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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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Tethys Ocean<br />

Tethys Ocean In geophysics, the continents<br />

of Laurasia <strong>and</strong> Gondwanal<strong>and</strong> were separated<br />

by the Tethys Ocean approximately 200 million<br />

years ago. This ocean has closed, <strong>and</strong> the<br />

Mediterranean Sea is a remnant. See continental<br />

drift.<br />

texture See cosmic texture.<br />

Thalassa Moon of Neptune also designated<br />

NVII. Discovered by Voyager 2 in 1989, it is<br />

a small, irregularly shaped body approximately<br />

40 km in radius. Its orbit has an eccentricity of<br />

0.00016, an inclination of 0.21 ◦ , a precession<br />

of 551 ◦ yr −1 , <strong>and</strong> a semimajor axis of 5.01 ×<br />

10 4 km. Its mass has not been measured. It<br />

orbits Neptune once every 0.3115 Earth days.<br />

Tharsis Province A broad Martian topographic<br />

rise centered on the equator at longitude<br />

115 ◦ W. It st<strong>and</strong>s as much as 10 km above the reference<br />

datum, measures ≈ 8000 km across, <strong>and</strong><br />

it occupies ≈ 25% of the surface area of Mars.<br />

It is the most pronounced region of central vent<br />

volcanism on Mars. It has four large shield volcanoes<br />

(Olympus Mons, Ascraeus Mons, Pavonis<br />

Mons, <strong>and</strong> Arsia Mons, the summits of<br />

which are concordant, st<strong>and</strong>ing 27 km above<br />

the reference datum). Olympus Mons st<strong>and</strong>s<br />

25 km above the plains, <strong>and</strong> the other three<br />

st<strong>and</strong> 17 km above the plains. All are considered<br />

to have formed by successive eruptions of<br />

low-viscosity lavas. The volcanoes account for<br />

half the planet’s volcanic production from the<br />

late Hesperian until the Amazonian.<br />

The province is asymmetrical being twice<br />

as steep at the northwestern limit as it is on<br />

the southeastern limit. At the NW, it forms a<br />

continuous slope (only broken by remnants of<br />

old cratered terrain, e.g., Tempe Terra) with the<br />

sparsely cratered northern lowl<strong>and</strong> terrain, <strong>and</strong><br />

on the SE, it forms a continuous slope grading<br />

into the high-st<strong>and</strong>ing, highly cratered southern<br />

hemisphere terrain. It demonstrates a complex<br />

<strong>and</strong> extended tectonic record, being at the center<br />

of a vast radial fracture system that affects<br />

half the planet, <strong>and</strong> a substantial free-air gravity<br />

anomaly. Additionally, the huge equatorial<br />

canyons of Noctis Labyrinthus start at the center<br />

of the bulge <strong>and</strong> extend down the eastern flank<br />

to form Valles Marineris.<br />

© 2001 by CRC Press LLC<br />

474<br />

Thebe Moon of Jupiter, also designated JXV.<br />

Discovered by S. Synnott in 1979, its orbit has<br />

an eccentricity of 0.015, an inclination of 0.8 ◦ ,<br />

<strong>and</strong> a semimajor axis of 2.22 × 10 5 km. Its size<br />

is 55 × 45 km, its mass 7.60 × 10 17 kg, <strong>and</strong> its<br />

density 1.6 g cm −3 . It has a geometric albedo of<br />

0.05 <strong>and</strong> orbits Jupiter once every 0.674 Earth<br />

days.<br />

thermal anisotropy See kinetic temperature,<br />

plasma stress tensor.<br />

thermal bar Due to cabbeling, mixing of<br />

two water masses with identical density but different<br />

temperature <strong>and</strong> salinity generates denser<br />

water. The thermal bar relates to the special<br />

case of mixing two water bodies with temperatures<br />

below <strong>and</strong> above 4 ◦ C. The mixed water<br />

has close to maximum density <strong>and</strong> subsequently<br />

sinks as thermal plumes. The term “bar” refers<br />

to the phenomenon that the original waters cannot<br />

cross the sinking plumes.<br />

thermal boundary layer A portion on the<br />

edge of a body with a high thermal gradient. In<br />

convective systems (such as the Earth’s mantle),<br />

this is commonly associated with the edges of<br />

each convecting layer. The oceanic lithosphere<br />

is one example of a thermal boundary layer<br />

<strong>and</strong> illustrates clearly the importance of this<br />

boundary layer for the convective process: the<br />

layer thickness is very small at mid-ocean ridges<br />

where new boundary layer material is erupted<br />

from beneath, but the thickness increases moving<br />

away from the ridge as heat is removed from<br />

the plate by diffusion. This production of a<br />

cool boundary layer causes negative buoyancy,<br />

which allows the oceanic slab to plunge down<br />

into the interior of the convective region, transporting<br />

a heat deficit inwards (<strong>and</strong> by implication,<br />

causing a net transport of heat towards the<br />

surface). It is quite likely that there is another<br />

thermal boundary layer at the base of the mantle,<br />

where the seismically distinct D” layer is to<br />

be found <strong>and</strong> where perhaps a reverse process is<br />

taking place except that boundary layer material<br />

appear to detach from the core-mantle boundary<br />

in the form of blobs rather than slabs.<br />

thermal bremsstrahlung See bremstrahlung<br />

[thermal].

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