Astro Study Buddy

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Jamie_Bee
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Astro Study Buddy
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2015-04-22 23:12:30
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An astronomy study buddy
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  1. Elliptical Galaxies
    • no disk
    • no spiral arms
    • almost no gas, dust or new stars forming
  2. Disk-shaped Galaxies
    • Usually have spiral arms, less or more prominent
    • generally large amounts of gas and dust
    • ongoing stellar formation
  3. Irregular Shaped Galaxies
    Gas, dust and star forming nebulae
  4. Largest Elliptical galaxies are called ______ are how big, and smallest elliptical galaxies are called ______, and how big
    • Giant, 5x bigger than Milky way
    • Dwarf, 1% diameter of Milky way
  5. Cosmological Distance Ladder from nearest to farthest
    • Nearby Stars = Parallx
    • Milky Way = Main Sequence Fitting
    • Nearby Galaxies = Cepheids
    • Galaxy Clusters = White Dwarf Supernovae, Tully Fisher relation
    • Everything else = Hubble's Law
  6. Parallax
    Apparent shift in a star's psition
  7. Main Sequence Fitting
    Apparent brightness of star cluster's main sequence tells us its distance
  8. Standard Candle/Bulb
    An object whose luminosity we can determine without measuring its distance
  9. What are Standard Candles/Bulb's used for?
    The measured apparent brightness of a Standard Candle can be used to determine its distance using the true luminosity and the inverse square law
  10. How to get apparent brightness
    Divide luminosity by area
  11. Cepheid Variables
    Giant stars that pulse in size, temperature and luminosity over a regular period
  12. Cepheid Variable stars with longer periods have
    Greater luminosities
  13. How to use Cepheid Variables to find distances
    • 1. Measure period
    • 2. Calculate Luminosity using period-Luminosity relationship
    • 3. Measure apparent brightness (l)
    • 4. Calculate distance from distance-luminosity relationship
  14. Why are Supernovae Type Ia good standard candles?
    • extremely bright
    • easily detected, though rare
    • uniform in brightness at maximum light
  15. Tully-Fisher Relation
    Entire galaxies can be used as standard candles because galaxy Luminosity is related to rotation speed.
  16. What is Hubble's Law?
    Relationship between a galaxy's velocity (redshift) and distance
  17. What was Hubble's telescope built for and did Hubble build it?
    • No, Hubble did not build it
    • The telescope was made to pin down the line of best fit in Hubble's Law, ie the rate of universal expansion
  18. What is the rotation curve method?
    The most precise method for measuring the mass of a galaxy
  19. What does the rotation curve method require knowing?
    • true sizes of orbits of stars of gas clouds (thus distance of that galaxy)
    • orbital speeds of the stars or gas clouds (using Doppler shift of spectral lines)
  20. How much more dark matter is there than visible matter?
    10x
  21. What is the evidence for Dark Matter in Spiral Galaxies?
    Spiral Galaxies have flat rotation curves indicating large amounts of dark matter
  22. Cosmology is... and is connected with...
    the study of the structure and evolution of the universe and is connected with the study of galaxies
  23. spiral galaxies are often found in
    groups (< 50)
  24. elliptical galaxies are much more common in
    clusters (hundreds to thousands of galaxies)
  25. How big is the Local Group? What galaxy does it contain?
    Around 40 galaxies. Contains the Milky Way
  26. In a group of galaxies like a cluster, the only important force acting between the galaxies is
    gravitation
  27. velocities indicate what inside the cluster [of galaxies]
    total mass
  28. How much larger is the mass we find from galaxy motions in a cluster than the mass in stars?
    50x
  29. Estimates of gravitational mass can be done most directly in what ways
    • 1. Observing galaxies orbiting massive central elliptical galaxies
    • 2. Gravitational Lensing
  30. What are the possible solutions for the difference in observed and gravitational mass? Which do astronomers prefer and why?
    • 1. Dark matter really exists and we are observing the effects of its gravitational attraction
    • 2. Something is wrong with our understanding of gravity, causing us to mistakenly infer the existence of dark matter

    Because gravity is so well tested, most astronomers prefer the dark matter explanation.
