Possible evidence for partial differentiation of asteroid Lutetia from Rosetta

Benjamin P. Weiss, Linda T. Elkins-Tanton, M. Antonietta Barucci, Holger Sierks, Colin Snodgrass, Jean Baptiste Vincent, Simone Marchi, Paul R. Weissman, Martin Pätzold, Ingo Richter, Marcello Fulchignoni, Richard P. Binzel, Rita Schulz

Research output: Contribution to journalArticlepeer-review

41 Scopus citations

Abstract

The petrologic diversity of meteorites demonstrates that planetesimals ranged from unmelted, variably metamorphosed aggregates to fully molten, differentiated bodies. However, partially differentiated bodies have not been unambiguously identified in the asteroid belt. New constraints on the density, composition, and morphology of 21 Lutetia from the Rosetta spacecraft indicate that the asteroid's high bulk density exceeds that of most known chondritic meteorite groups, yet its surface properties resemble those of some carbonaceous and enstatite chondrite groups. This indicates that Lutetia likely experienced early compaction processes like metamorphic sintering. It may have also partially differentiated, forming a metallic core overlain by a primitive chondritic crust.

Original languageEnglish (US)
Pages (from-to)137-146
Number of pages10
JournalPlanetary and Space Science
Volume66
Issue number1
DOIs
StatePublished - Jun 2012
Externally publishedYes

Keywords

  • Asteroids
  • Chondrites
  • Differentiation
  • Lutetia
  • Metamorphism
  • Planetary evolution
  • Planetesimals
  • Rosetta

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Possible evidence for partial differentiation of asteroid Lutetia from Rosetta'. Together they form a unique fingerprint.

Cite this