Date | May 2012 | Marks available | 3 | Reference code | 12M.2.SL.TZ1.7 |
Level | Standard level | Paper | Paper 2 | Time zone | Time zone 1 |
Command term | Deduce and Determine | Question number | 7 | Adapted from | N/A |
Question
Part 2 Gravitational fields
State Newton’s universal law of gravitation.
Deduce that the gravitational field strength g at the surface of a spherical planet of uniform density is given by
\[g = \frac{{GM}}{{{R^2}}}\]
where M is the mass of the planet, R is its radius and G is the gravitational constant. You can assume that spherical objects of uniform density act as point masses.
The gravitational field strength at the surface of Mars gM is related to the gravitational field strength at the surface of the Earth gE by
gM = 0.38 × gE.
The radius of Mars RM is related to the radius of the Earth RE by
RM = 0.53 × RE.
Determine the mass of Mars MM in terms of the mass of the Earth ME.
(i) On the diagram below, draw lines to represent the gravitational field around the planet Mars.
(ii) An object falls freely in a straight line from point A to point B in time t. The speed of the object at A is u and the speed at B is v. A student suggests using the equation v=u+gMt to calculate v. Suggest two reasons why it is not appropriate to use this equation.
Markscheme
there is an attractive force;
between any two point/small masses;
proportional to the product of their masses;
and inversely proportional to the square of their separation;
Accept formula with all terms defined.
use of \(g = \frac{F}{m}\) and \(F = \frac{{GmM}}{{{R^2}}}\);
evidence of substitution/manipulation;
to get \(g = \frac{{GM}}{{{R^2}}}\)
\(\frac{{{g_M}}}{{{g_E}}} = \frac{{\frac{{{M_M}}}{{R_M^2}}}}{{\frac{{{M_E}}}{{R_E^2}}}} \Rightarrow \frac{{{M_M}}}{{{M_E}}} = \frac{{{g_M}}}{{{g_E}}} \times {\left[ {\frac{{{R_M}}}{{{R_E}}}} \right]^2}\);
\({M_{\rm{M}}}\left( { = 0.38 \times {{0.53}^2}{M_{\rm{E}}}} \right) = 0.11{M_{\rm{E}}}\);
(i) radial field with arrows pointing inwards;
(ii) field between A and B is not equal to field at surface;
acceleration is not constant between these two points;