  31. Ordinary matter is made up of what and called
    • protons and neutrons
    • baryonic matter
  32. Nonbaryonic matter is what?
    extraordinary matter or dark matter
  33. What are MACHOs and where are they found
    • Ordinary dark matter
    • Massive Compact Halo Objects: dead or failed stars in halos of galaxies
  34. What are WIMPs?
    • Extraordinary dark matter
    • Weakly Interacting Massive Particles: mysterious neutrino-like particles
  35. MACHOs or WIMPs
    WIMPs are the best bet. There is too little evidence of MACHOs
  36. What do many nearby galaxies have at their centres?
    Supermassive Blackholes
  37. What do the supermassive blackholes at the centre of most nearby galaxies seem to be?
    dormant active galactic nuclei
  38. The universe is consistent with what structure?
    Soap bubble (as opposed to spaghetti)
  39. What does it mean to say the universe is isotropic and homogenous
    viewed on sufficiently large distance scales, there are no preferred directions (isotropic) or preferred places (homogenous) in the universe
  40. Our sky is isotropic except for
    the Milky Way, which is denser
  41. Simply, the cosmological principle states that
    Averaged over large enough distances, one part of the universe looks approximately like any other part.q
  42. What is the Edge-centre problem?
    Modern observations indicate the universe could be infinite and have no edge. If the universe has no edge, then it cannot have a centre
  43. If the universe is infinite why don't you see the surface of a star in every direction you look? (Why does the sky get dark at night?)
    The universe is infinite in size but not infinitely old- the night sky is dark because the universe had a beginning
  44. Hubble discovered nearby galaxies have ___ redshifts, but more distant galaxies have ____ redshifts. This implies...
    • nearby galaxies have small redshifts
    • more distant galaxies have large redshifts
    • This implies that the galaxies are receding from each other
  45. What does the Hubble constant describe?
    The universe's rate of expansion
  46. What is 1/H0?
    The age of the universe
  47. What are the observable characteristics of the universe?
    • 1) Redshift proportional to distance
    • 2) Cosmological principle: universe is isotropic and homogenous
    • 3) Content of universe is H and He changing into heavier elements inside stars
    • 4) Gravity warps fabric of space-time
  48. What determines the geometry of the universe?
    The average density of matter
  49. critical density of universe is
    6 H atoms/m3
  50. density>critical density
    universe is closed, finite
  51. density=critical density
    universe is flat but still infinite
  52. density<critical density
    universe is open, infinite
  53. What does low H0 imply?
    Slower expanding universe (older universe)
  54. What are the pillars of the Big Bang Theory?
    • 1) the expansion of the universe
    • 2) the primordial nucleosymthesis
    • 3) cosmic background radiation
  55. What elements were present at the Big Bang?
    H, He, H2, Li
  56. What is evidence for the Big Bang Theory?
    • 1) The theory correctly predicts the abundance of helium and other light elements
    • 2) CMB (cosmic microwave background radiation) we have detected the leftover radiation from the Big Bang
  57. What era does CMB come from?
    Era of atoms
  58. What is CMB
    stretched out photon wavelengths
  59. The Big Bang was an explosion...
    of space. Not in space
  60. zero curvature
    the number of galaxies should increase linearly
  61. positive curvature [shape and description]
    sphere, the number of galaxies increases with greater volume then decreases with very large volumes
  62. negative curvature [shape and description]
    saddle, number of galaxies increase more rapidly with ever greater volume than flat universe
  63. What does the Big Bang explain
    • observation of CMB
    • predicts abundance of light elements
    • predicts 3 types of neutrinos experimentally detected
  64. What does the Big Bang not explain
    • why matter>antimatter
    • origin of density fluctuations that grew into galaxies
    • uniformity of the universe
    • why the density of matter in the universe is close to critical and curvature flat
  65. What is the evidence for the Solar Nebula Hypothesis
    • orbits of the planets lie nearly in a plane
    • planets all revolve in the same direction
    • planets mostly rotate in the same direction
  66. What ended the era of planet formation?
    Solar wind blew away the leftover gases
  67. What is the dominant mass in our Solar System?
    the sun
  68. What is the difference between an asteroid, comet and meteorite?
    • Asteroids are rocky formations inside the frost line
    • Comets are icy formations outside the frost line beyond the orbit of Pluto (ie, Kuiper belt and Oort cloud)
    • A meteorite is a speck of dust grains of sand or tiny pebbles that reach Earth's surface)
  69. What is the reason for meteor showers?
    Earth goes into the path of a variety of comet trails, causing a meteor shower
  70. What is the definition of a planet?
    Must dominate its own orbit
  71. Where does Earth's water originate?
    Water may have to to earth from icy planetesimals from outer solar system. Currently we pick up water when we pass through comet trails
