Astronomy and Solar Physics Vocabulary

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Vocabulary terms and definitions related to light, telescopes, and solar activity from the lecture transcript.

Last updated 4:51 PM on 5/13/26
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20 Terms

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electromagnetic spectrum

the complete range of electromagnetic radiation from radio waves to gamma rays, including the visible spectrum.

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Photon

individual packet of electromagnetic energy that makes up electromagnetic radiation.

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Spectroscopy

the study of the way in which atoms absorb and emit electromagnetic radiation.

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Continuous spectrum

spectrum in which the radiation is distributed over all frequencies, not just a few specific wavelengths.

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Absorption spectrum

dark line in an otherwise continuous bright spectrum, where light within one narrow frequency range has been removed.

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Emission spectrum

the pattern of spectral emission lines produced by an element.

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Doppler effect

any motion induced change in the observed wavelength of a wave.

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Refracting telescope

a telescope that uses a lens to gather and focus light from a distant object.

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Chromatic aberration

the tendency for a lens to focus red and blue light differently, causing images to become blurred.

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Reflecting telescope

a telescope which uses a mirror to gather and focus light from a distant object.

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Radio telescope

Large instrument designed to detect radiation from space at radio wavelengths.

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Photosphere

the visible surface of the sun, lying just above the uppermost layer of the sun's interior.

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Chromosphere

the sun's lower atmosphere, lying just above the visible atmosphere.

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Corona

the tenuous outer atmosphere of the sun, which lies just above the chromosphere.

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Solar wind

an outward flow of fast moving charged particles from the sun.

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Sunspot

an Earth-sized dark blemish found on the surface of the sun.

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Prominence

loop or sheet of glowing gas ejected from an active region on the solar surface.

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Solar flare

Massive, sudden explosions on the sun’s surface that release intense bursts of radiation into space.

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Aurora

event that occurs when atmospheric molecules are excited by incoming charged particles from the solar wind, then emit energy as they fall back to their ground state.

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Nuclear fusion

mechanism of energy generation used in nuclear reactors on Earth. Heavy nuclei are combined into heavier ones, releasing energy in the process.