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Source Parent Bodies of Meteorites by Class

Asteroidal

  1. Acalpulcoite: Unknown but likely same as lodranite though hypothesized to derive from a shallower region within the parent body
  2. Angrite: 3819 Robinson or  289 Nenetta
  3. Aubrite: 3103 Eger, the only known E-class near-Earth asteroid (NEA)
  4. Carbonaceous Ornans (CO): 221 Eos
  5. Carbonaceous Rumuruti (CR): 2 Pallas
  6. HED (Howardite, Eucrite, Diogenite): 4 Vesta (largest asteroid in the asteroid belt and likely source of most HED meteorites)
  7. Iron meteorites: M-Class asteroids
  8. Lodranite: Unknown but likely same as acapulcoites though hypothesized to derive from a deeper region within the parent body
  9. Ordinary Chondrite H-type: Hebe

Planetary

  1. Lunar: Earth’s moon
  2. Martian: Mars

References:

  1. LINKING METEORITES TO ASTEROIDS: HOW MANY PARENT BODIES DO WE SAMPLE IN OUR METEORITE COLLECTIONS? (Click here)
  2. McSween, H. Jr. (1999). Meteorites and Their Parent Planets. 2nd Edition, Cambridge University Press, New York
  3. Hypervelocity impacts as a source of deceiving surface signatures on iron-rich asteroids (Click here)
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