Universal Law of Gravitation and G
PHXI08:GRAVITATION

360018 \({F_g},{F_e}\) and \({F_n}\) represent the gravitational, electromagnetic and nuclear forces respectively, then arrange the increasing order of their strengths

1 \({F_n},{F_e},{F_g}\)
2 \({F_g},{F_e},{F_n}\)
3 \({F_e},{F_g},{F_n}\)
4 \({F_g},{F_n},{F_e}\)
PHXI08:GRAVITATION

360019 Three masses, each equal to \(M\), are placed at the three corners of a square of side \(a\). The force of attraction on unit mass at the fourth corner will be

1 \(\dfrac{G M}{a^{2}}\left[\dfrac{1}{2}+\sqrt{2}\right]\)
2 \(\dfrac{3 G M}{a^{2}}\)
3 \(\dfrac{G M}{3 a^{2}}\)
4 \(\dfrac{G M}{a^{2}} \sqrt{3}\)
PHXI08:GRAVITATION

360020 Particles of masses \(2M,m\) and \(M\) are respectively at points \(A\), \(B\) and \(C\) with \(AB = \frac{1}{2}(BC),m\) is much smaller than \(M\) and at time \(t=0\), they are all at rest as given in figure. At subsequent times before any collision takes place.
supporting img

1 \(m\) will remain at rest
2 \(m\) will move towards \(M\)
3 \(m\) will move towards 2\(M\)
4 \(m\) will have oscillatory motion
PHXI08:GRAVITATION

360021 An astronaut of mass \(m\) is working on a satellite orbiting the earth at a distance \(h\) from the earth's surface. The radius of the earth is \(R\), while its mass is \(M\). The gravitational pull \(F_{G}\) on the astronaut is

1 Zero since astronaut feels weightless
2 \(\dfrac{G M m}{(R+h)^{2}} < F_{G} < \dfrac{G M m}{R^{2}}\)
3 \(F_{G}=\dfrac{G M m}{(R+h)^{2}}\)
4 \(0 < F_{G} < \dfrac{G M m}{R^{2}}\)
PHXI08:GRAVITATION

360018 \({F_g},{F_e}\) and \({F_n}\) represent the gravitational, electromagnetic and nuclear forces respectively, then arrange the increasing order of their strengths

1 \({F_n},{F_e},{F_g}\)
2 \({F_g},{F_e},{F_n}\)
3 \({F_e},{F_g},{F_n}\)
4 \({F_g},{F_n},{F_e}\)
PHXI08:GRAVITATION

360019 Three masses, each equal to \(M\), are placed at the three corners of a square of side \(a\). The force of attraction on unit mass at the fourth corner will be

1 \(\dfrac{G M}{a^{2}}\left[\dfrac{1}{2}+\sqrt{2}\right]\)
2 \(\dfrac{3 G M}{a^{2}}\)
3 \(\dfrac{G M}{3 a^{2}}\)
4 \(\dfrac{G M}{a^{2}} \sqrt{3}\)
PHXI08:GRAVITATION

360020 Particles of masses \(2M,m\) and \(M\) are respectively at points \(A\), \(B\) and \(C\) with \(AB = \frac{1}{2}(BC),m\) is much smaller than \(M\) and at time \(t=0\), they are all at rest as given in figure. At subsequent times before any collision takes place.
supporting img

1 \(m\) will remain at rest
2 \(m\) will move towards \(M\)
3 \(m\) will move towards 2\(M\)
4 \(m\) will have oscillatory motion
PHXI08:GRAVITATION

360021 An astronaut of mass \(m\) is working on a satellite orbiting the earth at a distance \(h\) from the earth's surface. The radius of the earth is \(R\), while its mass is \(M\). The gravitational pull \(F_{G}\) on the astronaut is

1 Zero since astronaut feels weightless
2 \(\dfrac{G M m}{(R+h)^{2}} < F_{G} < \dfrac{G M m}{R^{2}}\)
3 \(F_{G}=\dfrac{G M m}{(R+h)^{2}}\)
4 \(0 < F_{G} < \dfrac{G M m}{R^{2}}\)
PHXI08:GRAVITATION

