specification points Flashcards
what is the first law of thermodynamics
the change of internal energy of the object = the total energy transfer due to work done and heating
what is the temperature of absolute zero in celcius
-273 ℃
what is the work done by an ideal gas equal to
pΔV
what is molar mass equal to
the mass of 1 mol of the substance
what is brownian motion and how can it be observed
the random motion of a particle as a result of collisions with surrounding gaseous molecules.
can be observed in smoke particles under a microsope
boyles law and an equation for it
pressure is inversely proportional to volume
P₁V₁=P₂V₂
charles law and an equation for it
volume occupied by a fixed amount of gas is directly proportional to its absolute temperature, if the pressure remains constant.
V₁/T₁=V₂/T₂
pressure law (gay-lussac) an equation for it
pressure of a given mass of gas is directly proportional to the absolute temperature of the gas, when the volume is kept constant.
P₁/T₁=P₂/T₂
what are the 5 assumptions of the kinetic theory model
1: molecules move in random motion
2: they do not attract eachother
3: volume of each molecule is negligible compared with the volume of the gas
4: the collisions with eachother and the container are elestic collisions
5: each collision with the container surface is of much shorter duration than the time between impacts
what are the simalarities between electrostatic and gravitational forces
both have inverse square laws of force
field lines, use of potential concept, equipotential surfaces etc
what are the differences between electrostatic and gravitational forces
masses always attract, but charges may attract or repel
gravitational potential definition
the gravitational potential, V, at a point is the work done per unit mass to move a small object from infinity to that point
what is an equipotential
a line or surface in a field along which the electric or gravitational potential is constant
graphical representation of g against r
graphical representation of v against r
what is the area under a graph of g against r
ΔV
derive keplers third law T² ∝ r³
start with GM/r² = V²/r
uses speed = distance/time
arrives at r³/T² = GM/4𝜋²
what is the equation for escape velocity
Vesc = √2GM/R = √2gR
what is the equation for the energy of a satelite in circular orbit of radius r
(and derive it lmao get fukt)
E = -(GMm/2r)
what is geostationary orbit
orbits at a fixed position relative to the planet and at the same time period of the planet