Assigning a distance by redshift The Hubble law lets us use a simple spectrum of a galaxy to figure out where it is along the line-of-sight. Higher redshifts.
Astronomy 1 – Winter 2011 Lecture 24; March 7 2011.
Chapter 18 Cosmology Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
100 200 400 300 400 Solar Systems & Night Sky Galaxies 300 200 400 200 100 500 100 200 300 400 Cosmology 100 500 Tools, Laws & Methods The Sun & Other.
Cosmology Astronomy 315 Professor Lee Carkner Lecture 24.
March 7, 2006Astronomy 20101 Quasars – Unsolved mysteries? 2 basic things used for studying far away galaxies –the data encoded in the light received;
The Miracle of Stars or Why We Are Michael Bass, Professor Emeritus CREOL, The College of Optics and Photonics University of Central Florida Orlando, FL.
Lecture 6 Black hole (by D.Koo). The evolution of the Universe can be essentially derived using the Newtonian equations. This is due to a peculiarity.
Orbits and Galaxy Shape elliptical orbits random orientations different speeds in different directions.
Extragalactic Astronomy & Cosmology Lecture SR1 Jane Turner Joint Center for Astrophysics UMBC & NASA/GSFC 2003 Spring [4246] Physics 316.
Galaxy Morphology The Tuning Fork that Blossomed into a Lemon Lance Simms MASS Talk 9/8/08.
Cosmology: The Origin and Evolution of the Universe
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