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We Discover the Galaxies The nature of the nebulae the “island universe hypothesis” ---

We Discover the Galaxies The nature of the nebulae the “island universe hypothesis” ---

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We Discover the Galaxies The nature of the nebulae the “island universe hypothesis” ---

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  1. We Discover the Galaxies The nature of the nebulae the “island universe hypothesis” --- The “analogy (of the nebulae) with the system of stars in which we find ourselves ... is in perfect agreement with the concept that these elliptical objects are just island universes – in other words, Milky Ways” Kant 1755 Galactic or Extragalactic? -- the nature of the “nebulae” The Shapley – Curtis Debate 1920 Resolution of the controversy -- Cepheid variables in M31 and M33 Hubble 1923 – 24 using the new Mt Wilson 100-inch telescope

  2. Morphological Classification of Galaxies -- Hubble Spirals, Ellipticals and Irregulars Spiral Galaxies – normal and barred Based on size of nuclear bulge and openess of the arms Sa -- large bulge, tightly wound arms

  3. Spiral Galaxies Type Sb

  4. Spiral galaxies -- Types Sc and Sd small bulge, very open fragmented arms

  5. Barred Spirals

  6. Elliptical Galaxies -- giants and dwarfs Classification based on degree of ellipticity or flattening

  7. Irregular Galaxies

  8. Magellanic Irregulars

  9. Hubble’s Tuning Fork Diagram

  10. The Milky Way ?? Edge-on Sc Milky Way -- infrared SBbc type

  11. Galaxy Clustering Local Group of Galaxies -- 3 spirals + > 30 small Irr and dEll Virgo Cluster

  12. Rotation Curves and the Missing Mass

  13. Gravitational Lensing

  14. Einstein ring 

  15. Missing Mass in Galaxy Clusters and missing mass in halos of galaxies ? “cold dark matter” -- CDM WIMPS (weakly interacting massive particles) or MACHOS (massive compact halo objects)

  16. The Distance Scale of the Universe How do we determine the distances to the galaxies (and stars) Direct and indirect methods 1. Stellar parallaxes -- out to 500 pc with Hipparcos - direct 2. Moving cluster method -- 30pc, the solar neighborhood - direct 3. Cluster main sequence fitting -- out to several kpc – indirect 4. spectroscopic parallaxes – out to several kpc – indirect, calibration of brightest stars, Cepheids and RR Lyr 5. Period-Luminosity relation for Cepheids and RR Lyr – indirect RR Lyr --- 5 – 100 kpc Cepheids – 5 – 30 Mpc Brightest stars – out ot 30 Mpc 6. Supernovae Type Ia out to 1000 Mpc ! -- indirect

  17. Application Parallaxes -- solar neighborhood, Milky Way Moving cluster -- solar neighborhood Cluster MS fitting -- Milky Way Spec. parallaxes -- Milky Way, Magellanic Clouds RR Lyr – Milky Way, Mag Clouds, Local Group Cepheids and brightest stars – Local Group, Virgo Cluster Type Ia --Virgo cluster, Hubble flow and the Universe Redshift relation (Hubble Law ) -- Universe

  18. Distance – Redshift Relation or Hubble Law Slipher at Lowell Obs first noticed the redshift several years earlier

  19. A linear relation Vel = constant x Distance Constant = slope – km/sec/Mpc (Hubble Constant) V = H x D The inverse ? 1/H Time -- expansion age of the Universe

  20. H = 73 – 75 km/s/Mpc and 1/H ~ 13 – 15 x 109 yrs

  21. Galaxy Clusters, Superclusters and Large Scale Structure

  22. Large Scale Structure of the Universe from redshift surveys

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