Glossary
| Altitude |
The angular distance, usually measured in
degrees, of an object above the horizon. |
| Apparition |
An appearance in astronomy, the period of
observation of a planet,
or comet. |
| Aphelion |
The point where an object in orbit around the
sun is farthest from it. |
| Apollo |
U.S. space program that included six piloted
lunar landings between 1969 and 1972. |
| Apogee |
The point where an object in orbit around the
Earth is farthest from it. |
| Aurora |
Regions of glowing gas in the upper atmosphere
whose molecules are stimulated to emit light by
collisions with streams of electrons. Known popularly as the northern
lights. |
| Asteroid |
A mostly rocky body less than 620 miles (1,000
kilometers) across that orbits the sun more
accurately called a minor planet. Most asteroids orbit the sun between
Mars and Jupiter. Asteroids are the source of most meteorites. |
| Astrology |
An ancient system of beliefs that attempts to
explain or predict human actions by the position and
interaction of the sun, moon, and planets. It is not a science. |
| Astronomical
twilight |
The time when the sun is 12 to 18 degrees below
the horizon. |
| Astronomical
unit (AU) |
The average Earth-sun distance, equal to 149.60
million kilometers or 92.96 million miles. |
| Asterism |
A noticeable pattern of
such as the Big Dipper or the Pleiades, that is part
of a larger constellation. |
| Axis |
An imaginary line passing through the center of
a body, such as a planet, around which that body spins. |
| Azimuth |
The angular distance, usually measured in
degrees, of an object's direction along the horizon
starting from north (0° or 360°) through east (90°), south
(180°), and west (270°). |
| Binary star |
A system containing two or more stars
in orbit about one another. |
| Blue moon |
A popular term denoting the second full moon to
occur in a calendar month. Blue moons recur every 2.7
years on average with about 37 typically occurring each century.
Through 2010 the blue moon months are July 2004, June 2007, and December
2009. Blue moons can occur twice in years where
February, the shortest month, has no full moon this
next happens in 2018. |
| Bolide |
A fireball that breaks
up during its passage through the atmosphere. |
| Cassini |
U.S. mission to Saturn, launched in 1997 and,
following successful flybys of Venus (1998, 1999),
Earth (1999) and Jupiter (2001), due to arrive at Saturn in 2004.
It will drop the Huygens atmospheric probe into the atmosphere of
Saturn's largest moon, Titan, in early 2005. Cassini-Huygens web site Cassini Project information at NSSDC |
| Chaos |
In its scientific usage, the irregular motion or
dynamics of physical systems. Chaotic systems show two
defining characteristics -- periods of order interspersed with
randomness and evolution that is extremely sensitive to initial
conditions. Chaotic behavior is endemic to most, if
not all, physical systems, including the atmosphere
and solar system. |
| Clementine |
A global mapping mission to the moon launched in
1994 by the U. S. Department of Defense, with science
support from NASA. Clementine web site Clementine information at NSSDC |
| Comet |
A small body made of ice and rock that orbits
the sun, usually much less than 62 miles (100
kilometers) across. As it nears the sun it usually brightens and
develops a gaseous halo, or coma, and a tail of gas and dust. Most
comets travel in very elongated orbits that keep them
far from the inner solar system. International Comet Quarterly comet information site Comet Observation Home Page |
| Conjunction |
The alignment of two celestial bodies that
occurs when they share similar angles from the sun as
measured along the ecliptic. This is also roughly when the bodies
appear closest together in the sky. Inferior conjunction: That point in the motions of the
planets Mercury and Venus at which they pass between
Earth and the sun. Superior conjunction: That point in the motions of
Mercury and Venus at which they appear in line with
the sun on the far side of their orbits as viewed from
Earth. With the sun: That point in the motions of the superior
planets at which they appear in line with the sun as
viewed from Earth. |
| Constellation |
One of eighty-eight regions into which
astronomers divide the sky, based mainly on earlier
divisions formed by historical and mythological figures of Greek and
Roman tradition. |
| Corona |
The outermost atmosphere of the sun. It is
normally hidden by the sun's glare, but can be seen
during total solar eclipses or with the aid of coronagraphs.
