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 |