Manipal MET2014PhysicsGravitation
A system of binary stars of masses m_A and m_B are moving in circular orbits of radii r_A and r_B respectively. If T_A and T_B are the time periods of masses m_A and m_B respectively, then
Options
- AT_A T_B = ( r_A r_B )^ 3 / 2
- BT_A T_B (if r_A r_B )
- CT_A T_B (if m_A m_B )
- DT_A=T_B
Correct answer
D. T_A=T_B
Step-by-step solution
G m_A m_B (r_A+r_B )^2 = m_A r_A 4 ^2 T_A^2 = m_B r_B 4 ^2 T_B^2 aligned & m_A r_A & =m_B r_B & T_A & =T_B aligned