C A Raymond
Overview
Explore the profile of C A Raymond including associated specialties, affiliations and a list of published articles.
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Articles
115
Citations
258
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Recent Articles
1.
Scully J, Schenk P, Castillo-Rogez J, Buczkowski D, Williams D, Pasckert J, et al.
Nat Commun
. 2020 Aug;
11(1):3680.
PMID: 32778642
Before acquiring highest-resolution data of Ceres, questions remained about the emplacement mechanism and source of Occator crater's bright faculae. Here we report that brine effusion emplaced the faculae in a...
2.
Duarte K, Schmidt B, Chilton H, Hughson K, Sizemore H, Ferrier K, et al.
J Geophys Res Planets
. 2020 May;
124(12):3329-3343.
PMID: 32355585
Landslides are among the most widespread geologic features on Ceres. Using data from Dawn's Framing Camera, landslides were previously classified based upon geomorphologic characteristics into one of three archetypal categories,...
3.
Sizemore H, Platz T, Schorghofer N, Prettyman T, De Sanctis M, Crown D, et al.
Geophys Res Lett
. 2017 Oct;
44(13):6570-6578.
PMID: 28989206
Prior to the arrival of the Dawn spacecraft at Ceres, the dwarf planet was anticipated to be ice-rich. Searches for morphological features related to ice have been ongoing during Dawn's...
4.
De Sanctis M, Ammannito E, McSween H, Raponi A, Marchi S, Capaccioni F, et al.
Science
. 2017 Feb;
355(6326):719-722.
PMID: 28209893
Organic compounds occur in some chondritic meteorites, and their signatures on solar system bodies have been sought for decades. Spectral signatures of organics have not been unambiguously identified on the...
5.
Prettyman T, Yamashita N, Toplis M, McSween H, Schorghofer N, Marchi S, et al.
Science
. 2016 Dec;
355(6320):55-59.
PMID: 27980087
The surface elemental composition of dwarf planet Ceres constrains its regolith ice content, aqueous alteration processes, and interior evolution. Using nuclear spectroscopy data acquired by NASA's Dawn mission, we determined...
6.
Russell C, Raymond C, Ammannito E, Buczkowski D, De Sanctis M, Hiesinger H, et al.
Science
. 2016 Oct;
353(6303):1008-1010.
PMID: 27701107
On 6 March 2015, Dawn arrived at Ceres to find a dark, desiccated surface punctuated by small, bright areas. Parts of Ceres' surface are heavily cratered, but the largest expected...
7.
Hiesinger H, Marchi S, Schmedemann N, Schenk P, Pasckert J, Neesemann A, et al.
Science
. 2016 Oct;
353(6303).
PMID: 27701089
Thermochemical models have predicted that Ceres, is to some extent, differentiated and should have an icy crust with few or no impact craters. We present observations by the Dawn spacecraft...
8.
Buczkowski D, Schmidt B, Williams D, Mest S, Scully J, Ermakov A, et al.
Science
. 2016 Oct;
353(6303).
PMID: 27701088
Analysis of Dawn spacecraft Framing Camera image data allows evaluation of the topography and geomorphology of features on the surface of Ceres. The dwarf planet is dominated by numerous craters,...
9.
Ruesch O, Platz T, Schenk P, McFadden L, Castillo-Rogez J, Quick L, et al.
Science
. 2016 Oct;
353(6303).
PMID: 27701087
Volcanic edifices are abundant on rocky bodies of the inner solar system. In the cold outer solar system, volcanism can occur on solid bodies with a water-ice shell, but derived...
10.
Ammannito E, DeSanctis M, Ciarniello M, Frigeri A, Carrozzo F, Combe J, et al.
Science
. 2016 Oct;
353(6303).
PMID: 27701086
The dwarf planet Ceres is known to host phyllosilicate minerals at its surface, but their distribution and origin have not previously been determined. We used the spectrometer onboard the Dawn...