Editing Necron Red II

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Based on a combination of geologic surveys and the close examination of the planet's geology, the surface of Necron Red II appears to be composed primarily of basalt. Some evidence suggests that a portion of the planet's surface is more silica-rich than typical basalt, and may be similar to andesitic rocks on Earth; however, these observations may also be explained by silica glass. Much of the surface is deeply covered by a fine iron (III) oxide dust that has the consistency of talcum powder.
Based on a combination of geologic surveys and the close examination of the planet's geology, the surface of Necron Red II appears to be composed primarily of basalt. Some evidence suggests that a portion of the planet's surface is more silica-rich than typical basalt, and may be similar to andesitic rocks on Earth; however, these observations may also be explained by silica glass. Much of the surface is deeply covered by a fine iron (III) oxide dust that has the consistency of talcum powder.


Although Necron Red II has no intrinsic magnetic field, observations show that parts of the planet's crust have been magnetized and that alternating polarity reversals of its dipole field have occurred. This paleomagnetism of magnetically susceptible minerals has properties that are very similar to the alternating bands found on the ocean floors of [[Earth]]. One theory, is that these bands demonstrate plate tectonics on Necron Red II 4 billion years ago, before the planetary dynamo ceased to function and caused the planet's magnetic field to weaken to it's current level.
Although Necron Red II has no intrinsic magnetic field, observations show that parts of the planet's crust have been magnetized and that alternating polarity reversals of its dipole field have occurred. This paleomagnetism of magnetically susceptible minerals has properties that are very similar to the alternating bands found on the ocean floors of Earth. One theory, is that these bands demonstrate plate tectonics on Necron Red II 4 billion years ago, before the planetary dynamo ceased to function and caused the planet's magnetic field to weaken to it's current level.


Current models of the planet's interior imply a core region about 1,480 kilometers in radius, consisting primarily of iron with about 14–17% sulfur. This iron sulfide core is partially fluid, and has twice the concentration of the lighter elements than exist at Earth's core. The core is surrounded by a silicate mantle that formed many of the tectonic and volcanic features on the planet, but now appears to be inactive. The average thickness of the planet's crust is about 50 km, with a maximum thickness of 125 km. Earth's crust, averaging 40 km, is only a third as thick as Necron Red II’s crust relative to the sizes of the two planets.
Current models of the planet's interior imply a core region about 1,480 kilometers in radius, consisting primarily of iron with about 14–17% sulfur. This iron sulfide core is partially fluid, and has twice the concentration of the lighter elements than exist at Earth's core. The core is surrounded by a silicate mantle that formed many of the tectonic and volcanic features on the planet, but now appears to be inactive. The average thickness of the planet's crust is about 50 km, with a maximum thickness of 125 km. Earth's crust, averaging 40 km, is only a third as thick as Necron Red II’s crust relative to the sizes of the two planets.
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