Compositional trends in rock-forming elements of comet Halley dust
M N Fomenkova1, J F Kerridge, K Marti
1Space Research Institute, Academy of Sciences, Moscow, Russia.
Summary
Cometary dust particles from comet P/Halley show unusual compositions, including magnesium-rich and iron-rich grains. These findings suggest formation through aqueous alteration and secondary processes, not just equilibrium condensation.
Area of Science:
- Cosmic dust analysis
- Cometary science
- Astrochemistry
Background:
- Comet P/Halley dust composition is key to understanding solar system formation.
- Previous missions provided limited elemental composition data for cometary dust.
Purpose of the Study:
- Analyze elemental composition of dust particles from comet P/Halley.
- Investigate the origin and formation processes of unusual cometary grains.
Main Methods:
- Utilized mass spectrometers aboard the VEGA 1 and 2 spacecraft.
- Analyzed elemental composition and mass of dust particles.
Main Results:
- Identified cometary dust particles with unusual magnesium-rich and iron-rich compositions.
- Most particles were a mix of silicates and organic matter.
- Magnesium-rich particles likely represent magnesium carbonates.
Conclusions:
- Cometary dust formation involves processes beyond equilibrium condensation, such as aqueous alteration.
- Secondary processes play a significant role in shaping cometary grain composition.
- Findings offer insights into the early solar system's chemical environment.
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