JEE Advanced · Physics · 9. Gravitation
Consider a star of mass \(m_2 \mathrm{~kg}\) revolving in a circular orbit around another star of mass \(m_1 \mathrm{~kg}\) with \(m_1 \gg m_2\). The heavier star slowly acquires mass from the lighter star at a constant rate of \(\gamma \mathrm{kg} / \mathrm{s}\). In this transfer process, there is no other loss of mass. If the separation between the centers of the stars is \(r\), then its relative rate of change \(\frac{1}{r} \frac{\mathrm{~d} r}{\mathrm{~d} t}\left(\right.\) in s \(\left.^{-1}\right)\) is given by:
[Note: The original question was awarded bonus marks in the JEE Advanced 2025 exam. We have changed the options to make the question valid and solvable.]
- A \(\frac{3 \gamma}{2 m_2}\)
- B \(\frac{2 \gamma}{3 m_2}\)
- C \(\frac{2 \gamma}{m_1}\)
- D \(\frac{3 \gamma}{2 m_1}\)
Answer & Solution
Correct Answer
(B) \(\frac{2 \gamma}{3 m_2}\)
Step-by-step Solution
Detailed explanation
\(\begin{aligned} & v=v_0=\sqrt{\frac{G m_1}{r}} \\ & \frac{d v_0}{d t}=\frac{v_0}{2}\left[\frac{\gamma}{m_1}-\frac{1}{r} \frac{d r}{d t}\right]\end{aligned}\)

\(\begin{aligned} & F \alpha =m_2 \frac{d v}{d t} \\ & \frac{G m_1}{r^2} \frac{v_r}{v}=\frac{d v}{d t} \\ & \frac{v_0}{r} \cdot \frac{d r}{d t} \frac{1}{v_0}=\frac{d v}{d t}\end{aligned}\)
\(\frac{V_0}{\gamma} \frac{d \gamma}{d t}=\frac{X_0}{2}\left[\frac{r}{m_1}-\frac{1}{r} \frac{d r}{d t}\right]\)
\(\frac{3}{2} \frac{1}{\gamma} \frac{d \gamma}{d t}=\frac{r}{2 m_1} \rightarrow \frac{1}{\gamma} \frac{d r}{d t}=\frac{\gamma}{3 m_2}\)

\(\begin{aligned} & F \alpha =m_2 \frac{d v}{d t} \\ & \frac{G m_1}{r^2} \frac{v_r}{v}=\frac{d v}{d t} \\ & \frac{v_0}{r} \cdot \frac{d r}{d t} \frac{1}{v_0}=\frac{d v}{d t}\end{aligned}\)
\(\frac{V_0}{\gamma} \frac{d \gamma}{d t}=\frac{X_0}{2}\left[\frac{r}{m_1}-\frac{1}{r} \frac{d r}{d t}\right]\)
\(\frac{3}{2} \frac{1}{\gamma} \frac{d \gamma}{d t}=\frac{r}{2 m_1} \rightarrow \frac{1}{\gamma} \frac{d r}{d t}=\frac{\gamma}{3 m_2}\)
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