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Review for Quiz 2 Outline of Part 2 • Properties of Stars Distances, luminosities, spectral types, temperatures, sizes Binary stars, methods of estimating mass, stellar masses • The HR Diagram Spectral type, absolute magnitude, using the HR diagram • Stellar Evolution (Low Mass and High Mass stars) Hydrostatic equilibrium, sources of energy, energy transport Evolution in the HR diagram • Stellar Endpoints Planetary nebulae white dwarfs, supernovae, neutron stars Black holes • Binary Star Evolution Mass transfer and accretion; novae • Protostars and Star Formation The H-R Diagram Stellar Evolution • Main Sequence (core H fusion) Stellar Evolution • Main Sequence (core H fusion) • Red Giant (core contraction, Hydrogen shell burning) Stellar Evolution • Main Sequence (core H fusion) • Red Giant (core contraction, Hydrogen shell burning) • Core Helium burning Stellar Evolution • Main Sequence (core H fusion) • Red Giant (core contraction, Hydrogen shell burning) • Core Helium burning • 2nd Giant Branch (core contraction, H, He shell burning) Mass Loss Occurs Here Stellar Evolution • Main Sequence (core H fusion) • Red Giant (core contraction, Hydrogen shell burning) • Core Helium burning • 2nd Giant Branch (core contraction, H, He shell burning) Mass Loss Occurs Here If Core is Less Than 1.4 M • Planetary Nebula (ionization of mass lost by star) • White Dwarf (inert C/O core) Planetary Nebulae Stellar Evolution If Core is Greater Than 1.4 M • Series of core burning and core contractions Carbon to Magnesium, etc. Magnesium, etc., to Silicon, etc. Silicon, etc. to iron • SUPERNOVA Supernova Remnants Elemental Synthesis In the supernova explosion, all the elements are made, and are ejected into space Stellar Endpoints • If Remnant Core is less than 3 M Remnant is a Neutron Star If Magnetic Pole Points at Earth Remnant is a Pulsar Stellar Endpoints • If Remnant Core is less than 3 M Remnant is a Neutron Star If Magnetic Pole Points at Earth Remnant is a Pulsar • If Remnant Core is greater than 3 M Remnant is a Black Hole QuickTime™ and a Cinepak decompressor are needed to see this picture. The HR Diagram