gravitational (everything) Flashcards
what is a force field
a region where an object will experince a non-contact force
force fields can be represented as ______
vectors
in uniform feilds the field strenth is ______ and the field lines are _____
in radial feilds the lines ____ __ ____ _____. and gravitatinal field is ___ ______
uniform, parallel
meet at the center, not uniform
newtons law of gravitation formula
Therefore F∝
F=GMm/r^2
inversly preportinal to r^2
F∝1/r^2
g equation if we assume g is constent (uniform fields)
g equation of we assue g is not constent (radial fields)
unit for both
g = F/M
g=GM/r^2
Nkg^-1
what value is the gravitational constent G
6.67x10^-11 Nm^2Kg^-2
gravitatinal potential (v) (simple defonition) is …..
(Double check)
potential enegy per unit mass
gravitatinal potential equation and unit
V=-GM/r
JKg^-1
gravitatinal potential enegy is what times gravitatinal potential
(show this in equation)
times m (mass of second object)
gravitatinal potential V = -GM/r
gravitatinal potential enegy =GMm/r
gravitatinal potential is 0 at ____
∞
What is gravitational field stength in terms of gravitational potential and distance from centre of mass
give the equation for this
Draw this graph (v over r graph)
The graidient is….
force per unit mass
(use this one on most cases unless the question heavaly talks about gravitatinal potential)
OR
the rate of change of gravitational potential (v) over distence r from center of mass
g=-ΔV/Δr
See pg 122
Gradient = g
draw g over r graph. what is the area
see pg 122
area = ΔV
excape velocity is when…
thereofre derive velocity for needed for the excape velocity
at wich the objects Ek = - gravitatinal potential enegy
1/2 mv^2 = - - GMm/r
1/2 v^2 = GM/r
V^2 = 2GM/r
V = root2GM/r
gravitatinal potential diffrence is…
thereofre
give the equation for work done to move a mass between 2 points in a gravitatinal feild
the enegy neded to move a unit of mass between 2 points in a gravitaional field
(the diffrence in gravitatinal potential bewteen the 2 ponts)
ΔWd=mΔV
when you travel along a equapotantial you dont ____ or _____ ______
lose or gain enegy
derive the fact T^2 ∝ r^3 of an object in orbit
F=GMm/r^2 F=mv^2/r
centrepetal force = centrepetal foce
F=F
GMm/r^2=mv^2/r
1/r=mv^2/GMm
r=GM/v^2
v^2=GM/r
v=rootGM/r
s=d/t
d=2πr
t=T
s=2πr/T
s=v
2πr/T=rootGM/r
4π^2r^2/T=GM/r
1/T=GM/4π^2r^3
T=4π^2r^3/GM
all constent exept T and r
therefore
T^2∝r^3
orbating objects have constent total enegy consisting of __ + ____ _____
since total enegy is constent if potential enegy decreases (distence from mass (r) becomes smaller) then __ _______ meaning _____ ______
Ek + potantial enegy
Ek incresease, velocity increases
geosationary orbat
distence form earths center
and
time preied
42000km
24hours
LEO
distence from earth
below 2000Km
ΔEk=
(For an object in orbit with constant total energy)
ΔGPE
exam question (2mark):
define the gravitatinal potential enegy at a point in the gravitatianl feild
gravitatinal potential is the word done per a unit mass moving a unit mass from from ∞ to that point
some characteristics of lower poler orbit (3)
- orbiting height is low (below 2000Km)
thereofre lower signal strenth requierd - can collect data from regions inexessible to man
- contact with revever is intemitent
some characteristics of geosyncrinyis orbat above equator (4)
-maintains same position reletive to earth (T=24hours)obit
- hight is high (42000Km)
- sacns a resticted and fixed area of the earth only
- arial can be in a fixed position
exam question (2mark):
define gravitational feild strenth and define weather it is a vector or a scaler
- g is force per unit mass
- g is a vector quantity
exam question (1mark):
state what is represented by gravitaional field lines
they show the direction of force and the reletive magnatude a mass will experince within a gravitational field
equapotential lines cross…
field lines at 90 degrees
what is the Ek of an object in orbit?
(extra equation tutur said is hlpfull to rember)
Ek=GMm/2R
for an object within a circular obit:
(not a needed derivation but may help):
V(velocity) ∝ (includes r)
derive it
1/root r
F=F
mv^2/r=GMm/r^2
v^2=GM/r
v=rootGM/r
therefore
v=root1/r