AST201 Week 1

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36 Terms

1
solar system
our solar system is made up of the sun, planets, and their moons, rockey asteriods and icy comets
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2
galaxy clusters
groups of galaxies with many more large members
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3
astronomical unit (AU)
earths average distance from the sun
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4
light year (LY)
the distance that light can travel in 1 year, about 10 trillion km
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5
age of the universe
14 billion years
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6
big bang
where the expansion of the universe began, most galaxies including our own milky way formed within a few billion years after
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7
star birth
when gravity compresses the material in a cloud to the point at which the centre becomes dense enough and hot enough to generate energy by nuclear fusion
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8
star life cycle
it ā€˜livesā€™ as long as it can shine with energy from fusion, and ā€˜diesā€™ when it exhausts its useable fuel
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9
supernova
when a massive star dies, it throws it energy back out into space
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10
chemical elements in early universe
hydrogen and helium (trace of lithium)
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11
earths orbit speed
average speed of 100,000 km/hr
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12
axis tilt
almost directly at the North Star
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13
constellation speed
incredibly slow speed, but over time will be unrecognizable and they previously have been shaped differently as well
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14
dark matter
matter which is completely invisible to our telescopes
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15
dark energy
the expansion of the universe is getting faster with time, this means there is some invisible energy that is a lot of the unvierse
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16
galaxies
galaxies
all smudges are galaxies
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17
looking out is looking back
when you look up at the sky you are looking back in time
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18
contents of the universe (1920s)
most (99.9%) is stars, galaxies, planets, gas, dust, etc
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19
fritz zwicky (1898 - 1974)
started looking at clusters of galaxies, idea of ā€œmissing massā€
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20
vera rubin (1928 - 2016)
measure how fast a galaxy spins
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21
milky way galaxy spin
takes 100 million years to rotate once
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22
original observation of galaxy rotation speed
original observation of galaxy rotation speed
the further from the center of the galaxy, the slower the orbital speed
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23
vera rubinā€™s observation of galaxy rotation speed
vera rubinā€™s observation of galaxy rotation speed
the further from the center of the galaxy, the faster the orbital speed, mass is concentrated on the outside and is invisible
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24
contents of the universe (1980s - 1990s)
most (95%) is invisible dark matter, little (5%) is stars, galaxies, planets, gas, dust etc
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25
contents of the universe (2023)
normal matter = 4.9%, dark matter = 26.6%, dark energy = 68.5%
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26
relativity
we can only measure motion RELATIVE to a given frame of reference
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27
speed of light
use the constant c, 300,000 km/s
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28
light around the earth
7\.5 times per second
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29
speed of light rules
light always travels at c, no object w/ mass can ever reach or exceed light speed
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30
speed of light in experiment
no matter how the experiment is done, all observers measure the same speed of light, the speed of light is the same in all frames of reference
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31
speed of the bowling ball
is different in different ā€œframes of referenceā€
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32
invariant
unchanging, the speed of light
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33
different frames of reference
different frames of reference
povs are different so they see time and lengths differently
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34
foundations of special relativity
  1. we can only measure speeds of objects relative to one another

  2. the speed of light is invariant

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35
time dilation
if someone is moving relative to you, their clock will appear to run slower to you
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36
length contraction
if someone is moving relative to you, their lengths will all appear shorter to you
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