Orbits and The Wider Universe Flashcards

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1
Q

Kepler’s First Law

A

Each planet moves in an ellipse with the sun at one focus

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2
Q

Kepler’s Second law

A

The line joining a planet to the center of the sun sweeps out equal areas in equal times

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3
Q

Kepler’s Third Law

A

The square of the period, of the planets orbital motion is proportional to the orbital radius cubed

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4
Q

Explain how we know dark matter exists

A

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

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5
Q

When using Kepler’s third law, what is something that we assume

A

We assume that a small mass is orbiting a larger mass

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6
Q

What are three that we can infer about a system where two masses orbit a center of mass

A
  1. The center of mass must be in line with the two masses
  2. The center of mass must be between the objects, as centripetal acceleration must be towards it
  3. The angular velocities of the objects must be identical
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7
Q

If a star/galaxy is moving towards us what happens to the wavelength

A

It decreases, this is known as blue shift

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8
Q

If a star/galaxy is moving away from us what happens to the wavelength

A

It increases, this is known as red shift

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9
Q

Radial velocity, in Doppler shift equation

A

The component of the objects velocity along the line joining the observer to the object

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10
Q

What is the equation for Doppler shift in words

A

Delta lambda over lambda = radial velocity over the speed of light

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11
Q

Radial Velocity, When related to the Doppler shift equation

A

The Radial velocity is the component of the objects velocity along the line joining the observer to the object

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12
Q

What did Hubble notice with the red shift from stars and galaxies

A

That the redshift of the stars and galaxies was greater the further from earth they were.

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13
Q

What is the equation taken from the graph Hubble created using data from redshift of galaxies

A

Hubble’s constant = Velocity over distance

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14
Q

Hubble’s law

A

The speed of the recession of a galaxy is directly proportional to its distance from the earth

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15
Q

What is the value of Hubble’s constant

A

2.2x10^-18s^-1

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16
Q

What does Hubble’s constant give a measure of

A

The expansion rate of the universe, how fast objects appear to be moving away from our galaxy as a function of distance

17
Q

What do we have to assume about radial velocity of galaxies to calculate the age of the universe

A

That the radial velocity has been constant since the beginning of the universe

18
Q

What is the equation for the age of the universe

A

1 over Hubble’s constant

19
Q

What are the two problems with Hubble’s constant

A
  1. Uncertainty in the value, since it is determined using redshift and distance to the stars.
  2. The assumption that the radial velocity of the galaxies has been constant
20
Q

What are the three fates of the universe

A

Open
Close
Flat

21
Q

Describe and open Universe, in terms of denisty

A

It is where the density of the universe is less than the critical density, so the universe will always expand

22
Q

Describe a closed universe in terms of density

A

It is where the density of the universe is greater than the critical density, so the universe will eventually stop expanding and collapse back in on itself.

23
Q

What is the equation used for critical density with Hubble’s law in

A

Critical Density = (3 x Hubble’s constant squared) over ( 8 times pi times the gravitational constant)

24
Q

What is the value of the gravitational constant

A

6.67x10^-11 Nm^2Kg^-2

25
Q

Critical Density

A

The average density of matter required for the universe to just halt its expansion, but only after an infinite time

26
Q

Red shift is … earth

A

away from

27
Q

Blue shift is … earth

A

towards