Lecture 5 Flashcards

1
Q

what did tycho Brahe do

A

combined copernican and geocentric model with sun orbiting earth, planets orbit sun
showed supernovae appeared beyond moon
most accurate star and planetary table ever made

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2
Q

what did Kepler do

A

realised you could throw away the assumption of circular motion, found simpler models that explained observations accurately

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3
Q

what are Keplers laws

A

planets orbit in an ellipse with the sun at one focus

sun-planet line sweeps out area at a constant rate

square of a planets orbital period is proportional to the cube of the length of the semi-major axis of its orbit

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4
Q

what was newtons explanation for Keplers laws

A

same law of gravity applies on stars

when this is combined with newtons 3 laws, it predicts Keplers laws

speculated stars were like the sun and had their own planets

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5
Q

impact of newtons explanations

A

unified terrestrial and celestial mechanics

accurate enough for terrestrial purposes like navigation

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6
Q

what are the 1760s transits of Venus

A

venus passes infront of the sun rarely due to orbit angle, happens in pairs 8 years apart
in 1761&69, time of transit from different locations was measured and distance calculated within 1% accuracy

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7
Q

what happened in 1780’s-1900s to do with the models of the universe

A

nature and matter of stars was established, confirmed stars were sun like, established basic distances to nearby stars

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8
Q

what is the base for all modern cosmology

A

Einsteins special relativity and general relativity

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9
Q

what is special relativity

A

laws of physics, particularly electricity and magnetism, are the same in any non-accelerating situation, regardless of speed

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10
Q

what is general relativity

A

cannot distinguish free-falling under gravity from being weightless a long way from any gravity

matter tells space how to curve, space tells matter how to move

as a metric, GR describes structure of space time within GR, tells you the length of a journey along any path through space and time

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11
Q

what is the FLRW metric

A

metric for matter density constant throughout space
defined by an overall curvature, K, of space and a scalling of time as it passes

current model for the universe on large scales

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12
Q

what is the great debate

A

were spiral nebulae (galaxies)
clouds within Milky Way (Shapley)
or
distant galaxies about the same size as the MW (Curtis)

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13
Q

great debate main arguments for Curtis

A
  • why would there be as many novae in one tiny cloud as in the rest of the Milky Way
  • dark lanes in the nebulae look like dust in the MW
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14
Q

great debate main arguments for Shapley

A

pinwheel galaxy had been observed to rotate over the course of years if it was as big of the Milky Way, would have rotated faster

Andromeda would have to be very far away to be the size of the Milky Way

one nova in Andromeda outshone the rest of it, how could one star be brighter than billions of others

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15
Q

how are distances measured beyond the Milky Way

A

standard candles

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16
Q

what are cepheids

A

young bright star type found to pulsate
brightness and radius changes over days to months

relationship between brightness and period found by leavitt

17
Q

what did Hubble observe and measure

A

individual stars in Andromeda and other galaxies
found cepheids

measured period, absolute luminosity thus distance