Gravitation
Gravitation
3. Conservative force g
h
GM gR2 R
r
Vo = =
4. Force between any two masses - d g = g [ 1-
l d
] Re (R+H) (R+H)
gl R
Gravitational force R
r
M
GM gR R
R
Force between earth and any other body - Vo = =
M Re R
Force of gravity FOUR EQUAL MASSES UNDER MUTUAL
-GMm -GMm
GRAVITATIONAL FORCE If orbit is closer to GM gR
W = (U f - Ui
(
= -
Vo = = R R+h
earth‛s surface( neglect ‘h‛) R
g dg Or, R
= g-g =
l
l GM Absolute decrease = (called minimum orbit, velocity-first cosmic velocity) W = mgh
V = (2 2+1) g R
R+h
VECTOR FORM 2 2 l Note - for easy calculations
F21 force on 2 due to 1 g g-gl d Work done to move object W =
mgR
y
l l 1 GM Fractional decrease = = = gR = 8 km/s or GM = 8 km/s = 8x 10 m/s to a height h = R 2
r12 vector from m1 to m2 V = g g R
3
R (2 2+1) R
r12
G m1m2 2 R d mgR
m1
m2
-r12 l Percentage decrease = g x100
GM Work done to move object W =
F21 = x100 = or = 64 x 106 3
r2 r122 T2 l3 Here R = g R R to a height h = R/2
l
r1 2
Very imp graph
G m1m2
x or - r12 The graphical representation of change in KE, PE OR TE FOR AN ORBITING
r123 WORK DONE IN MOVING OBJECT
Similarly the value of g‛ with height and depth SATELLITE
GRAVITY gl m,Vo FROM SURFACE TO CIRCULAR ORBIT
F12 force on 1 due to 2
GMm GMm h
Acceleration due to gravity GMe KE = U =-
G m1m2 G m1m2 2r r
r Vo
KE
The principle of superposition is valid here. g IN TERMS OF DENSITY OF EARTH TE
“Force on a particle due to a no. of particles distance
U
g=4 G Re g Re
GRAVITATION
is the resultant of forces due to individual
particles.” “If density is mentioned use the PHYSICS
above equation”
WALLAH