UNIT 3 Flashcards
Vector Impact
the velocity of a projectile immediately before striking the ground
Resolution
determining the components of a vector, usually at right angles to each other
Force
a push or pull between objects, which may cause one or both objects to change speed and/or the direction of their motion (i.e. accelerate) or change their shape
weight
a measure of the force of gravity acting on an object
Mass
an object’s resistance to a change in motion; also commonly stated as the amount of matter in an object (symbol: m; SI unit: kilogram; unit symbol: kg)
Friction
is the resistance to motion of two surfaces moving relative to another. It is the result of the electromagnetic attraction between the charged particles in two touching surfaces
uniform circular motion
the motion of an object travelling at a constant speed in a circle
centripetal force
the force acting on an object travelling in a circle that constantly acts on an object towards the centre of motion (symbol: Fc ; SI unit: newton; unit symbol: N)
centripetal acceleration
the acceleration experienced by any object moving in a circular path directed towards the centre of motion (symbol: ac; SI unit: metres per second squared; unit symbol: m s–2)
rotational speed
the number of revolutions an object does per second, as distinguished from the term ‘average speed’, which is the linear speed.
Newton’s law of universal gravitation
states that the force of attraction between each pair of point particles is directly proportional to the product of their masses and inversely proportional to the square of the distance between them
The first law of planetary motion (law of orbits)
states that all planets move about the Sun in elliptical orbits that have the Sun as one of the foci
Kepler’s second law of planetary motion (the law of areas)
states that a radius vector joining any planet to the Sun sweeps out equal areas in equal lengths of time.
The third law of planetary motion (law of periods)
states that the square of the sidereal periods of a planet is directly proportional to the cube of its mean distance from the Sun: T² ∝ r³.
Electric field
a region of space near an electrically charged particle or object within which a force would be exerted on other electrically charged particles or objects