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TermMeaning
Abberation of starlightThe tiny apparent displacement of stars resulting from the motion of the Earth though space.
Absolute magnitudeThe magnitude that would be assigned to a star if it were placed at a distance of 10 parsecs (or 32.6 light years) from the observer. The sun, for example, has an absolute magnitude of 4.7.
Absolute visual magnitudeThe absolute magnitude of an object measured through a special yellowish filter that approximates the visual range of the human eye.
Absorption nebulaA nebula seen in silhouette as it absorbs light from behind; also called a dark nebula.
Achromatic lensA lens that transmits white light without dispersing it into a color spectrum. It usually consists of two component parts, cemented together to form one unit.
AlbedoPercentage of light reflected by a body, such as a planet, from the total amount of light falling on it.
AltitudeAngular distance between the horizon and given object, measured along a vertical circle.
AnalemmaThe figure 8 representing the equation of time and the variation of the sun’s altitude in the sky during the course of a year.
AngstromA unit of wavelength or distance, equivalent to 1/10,000 micrometer or 1/10,000,000,000 meter.
Annular eclipseAn eclipse of the central portion of the solar disk; an outer ring shows.
AphelionThe point on a planet’s orbit farthest from the Sun.
ApogeePoint on the moon’s orbit farthest from the Earth.
ApolloThe name assigned to the U.S. project whose mission was to land men on the moon. Also the name of the vehicles used. Apollo II landed Neil Armstrong and Edwin Aldrin on the moon on July 20, 1969.
Apparent magnitudeMagnitude as seen by an observer.
Apparent solar timeTime determined by the actual position of the sun in the sky; corresponds to time on most sundials.
Ascending NodeThe point in the Moon's orbit where it rises above the ecliptic.
AsterismA noticeable pattern of stars that makes up part of one or more constellations; not a constellation itself.
AsteroidA minor planet, smaller than any major planet in our solar system; not one of the satellites (moons) of a major planet such as the Earth or Jupiter.
Astronomical unitThe average distance between the Earth and the sun 93 million miles or, more exactly, 92,955,700
AuroraA diffused glow of light in the form of curtains, or bands, seen at high latitudes (70ºN or 70ºS). The glow is due to the interaction between the solar wind and the particles in the Earth’s atmosphere. The Aurora in the northern hemisphere is known as the Aurora Borealis, or northern lights; in the southern hemisphere it is known as the Aurora Australis, or southern lights.
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