Slide 1 Reading Unit 28, Unit 29, Unit 30 Will not be covered by the first exam Slide 2 As a blackbody object becomes hotter, it also becomes ____________ and _____________…
The Sun and other stars The physics of stars A star begins simply as a roughly spherical ball of (mostly) hydrogen gas, responding only to gravity and itâs own pressure.…
GEARS Workshop Wednesday Don’t forget there are hidden slides and notes – don’t just use the show 2011 Warm Up Online – and paper evaluation – Discuss how spectroscopy…
Chapter 19 The Nature of the Stars Figuring out what the rest of the Universe is like Properties Distance Parallax (triangulation) Spectroscopic parallax Properties from…
NGC 743 NGC 743 David Randall Topics What is a H-R Diagram? What is an open cluster? Why open clusters? Procedure H-R Diagrams Ejnar Hertzsprung plotted luminosities of stars…
1.BLACK HOLES IN GALAXIES Bryan Nozaleda 2. Aside from stars and the interstellar medium, what else do galaxies contain? • Galaxies often have large magnetic fields that…
Properties of Stars Distances to Stars The distance to a nearby star can be measured by observing its parallax - the apparent shift of its position on the sky relative to…