The corona is an extremely hot (up to two million Kelvins), tenuous
(about a billion electrons per cubic centimeter), gas
arrayed in nearly radial streamers and extending
millions of miles from the solar surface. Its shape varies from
spherical at the peak of the solar activity cycle to
elliptical at the minimum. |
| Coronagraph |
A telescope in which an opaque disk blocks light
from the solar surface it is thus able to reveal the
faint solar corona and objects such as stars, planets and comets that lie very close to the sun. In effect, a
coronagraph produces an artificial total solar eclipse. |
| Coronal hole |
A large, tenuous, low temperature region in the
solar corona from which extreme ultraviolet and
x-ray emission is unusually low. Coronal holes are
often found at the sun's poles and persist for about ten solar
rotations. High speed (up to 1,000 kilometers per
second) components of the solar
wind are known to originate from coronal holes. |
| Coronal Mass Ejection (CME) |
Eruptive events in the sun's corona
that result in its most rapid and dramatic changes.
CMEs can carry up to 10 billion tons of plasma traveling
at speeds as high as 2,000 kilometers per second. Three or more may
occur on a typical day during the sun's activity
maximum, with this rate dropping to about one every
ten or so days at solar minimum. They are commonly associated with
eruptive prominences and long-lasting soft x-ray
events, and sometimes with optical flares and hard x-ray
events as well. The faster CMEs are associated with Type II and IV radio
bursts. CMEs resemble smoke rings in satellite coronagraph images. Those directed toward the Earth expand symmetrically around the sun and are termed " halo" events. Such CMEs can excite geomagnetic storms as they sweep past Earth. These storms have been linked to satellite communication failures and, in extreme cases, can induce electric currents that damage electric power transmission equipment. |
| Double star |
Two stars that appear close
to one another. They can be physically associated (a
binary) or simply appear together from the point of view of an observer on Earth. |
| Earthshine |
A blue-gray light seen during the moon's
crescent phases on the portion not illuminated by the
sun. The sunlit portion of the Earth is the source. Earthshine Project |
| Eclipse,
lunar |
An event during which the moon enters into the
shadow of the Earth as seen from some locations on
Earth. Penumbral lunar eclipse: A lunar eclipse in which the
moon remains entirely in the penumbral shadow of the
Earth. Partial lunar eclipse: A lunar eclipse in which the moon
partially enters the umbra of the Earth's shadow. Total lunar eclipse: A lunar eclipse in which the moon
passes completely into the umbra of the Earth's shadow. |
| Eclipse,
solar |
An event during which the moon passes in front
of the sun as seen from some locations on Earth. Partial solar eclipse: A solar eclipse in which the
umbral shadow of the moon completely misses the Earth,
but the penumbral shadow does not. At locations
outside of the central track of total, annular, and hybrid eclipses the
eclipse is commonly said to be partial since maximum obscuration of the
sun never occurs. Total solar eclipse: A solar eclipse in which the moon
entirely covers the sun. Annular eclipse: A solar eclipse in which the moon
covers all but a thin ring, or annulus, of the sun. Hybrid eclipse: A solar eclipse that would otherwise be
classified as annular but for a small region along the
eclipse's central track that experiences a short
total eclipse. |
| Ecliptic |
The apparent yearly path of the sun through the
sky. Since this apparent motion is actually a
reflection of Earth's movement, the ecliptic also marks the plane
of Earth's orbit. The moon and planets also roughly follow this path. |
| Electrophonic
sounds |
Sound produced through the conversion of radio
energy at audible wavelengths by the vibration of
objects near the observer, such as hair or eyeglasses. Meteors,
lightning and the aurora can produce sound in
this way. Global Electrophonic Fireball Survey Colin Keay's home page |
| Equinox |
The date of the year at which the sun's rays
illuminate half the Earth, from pole to pole neither
the north pole nor the south pole is angled into the sun. This
phenomenon occurs on two days of the year, near March 21 and September
23. On these dates, the hours of daylight equal the
hours of night (hence the name, meaning " equal
night"
). The March equinox is considered the first day of spring in the
northern hemisphere the September equinox the first day of fall. |
| Farside |
The side of the moon always turned away from
Earth. |
| Fireball |
An extremely bright meteor,
usually one brighter than magnitude -4. |
| Galaxy |
A vast collection of billions of stars,
gas, and dust held together by the gravity of its
members. The galaxy in which the sun resides is called the Milky Way. |
| Galileo |
U. S. space mission to study Jupiter's
atmosphere, moons, and magnetosphere. The Galileo
spacecraft arrived at Jupiter in 1995, dropped a probe into the planet's
atmosphere, monitored jovian weather and undertook a series of close
encounters with the four major moons Io, Europa,
Ganymede and Callisto over the next six years, returning a total of
over 14,000 images. It will be sent into the jovian atmosphere in 2003. Galileo Project web site Galileo information at NSSDC |
| Gas giants |
The planets Jupiter, Saturn, Uranus, and Neptune. |
| Inferior conjunction |
See conjunction. |
| Latitude |
The angular distance north or south from the
Earth's equator measured in degrees. The equator is at
0° and the poles are at 90° N and 90° S. |
| Light-year |
The distance traveled through space by a beam of
light in one year. Light travels at 186,282 miles
(299,792 kilometers) per second, so a light-year is 5.88 trillion
miles (9.50 trillion kilometers), or 63,240 times Earth's distance from
the sun. |
| Longitude |
The angular distance east or west between the
meridian of a particular place on Earth and that of
Greenwich, England, expressed either in degrees or time. |
| Luna |
One of two successful series of Soviet lunar
missions. There were twenty-four missions to the moon
in the Luna series. (The other series, Zond, had five lunar missions.)
