Gravitational fields Flashcards
Gravitational fields
Define a gravitational field
A field is a region in which a force may be exerted by an object.
What are the rules for drawing gravitational field lines?
Gravitational Field lines represent the direction of force on a mass at a point.
The separation between fields lines represents their strength
Field lines drawn for a single mass (gravitational or otherwise) never cross each other.
Gravitational field lines always point towards the centre of mass. (Gravitational force is always attractive).
Define the strength of a gravitational field (g)
The force per unit mass on a small test mass placed in the field.
Describe a radial field
The field lines are like the spokes of a wheel, towards the centre.
What happens to g in a radial field?
Decreases with increasing distance from the massive body.
Describe a uniform field
Field lines are parallel and equally spaced.
What happens to g in a uniform field?
Magnitude and direction of g is constant.
Define gravitational potential energy
The gravitational potential energy (W) at a point in a field, is the work done to move an object from infinity to that point.
Define gravitational potential
Gravitational potential at a point is the work done per unit mass to move a small object from infinity to that point.
What are equipotentials?
surfaces that join up points of equal potential.
Define potential gradient (gravitational)
Potential gradient at a point in a gravitational field is the change in potential per metre at that point.
What is Kepler’s Third Law?
The period of planet’s orbit squared is proportional to the cube of the average radius of its orbit.
What are the assumptions in Newton’s law of gravitation?
Always attractive
Proportional to the mass of each object
Proportional to 1/r^2 (r is distance between objects)
State Kepler’s first law
The orbital path of a planet around the Sun is an ellipse, not a perfect circle. The Sun lies at one of the foci of the ellipse
Define escape velocity
The minimum velocity an object must be given to escape from the planet when projected vertically from the surface.
For this to happen, the kinetic energy of the mass must be equal to the GPE gained