20.1 - 20.5 Flashcards

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1
Q

what is the cosmological principle

A

the assumption that the universe is homogenous and isotropic when viewed on a large enough scale and the laws of physics are universal

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2
Q

what’s an astronomical unit

A

the mean distance from the earth to the sun

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3
Q

what’s a light year

A

the distance travelled by light in a vacuum in a time of one year

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4
Q

what’s a parsec

A

the distance at which a radius of one AU subtends an angle of one arcsecond

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5
Q

what is an arcminute

A

unit of an angle. 1° = 60 arcminutes

1 arcminute = 60 arcseconds

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6
Q

what is stellar parallax

A

a technique used to measure the distance of stars from the earth that are less than 100pc away by comparing their position with distance stars 6 months apart

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7
Q

what’s a parallax angle

A

the angle of the apparent shift in the position of a relatively close star against the backdrop of much more distant stars

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8
Q

what’s the doppler effect

A

the change in frequency and wavelength of waves received from an object moving relative to the observer compared to what would be observed without relative motion

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9
Q

define ‘blue-shifted’

A

the shortening of observed wavelengths when the source is moving towards the observer. (causes light to shift towards the blue end of the spectrum)

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10
Q

define ‘red-shifted’

A

the lengthening of observed wavelengths when the source is moving away from the observer. (causes light to shift towards the red end of the spectrum)

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11
Q

what’s the ‘big bang’

A

the theory that at a moment in the past all of the matter contained in the universe was in a singularity that expanded rapidly outwards

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12
Q

what’s Hubble’s law

A

the recessional speed of a galaxy is proportional to its distance from earth

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13
Q

what’s the ‘expanding universe’

A

the idea that the fabric of space and time is expanding in all directions. therefore any point in the universe is moving away from all other points.

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14
Q

define homogenous

A

uniform in terms of the distribution of matter across the universe when viewed on a large enough scale

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15
Q

define isotropic

A

the same in all positions. ( the universe appears the same to an observer regardless of their position)

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16
Q

what’s the microwave background radiation

A

the microwave signal of uniform intensity detected in all directions. it fits the profile for a black body at 2.7 kelvin

17
Q

what’s dark energy

A

a hypothetical form of energy that fills the universe explaining the accelerating expansion

18
Q

what’s dark matter

A

a hypothetical form of matter spread throughout galaxies that could explain the difference between actual and predicted velocities of stars. it doesn’t absorb or emit light