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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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Z<br />

Zeeman effect The splitting of spectral lines<br />

into groups of closely spaced lines in the presence<br />

of a strong magnetic field. The Zeeman effect<br />

occurs in the spectra of sunspots <strong>and</strong> stars.<br />

This effect demonstrates the existence of magnetic<br />

fields in celestial bodies, <strong>and</strong> since the degree<br />

of the splitting depends on the magnitude<br />

of the magnetic fields, it allows measurement of<br />

the field to be made.<br />

Zeldovich process A process of energy extraction<br />

from a rotating black hole via incident<br />

electromagnetic or gravitational radiation.<br />

When radiation hits a black hole, part of it is<br />

absorbed <strong>and</strong> part is carried away. Normally,<br />

the absorbed part has positive energy <strong>and</strong> the<br />

amplitude of the transmitted wave is reduced.<br />

However, in the case of cylindrical waves, the<br />

absorbed wave may carry negative energy, in<br />

which case the transmitted wave is amplified.<br />

This is the variant with electromagnetic radiation<br />

of the Penrose process. See Penrose process.<br />

zenith The point directly overhead an observer,<br />

as defined by the local horizontal. Technically,<br />

there are three zenith directions: geocentric<br />

zenith, the direction directly away from<br />

the Earth’s center; geodetic zenith, the direction<br />

of the local upwards normal from the Earth<br />

ellipsoid; <strong>and</strong> astronomical zenith, the direction<br />

of the upwards normal from the geoid.<br />

Normally, when used without another qualifier,<br />

zenith refers to either the geodetic or astronomical<br />

zenith, which are within a few arc seconds<br />

of each other. See also altitude, nadir.<br />

zenith angle The angle from the vertical, or<br />

zenith, to a given direction. The zenith angle is<br />

the complement of the altitude.<br />

zero mode See fermionic zero mode.<br />

Zwicky compact galaxies<br />

zero up-crossing The point where the water<br />

surface in a water wave profile crosses the<br />

zero line <strong>and</strong> is trending upward. Used in the<br />

definition of wavelength.<br />

zodiac The apparent path of the sun through<br />

the background stars over the course of the year;<br />

the intersection of the plane of the ecliptic with<br />

the celestial sphere.<br />

zodiacal light A b<strong>and</strong> of diffuse light seen<br />

along the ecliptic near the sun immediately after<br />

sunset or before sunrise. It is created by sunlight<br />

reflecting off the interplanetary dust particles,<br />

which are concentrated along the ecliptic plane.<br />

To see the zodiacal light, you must have very<br />

dark skies; under the best conditions it rivals<br />

the Milky Way in terms of brightness. The material<br />

within the zodiacal light is slowly spiraling<br />

inward toward the sun, due to the Poynting–<br />

Robertson Effect; hence, it must be continuously<br />

replaced by asteroid collisions <strong>and</strong> the debris<br />

constituting comet tails. The zodiacal light is<br />

the name given to the b<strong>and</strong> of light seen close<br />

to the sun while gegenschein is the term applied<br />

to the same b<strong>and</strong> of light located 180 ◦ from the<br />

sun.<br />

zonal In the direction parallel to the equator,<br />

i.e., east-west. See also meridional.<br />

zooplankton Animal forms of plankton.<br />

Z-string See embedded defect.<br />

Zulu Time See Universal Time.<br />

Zwicky compact galaxies Galaxies originally<br />

defined by F. Zwicky as distinguishable<br />

from stars on the Palomar 1.2 m Schmidt telescope<br />

plate <strong>and</strong> with angular diameter between<br />

2 <strong>and</strong> 5 sec of arc. “Compact” is, in astronomy,<br />

a loose synonym of “not fully resolved”.<br />

The notion of compactness of a galaxy therefore<br />

depends on the resolving power of the observational<br />

equipment, although compact galaxies<br />

have, in general, high surface brightness <strong>and</strong><br />

sharp borders. F. Zwicky circulated seven lists<br />

of compact galaxies including about 200 objects<br />

in the mid-1960s. Most of them are of blue<br />

color <strong>and</strong> show emission lines in their spectra.<br />

© 2001 by CRC Press LLC<br />

c○ 2001 by CRC Press LLC 525

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