spectrometer
spect
ˈspɛkt
spekt
ro
rɑ
raa
me
mə
mē
ter
tɜr
tēr
/spɛktɹˈɒmÉĒtɐ/

āχāĻ‚āϰ⧇āϜāĻŋāϤ⧇ "spectrometer"āĻāϰ āϏāĻ‚āĻœā§āĻžāĻž āĻ“ āĻ…āĻ°ā§āĻĨ

01

āĻ¸ā§āĻĒ⧇āĻ•āĻŸā§āϰ⧋āĻŽāĻŋāϟāĻžāϰ

a scientific instrument used to measure and analyze the properties of light over a specific range of wavelengths
āωāĻĻāĻžāĻšāϰāĻŖ
Astronomers use spectrometers to study the spectra of stars and galaxies, revealing information about their chemical composition and temperature.
āĻœā§āϝ⧋āϤāĻŋāĻ°ā§āĻŦāĻŋāĻœā§āĻžāĻžāύ⧀āϰāĻž āύāĻ•ā§āώāĻ¤ā§āϰ āĻāĻŦāĻ‚ āĻ—ā§āϝāĻžāϞāĻžāĻ•ā§āϏāĻŋāϰ āĻŦāĻ°ā§āĻŖāĻžāϞ⧀ āĻ…āĻ§ā§āϝāϝāĻŧāύ āĻ•āϰāϤ⧇ āĻ¸ā§āĻĒ⧇āĻ•āĻŸā§āϰ⧋āĻŽāĻŋāϟāĻžāϰ āĻŦā§āϝāĻŦāĻšāĻžāϰ āĻ•āϰ⧇āύ, āϝāĻž āϤāĻžāĻĻ⧇āϰ āϰāĻžāϏāĻžāϝāĻŧāύāĻŋāĻ• āĻ—āĻ āύ āĻāĻŦāĻ‚ āϤāĻžāĻĒāĻŽāĻžāĻ¤ā§āϰāĻž āϏāĻŽā§āĻĒāĻ°ā§āϕ⧇ āϤāĻĨā§āϝ āĻĒā§āϰāĻ•āĻžāĻļ āĻ•āϰ⧇āĨ¤
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āύāĻŋāĻ•āϟāĻŦāĻ°ā§āϤ⧀ āĻļāĻŦā§āĻĻ
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āĻ…ā§āϝāĻžāĻĒ āĻĄāĻžāωāύāϞ⧋āĻĄ āĻ•āϰ⧁āύ