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Study Guides for Astronomy & Astrophysics at University of Toronto St. George (UTSG)

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UTSGAST201H1Bryan GaenslerSpring

AST201H1- Final Exam Guide - Comprehensive Notes for the exam ( 119 pages long!)

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Fritz zwicky (1898- 1974: zwi(cid:272)k(cid:455)"s (cid:272)olleagues thought his (cid:373)issi(cid:374)g (cid:373)ass idea was odd, he was unhappy wit
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UTSGAST251H1Hilding NeilsonFall

AST251H1- Final Exam Guide - Comprehensive Notes for the exam ( 32 pages long!)

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In the spiral arms and molecular clouds stars are formed. Our local groups are also grouped into a supercluster of galaxies. Theres no such thing as th
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UTSGAST101H1Bryan GaenslerFall

AST101H1- Final Exam Guide - Comprehensive Notes for the exam ( 46 pages long!)

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Earth solar system milky way galaxy local group super cluster universe. Milky way galaxy: used both as the name of our galaxy and to refer to the band
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UTSGAST101H1Netterfield

AST101H1- Final Exam Guide - Comprehensive Notes for the exam ( 38 pages long!)

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Solar system is the sun, planets and all their moons: a star and all the objects that orbit it. Universe is the totality of all space, time, energy and
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UTSGAST101H1Bryan GaenslerFall

AST101H1- Final Exam Guide - Comprehensive Notes for the exam ( 88 pages long!)

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UTSGAST101H1C.B.NetterfieldFall

[AST101H1] - Final Exam Guide - Comprehensive Notes for the exam (41 pages long!)

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Terrestrial (earth-like) planets: small, rocky, thin or no atmosphere, not many moons, made of heavy elements. Jovian (jupiter-like) planets: large, li
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UTSGAST101H1Michael ReidFall

[AST101H1] - Final Exam Guide - Ultimate 40 pages long Study Guide!

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UTSGAST201H1Michael ReidFall

[AST201H1] - Final Exam Guide - Ultimate 239 pages long Study Guide!

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Ast201 - the sun: part 1 (chp 5. 1-5. 4) Can"t for diagonal or across our line of sight) for rotation- faster the object is rotating, the broader the w
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UTSGAST251H1Michael Reid Winter

AST251H1 Study Guide - Final Guide: Late Heavy Bombardment, Protoplanetary Disk, Big Bang

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UTSGAST201H1Bryan GaenslerWinter

AST201H1 Study Guide - Final Guide: Low Mass

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UTSGAST101H1Bryan GaenslerFall

AST101H1 Final: Ast finals

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Temperature of light = peak of continuum spectrum (blackbody curve) Density of light = continuum line vs. line spectrum. Composition of light = which e
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UTSGAST101H1Bryan GaenslerFall

AST101H1 Study Guide - Final Guide: Galilean Moons

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Hydrogen with other gas and clouds at the top. Low temperature emit infrared light we cannot see. Get brighter as it heats up ( changes from red to whi
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