Exams are coming!
Get ready with premium notes and study guides!

All Educational Materials for AST201H1 at University of Toronto St. George (UTSG)

UTSGAST201H1Bryan GaenslerWinter

[AST201H1] - Midterm Exam Guide - Ultimate 10 pages long Study Guide!

OC115122010 Page
6 Feb 2017
74
Ast101 lecture 3: time dilation and the twin paradox. The speed of light: light always travels at c (in a vacuum, slightly slower in air, no object wit
View Document
UTSGAST201H1Ian SheltonFall

AST201H1- Midterm Exam Guide - Comprehensive Notes for the exam ( 14 pages long!)

OC105000614 Page
5 Oct 2017
0
Wavelength is the distance between two wave peaks. Frequency is the number of times per second that a wave vibrates up and down. This is like water, th
View Document
UTSGAST201H1Michael ReidFall

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

OC755883239 Page
5 Oct 2016
42
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
View Document
UTSGAST201H1Bryan GaenslerSpring

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

Michelle Shen119 Page
29 Mar 2018
0
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
View Document
UTSGAST201H1Michael ReidFall

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

OC755883239 Page
29 Nov 2016
24
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
View Document
UTSGAST201H1Jeffrey ReidWinter

AST201H1 Final: AST201 Important notes from each lecture - EXAM STUDY

OC51018222 Page
4 Aug 2015
69
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Study Guide - Midterm Guide: Neutrino, Superbubble

OC17104063 Page
16 Apr 2014
75
View Document
UTSGAST201H1Michael ReidWinter

notes from lec. for mid term two

OC806928 Page
6 Dec 2012
22
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Study Guide - Midterm Guide: Compact Star, Subgiant, Black Body

OC806926 Page
5 Dec 2012
30
100, 000 light years across (diameter across) 1000 light years thick (up and down) Our sun is located about 28, 000 light years from the galactic centr
View Document
UTSGAST201H1Stefan MochnackiWinter

Midterm 1 Review Notes

OC16795 Page
2 Feb 2011
196
View Document
View all (70+)

Trending

Frequently-seen exam questions from 2014 - 2018.
UTSGAST101H1Bryan GaenslerFall

AST101H1 Study Guide - Midterm Guide: Orbital Period, Northern Hemisphere, Apparent Retrograde Motion

OC24948335 Page
13 Dec 2018
0
Which of the following is false? (a) our solar system contains many planets (b) our galaxy contains many solar systems (c) our universe contains many g
View Document
UTSGAST101H1AllFall

AST101H1 Midterm: AST101H1 Exam 1

OC254029418 Page
16 Oct 2018
0
View Document
UTSGAST101H1AllFall

AST101H1 Midterm: AST101H1 Exam 2

OC254029416 Page
16 Oct 2018
0
View Document
UTSGAST101H1AllFall

AST101H1 Study Guide - Midterm Guide: Scantron Corporation, Multiple Choice, Full Moon

OC25402949 Page
16 Oct 2018
0
Then sign the card: for each multiple choice question, mark your answer in pencil on the scantron card by darkly shading the appropriate bubble. All an
View Document
UTSGAST101H1AllFall

AST101H1 Midterm: AST101H1 Exam 3

OC254029417 Page
16 Oct 2018
0
View Document
UTSGRSM230H1Laurence BoothWinter

RSM230H1 Midterm: important questions summary

OC179885846 Page
22 Oct 2019
0
View Document
UTSGRSM260H1XianFall

RSM260H1 Study Guide - Midterm Guide: Organizational Commitment, Absenteeism, Stereotype

OC27464826 Page
9 Oct 2019
0
View Document
UTSGRSM324H1Matthew RomanFall

RSM324H1 Lecture 4: RSM324 - T4 (Oct 7)

OC21189214 Page
10 Oct 2019
0
View Document
UTSGRSM324H1Matthew RomanFall

RSM324H1 Lecture Notes - Lecture 1: Term Life Insurance

OC21189212 Page
10 Oct 2019
0
View Document
UTSGRSM324H1Matthew RomanFall

RSM324H1 Lecture Notes - Lecture 2: Term Life Insurance, Papyrus 46, Union Dues

OC21189214 Page
10 Oct 2019
0
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 23: Main Sequence, Cosmic Distance Ladder, Edwin Hubble

OC25354552 Page
30 Mar 2019
0
The stars all have the same age and the stars are all at around the same distance. They are all at around the same distance. Step 1: use radar to deter
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 24: Graph Paper, Nucleosynthesis, Neutrino

OC25354552 Page
30 Mar 2019
0
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 22: Elliptical Galaxy, Disc Galaxy, Cosmic Distance Ladder

