+
NASA Homepage
+
NASA en Español
+
Contact NASA
SSE Home
> Dictionary
Dictionary Lookup
Can't find it? Don't understand it?
Ask us.
Find entries
starting with
containing
caldera
Crater formed by an explosion or collapse of a volcanic vent. A large volcanic crater produced by the collapse of underground lava reservoirs. (Image: Tupan Patera's caldera on Io.)
canyon
A deep valley with steep sides. (Also
chasma
)
carbon
abundant element found in all known organic compounds (living things) and many inorganic compounds. Carbon is found in everything from graphite (pencil lead) to diamonds to gasoline.
carbon dioxide
A colorless and odorless gas. Plants on Earth need carbon dioxide to live.
carbonate
A compound containing carbon and oxygen (i.e. calcium carbonate a.k.a. limestone).
cartographic
Having to do with the science and art of constructing maps and charts.
cartography
The science and art of constructing maps and charts.
catena
A chain of craters.
cavus
A hollow, irregular depression.
chaos
A distinctive area of broken terrain.
charge-coupled device (CCD)
An electronic device that consists of a regular array of light sensitive elements that emit electrons when exposed to light.
chasma
A canyon.
Chicxulub crater
a very large impact crater near the Yucatan Peninsula in Mexico. The effects of this particular impact may have been responsible for the extinction of the dinosaurs 65 million years ago.
chromophores
Groups of atoms or molecules that are responsible for pigmentation (color).
chromosphere
The lower level of the solar atmosphere between the photosphere and the corona.
colles
Small hills or knobs.
coma
A spherical cloud of material surrounding the head of a comet. This material is mostly gas that the Sun has caused to boil off the comet's icy nucleus. This gas is illuminated both by reflected sunlight and light emitted by excited molecules. A cometary coma can extend up to a million miles from the nucleus.
comet
A chunk of frozen gasses, ice, and rocky debris that orbits the Sun. A comet nucleus is about the size of a mountain on Earth. When a comet nears the Sun, heat vaporizes the icy material producing a cloud of gaseous material surrounding the nucleus, called a coma. As the nucleus begins to disintegrate, it also produces a trail of dust or dust tail in its orbital path and a gas or ion tail pointing away from the Sun. Comet comas can extend up to a million miles from the nucleus and comet tails can be millions of miles long. There are thought to be literally trillions of comets in our solar system out past Neptune and Pluto, but only once a decade or so does one become near and bright enough to see easily without binoculars or a telescope. (Photo copyright:
Gerald Rhemann
)
More on comets >>
compression
A packing or reduction in the amount of data being transmitted, using a mathematical formula similar to averaging, in order to optimize the transmission of data from the spacecraft. Once received, these data are "unpacked" (decompressed) to reconstruct the full image. However, if noise (see Radiation) is present it may cause incorrect values for the picture elements it was averaged with, which also affects the resulting image.
conjunction
An inferior planet (closer to the sun than Earth - Mercury and Venus) is said to be "in inferior conjunction" when it is directly between the Earth and the Sun. It is "in superior conjunction" when it is on the opposite side of the Sun from the Earth.
The superior planets (the six planets farther from the Sun than Earth) are "in conjunction" when it is on the opposite side of the Sun from the Earth. A superior planet obviously cannot have an inferior conjunction. When the Earth is at inferior conjunction with respect to an observer on a superior planet we say that planet is "in opposition" from Earth's perspective.
constellation
One of the stellar patterns identified by name, usually of mythological gods, people, animals and objects. Also the region of the sky containing that star pattern.
convection
The transfer of heat from a region of high temperature to a region of lower temperature by the displacement of the cooler molecules by the warmer molecules.
corona
the uppermost level of the solar atmosphere, characterized by low densities and high temperatures (> 1.0E+06? K).
coronagraph
A special telescope which blocks light from the disk of the Sun in order to study the solar atmosphere. See the image on the right for more information.
cosmic ray
An extremely energetic charged particle.
crater
A typically bowl-shaped pit, depression, cavity or hole, generally of considerable size and with steep slopes, formed on a surface or in the ground by the explosive release of chemical or kinetic energy. Also depression around the mouth of a volcano.
crater density
The number of craters on a surface per unit area.
crater size distribution
The relative numbers of craters of given sizes on a surface.
cross-cut
An interruption of a geologic feature by another, which can give an indication of the relative ages of these geologic features/events. (i.e. a fault cutting across an impact crater would be younger than the crater.)
crust
The outermost layer of a planet, i.e. the surface. On Earth, we live on the crust.
Explore more of NASA on the Web:
NASA Site Network
Ciencia@NASA
Earth Observatory
Great Images in NASA
Human Space Flight Web
Liftoff to Learning
Mars Exploration
NASA Education Program
NASA History
NASA Image Exchange
NASA Kids
NASA Science Update Newsletter
Planetary Photojournal
Science@NASA
NASA Technology
NASA Enterprises and Field Centers
Aeronautics Research
Earth Science
Exploration Systems
Office of Space Operations
Space Science
NASA Headquarters
Ames Research Center
Dryden Flight Research Center
Glenn Flight Research Center
Goddard Space Flight Center
Jet Propulsion Laboratory
Johnson Space Center
Kennedy Space Center
Langley Research Center
Marshall Space Flight Center
Stennis Space Center
+
Awards & Recognition
+
Send to a Friend
+
The Vision for Space Exploration
+
NASA Solar System Exploration Roadmap
+
Privacy/Copyright/Image Use Policy
NASA Official: Marilyn Lindstrom
Outreach Manager: Alice Wessen
Editors: Phil Davis and Kirk Munsell
Science Writer: Samantha Harvey
Webmaster: David Martin
Last Updated: 30 Dec 2008
+
Contact Us