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REVIEW SHEET: ASTRON 103, PART III. Milky Way Galaxy – structure, features: Disk; bulge/halo; nucleus (supermassive black hole) Location of Sun Interstellar matter, star formation (where present/absent) Population I, II stars: characteristics Open, globular clusters Turnoff point – age of star clusters Spiral arms Spiral Density Wave theory Formation of Galaxy: top-down, monolithic collapse Galaxies (formerly ‘Spiral Nebulae’) Classification scheme (Hubble): Ellipticals Normal Spirals Barred Spirals Irregulars Types of stars; presence/absence of interstellar matter Rotation Curves (spiral galaxies); distribution of matter Evidence for Dark Matter Composition of Dark Matter MACHOs WIMPS Alternate explanation(s): MOND Galaxy Clusters; interactions Local Group [Poor Cluster]: characteristics Rich clusters: characteristics Calculation of cluster mass(es): internal motions Evidence for Dark Matter Gravitational Lenses Einstein’s General Theory of Relativity Superclusters: filaments, voids Origins in primordial density variations Role of Dark Matter in simulations Galaxy evolution Mergers/acquisitions Radio Astronomy: techniques for increasing sensitivity, resolution Active Galaxies: definition; abundance Light travel time determines maximum size limit Radio Galaxies Lobes; jets; orientations Seyfert Galaxies Quasars: characteristics; interpretations Active Galactic Nuclei (AGN) – unified model: Supermassive black holes, accretion disks, jets Expansion of the Universe (Standard Big Bang model) Velocity-Distance relation (Hubble’s Law) Apparent centrality of observer(s) Hubble’s Constant (H0) Age of Universe = 1 / H0 Standard Big Bang theory (origin of Universe) Cosmic Microwave Background Radiation (CMBR) Origin (recombination after Big Bang) Cosmological redshift Oldest ‘picture’ of Universe Origin of matter (nucleosynthesis) during Big Bang Fate(s) of Universe Open Critical Density Closed Deviations from Standard Big Bang model: Inflationary Universe Horizon, flatness problems Acceleration; Dark Energy Evidence from Type Ia supernovae Composition of Universe Einstein’s ‘cosmological constant’ – reintroduced?