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CALDERA
A caldera is a large depression at the top of a volcano, caused
by collapse or explosion. |
CALLIPUS
Callipus of Cyzicus (370 - 300 BC) was an ancient Greek who
accurately measured the length of the seasons. Callipus improved
the Greek calendar, reconciling the lunar month with the solar
year, by introducing a unit of time called the Callippic cycle
(it was an improvement on the Metonic cycle of 6939.6 days or 19
solar years or 235 lunar months; the Callippic cycle was 4
Metonic cycles). He also added to the (incorrect) theory of the
motions of the plants, as spheres within spheres, adding 7 more
|

CALLISTO
Callisto is a large, icy, dark-colored, low-density outer moon
of
Jupiter that is scarred with impact craters and ejecta. It
has a diameter of about 3,000 miles (4800 km), the second
largest moon of Jupiter, roughly the size of Mercury. It orbits
Jupiter at a mean distance of 1,170,000 miles (1,883,000 km).
Its mass is 1.08x1023 kg. It
takes Callisto 400.5 hours to orbit Jupiter. Callisto was
discovered by
Galileo and S. Marius (independently) in 1610. |
CALORIS BASIN
The Caloris Basin is the largest surface feature on t.he planet
Mercury. This circular depression was formed in a collision
with an
asteriod, and is about 1,300 kilometers (800 miles) across.
The Caloris Basin is near Mercury's subsolar point, the point on
Mercury that is closest to the Sun when Mercury is at
perihelion (the point in its orbit when it is nearest to the
Sun), so the Caloris Basin gets extremely hot; this is why
it is called Caloris, which means "heat" in Latin. |

CALYPSO
Calypso is one of the 18
moons of Saturn. It was discovered by B. Smith, H. Reitsema,
S. Larson, J. Fountain in 1980. It is irregularly-shaped and has
a radius of 15.0x8.0x8.0 km. Calypso an orbit with
Telesto (294,660 km from the center of
Saturn); these 2 moons are also called the Tethys Trojans
because they orbit Saturn in Tethys' orbit, Telesto is 60° ahead
of
Tethys, Calypso is 60° behind Tethys. |
CANADARM
The
Candarm is the robotic arm on the
Space Shuttle. The robotic arm lets astronauts on the flight
deck of the Space Shuttle manipulate objects (like satellites)
in space. The arm was built by Spar Aerospace Ltd., Canada for
the U.S. (NASA's) Space Shuttle Program. Canadarm was launched
aboard the Space Shuttle Columbia STS-2 on the second shuttle
flight on November 12, 1981. It was deployed for the first time
on Friday Nov. 13, 1981, operated by astronaut Richard Truly. |

CANCER
[Abbreviation: Cnc] Cancer (the crab) is a very faint
constellation of the
zodiac that is shaped like a crab. Cancer is seen along the
ecliptic and is located between Leo and Gemini. At the
center of the crab's shell is a huge open cluster, the Beehive
cluster, also known as Praesepe (M44). The open cluster M67 is
nearby. The brightest star in Cancer is Acubens (meaning claw);
the second-brightest is Al Tarf (meaning tip). |

CANIS MAJOR
Canis major (The Great Dog) is a
constellation near
Orion. The brightest star in Canis Major (and the brightest
star in the sky) is Sirius, also known as the dog star. Canis
Major is one of the constellation Orion's hunting dogs (together
with Canis Minor). |

CANIS VENATICI
Canes Venatici (The Two Hunting Dogs [or greyhounds, called
Astarion and Chara, who belong to the herdman Boötes]) is a
small Northern Hemisphere
constellation near
Ursa Major and
Boötes. The brightest star in Canis Venatici is Cor Caroli
(alpha CVn), a blue-white star (magnitude 2.9) with a companion
star (magnitude 5). Beta CVn is a star called Chara. The
Whirlpool Nebula (M51), the Sab galaxy (M94), the Sunflower
Galaxy (M63), and the globular cluster M3 (magnitude 6) can be
found in Canis Venatici. The Canes Venaticids
meteor shower occurs from January 13 - January 30. Canes
Venatici was named by the Polish astronomer Johannes Hevelius in
1690. |
CANNON, ANNIE J.
Annie Jump Cannon (1863-1941) was an American astronomer who
cataloged 225,300 stars in the HD (Henry
Draper) catalog; every star is classified by its stellar
spectra. Cannon and Edward C. Pickering (director of the Harvard
Observatory) published the original
HD catalog (9 volumes) from 1918 to 1924. The catalog was
later expanded by Cannon and Margaret W. Mayall in 1949. |
CAPELLA
Capella is a multiple star system containing at least 9 stars.
This bright system is in the Northern Hemisphere, 45 degrees
from
Polaris (the northern
pole star); it is in the
constellation Auriga. The two brightest stars in Capella are
a
binary star system. They are both yellow (like our Sun) with
masses 2.6 times and 2.7 times that of the
Sun. One is 9 times as large as the Sun, the other is 12
times as large. Each gives off roughy 78 times the light as the
Sun. These two stars are about 43 light years from
Earth. |

