Physics unit 4 definitions. (unfin)

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  • Created by: Phil
  • Created on: 10-04-13 19:26
Gravitational field strength
Gravitational force per unit mass at a point.
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Newton's law of universal gravitation
F=-Gm1m2/r^2
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internal Energy at absolute 0
Is at a minimum
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Average Ke of a molecule
E = 3/2kT
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Boyle's Law
Pressure is inversely proportional to volume for a fixed mass of gas at a const temp.
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Brownian motion
Shows gas molecules have rapid and random motion.
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Centipetal acceleration
a= V^2/r
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Centripetal Force
F=mv^2/r
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Simple harmonic motion
It's acceleration is always directed toward the equilibrium position and the acceleration is always proportional to it's displacement.
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SHM displacement.
X= A sin 2(Pi)ft or x=A cose2(pi)ft
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Forced oscillations
A periodic force is applied
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Light damping
There is an exponential decrease in amplitude over several oscillations.
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Critical damping
The mass retuns to rest in the shortest possible time without over shooting.
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Resonance
A periodic force is applied to a system at the same freq as it's natural frequency resulting in oscillations of max amp.
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Internal energy of a gas
If the sum of all the randomly dist kinetic and potential energies of all it's molecules.
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Specific heat capacity
The energy needed to change a temperature of 1kg of a substance by 1oC
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SHC formula
E=Mc(delta Pheta)
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Ideal gas law
pV = nRT or pV= NkT
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gas law
Sometimes used as p1V1/T1 = p2V2/T2
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Ideal gas (Assumptions)
The molecules make elastic collisions, there are no inter molecular forces.
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Newton's first law.
Every body remains in a state of rest or of uniform motion in a straight line (const velo) unless acted upon bu a resultant force.
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Newton's 2nd Law
The rate of change of a momentum of a body is proportional to the resultant force which acts on it and occurs in the direction of the force.
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Newton's third law
If Body A exerts a force on Body B, Then body B exerts an equal and oppo force on body A.
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Momentum
Mass x Velocity.
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Ft (Impulse)
Mu=Mv Change in momentum.
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The law (or principle) of Conservation of momentum
If no resultant force acts on a system of objects the TOTAL momentum (mass and velo) does not change.
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Elastic collisions.
Collisions where Ke is conserved.
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Geostationary Satellies
Orbit above a fixed point on the equator with a period of 24hrs.
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Kepler's third law.
T^2 ∝ R^3
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Temperatures in kelvin.
+273.15
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Mole
Contrained 6.02 * 10^23 particles
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Latent heat of Fusion
Energy needed to change the state of a solid to a liquid without a change in temperature.
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Latent heat of vaporisation.
The energy needed to change the state of a liquid to a gas without a change in temperature.
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Other cards in this set

Card 2

Front

F=-Gm1m2/r^2

Back

Newton's law of universal gravitation

Card 3

Front

Is at a minimum

Back

Preview of the back of card 3

Card 4

Front

E = 3/2kT

Back

Preview of the back of card 4

Card 5

Front

Pressure is inversely proportional to volume for a fixed mass of gas at a const temp.

Back

Preview of the back of card 5
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