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Physics 490: Introductory Astrophysics Dr. Rulison M51 (The Whirlpool Galaxy) from Kitt Peak/HST Composite, in visible, Near IR 1
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Tentative Course Outline 1.Our Place in the Universe 2.Physical Principles in Astrophysics 3.Stars 4.General Relativity 5.Galaxies 6.Cosmology 2
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The Gott Logarithmic Map from the Earth’s Core to Chandra 3
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The Celestial Sphere 4
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Solar vs. Sidereal Day 5
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Star Trails 6 N EW ~20 deg.=1.3 hours
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A better view of circumpolar stars 7
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Stars “move” through the sky 8
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Declination 9
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Gott Projection to man-made satellites 10
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Hubble and Chandra (and views of Sgr A*, the center of our galaxy) 11 Hubble (Optical) Chandra (X-Ray)
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The Gott Projection to L 1 and L 2 12
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The Phases of the Moon 13
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SOHO Satellite at L 1 14 Observes the sun in the UV
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Lots of Satellites at L 2 15 WMAP Microwave (3-13 mm) CMB Herschel Satellite Far Infrared (60-670 m) Milky Way Planck Satellite Microwave (0.35-10mm) First Light
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Lagrange Points 16
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Gott Projection of the Inner Solar System 17
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Planets 18 “Superior” Planets“Inferior” Planets
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The Terrestrial Planets 19
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Kepler’s 3 rd Law 20 P 2 =a 3
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Configuration of Planets 21
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The Phases of Venus (Galileo) 22 Also, he saw the rings of Saturn
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Gott map of outer solar system 23
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The outer planets 24
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The very outer solar system is very empty 25
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Nearby Stars 26
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Parallax 27
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28 Local Galaxy Residents M45, the Pleiades, an open cluster, seen in optical M42, the Orion Nebula, a star forming region, seen in optical from HST M57, the Ring Nebula, a planetary nebula, seen in optical from HST.
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The Milky Way 29
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Orbiting stars around Sgr A* 30
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The Milky Way 31
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Gott Map to the Local Group 32
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The Local Group 33
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Gott Map of Nearby Groups and Clusters 34
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A1689 35
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Gott map of Distant Galaxies (Gpc Scale) 36
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CMB (from WMAP) 37
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