CAPRICORNUS
[Abbreviation: Cap] Capricornus (the goat) is a constellation of
the
zodiac. Capricorn is seen along the
ecliptic between Sagittarius and Aquarius. The brightest
stars in Capricornus are Prima Giedi (Alpha 1 Cap) and Secunda
Giedi (Alpha 2 Cap). The globular cluster M30 is in Capricorn. |
CARBONADO
A carbonardo is a rare type of opaque black diamond; they are
not used for jewels, but for items like drilling bits and
abrasive wheels. They were once thought to have been formed as a
result of a comet impact 2 billion years ago, but this is no
longer thought to be true. The largest diamond ever found was a
carbonardo that weighed over half a kilogram. Carbonadoes are
found in Bahia, Brazil, South America. Unlike other diamonds,
carbonadoes are not found in a crystallized form - they are
found in irregular or rounded fragments. Carbonadoes have a
hardness of 10 and a
specific gravity (density) of 3.1-3.3. Diamonds have a very
hard polycrystalline carbon structure. |
CARME
Carme is Jupiter's
fourteenth moon. Carme is 18.5 miles (30 km) in diameter and
orbits 13,800,000 miles (22,600,000 km) from Jupiter. Carme has
a mass of 9 x 1016kg. It
orbits Jupiter in 692 (Earth) days and is in a retrograde orbit
(orbiting opposite to the direction of Jupiter). Very little is
known about Carme. Carme was discovered by S. Nicholson in 1938. |

CARTWHEEL GALAXY
The Cartwheel Galaxy has a ring-like structure that is the
result of a head-on collision of two
galaxies! It started out as a regular
spiral galaxy that was hit by a smaller galaxy. The
ring-like band of stars formed much like ripples form in water
when a rock is tossed into it. The Cartwheel Galaxy is about 500
million
light-years from Earth in the
constellation Sculptor. |

CASSEGRAIN TELESCOPE
A Cassegrain telescope is a wide-angle reflecting telescope with
a concave mirror that receives light and focuses an image. A
second mirror reflects the light through a gap in the primary
mirror, allowing the eyepiece or camera to be mounted at the
back end of the tube. The Cassegrain relecting telescope (named
for the French sculptor Sieur Guillaume Cassegrain) was
developed in 1672. A correcting plate (a lens) was added in 1930
by the Estonian astronomer and lens-maker Bernard Schmidt
(1879-1935), creating the
Schmidt-Cassegrain telescope which minimized the spherical
aberration of the Cassegrain telescope. |

CASSINI, G. D.
Giovanni Domenico Cassini (1625-1712) was an
astronomer born in Italy who later became a naturalized
French citizen. He discovered four of
Saturn's moons (Tethys, Dione, Rhea, and Iapetus) and a dark
division in
Saturn's rings (called the Cassini Division). |

CASSINI DIVISION
The Cassini Division is the main, dark division between
Saturn's largest rings (the A and B rings). This gap is
2,920 miles (4,700 km) wide and is 73,010 miles (117,500 km)
from the center of Saturn. It was discovered by G.D. Cassini in
1675. |
CASSINI - HUYGENS
NASA's Cassini-Huygens
spacecraft was launched from Earth on October 1997 to go on an
11-year mission to Saturn. The spacecraft was named after the
main division in
Saturn's rings, called the
Cassini Division. Cassini sent back photos and scientific
information from Venus (in 1998) and Jupiter (in 2000) - it used
the planets' gravitational fields to boost the spacecraft
towards Saturn. In 2004, Cassini will send a probe called
Huygens (built by the European Space Agency) to the surface of
Titan, (Saturn's
biggest moon). |

CASSIOPEIA
Cassiopeia is an easily-seen
constellation that is in the far northern sky. It circles
the polestar (Polaris)
throughout the year and also straddles the
Milky Way. The five major stars of Cassiopeia (also known as
"The Lady of the Chair") are shaped like a "W" (or an "M,"
depending on your orientation). All of the stars in Cassiopeia
are all less than second magnitude brightness. The brightest
star in Cassiopeia is Schedar (alpha CAS), which is a multiple
star that is pale rose in color and varies in magnitude from 2.2
to 2.8 magnitudes. The second-brightest, called Caph (beta CAS),
is a white star of magnitude 2.4. Cassiopeia contains two open
clusters, M52 (magnitude 7.3) and M103 (magnitude 7.4). The
srongest radio source, Cassiopeia A, emanates from Cassiopeia;
it is the remnant of a supernova which ocurred about 1660 A.D.,
and is 10,000 light years from us. The constellation Cassiopeia
was named for Cassiopeia, the mother of Andromeda (and the wife
of Cephus) in Greek mythology. |
|
CATENA
A catena is a chain of craters. |

