Chondrule

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Most meteorites are full of millimeter-sized silicate spherules which are called chondrules (from Greek chondros, grain), suspended in a fine-grained matrix which includes cosmic dust grains and chondrule fragments. Meteorites which contain chondrules are called chondrites or chondritic meteorites. They can consist of up to 80% chondrules.

Chondrites represent the oldest solid material within our solar system and are believed to be the building blocks of the planetary system. Hence, from the abundance of chondrules within these meteorites, it follows that an understanding of the formation of chondrules is important to understand the initial development of the planetary system.

1 Formation
2 Organic compounds in chondrites
3 References
4 Further reading
5 See also
6 External links

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Formation

Chondrules are formed by a rapid heating (within minutes or less) of solid precursor material to temperatures between 1500°C and 1900°C and subsequent melting. This is followed by a cooling within one to several hours (Wood, 1999). However, the environmental setting, the energy source for the heating, and the precursor material are not known. The solar nebula or a protoplanetary environment are possible places of formation.

Proposed energy sources are:

Impact melting
Meteor ablation
Hot inner nebula
FU Orionis outburst of the early sun
Energetic bipolar-shaped outflows
Nebular lightning
Magnetic flares
Accretion shocks
Nebular shocks
Supernova radiation and shockwave

Isotope studies indicate a nearby supernova explosion added fresh material to what became our solar system. The Ningqiang carbonaceous chondrite contained sulfur-36 derived from chlorine-36. As chlorine-36 has a half-life of only 300,000 years, it could not have travelled far from its origin. The presence of iron-60 also indicates a nearby supernova. Such proximity implies the radiation and shockwave would have been significant, although the degree of heating is not known.

In contrast, the fine grained matrix, in which the chondrules are embedded after their accretion into the chondrites parent body, is assumed to have been condensed directly from the solar nebula.

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Organic compounds in chondrites

Most of the organic carbon in CI and CM carbonaceous chondrites is an insoluble complex material. That is similar to the description for kerogen. A kerogen-like material is also in the ALH84001 Martian meteorite (an achondrite).

The CM meteorite from Murchison, Victoria has over 70 extraterrestrial amino acids and other compounds including carboxylic acids, hydroxy carboxylic acids, sulphonic and phosphonic acids, aliphatic, aromatic and polar hydrocarbons, fullerenes, heterocycles, carbonyl compounds, alcohols, amines and amides.

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