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Newton's Third Law
For every action, there is an equal and opposite reaction.
Ptolemy's Model
An astronomical model that assumed planets moved at constant speeds and required adjustments known as epicycles.
Newton's Second Law
The acceleration of an object is directly proportional to the net force applied and inversely proportional to its mass.
Velocity-time graph
The area under this graph represents displacement.
Kepler's First Law
States that planetary orbits are ellipses with the Sun at one focus.
Inertia
The property of an object to remain at rest or in uniform motion unless acted upon by an unbalanced force.
Gravitational force
The force that keeps planets in orbit around the Sun.
Free fall
When an object falls towards Earth, experiencing an acceleration of approximately 9.8 m/s².
Galileo's telescope
Allowed observations that contradicted Aristotle's claims that celestial bodies were perfect.
Eratosthenes
Measured Earth's circumference using the angles of shadows cast at different latitudes.
Circular orbit
An orbit that maintains a constant distance from the center, where the gravitational pull from the central body provides the necessary centripetal force.
Escape velocity
The minimum velocity an object requires to break free from a planet's gravitational attraction.
Momentum
The product of an object's mass and its velocity, which is conserved in the absence of external forces.
Orbital speed
The speed at which an object travels along its orbit, varying with distance from the central body.
Gravity assist
A technique used to gain speed by passing close to a massive body.
Weightlessness
The sensation experienced by astronauts in orbit as they are in free fall towards Earth.
Elliptical orbit
An oval-shaped path that a planet follows around the Sun, as described by Kepler's laws.
Mass and distance
Factors that affect the strength of gravitational attraction between two objects.
Air resistance
A force that opposes the motion of an object through the air, affecting falling objects.