About: Mercury and other iron-rich planetary bodies as relics of inefficient accretion

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rdf:type	Item
description	wetenschappelijk artikel (nl) наукова стаття, опублікована в липні 2014 (uk) article scientifique publié en 2014 (fr) im Juli 2014 veröffentlichter wissenschaftlicher Artikel (de)
publication date	wds:Q56082920-3F0601B0-396C-4FC2-9732-D9D9B1A9339E
publication date	2014-07-06 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q56082920-825CDFE1-E81A-46F1-A292-77996AB3E86F
language of work or name	English
exact match	wds:Q56082920-B118BC27-0384-48BE-80F3-B6840A020ECC
exact match	https://scigraph.springernature.com/pub.10.1038/ngeo2189
cites work	wds:Q56082920-0DC331C6-B7EB-469F-9185-B3DD06C84A74 wds:Q56082920-1646F72F-FD1B-46CA-B833-7FBB930D082B wds:Q56082920-22469E37-E4E0-4A07-AD9D-FFF116E0CEFF wds:Q56082920-3C114CCF-7975-464F-AB3C-7AE670C1F2C1 wds:Q56082920-4553F5AE-9BF0-4F3B-988D-A291680D473F wds:Q56082920-5952D102-36D3-4718-B7DF-0AF3A0FDD1B8 wds:Q56082920-7A361F5F-9778-4DD0-91DB-AEDCDBE74987 wds:Q56082920-8AE3560D-1E96-43CC-B1CB-5193008C6B1D wds:Q56082920-B039A20C-9EE3-4F83-948F-B8F381ADC7BB wds:Q56082920-D501E880-E84A-4439-B93B-0180622A9B67 wds:Q56082920-D8021F6B-F179-491E-8ADC-CEFCF639474B wds:Q56082920-D93D370D-8069-45E7-B064-FFFCBC59E602 wds:Q56082920-DAEF58A8-9E11-4871-B60B-E7FF025783BE wds:Q56082920-EA340131-968D-4C3A-BBE9-614D80E5C884 wds:Q56082920-F339A945-A1BA-43AC-A71E-BBB3C7B874B0
cites work	Formation of the Terrestrial Planets Iron meteorites as remnants of planetesimals formed in the terrestrial planet region A hit-and-run giant impact scenario Early core formation in asteroids and late accretion of chondrite parent bodies: Evidence from 182Hf-182W in CAIs, metal-rich chondrites, and iron meteorites Dynamics of Lunar Formation Accretion efficiency during planetary collisions Iron meteorite evidence for early formation and catastrophic disruption of protoplanets. Late-stage planetary accretion including hit-and-run collisions and fragmentation Hit-and-run planetary collisions Collisional stripping of Mercury's mantle Collisions between gravity-dominated bodies. II. The diversity of impact outcomes during the end stage of planet formation Asteroids were born big Radioactive elements on Mercury's surface from MESSENGER: implications for the planet's formation and evolution The curious case of Mercury's internal structure Size of the group IVA iron meteorite core: Constraints from the age and composition of Muonionalusta
author name string	wds:Q56082920-879ECA20-B4F0-4505-9B6F-12B7DE783E08 wds:Q56082920-EDA5C107-C935-4FB1-ADBC-9AB67EE6D901
author name string	A. Reufer E. Asphaug
rdfs:label	Mercury and other iron-rich planetary bodies as relics of inefficient accretion (en) Mercury and other iron-rich planetary bodies as relics of inefficient accretion (nl)
skos:prefLabel	Mercury and other iron-rich planetary bodies as relics of inefficient accretion (en) Mercury and other iron-rich planetary bodies as relics of inefficient accretion (nl)
name	Mercury and other iron-rich planetary bodies as relics of inefficient accretion (en) Mercury and other iron-rich planetary bodies as relics of inefficient accretion (nl)
title	wds:Q56082920-C8C25611-2466-4F1B-8E70-79B11927E215
title	Mercury and other iron-rich planetary bodies as relics of inefficient accretion (en)
page(s)	wds:Q56082920-218FE903-E110-4BDB-95D2-665F02880330
page(s)	564-568
instance of	wds:Q56082920-BE9F53DE-4993-4020-97B9-397081B0ED71
instance of	scholarly article
published in	wds:Q56082920-AAF5BB6B-113F-47AE-A000-4480D9332428
published in	Nature Geoscience
issue	wds:Q56082920-E823C2E4-3E7F-4EF4-BE7D-5017E928B534
volume	wds:Q56082920-BB22CF27-62BA-43B3-8D89-58735CD95B83
issue	8
volume	7
DOI	wds:Q56082920-D22A1B86-771C-4E42-A159-6034572F60B9
DOI	http://dx.doi.org/10.1038/NGEO2189
DOI	10.1038/NGEO2189
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q56082920
is cites work of	Refining the Transit-timing and Photometric Analysis of TRAPPIST-1: Masses, Radii, Densities, Dynamics, and Ephemerides Percolative core formation in planetesimals enabled by hysteresis in metal connectivity Did Jupiter's core form in the innermost parts of the Sun's protoplanetary disc?
is cites work of	wds:Q56674476-3030CD1E-49E5-4034-BBB5-C711E1C121DB wds:Q110248235-820C33F4-F991-4C07-A625-02F28791D281 wds:Q46300258-B74C34EA-41AE-4AB3-9935-0C4D3537A5F5

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