OC25354552 Page
21 Mar 2019
0
Irregular galaxies are a result of a collision of two galaxies (mergers. ) When its finish its star bursts, it will probably another disk galaxy. But i
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 20: Semi-Major And Semi-Minor Axes, Orbital Period, Vera Rubin

OC25354552 Page
17 Mar 2019
0
Johannes kepler: had worked from tycho bache"s data and came up with an accurate description of the motion of the planets. #1: planets orbit the sun in
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 19: Light Pollution

OC25354552 Page
18 Mar 2019
0
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 18: Angular Momentum, Degenerate Matter, Tablespoon

OC25354552 Page
10 Mar 2019
0
Topic: the afterlives of massive stars, neutron stars. The finale stage of a massive star"s life. When there is no more core fusion then gravity starts
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 15: AST201 lecture 13

OC25354552 Page
2 Mar 2019
0
Topic: lifecycle of a 1 solar mass star. The core expanding and cooling slows things down and stops fusion in the sun"s core from happening faster and
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 16: Neon Neon, Nucleon, Solar Mass

OC25354552 Page
1 Mar 2019
0
Talking about what happens to a star that is above 8 solar masses, and the difference between a low-mass star and high mass star. When all the helium i
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 12: AST 201 - lecture 12

OC25354552 Page
16 Feb 2019
0
Rule #1 = hotter is brighter if it is the same size. If a star is bluer than it is hotter, if it is redder than it is cooler. In our story, we have com
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 11: AST 201 - lecture 11

OC25354552 Page
16 Feb 2019
0
In the previous lecture we discussed how to find certain properties of stars without having to go send probes to the stars. We can find the chemical co
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 10: AST 201 - lecture 10

OC25354552 Page
7 Feb 2019
0
If you know a star"s distance and its brightness, you can figure out the luminosity of a star. You can figure out the temperature by the colour it is a
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 9: Stellar Parallax, Inverse-Square Law

OC25354552 Page
5 Feb 2019
0
We have information about our sun, mostly because we have sent probes to measure things or observe the sun. However, we have information about distant
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 8: AST 201 LECTURE 8

OC25354552 Page
1 Feb 2019
0
A star with a spectrum in the middle (close to where the green light area is) appear white. That is why there is no green stars in the sky. Historicall
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 7: Cygnus X-1, Photon, Astronomical Object

OC25354552 Page
30 Jan 2019
0
The black hole in the centre of our galaxy is actually much larger than cygnus x-1. Some elements tend to escape being devoured by black holes, and the
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 6: Cygnus X-1, Event Horizon, Escape Velocity

OC25354552 Page
29 Jan 2019
0
If you shrank the size of earth while keeping its mass the same means that the escape speed goes up. If you keep crushing the earth smaller and smaller
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 5: Gravitational Lens, Strong Gravity, Equivalence Principle

OC25354552 Page
25 Jan 2019
0
Equivalence principle: no experiment can distinguish a difference between gravity pulling things back to the surface of earth and acceleration. We feel
View Document
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
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 4: AST201 - lecture 4

OC25354552 Page
20 Jan 2019
0
Objects will move with a constant speed and direction unless acted on by an external. You feel gravity every day, every other force you feel (wind, pus
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 2: LIGHT

OC25354552 Page
19 Jan 2019
0
How can you tell if a train has moved: you can be looking out the window, seeing if the landscape moves. If there are no windows, you can hear the trai
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 3: Relativity part 2

OC25354552 Page
15 Jan 2019
0
Time dilation: when someone is moving relative to you, their clock will seem to be running slower. Not only does time slow down, but also length. Thing
View Document
View all Premium Notes (20+)
View all professors (10+)
UTSGAST201H1Bryan GaenslerFall

AST201H1 Lecture Notes - Lecture 1: Stellar Evolution, Thermostat, Degenerate Matter

OC8541953 Page
22 Apr 2017
0
Lecture 1 a very big mystery: the dark universe (january 5th) Identify one piece of evidence for the existence of dark matter: de(cid:448)elop (cid:455
View Document
UTSGAST201H1Bryan GaenslerSpring

AST201H1 Lecture Notes - Lecture 2: Special Relativity, Pearson Education

Michelle Shen6 Page
25 Jan 2018
0
Figure 1 (pearson education, 2008: you fall asleep o(cid:374) a trai(cid:374) , you fall asleep o(cid:374) a floati(cid:374)g space ship , we can only
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Lecture Notes - Special Relativity, Itch

OC2520911 Page
20 Feb 2014
125
Stand still->ball move up and down for everyone. Moving->we see ball doing arc, she sees ball moving up and down. No clock -> know speed and distance t
View Document
UTSGAST201H1Bryan GaenslerWinter

