Sugars in Carbonaceous Chondrites [PDF]
Yoshihiro Furukawa +7 more
openaire +1 more source
Low delta-V near-Earth asteroids: A survey of suitable targets for space missions
In the last decades Near-Earth Objects (NEOs) have become very important targets to study, since they can give us clues to the formation, evolution and composition of the Solar System.
Barucci, M. A. +9 more
core +2 more sources
Forming the Noncarbonaceous Chondrite Parent Bodies in the Presence of the Jupiter Barrier
Meteorites can be divided into two groups—noncarbonaceous chondrite like (NC) and carbonaceous chondrite like (CC)—with distinct stable-isotope compositions. Parent bodies of NC and CC meteorites have overlapping formation ages. This suggests they formed
John Chambers
doaj +1 more source
Antarctic Meteorite Newsletter. Volume 7, number 1: Sample requests and allocations [PDF]
Antarctic meteorites, achondrites, carbonaceous chondrites, ions, and stony-irons are ...
core +1 more source
Glassy chondrule mesostasis in EET 96029: a CM3 component of a minimally altered CM2 carbonaceous chondrite [PDF]
No abstract ...
Lee, M.R., Lindgren, P.
core
Magnetization of carbonaceous asteroids by nebular fields and the origin of CM chondrites [PDF]
Samuel W. Courville +5 more
openalex +1 more source
Iron‐rich aureoles in the CM carbonaceous chondrites Murray, Murchison, and Allan Hills 81002: Evidence for in situ aqueous alteration [PDF]
Nicolaus Hanowski, A. J. Brearley
openalex +1 more source
Life on Earth can grow on extraterrestrial organic carbon
The universe is a vast store of organic abiotic carbon that could potentially drive heterotrophy on habitable planets. Meteorites are one of the transporters of this carbon to planetary surfaces.
Annemiek C. Waajen +3 more
doaj +1 more source
Evolution of carbonaceous chondrite parent bodies: Insights into cometary nuclei [PDF]
It is thought that cometary samples will comprise the most primitive materials that are able to be sampled. Although parent body alteration of such samples would not necessarily detract from scientists' interest in them, the possibility exists that ...
Mcsween, Harry Y., Jr.
core +1 more source
Recurrent planetesimal formation in an outer part of the early solar system
The formation of planets in our solar system encompassed various stages of accretion of planetesimals that formed in the protoplanetary disk within the first few million years at different distances to the sun.
Wladimir Neumann +3 more
doaj +1 more source