CAVENDISH, HENRY
Henry Cavendish (1731-1810) was an English chemist and
physicist. Cavendish discovered that hydrogen gas was a
substance different from ordinary air (whose components he
analyzed), he described the composition of water (hydrogen and
oxygen) and made other important discoveries. Cavendish was the
first person to determine
Isaac Newton's
gravitational constant and accurately measured the
Earth's mass and density. |
|
CCD
CCD stands for charge-coupled device; it is a type of digital
camera containing an array of extremely light-sensitive
capacitors. When a photon (a particle of light) hits a
capacitor, the photon dispaces some electrons, generating a
small current - charging the capacitor. A CCD can detect light
coming in at rates as low as one photon per minute. In CCD
astronomy, this light-sensitive integrated circuit is hooked up
to a telescope, detecting even extremely faint images that were
impossible to detect before. All optical observatories
(including the orbiting
Hubble Space Telescope) use this type of device. George
Elwood Smith and Willard S. Boyle (both of Bell Labs) invented
the charge-coupled device in 1969. In 1970, they used their CCD
to built the first solid-state video camera.
|
CELESTIAL COORDINATES
Celestial coordinates are pairs of numbers (right ascension and
declination) which are used to locate objects on the celestial
sphere. They are similar to the coordinates of longitude and
latitude on Earth. |
CELESTIAL EQUATOR
The celestial equator is the projection of the Earth's equator
onto the celestial sphere. |
CELESTIAL POLES
The celestial poles are the projection of the Earth's poles onto
the celestial sphere. |
CELESTIAL SPHERE
The celestial sphere is an imaginary sphere whose center is the
Earth. This sphere is used by
astronomers to map celestial objects. |

CELSIUS, ANDERS
Anders Celsius (1701-1744) was a Swedish professor of astronomy
who devised the Celsius thermometer. He also ventured to the far
north of Sweden with an expedition in order to measure the
length of a degree along a meridian, close to the pole, later
comparing it with similar measurements made in the Southern
Hemisphere. This confirmed that that the shape of the earth is
an ellipsoid which is flattened at the poles. He also cataloged
300 stars. With his assistant Olof Hiorter, Celsius discovered
the magnetic basis for auroras. |
CENTAUR
Centaurs are relatively small objects (half
asteroid, half comet) that are in unstable orbits (on a time
scale of millions of years) located between
Jupiter and
Neptune. About 9 centaurs have been found so far; the
largest centaur is 2060
Chiron (which is about 170 km in diameter and has a
detectable
coma). Centaurs are objects that probably came from the
Kuiper belt. |
CENTER OF MASS
The center of mass is the location at which the entire mass of
an object (or set of objects) may be considered for purposes of
calculations. It is the point of the average weighted position
in space of an object (or a collection of objects). |
CENTRIFUGAL
Centrifugal (meaning "center fleeing" in Latin) means directed
outwards from the center. |
CENTRIFUGAL FORCE
Centrifugal force is a force that acts upon a body spinning on
an
axis. This force is directed away from the body. Centrifugal
force is equal to, but opposite the centripeta force. |
CENTRIPETAL
Centripetal (meaning "center seeking" in Latin) means directed
towards the center. |
CENTRIPETAL FORCE
Centripetal force is a force that acts upon a body moving in a
curved path. This force is directed towards the center of the
curvature of the path. It is equal to, but opposite the
centrifugal force. |

CEPHEID VARIABLE STARS
Cepheid variables are supergiant stars that regularly pulsate in
size and change in brightness. As the star increases in size,
its brightness decreases; then, the reverse occurs. The
luminosity is proportional to the period. Cepheid Variables may
not be permanently variable; the fluctuations may just be an
unstable phase the star is going through.
Polaris and Delta Cephei are examples of Cepheids. |

CEPHEUS
Cepheus is a house-shaped
constellation in the Northern Hemisphere. It is a
circumpolar constellation; it never dips under the horizon in
the Northern hemisphere. Errai (Gamma Cephei) is a
third-magnitude orange subgiant star that will become the
Earth's north polar star in 2,000 years. Cepheus is next to the
constellations
Andromeda and
Perseus. Cepheus was named after King Cepheus in Greek
mythology, and is abbreviated Cep. |
CERES
Ceres is the largest of the
asteroids. It was the first asteroid ever discovered (by
Italian
astronomer Giuseppe
Piazzi on January 1, 1801). Its mass is equal to over
one-third of the 2.3 x 1021 kg
estimated total mass of all the 3,000 cataloged asteroids. It is
about 578 miles (930 kilometers) in diameter. |

CETUS
Cetus is a
constellation that straddles the
celestial equator. Cetus means whale, and is abbreviated Cet.
The first-known variable star
Mira, is Omicron Ceti. |

