149952 A flywheel of mass \(1 \mathrm{~kg}\) and radius vector \((2 \hat{i}+\hat{\mathbf{j}}+2 \hat{\mathbf{k}}) \mathbf{m}\) is at rest. When a force \((3 \hat{i}+2 \hat{j}-4 \hat{k}) \quad N\) acts on it tangentially, it can rotate freely. Then, its angular velocity after \(4.5 \mathrm{~s}\) is
149955
The distance between Sun and Earth is \(1.6 \times\)
\(10^{11} \mathrm{~m}\) and the radius of Earth is \(6.4 \times 10^{6} \mathrm{~m}\). The ratio of the angular momentum of Earth around the Sun to the angular momentum around its own axis is approximately (Assume Earth as a solid sphere with uniform mass density and rotates around the Sun in a circular path.)
149952 A flywheel of mass \(1 \mathrm{~kg}\) and radius vector \((2 \hat{i}+\hat{\mathbf{j}}+2 \hat{\mathbf{k}}) \mathbf{m}\) is at rest. When a force \((3 \hat{i}+2 \hat{j}-4 \hat{k}) \quad N\) acts on it tangentially, it can rotate freely. Then, its angular velocity after \(4.5 \mathrm{~s}\) is
149955
The distance between Sun and Earth is \(1.6 \times\)
\(10^{11} \mathrm{~m}\) and the radius of Earth is \(6.4 \times 10^{6} \mathrm{~m}\). The ratio of the angular momentum of Earth around the Sun to the angular momentum around its own axis is approximately (Assume Earth as a solid sphere with uniform mass density and rotates around the Sun in a circular path.)
149952 A flywheel of mass \(1 \mathrm{~kg}\) and radius vector \((2 \hat{i}+\hat{\mathbf{j}}+2 \hat{\mathbf{k}}) \mathbf{m}\) is at rest. When a force \((3 \hat{i}+2 \hat{j}-4 \hat{k}) \quad N\) acts on it tangentially, it can rotate freely. Then, its angular velocity after \(4.5 \mathrm{~s}\) is
149955
The distance between Sun and Earth is \(1.6 \times\)
\(10^{11} \mathrm{~m}\) and the radius of Earth is \(6.4 \times 10^{6} \mathrm{~m}\). The ratio of the angular momentum of Earth around the Sun to the angular momentum around its own axis is approximately (Assume Earth as a solid sphere with uniform mass density and rotates around the Sun in a circular path.)
149952 A flywheel of mass \(1 \mathrm{~kg}\) and radius vector \((2 \hat{i}+\hat{\mathbf{j}}+2 \hat{\mathbf{k}}) \mathbf{m}\) is at rest. When a force \((3 \hat{i}+2 \hat{j}-4 \hat{k}) \quad N\) acts on it tangentially, it can rotate freely. Then, its angular velocity after \(4.5 \mathrm{~s}\) is
149955
The distance between Sun and Earth is \(1.6 \times\)
\(10^{11} \mathrm{~m}\) and the radius of Earth is \(6.4 \times 10^{6} \mathrm{~m}\). The ratio of the angular momentum of Earth around the Sun to the angular momentum around its own axis is approximately (Assume Earth as a solid sphere with uniform mass density and rotates around the Sun in a circular path.)
149952 A flywheel of mass \(1 \mathrm{~kg}\) and radius vector \((2 \hat{i}+\hat{\mathbf{j}}+2 \hat{\mathbf{k}}) \mathbf{m}\) is at rest. When a force \((3 \hat{i}+2 \hat{j}-4 \hat{k}) \quad N\) acts on it tangentially, it can rotate freely. Then, its angular velocity after \(4.5 \mathrm{~s}\) is
149955
The distance between Sun and Earth is \(1.6 \times\)
\(10^{11} \mathrm{~m}\) and the radius of Earth is \(6.4 \times 10^{6} \mathrm{~m}\). The ratio of the angular momentum of Earth around the Sun to the angular momentum around its own axis is approximately (Assume Earth as a solid sphere with uniform mass density and rotates around the Sun in a circular path.)