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Astronomical Measurements

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Solar Mass (MM_\odot)

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Solar Mass is a standard unit of mass in astronomy equivalent to the mass of the Sun. It is often used to express the mass of other stars or galaxies.

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Parsec

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A parsec is a unit of distance used in astronomy, equivalent to about 3.26 light-years, defined as the distance at which one astronomical unit subtends an angle of one arcsecond.

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Spectral Class

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The spectral class of a star is a classification system that categorizes stars based on their spectral characteristics, which correspond to surface temperatures and other stellar properties.

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Redshift (z)

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Redshift is a measure of how much the wavelength of light or other electromagnetic radiation from an object has increased. It can be used to determine the relative speed and distance of galaxies.

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Bolometer

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A bolometer is an instrument used in astronomy to measure the power of incident electromagnetic radiation via the heating of a material with a temperature-dependent electrical resistance.

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Julian Date (JD)

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Julian Date is a continuous count of days since the beginning of the Julian Period used primarily by astronomers to avoid confusion with dates in historical timekeeping.

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Astronomical Unit (AU)

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The astronomical unit is the average distance from Earth to the Sun, approximately 149.6 million kilometers. It's a convenient measure for distances within our solar system.

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Hertz (Hz)

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Hertz is the unit of frequency in the International System of Units (SI), used to measure the number of cycles per second of a periodic phenomenon, such as waves.

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Light-year

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A light-year is a measurement of distance that represents how far light travels in one year. It is commonly used to express astronomical distances between celestial objects.

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Magnitude

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Magnitude is a measure of the brightness of a celestial object as seen from Earth. The scale is logarithmic and inverted; a lower number indicates a brighter object.

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