CHALLENGER, SPACE SHUTTLE
The Space Shuttle Challenger was the second NASA Space Shuttle
to be used (Columbia was the first). Challenger's first launch
was the sixth Space Shuttle launch, called STS-6 Challenger; it
took off on April 4, 1983 (from Florida), and landed on April
16, 1983 (at Edwards Air Force Base, CA). The first crew
consisted of Paul J. Weitz, Karol J. Bobko, Donald H. Peterson,
and F. Story Musgrave. It orbited the Earth 81 times, flying for
5 days, 0 hours, 23 min, 42 seconds; the first Shuttle space
walk occured on this mission (it lasted four hours, 17 minutes).
After nine flights into space, STS-51L (the mission number)
Challenger, exploded 73 seconds into its launch on January 28,
1986, killing the crew (Gregory Jarvis, S. Christa McAuliffe,
Ronald McNair, Ellison Onizuka, Judy Resnik, Francis Scobee and
Michael Smith). |
CHAMBERLAIN, THOMAS C.
Thomas Chrowder Chamberlain (Sept. 25, 1843 - Nov. 15, 1928) was
an American geologist and teacher who proposed the planetesimal
hypothesis of the formation of the Solar System. In this theory,
a star is supposed to have passed near the Sun, pulling matter
away from the Sun. Later, this matter is to have condensed into
larger masses, forming the planets. |
|

CHANDRA
The orbiting Chandra X-ray Observatory is the world's most
powerful X-ray telescope. This 45 ft long satellite observes
X-rays from high-energy parts of the sky, like exploding stars
(temperatures in the millions of degrees Celsius produce
X-rays). Chandra was launched on the Space Shuttle Columbia
(STS-93) on July 23, 1999. It orbits more than 1/3 of the way to
the moon. Electrical power is generated by solar panels, which
generate the 2000 Watts it uses (this is about the power that a
hair dryer uses). The extraordinarily smooth, barrel-shaped
mirrors are coated with a very thin film of iridium (a rare
metal). Chandra was named to honor astrophysicist Subrahmanyan
Chandrasekhar. Chandra also means "Moon" or "luminous" in
Sanskrit. |
CHANDRASEKHAR, S.
Subrahmanyan Chandrasekhar (born Lahore, India, in 1910 -died
Chicago, USA, in 1995) was an Indian-American
astrophysicist who studied stellar physics, evolution, and
black holes. He realized that the fate of dying stars depended
upon their mass, and above a certain point (1.4 times the mass
of the
Sun, now known as the "Chandrasekhar limit"), a star will
undergo extreme collapse and not simply becomes a white dwarf.
He won the Nobel prize in physics in 1983. The orbiting X-ray
Observatory Chandra was named to honor S. Chandrasekhar. |

CHARLIER, CARL V. L.
Carl Vilhelm Ludvig Charlier (1862-1932) was a Swedish
astronomer who studied celestial mechanics, the calibration
of photographic photometry, and the theory of lenses. Charlier
also worked in statistics, including the theory of errors; he
studied the distribution and motions of stars. Charlier showed
that hotter stars and galactic clusters formed flattened
systems. In Charlie's hierarchical model of the Universe, he
argued that the Universe has infinite mass, and that the density
of matter approaches zero as one goes farther into space
(resolving
Olber's paradox). A 100 km wide crater on Mars (at 68.6
south, 168.4 west, shown above) was named for Charlier in 1973. |
CHARON
Charon is the only moon orbiting the planet
Pluto. It is small, about 1,172 km in diameter. It orbits
about 19,640 km from Pluto on average. It may be covered by
water ice and probably has no atmosphere. Charon is in a
synchronous orbit around Pluto. That is, Charon is always over
the same spot on Pluto; Charon's orbit takes exactly one Pluto
day. Charon was discovered by Jim Christy in 1978. Charon was
named after the mythological demon who ferried people across the
mythological river Styx into Hades. |
CHICXULUB CRATER
The Chicxulub crater at the tip of the Yucatán Peninsula is an
impact crater that dates from 65 million years ago. It is
120 miles wide and 1 mile deep. It is probably the site of the
K-T
meteorite or
comet impact that caused the
extinction of the dinosaurs and other groups of organisms. |
CHIRON
2060 Chiron (also known as Comet 95P/Chiron) is the
largest-known
centaur (half
asteroid, half comet). It is in a very elliptical, unstable
orbit (on a timescale of millions of years) located between
Jupiter and
Neptune. Chiron is about 170 km in diameter and has a
detectable
coma. It was discovered by Charles Kowal on November 1,
1977. |

