359973 Two planets \(A\) and \(B\) having masses \(m_{1}\) and \(m_{2}\) move around the sun in circular orbits of \(r_{1}\) and \(r_{2}\) radii, respectively. If angular momentum of \(A\) is \(L\) and that of \(B\) is \(3 L\), the ratio of time \(\operatorname{period}\left(\dfrac{T_{A}}{T_{B}}\right)\) is
359973 Two planets \(A\) and \(B\) having masses \(m_{1}\) and \(m_{2}\) move around the sun in circular orbits of \(r_{1}\) and \(r_{2}\) radii, respectively. If angular momentum of \(A\) is \(L\) and that of \(B\) is \(3 L\), the ratio of time \(\operatorname{period}\left(\dfrac{T_{A}}{T_{B}}\right)\) is
359973 Two planets \(A\) and \(B\) having masses \(m_{1}\) and \(m_{2}\) move around the sun in circular orbits of \(r_{1}\) and \(r_{2}\) radii, respectively. If angular momentum of \(A\) is \(L\) and that of \(B\) is \(3 L\), the ratio of time \(\operatorname{period}\left(\dfrac{T_{A}}{T_{B}}\right)\) is
359973 Two planets \(A\) and \(B\) having masses \(m_{1}\) and \(m_{2}\) move around the sun in circular orbits of \(r_{1}\) and \(r_{2}\) radii, respectively. If angular momentum of \(A\) is \(L\) and that of \(B\) is \(3 L\), the ratio of time \(\operatorname{period}\left(\dfrac{T_{A}}{T_{B}}\right)\) is
359973 Two planets \(A\) and \(B\) having masses \(m_{1}\) and \(m_{2}\) move around the sun in circular orbits of \(r_{1}\) and \(r_{2}\) radii, respectively. If angular momentum of \(A\) is \(L\) and that of \(B\) is \(3 L\), the ratio of time \(\operatorname{period}\left(\dfrac{T_{A}}{T_{B}}\right)\) is