The first image of the farside of the moon was taken by the Soviet Luna
3 spacecraft in 1959. Luna 3 information at NSSDC |
| Lunar
Prospector |
U. S. mission to the moon launched on January 6,
1998. Its instruments were designed to provide global
maps and data sets of the moon's composition and magnetic and
gravity fields from a low polar orbit. The mission lasted eighteen
months and ended July 31, 1999 with a controlled crash
landing into a crater at the moon's south pole. Lunar Prospector web site Lunar Prospector information at NSSDC |
| Magnitude |
A measure of the relative brightness of stars
and other celestial objects. The brighter the object
the lower its assigned magnitude. This logarithmic scale is based on
the ancient practice of noting that the brightest stars in the sky were
of " first importance" or " first magnitude," the next
brightest being " second magnitude," etc. In 1854
Norman Pogson formalized this scale and defined a
difference of 5 magnitudes to be exactly a factor of 100 in brightness.
The faintest naked-eye magnitude visible from a dark
site is +6.5, Mars at its brightest is -2.9, Venus at
its brightest is -4.7 and the full moon is -12.5. |
| Mariner 9 |
U. S. space mission to Mars, launched in 1971,
achieved global imaging of the surface, including the
first detailed views of the martian volcanoes, Valles Marineris, the
polar caps, and the satellites Phobos and Deimos. The spacecraft
gathered data on atmospheric composition, density,
pressure and temperature and also on surface composition,
temperature, gravity and topography of Mars. Mariner 9 information at NSSDC Mariner 8 and 9 overview at JPL |
| Mars
Global Surveyor |
U.S. mission to Mars launched in 1996. Its main
instruments include a camera, laser altimeter, thermal
emission spectrometer and magnetometer. Image resolution is several times better than any of those taken by the Viking
Orbiter cameras, enabling features just a few meters across to be seen.
An extended mission phase began in 2001. Mars Global Surveyor web site |
| Mars
Odyssey |
U.S. mission to Mars launched in 2001. Its main
instruments include gamma-ray and neutron
spectrometers, a neutron detector and a thermal imaging camera. In
February 2002, early results indicated large amounts of hydrogen,
implying the presence of frozen water, in the martian
soil. Mars Odyssey web site |
| Mars
Pathfinder |
U.S. mission that on July 4, 1997, landed
successfully on Mars, returning over 16,000 images
during a four-month-long mission. An autonomous rover named Sojourner
explored the area beyond the lander. Mars Pathfinder web site |
| Meteor |
The streak of light caused by a solid body in
orbit about the sun (a meteoroid) passing through the
atmosphere
also called a " shooting star." A meteorite
is a meteoroid that strikes the surface of a planet
or moon. |
| Meteor
shower |
The appearance of many
within a few hours that seem to radiate from the same
region of the sky. They occur when the Earth passes through
the dusty debris near a orbit. |
| Milky Way |
A faint band of light around the sky composed of
vast numbers of stars too faint to see individually.
Also, the name of the galaxy in which
the sun resides. |
| Moon |
A natural satellite orbiting a planet. Also, the
name of Earth's natural satellite. |
| Nautical
twilight |
The time when the sun is 6 to 12 degrees below
the horizon. The sky begins to brighten noticeably. |
| Near Earth
Asteroid Rendezvous (NEAR) |
U.S. space mission launched on February 17,
1996. Placed into orbit around asteroid 433 Eros
on February 14, 2000, NEAR returned data on the body's bulk
properties, composition, mineralogy, morphology, internal mass
distribution and magnetic field. On February 12,
2001, it became the first spacecraft to land on an asteroid. NEAR mission web site |
| Nearside |
The side of the moon that always faces Earth. |
| Nebula |
A cloud of gas and dust, sometimes glowing from
the light of nearby stars and sometimes a dark patch
that blocks starlight. New stars are born within
a nebula. |
| Nova |
A star which suddenly
erupts, greatly increasing its brightness. |
| Nucleus |
Of a comet, the solid
ice-rock mixture at the center of a comet's gaseous
head and tail. Of a spiral galaxy, the dense
central portion made of older, redder stars. (plural: nuclei). |
| Opposition |
The point in a planet's
orbit at which it appears opposite the sun in the sky.
