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相关论文: Statistical Tests of Chondrule Sorting

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Chondritic meteorites provide valuable opportunities to investigate the origins of the solar system. We explore impact jetting as a mechanism of chondrule formation and subsequent pebble accretion as a mechanism of accreting chondrules onto…

地球与行星天体物理 · 物理学 2016-03-23 Yasuhiro Hasegawa , Neal J. Turner , Joseph Masiero , Shigeru Wakita , Yuji Matsumoto , Shoichi Oshino

In recent years many models of chondrule formation have been proposed. One of those models is the processing of dust in shock waves in protoplanetary disks. In this model, the dust and the chondrule precursors are overrun by shock waves,…

地球与行星天体物理 · 物理学 2014-08-21 Sebastian M. Stammler , Cornelis P. Dullemond

We consider the size distribution of superbubbles in a star forming galaxy. Previous studies have tried to explain the distribution by using adiabatic self-similar evolution of wind driven bubbles, assuming that bubbles stall when pressure…

星系天体物理 · 物理学 2020-04-23 Biman B Nath , Pushpita Das , M. S. Oey

Chondrules are primitive materials in the Solar System. They are formed in the first about 3 Myr of the Solar System's history. This timescale is longer than that of Mars formation, and it is conceivable that protoplanets, planetesimals and…

地球与行星天体物理 · 物理学 2017-03-15 Yuji Matsumoto , Shoichi Oshino , Yasuhiro Hasegawa , Shigeru Wakita

An intriguing aspect of chondritic meteorites is that they are complementary: while their separate components have wildly varying abundances, bulk chondrites have nearly solar composition. This implies that the nearly-solar reservoirs in…

地球与行星天体物理 · 物理学 2016-05-25 Alexander Hubbard

Cell sorting, the segregation of cells with different properties into distinct domains, is a key phenomenon in biological processes such as embryogenesis. We use a phase-field model of a confluent cell layer to study the role of activity in…

生物物理 · 物理学 2024-03-05 James N. Graham , Guanming Zhang , Julia M. Yeomans

Major components of chondrites are chondrules and matrix. Measurements of the volatile abundance in Semarkona chondrules suggest that chondrules formed in a dense clump that had a higher solid density than the gas density in the solar…

地球与行星天体物理 · 物理学 2020-01-08 Yuji Matsumoto , Shigeru Wakita , Yasuhiro Hasegawa , Shoichi Oshino

We study a two-species bidirectional exclusion process, and a single species variant, which is motivated by the motion of organelles and vesicles along microtubules. Specifically, we are interested in the clustering of the particles and…

统计力学 · 物理学 2020-03-17 Jim Chacko , Sudipto Muhuri , Goutam Tripathy

Chondrules are considered to have much information on dust particles and processes in the solar nebula. It is naturally expected that protoplanetary disks observed in present star forming regions have similar dust particles and processes,…

天体物理学 · 物理学 2010-11-11 Hitoshi Miura , Taishi Nakamoto

The proper sorting of membrane components by regulated exchange between cellular organelles is crucial to intra-cellular organisation. This process relies on the budding and fusion of transport vesicles, and should be strongly influenced by…

生物物理 · 物理学 2018-02-07 Quentin Vagne , Pierre Sens

The effect of turbulence on snow precipitation is not incorporated into present weather forecasting models. Here we show evidence that turbulence is in fact a key influence on both fall speed and spatial distribution of settling snow. We…

流体动力学 · 物理学 2021-02-24 Cheng Li , Kaeul Lim , Tim Berk , Aliza Abraham , Michael Heisel , Michele Guala , Filippo Coletti , Jiarong Hong

We assess whether chondrules, once-molten mm-sized spheres filling the oldest meteorites, could have formed from super-km/s collisions between planetesimals in the solar nebula. High-velocity collisions release hot and dense clouds of…

地球与行星天体物理 · 物理学 2021-03-30 Nick Choksi , Eugene Chiang , Harold C. Connolly , Zack Gainsforth , Andrew J. Westphal

Chondrules are spherical or subspherical particles of crystallized or partially crystallized liquid silicates that constitute large-volume fractions of most chondritic meteorites. Chondrules typically range $0.1-2\,$mm in size and…

地球与行星天体物理 · 物理学 2025-11-25 Sin-iti Sirono , Diego Turrini

Reliably predicting the geomorphology and climate of planetary bodies requires knowledge of the dynamic threshold wind shear velocity below which saltation transport ceases. Here we measure this threshold in a wind tunnel for four…

地球物理 · 物理学 2019-10-28 Wei Zhu , Xinghui Huo , Jie Zhang , Peng Wang , Thomas Pähtz , Ning Huang , Zhiguo He

The lifetime of mm size dust grains, such as chondrules, in the nominal solar nebula model is limited to $\sim 10^{5}$ yr due to an inward drift driven by gas drag. However, isotopic and petrological studies on primitive meteorites indicate…

地球与行星天体物理 · 物理学 2024-01-08 Tetsuo Taki , Shigeru Wakita

A statistical description of heavy particles suspended in incompressible rough self-similar flows is developed. It is shown that, differently from smooth flows, particles do not form fractal clusters. They rather distribute inhomogeneously…

混沌动力学 · 物理学 2007-05-23 J. Bec , M. Cencini , R. Hillerbrand

Systematic abundance differences that depend on the condensation temperatures of elements have been observed, in particular for stars similar to the Sun; solar twins and solar analogs. Similar differences have also recently been shown to…

地球与行星天体物理 · 物理学 2025-06-13 Åke Nordlund

Following recent evidence that the vortices in decaying two-dimensional turbulence can be classified into small--mobile, and large--quasi-stationary, this paper examines the evidence that the latter might be considered a `crystal' whose…

流体动力学 · 物理学 2021-08-04 Javier Jiménez

Spontaneous segregation of run-and-tumble particles with different velocities in microchannels is investigated by numerical simulations. Self-propelled particles are known to accumulate in the proximity of walls. Here we show how fast…

软凝聚态物质 · 物理学 2014-09-05 Andrea Costanzo , Jens Elgeti , Thorsten Auth , Gerhard Gompper , Marisol Ripoll

In this paper, the possibility that the moderately volatile element depletions observed in chondritic meteorites are the results of planetesimals accreting in a solar nebula that cooled from an initially hot state (temperatures > 1350 K out…

天体物理学 · 物理学 2015-06-24 Fred J. Ciesla