ASTR 103 - Astronomy

Glossary - S


Latest Modification: March 5, 2003

saros
Period of 18 years and 11 days in which eclipses repeat themselves.
satellite
 
Schwarzschild radius
Critical radius of the event horizon reached by a gravitationally collapsing body between the point of visibility as a highly compressed body and nonvisibility as a black hole.
scattering
 
scintillation
Twinkling effect observed when light from a very small radiating source passes through a turbulent medium.
sedimentary rocks
 
seeing
The astronomical term used to denote our atmosphere's influence on image quality.
seismic
Pertaining to earthquakes.
semimajor axis (of an ellipse)
 
Seyfert galaxy
class of spiral galaxy that exhibits intense, irregular, electromagnetic radiations within a small active nucleus.
shock wave
conical pattern in space produced when an object moves at supersonic speed in a gaseous medium and creates a disturbed wake.
short-period comet
comet that orbits the Sun in a period less than about 200 years.
sidereal day
 
sidereal month
 
sidereal period
one complete revolution of a celestial body with respect to a fixed point in the heavens, such as a star.
sidereal time
 
sidereal year
 
signs of the zodiac
twelve equally spaced constellation divisions centered on the ecliptic, through which the Sun passes monthly in succession.
silicates
mineral compositions largely containing silicon and oxygen.
solar activity
 
solar constant
rare at which solar radiation is received on a unit surface perpendicular to the incident radiation per unit of time at Earth's mean distance, just outside Earth's atmosphere.
solar luminosity (L.)
 
solar masses (M.)
 
solar nebula
fragmented portion of an interstellar cloud that has begun to contract under its own gravitation, eventually leading to the formation of a planetary system.
solar radii (R.)
 
Solar System
 
solar wind
continuous stream of charged particles (mostly protons and electrons) ejected radially from the Sun at high velocities.
solid
that state of matter in which the constituent
particles maintain a permanent relation to each other.
solstice
 
space-time
four-dimensional world of space and time as visualized in the theory of relativity. An event is located in the space-time continuum analogous to a point in three-dimensional space.
space velocity
true motion of the star in space relative to the Sun.
special relativity
part of Einstein's theory relating to observers moving uniformly with respect to each other.
speckle photography
technique of taking very short exposures of a star, which freezes the image in a set position on each photograph, and computer-analyzing the many photographs to obtain the star's unsmeared, better-resolved image.
spectral class
 
spectral type
 
spectrogram
photographic plate on which the spectrum of an object is recorded by the telescope.
spectrograph
basically the same as the spectroscope except that the eyepiece is replaced by a photographic plate for recording the spectrum.
spectroheliogram
photograph of the Sun taken with a spectroheliograph.
spectroheliograph
spectrograph modified to photograph the solar disk or the chromosphere in the light of a single spectral line, either in the red hydrogen alpha line or the violet H or K line of calcium.
spectroscope
optical instrument containing a prism or grating with appropriate lenses to permit direct viewing of the spectrum of a radiating source.
spectroscopic binary
double star whose components are not observed separately in a telescope but whose binary character is revealed by the periodic Doppler shift of spectral lines.
spectroscopic parallax
derivation of the star's distance (or parallax) from its apparent magnitude and its absolute magnitude on the basis of its luminosity and spectral characteristics.
spectroscopy
that branch of physics and astronomy dealing with the color or wavelength composition of composite or white light.
spectrum
spreading out of the energy of a radiating source into its component wavelengths by means of a prism, grating, or other dispersing device.
spectrum-luminosity diagram
Hertzsprung-Russell diagram that exhibits the relationship between the absolute magnitudes of stars and their spectral classes.
speed
 
spherical aberration
failure of light rays striking all parts of a lens or a mirror with a spherical surface to converge at the same focal setting.
spicule
small spikeline protrusion arising within the chromosphere.
spiral arms
 
spiral galaxy (normal)
large system of stars and interstellar matter having the shape of a flattened disk with outlying spiral arms.
s process
 
standard time
 
star
 
state of motion
the motion of a body is some frame of reference as denoted by its velocity.
static cosmological model
 
steady-state cosmology
model in which it is assumed that the density of matter within the Universe remains constant as the Universe expands.
Stefan-Boltzmann law
Formula that relates the emission (E) of electromagnetic radiation by a blackbody to the fourth power of its temperature (T), E oc T4.
stellar association
spare aggregation of young population I stars having a common origin and found in the outer gas-dust regions of the Galaxy.
stellar cluster
 
stellar evolution
 
stellar model
 
stratosphere
narrow atmospheric zone that lies above the lowest level of Earth's atmosphere, the troposphere. It extends from about 11 to 25 kilometers above sea level and has a constant temperature of -55oC.
strong nuclear force
nuclear "glue" or binding force that holds the nucleons together against the disruptive repulsive force of the positively charged protons. It operates within the nuclear domain (-10-13 centimeter).
subatomic particle
the constituent parts of the atom, such as the electron, proton, neutron, etc.
subduction zone
 
subdwarf star
 
subgiant star
 
summer solstice
 
Sun
 
sunspot
Dark marking visible on the Sun's surface. Although the sunspot temperature is about 4500 K, it appears dark by comparison with the brighter and hotter photospheric background.
sunspot cycle
 
sunspot group
 
supercluster
A cluster of clusters of galaxies.
supergiant
Large massive star of the greatest luminosity.
superior conjunction
Position of a superior planet, as viewed from Earth, when it is in the same direction as the Sun and farthest from Earth.
superior planet
Planet whose orbit lies outside Earth's orbit.
supernova
Exploding star that suddenly attains a luminosity up to 100 million times the Sun's brightness.
surface gravity
Acceleration at the surface of a body arising from its gravitational force.
S (seismic) waves
Transverse waves of an earthquake that cause Earth's material to vibrate perpendicular to the direction of the waves' travel. Also called secondary or shear waves.
synchronous
Locking of the rotation of a spinning body with its orbital revolution in which the rotation is an integer or simple fraction of its revolution.
synchrotron radiation
Continuous polarized radiation emitted by fast-moving electrons spiraling around the magnetic lines of force.
synodic month
Period of the Moon's phases, 29.53 days.
synodic period
Time between consecutive similar configurations of a planet; for example, between successive inferior conjunctions or oppositions.


Physics & Astronomy Department, George Mason University
Maintained by J. C. Evans; jevans@gmu.edu