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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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Celsius, Anders<br />

tions from the Earth. The celestial sphere thus<br />

surrounds the Earth, <strong>and</strong> locations on the sphere<br />

are given by the two angles necessary to define<br />

a given direction.<br />

Celsius, Anders Astronomer (1701–1744).<br />

Proposed the Centigrade temperature scale.<br />

Celsius scale Also called Centigrade Scale,<br />

scale for measuring temperature in which the<br />

melting point of ice is 0 ◦ , <strong>and</strong> the boiling point<br />

of water is 100 ◦ . This definition has been superseded<br />

by the International Temperature Scale<br />

1968, which is expressed both in Kelvin <strong>and</strong><br />

degrees Celsius. Named after Anders Celsius<br />

(1701–1744).<br />

Centaur An “outer planet crosser.” A minor<br />

body whose heliocentric orbit is between<br />

Jupiter <strong>and</strong> Neptune <strong>and</strong> typically crosses the<br />

orbits of one of the other outer giant planets<br />

(Saturn, Uranus, Neptune). The orbits of the<br />

Centaurs are dynamically unstable due to interactions<br />

with the giant planets, so they must<br />

be transition objects from a larger reservoir of<br />

small bodies to potentially active inner solar system<br />

objects. The Kuiper belt is believed to be<br />

this source reservoir.<br />

Centaurus A (Cen A) Active galaxy at<br />

RA13 h 25 m 28 s , dec −43 ◦ 01 ′ 11 ′′ in constellation<br />

Centaurus. Also classified as NGC5128. Distance<br />

approximately 3.4Mpc. Large, elliptical<br />

galaxy with strong dust lanes seen in the visible<br />

<strong>and</strong> infrared, strong jets seen in radio (double<br />

lobed) <strong>and</strong> in the X-ray (single lobed). Also<br />

visible in the gamma ray range.<br />

center of figure To a first approximation the<br />

earth is a sphere. However, the rotation of the<br />

earth creates a flattening at the poles <strong>and</strong> an<br />

equatorial bulge. The shape of the earth can be<br />

representedasanoblatespheroidwithequatorial<br />

radius larger than the polar radius by about a factor<br />

of 1/300. The center of the best fit spheroid<br />

to the actual shape of the earth is the center of<br />

figure. There is an offset between the center of<br />

figure <strong>and</strong> the center of mass of a few kilometers.<br />

center of mass In Newtonian mechanics, the<br />

“average” location X of the mass, given in com-<br />

© 2001 by CRC Press LLC<br />

ponents by<br />

X a =<br />

<br />

m(i)x a (i)<br />

<br />

m(i)<br />

,a = 1, 2, 3 ,<br />

where the sums indicated by are over all the<br />

masses, labeled (i). In relativistic mechanics<br />

there are many inequivalent formulations which<br />

all reproduce this nonrelativistic result in the<br />

limit of small velocities.<br />

Centigrade scale See Celsius scale.<br />

centimeter burst A transient solar emission<br />

of radiation at radio wavelengths ∼1 to<br />

10 cm. Centimeter bursts provide a powerful<br />

diagnostic of energetic electrons in the solar<br />

atmosphere, especially during solar flares.<br />

The production mechanisms include thermal<br />

bremsstrahlung, gyrosynchrotron radiation, <strong>and</strong><br />

collective plasma processes.<br />

central meridian passage The passage of a<br />

solar feature across the longitude meridian that<br />

passes through the apparent center of the solar<br />

disk. Useful for identifying a characteristic time<br />

during the transit of a solar feature (e.g., an active<br />

region) across the solar disk.<br />

central peak A mound of deformed <strong>and</strong> fractured<br />

rock found in the center of many impact<br />

craters. This material originally existed under<br />

the crater floor <strong>and</strong> was uplifted by the stresses<br />

associated with the impact event. Central peaks<br />

are believed to form by hydrodynamic flow during<br />

crater collapse. The target material behaves<br />

as a Bingham fluid, which displays properties<br />

of viscous fluids yet has a definite plastic yield<br />

stress. As the crater formed in this target material<br />

collapses, shear stresses cause material to<br />

be jetted up in the center of the crater. When the<br />

shear stresses fall below the cohesion of the target<br />

material, the motion of this central jet ceases,<br />

<strong>and</strong> the material freezes into a central peak.<br />

Central peaks are common features of complex<br />

craters but are associated with the smaller complex<br />

craters. As crater size increases, central<br />

peaks tend to be replaced first by craters with a<br />

ring of central peaks (called a peak ring), then<br />

by a combination of central peaks surrounded<br />

by a peak ring, <strong>and</strong> finally a multiple-ring basin.

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