D.1 Gravitational fields SL Flashcards
Kepler’s First Law
Planets move in elliptical orbits with the Sun at one focus
Kepler’s Second Law
A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time
Kepler’s Third Law
The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
Newton’s Universal Law of Gravitation Equation
F is the force between masses, G is the gravitational constant, m1 and m2 are the masses, and r is the distance between their centers.
Gravitational Constant G
Gravitational Field
A region of space around a mass where another mass experiences a force of attraction
Gravitational Field Lines
Imaginary lines that represent the direction of gravitational force; they point towards the center of the mass creating the field and never cross
Gravitational Field Strength (g)
The force per unit mass experienced by a mass in a gravitational field
Equation for Gravitational Field Strength near Earth
How does distance affect gravitational field strength?
The strength of a gravitational field weakens in proportion to the square of the increase in distance from the mass creating the field.