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Astronomy test 1

Olivia Gniadek Astronomy Tertiary English 116 cards

Cards in this deck (116)

  1. 1What are planetsWanderers of the solar system
  2. 2What is the increasing scale of the objects in the universegalaxies-stars-planets
  3. 3what are starsour sun is powered by thermonuclear fusion
  4. 4what is a nebulaeclouds of glowing gas
    birthplaces of stars
  5. 5what are supernovaespectacular detonations at the end of lives of some stars
    may lead to pulsars, neutron stars and black holes
  6. 6How many stars are in our milky way?approx 200 billion
  7. 7what are the different galaxy typesspiral
    elliptical
    irregular
  8. 8What are the exotic galaxies with powerful sources of radiationActive galactic nuclei
  9. 9what is cosmologycreation and fate of the universe
  10. 10how fast is the speed of light300,000 km/sec
  11. 11what is one light yearmeasure of distance that travelled by light in a vacuum in one year
    approx 10 to the 16th
    written with a c symbol
  12. 12What is an astronomical unitlength of the semi-major axis of Earth's orbit around sun
    approx 8 light minutes for suns light to reach earth
    Distance from sun to earth
  13. 13what does star colour depend onrange of wavelengths emitted
    i.e. the spectrum
  14. 14what is a parseca unit of distance used in astronomy, equal to about 3.26 light years
  15. 15what is the parallax methodSimply put, they measure a star's apparent movement against the background of more distant stars as Earth revolves around the sun
  16. 16what is the radius of the milky way50,000 light years
  17. 17how long does it take for the earth to rotate on its axis23 hours and 56 minutes
  18. 18How long does it take for the earth to orbit the sun365 1/4 days
  19. 19What is the tilt of the earth23 1/2º
  20. 20What is the ecliptic planea plane in space defined by the earth's orbit around the sun
  21. 21where do the zodiacs originate fromplanets pass through them at different times during the year
  22. 22what causes the seasonsdue to axis tilt, as earth orbits the sun is in different parts of the world will get more sun then the other
    i.e. NH summer in June
    SH summer in December
  23. 23what does perihelion meanclosest point to the sun
  24. 24what does aphelion meanfarthest point away from the sun
  25. 25How many constellations are there88 constellation
    i.e. Cygnus, Orion, Ursa Major, Southern Cross (Crux)
  26. 26What way do stars rotate around the southern celestial poleclockwise
  27. 27Why are there latin names for constellations in the southern hemisphereconstellation names are due to the modern explorers
  28. 28Do constellations vary in different religionsyes
    Indigenous Australians form constellations by using stars and the dark parts of the milky way
  29. 29How long does it take for the milky way to turn on its axis150 million years
  30. 30what is the constellation star brightness defined bybrightness
  31. 31do constellations change during the year? if yes how early do they riseyes they do due to earth's orbit around the sun
    constellations rise 4 minutes earlier than previous night
  32. 32What is one solar daytime interval between one noon and the next
  33. 33What is a sidereal daytime taken for one rotation of the earth on its axis
  34. 34what is the difference between a sidereal day and a solar daysidereal = 23 hours and 56 mins
    solar day = 24 hours
  35. 35does a solar day change during the yearyes due to the earth's orbit being elliptical
  36. 36What is a sidereal monthtime taken for moon to return to original spot in the sky = 27.3 days
  37. 37What is a synodic monththe time between successive new moons = 29.5 days
    caused by motion of earth around the sun
  38. 38Why can't stars be seen during the daysun's light scatters atmosphere therefore making it too hard for starlight to penetrate atmosphere during the day
  39. 39In several billion years, how long will it take for the moon to orbit earth60 days
  40. 40what is the bright thing around the sun during an eclipse and how hot is itcorona
    1,000º K
  41. 41what occurs during a lunar eclipsemoon is lost in shadow of earth
    may be full/ partial depending if it passes through umbra or penumbra
    can last 1.5 hours
    path of moon and earth is inclined 5º therefore moon is either below or above shadow
  42. 42what makes a blood moonearth's atmosphere scatters suns light effectively
    when viewing blood moon from moon, earth blocks out sun and around rim of earth there is a reddish glow which is reflected onto the moon, hence BLOOD MOON
