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6. Conclusions
A run-away georeactor in the CMB can provide the missing energy source
for the Darwin-Ringwood-Wise fission model for Moon formation. Our
hypothesis provides an alternative explanation for the striking similarity in
elemental and isotopic composition of the Earth’s mantle and lunar rocks, and is
consistent with the sequence of differentiation events during our planet’s earliest
history. Future Moon missions returning lunar samples from greater depths may
contain conclusive evidence for the validity of our hypothesis. The 3He contents
and xenon isotopic compositions in particular, will be a crucial test.
Scientists estimate there are about 1 million tons of helium 3 on the moon, enough to power the world for thousands of years. The equivalent of a single space shuttle load or roughly 25 tons could supply the entire United States' energy needs for a year, according to Apollo17 astronaut and FTI researcher Harrison Schmitt. Cash crop of the moon.
Originally posted by Sinter Klaas
reply to post by Mactire
Well...
It seems we are finding more water at more places previously thought of as hostile towards water.
IMO it is save to assume water is omnipresent. That would mean no need for big space rocks full with water. Which If I'm remembering it correctly, hold a different type of water then the type we have on Earth. Well at least the few we were able to take a look it.
Second A big meteor or asteroid impact is of a massive smaller scale then what the "so called proto planet Thea" supposed to have caused resulting in that big pile of space debris we call our Moon.
But I'm no expert so don't take my word for it...
Internal structure
Main article: Internal structure of the Moon
Chemical composition of the lunar surface regolith (derived from crustal rocks)[22]Compound Formula Composition (wt %)
Maria Highlands
silica SiO2 45.4% 45.5%
alumina Al2O3 14.9% 24.0%
lime CaO 11.8% 15.9%
iron(II) oxide FeO 14.1% 5.9%
magnesia MgO 9.2% 7.5%
titanium dioxide TiO2 3.9% 0.6%
sodium oxide Na2O 0.6% 0.6%
Total 99.9% 100.0%
The Moon is a differentiated body: it has a geochemically distinct crust, mantle, and core. This structure is thought to have developed through the fractional crystallization of a global magma ocean shortly after the Moon's formation 4.5 billion years ago.[23] Crystallization of this magma ocean would have created a mafic mantle from the precipitation and sinking of the minerals olivine, clinopyroxene, and orthopyroxene; after about three-quarters of the magma ocean had crystallised, lower-density plagioclase minerals could form and float into a crust on top.[24] The final liquids to crystallise would have been initially sandwiched between the crust and mantle, with a high abundance of incompatible and heat-producing elements.[1] Consistent with this, geochemical mapping from orbit shows the crust is mostly anorthosite,[5] and moon rock samples of the flood lavas erupted on the surface from partial melting in the mantle confirm the mafic mantle composition, which is more iron rich than that of Earth.[1] Geophysical techniques suggest that the crust is on average ~50 km thick.[1]
The Moon is the second densest satellite in the Solar System after Io.[25] However, the core of the Moon is small, with a radius of about 350 km or less;[1] this is only ~20% the size of the Moon, in contrast to the ~50% of most other terrestrial bodies. Its composition is not well constrained, but it is probably metallic iron alloyed with a small amount of sulphur and nickel; analyses of the Moon's time-variable rotation indicate that it is at least partly molten.[26]
The moon was created by an explosion of matter from of the Earth's interior, where it formed in a runaway uranium fission georeactor at the boundary between the core and mantle according to a radical theory by Rob de Meijer of the University of the Western Cape in South Africa and Wim van Westrenem of VU University Amsterdam.