ASTR 103 - Astronomy
Glossary - A
Latest Modification: March 5, 2003
- absolute
- Intrinsic or characteristic to the body, not dependent on distance or position of the observer or the body.
- absolute brightness
- The intrinsic brightness or luminosity, a measure of the rate at which radiant energy is emitted.
- absolute magnitude
- The apparent magnitude a celestial body would have if placed at a distance of 10 pc (32.6 ly) from the Sun.
- absolute zero
- Temperature at which molecules and atoms have a zero average kinetic energy. It corresponds to 0 K on the Kelvin scale, -273.16o C on the Celsius (centigrade) scale, and -459.69o F on the Fahrenheit scale.
- absorption
(of electromagnetic energy)
- The conversion of electromagnetic energy to some other form of energy by matter when electromagnetic radiation is incident upon matter.
- absorption line
- The absence or reduction of radiation at one or several adjacent wavelengths in a continuous spectrum.
- absorption spectrum
- Continuous spectrum interrupted by absorption lines or a continuous spectrum having a number of discrete wavelengths missing or reduced in intensity.
- acceleration
- The time rate of change in a particular direction of the velocity, which can be either the time rate of change of speed or direction, or both.
- acceleration of gravity
- The acceleration imparted to a body by the gravitational field of some small body, planet, star, galaxy, or cluster of galaxies; a measure of the intensity of a gravitational field.
- accretion
- The accumulation of matter in one location, for example, through the action of gravity.
- accretion disk
- A flattened, roughly circular disk of gas or plasma attracted to a star, black hole, or other massive body, often by mass transfer during binary evolution of stars.
- accretion theory
- The formation of a planet, star, or other body by the addition of small pieces of matter to it.
- active galactic nucleus
-
- active galaxy
- Galaxies with active nuclei that are very luminous and emit both thermal and nonthermal radiation.
- active region
- Regions on the Sun, and presumably other stars, that are the centers of intense magnetic fields, plages, sunspots, flares, prominences, etc.
- airglow
- Faint, visible and infrared emission in Earth's upper atmosphere caused by solar radiation.
- albedo
- The fraction of incident light reflected by a body.
- alpha particle
- 4He2 nucleus of the helium atom possessing two protons and two neutrons.
- altazimuth mounting
- Mounting an arrangement of a telescope permitting it to be rotated horizontally and vertically.
- altitude
- The height above the surface of a planet. Also, the name of the astronomical coordinate measuring the angular distance above the horizon.
- amino acid
- Constituents of proteins containing the amino (NH2) and carboxyl (COOH) groups of compounds.
- amplitude
- Maximum displacement from the equilibrium position in wave motion or light curve, etc.
- angstrom (A)
-
- angular momentum
- Measure of the quantity of rotation possessed by a spinning body about an axis or external point.
- angular size
- The angle subtended by an object at a given distance.
- angular velocity
- The rate at which a body rotates as expressed by an angular change of position per unit time.
- annihilation
-
- annular eclipse
- Solar eclipse in which the Moon's disk does not quite cover the Sun's disk, leaving a bright ring of sunlight around the Sun.
- antapex (of the solar motion)
- Point on the sky from which the Sun appears to be receding relative to its stellar neighbors. It is exactly opposite to the apex.
- antimatter
- Matter identical in behavior to ordinary matter but containing the oppositely charged or neutral counterparts of ordinary matter. Example: the proton carries a positive charge; the antiproton carries an equal but negative charge.
- aperture
- Diameter of a telescope objective or radio dish or antenna structure.
- apex (of the solar motion)
- Point on the sky in the constellation Hercules toward which the Sun appears headed relative to its closest stellar neighbors.
- aphelion
- Point in the orbit of a body orbiting the Sun where it is farthest from the Sun.
- apogee
- Point in orbit at which any body circling Earth is farthest from the Earth.
- apparent
- Not intrinsic or a characteristic of a body, but depends on the distance of position of the observer.
- apparent brightness
- The brightness as perceived by an observer at some distance from the radiating body (see also inverse-square law of light).
- apparent magnitude
- Apparent brightness of a celestial body based on a logarithmic scale of brightness.
- apparent solar day
-
- apparent solar time
-
- association
- A physical grouping of young stars, such as the O and B associations or Tauri associations.
- A star
- Stars of spectral type A with surface temperatures of about 7,500 to 10,000 K in whose spectrum the Balmer lines of hydrogen attain their greatest strength.
- asterism
- The configuration of stars or "catch figure" used to identify a constellation. Example: the Big Dipper is the asterism for Ursa Major.
- asteroid
- One of thousands of small rocky-material bodies revolving in orbits, chiefly between Mars and Jupiter in the asteroid belt.
- astrology
- Pseudo-science that claims human events can be predicted from the positions that the Sun, Moon, and planets occupy in the zodiac at different times.
- astrometric binary
- Double star having an invisible companion whose presence is inferred from the wobbly motion of the visible component.
- astrometry
- Division of astronomy dealing with precise determinations of the positions, motions, and parallaxes of astronomical bodies.
- astronomical unit (AU)
- The mean distance between Earth and the Sun (about 150 million kilometers).
- astronomy
- Science that deals with the Universe, its radiation and their descriptions, radiations, movements, structures, physical and chemical characteristics, origin, evolution, and arrangement.
- astrophysics
- Field of astronomy concerned with the physical, chemical, and thermal properties of celestial bodies accessible to direct observation and also inferred from theory.
- asymptotic branch
-
- atmosphere
- The outermost gaseous medium or layers surrounding a planet or a star. Important to its understanding are its thermal structure and chemical composition.
- atmospheric refraction
- The refraction of light entering the Earth's atmosphere from the near-vacuum of space; it is best toward the zenith.
- atom
- The smallest unit of a chemical element possessing the properties of the element (see also subatomic particles).
- atomic mass unit (amu)
- Standard unit that corresponds to one twelfth of the mass of the carbon isotope 12C6 (= 1.6604 x 10-24 g).
- atomic number
- Number assigned to an atom corresponding to the number of protons in its nucleus.
- atomic weight
- Mass of an element in atomic mass units.
- aurora
- Sporadic visible emission in the upper atmosphere most prominent at high latitudes in both hemispheres caused by an influx of atomic particles from the Sun.
- autumnal equinox
- (see also equinoxes).
- azimuth
- Horizontal arc from the north point of the horizon measured clockwise to the object's position projected on the horizon.
Physics & Astronomy Department, George Mason University
Maintained by J. C. Evans; jevans@gmu.edu