  43. 43What happens at solar eclipsesmoon is situated between the earth and the sun
    moon shadow is small on the earth, so area of total eclipse (umbra) is small
  44. 44where are the biggest telescopes situatedat high altitudes e.g. chile and the himalayas
  45. 45who invented the refractorGalileo Gallilei
  46. 46Who invented the reflectorIsaac Newton
    Hence newtonian telescope
  47. 47can light be brought to a focus? by what instrument and in what formyes by a telescope
    can be achieved by a lens or a curved mirror
  48. 48what does wave nature of light cause and can it be resolved?Diffraction
    instead of point on the telescope, get pattern
    makes it difficult to resolve
  49. 49why can resolution be worse than diffraction limitpoor optical quality of telescope
    turbulent atmosphere
    at good sites, seeing imposes a resolution of about 1 arcsec
  50. 50what has caused people to put telescopes in spaceatmosphere is turbulent and dynamic
    not properly focusing
  51. 51what is a reflecting telescopefocus is produced by the objective mirror
  52. 52What is a cassegrainsecond mirror can be flat but is usually curved to defocus
    more complicated to use
    celestron and Meade telescopes are cassegrains
  53. 53how can turbulence affect the telescope's imagechanges path of light rays from stars in small amounts
    increases size of object
    imposes resolution limits of 1 arcsecond
  54. 54How can you track starsalt-azimuth or an equatorial mount
  55. 55What is an alt-azimuth mountsimplest to set up
    adjust both axis (earth rotates on these axis)
    ok with 2 computer controlled motors
  56. 56What is an equatorial mountone axis parallel with earth's axis
    one motor needed
    running at constant speed to track star
    tilts telescope to earth's latitude
  57. 57why are the dishes used for radio astronomy so big?radio signals are weak
    with many dishes approx 100 m apart, the resolutionary power is stronger
  58. 58How are the northern lights formedsolar particle charges funnel towards the Earth's north and south poles
    hit earth's atmospheric gases i.e. H, O2, N
    particles excite atmosphere
    colours come from different gases
  59. 59What is the bright part of the sun defined byphotosphere is one of the suns outer layers that emits most of the light
    site of sunspots
    thin layer ~500 km thick
  60. 60What are the other layers of the sunchromosphere and the corona
    only visible during eclipses
  61. 61how far can the corona of the sun extend to10 million kms
  62. 62how far can solar wind extend tofurther than the corona
  63. 63How big is the suns diameter100 x bigger than the earth's
  64. 64What is Kepler's third lawsemi-major axis of planetary orbit; a
    Roughly, a is the average distance between planet and sun
    period P of orbit (time taken for one orbit)
    law can be used for anything gravity related
  65. 65What do star colours determinesurface temperature of star
  66. 66How hot is the surface of the photosphere5800K
  67. 67what is the difference between kelvin and celciussame as celcius but with an offset of 0
    0K = -273ºC
    i.e. the suns surface temp is about 5500ºC
  68. 68How much energy does the sun put out every second1000 Joules per second
  69. 69what is the density of the sun1.4 grams per cubic cm
    same density as jupiter or 1.4 times the density of water
  70. 70what is a blackbody theoryone for which we can relate the temp and colour exactly thru simple expressions
  71. 71What is the red and blue colour associated with in terms of star colourRed is cool planet
    Blue is hot planet
  72. 72what is Einsteins special theory of relativityE=mc2
    E = Energy
    M = Mass
    C = Speed of light
  73. 73The Sun's surface is made of granules, how big are they and what is their lifespan?1000 km across
    10 min lifespan
  74. 74what are sunspotsdark spots in photosphere. central dark core (umbra) surrounded by a less dark border (penumbra)
  75. 75Why are sunspots darkthey're cooler
  76. 76How was it discovered that sunspots movethe Chinese 2000 years ago observed that the sun was rotating and sunspots were seen to move
  77. 77how long is a solar rotation period4 weeks
    depends on solar latitude
  78. 78does the sun rotate at quickly at different latitudesequatorial region spins faster than polar regions
  79. 79where do sunspots appear mostlatitudes +30 and -30
  80. 80how strong are sunspot magnetic fields10,000 times stronger than suns magnetic field
  81. 81what causes sunspotsas the equator moves faster than the poles wrapping of magnetic field process causes polarity of the sun's magnetic field to flip every 11 years
