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Class Notes for Astronomy & Astrophysics at University of Toronto St. George (UTSG)

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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 13: Meteor Crater, Himalayas, Basalt

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4 Nov 2015
37
Earth: oceans and land, geologically active : processes that change the surface of a planet over time, interior continual radioactivity decay, core (me
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 18: Cryovolcano, Protoplanet, Not Proven

OC5374883 Page
25 Nov 2015
68
Ast101 lecture 18 dwarf planets & jovian planets. Could possibly be a surviving protoplanet - celestial body with collection of matter that survived fr
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 6: Elipse, Semi-Major And Semi-Minor Axes, V Speeds

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7 Oct 2015
43
Ast101 lecture 6 gravity and orbits (part 1) A physical body of mass that exerts force on an object and as result, the object is attracted toward the b
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 1: Milky Way, Observable Universe, Local Group

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29 Sep 2015
47
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 20: Methods Of Detecting Exoplanets, Astronomical Object, Light Curve

OC5374883 Page
3 Dec 2015
35
Extrasolar planet, often referred to as exoplanets planets that orbit a star other than the sun. The exoplanets are named according to a system: star:
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UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 1: Vera Rubin, Spiral Galaxy, Orbital Speed

OC25354552 Page
19 Jan 2019
0
One patch of the night sky can have numerous galaxies. If you are looking at things in the sky, it actually means you are looking back in time, as ligh
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 14: Black-Body Radiation, Volcanism, Pearson Education

OC5374884 Page
6 Nov 2015
57
Venus vs earth: average surface temperature: 470 o c vs 15 o c, atmosphere(s): 90 vs 1, presence of co 2 in the atmosphere: 95% vs 0. 04, rotation: clo
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 9: Pearson Education, Asteroid Family, The Cooler

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16 Oct 2015
58
Ast101 lecture 9 the sun: the nearest star (part 2) *note: e=mc2 shows that mass contains potential energy which at the speed of light squared converts
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture 10: The Solar Spectrum (Light and Matter)

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21 Oct 2015
72
Ast101 lecture 10 the solar spectrum (light and matter) Light (also known as electromagnetic radiation): a form of energy, more specifically radiative
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 11: Photosphere, 30 Foot Fall, Photon

OC5374884 Page
26 Oct 2015
50
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 12: Oort Cloud, Small Solar System Body, Kuiper Belt

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3 Nov 2015
31
Ast101 lecture 12 formation of the solar system. Doppler effect for light: a small effect for light: light sources moving away from you appear redder =
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UTSGAST101H1Michael ReidFall

AST101H1 Lecture Notes - Lecture 15: Carbon Footprint, Thermostat, Carbon Cycle

OC5374884 Page
16 Nov 2015
65
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