Q1: A particle of mass m is under the influence of the gravitational field of a body of mass M (≫ m). The particle is moving in a circular orbit of radius r₀ with time period T₀ around the mass M. Then, the particle is subjected to an additional central force, corresponding to the potential energy Vc(r) = mα/r³, where α is a positive constant of suitable dimensions and r is the distance from the center of the orbit. If the particle moves in the same circular orbit of radius r₀ in the combined gravitational potential due to M and Vc(r), but with a new time period T₁, then (T₁² - T₀²) / T₁² is given by [G is the gravitational constant.] [ JEE Advanced 2024 Paper 2]
(a) 3αGM r02
(b) α2GM r02
(c) αGM r02
(d) 2αGM r02
Ans: (a)
Solution:
F1 = GMmr02
F2 = GMmr02 - 3mαr04
ω12ω02 = F2F1 = GMr02 - 3αr04GMr02
T12T02 = 1 - 3αGMr02
T12 - T02T12 = 3αGMr02
(a) 3R /5
(b) R / 6
(c) 6R / 5
(d) 5R/5
Ans: (a)
Solution: The formula to calculate the acceleration due to gravity at a height ( h ) from the surface of the Earth is expressed as :
To find the ratio of gravitational acceleration at two different heights ( hP ) and ( hQ ) above the Earth's surface, use the formula for each and form a ratio :
Given ℎP=Re/3, the ratio simplifies to:
Solving for ℎQ in terms of Re yields .
Q1: Two spherical stars Aand B have densities ρAand ρB, respectively. Aand Bhave the same radius, and their masses MAand MBare related by MB = 2MA. Due to an interaction process, star Aloses some of its mass, so that its radius is halved, while its spherical shape is retained, and its density remains ρA. The entire mass lost by Ais deposited as a thick spherical shell on Bwith the density of the shell being ρA. If vAand vBare the escape velocities from Aand Bafter the interaction process, the ratio . The value of nis __________ . [JEE Advanced 2022 Paper 1]
Ans: 2.2 to 2.4
Solution:
Due to an interaction process, star A losses some of it's mass and radius becomes R/2. Let new mass of star A is M'A. Here in both cases density of star A remains same ρA.
Initially
Finally
Density remains same,
So, Lost mass by
This lost mass 7MA / 8is attached on the star B and density of the attached mass stay ρA. So new radius of star B is R2.
Density of the removed part from star A is,
Density of the added part in star B stay's same as ρA,
Escape velocity from star A after interaction process,
And escape velocity from star B after interaction process,
Given,
Comparing equation (1) and (2), we get,
10n = 23
⇒ n = 2.3
Ans:9
Solution: For earth-sun system,
For binary system
Using Eqs. (i) and (ii), we get
T = 9T0
So, n = 9
Ans: (d)
Solution:
Gravitational force = Centripetal force of the earth
(∵ M = total mass from 0 to r)
Differentiate on both sides, we get
(∵ volume = mass × density)
Ans: (b)
Solution: Given m1/m2 = 2 and R1/R2 = 1/4
Now,
Thus, the correct mapping is P → 3.
Now, L = mvR
Thus, the correct mapping is Q → 2.
Now,
Thus, the correct mapping is R → R.
Now,
Thus, the correct mapping is S → 1.
Therefore, option (B) is correct.
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