Orbits and the Wider Universe 4.3 Flashcards
define Kepler 1st law?
The orbit of a planet is an ellipse with the Sun at one focus.
Define Kepler 2nd law?
The line joining the planet to the sun sweeps out equal areas in equal intervals of time.
Define Kepler 3rd Law?
The square of the period (T) of the orbit is proportional to the cube of the semi-major axis (a) of its orbit.
(T^2 directly proportional to a^3)
relateing to any elliptical orbit.
T^2 = 4 pi^2a^3/GM
Energy of an object in elliptical orbit equation?
E = -1/2 GMm/a
finding speed for any circular orbit.
V^2 = GM/r
define a rotation curve?
a plot of orbital velocity against distance from the centre for an astronomical system.
Rotation curve has this simple form because?
- The Sun contains great bulk of mass in solar system.
- The Solar System objects outside the sun
- The Sun is almost spherically symmetrical.
Define Nonbaryonic matter?
matter which is not composed of quarks + leptons but interacts with the gravitational force.
(Main component of dark matter. )
Define radial velocity?
component of its velocity relative to an observer on earth.
How is the position of the centre of mass calculated for 2 small objects?
M1R1 = M2R2
M = mass
R = Radius
define a exoplanet?
a planet which orbits a star other than the sun.What
What does Hubble’s law state?
Recession Velocity of deep space objects is proportional to their proper distance.
Hubble’s law equation?
v = HD
v = velocity
H = hubbles constant
D = Distance
The Hubble time?
estimate of the age of the universe and is defined as the reciprocal of the Hubble constant.