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• W2049291263 abstract "[1] Carbonaceous chondrites are considered to be the most primitive meteorites that contain some of the earliest formed solar system phases, e.g., Ca-Al-rich inclusions and chondrules. The parent bodies of the carbonaceous chondrites are traditionally known to have experienced aqueous alteration. However, the recent paleomagnetic records of the CV chondrite, Allende, indicate remnant magnetism that suggests that these chondrites possibly evolved on the crustal region of a partially differentiated asteroid having a convective molten iron core. We present results based on our comprehensive numerical simulations of the scenario involving melting and planetary differentiation of asteroids. The possibility of a sizable carbonaceous chondritic crust on these differentiated bodies is explored. The simulations indicate that it could be possible to explain the paleomagnetic records of the chondrites by the dynamo-generated magnetic field from the convective molten iron core. Apart from the slow linear accretion scenario, we envisage a scenario involving two episodes of accretion of the asteroids. An early rapid accretion of the asteroids in the initial stage, perhaps within the initial ∼2 Myr, would produce a sizable molten iron core subsequent to differentiation to produce the required magnetic fields. This would be followed by a slow accretion of consolidated chondritic crust, perhaps over several million years. There is also a possibility of the disrupted expulsion of the chondritic crust by the internal pressures generated by gases released during hydration/dehydration reactions." @default.
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• W2049291263 date "2011-06-23" @default.
• W2049291263 modified "2023-09-30" @default.
• W2049291263 title "Did the carbonaceous chondrites evolve in the crustal regions of partially differentiated asteroids?" @default.
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• W2049291263 doi "https://doi.org/10.1029/2010je003757" @default.
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