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Fundamental Astronomy

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surrounding an elevated plain, the diameter of which<br />

can be as big as several hundreds of kilometres. They<br />

are possibly examples of local hot spots, mantle upwellings<br />

that have expanded and formed bulges. When<br />

the flow has stopped, the bulge has sunk and formed<br />

a set of ring mountains.<br />

In other places fluid lava flows have produced long,<br />

sinuous channels extending for hundreds of kilometres.<br />

Most of the Venusian impact craters are undeformed.<br />

This indicates that the Venusian surface must be young<br />

because erosion, volcanism and tectonic forces should<br />

affect the craters, too. Resurfacing processes may frequently<br />

cover the old craters, and all craters visible<br />

are therefore young, presumably less than 500 million<br />

years. There are no impact crates smaller than about<br />

1.5–2 km because smaller meteoroids are burned in the<br />

thick atmosphere.<br />

The Earth and Venus are almost equal in size, and<br />

their interiors are assumed to be similar. Venus has an<br />

iron core about 3000 km in radius and a molten rocky<br />

mantle covering the majority of the planet. Probably due<br />

to its slow rotation, however, Venus has no magnetic<br />

field. The analyses made by the Venera landers have<br />

shown that the surface material of Venus is similar to<br />

terrestrial granite and basalt (Fig. 7.26).<br />

Venus has no satellites.<br />

7.12 The Earth and the Moon<br />

The third planet from the Sun, the Earth, and its satellite,<br />

the Moon, form almost a double planet. The relative size<br />

of the Moon is larger than that of any other satellite,<br />

excluding the moon of Pluto. Usually satellites are much<br />

smaller than their parent planets.<br />

The Earth is a unique body, since a considerable<br />

amount of free water is found on its surface. This is possible<br />

only because the temperature is above the freezing<br />

point and below the boiling point of water and the atmosphere<br />

is thick enough. The Earth is also the only planet<br />

where life is known to exist. (Whether it is intelligent or<br />

not is yet to be resolved...). The moderate temperature<br />

and the water are essential for terrestrial life, although<br />

some life forms can be found in extreme conditions.<br />

The diameter of the Earth is 12,000 km. At the centre,<br />

there is an iron–nickel core where the temperature is<br />

7.12 The Earth and the Moon<br />

Fig. 7.27. Internal structure of the Earth. The speed of the<br />

seismic waves, density, pressure, and temperature are shown<br />

as a function of depth<br />

5000 K, the pressure 3 × 10 11 Nm −2 and the density<br />

12,000 kg m −3 (Fig. 7.27).<br />

The core is divided into two layers, inner and outer<br />

core. The inner core, below 5150 km comprises only of<br />

1.7% of the mass of the Earth. It is solid because of<br />

high pressure. The nonexistence of the seismic transverse<br />

S waves below a depth of 2890 km indicates that<br />

the outer core is molten. However, the speed of the longitudinal<br />

P waves change rapidly at a depth of 5150 km<br />

showing an obvious phase transition. It has been discovered<br />

that the solid inner core rotates with respect to<br />

the outer core and mantle.<br />

161

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