29.03.2013 Views

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

TT+LG·(JD−2443144.5)·86400 sec, where<br />

LG = 6.96929 · 10 −10 by definition as of 1992,<br />

JD st<strong>and</strong>s for the Julian Date in TDT, <strong>and</strong> TT<br />

st<strong>and</strong>s for Terrestrial Time, which is essentially<br />

the same as TDT. Presumably, the “constant”,<br />

LG, is subject to revision when <strong>and</strong> if the potential<br />

on the geoid is redetermined. For details,<br />

seeIERSTechnicalNote13, TheIERSSt<strong>and</strong>ards<br />

(Ed.: D.D. McCarthy) (U.S. Naval Observatory,<br />

Washington, 1992).<br />

Terrestrial Dynamical Time (TDT) In<br />

1977, Dynamical Time was introduced in two<br />

forms, TDT <strong>and</strong> Barycentric Dynamical Time<br />

(TDB). The difference in these two consists of<br />

periodic terms due to general relativity <strong>and</strong> does<br />

not exceed about 1.7 milliseconds in any year.<br />

TDT is used for the determination of the orbits<br />

of objects orbiting the Earth. It advances at the<br />

same rate as International Atomic Time (TAI),<br />

being equal, for all practical purposes, to TAI +<br />

32.184 s. Both TAI <strong>and</strong> TDT contain relativistic<br />

effects of the Earth’s motion around the sun,<br />

which reflect the fact that any reference frame<br />

centered on Earth’s center is not inertial. Any of<br />

TDT, TAI, <strong>and</strong> TCG are thus subject to further<br />

special relativistic corrections in their relationship<br />

to any barycentric time st<strong>and</strong>ard, such as<br />

TCB. For details, see IERS Technical Note 21,<br />

The IERS Conventions (Ed.: D.D. McCarthy)<br />

(U.S. Naval Observatory, Washington, 1996).<br />

See dynamical time.<br />

terrestrial heat flow Heat flux from the interior<br />

of the Earth. It usually means the conductive<br />

heat flux measured at the surface of the<br />

Earth, <strong>and</strong> it is usually called heat flow or heat<br />

flowdensity. Thepresentglobalaverageisabout<br />

0.06 W/m 2 .<br />

terrestrial planets Those planets that are<br />

similar to the Earth in their characteristics.<br />

There are four terrestrial planets in our solar system:<br />

Mercury, Venus, Earth, <strong>and</strong> Mars. Characteristics<br />

of the terrestrial planets include small<br />

size (< 13,000 km in diameter), high density<br />

(> 3000kg/m 3 , indicatingrockycompositions),<br />

close to the sun (< 1.5 astronomical units), few<br />

or no moons, <strong>and</strong> no rings. These characteristics<br />

differ considerably from those of the Jovian<br />

planets, which dominate the outer solar sys-<br />

© 2001 by CRC Press LLC<br />

Tethys<br />

tem. Although Pluto is similar to the terrestrial<br />

planets with its small size, one moon, <strong>and</strong> lack<br />

of rings, its large distance from the sun <strong>and</strong> its<br />

lower density (about 2000 kg/m 3 , indicating an<br />

icy composition) place it in a category of its own,<br />

where it shares characteristics with many of the<br />

large icy bodies in the outer solar system. The<br />

terrestrial planets are sometimes also called the<br />

inner planets, since they are located in the inner<br />

part of the solar system.<br />

Terrestrial Time (TT) In 1991, the International<br />

Astronomical Union (IAU) defined an<br />

“ideal form of Terrestrial Dynamical Time”, <strong>and</strong><br />

designated Terrestrial Time. This definition appears<br />

to be primarily intended to extend the<br />

scope of TDT off the geoid, by imposing certain<br />

restrictions on relativistic coordinate systems.<br />

It is used in dynamical theories of solar<br />

system motions, <strong>and</strong> it could take into consideration<br />

the need to bring dynamical measures of<br />

time (from the motions of spacecraft orbiting the<br />

Earth) into accord with atomic time. For practical<br />

purposes, it is identical with Terrestrial Dynamical<br />

Time. For details, see IERS Technical<br />

Note 13, The IERS St<strong>and</strong>ards (Ed.: D.D. Mc-<br />

Carthy) (U.S. Naval Observatory, Washington,<br />

1992).<br />

tesla A unit of magnetic flux equal to one<br />

weber per square meter.<br />

Tethys Moon of Saturn, also designated<br />

SIII. Discovered by Cassini in 1684. Its surface<br />

shows a crater, Odysseus, with a radius<br />

of 200 km. This is some 40% of the radius of<br />

Tethys <strong>and</strong> is probably at the limit of what the<br />

moon could sustain without breakup. The crater<br />

is now flattened <strong>and</strong> conforms to Tethys’ spherical<br />

shape. There is also a large valley, Ithaca<br />

Chasma, which is 2000 km long <strong>and</strong> extends 3/4<br />

of the way around Tethys. It is some 100 km<br />

wide <strong>and</strong> 3 to 5 km deep. Tethys’ orbit has an<br />

eccentricity of 0, an inclination of 1.86 ◦ , a precession<br />

of 72.25 ◦ yr −1 , <strong>and</strong> a semimajor axis of<br />

2.95 × 10 5 km. Its radius is 530 km, its mass<br />

7.55 × 10 20 kg, <strong>and</strong> its density 1.21 g cm −3 .It<br />

has a geometric albedo of 0.9, <strong>and</strong> orbits Saturn<br />

once every 1.888 Earth days.<br />

473

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!