Animated Solution for Physics - Oscillations: The mass and the diameter of a planet are three times the respective values for the earth. The period of oscillation of a simple pendulum on the earth is 2 s. The period of oscillation of the same pendulum on the planet would be
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Visualized Solution
Visualizing the Planets
Let the mass and radius of Earth be Me and Re.
For the new planet, mass Mp=3Me.
Since diameter is 3 times, radius Rp=3Re.
Acceleration due to Gravity
Acceleration due to gravity on a planet's surface is given by:
g=R2GM
Gravity on the New Planet
Substitute the values for the new planet:
gp=(3Re)2G(3Me)
Simplifying Gravity
gp=9Re23GMe
gp=31(Re2GMe)
gp=31ge
Time Period of Simple Pendulum
The time period of a simple pendulum is:
T=2πgl
Ratio of Time Periods
Since length l is constant, T∝g1
TeTp=gpge
Substituting Gravity Ratio
Substitute gp=3ge:
TeTp=ge/3ge
TeTp=3
Final Calculation
Tp=3Te
Given Te=2 s
Tp=23 s
The Way Forward
What if the planet's density was given instead of mass?
Recall M=Volume×Density=34πR3ρ
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The Sigma Insight: Simple Harmonic Motion (SHM)
Solution Diagram
Imagine you are an astronaut carrying a simple pendulum from Earth to a newly discovered giant planet. This planet is massive—its mass and diameter are both three times that of Earth. How would your pendulum behave there? Let's embark on a journey to find out!
Analyzing the Setup
First, let's decode the dimensions of our new planet. We are given that its mass Mp is three times the mass of Earth Me, so Mp=3Me.
We are also told its diameter is three times Earth's diameter. Since the radius is just half of the diameter, the ratio of the radii is exactly the same as the ratio of the diameters. Therefore, the radius of the new planet Rp is three times the radius of Earth Re, giving us Rp=3Re.
The Gravity of the Situation
To understand how the pendulum swings, we need to know the gravitational pull on this new planet. According to Newton's Law of Universal Gravitation, the acceleration due to gravity g on the surface of any spherical body is given by:
g=R2GM
Let's calculate the gravity on our new planet, gp:
gp=(3Re)2G(3Me)
Be very careful here—don't forget to square the 3 in the denominator! Expanding the denominator gives us 9Re2:
gp=9Re23GMe=31(Re2GMe)
Since Re2GMe is simply the gravity on Earth (ge), we find that the gravity on the new planet is surprisingly weaker:
gp=31ge
The Pendulum's Rhythm
Now, let's look at our simple pendulum. The time period T of a simple pendulum is determined by its length l and the local gravity g:
T=2πgl
Because we are using the exact same pendulum, its length l remains constant. This means the time period is inversely proportional to the square root of gravity (T∝g1).
Let's set up a ratio to compare the time period on the new planet (Tp) to the time period on Earth (Te):
TeTp=gpge
Final Calculation
Substitute our finding that gp=3ge into the ratio:
TeTp=ge/3ge=3
This tells us that the pendulum will swing slower on the new planet. We are given that the time period on Earth is Te=2 s. Multiplying this by 3, we get our final answer:
Tp=23 s
The pendulum takes 23 seconds to complete one full oscillation on this giant, yet gravitationally weaker, planet!