Orbits and The Wider Universe Flashcards
Kepler’s First Law
Each planet moves in an ellipse with the sun at one focus
Kepler’s Second law
The line joining a planet to the center of the sun sweeps out equal areas in equal times
Kepler’s Third Law
The square of the period, of the planets orbital motion is proportional to the orbital radius cubed
Explain how we know dark matter exists
The measured rotational velocity of stars further out from the center of the galaxy is higher than expected. This implies that the mass is greater than what we can see, this suggests dark matter exists
When using Kepler’s third law, what is something that we assume
We assume that a small mass is orbiting a larger mass
What are three that we can infer about a system where two masses orbit a center of mass
- The center of mass must be in line with the two masses
- The center of mass must be between the objects, as centripetal acceleration must be towards it
- The angular velocities of the objects must be identical
If a star/galaxy is moving towards us what happens to the wavelength
It decreases, this is known as blue shift
If a star/galaxy is moving away from us what happens to the wavelength
It increases, this is known as red shift
Radial velocity, in Doppler shift equation
The component of the objects velocity along the line joining the observer to the object
What is the equation for Doppler shift in words
Delta lambda over lambda = radial velocity over the speed of light
Radial Velocity, When related to the Doppler shift equation
The Radial velocity is the component of the objects velocity along the line joining the observer to the object
What did Hubble notice with the red shift from stars and galaxies
That the redshift of the stars and galaxies was greater the further from earth they were.
What is the equation taken from the graph Hubble created using data from redshift of galaxies
Hubble’s constant = Velocity over distance
Hubble’s law
The speed of the recession of a galaxy is directly proportional to its distance from the earth
What is the value of Hubble’s constant
2.2x10^-18s^-1