CHONDRITIC METEOR
Chondritic
meteors are stony meteors with chondrules, tiny glass
spheres. These meteors are unchanged since their formation,
shortly after the formation of the
Sun. These meteors consist of elements also common in the
Earth's core. |
CHROMOSPHERE
The chromosphere is the inner, reddish layer in the sun's
atmosphere, between the
photosphere and the
corona. The chromosphere is visible during a total
solar eclipse. |
CIRCUMPOLAR CONSTELLATION
A circumpolar
constellation is one whose apparent path seems to circle a
celestial pole. A circumpolar constellation never sets; it is
always above the observer's horizon. |
CIRCUMPOLAR STAR
A circumpolar star is one whose apparent path seems to circle a
celestial pole. A circumpolar star never sets; it is always
above the observer's horizon. |
CISLUNAR
Cislunar refers to the space between the Earth and the orbit of
the Moon. Compare to
translunar. |

CLASSCAL CEPHEID
A classical Cepheid is a young, Helium-burning, supergiant star
(spectral class F-K) that regularly pulsates in size and changes
in brightness (with a period from 1-50 days). As the star
increases in size, its brightness decreases; then, the reverse
occurs. The luminosity is proportional to the period, so the
absolute magnitude of the star can be calculated from the
observed period, which can then give the distance to the star. |
CLOSED UNIVERSE
A closed universe is a model of the universe in which the
universe first expands (after the big bang), and then contracts,
due to the gravitational forces of the matter in the universe.
In this model, the universe is finite in space and time.
Contrast with an
open universe. |
CLOSEST STAR
The closest star to us is the
Sun! Other than that, the closest star is Proxima Centauri,
aka Alpha Centauri C (the dimmest star in the Alpha Centauri
system). Proxima Centauri is 4.3 light-years from the Sun. It
has an absolute magnitude of 15.5. |

CLUSTER
A cluster is a group of stars or
galaxies. Our own galactic cluster, the
Local Group, is about 5 million
light-years across and contains about 30 galaxies (the
largest of which are the
Andromeda galaxy, Triangulum, and our
Milky Way). The next-closest cluster is the Virgo Cluster,
which is about 60 million
light-years from Earth. |
CMB
CMB stands for Cosmic Background Radiation and is also
abbreviated CMBR and CBR. CMB is the radiation (energy) which
remains from the original Big Bang explosion which formed the
universe. CMB has cooled as the universe has expanded and is now
slightly less than 3 degrees above absolute zero. |
COBE
COBE (Cosmic Background Explorer) is a NASA satellite that was
launched in 1992. COBE detected extremely fluctuations (anisotropy),
in the cosmic microwave background (the heat left over from the
Big Bang). The differences in temperature were tiny, ranging
from 2.7281 Kelvin (degrees above absolute zero) to 2.7280
Kelvin, but imply fluctuations in the density of matter in the
early universe. |
COLLIMATE
To collimate a telescope, one lines up the optical components,
the lenses, mirrors, prisms, and eyepieces, into their proper
positions. Collimating maximizes image quality. |
|

COLLINS,
MICHAEL
Michael Collins (1930- ) is an American astronaut and US Air
Force pilot. Collins piloted NASA's 3-day Gemini 10 Mission,
which was launched on July 18, 1966; this mission successfully
rendezvoused and docked with a separate Agena target vehicle,
and Collins walked in space twice during this mission. Collins
piloted the Command Module pilot of Apollo 11 (the mission that
landed Neil Armstrong and Edwin Aldrin Jr. on the moon, it flew
from July 16-24, 1969); Collins circled the moon while Armstrong
and Aldrin landed on the moon, and later rendezvoused with them. |

COLUMBA
Columba (the dove, abbreviated Col) is a small
constellation in the Southern Hemisphere. This constellation
pictures a dove holding an olive branch in its mouth. Columba is
a member of the "Heavenly
Waters," a
constellation family. Columba was named by the astronomer
Bayer, but was populatized by the French
astronomer Augustin Royer in 1679 (before that, Colmba's
stars have been included in the constellation
Canis Major). Alpha Col (the brightest star in Columba) is
called Phaet; beta Col (the second-brightest star in Columba) is
called Wezn. The
globular cluster NGC 1851 and the blue
magnitude 5 star (mu Col, a "runaway
star") are in Columba. |
|

COLUMBIA, SPACE SHUTTLE
The first Space Shuttle, STS-1 Columbia (OV-102), launched on
April 12, 1981 (from Florida), and landed April 14, 1981 (at
Edwards Air Force Base, CA). The first crew consisted of
Commander John W. Young and Pilot Robert L. Crippen. It orbited
the Earth 37 times, flying 1,074,567 miles in 2 days, 6 hours,
20 min, 53 seconds. After dozens of flights into space, STS-107
(the mission number) Columbia, disintegrated during atmospheric
re-entry on February 1, 2003, killing the seven crew members
(Rick D. Husband, Kalpana Chawla, William C. McCool, David M.
Brown, Laurel B. Clark, Michael P. Anderson, Ilan Ramon). |

