A theory of local formation of isotopic anomalies in meteorites

The consequences of a postulated collision between planets in the early solar system have been investigated. At least one of the planets has been taken with a D/H ratio similar to that of Venus (0.016) and the temperature of the collision interface (3 × 10⁶ K) triggers chain reactions in near-surface material beginning with D-D reactions. The initial composition of the reacting material is consistent with a silicate + ices surface and a hydrogen-helium-inert gas atmosphere. The reaction chain contains 284 reactions, plus reverse reactions, and 40 radioactive decay processes. When the pressure in the reacting region is sufficiently high the colliding planets are blown apart and the highly-processed material at the heart of the explosion mixes with less processed and unprocessed material from cooler parts of the system. Mixtures of materials are found to explain isotopic anomalies associated with oxygen, magnesium, neon, silicon, carbon and nitrogen. The local production of isotopic anomalies avoids the problems associated with other suggested explanations - in particular the observation of neon E, almost pure²²Ne, assumed as the product of the decay of²²Na with a half-life of 2.6 years.