OATo Seminars on formation and Evolution of the Galaxy 1 The GAIA Space Mission: Observational Principles and Scientific Objectives Mario G. Lattanzi -
LECTURE 21, NOVEMBER 16, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT [email protected] 1ASTR 101-3, FALL 2010.
AST 5.3 PPT
The Big Bang
Astro 10-Lecture 13: Quiz 1. T/F We are near the center of our Galaxy 2.Cepheid variable stars can be used as distance indicators because a) They all have.
August 28, 2014PTF Summer School Novae in Local Group Galaxies, but really just Andromeda A. W. Shafter San Diego State University Modified and delivered.
The Accelerating Universe and the Sloan Digital Sky Survey Supernova Search Jon Holtzman (NMSU) + many collaborators (FNAL, U. Chicago, U. Washington,
Measuring the Stars (Part III). The “Cosmic Distance Ladder”
Gaia A Stereoscopic Census of our Galaxy November 2003 .
Post Main Sequence Evolution of “Low-Mass” Stars Chapter 19 (and some of 20) 1.
Class 21 : Other galaxies The distance to other galaxies Cepheid variable stars. Other methods. The velocities of galaxies Doppler shifts. Hubble’s law.