  72. How many times bigger is the Sun than the Moon?
    100x
  73. How old is the universe?
    13.8 billion years old
  74. Planets and Solar system probably formed when? How do we know?
    • 4.6 billion years ago
    • radiometric dating of oldest meteorites
  75. What theory best explains the features of our solar system?
    Nebular theory states that the Solar System formed from a large interstellar gas cloud
  76. How did terrestrial planets form?
    • rock and metals collected into planetesimals
    • planetesimals accreted into planets
  77. How did jovian planets form?
    • additional ice particles outside the frost line made planets more massive
    • gravity of these massive planets drew in H, He gases
  78. How do we explain the existence of Earth's moon?
    Material torn from Earth crust by giant impact formed the moon
  79. What is photometry and what is it used for?
    • Photometry is measuring the brightness of a star and how much fainter it gets when a planet passes in front of it
    • Photometry is used to detect planets and determine its size and mass
  80. What is the Habitable zone?
    Zone around star where we expect to find liquid water
  81. What is called the morning and evening star and why?
    Venus, because when we look at Venus we are looking towards the Sun
  82. Why are big planets formed away from the Sun?
    Gas close to the Sun is vapourized and can't be used for adding size to a planet
  83. What is the composition of both Saturn and Jupiter?
    Primordial solar nebula
  84. What is special about how much energy Jupiter and Saturn radiate?
    They both radiate more energy into space that they receive from the sun
  85. What are some common properties of living organisms?
    • obtain energy from surroundings
    • self-maintenance
    • adapting to surroundings to survive
    • information storage
    • reproduction
  86. What are the necessities for life?
    • nutrient source
    • energy
    • liquid water
  87. What is the order of cosmic evolution?
    • 1) origin of matter
    • 2) formation of milky way
    • 3) formation of Earth
    • 4) origin of life on Earth
    • 5) present
  88. What is a bio indicator?
    Nitrogen is a bio indicator because it is the exhaust of organic life
  89. What is Europa and why is it a suspect for life after Mars?
    • Moon of Jupter
    • Criss cross lines indicate liquid water underneath
  90. What happens when a star can no longer fuse H into He in its core?
    Core shrinks and heats up
  91. What happens as a star's inert helium core starts to shrink?
    Hydrogen fuses in a shell around the core
  92. What happens to a white dwarf when it accretes enough matter to reach 1.4 solar masses?
    it explodes
  93. could there be neutron stars that appear as pulsars to other civilizations but not to us?
    yes
  94. How does the radius of the event horizon change when you add mass to a black hole?
    It increases (dropping a big rock makes a hole with a big radius)
  95. What types of celestial object did Edwin Hubble observe to measure the distance to M31?
    Cepheid variable stars
  96. What evidence tells us that other galaxies contain dark matter?
    their rotational speeds do not steadily decrease with distance form their centers
  97. What do we assume when we use a standard candle to find distance?
    • light intensity is inversely proportion to distance squared
    • we know the luminosity of the standard bulb
  98. Rotational velocity of a spiral galaxy is related to what other characteristic?
    intrinsic luminosity (by Tully-Fisher relation)
  99. Hubble's law describes what type of relationship?
    velocity-distance
  100. What data on a galaxy is necessary to use Hubble's Law as a distance indicator?
    redshift in galaxy's spectrum
  101. what does the value of the Hubble constraint tell us?
    expansion rate of the universe
  102. How is the Hubble constant related to the age of the universe?
    inversely
  103. What effect does gravity have on the expansion rate of the universe?
    gravity tends to  decrease the rate of expansion
  104. What evidence suggests that the universe's rate of expansion is increasing?
    distance type IA supernova explosions are dimmer than expected
  105. What is the fate of the universe based on the rate of expansion and changes in the rate of expansion?
    the universe will expand forever at an increasing rate
  106. How does the temperature and density of the early universe compare to these same conditions today?
    the early universe was hotter and denser
  107. What is the most abundant amount of matter and in what form?
    dark energy
  108. What is the most matter in galaxy clusters?
    dark matter
  109. In what form do we observe radiation left over from BB?
    radio
  110. Where did the solar system come from?
    cloud of gas through recycling of gas through many generations of stars
  111. What was the solar nebula?
    Piece of interstellar cloud from which Solar System was born
  112. Rank sizes of planets from smallest to largest
    Pluto, Mercury, Mars, Venus, Earth, Neptune, Uranus, Saturn and Jupiter
  113. Where do we find asteroids and comets in our solar system?
    • Asteroids: asteroid belt
    • Comets: Kuipter belt and Oort cloud
  114. What property of planets can be obtained from the study of moons and law of gravity?
    mass
  115. Which two planets have nearly the same chemical make up as the Sun?
    Saturn and Jupiter
  116. Which method has been the most successful in locating planets orbiting other stars?
    planet transit method
  117. Which body in the outer solar system has the greatest possibility of harboring life?
    Europa

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