Mar 5, 2019

Javahar Navoday exam hall ticket download start now see here and download

Javahar Navoday exam hall ticket download start now see here and download

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Like Earth, Mars has differentiated into a dense metallic core overlaid by less dense materials.[38] Current models of its interior imply a core with a radius of about 1,794 ± 65 kilometers (1,115 ± 40 mi), consisting primarily of iron and nickel with about 16–17% sulfur.[39] This iron(II) sulfide core is thought to be twice as rich in lighter elements as Earth's.[40] The core is surrounded by a silicate mantle that formed many of the tectonic and volcanic features on the planet, but it appears to be dormant. Besides silicon and oxygen, the most abundant elements in the Martian crust are iron, magnesiumaluminumcalcium, and potassium. The average thickness of the planet's crust is about 50 km (31 mi), with a maximum thickness of 125 km (78 mi).[40] Earth's crust averages 40 km (25 mi).

Surface geology



Mars is a terrestrial planet that consists of minerals containing silicon and oxygen, metals, and other elements that typically make up rock. The surface of Mars is primarily composed of tholeiitic basalt,[41]although parts are more silica-rich than typical basalt and may be similar to andesiticrocks on Earth or silica glass. Regions of low albedo suggest concentrations of plagioclase feldspar, with northern low albedo regions displaying higher than normal concentrations of sheet silicates and high-silicon glass. Parts of the southern highlands include detectable amounts of high-calcium pyroxenes. Localized concentrations of hematite and olivine have been found.[42] Much of the surface is deeply covered by finely grained iron(III) oxide dust.[43][44]

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