(a) What linear speed must an Earth satellite have to be in a circular orbit at an altitude of 160kmabove Earth’s surface?

(b) What is the period of revolution?

Short Answer

Expert verified
  1. The linear speed is7.81×103m/s.
  2. The period of revolution is87.5 min

Step by step solution

01

Given

Altitude is 160km103 m1 km=1.60×105 m.

02

Determining the concept

Newton's second law says that when a constant force acts on a massive body, it causes it to accelerate, i.e., to change its velocity, at a constant rate. In the simplest case, a force applied to an object at rest causes it to accelerate in the direction of the force.

The formulae are as follows:

R=GMr

Here,R is the radius of the planet andM is the mass of the planet.

03

(a) Determining the linear speed

If r is the radius of the orbit, then the magnitude of the gravitational force acting on the satellite is given by,

GMmr2,

Here M is the mass of Earth and m is the mass of the satellite.

The magnitude of the acceleration of the satellite is given by,

v2r,

Here vis its speed.

Newton's second law yields,

GMmr2=mv2r

Since the radius of Earth is 6.37×106 m, therefore the orbit radius will be,

r=(6.37×106 m+1.60×105 m)=6.53×106 m

The solution forv is

v=GMr=(6.67×10-11Nm2/kg2)(5.98×1024 kg)6.53×106m=7.81×103m/s

Therefore, the linear speed is7.81×103m/s

04

(b) Determining the period of revolution 

Since the circumference of the circular orbit is 2πr, the period is,

T=2πrv=2π(6.53×106m)7.82×103m/s=5.25×103s1min60s=87.5min

Therefore, the period of revolution is 87.5min.

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

Miniature black holes.Left over from the big-bang beginningof the universe, tiny black holes might still wander through the universe. If one with a mass of1×1011kg(and a radius of only1×1016m) reached Earth, at what distance from your headwould its gravitational pull on you match that of Earth’s?

The Sun, which is2.2×1020mfrom the center of the Milky Way galaxy, revolves around that center once every 2.5×108years. Assuming each star in the Galaxy has a mass equal to the Sun’s mass of 2.0×1030kg, the stars are distributed uniformly in a sphere about the galactic center, and the Sun is at the edge of that sphere, estimate the number of stars in the Galaxy.

In 1610, Galileo used his telescope to discover four prominent moons around Jupiter. Their mean orbital radiiaand periodsTare as follows:

(a) Plot log a (y-axis) against log T (x-axis) and show that you get a straight line.

(b) Measure the slope of the line and compare it with the value that you expect from Kepler’s third law.

(c) Find the mass of Jupiter from the intercept of this line with the y axis.

Question: The orbit of Earth around the Sun is almost circular. The closest and farthest distances are 1.47×108kmand 1.52×108kmrespectively. Determine the corresponding variations in (a) total energy, (b) gravitational potential energy, (c) kinetic energy, and (d) orbital speed. (Hint:Use conservation of energy and conservation of angular momentum.)

Certain neutron stars (extremely dense stars) are believed to be rotating at about1rev/s. If such a star has a radius of20 km, what must be its minimum mass so that material on its surface remains in place during the rapid rotation?

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