Results 81 to 90 of about 4,638 (257)
Abstract Enstatite chondrites formed under extremely reducing conditions in the protoplanetary disk. They are derived from two or more parent bodies, EH and EL, and both EH and EL groups contain petrologic type 3–6 samples. The rare lithophile‐ and halogen‐bearing sulfide, djerfisherite, occurs in low abundance in enstatite chondrites, most frequently ...
Peter Mc Ardle +9 more
wiley +1 more source
Boulders on Bennu: Low Apparent Thermal Inertia Caused by Thermal Fatigue Fractures
Abstract Boulders covering the surfaces of asteroids Bennu and Ryugu have apparent thermal inertias substantially lower than their meteorite analogs. This has led to the inference that boulders on Bennu may be unlike any known meteorite. However, samples returned from Ryugu have a thermal inertia 3.5 times higher than the apparent thermal inertia ...
Catherine M. Elder
wiley +1 more source
We present in this study the effects of short-term heating on organics in the Tagish Lake meteorite and how the difference in the heating conditions can modify the organic matter (OM) in a way that complicates the interpretation of a parent body’s ...
,, ,, Chan, Queenie H. S., Nakato, Aiko
core +1 more source
Petrography of phosphates in CI and CY carbonaceous chondrites
Abstract Phosphate minerals are significant carriers of volatiles (e.g., OH) and halogens in chondritic material; however, their origin in most groups of carbonaceous chondrites remains poorly characterized. We have determined the abundance, morphology, texture, and composition of phosphate grains in aqueously altered CI chondrites and in hydrated and ...
C. S. Harrison +3 more
wiley +1 more source
Structural and compositional changes of constituents in Murchison CM chondrite by He+ ion irradiation [PDF]
第8回極域科学シンポジウム/個別セッション:[OA] 南極隕石12月6日(水)国語研究所 2階講堂The Eighth Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteoritesWed.
core +1 more source
Regolith behavior under asteroid-level gravity conditions: low-velocity impact experiments
The dusty regolith covering the surfaces of asteroids and planetary satellites differs in size, shape, and composition from terrestrial soil particles and is subject to very different environmental conditions.
Abukhalil, Sumayya +5 more
core +1 more source
Special issue “Science of solar system materials examined from Hayabusa and future missions (II)” [PDF]
Six years have passed since the first asteroid sample was returned from the S-type near-Earth asteroid 25143 Itokawa by the JAXA’s Hayabusa mission in 2010 (Yada et al. 2014). Considerable progress has been made in the study of surface regolith materials
Binzel, Richard P +5 more
core +3 more sources
Transmission electron microscopy analyses of Hayabusa2 samples show that Ryugu organic matter exhibits a range of morphologies, elemental compositions, and carbon functional chemistries consistent with those of carbonaceous chondrites that have ...
Rhonda M. Stroud +112 more
semanticscholar +1 more source
Multi-scale science from orbiter, lander, and sample-return by Hayabusa2 [PDF]
第7回極域科学シンポジウム:[OA] 南極隕石/はやぶさ11月29日(火)国立国語研究所 ...
core +1 more source

