Paper 1 Gravitational Fields Answers
| Q | Ans | Brief reason |
|---|
| 1 | B | Newton’s law is inverse-square. |
| 2 | C | F∝1/r2. |
| 3 | A | g=F/m. |
| 4 | A | Equivalent to ms−2. |
| 5 | B | Gravity is attractive. |
| 6 | B | Potential is the work done per unit mass in bringing a small test mass from infinity to the point; equivalently, it is potential energy per unit mass. |
| 7 | B | Work is released approaching from infinity, so ϕ<0. |
| 8 | B | ϕ=−GM/r. |
| 9 | B | Potential has no direction. |
| 10 | A | Equal opposite field vectors cancel. |
| 11 | B | Potentials are scalars and add, both negative. |
| 12 | C | Gravity is the inward resultant. |
| 13 | A | From GMm/r2=mv2/r. |
| 14 | B | v=GM/r. |
| 15 | C | It matches Earth’s rotation period. |
| 16 | A | It must remain above the same point on Earth. |
| 17 | B | g=GM/r2. |
| 18 | A | g is related to the negative potential gradient. |
| 19 | B | Gravitational interaction between masses is attractive. |
| 20 | A | U=mϕ. |