Gravitational fields Flashcards

(12 cards)

1
Q

State Newtons law of gravitation

A

gravitational force of attraction between two point masses is directly proportional to the product of their masses and inversely proportional to the square of the separation between their centres.

F = GMm/r^2
negative in graph but ignored for magnitude of force

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2
Q

Define Gravitational field strength

A

gravitational field strength at a point g is defined as the gravitational force per unit mass exerted on a small test mass

from g = f/m g = gmm/r^2/m
= gm/r^2 Nkg^-1

vector same direction a gravitational force
negative for graph

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3
Q

Why is value of g approximately constant near surface of earth

A

For distance h above earth surface, it is much smaller than radius of earth.
g=f/m = gMe/(Re + h)^2 approx = gMe/r^2

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4
Q

Define Gravitational Potential energy

A

The gravitational potential energy,U, of a mass m at a point in the gravitational field due to a mass M is work done by an external force in bring the mass m from infinity to that point

Work done is opposite to gravitational attraction, against gravity in bringing mass from infinity to that point

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5
Q

Derive U

A

integrate force external which is negative of the -ve gravitational force, Gmm/r^2
integrate from r to infinity.
Since at infinity U=0,
U= -GMm/r

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6
Q

Define gravitational potential

A

Work done per unit mass in bringing small test mass from infinity to that point

= -Gm/r
negative because in its WD, F and S in opposite directions
Gravitational Potential energy of a mass depends on both value of mass as well as position of mass. However gravitational potential is only dependent on position

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7
Q

Define equipotential lines

A

is formed by all the points that are at the same gravitational potential. in 2 dimensions. These points from a circle while in three dimensions these point for a sphere around a spherical massive object.

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8
Q

What can be derived from graphs

A

Negative Gradient at a point of potential-r graph is g

Area under g-r graph is magnitude change in potential

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9
Q

Derive escape speed

A

minimum energy at infinity to escape =
-gmm/r^2 + 1/2mv^2 = 0

Total energy at point =

-gmm/r^2 + 1/2mv^2

sub both to get v= root(2gr)

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10
Q

Derive relationship between T and r

A

Gravitation force provides for Fc

Gmm/r^2 = m(r)(omega)^2

since omega = 2pi/t

derive until get
r^3 = GM/4pi^2 T2

r^3 proportional to T^2

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11
Q

Explain Significance of - total energy of object in orbit

A

Bound to orbit cannot escape (0 or +ve)

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12
Q

To derive total energy of orbit

A

Gravitational force provides for centripetal force
gravitational force=mv^2/r

Derive 1/2mv^2 = 1/2gmm/r

then add with potential (rmb -ve) sign

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