space lab book

  1. Celestial Object
    Any object that exists in space, such as a planet, a star or the moon
  2. Astronomer
    A scientist who studies astronomy, which is the study of the Night Sky
  3. Revolution
    The time it takes for an object to orbit another object: Earth's revolution around the Sun is 365.24 days
  4. Rotation
    The turning of an object around an imaginary axis running through it
  5. Constellation
    A group of stars that seem to form a distinctive pattern in the sky
  6. Light Year
    The distance that light travels in one year, about 9.5 x 10 to the power of 12 km
  7. Apparent Magnitude
    The brightness of a star as seen from Earth
  8. Asterism
    • Smaller groups of stars that form patterns within or between constellations.
    • Example: Big Dipper in Ursa Major
  9. Pointer stars
    Stars that point toward Polaris
  10. Circumpolar Constellations
    Constellations that can be seen all year long
  11. Zenith
    The point or celestial sphere in the sky directly above an observer
  12. Tides
    The rising and falling of oceans as a result of the Moon's gravity and Earth's gravity
  13. Phases of the Moon
    The monthly progression of changes in the appearance of the moon, which result from different portions of the Moon's sunlit side being visible from Earth
  14. Lunar Eclipse
    The phenomenon in which the full moon passes into Earth's shadow
  15. Solar Eclipse
    The phenomenon in which the shadow of the moon falls on Earth's surface
  16. Why do we have season?
    A result of Earth's evolution around the sun, combined with Earth's tilt
  17. Planet
    An object that orbits one or more stars (and is not a star itself), is spherical, and does not share its orbit with another object. Inner planets are Mercury, Venus, Earth and Mars, Outer Planets are Jupiter, Saturn, Uranus and Neptune
  18. Solar System
    A group of planets that circle one or more stars
  19. Retrograde motion
    The movement of an object in the sky, usually a planet, from east to west, rather than its normal motion from west to east
  20. Astronomical unit
    The average distance between Earth and the sun, about 150 x 10 to the power of 6 km
  21. Orbital Radius
    The average distance between the sun and an object that is orbiting the Sun
  22. Geocentric model
    The first model of the Solar System, stated that Earth was the centre of all planetary motion
  23. Heliocentric Model
    States that the sun is the centre of the solar system and has planets orbit the sun in perfect circles
  24. Comet
    An object composed of rocky material, ice and gas; comes from the kuiper Belt and Oort cloud
  25. Asteroid
    A small object that ranges in size from a tiny speck, like a grain of sand, to 500 km wide; most asteroids originate in the asteroid belt between Mars and Jupiter
  26. Meteoroid
    A piece of rock moving through space
  27. Metoer
    A meteoroid that hit's Earth's atmosphere and burns up
  28. Meteroite
    A meteoroid that is large enough to pass through Earth's atmosphere and reach the ground, without being totally burned up
  29. Trans-Neptunian object
    Objects that circle the Sun beyond the orbit of neptune
  30. Electromagnetic Radiation
    • Radiation consisting of Electromagnetic waves that travel at the speed of light
    • Examples: visible light, radio waves, and X rays
  31. Refracting telescope
    A telescope that uses a lens to collect the light from an object
  32. Reflecting telescope
    A telescope that uses a mirror to collect the light from an object
  33. Satellite
    • An artificial (human made) object or vehicle that Orbits Earth, moon or other celestial bodies; also, a celestial body that orbits another of larger size.
