LECTURE 15, OCTOBER 21, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT [email protected] 1ASTR 101-3, FALL 2010.
Inter 2nd Year Physics
Evolution of the Universe From the Big Bang to the Big Chill Dan Caton.
Minerals A mineral is a naturally occurring, inorganic, usually non-biologic, crystalline solid, which is physically and chemically distinctive. Form in.
Star Formation Evolution of Low-Mass Stars Evolution of High-Mass Star.
Stars Part Two: Stellar Evolution. Overview of the life of a star: 1.Formation of protostar from a cloud of mostly Hydrogen gas. 2.Main sequence star.
Units to cover 60-63. Homework 8 Unit 56 problems 6,7 Unit 59 problems 6, 8, 9 Unit 60 problems 6, 8, 11 Unit 61 problems 4, 7 Unit 62, problem 8.
Units to cover: 61, 62. Our Sun will eventually A. Become white dwarf B. Explode as a supernova C. Become a protostar D. Become a black hole.
Nuclear fusion is said when two lights nuclei combine to form a heavier nucleus.
Minerals
SUPER -KAMIOKANDE
Astronomy 1020-H Stellar Astronomy Spring_2015 Day-35.
