighter and the other twice as massive, describe different orbits around the earth,...

    two satellites, one lighter and the other twice as massive, describe different orbits around the earth, the lighter one going on an orbit of radius twice the radius of the heavier one, 2m, r, 2r. 1.) consider one single satellite, say the lighter one. write down the equation for the gravitational force exerted by the Earth on this satellite. 2.) write down Newton second law for this satellite to go in a circular orbit. 3.) determine the equation for the...

  • tonHint: The assumption was not "it's moving in a circle."1 2. Claiming that a particle is...

    tonHint: The assumption was not "it's moving in a circle."1 2. Claiming that a particle is moving in a circle with a constant radius is logically/mathematically equiv- 3. Consider a particle moving in a cirele of radius R. How is it posible for the particle to experience an 4. After deriving the formula for centripetal acceleration, we were inspired by Newton's d Law to alent to two other claims. State at least one of those claims. acceleration when its speed...

  • Learning Goal: To understand Newton's law of gravitation and the distinction between inertial and gravitational masses....

    Learning Goal: To understand Newton's law of gravitation and the distinction between inertial and gravitational masses. In this problem, you will practice using Newton's law of gravitation. According to that law, the magnitude of the gravitational force Fg between two small particles of masses m1 and m2 separated by a distance r, is given by m1m2 T2 where G is the universal gravitational constant, whose numerical value (in SI units) is 6.67 x 10-11 Nm2 kg2 This formula applies not...

  • could you please solve a and b? Chapier 2i. Note: you needn't derive Kepler's laws-but do...

    could you please solve a and b? Chapier 2i. Note: you needn't derive Kepler's laws-but do mention when you are using them, an describe the physical concepts involved and the meanings behind the variables. u) Consider two stars Mi and M; bound together by their mutual gravitational force (and isolated from other forces) moving in elliptical orbits (of eccentricity e and semi-major axes ai and az) at distances 11 in n and r from their center of mass located at...

  • Mahiindra cole Centrale Tutorial Sheet-3 Central forces/SHM PHYSICS-101 Date 150220 1) Let a particle be subject to an attractive central force of the form n where r is the distance between the parti...

    Mahiindra cole Centrale Tutorial Sheet-3 Central forces/SHM PHYSICS-101 Date 150220 1) Let a particle be subject to an attractive central force of the form n where r is the distance between the particle and the centre of the force. Find fn), if all circular orbits are to have identical areal velocities, A 2) For what values of n are circular orbits stable with the potential energy un-Ai where A > 0? 3) A satellite of mass m 2,000 kg is...

  • after the explost Show the A 3 kg block Niides and with a speed H There...

    after the explost Show the A 3 kg block Niides and with a speed H There fric between block and track the block at A- Find the normal force on Find the normal foror Use the work energy theorem to lind the frieuon as the block he trte tion force hat the magnitude oi ar 30 N, what is the areeleration as the block passes de and directio the total ion vector the direetion of a in clear diagram. At...

  • 8.4 The Two-Dimensional Central-Force Problem The 2D harmonic oscillator is a 2D central force pr...

    8.4 The Two-Dimensional Central-Force Problem The 2D harmonic oscillator is a 2D central force problem (as discussed in TZD Many physical systems involve a particle that moves under the influence of a central force; that is, a force that always points exactly toward, or away from, a force center O. In classical mechanics a famous example of a central force is the force of the sun on a planet. In atomic physics the most obvious example is the hydrogen atom,...

  • Rotational Dynamics Assignment (200 Points) • Due Friday, July 31 at 5:00 pm Equations are in...

    Rotational Dynamics Assignment (200 Points) • Due Friday, July 31 at 5:00 pm Equations are in a separate document entitled “Equations for Rotational Dynamics Assignment” • Moments of inertia formulas are provided on the last page of this document • Show all of your work when solving equations. It is not sufficient to merely have a correct numerical answer. You need to have used legitimate equations and algebra. You also need to have correctly used the data. • Units must...

ADVERTISEMENT
Free Homework Help App
Download From Google Play
Scan Your Homework
to Get Instant Free Answers
Need Online Homework Help?
Ask a Question
Get Answers For Free
Most questions answered within 3 hours.
ADVERTISEMENT
ADVERTISEMENT
ADVERTISEMENT