Embibe Experts Solutions for Chapter: Gravitation, Exercise 4: BEGINNER'S BOX - 4

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Embibe Experts Physics Solutions for Exercise - Embibe Experts Solutions for Chapter: Gravitation, Exercise 4: BEGINNER'S BOX - 4

Attempt the practice questions on Chapter 11: Gravitation, Exercise 4: BEGINNER'S BOX - 4 with hints and solutions to strengthen your understanding. Beta Question Bank for Medical: Physics solutions are prepared by Experienced Embibe Experts.

Questions from Embibe Experts Solutions for Chapter: Gravitation, Exercise 4: BEGINNER'S BOX - 4 with Hints & Solutions

MEDIUM
NEET
IMPORTANT

If earth describes an orbit round the sun of double its present radius, what will be the year on earth ?

MEDIUM
NEET
IMPORTANT

If the gravitational force were to vary inversely as mth power of the distance, then the time period of a planet in a circular orbit of radius r around the sun will be proportional to:

EASY
NEET
IMPORTANT

A planet is revolving around the sun in an elliptical orbit. Its closest distance from the sun is rmin. The farthest distance from the sun is rmax. If the orbital angular velocity of the planet when it is nearest to the sun is ω, then the orbital angular velocity at the point when it is at the farthest distance from the sun is:-

MEDIUM
NEET
IMPORTANT

The time period of revolution of moon around the earth is 28 days and radius of its orbit is 4 × 105 km.
If G = 6.67 × 10–11 Nm2/kg2 then find the mass of the earth.

MEDIUM
NEET
IMPORTANT

Let the speed of the planet at the perihelion P in Fig. be vP and the Sun-planet distance SP be rp. Relate (rp, vP) to the corresponding quantities at the aphelion (rA, vA). Will the planet take equal times to traverse BAC and CPB ?
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MEDIUM
NEET
IMPORTANT

Asatellite moves in a circular orbit around the earth. The radius of this orbit is one half that of the moon’s orbit. Find the time in which the satellite completes one revolution.

MEDIUM
NEET
IMPORTANT

A small satellite revolves round a planet in an orbit just above planet’s surface. Taking the mean density of planet as ρ, calculate the time period of the satellite.

EASY
NEET
IMPORTANT

An object weighs 10 N at the North Pole of the earth. In a geostationary satellite distant 7R from the centre of the earth (of radius R), the true weight and the apparent weight are, respectively,