Star
- Self-luminous, gaseous objects that fuse elements
 - Obtain energy from nuclear fusion
 - Considered a star when it can sustain itself through nuclear reactions (making its own energy)
 - How long it takes a star to form depends on its mass
 - Twinkle due to the atmosphere
 - The brightest stars are not the ones close to us
 - A star is said to be true if it becomes hot enough to fuse protons to form helium
 
Measuring the Characteristics of Stars
| Characteristic | Technique | 
|---|---|
| Surface temperature | Determine the colour (very rough) | 
| Measure the spectrum and get the spectral type | |
| Chemical composition | Determine which lines are present in the spectrum | 
| Luminosity | Measure the apparent brightness and compensate for distance | 
| Radial velocity | Measure the doppler shift in the spectrum | 
| Rotation | Measure the width of spectral lines | 
| Mass | Measure the period and radial velocity curves of spectroscopic binary stars | 
| Diameter | Measure the way a star's light is blocked by the Moon | 
| Measure the light curves and doppler shifts for eclipsing binary stars | 
Measuring Distance from Earth
- Parallax
- Rely only on geometry
 
 - Using brightness measurements
- Look at the star, determine it's color spectrum (good indication of it's actual brightness)
 - Compare the actual brightness with the apparent brightness, they can determine the distance
- It's apparent brightness will be dimmer
 
 
 - Using an H-R diagram
- Observe distant star's apparent magnitude and spectral type
 - Spectrum gives luminosity class
 - Spectral class and luminosity class gives a brightness independent of distance
 - Distance-magnitude relationship gives you distance
 
 
Mass
- Knowing the mass of a star helps us estimate how long it will shine and what its ultimate fate will be
 - The smallest mass that a true star can have is about $\frac{1}{2}$ that of the Sun
 - Massive stars live for a short amount of time (die faster)
- They are brighter
 - The brighter they are, the faster they burn
 - More mass --> hotter core and denser core
- Makes fusion process happen faster
 
 
 
Luminosity
- Luminosity
 - How much light a star is emitting
 - Photometry is used for measuring apparent magnitudes
 
Types of Stars
- H-R diagram helps plot luminosity against temperature or spectral type
 - Main sequence stars
- Most populated
 - Generally hotter and more luminous
 
 - Giant stars
- More luminous
 - More red
 
 - Supergiant stars
- Even more luminous
 
 - White dwarfs
- Very faint but still hot
 
 - Neutron Stars
 
Colour and Temperature
| Star Colour | Approximate Temperature | 
|---|---|
| Blue | 25,000 K | 
| White | 10,000 K | 
| Yellow | 6000 K | 
| Orange | 4000 K | 
| Red | 3000 K |