    loops of tangled magnetic field rise through the surface
  82. 82what is apparent magnitudehow bright does a star appear to be from earth
  83. 83what is magnitude 1the brightest star in the sky
  84. 84What is magnitude 6the dimmest star in the sky
  85. 85how much brightness results in the difference of 5 magnitudes100
  86. 86apparent magnitude be defined by using different filters, what are the three filters and how much magnitude do they showU filters = 300 - 400nm (UV)
    B filter = 400 - 500nm (Blue light)
    V filter = 500 - 600nm (visible, green-red)
  87. 87what is apparent magnitudehow bright stars appear on earth
  88. 88what is luminositytotal radiation emitted by a star in all directions
  89. 89what is absolute magnitudeapparent magnitude that a star would have if it were at a standard distance of 10 parsecs
  90. 90What is a binary star systemtwo stars orbit around a centre of mass
  91. 91what is Wein's Lawmeasure temperature of a blackbody (star) by colour
    is more sophisticated when using a spectroscope
  92. 92what is a spectroscopecontains a prism to split light up into component wavelengths
  93. 93What element is most predominant in starsHydrogen
    75%
  94. 94What is the Harvard classification system for starsOh
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  95. 95what is the main sequence for starsa diagonal band across Hertzsprung diagram from hot, bluish, bright stars on the top left to cool, dim, reddish stars in the bottom right
    stars have sizes about the same as sun
  96. 96What is a red giantboth bright and cool
    have sizes about 10-100 times that of sun
  97. 97what is a super giantrare, bigger and brighter than red giants
    e.g. betelgeuse
  98. 98what is a white dwarfhot and dim star
    similar size to earth
  99. 99What is a star embryo calledprotostars
    shockwaves due to supernovas contract regions of nebulas which give birth to stars
  100. 100how hot is a protostar10 million K
    sufficient to start fusion which makes a protostar a star which joins main sequence
  101. 101how long is a stars life10 to the 10 years
  102. 102what is a H2 regionionised Hydrogen gas in nebulae
  103. 103What is a H1 regionWhen nebulas have 1 proton and electron
  104. 104what is the future of the sunlive for another 5 billion years
    in 5 billion years the sun will be twice as luminous as present
    will swell to 100 times its current diameter
    earth destroyed by radiation
  105. 105why are larger mass stars so specialHigher core temperatures
    fusion rate strong
    hot enough to fuse hydrogen
    luminosity is strong
  106. 106how do stars transition to red giantshydrogen in star is exhausted
    starved of heat source
    gravity wins
    no balance between thermal pressure outwards and gravity inwards
    core heats up
    hydrogen shell burning
  107. 107How can you determine if a star is dead on a globular cluster graphhave moved away from turn off point
  108. 108How does a star become a Red giantdepends on mass
    low-medium stars turn into white dwarfs
    high mass stars turn into supernovas
  109. 109What is the evolution of a low-medium mass starhelium burning exhausted at core
    core composed of oxygen and carbon contracts
    contraction leads to heating of core
    core is hotter than usual
    helium shell burning around core
  110. 110low-medium mass star continuationstar expands in size
    red giant forms
    radius is size of earth's orbit
    have short lives
    unstable
    layers cool and become opaque
    radiation from inside strips outer layers
  111. 111what does a low-medium mass star formplanetary nebula
  112. 112how many planetary nebulas are there20,000 - 50,000
    short lived phenomenon
  113. 113what is the radius and density of a white dwarfradius of earth
    10 to the 6th g/cm3
  114. 114what are the main star fuelshydrogen
    helium
    carbon
    oxygen
    neon
    silicon
  115. 115what does a star end up withiron core surrounded by shells of fusing material
    iron core contracts under gravity
  116. 116What happens during a supernovainner regions of star fall towards core and bounce off
    outward shock waves blow star apart
    nuclear density core becomes neutron star
    (or core can be destroyed)
    black hole forms in extreme cases

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Tertiary Astronomy Flashcards on Astronomy test 1, created by Olivia Gniadek on 20/08/2018.
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Olivia Gniadek
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astronomyadelaide university
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