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Enhancement Lesson
   Red Giant – a
    large, reddish star
    late in its life cycle
    that fuses helium
    into carbon or
    oxygen.
   Supergiant –
    an extremely
    large star
    that creates
    elements as
    heavy as
    iron.
   Supernova –
    a powerful
    explosion
    that occurs
    when a
    massive star
    dies.
   White Dwarf
    – A small, very
    dense star
    that remains
    after fusion in
    a red giant
    stops.
   Neutron Star
    – a dead star
    with the
    density of
    atomic nuclei.
   Black Hole –
    an object so
    massive and
    dense that not
    even light can
    escape its
    gravity.
   Coronal
    streamer-A wisp-
    like stream of
    particles that
    gradually moves
    away from the
    Sun and becomes
    part of the solar
    wind.
   Coronal holes -
    are areas of the
    Sun's surface that
    are the source of
    open magnetic
    field lines that
    head way out
    into space.
   Photosphere -
      imaginary
    surface from
    which the solar
    light that we see
    appears to be
    emitted.
   Sunspot –
    temporary
    phenomena on
    the photosphere
    caused by
    magnetic activity
    which inhibits
    convection
    forming areas of
    reduced
    temperature.
   Chromosphere –
    An incandescent,
    transparent layer
    of gas, primarily
    hydrogen, several
    thousand miles in
    depth, lying above
    and surrounding
    the photosphere
    of a star, such as
    the sun, but
    distinctly separate
    from the corona.
   Filament – are
    formed in
    magnetic loops
    that hold
    relatively cool,
    dense gas
    suspended above
    the surface of the
    Sun.
   Corona hole –
    areas where the
    Sun's corona is
    darker, colder,
    and has lower-
    density plasma
    than average.
   Convective Zone
    – the range
    of radii in which
    energy is
    transported
    primarily
    by convection.
   Radiative Zone –
    In the radiation
    zone, energy is
    transported by
    radiation.
   Core – The core is
    the source of all
    the Sun's
    energy. The Sun's
    core has a very
    high temperature,
    more than 15
    million degrees
    Kelvin, and the
    material in the
    core is very tightly
    packed or dense
1




                 Fusion        Main
Protostar       Ignition     Sequence




   Red &
 Supergiants   White Dwarf    Black Hole

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1.2e the sun and stars

  • 2. Red Giant – a large, reddish star late in its life cycle that fuses helium into carbon or oxygen.
  • 3. Supergiant – an extremely large star that creates elements as heavy as iron.
  • 4. Supernova – a powerful explosion that occurs when a massive star dies.
  • 5. White Dwarf – A small, very dense star that remains after fusion in a red giant stops.
  • 6. Neutron Star – a dead star with the density of atomic nuclei.
  • 7. Black Hole – an object so massive and dense that not even light can escape its gravity.
  • 8. Coronal streamer-A wisp- like stream of particles that gradually moves away from the Sun and becomes part of the solar wind.
  • 9. Coronal holes - are areas of the Sun's surface that are the source of open magnetic field lines that head way out into space.
  • 10. Photosphere - imaginary surface from which the solar light that we see appears to be emitted.
  • 11. Sunspot – temporary phenomena on the photosphere caused by magnetic activity which inhibits convection forming areas of reduced temperature.
  • 12. Chromosphere – An incandescent, transparent layer of gas, primarily hydrogen, several thousand miles in depth, lying above and surrounding the photosphere of a star, such as the sun, but distinctly separate from the corona.
  • 13. Filament – are formed in magnetic loops that hold relatively cool, dense gas suspended above the surface of the Sun.
  • 14. Corona hole – areas where the Sun's corona is darker, colder, and has lower- density plasma than average.
  • 15. Convective Zone – the range of radii in which energy is transported primarily by convection.
  • 16. Radiative Zone – In the radiation zone, energy is transported by radiation.
  • 17. Core – The core is the source of all the Sun's energy. The Sun's core has a very high temperature, more than 15 million degrees Kelvin, and the material in the core is very tightly packed or dense
  • 18. 1 Fusion Main Protostar Ignition Sequence Red & Supergiants White Dwarf Black Hole