COMA
A coma is the roughly spherical blob of gas that surrounds the
nucleus of a
comet. The coma is comprised of water vapor, carbon dioxide
gas, and other neutral gases that have
sublimed from the solid nucleus. The coma and the nucleus
form the head of a comet. |

| A Few Comets |
Discovered |
Last Visit |
Next Visit |
Period
(years) |
|
Halley |
240 B.C. |
1986 |
2061 |
76.00 |
| Encke |
1786 |
1997 |
2000 |
3.28 |
| Biela |
1772 |
1852 |
broken up |
6.62 |
| Faye |
1843 |
1991 |
1999 |
7.34 |
COMET
A comet is a celestial body that orbits around the sun. It is
made up of a nucleus (solid, frozen ice, gas and dust), a
gaseous coma (water vapor, CO2,
and other gases) and a tail (dust and ionized gases). Its long
tail of gas and dust always points away from the sun, because of
the force of the
solar wind. The tail can be up to 250 million km long, and
is most of what we see. Comets are only visible when they're
near the sun in their highly
eccentric orbits. NASA's
Stardust Mission will visit Comet Wild 2 in 2004. |
|
COMPACT STAR
Compact stars are very dense stars with a radius much smaller
than than the our Sun. Some compact stars include black holes,
white dwarfs, and neutron stars. |

COMPLEX IMPACT CRATER
A complex impact
crater is a large crater with a single or many peaks in the
middle of the crater. On the moon, these craters have diameters
between about 12 and 110 miles (20 and 175 km), and the central
uplift is usually one or a few peaks. Craters with diameters
over 110 miles (175 km) can have more complex, ring-shaped
uplifts within the crater.
|

COMPTON GAMMA RAY OBSERVATORY
The Compton Gamma Ray Observatory (CGRO) is an orbiting
telescope that NASA launched in 1991. It observes the
electromagnetic spectrum from 30 keV to 30 GeV. The CGRO led to
the discovery of
blazars. CGRO was named to honor Dr. Arthur Holly Compton,
who studied the scattering of high-energy photons by electrons.
It will fall into the remote Pacific on June 3, 2000. CGRO
detected more than 400 gamma ray sources and recorded more than
2,500 gamma ray bursts. |
CONDENSATION
Condensation is the process in which a vapor (gas) is cooled to
the liquid phase. Clouds are formed by the condensation of
atmospheric water vapor. |
|

CONJUNCTION
Conjunction is the apparent close approach of a planet to the
Sun (or another planet), from the point of view of an observer
on the Earth. A planet is in conjunction when the Sun is exactly
between that planet and the Earth or, for
Mercury and
Venus (the two inferior planets), when that planet, the
Sun, and the
Earth are lined up. Mercury and Venus have two positions of
conjunction: when either planet is directly between the earth
and the Sun, it is in inferior conjunction; when either planet
is on the far side of the Sun from the earth, it is in superior
conjunction. During conjunction, a planet cannot be seen from
Earth (unless it is in
transit); it is either behind the Sun or is lost in the
glare of the Sun. |
CONSERVATION OF ENERGY
Conservation of energy is a basic principle of physics stating
that energy can never be created or destroyed, it just changes
form. For example, the chemical energy in an atom's bond turns
into heat during combustion. |
|

CONSTELLATION
A constellation is a group of stars that, when seen from Earth,
form a pattern. There are 88 constellations, including the
Andromeda (pictured above).
|
CONSTELLATION FAMILY
There are many families of
constellations, constellations that are either close to one
another or have some other relationship. Some constellation
families include the
Zodiac (the 12 constellations representing the signs of the
Zodiac), the Ursa Major Family (10 constellations, including
Ursa Major, Ursa Minor Canes Venatici, Bootes, Coma Berenice,
Corona Borealis, etc.), the Perseus Family (9 constellations,
including Cassiopeia, Cepheus, Andromeda, Perseus, etc.), the
Hercules Family (19 constellations, including Hercules, Sagitta,
Aquila, etc.), the Orion Family (5 constellations, including
Orion, Canis Major, Canis Minor, Monoceros, and Lepus), the
Heavenly Waters (9 constellations, including Delphinus, Columba,
Equuleus, Vela, Puppis, etc.), the Bayer Group (11
constellations, including Hydrus, Dorado, Volans, Apus,etc.),
the La Caille Family (13 constellations, including Norma, Fornax,
Circinus, etc.). |
CONTINENTAL DRIFT
Continental drift is the movement of the Earth's continents. The
land masses are hunks of Earth's crust that float on the molten
core. The ideas of continental drift and the existence of a
supercontinent (Pangaea)
were presented by Alfred Wegener in 1915.
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CONTINENTAL PLATES
The crust of the
Earth is
broken into plates. The plates are enormous chunks of rock
that float atop the soft mantle. The plates are moving at a
speed that has been estimated at 1 to 10 cm per year.
Continental plates are thicker, older, and less dense than
oceanic plates. These plates are about 125 kilometers thick and
are made of granite that is about 3 billion years old. |

