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- absolute magnitude
- the brightness of an object that would be measured by an observer if the
object was 10 parsecs
away. It is a measure of the object's luminosity.
- absorption line spectrum
- dark lines in a continuous spectrum that are produced by cool, thin
(low-pressure) gases. Made by electrons jumping up farther from the nucleus.
- acceleration
- a change in motion = (the velocity
change)/(time interval of change). It involves a change in the speed (increase
or decrease) OR direction OR both speed and direction.
- accretion disk
- disk of gas that forms around a massive object as material spirals onto
the massive object. Accretion disks around white
dwarfs, neutron
stars, and black
holes form when material is drawn off a nearby normal or giant star.
Accretion disks around neutron
stars and black
holes can be hot enough to radiate X-rays.
- active galaxy
- luminous galaxy that produces most of its energy from a very compact
source at its center. It has a non-thermal continuous spectrum. The energy is
coming from an accretion disk of gas around a supermassive black hole at the
nucleus of the galaxy.
- adaptive optics
- a technique that compensates for atmospheric turbulence by quickly
adjusting the light path in the optics. This removes seeing effects and
enables the telescope to achieve much better resolution, closer to its
theoretical resolving
power.
- altitude
- position on the celestial sphere that is the number of degrees an object
is above the nearest horizon. Varies from 0° at horizon to 90° at zenith.
Vertical position of an object.
- angular momentum
- a measure of the amount of spin or orbital motion an object has. It is
proportional to the mass of the object multiplied by its radius multiplied by
its spin or orbital speed.
- angular diameter
- see angular
size.
- angular size
- the apparent size of an object measured by the angle between two lines of
sight along each side of an object. An object's actual linear diameter can be
found from the angular size if the distance is already known. The
linear diameter = (2p/360°) × (its distance × angular
size in degrees).
- annular eclipse
- a type of solar
eclipse that happens when the Sun and Moon are exactly lined up but the
Moon is too far away from the Earth to totally block the Sun's surface. A ring
(annulus) of sunlight is seen around the dark Moon (contrast with total
solar eclipse).
- aphelion
- point in an object's orbit around the Sun that is furthest from
the Sun.
- apparent magnitude
- the apparent brightness of an object measured by an observer at an
arbitrary distance away.
- arc minute
- a small angle unit = 1/60th of a degree.
- arc second
- a tiny angle unit = 1/3600th of a degree = 1/60th of an arc
minute.
- asteroid
- boulder to mountain-sized piece of rock remaining from the early solar
system. The largest asteroid is only 1000 kilometers across but most are much
smaller.
- astrology
- a non-scientific belief system in which the positions of the planets among
the stars are thought to hold the key to understanding what you can expect
from life.
- astronomical unit
- (A.U.): average distance between the Earth and the Sun (149.6 million
kilometers). Used for interplanetary distances.
- astronomy
- a discipline that uses the scientific method to understand the physical
universe (usually beyond the Earth's atmosphere).
- astrophysics
- a branch of astronomy that deals with the physical properties and
interactions of celestial bodies---the application of the principles of
physics to celestial bodies and phenomena.
- aurora australis
- aurorae
seen in the southern hemisphere.
- aurora borealis
- aurorae
seen in the northern hemisphere.
- aurorae
- light displays produced by molecules and atoms high up in an atmosphere.
The gas particles are excited by collisions with solar wind particles that
were deflected by the planet's magnetic field toward the magnetic poles of the
planet.
- autumnal equinox
- specific moment in the year (on September 22) when the Sun is directly on
the celestial equator, moving south of the celestial equator.
- azimuth
- position on the celestial sphere that is the number of degrees along the
horizon away from the exact north point. Exact North = 0°, exact East = 90°,
exact South = 180°, exact West = 270°, exact North = 360° (or 0°). Horizontal
position of an object.
Glossary links (select a letter for definitions of astronomy terms beginning
with that letter):
A
- B -
C -
D -
E -
F -
G -
H -
I -
J -
K -
L -
M -
N -
O -
P -
Q -
R -
S -
T -
U -
V -
W -
X -
Y -
Z
last update: 06 August 1999
Nick Strobel -- mailto:strobel@lightspeed.net
(661) 395-4526
Bakersfield College
Physical Science Dept.
1801
Panorama Drive
Bakersfield, CA 93305-1219