Formulas & Constants for “A
Classical & Relativistic Trip to a Black Hole”
constant |
symbol |
value |
speed of light |
c |
3.00 X 108 m/s |
gravitational constant |
G |
6.67 X 10-11 Nm2/kg2 |
mass of Earth |
Me |
5.98 X 1024 kg |
radius of Earth |
Re |
6.37 X 106 kg |
acceleration due to gravity on Earth |
g |
9.81 m/s2 |
equivalencies |
||
1 m3 = 106 cm3 |
||
1 light year = 9.46 X 1015 m |
quantity |
symbol |
unit |
equation |
notes |
velocity |
v |
m/s |
v = d/t |
d = distance, t =
time |
acceleration |
a |
m/s2 |
a = Dv/t |
rate at which
velocity changes (Dv = vf - vi) |
net force |
F |
N |
F = ma |
Newton’s 2nd
law, m=mass in kg |
volume of a sphere |
V |
m3 |
V = 4/3pr3 |
r is the radius |
density |
D |
kg/m3 |
D = M/V |
mass per unit volume |
centripetal force |
Fc |
N |
Fc = mv2/r |
force that keeps an object in a circular path, directed towards the center of the circle |
period of object in circular motion |
T |
s |
T = 2pr/v |
time to go around the circle (orbit) once |
gravitational force between two objects |
FG |
N |
FG = GmM/r2 |
G = gravitational
constant, m = mass of small object, M = mass of large object, r = distance between their centers |
escape velocity |
vesc |
m/s |
= sqrt(2GM/R) |
Escape velocity
is the minimum speed to escape an object’s (planet’s or star’s, etc) gravitational
field where G = gravitational const., M = mass of object, R = radius of object |
Special relativity (time dilation at high velocities) |
Dt |
s |
Dt = Dto/sqrt[1-(v/c)2] |
Dto = change in
time from perspective that sees events occur in same place, Dt = change in time from
perspective that sees events occur in different places, v = velocity, c = speed of
light |