Proof of planetesimals for asteroid belt?

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    Asteroid Belt Proof
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SUMMARY

The discussion confirms that the metallic components of some asteroid belt objects, specifically M-type asteroids, are remnants of differentiated planetesimals that solidified from liquid cores. This differentiation was facilitated by the presence of Aluminium-26, which provided the necessary heat for core formation through radioactive decay. The total mass of the asteroid belt is approximately 4% of the Moon's mass, indicating its relatively small size compared to larger celestial bodies.

PREREQUISITES
  • Understanding of asteroid classification, particularly M-type asteroids.
  • Knowledge of planetary differentiation processes.
  • Familiarity with Aluminium-26 and its role in planetary formation.
  • Basic concepts of the Solar System's formation timeline.
NEXT STEPS
  • Research the classification and characteristics of M-type asteroids.
  • Study planetary differentiation and its implications for celestial body formation.
  • Explore the role of Aluminium-26 in the early Solar System.
  • Investigate the mass distribution and composition of the asteroid belt.
USEFUL FOR

Astronomers, planetary scientists, and educators interested in the formation and composition of celestial bodies in the Solar System.

zankaon
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If asteroid belt objects are in part iron, is this then consistent with such differentiated pieces being solidified remains of a liquid core(s) of previous colliding planetesimals?

p.s. total mass of asteroid belt may be just 4% of moon. http://en.wikipedia.org/wiki/Asteroid_belt"
 
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zankaon said:
If asteroid belt objects are essentially of just iron,

Hmmm...I thought I answered this.

Most asteroid belt objects are not just iron. Only the M-types.
 
zankaon said:
If asteroid belt objects are in part iron, is this then consistent with such differentiated pieces being solidified remains of a liquid core(s) of previous colliding planetesimals?

p.s. total mass of asteroid belt may be just 4% of moon. http://en.wikipedia.org/wiki/Asteroid_belt"

Simply put, yes. More correctly the metallic meteorites are evidence of a parent body which had differentiated into metals in the core and silicates floating on top to make the crust. This was only possible while extensive amounts of Aluminium-26 was available to create sufficient heat from its radioactive decay. As Al-26 had a half-life of less than ~0.8 million years that means the parent bodies of the metallic meteoroids formed within a few million years of the formation of the Solar system.
 
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