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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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I<br />

Iapetus Moon of Saturn, also designated<br />

SVIII. Discovered by Cassini in 1671, it is noted<br />

for a surface where the leading edge has an<br />

albedo of 0.02 to 0.05, <strong>and</strong> the trailing edge has<br />

an albedo of 0.5. It has been conjectured that<br />

the difference is due to the leading edge accreting<br />

dark material (possibly from Phoebe) as it<br />

orbits. Its orbit has an eccentricity of 0.028, an<br />

inclination of 14.72 ◦ , <strong>and</strong> a semimajor axis of<br />

3.56 × 10 6 km. Its radius is 730 km, its mass is<br />

1.88 × 10 21 kg, <strong>and</strong> its density is 1.15 g cm −3 .<br />

It orbits Saturn once every 79.33 Earth days.<br />

Icarus An Earth-crossing Apollo asteroid<br />

with perihelion 0.187 AU, aphelion 1.969 AU,<br />

approaching within 0.04 AU of the Earth’s orbit.<br />

Its orbital inclination is 22.9 ◦ <strong>and</strong> its orbital period<br />

is about 1.12 years. Based on its brightness,<br />

its diameter is 1 to 2.5 km.<br />

ice A generic term referring to those substances<br />

of intermediate volatility, which are<br />

sometimes solid <strong>and</strong> sometimes gaseous. Examples<br />

of ices that are commonly encountered<br />

in astrophysical contexts are H2O, NH3, CH4,<br />

<strong>and</strong> CO2. Organic materials with intermediate<br />

volatilities are sometimes called organic ices,<br />

CHON (i.e., substances composed mainly of the<br />

elements C, H, O, <strong>and</strong> N) or simply organics.<br />

ice age A period of geologic history during<br />

which considerable portions of the Earth were<br />

covered with glacial ice. There have been many<br />

ice ages in the geological history of the Earth;<br />

during some of them, the ice sheets were situated<br />

in the polar regions <strong>and</strong> some of them were<br />

in equatorial regions. In the last ice age, the<br />

Pleistocene, about one-fifth of the Earth’s surface<br />

was covered by glacial ice. The climatic<br />

feature of ice ages is a very large temperature<br />

decrease. Over mid-latitude region, temperature<br />

can decrease more than 10 ◦ C <strong>and</strong> ice <strong>and</strong><br />

snow can cover 20 to 30% of the Earth’s surface.<br />

The reasons for the ice ages may include the<br />

igneous<br />

long-term variations of solar radiation, orbit parameters<br />

of the Earth, <strong>and</strong> variations of climatic<br />

systems <strong>and</strong> processes of the rock lithosphere<br />

(including nonlinear feedback processes).<br />

ICM-ISM stripping An important consequence<br />

of the interactions between a member<br />

galaxy in a cluster <strong>and</strong> the intracluster medium<br />

(ICM), resulting in stripping the galaxy of its interstellar<br />

medium (ISM) due to the ram pressure<br />

of ICM (Gunn <strong>and</strong> Gott, 1972). Suspected sites<br />

of the ongoing ICM-ISM stripping include some<br />

of the ellipticals <strong>and</strong> spirals in the Virgo cluster,<br />

<strong>and</strong> a few spirals in the cluster A1367. Observed<br />

signatures for the ICM-ISM stripping rather than<br />

other internal processes such as starbursts, cooling<br />

flows, or gravitational interactions between<br />

member galaxies, consist in a relatively undisturbed<br />

stellar disk, together with a selectively<br />

disturbed HII region containing abruptly truncated<br />

Hα disk <strong>and</strong> one-sided filamentary structures<br />

above the outer disk plane. The ISM-ICM<br />

stripping is consistent with observational facts<br />

about spiral galaxies in clusters: many of them<br />

are deficient in gaseous disks, those with truncated<br />

gaseous disks have relatively undisturbed<br />

stellar components, they sustain vigorous star<br />

formation in the inner disks but very little in the<br />

outer disks. The degree of severity of HII disk<br />

truncation signifies the decline in star formation<br />

rates <strong>and</strong> the time elapsed since the ISM-ICM<br />

stripping began in cluster spirals.<br />

ideal gas A theoretical gas consisting of perfectly<br />

elastic particles in which the forces between<br />

them are zero or negligible.<br />

ideal gas [equation of state] The thermodynamic<br />

relationship between pressure, volume,<br />

number of particles, <strong>and</strong> temperature for an ideal<br />

gas. It is mathematically expressed by the equation<br />

PV = NkT, where P is the pressure, V<br />

is the volume, N is the number of particles, k<br />

is Boltzmann’s constant, <strong>and</strong> T is the absolute<br />

temperature.<br />

igneous Referring to rock that has been in a<br />

totally molten state. Igneous rocks are classified<br />

as volcanic, or extrusive, if they have been<br />

extruded from the Earth in volcanic flow. Examples<br />

are rhyolite, <strong>and</strong>esite, <strong>and</strong> basalt. Igneous<br />

© 2001 by CRC Press LLC<br />

c○ 2001 by CRC Press LLC 237

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