    • Example: The Moon is the Earth Natural Satellite
  34. Solar Nebula Theory
    The theory that describes how stars and planets form from contracting, spinning disks of gas and dust
  35. Star
    A celestial body made of hot gases, mainly hydrogen and some helium
  36. Nebula
    A vast cloud of gas and dust, which may be the birthplace of stars and planets
  37. Protostar
    Hot, condensed object at the centre of a nebula
  38. Nuclear fusion
    the process of energy production in which hydrogen nuclei combine to form helium nuclei
  39. Photosphere
    The surface layer of the sun
  40. Sunspot
    An area of strong magnetic fields on the photosphere
  41. Solar wind
    A stream of fast moving charged particles ejected by the Sun into the Solar System
  42. Importance of the Sun
    The Sun is needed for all life on Earth. Drives processes like finding sufficient food and providing ourselves with adequate shelter. Also powers the winds and ocean currents. Creates and provides weather and seasons. The sunlight also provides energy for photosynthesis
  43. Luminosity
    A star's total energy output per second; it's power in joules per second (j/s)
  44. Absolute Magnitude
    The magnitude of a star that we would observe if the star were placed 32.6 light years away from Earth
  45. Spectroscope
    An optical instrument that produces a spectrum from a narrow beam of light, and usually projects the spectrum onto a photographic plate or a digital detector
  46. Spectral lines
    Certain specific wavelengths within a spectrum characterized by lines; spectral lines identify specific chemical elements
  47. Hertzsprung-Russel (H-R) diagram
    A graph that compares the properties of stars
  48. Main Sequence
    A narrow band of stars on the H-R diagram that runs diagonally from the upper left (bright,hot stars) to the lower right (dim,cool stars); about 90% of stars, including the Sun, are in the main sequence
  49. White dwarf
    A small, dim, hot star
  50. Supernova
    A massive explosion in which the entire outer portion of a star is blown off
  51. Neutron Star
    A star so dense that only neutrons can exist in the core. The pressure is so great that electrons are squeezed into protons, and eventually forming it.
  52. How Low Mass-Stars evolve
    They consume their hydrogen slowly, as long as 100 billion years and lose significant mass during that time
  53. How Intermediate-Mass Stars evolve
    They consume their hydrogen in about 10 billion years. Once their hydrogen is used up, the core collapses, stars to contract, the temperature increases and the outer layers begin to expand.
  54. How High-Mass Stars Evolve
    They consume their hydrogen even faster that Indermedite-Mass stars causing the star to not lose much weight and remain 12 or more solar masses after the core's temperature rises quickly and to much higher temperatures and the star begins to expand
  55. Milky Way
    The galaxy that includes the solar system; appears as a hazy white band in the Night Sky
  56. Galaxy
    A huge collection of stars, planets, gas, and dust that is held together by gravity
  57. Star cluster
    A collection of stars held together by gravity
  58. Open cluster
    A collection of 50 to 1000 stars; appear along the main band of the Milky Way
  59. Globular Cluster
    A collection of 100,000 to 1,000,000 stars, arranged in a distinctive spherical shape; appear around the centre of the Milky Way
  60. Local Group
    The small group of 40 galaxies, includes the Milky Way
  61. Supercluster
    A gigantic of 4 to 25 clusters of galaxies, which is hundreds of millions of light-years in size
  62. Shapes of Galaxies
    • A spiral galaxy: Appears like a pinwheel and looks like a plate with a bulge in the middle.
    • Elliptical galaxies: Range in shape from perfect a sphere to a stretched out Ellipse. Some look like footballs and some like cigars.
    • Irregular galaxies: Do not have a regular shape and made of new forming stars and old stars
  63. Cosmology
    The study of the universe
  64. Doppler Effect
    • The change in frequency of a light source due to it's motion relative to an observer; also the change in the pitch of a sound due to the motion of the source relative to an observer.
    • Example: Change of the pitch of an ambulance siren approaches you, passes you and then moves away
  65. Redshift
    The effect in which objects are moving away from an observer have their wavelengths lengthened, towards the red end of the visible spectrum
  66. Blueshift
    The effect in which objects are moving towards an observer have their wavelengths shortened, toward the blue end of the visible spectrum
  67. Big Bang
    The event that may have triggered the expansion of the universe 14 billion years ago
  68. Cosmic Microwave Background (CMB) radiation
    The radiation left over from the big bang, which fills the universe
  69. Dark Matter
    The most abundant form of matter in the universe; invisible to telescope. It's true identity is unknown and very little is learned about it.
  70. Dark energy
    A form of energy that makes up nearly three quarters of the universe; has the affect of increasing the expansion of the universe. Astronomers don't understand it's true nature
Author
Waleed
ID
345719
Card Set
space lab book
Description
Glossary terms for the space lab book
Updated