final Flashcards

1
Q

how many stars in our galaxy

A

100 billion

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2
Q

universe hierarchy

A

solar system
milky way
local group
(virgo) local supercluster

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3
Q

how many galaxies in observable universe

A

100 billion

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4
Q

distance to sun

A

8 light min

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5
Q

distance to closest star (and name)

A

alpha centuri
3 years

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6
Q

closest galaxy and name

A

andromeda
2.5 million years

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7
Q

radius of observable universe

A

14 billion years

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8
Q

when in the year is does milky way form

A

feb

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9
Q

when in year does earth form

A

sept 3

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10
Q

when does life begin on earth

A

sept 22

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11
Q

what is science

A

questions, evidence, experiments, trial and error

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12
Q

what was the ancient model of the universe

A
  • geocentric
  • heavens are perfect
  • everything orbits the earth
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13
Q

ptolemys model of universe

A

same as greeks but with epicycles due to retrograde of mars

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14
Q

copernican model

A

sun centred model

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15
Q

keplers 3 laws

A

1) planets orbit sun in elliptical path with sun at focus
2) planet sweeps out equal area of ellipse in equal time
3) P^2 = a^3

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16
Q

what did gelileo do

A

prove keplers ideas and thus proved heliocentric model

17
Q

how do we get info from universe

A
  • light
  • neutrinos
  • gravitational waves
18
Q

3 types of astronomical data

A
  • imaging
  • spectroscopy
  • time series
19
Q

what is imaging

A
  • detect pos and brightness of light
  • can tell us about shape, color, and brightness
20
Q

spectroscopy

A
  • intensity of light at different wavelengths or colors
  • tells about temp, composition, density
21
Q

time series

A
  • change of intensity of light, or change in position
22
Q

what is a atom made of

A

-elec, prot, neutrons
- most mass is in nucleus

23
Q

absorbtion of light

A
  • atom jumps up level as it gained energy
  • look at cloud of gas directly in front of source
24
Q

emission of light

A

spontanius
- electron fall a level as it lost energy
- look at cloud of gas from the side

25
chemical fingerprint
we can look at star and see the absorbtion/emission lines to see the composition of the surface. it also lets us mesure the speed of the object with doppler shift
26
refracting telescope
- has a lens that collects light - light is focused to the focal point - light then goes to eyepiece
27
reflecting telescope
- a concave mirror that focuses light to a mirror that directs it to the eye peice
28
2 most important properties of telescope
- light collecting power - angular resolution
29
what is light collecting power
- depends on area of mirror/lens - makes image more clear
30
what is angular resolution
- depends on diameter of mirror/lens and wl of observation - is the smallest detail you can resolve
31
what is interometry / apreature synthesis
linking telescopes to mimic a large angular resolution (largest speration between dishes)
32
why put telescopes in space
to prevent atmospheric blurring, only needed for xray, uv, gamma, ir
33
what is adaptive optics
deform mirror to compensate for distortion of the atmosphere, by using laser and reference star