The formula for gravitational potential energy \(U\) between two point masses \(m_1\) and \(m_2\) separated by a distance \(r\) is given by: \[ U = -\frac{G m_1 m_2}{r} \] Where:
\(G\) is the gravitational constant,
\(m_1 = m_2 = 1 \, \text{kg}\),
\(r = 1 \, \text{cm} = 0.01 \, \text{m}\).
Substituting the values: \[ U = -\frac{G \cdot 1 \cdot 1}{0.01} = -\frac{G}{0.01} = -100G \] Since the gravitational potential energy is negative (by convention), the magnitude is \(100G\).
The correct option is (B) : \(100\ G\)
The gravitational potential energy between two point masses is given by:
$$ U = -\frac{G m_1 m_2}{r} $$
Here, \( m_1 = 1\, \text{kg} \), \( m_2 = 1\, \text{kg} \), \( r = 1\, \text{cm} = 0.01\, \text{m} \)
Substituting the values: $$ U = -\frac{G \cdot 1 \cdot 1}{0.01} = -\frac{G}{0.01} = -100G $$
The magnitude of gravitational potential energy is 100G J.
Correct answer: 100G
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of