A planet at opposition is visible all night long. Because they
orbit closer to the sun than Earth, Mercury and Venus never reach
opposition. |
| Perigee |
The point where an object in orbit around the
Earth is nearest to it. |
| Perihelion |
The point where an object in orbit around the
sun is nearest to it. |
| Phases |
The cycle of varying shape in the sunlit portion
of a planet or moon. The
moon, Venus, and Mercury all show phases as seen from
Earth. |
| Photosphere |
The visible surface of the sun. |
| Planet |
A body of substantial size held in orbit by the
gravity of a star. A planet
shines by reflecting the star's light. |
| Radar |
Radio signals transmitted to and bounced back
from an object. It stands for Radio DetectionAnd |
| Radiant |
The point in the sky from which shower meteors seem to
appear. |
| Radiation |
Energy transmitted through space as waves or
particles. |
| Retrograde
motion |
The apparent backward (westward) loop in a planet's motion across the sky.
All planets display retrograde motion, but that of Mars is most
striking. |
| Satellite |
A natural or artificial body in orbit around a planet. |
| Scintillation |
A tremulous effect of starlight -- twinkling --
caused by its passage through our turbulent
atmosphere. Planets usually don't exhibit this
effect. |
| Sidereal
period |
The time taken by a planet
to complete one revolution around the sun (or for the
moon to complete an orbit around the Earth) as measured by reference
to the background stars. |
| Solar wind |
A stream of electrically charged particles
(mainly electrons and ionized hydrogen) moving outward
from the sun with velocities in the range 180-310 miles (300-500 kilometers) per second. |
| Solstice |
The date of the year at which either the Earth's
north or south pole is angled most directly toward the
sun. This occurs on two days of the year, near June 21 and December 21. The June solstice, the longest day of the year in the northern
hemisphere, is considered the first day of summer
there
the sun makes its most northerly arc through
the sky. The December solstice, marks the start of northern winter and
is the shortest day of the year the sun then makes
its most southern arc through the sky. |
| Star |
A hot, glowing sphere of gas, usually one that
emits energy from nuclear reactions in its core. The
sun is a star. |
| Sunspot |
A magnetic disturbance on the sun. It is cooler
than the surrounding area and, consequently, appears
darker. |
| Superior conjunction |
See conjunction. |
| Supernova |
An enormous stellar explosion that increases the
brightness of a star by a factor
of more than 100,000. Although the star itself is destroyed, a small
portion of its central core may survive as a neutron star. |
| Synodic
period |
The average time between successive returns of a
planet or the moon to the same apparent position
relative to the sun -- for example, new moon to new moon, or opposition to opposition. |
| Terminator |
The edge of the sunlit portion of the moon or
planets
the line between day and night. |
| Terrawatt |
An amount of power equal to 1 x 1012
watts. |
| Terrestrial
planets |
Mercury, Venus, Earth, and Mars. |
| Tides |
Periodic changes in the shape of a planet, moon,
or star caused by the gravity of a body near it. |
| Train |
A dimly visible path left in the sky by the
passage of a meteor. |
| Transit |
The passage of a planet across the face of the
sun. From Earth, only Mercury and Venus can transit. |
| Twinkling |
See scintillation. |
| Variable
star |
A star that exhibits
significant brightness changes. |
| Viking |
U.S. mission to Mars, composed of two
spacecraft, launched in 1975. Viking 1 and Viking 2 both
consisted of an orbiter and a lander. Primary mission objectives
were to obtain high-resolution images of the Martian surface (55,000
were returned by the orbiters, 1,400 from the
landers), characterize the structure and composition
of the atmosphere and surface and search for evidence of life. National Air and Space Museum exhibit Viking Project Information at NSSDC |
| Voyager |
U.S. mission consisting of two spacecraft
launched in 1977 to explore Jupiter, Saturn, their
moons, rings, and magnetic environments, each taking two years to reach
Jupiter. Voyager 2 went on to explore Uranus and Neptune as well.
Each spacecraft took two years to reach Jupiter. The
last image was taken in 1989 and now both spacecraft are headed out of the solar system. Voyager Project web site Voyager information at NSSDC Voyager information at USGS |
| White dwarf |
A collapsed object formed from a star that has
exhausted its nuclear fuel. The sun will one day
become a white dwarf. |
| Zenith |
The point directly overhead, 90° above the
horizon. |