20 Flashcards

1
Q

Define light year

A

The distance travelled by light in a vacuum in one year.

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2
Q

Define the AU

A

Astronomical unit . The average (cos elliptical) distance from Earth to sun.

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3
Q

Define a parsec (pc)

A

The distance at which a radius of 1AU subtends an angle of 1 arcsecond

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4
Q

What is stellar parallax?

A

The apparent shift in the position of an object relative to a background of distant objects

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5
Q

Why is it not accurate to Measure distances above 100pc

A

Angießen are so small they are not accurate to measure

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6
Q

What is the formula for using parallax to calculate distance ?

A
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7
Q

What is the cosmological principle?

A

Universe is isotopic and homogeneous and the law of physics are universal. Isotropic means same in all directions to every observer, no centre/edge. Homogeneous means that matter is uniformly distributed- density is the same throughout

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8
Q

What is the Doppler Effect?

A

The apparent shift in wavelength occurring when the source of waves is moving

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9
Q

What is the Doppler equation?

A
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10
Q

What is Hubbles law?

A

The recessional velocity v of a galaxy is proportional to its distance from Earth. The further away a star is from Earth, the a faster it is moving from us

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11
Q

How does Hubbles law provide evidence that the universe is expanding?

A

Most light from distant galaxies is red shifted, showing that galaxies are moving away from Earth, this suggested that space and time is expanding

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12
Q

What is the big bag theory?

A

All objects were initially contained in singularity, which suddenly expanded outwards

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13
Q

What are the two pieces of evidence for big bang theory?

A

CMBR (cosmic microwave background radiation): gamma wavelength expanded to now be in microwave region
Hubbles law : red shift of distant galaxies

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14
Q

What explains why acceleration of universe “outwards” has sped up recently?

A

Acceleration needs a source of energy, aka dark energy which hasn’t been detected (68% of universe)

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15
Q

Explain reasoning behind this

A

Predicted to be decreasing as distance from centre of galaxy increases and so velocity decreases.

Explanation: mass of galaxy not concentrated in the centre

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16
Q

Light from a distant galaxy is red shifted. Suggest how by measuring the red shift of different parts of the galaxy , astronomers can determine the speed of rotation of the galaxy

A

Each side of rotating galaxy will have a different relative velocity and so a different red shift. The side rotating away from us will have a greater velocity (and so greater red shift) than the side rotating towards us.. using Doppler equations the relative velocity of each side can be calculated. The differences in these relative velocities can be used to determine the speed of rotation

17
Q

What was the nature of universe (10^-34)?

A

Temp= 10^28
Only EM radiation existed (gamma)
Acceleration (inflation)

18
Q

What was nature of universe (10^-6)?

A

First particles gain mass

19
Q

What was the nature of universe (1s)

A

Creation of matter stops after about 1s once temperature has dropped to 10^9K

20
Q

what are some charactertistics of black holes?

A
  • escape velocity > c
  • absorbs all light/ doesnt emit
  • infinte
21
Q

why do measurements deviate of nearby galaxies deviate for hubbles constant?

A

strong gravitational force between nearby galaxies affects motion

22
Q

why do measurements deviate of far away galaxies deviate for hubbles constant?

A

expansion rate may not be linear coz of dark matter distribution