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What do spectral lines do?
They help decode what elements are in stars/galaxies
Doppler effect
Motion impacts how light waves look. They can either be spread out/bunched up depending on whether the light source is away/toward us
What type of relationship do wavelength and frequency have?
They have an inverse relationship.
Radial velocity
Movement toward/away from an observer.
Does a wave source moving toward you increase or decrease wavelength
Decrease
Blueshift
When a wave moves toward the blue end of this spectrum as the wavelength gets shorter
Redshift
When a wave length moves toward the red end of the light spectrum as the wavelength gets longer
Doppler equation
Δλ/λ=𝑣/𝑐
What happens to dark lines as a star approaches/recedes
They also widen/shrink
Electron
Negatively charged particle. Balanced by the same amount of positive charge
Nucleus
Positive-charged particle. Majority of mass is stored in nucleus
Hydrogen
Most common element in the sun/stars. One proton in nucleus, one electron orbiting the nucleus. Their attraction to each other produces the orbit.
Helium
Two protons in nucleus, two orbiting it, two nucleus. 2nd most common element
What determines an element?
The amount of protons in a nucleus
Isotopes
Elements that have the same protons but different neutrons
The Bohr Model
In order for atoms to move to orbits, it must shift its energy level by either emitting a proton or absorbing a proton
Ground state
Innermost orbit. When atoms have the lowest possible energy
Excitation
When an atom absorbs a proton and moves to a higher, outermost orbit. Doesn’t last for long.
Why do dark lines exist?
As light is remitted, it’s spread out in all directions, some directions not visible to the observer’s eye, causing these lines
How can absorption lines give info on temperature?
Absorption lines showcase electrons jumping to an outermost orbit. The hotter the temperature of a star, the more likely it is to jump to an outermost orbit.
Ionization
When an electron gets REALLY excited, it tends to leave the nucleus
Ion
Atom without an electron due to ionization
Ionization energy
The amount of energy needed to remove electrons from atoms in ground state
Electromagnetic Spectrum Mnemonic
Raging Martians Invaded Venus Using X-ray Guns. LOWEST TO HIGHEST FREQUENCY
R – Radio waves More than 109
M – Microwaves 106–109 nm
I – Infrared 103–106 nm
V – Visible light 400–700 nm
U – Ultraviolet 20–400 nm
X – X-rays 0.01–20 nm
G – Gamma rays less than 0.01 nm
What type of relationship do frequency and energy have?
Proportional relationship
Inverse square law
As light leaves its source, the light gets weaker and weaker
What speed to waves move at?
At the speed of light
Frequency
Number of cycles/hills per second/in a wavelength
Frequency of light
c = fλ
Why can’t we see gamma rays, x-rays, and ultraviolet
They are blocked by gases in Earth’s atmosphere
Refraction
When light bends because it passes from one transparent material to another. This is used in telescope lenses/glasses
Dispersion
Its wavelength and material influence how much light bends
Continuous spectrum
The rainbow spectra
Absorption Spectrum
Dark lines projected onto the continuous spectrum. Missing colors. This happens when white light passes through cool, thing gas
Emission Spectrum
Bright lines. Happens with HOT thin gas
What is temperature’s impact on lines?
It can make them brighter or darker
What relationship do temperature and wavelength have?
Shorter wavelength=higher temperature. Inverse relationship
What are the characteristics of short wavelengths?
Hot temperature, high energy, high frequency, blue
Wien’s law
λmax=b/T. The hotter the object, the shorter the wavelength
Energy flux
Power emitted by a star
Stefann-Boltzmann law/Emitted energy flux
Hotter the star, more energy it has. I = σT4
What determines the type of electromagnetic radiation emitted by the sun?
Temperature. It gets a temper if they don’t listen to what she determines
What creates electromagnetic radiation?
The movement of molecules/atoms creates this
What is the spectrum of visible light?
400 nm (blue) to 700 nm (red)