The Winchcombe meteorite, a unique and pristine witness from the outer solar system
Average rating
Cast your vote
You can rate an item by clicking the amount of stars they wish to award to
this item.
When enough users have cast their vote on this item, the average rating will also be shown.
Star rating
Your vote was cast
Thank you for your feedback
Thank you for your feedback
Authors
King, Ashley JDaly, Luke
Rowe, James
Joy, Katherine H
Greenwood, Richard C
Devillepoix, Hadrien AR
Suttle, Martin D
Chan, Queenie HS
Russell, Sara
Bates, Helena C
Bryson, James FJ
Clay, Patricia L
Vida, Denis
Lee, Martin R
O’Brien, Áine
Hallis, Lydia J
Stephen, Natasha R
Tartèse, Romain
Sansom, Eleanor K
Towner, Martin C
Cupak, Martin
Shober, Patrick M
Bland, Phil A
Findlay, Ross
Franchi, Ian A
Verchovsky, Alexander B
Abernethy, Feargus AJ
Grady, Monica M
Floyd, Cameron J
van Ginneken, Matthias
Bridges, John
Hicks, Leon J
Jones, Rhian H
Mitchell, Jennifer T
Genge, Matthew J
Jenkins, Laura
Martin, Pierre-Etienne
Sephton, Mark A
Watson, Jonathan S
Salge, T
Shirley, Katherine A
Curtis, Rowan J
Warren, Tristram J
Bowles, Neil E
Stuart, Finlay M
Di Nicola, Luigia
Györe, Domokos
Boyce, Adrian J
Shaw, Kathryn MM
Elliott, Tim
Steele, Robert CJ
Povinec, Pavel
Laubenstein, Matthias
Sanderson, David
Cresswell, Alan
Jull, Anthony JT
Sýkora, Ivan
Sridhar, Sanjana
Harrison, Richard J
Willcocks, Francesca M
Harrison, Catherine S
Hallatt, Daniel
Wozniakiewicz, Penny J
Burchell, Mark J
Alesbrook, Luke S
Dignam, Aishling
Almeida, Natasha V
Smith, Caroline L
Clark, Brett
Humphreys-Williams, Emma R
Schofield, Paul F
Cornwell, Luke T
Spathis, Vassilia
Morgan, Geraint H
Perkins, Mark J
Kacerek, Richard
Campbell-Burns, Peter
Colas, Francois
Zanda, Brigitte
Vernazza, Pierre
Bouley, Sylvain
Jeanne, Simon
Hankey, Mike
Collins, Gareth S
Young, John S
Shaw, Clive
Horak, Jana
Jones, Dave
James, Nick
Bosley, Steve
Shuttleworth, Alan
Dickinson, Paul
McMullan, Ian
Robson, Derek
Smedley, Andrew RD
Stanley, Ben
Bassom, Richard
McIntyre, Mark
Suttle, Adam A
Fleet, Richard
Bastiaens, Luc
Ihász, Míra B
McMullan, Sarah
Boazman, Sarah J
Dickeson, Zach I
Grindrod, Peter M
Pickersgill, Annemarie E
Weir, Colin J
Suttle, Fiona M
Farrelly, Sarah
Spencer, Ieun
Naqvi, Sheeraz
Mayne, Ben
Skilton, Dan
Kirk, Dan
Mounsey, Ann
Mounsey, Sally E
Mounsey, Sarah
Godfrey, Pamela
Bond, Lachlan
Bond, Victoria
Wilcock, Cathryn
Wilcock, Hannah
Wilcock, Rob
Issue date
2022-11-16Submitted date
2022-10-20
Metadata
Show full item recordAbstract
Direct links between carbonaceous chondrites and their parent bodies in the solar system are rare. The Winchcombe meteorite is the most accurately recorded carbonaceous chondrite fall. Its pre-atmospheric orbit and cosmic-ray exposure age confirm that it arrived on Earth shortly after ejection from a primitive asteroid. Recovered only hours after falling, the composition of the Winchcombe meteorite is largely unmodified by the terrestrial environment. It contains abundant hydrated silicates formed during fluid-rock reactions, and carbon- and nitrogen-bearing organic matter including soluble protein amino acids. The near-pristine hydrogen isotopic composition of the Winchcombe meteorite is comparable to the terrestrial hydrosphere, providing further evidence that volatile-rich carbonaceous asteroids played an important role in the origin of Earth’s water.Citation
Ashley J. King et al. ,The Winchcombe meteorite, a unique and pristine witness from the outer solar system. Sci. Adv.8,eabq3925(2022).DOI:10.1126/sciadv.abq3925Journal
Science AdvancesType
Journal ArticleItem Description
Copyright © 2022 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution License 4.0 (CC BY). The linked file is the published version of the article.NHM Repository
ISSN
2375-2548EISSN
2375-2548ae974a485f413a2113503eed53cd6c53
10.1126/sciadv.abq3925
Scopus Count
Collections
Related items
Showing items related by title, author, creator and subject.