CONTINUOUS SPECTRUM
A continuous spectrum is a spectrum of emitted light that
contains all wavelengths of the colors that compose white light
(red, orange, yellow, green, blue, indigo, violet, from long to
short wavelength). Continuous spectra are emitted by
incandescent solids, liquids, or compressed gases. If some
discrete lines are missing from a
spectrum, it is an absorption spectrum (indicating the
presence of elements that absorb particular wavelengths). |
CONVECTION
Convection is the transfer of heat by circulation through a gas
or liquid. |

COPERNICAN SYSTEM
The Copernican system is the model of the
solar system in which the planets (including the Earth)
orbit the sun. This controversial theory was developed by
Copernicus. |

COPERNICUS, NICOLAUS
Nicolaus Copernicus (1473-1543) was an amateur Polish
astronomer who developed the revolutionary Copernican
system, a model of the
solar system in which all the planets orbit the
Sun. His ideas overturned the old
Ptolemaic System. His seminal work was De Revolutionibus
Orbium Coelestium ("On the Revolutions of the Celestial
Orb"), published in 1543. |

CORE
The core is the innermost layer of the
Earth (or any planet, moon, or star). It is usually under
great pressure and is very hot. |

CORIOLIS FORCE
The Coriolis force is the force that results from the rotation
of the Earth around its axis; it makes storms rotate
counterclockwise in the Northern and clockwise in the Southern
Hemispheres. The French engineer/mathematician Gustave-Gaspard
Coriolis discovered this force in 1835. This force has no effect
on the direction of water going down a drain. |

CORONA
The corona is the top layer of the
sun's atmosphere; it extends for millions of miles beyond
the Sun's surface. The corona has very high temperatures (over a
million K) and a very low density. During a complete
solar eclipse (pictured above), only the ghostly corona is
visible. |
CORONAL HOLES
Coronal holes are areas in the coronal where the
Sun's magnetic field loops out into space instead of looping
back into the Sun, areas of magnetic anomalies (they often occur
at the poles). In X-ray photographs of the Sun, coronal holes
are black areas. Coronal holes can last for months or years. The
solar wind is emitted from coronal holes. |
CORONAL MASS EJECTION
Coronal mass ejections (CME's) are huge, balloon-shaped
plasma bursts that come from the
Sun. As these bursts of solar wind rise above the Sun's
corona, they move along the Sun's magnetic field lines and
increase in temperature up to tens of millions of degrees. These
bursts release up to 220 billion pounds (100 billion kg) of
plasma. CME's can disrupt Earth's satellites. |
COSMIC BACKGROUND RADIATION
Cosmic Background Radiation (abbreviated CMB, CMBR and CBR) is
the radiation (energy) which remains from the original Big Bang
explosion which formed the universe. This radiation has cooled
as the universe has expanded and is now slightly less than 3
degrees above absolute zero. |
COSMIC RAYS
Cosmic rays are very high energy particles that travel through
space near the speed of light. The 10 most abundant elements in
cosmic rays are hydrogen, helium, oxygen, carbon, neon,
nitrogen, magnesium, silicon, iron, and sulfur. Cosmic rays many
sources, including the Sun, supernovae, and distant galaxies.
Some cosmic rays enter the Earth's atmosphere. |
COSMIC SNOWBALL
There is a new and very controversial theory that there are
comets composed of frozen water that are constantly
bombarding the
Earth. These "cosmic snowballs" have (perhaps) been seen by
the visible imaging system of the Polar Satellite. These frozen
comets vaporize in the atmosphere, adding water vapor to the
environment. |
COSMIC YEAR
A cosmic year is the time it takes the
Sun (and our entire
solar system) to complete an orbit around the center of the
Milky Way galaxy. A cosmic year is roughly 225 million
years. |
COSMOLOGY
Cosmology is the study of the structure, origin, and evolution
of the universe. |
COSMOLOGICAL RED SHIFT
The cosmological red shift is a phenomenon in which light from
distant sources is
red-shifted because space is expanding (and objects in the
universe are receding from other objects due to this expansion). |

COSMONAUT
Cosmonaut is the Russian word for astronaut, a person who
ventures into space. |
COSMOS
The cosmos refers to a universe that is a complete, harmonious,
and orderly system. |

CRAB NEBULA
The Crab Nebula (M1) is a cloud of intergalactic gas and dust.
It is the remnant of a
supernova that was seen on Earth in 1054. The Crab Nebula
can be found in the
constellation Taurus. |

CRATER
Impact craters are the remains of collisions between an
asteroid, or
meteorite and a planet, planetoid, or moon. |
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CRATER RAYS
Crater rays are lines of ejecta radiating from a crater. |

