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Spectroscopy
The study of light emitted by stars to determine their composition, temperature, and movement.
Spectroscope
A tool that splits starlight into a rainbow spectrum to reveal a star's composition, temperature, and movement.
Continuous Spectrum
An unbroken rainbow of all light wavelengths produced by a hot, dense object like an incandescent bulb core.
Absorption Spectrum
A rainbow broken by dark lines created when cool gas absorbs specific wavelengths of light passing through it.
Emission Spectrum
A series of bright colored lines on a dark background produced when hot, glowing gas emits light at specific wavelengths.
Apparent Magnitude
How bright a star appears from Earth.
Absolute Magnitude
The true intrinsic brightness of a star if placed at a standard distance from Earth.
Luminosity
The total amount of light energy a star emits per second.
Parallax
The apparent shift in a star's position when viewed from different points in Earth's orbit, used to measure stellar distances.
Light-Year
The distance light travels in one year (about 6 trillion miles), used to measure vast distances in space.