AST-1A Lecture Notes - Lecture 30: Roman Numerals, Low Mass, Fusion Power

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School
Department
Course
Professor
Introduction to the Solar System
Notes
Joseph Yang
Patterns among Stars
Most of the very brightest stars are reddish colour
There’s a general trend to luminosities and colours: brighter ones are white with a bit of
blue ting, modest are yellow and dimmest are red
Colours tell us about surface temperature
H-R diagrams are one of the most important tools
Horizontal axis rep surface temperature: decreases from left to right
Vertical axis rep stellar luminosity
Stars near the upper left are hot and luminous, and stars near upper right are cool
and luminous
Also provides info on stellar radii
More luminous = larger in size
Patterns in HR Diagrams
Most stars fall under main sequence: upper left to lower right
Supergiants are located in the upper right
Giants are just below super giants
Dwarf stars are located in the lower left
Luminosity Classes
Classified with a roman numeral
I for supergiants
III for giants
V for main sequence
II and IV for others
Complete Stellar Classification
A stars spectral type (OBAFGKM)
Luminosity class (roman numeral)
Our sun is G2 V
Main Sequence Stars
Stellar masses decrease downward
Low mass stars are more common
Mass is important attribute of a hydrogen fusing star
Mass determines balance point
Very luminous star must be very large or have a vary high surface temperature
Not only main sequence stars follow this simple relationship between mass, temp,
and luminosity
Doesn’t hold for giants, super giants, or white dwarfs
Lifetime of Main Sequence Stars
Stars are born with limited amounts of hydrogen
Main sequence lifetime: when a star is hydrogen fusing
Massive stars have shorter lives
Dependent on both its mass and luminosity
Mass determines how much hydrogen fuel is initially in the core
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Document Summary

Most of the very brightest stars are reddish colour. There"s a general trend to luminosities and colours: brighter ones are white with a bit of blue ting, modest are yellow and dimmest are red. H-r diagrams are one of the most important tools. Horizontal axis rep surface temperature: decreases from left to right. Stars near the upper left are hot and luminous, and stars near upper right are cool. Also provides info on stellar radii and luminous. Most stars fall under main sequence: upper left to lower right. Supergiants are located in the upper right. Dwarf stars are located in the lower left. Mass is important attribute of a hydrogen fusing star. Very luminous star must be very large or have a vary high surface temperature. Not only main sequence stars follow this simple relationship between mass, temp, and luminosity. Doesn"t hold for giants, super giants, or white dwarfs. Stars are born with limited amounts of hydrogen.

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