360018 \({F_g},{F_e}\) and \({F_n}\) represent the gravitational, electromagnetic and nuclear forces respectively, then arrange the increasing order of their strengths

1 \({F_n},{F_e},{F_g}\)
2 \({F_g},{F_e},{F_n}\)
3 \({F_e},{F_g},{F_n}\)
4 \({F_g},{F_n},{F_e}\)
PHXI08:GRAVITATION

360019 Three masses, each equal to \(M\), are placed at the three corners of a square of side \(a\). The force of attraction on unit mass at the fourth corner will be

1 \(\dfrac{G M}{a^{2}}\left[\dfrac{1}{2}+\sqrt{2}\right]\)
2 \(\dfrac{3 G M}{a^{2}}\)
3 \(\dfrac{G M}{3 a^{2}}\)
4 \(\dfrac{G M}{a^{2}} \sqrt{3}\)
PHXI08:GRAVITATION

360020 Particles of masses \(2M,m\) and \(M\) are respectively at points \(A\), \(B\) and \(C\) with \(AB = \frac{1}{2}(BC),m\) is much smaller than \(M\) and at time \(t=0\), they are all at rest as given in figure. At subsequent times before any collision takes place.
supporting img

1 \(m\) will remain at rest
2 \(m\) will move towards \(M\)
3 \(m\) will move towards 2\(M\)
4 \(m\) will have oscillatory motion
PHXI08:GRAVITATION

360021 An astronaut of mass \(m\) is working on a satellite orbiting the earth at a distance \(h\) from the earth's surface. The radius of the earth is \(R\), while its mass is \(M\). The gravitational pull \(F_{G}\) on the astronaut is

1 Zero since astronaut feels weightless
2 \(\dfrac{G M m}{(R+h)^{2}} < F_{G} < \dfrac{G M m}{R^{2}}\)
3 \(F_{G}=\dfrac{G M m}{(R+h)^{2}}\)
4 \(0 < F_{G} < \dfrac{G M m}{R^{2}}\)
NEET Test Series from KOTA - 10 Papers In MS WORD WhatsApp Here
PHXI08:GRAVITATION

360018 \({F_g},{F_e}\) and \({F_n}\) represent the gravitational, electromagnetic and nuclear forces respectively, then arrange the increasing order of their strengths

1 \({F_n},{F_e},{F_g}\)
2 \({F_g},{F_e},{F_n}\)
3 \({F_e},{F_g},{F_n}\)
4 \({F_g},{F_n},{F_e}\)
PHXI08:GRAVITATION

360019 Three masses, each equal to \(M\), are placed at the three corners of a square of side \(a\). The force of attraction on unit mass at the fourth corner will be

1 \(\dfrac{G M}{a^{2}}\left[\dfrac{1}{2}+\sqrt{2}\right]\)
2 \(\dfrac{3 G M}{a^{2}}\)
3 \(\dfrac{G M}{3 a^{2}}\)
4 \(\dfrac{G M}{a^{2}} \sqrt{3}\)
PHXI08:GRAVITATION

360020 Particles of masses \(2M,m\) and \(M\) are respectively at points \(A\), \(B\) and \(C\) with \(AB = \frac{1}{2}(BC),m\) is much smaller than \(M\) and at time \(t=0\), they are all at rest as given in figure. At subsequent times before any collision takes place.
supporting img

1 \(m\) will remain at rest
2 \(m\) will move towards \(M\)
3 \(m\) will move towards 2\(M\)
4 \(m\) will have oscillatory motion
PHXI08:GRAVITATION

360021 An astronaut of mass \(m\) is working on a satellite orbiting the earth at a distance \(h\) from the earth's surface. The radius of the earth is \(R\), while its mass is \(M\). The gravitational pull \(F_{G}\) on the astronaut is

1 Zero since astronaut feels weightless
2 \(\dfrac{G M m}{(R+h)^{2}} < F_{G} < \dfrac{G M m}{R^{2}}\)
3 \(F_{G}=\dfrac{G M m}{(R+h)^{2}}\)
4 \(0 < F_{G} < \dfrac{G M m}{R^{2}}\)