Slide 11 Endpoints of stellar evolution The end of stellar evolution is an inert core of spent fuel that cannot maintain gas pressure to balance gravity Chandrasekhar Mass:…

Slide 1The Universe of Galaxies Slide 2 A Brief History 1610 - Galileo Slide 3 1610 - Galileo resolves the Milky Way into stars Slide 4 1784 – Hershel maps the Milky Way…

Slide 1 Slide 2 Slide 3 ‘SIDE VIEW’ ‘TOP VIEW’ Solar System on outside of Orion Arm (25,000 light years from centre) 100,000 ly Slide 4 Nebular hypothesis Important…

Slide 1 Unit 1 College Slide 2 Objectives  Successful implementation of field work.  Developing competence in arranging data in time order and clarifying relationships.…

Slide 1 Introduction to Stars Slide 2 Stellar Parallax Given p in arcseconds (”), use d=1/p to calculate the distance which will be in units “parsecs” By definition,…

Slide 1 Measuring Distance and Size of Stars Physics 113 Goderya Chapter(s): 9 Learning Outcomes: Slide 2 Light as a Wave (1) We already know how to determine a star’s…

Slide 1 ARE BILINGUALS LIKE TWO MONOLINGUALS IN ONE PERSON? EVIDENCE FROM RESEARCH IN SENTENCE PROCESSING Eva M. Fernández [email protected] Queens College & Graduate…

Slide 1 ASTR100 (Spring 2008) Introduction to Astronomy The Milky Way Prof. D.C. Richardson Sections 0101-0106 Slide 2 What does our galaxy look like? Slide 3 The Milky Way…

Slide 1 Unit 1: Reviewing Parts of Speech and How Diction Creates Meaning How can grammar control a reader’s understanding and create a distinguished style? Slide 2 Learning…

Slide 1 The Grammar Business © 2001 Glenrothes College The Grammar Business Part One 4. Naming of Parts Slide 2 The Grammar Business © 2001 Glenrothes College 2` Names…