Neutron Stars, Pulsars, Magnetars, and Black Holes – the “corpses” of high-mass stars Combination X-ray & visible light image of the Crab Nebula Pulsar.
Chapter 22: Black Holes Einstein’s relativity: –Special –General –Relativity and black holes Evidence of black holes Properties of black holes Long-time.
The general theory of relativity is our most accurate description of gravitation Published by Einstein in 1915, this is a theory of gravity A massive object.
Graviational Field and Orbits
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.
48578900 GRE Physics 8677 Solutions
Binary star motion demonstration What does the first demo represent? What will happen if I replace one ball with a smaller ball? What does the second model.
Historically very interesting, heliocentric vs. geocentric universe The main cast: Copernicus, Brahe, Galileo, Kepler, Newton Satellite motion Chapter.
Solar System Planets: The Earth + Moon I.Moon - Atmosphere - Surface/Geological Features/Moon Rocks - Interior - Origin II. Mercury - Basic Facts - Exploration.
The Sun 1. Vital Statistics: A. Diameter – 865,000 miles B. Color – Yellow C. Apparent Magnitude - -26.5 D. Absolute Magnitude - +4.7 E. Period of Rotation.
The feeding and feedback of massive protostars Michael D Smith et al. CAPS University of Kent September 2012.
Black Holes Chapter Twenty-Four. Guiding Questions 1.What are the two central ideas behind Einstein’s special theory of relativity? 2.How do astronomers.
