To solve this problem, we need to understand the relationship between the time period of a satellite's orbit and its orbital radius. Kepler's Third Law of Planetary Motion states that the square of the period of revolution \( T \) of a satellite is directly proportional to the cube of the semi-major axis of its orbit (which is the radius \( R \) in the case of a circular orbit):
\(T^2 \propto R^3\)
Thus, for a satellite in orbit, the relationship can be written as:
\(T^2 = kR^3\)
where \( k \) is a constant of proportionality that depends on the gravitational constant and the mass of the Earth.
Let's denote the time period of the first satellite as \( T_1 \) and its orbital radius as \( R \). Thus,
\(T_1^2 = kR^3\)
For the second satellite with orbital radius \( 1.03R \), its time period \( T_2 \) is given by:
\(T_2^2 = k(1.03R)^3\)
Taking the ratio of the two time periods squared:
\(\left(\frac{T_2}{T_1}\right)^2 = \frac{k(1.03R)^3}{kR^3}\)
Simplifying this equation gives:
\(\left(\frac{T_2}{T_1}\right)^2 = (1.03)^3\)
Calculating \((1.03)^3\):
\(1.03^3 = 1.03 \times 1.03 \times 1.03 \approx 1.092727\\)
Thus,
\(\left(\frac{T_2}{T_1}\right)^2 = 1.092727\)
Taking the square root on both sides gives:
\(\frac{T_2}{T_1} = \sqrt{1.092727} \approx 1.045\)
This implies that \( T_2 \) is approximately 1.045 times the period of the first satellite, or 4.5% larger.
So, the time period of revolution of the second satellite is approximately larger than the first one by 4.5%. Hence, the correct answer is:
4.5%
Given: A satellite is launched into a circular orbit of radius \( R \) around the Earth. A second satellite is launched into an orbit of radius \( 1.03R \). We are asked to find how much larger the time period of revolution of the second satellite is compared to the first one.
The time period \( T \) of a satellite in a circular orbit around a planet is given by Kepler's third law, which can be expressed as: \[ T = 2\pi \sqrt{\frac{R^3}{GM}}, \] where: - \( T \) is the time period of revolution, - \( R \) is the radius of the orbit, - \( G \) is the gravitational constant, and - \( M \) is the mass of the Earth. This formula shows that the time period is proportional to the \( 3/2 \) power of the orbit radius: \[ T \propto R^{3/2}. \]
Let \( T_1 \) be the time period of the first satellite with orbit radius \( R \), and \( T_2 \) be the time period of the second satellite with orbit radius \( 1.03R \). Using the proportionality, we can write: \[ \frac{T_2}{T_1} = \left(\frac{R_2}{R_1}\right)^{3/2} = \left(\frac{1.03R}{R}\right)^{3/2} = (1.03)^{3/2}. \]
Now, calculate \( (1.03)^{3/2} \): \[ (1.03)^{3/2} \approx 1.045. \] Therefore, the time period of the second satellite is approximately 1.045 times the time period of the first satellite, or about a 4.5% increase. \[ \text{Percentage increase} = 1.045 - 1 = 0.045 \times 100 = 4.5\%. \]
The time period of revolution of the second satellite is larger than the first one approximately by \( \boxed{4.5\%} \).
Two projectile protons \( P_1 \) and \( P_2 \), both with spin up (along the \( +z \)-direction), are scattered from another fixed target proton \( T \) with spin up at rest in the \( xy \)-plane, as shown in the figure. They scatter one at a time. The nuclear interaction potential between both the projectiles and the target proton is \( \hat{\lambda} \vec{L} \cdot \vec{S} \), where \( \vec{L} \) is the orbital angular momentum of the system with respect to the target, \( \vec{S} \) is the spin angular momentum of the system, and \( \lambda \) is a negative constant in appropriate units. Which one of the following is correct?

A solution of aluminium chloride is electrolyzed for 30 minutes using a current of 2A. The amount of the aluminium deposited at the cathode is _________
If \[ \int \frac{2x^2 + 5x + 9}{\sqrt{x^2 + x + 1}} \, dx = \sqrt{x^2 + x + 1} + \alpha \sqrt{x^2 + x + 1} + \beta \log_e \left( \left| x + \frac{1}{2} + \sqrt{x^2 + x + 1} \right| \right) + C, \] where \( C \) is the constant of integration, then \( \alpha + 2\beta \) is equal to ________________