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4
|
an extremely dense, collapsed star, that nothing can escape from
|
7
|
sequence in a star's life where fusion begins; most stars are in this sequence
|
8
|
the theory of how our universe started as an extremely small, hot, dense state
|
9
|
sun grows about 100x its own size
|
10
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the theory that as something moves towards an object, the frequency of the wave produced increases
|
13
|
characteristics include shorter wavelength, higher energy, and higher temperature
|
15
|
a dead star, and a solid floating ball of carbon
|
18
|
a small, white, hot star that glows from leftover heat
|
21
|
sequence of a star where it either becomes a super giant or planetary nebula
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|
|
|
|
1
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the process of atoms being broken apart by adding neutrons to it
|
2
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characteristics include longer wavelength, lower energy, and lower temperature
|
3
|
the process of fusing atoms together under extreme heat, by smashing them into each other at extreme speeds
|
5
|
the highest part of a wavelength
|
6
|
the spectrum on which light is emitted
|
11
|
the amount of energy and noise produced by an energy wave
|
12
|
the lowest part of a wavelength
|
14
|
sequence where a star has just been formed from a nebula
|
16
|
the distance between 2 troughs or 2 crests
|
17
|
large clouds of gas and dust where stars are formed
|
19
|
used for night vision
|
20
|
used to see broken bones
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|
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