D L Buczkowski
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Explore the profile of D L Buczkowski including associated specialties, affiliations and a list of published articles.
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Articles
9
Citations
63
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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.
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...
3.
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...
4.
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,...
5.
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...
6.
Marchi S, Ermakov A, Raymond C, Fu R, OBrien D, Bland M, et al.
Nat Commun
. 2016 Jul;
7:12257.
PMID: 27459197
Asteroids provide fundamental clues to the formation and evolution of planetesimals. Collisional models based on the depletion of the primordial main belt of asteroids predict 10-15 craters >400 km should...
7.
Nathues A, Hoffmann M, Schaefer M, Le Corre L, Reddy V, Platz T, et al.
Nature
. 2015 Dec;
528(7581):237-40.
PMID: 26659183
The dwarf planet (1) Ceres, the largest object in the main asteroid belt with a mean diameter of about 950 kilometres, is located at a mean distance from the Sun...
8.
Denevi B, Blewett D, Buczkowski D, Capaccioni F, Capria M, De Sanctis M, et al.
Science
. 2012 Sep;
338(6104):246-9.
PMID: 22997131
We investigated the origin of unusual pitted terrain on asteroid Vesta, revealed in images from the Dawn spacecraft. Pitted terrain is characterized by irregular rimless depressions found in and around...
9.
Jaumann R, Williams D, Buczkowski D, Yingst R, Preusker F, Hiesinger H, et al.
Science
. 2012 May;
336(6082):687-90.
PMID: 22582254
Vesta's surface is characterized by abundant impact craters, some with preserved ejecta blankets, large troughs extending around the equatorial region, enigmatic dark material, and widespread mass wasting, but as yet...