-
Brecciation at the grain scale within the lithologies of the Winchcombe Mighei‐like carbonaceous chondriteDaly, Luke; Suttle, Martin D; Lee, Martin R; Bridges, John; Hicks, Leon; Martin, Pierre‐Etienne MC; Floyd, Cameron J; Jenkins, Laura E; Salge, T; King, Ashley J; et al. (Wiley, 2024-05-10)Abstract: The Mighei‐like carbonaceous (CM) chondrites have been altered to various extents by water–rock reactions on their parent asteroid(s). This aqueous processing has destroyed much of the primary mineralogy of these meteorites, and the degree of alteration is highly heterogeneous at both the macroscale and nanoscale. Many CM meteorites are also heavily brecciated juxtaposing clasts with different alteration histories. Here we present results from the fine‐grained team consortium study of the Winchcombe meteorite, a recent CM chondrite fall that is a breccia and contains eight discrete lithologies that span a range of petrologic subtypes (CM2.0–2.6) that are suspended in a cataclastic matrix. Coordinated multitechnique, multiscale analyses of this breccia reveal substantial heterogeneity in the extent of alteration, even in highly aqueously processed lithologies. Some lithologies exhibit the full range and can comprise nearly unaltered coarse‐grained primary components that are found directly alongside other coarse‐grained components that have experienced complete pseudomorphic replacement by secondary minerals. The preservation of the complete alteration sequence and pseudomorph textures showing tochilinite–cronstedtite intergrowths are replacing carbonates suggest that CMs may be initially more carbonate rich than previously thought. This heterogeneity in aqueous alteration extent is likely due to a combination of microscale variability in permeability and water/rock ratio generating local microenvironments as has been established previously. Nevertheless, some of the disequilibrium mineral assemblages observed, such as hydrous minerals juxtaposed with surviving phases that are typically more fluid susceptible, can only be reconciled by multiple generations of alteration, disruption, and reaccretion of the CM parent body at the grain scale.
-
A global phylogeny of butterflies reveals their evolutionary history, ancestral hosts and biogeographic originsKawahara, Akito Y; Storer, Caroline; Carvalho, Ana Paula S; Plotkin, David M; Condamine, Fabien L; Braga, Mariana P; Ellis, Emily A; St Laurent, Ryan A; Li, Xuankun; Barve, Vijay; et al. (Springer Science and Business Media LLC, 2023-05-15)Abstract: Butterflies are a diverse and charismatic insect group that are thought to have evolved with plants and dispersed throughout the world in response to key geological events. However, these hypotheses have not been extensively tested because a comprehensive phylogenetic framework and datasets for butterfly larval hosts and global distributions are lacking. We sequenced 391 genes from nearly 2,300 butterfly species, sampled from 90 countries and 28 specimen collections, to reconstruct a new phylogenomic tree of butterflies representing 92% of all genera. Our phylogeny has strong support for nearly all nodes and demonstrates that at least 36 butterfly tribes require reclassification. Divergence time analyses imply an origin ~100 million years ago for butterflies and indicate that all but one family were present before the K/Pg extinction event. We aggregated larval host datasets and global distribution records and found that butterflies are likely to have first fed on Fabaceae and originated in what is now the Americas. Soon after the Cretaceous Thermal Maximum, butterflies crossed Beringia and diversified in the Palaeotropics. Our results also reveal that most butterfly species are specialists that feed on only one larval host plant family. However, generalist butterflies that consume two or more plant families usually feed on closely related plants.
-
Calathus: A sample-return mission to CeresGassot, Oriane; Panicucci, Paolo; Acciarini, Giacomo; Bates, HC; Caballero, Manel; Cambianica, Pamela; Dziewiecki, Maciej; Dionnet, Zelia; Enengl, Florine; Gerig, Selina-Barbara; et al. (Elsevier BV, 12/01/2021)Ceres, as revealed by NASA's Dawn spacecraft, is an ancient, crater-saturated body dominated by low-albedo clays. Yet, localised sites display a bright, carbonate mineralogy that may be as young as 2 Myr. The largest of these bright regions (faculae) are found in the 92 km Occator Crater, and would have formed by the eruption of alkaline brines from a subsurface reservoir of fluids. The internal structure and surface chemistry suggest that Ceres is an extant host for a number of the known prerequisites for terrestrial biota, and as such, represents an accessible insight into a potentially habitable “ocean world”. In this paper, the case and the means for a return mission to Ceres are outlined, presenting the Calathus mission to return to Earth a sample of the Occator Crater faculae for high-precision laboratory analyses. Calathus consists of an orbiter and a lander with an ascent module: the orbiter is equipped with a high-resolution camera, a thermal imager, and a radar; the lander contains a sampling arm, a camera, and an on-board gas chromatograph mass spectrometer; and the ascent module contains vessels for four cerean samples, collectively amounting to a maximum 40 g. Upon return to Earth, the samples would be characterised via high-precision analyses to understand the salt and organic composition of the Occator faculae, and from there to assess both the habitability and the evolution of a relict ocean world from the dawn of the Solar System.