Astronomy Chapter 5

Properties of light

light can be a wave and a particle. they have a wavelength and a frequency.

Photons

particles of light

Electromagnetic spectrum

entire range of wavelengths or light

Wavelength

distance between two adjacent peaks

Frequency

number of times per second a wave vibrates up and down

Speed of light

Frequency x wavelength

Spectrum

a prism split light into the rainbow of light

What we can learn from spectra

chemical composition, surface temp, and how fast an object is moving

Continuous spectra

spectrum of a common light bulb spans all visible wavelengths, without interuption

Emission

a thin or low density cloud of warm gas emits light at specific wavelengths that depend of its composition and temperature producing a spectrum with bright emission lights

Absorption

a cooler gas cloud between us and a light bulb can absorb light of specific wavelengths that depend on cooler gas composition and temperature, leaving dark absorption lines in the spectrum

Transparent

materials that transmit light

Opaque

materials that absorb light

Chemical Fingerprints

every kind of atom, ion and molecule has a unique set of energy levels

Continuous Spectrum

densley packed atoms and molecules cannot be considered independent, so they have much more complex set of energy levels

Thermal spectra

thermal radiation all objects emit it

Stefan- Boltzman Law

hotter objects emit more light at all frequences per unit area

Wilen's Law

hotter objects emit photons with a higher average energy

The doppler shift

tells us how fast an object is moving towards or away from us

Reflection

light can bounce off matter

Radio Waves

longest-wavelength light; form of light not sound

Ultra violet

light with wave lengths somewhat shorter than blue light

Gamma rays

shortest wave length