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典型文献
Early planetary processes and light elements in iron-dominated cores
文献摘要:
This paper discusses the latest research on the accretion and differentiation of terrestrial planets and multidisciplinary constraints on light elements in iron-dominated metallic cores.The classic four-stage model of terrestrial planet formation advocates slow and local accretion.Meanwhile,the pebble accretion model suggests fast accretion for planets,while the Grand Tack model provides heterogeneous accretion mechanisms.Terrestrial planets and small interstellar bodies may have experienced at least some degree of partial melting due to the three primary energy sources(i.e.,the decay of short-lived radioactive nuclides,the kinetic energy delivered by impacts,and the conversion of gravitational potential energy).Together with metal-silicate separation mecha-nisms,the magma ocean theory depicts the pattern of core formation in terrestrial planets.Several hypotheses have been proposed to explain the concentration of siderophile elements in the mantle,including the single-stage,contin-uous,and multistage core formation models,and the late-veneer model.Some light elements have been postulated in the core to account for Earth's outer core density deficit.A plethora of constraints on the species and concentration of light elements have been put forward from the perspectives of cosmochemical and geochemical fingerprints,geophys-ical observations,mineral physics,numerical modeling,and theoretical prediction.Si and O may be the two leading candidates for Earth's outer core light elements;however,it still remains an open question.S is another potential light element in Earth's core,most likely with less than 2 wt%.Other light elements including H and C,may not exceed 1 wt%in the core.Moreover,the accretion and differen-tiation history would provide some clues to light elements in other terrestrial planetary cores.In principle,a larger heliocentric distance corresponds to accretion from more oxidized materials,leading to a higher S concentration in the Martian core.On the contrary,Mercury is close to the Sun and has accreted from more reduced materials,resulting in more Si in the core.
文献关键词:
作者姓名:
Chaojia Lv;Jin Liu
作者机构:
Center for High Pressure Science and Technology Advanced Research,Beijing 100094,China;CAS Center for Excellence in Deep Earth Science,Guangzhou 510640,China
引用格式:
[1]Chaojia Lv;Jin Liu-.Early planetary processes and light elements in iron-dominated cores)[J].地球化学学报(英文版),2022(04):625-649
A类:
Tack,siderophile,veneer,cosmochemical,geophys
B类:
Early,planetary,processes,light,elements,iron,dominated,cores,This,paper,discusses,latest,research,accretion,differentiation,terrestrial,planets,multidisciplinary,constraints,metallic,classic,four,formation,advocates,slow,local,Meanwhile,pebble,suggests,fast,Grand,provides,heterogeneous,mechanisms,Terrestrial,small,interstellar,bodies,may,have,experienced,least,some,degree,partial,melting,due,three,primary,energy,sources,decay,short,lived,radioactive,nuclides,kinetic,delivered,by,impacts,conversion,gravitational,potential,Together,silicate,separation,magma,ocean,theory,depicts,pattern,Several,hypotheses,been,proposed,explain,concentration,mantle,including,single,contin,uous,multistage,models,Some,postulated,account,Earth,outer,density,deficit,plethora,species,put,forward,from,perspectives,geochemical,fingerprints,observations,mineral,physics,numerical,modeling,theoretical,prediction,Si,two,leading,candidates,however,still,remains,open,question,another,most,likely,less,than,wt,Other,exceed,Moreover,history,would,clues,In,principle,larger,heliocentric,distance,corresponds,more,oxidized,materials,higher,Martian,On,contrary,Mercury,close,Sun,has,accreted,reduced,resulting
AB值:
0.538448
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