Chondrule formation by collisions of planetesimals containing volatiles triggered by Jupiter’s formation [PDF]
Chondrules are spherical or subspherical particles of crystallized or partially crystallized liquid silicates that constitute large-volume fractions of most chondritic meteorites.
Sin-iti Sirono, Diego Turrini
doaj +4 more sources
How to form planetesimals from mm-sized chondrules and chondrule aggregates [PDF]
The size distribution of asteroids and Kuiper belt objects in the solar system is difficult to reconcile with a bottom-up formation scenario due to the observed scarcity of objects smaller than $\sim$100 km in size.
Daniel Carrera +2 more
core +5 more sources
Chondrule-like objects and Ca-Al-rich inclusions in Ryugu may potentially be the oldest Solar System materials [PDF]
Chondrule-like objects and CAIs in the Ryugu samples are early generations of chondrules and possibly oldest solids in the Solar System. They were transported from the inner solar nebula to the formation location of the Ryugu original parent body.
Daisuke Nakashima +32 more
doaj +2 more sources
Bubbles to Chondrites-I. Evaporation and condensation experiments, and formation of chondrules [PDF]
We propose a simple model of chondrule formation that is supported by our new experiments. With a laser-heating and inert-gas-cooling technique, we obtained evaporation and condensation pathways starting with chondritic compositions till ends, and ...
Yuki Nakano, Akihiko Hashimoto
doaj +2 more sources
Trace element geochemistry of ordinary chondrite chondrules: The type I/type II chondrule dichotomy [PDF]
We report trace element concentrations of silicate phases in chondrules from LL3 ordinary chondrites Bishunpur and Semarkona. Results are similar to previously reported data for carbonaceous chondrites, with rare earth element (REE) concentrations ...
Emmanuel Jacquet +2 more
openalex +5 more sources
Photophoretic Strength on Chondrules. 2. Experiment [PDF]
Photophoretic motion can transport illuminated particles in protoplanetary disks. In a previous paper we focused on the modeling of steady state photophoretic forces based on the compositions derived from tomography and heat transfer.
Bischoff, Addi +5 more
core +4 more sources
Abundant microchondrules in 162173 Ryugu suggest a turbulent origin for primitive asteroids [PDF]
Chondrules are a characteristic feature of primitive Solar System materials and are common in all primitive meteorites except the CI-chondrites. They are thought to form owing to melting of solid dust aggregates by energetic processing within the solar ...
Matthew J. Genge +7 more
doaj +2 more sources
Chondrule Survivability in the Solar Nebula [PDF]
The lifetime of millimeter-sized dust grains, such as chondrules, in the nominal solar nebula model is limited to ∼10 ^5 yr, due to an inward drift driven by gas drag.
Tetsuo Taki, Shigeru Wakita
doaj +2 more sources
Chondrule Dust Rim Growth: Influence of Restructuring Using Molecular Dynamics Simulations [PDF]
We investigate the influence of disruptive collisions on chondrule rim growth, emphasizing the role of kinetic energy in determining the outcomes of these interactions.
Chuchu Xiang +4 more
doaj +2 more sources
THE Formation of chondrule-like particles in RF discharge plasma
Chondrules are fundamental components of chondritic meteorites and play a vital role in understanding the formation of the early solar system. This study focuses on the synthesis of chondrule-like particles in a plasma environment using a radiofrequency
Assan Abdirakhmanov +8 more
doaj +1 more source

