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First observational evidence against geocentric model
Some planets were observed to undergo phases, like the Moon does.
Galileo's telescope observation of Venus
Venus goes through all of the phases (crescent, gibbous, etc.)
Spectroscopy in astronomy
They measure the widths of emission and/or absorption lines in a star's spectrum.
Telescopes for low-energy light detection
Radio telescopes
Effect of doubling telescope's primary mirror size on resolution
get better by a factor of 2
Composition of light
electric & magnetic fields
Regions of the light spectrum by energy
Gamma Rays → X Rays → Ultraviolet → Visible → Infrared → Radio
Black-body radiation and star measurement
temperature
Power increase with tripled temperature
increase by a factor of 81 (81x)
Electron transition and light emission
emits light
Telescope resolution measurement
A telescope's resolution is measured in units of arcseconds.
Resolution of a telescope
Depends on the size of the telescope and the wavelength of light being observed.
Kelvin temperature scale
Sets the point where all thermal motion stops equal to a temperature of 0.
Temperature of an object
A direct measure of the amount of microscopic motion within it.
Color of the coolest stars
Appear red.
Constant of a visible light wave
The speed is constant, regardless of the color.
Refracting telescope
Uses lenses to focus light.
X-ray telescope placement
Must be placed in outer space because Earth's atmosphere is opaque to X-rays.
Brightness comparison through filters
Can measure the temperature of a star.
Energy associated with green light
For an electron transition from n=4 to n=2 in hydrogen, it is 10.2 eV.
Type of spectrum produced by the Sun
Continuous (black-body) spectrum.
Wavelength peak of black-body spectrum
If the object's temperature doubles, the peak would be at 300 nm.
Movement indication from light source
If the measured wavelength of green light is 488.5 nm, it is moving away from you.
Spectrum observation above Earth's atmosphere
Would show slightly fewer absorption lines compared to ground-based observations.
Dark lines in observed spectrum
Reveal the chemical composition of the cool gas in front of a hot light bulb.