AST201H1 Lecture 11: Building the H-R diagram

OC11512202 Page
9 Feb 2017
20
E(cid:454)plai(cid:374) ho(cid:449) the follo(cid:449)i(cid:374)g i(cid:374)fo(cid:396)(cid:373)ao(cid:374) a(cid:271)out a sta(cid:396) (cid:272)a(cid
View Document
UTSGAST201H1Bryan GaenslerSpring

AST201H1 Lecture Notes - Lecture 1: Bryan Gaensler, Observable Universe, Orbital Speed

OC7652261 Page
7 Jan 2018
0
The lights of the stars we see today travel in the speed of light, which is very fast but not instantaneous. When we see the moon, we see the moon as i
View Document
UTSGAST201H1Bryan GaenslerSpring

AST201H1 Lecture Notes - Lecture 5: Pearson Education, Spacetime, Event Horizon

Michelle Shen5 Page
25 Jan 2018
0
View Document
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
View Document
UTSGAST201H1Bryan GaenslerSpring

AST201H1 Lecture 4: AST201- Lecture 4

Michelle Shen6 Page
25 Jan 2018
0
Figure 2 (credit: prof. gaensler: gravity, from 1687-1916, ne(cid:449)to(cid:374)"s description of gravity changed time to time. Re(cid:373)e(cid:373)(
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 9: Stellar Parallax, Inverse-Square Law

OC25354552 Page
5 Feb 2019
0
We have information about our sun, mostly because we have sent probes to measure things or observe the sun. However, we have information about distant
View Document
UTSGAST201H1Bryan GaenslerWinter

AST201H1 Lecture Notes - Lecture 3: Twin Paradox, Time Dilation, Length Contraction

OC11512202 Page
17 Jan 2017
17
Ast101 lecture 3: time dilation and the twin paradox. The speed of light: light always travels at c (in a vacuum, slightly slower in air, no object wit
View Document
View all (200+)
UTSGAST201H1Michael ReidWinter

AST201H1 Chapter Notes - Chapter 14.1-14.2: Solar Luminosity, Nuclear Fusion, Solar Core

OC418657 Page
15 Apr 2016
24
Most ancient peoples thought of the sun as some type of fire (i. e. a lump of burning coal or wood): eventually ruled out because this could not accoun
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Chapter Notes - Chapter S3: Event Horizon, Gravitational Redshift, Distant Star

OC418658 Page
5 Mar 2016
33
The general theory of relativity explains gravity as a consequence of the structure of space and time. If you launch two probes in opposite directions
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Chapter Notes - Chapter S2: Infinite Mass, Time Dilation, Length Contraction

OC418657 Page
5 Mar 2016
38
Universe consists of matter and energy moving through space with the passage of time. Einstein developed his theory of relativity in two parts: special
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Chapter Notes - Chapter 15: Inverse-Square Law, Dim Stars, Apparent Magnitude

OC418659 Page
15 Apr 2016
22
All stars form in great clouds of gas/dust, and each begins its life with roughly the same chemical composition as the sun: h, he, and. Stars differ in
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Chapter Notes - Chapter 5: Mass Number, Submillimetre Astronomy, Diffraction Grating

OC4186511 Page
15 Apr 2016
19
View Document
UTSGAST201H1Bryan GaenslerWinter

AST201H1 Chapter Notes - Chapter 18.3: Angular Momentum, Degenerate Matter, Electric Charge

OC24248682 Page
15 Apr 2018
0
If gravity in stellar corpse becomes so strong, nothing can prevent the corpse from collapsing under its own weight. Collapses, crushing itself out of
View Document
UTSGAST201H1Ian SheltonSummer

AST201H1 Chapter Notes - Chapter 5: Electric Light

OC9291714 Page
19 Jul 2015
22
View Document
UTSGAST201H1Bryan GaenslerWinter

AST201H1 Chapter Notes - Chapter S3.1-S3.4: Observable Universe, Equivalence Principle, Rocket Engine

OC24248683 Page
15 Apr 2018
0
S3. 1, s3. 2 (only the part called what is curved spacetime? ), Three dimensions of space and one dimension time --> four dimensional combo called spac
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Chapter Notes - Chapter 1: Cosmic Calendar, Usable Fuel, Ecliptic

OC418654 Page
5 Mar 2016
17
Chapter 1: a modern view of the universe. The old belief was in a geocentric universe where everything revolved around the. Earth is a planet in our so
View Document
UTSGAST201H1Michael ReidWinter

AST201H1 Chapter Notes - Chapter 18.3-19.4: Rotating Black Hole, Gravitational Redshift, Event Horizon

OC418654 Page
15 Apr 2016
31
Section 18. 3 black holes: gravity"s ultimate victory. They then said that light from this object would behave like a rock thrown up it would raise, sl
View Document
View all (60+)

Most Popular

Your classmates’ favorite documents.
UTSGAST201H1Bryan GaenslerWinter

[AST201H1] - Midterm Exam Guide - Ultimate 10 pages long Study Guide!

