Explain the formation of interference patterns
Assess the evidence for Newton’s theory of light
Assess the evidence for Huygen’s theory of light
Assess Maxwell’s contribution to the classical theory of electromagnetism
Explain how the spectra of a star is produced, and how it can be used to show the star’s composition
characteristics of stars found from its spectra
surface temp
- determined through Wein’s Law, where wavelength max is determined from the stars spectrum.
- longer wavelengths > cooler temp
- shorter wavelengths > warmer temp
chemical comp
- found by comparing the emission spectra of known elements, with the absorption spectra of a star
- the absorption levels ate present due to the atomic energy level transitions of the atoms in the photosphere
- shared bonds indicate the elements presence
translational velocity
- obtained through red or blue shift
- red-shifted (longer wavelength) it is moving away
- blue-shifted (shorter wavelength) it is moving towards
- the larger the shift, the faster it’s moving
rotational velocity
- determined through the width of the absorption bands
- faster it is rotating, the wider the absorption bands are
density layers
- obtained through the spectra
- wider absorption pattern for more dense (as a more dense star has more collisions)
- this is called collisional broadening
Explain strategies to improve transformer efficiency