Universal Law of Gravitation and G
NEET Test Series from KOTA - 10 Papers In MS WORD WhatsApp Here
PHXI08:GRAVITATION

360027 Which of the following is the evidence to show that there must be a force acting on earth and directed towards Sun?

1 Apparent motion of sun around the earth
2 Phenomenon of day and night
3 Revolution of earth round the Sun
4 Deviation of the falling body towards earth
PHXI08:GRAVITATION

360028 Two equal masses separated by a distance \(d\) attract each other with a force \((F)\). If one unit of mass is transferred from one of them to the other, the force

1 Does not change
2 Decreases by \(\left( {G/{d^2}} \right)\)
3 Becomes \(d^{2}\) times
4 Increases by \(\left( {2G/{d^2}} \right)\)
PHXI08:GRAVITATION

360029 The distance of the centres of moon and earth is \(D\). The mass of earth is 81 times the mass of the moon. At what distance from the centre of the earth, the gravitational force on a particle will be zero

1 \(\frac{D}{2}\)
2 \(\frac{{2D}}{3}\)
3 \(\frac{{4D}}{3}\)
4 \(\frac{{9D}}{{10}}\)
PHXI08:GRAVITATION

360030 The figure shows four arrangements of three particles of equal masses. Rank the arrangement according to the magnitude of the net gravitational force on the particle marked \(m\), greatest first
supporting img

1 \(a\), tie of \(c\) and \(d\), then \(b\)
2 \(a,d,c,b\)
3 \(b,c,d,a\)
4 \(d,c,a,b\)
PHXI08:GRAVITATION

360027 Which of the following is the evidence to show that there must be a force acting on earth and directed towards Sun?

1 Apparent motion of sun around the earth
2 Phenomenon of day and night
3 Revolution of earth round the Sun
4 Deviation of the falling body towards earth
PHXI08:GRAVITATION

360028 Two equal masses separated by a distance \(d\) attract each other with a force \((F)\). If one unit of mass is transferred from one of them to the other, the force

1 Does not change
2 Decreases by \(\left( {G/{d^2}} \right)\)
3 Becomes \(d^{2}\) times
4 Increases by \(\left( {2G/{d^2}} \right)\)
PHXI08:GRAVITATION

360029 The distance of the centres of moon and earth is \(D\). The mass of earth is 81 times the mass of the moon. At what distance from the centre of the earth, the gravitational force on a particle will be zero

1 \(\frac{D}{2}\)
2 \(\frac{{2D}}{3}\)
3 \(\frac{{4D}}{3}\)
4 \(\frac{{9D}}{{10}}\)
PHXI08:GRAVITATION

360030 The figure shows four arrangements of three particles of equal masses. Rank the arrangement according to the magnitude of the net gravitational force on the particle marked \(m\), greatest first
supporting img

1 \(a\), tie of \(c\) and \(d\), then \(b\)
2 \(a,d,c,b\)
3 \(b,c,d,a\)
4 \(d,c,a,b\)
PHXI08:GRAVITATION

360027 Which of the following is the evidence to show that there must be a force acting on earth and directed towards Sun?

1 Apparent motion of sun around the earth
2 Phenomenon of day and night
3 Revolution of earth round the Sun
4 Deviation of the falling body towards earth
PHXI08:GRAVITATION

360028 Two equal masses separated by a distance \(d\) attract each other with a force \((F)\). If one unit of mass is transferred from one of them to the other, the force

1 Does not change
2 Decreases by \(\left( {G/{d^2}} \right)\)
3 Becomes \(d^{2}\) times
4 Increases by \(\left( {2G/{d^2}} \right)\)
PHXI08:GRAVITATION

360029 The distance of the centres of moon and earth is \(D\). The mass of earth is 81 times the mass of the moon. At what distance from the centre of the earth, the gravitational force on a particle will be zero

1 \(\frac{D}{2}\)
2 \(\frac{{2D}}{3}\)
3 \(\frac{{4D}}{3}\)
4 \(\frac{{9D}}{{10}}\)
PHXI08:GRAVITATION

360030 The figure shows four arrangements of three particles of equal masses. Rank the arrangement according to the magnitude of the net gravitational force on the particle marked \(m\), greatest first
supporting img

1 \(a\), tie of \(c\) and \(d\), then \(b\)
2 \(a,d,c,b\)
3 \(b,c,d,a\)
4 \(d,c,a,b\)
PHXI08:GRAVITATION

360027 Which of the following is the evidence to show that there must be a force acting on earth and directed towards Sun?

1 Apparent motion of sun around the earth
2 Phenomenon of day and night
3 Revolution of earth round the Sun
4 Deviation of the falling body towards earth
PHXI08:GRAVITATION

360028 Two equal masses separated by a distance \(d\) attract each other with a force \((F)\). If one unit of mass is transferred from one of them to the other, the force

1 Does not change
2 Decreases by \(\left( {G/{d^2}} \right)\)
3 Becomes \(d^{2}\) times
4 Increases by \(\left( {2G/{d^2}} \right)\)
PHXI08:GRAVITATION

360029 The distance of the centres of moon and earth is \(D\). The mass of earth is 81 times the mass of the moon. At what distance from the centre of the earth, the gravitational force on a particle will be zero

1 \(\frac{D}{2}\)
2 \(\frac{{2D}}{3}\)
3 \(\frac{{4D}}{3}\)
4 \(\frac{{9D}}{{10}}\)
PHXI08:GRAVITATION

360030 The figure shows four arrangements of three particles of equal masses. Rank the arrangement according to the magnitude of the net gravitational force on the particle marked \(m\), greatest first
supporting img

1 \(a\), tie of \(c\) and \(d\), then \(b\)
2 \(a,d,c,b\)
3 \(b,c,d,a\)
4 \(d,c,a,b\)