CREPE RING
The Crêpe ring (also called the C ring) is the inner ring of
Saturn's three major rings; it is smaller and less visible
than the A and B rings. It is visible using a small telescope. |
CREPUSCULAR RAYS
Crepuscular rays are shafts of sun rays and shadows that energe
from behind puffy cumulus clouds. |

CRESCENT MOON
A crescent moon is part way between a half moon and a new moon,
or between a new moon and a half moon. |
CRITICAL FLUID
A critical (or supercritical) fluid is a liquid/gas under
extreme pressure. These critical fluids have unique
characteristics, the density of a liquid and the mobility of a
gas. Critical fluids exist deep inside some planets; for
example, there is supercritical water deep inside the
Earth. |
CRUITHNE
Cruithne is an
asteroid about 3 miles (5 kilometres) in diameter that is
co-orbital with the Earth, which means that it shares roughly
the same orbit as the Earth. It is a
Near-Earth asteroid (NEA 3753). From the Earth, it appears
to have a horseshoe-shaped orbit; it get3s close to the Earth,
then it moves away again. It's orbit is highly inclined to
Earth's orbit. At its closest approach (which happens ever
100,000 years, Cruithne comes to within 10 million miles (15
million km) of Earth (40 times the distance from the Earth to
the Moon). Cruithne was named for the first Celtic tribal group
that settled in the British Isles. Cruithne was discovered on
October 10, 1986 by D. Waldron at Siding Spring Observatory,
Coonabarabran, Australia. |

CRUST
The crust is the outermost layer of the lithosphere (the solid
part of the
Earth consisting of the crust (broken
into plates) and the upper mantle). |

CRUX
Crux (or Crux Australis) is the scientific name of the
Southern Cross constellation. This well-known, cross-shaped
Southern Hemisphere constellation is on the Australian flag. The
brightest star in Crux is Acrux (alpha Cru), a double-star
system at the base of the cross. The second-brightest star is
Becrux or Mimosa (Beta Cru); the third-brightest is Gacrux
(Gamma Cru). The Jewel Box (also known as Kappa Crucis) is an
open cluster of about 100 stars in the Southern Cross. Crux lies
on the Milky Way and is surrounded by the constellation
Centaurus on three sides. |

CRYPTOVOLCANO
A cryptovolcano is a volcano-like feature on a planet or
moon. They may or may not be volcanoes. For examples,
cryptovolcanoes have been seen on the surface of Ganymede, a
moon of Jupiter (one is pictured above). |
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CRUX
Crux (or Crux Australis) is the scientific name of the Southern
Cross
constellation. This well-known, cross-shaped Southern
Hemisphere constellation is on the Australian flag. The
brightest star in Crux is Acrux (alpha Cru), a double-star
system at the base of the cross. The second-brightest star is
Becrux or Mimosa (Beta Cru); the third-brightest is Gacrux
(Gamma Cru). The
Jewel Box (also known as Kappa Crucis) is an
open cluster of about 100
stars in the Southern Cross. Crux lies on the Milky Way and
is surrounded by the constellation Centaurus on three sides. |

CRYPTOVOLCANO
A cryptovolcano is a volcano-like feature on a planet or moon.
They may or may not be volcanoes. For examples, cryptovolcanoes
have been seen on the surface of Ganymede, a moon of
Jupiter (one is pictured above).
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CRYSTALS
Crystals are solids whose atoms form a very regular pattern. |
CUBEWANO
A Cubewano is a main
Kuiper belt objects, ones that are not influenced by the
resonances of the outer planets. Cubewanos are farther from the
Sun than about 41
AU. Compare with
Plutino. |
CULMINATION
Culmination is the highest altitude that a celestial object
attains above the horizon (as seen from Earth); an object
culminates as it crosses the observer's
meridian. |
CURTATE
Curtate means shortened or abbreviated. |
CURVATURE OF SPACE-TIME
The curvature of space-time is a distortion of space-time that
is caused by the gravitational field of matter. The degree of
curvature depends on the strength of the gravitational field
(which depends on the massiveness of the objects in that part of
space). An object traveling in space moves along the curves in
space-time. |

CYGNUS
Cygnus (the swan) is a
constellation that is shaped like a large cross. It is also
known as the Northern Cross. It is seen along the
Milky Way in the northern hemisphere. At its tail is the
very bright star
Deneb, (alpha Cygni) and at its head is the double star
Albireo, (beta Cygni). |

CYGNUS A
Cygnus A (located in the
constellation Cygnus) is the most powerful radio source
visible from
Earth. This double-lobed
radio galaxy is 500,000 light-years wide and is located 600
million
light-years from Earth. It was identified by Hey, Parsons
and Phillips in 1946. |

CYGNUS LOOP
The Cygnus loop is a
nebula, a
supernova remnant in the
constellation Cygnus. It covers a region in the sky six
times the diameter of the full
Moon. The supernova exploded about 15,000-20,000 years ago
and is still expanding. The nebula is almost spherical with some
bright filaments. |
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