OC115122010 Page
6 Feb 2017
74
Ast101 lecture 3: time dilation and the twin paradox. The speed of light: light always travels at c (in a vacuum, slightly slower in air, no object wit
View Document
UTSGAST201H1Ian SheltonFall

AST201H1- Midterm Exam Guide - Comprehensive Notes for the exam ( 14 pages long!)

OC105000614 Page
5 Oct 2017
0
Wavelength is the distance between two wave peaks. Frequency is the number of times per second that a wave vibrates up and down. This is like water, th
View Document
UTSGAST201H1Bryan GaenslerSpring

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

Michelle Shen119 Page
29 Mar 2018
0
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
View Document
UTSGAST201H1Michael ReidFall

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

OC755883239 Page
29 Nov 2016
24
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
View Document
UTSGAST201H1Jeffrey ReidWinter

AST201H1 Final: AST201 Important notes from each lecture - EXAM STUDY

OC51018222 Page
4 Aug 2015
69
View Document
UTSGAST201H1Bryan GaenslerWinter

AST201H1 Study Guide - Final Guide: Length Contraction, Triple-Alpha Process, Schwarzschild Radius

OC114458512 Page
11 Jun 2017
0
View Document
UTSGAST201H1Michael ReidFall

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

OC755883239 Page
5 Oct 2016
42
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
View Document
UTSGAST201H1Bryan GaenslerFall

AST201H1 Midterm: AST201 Midterm study notes

OC11643159 Page
16 Feb 2017
5
View Document
UTSGAST201H1Bryan GaenslerFall

AST201H1 Final: AST201 Final Exam Notes

OC116431518 Page
8 Apr 2017
0
View Document
UTSGAST201H1Bryan GaenslerFall

AST201H1 Lecture Notes - Lecture 1: Stellar Evolution, Thermostat, Degenerate Matter

OC8541953 Page
22 Apr 2017
0
Lecture 1 a very big mystery: the dark universe (january 5th) Identify one piece of evidence for the existence of dark matter: de(cid:448)elop (cid:455
View Document

Most Recent

The latest uploaded documents.
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 25: Type Ia Supernova, Density, Big Crunch

OC25354552 Page
15 Apr 2019
0
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 26: Cosmic Microwave Background, Horizon Problem, Energy Density

OC25354552 Page
13 Apr 2019
0
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 23: Main Sequence, Cosmic Distance Ladder, Edwin Hubble

OC25354552 Page
30 Mar 2019
0
The stars all have the same age and the stars are all at around the same distance. They are all at around the same distance. Step 1: use radar to deter
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 24: Graph Paper, Nucleosynthesis, Neutrino

OC25354552 Page
30 Mar 2019
0
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 22: Elliptical Galaxy, Disc Galaxy, Cosmic Distance Ladder

OC25354552 Page
21 Mar 2019
0
Irregular galaxies are a result of a collision of two galaxies (mergers. ) When its finish its star bursts, it will probably another disk galaxy. But i
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 19: Light Pollution

OC25354552 Page
18 Mar 2019
0
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 20: Semi-Major And Semi-Minor Axes, Orbital Period, Vera Rubin

OC25354552 Page
17 Mar 2019
0
Johannes kepler: had worked from tycho bache"s data and came up with an accurate description of the motion of the planets. #1: planets orbit the sun in
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 18: Angular Momentum, Degenerate Matter, Tablespoon

OC25354552 Page
10 Mar 2019
0
Topic: the afterlives of massive stars, neutron stars. The finale stage of a massive star"s life. When there is no more core fusion then gravity starts
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture 15: AST201 lecture 13

OC25354552 Page
2 Mar 2019
0
Topic: lifecycle of a 1 solar mass star. The core expanding and cooling slows things down and stops fusion in the sun"s core from happening faster and
View Document
UTSGAST201H1Bryan Gaensler, C. Barth Netterfield, Ilana MacDonaldWinter

AST201H1 Lecture Notes - Lecture 16: Neon Neon, Nucleon, Solar Mass

OC25354552 Page
1 Mar 2019
0
Talking about what happens to a star that is above 8 solar masses, and the difference between a low-mass star and high mass star. When all the helium i
View Document

All Materials (1,800,000)
CA (950,000)
UTSG (70,000)
AST (1,000)
AST201H1 (300)