Search Results - "Pieters, C.M."
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The geology of the Kerwan quadrangle of dwarf planet Ceres: Investigating Ceres’ oldest, largest impact basin
Published in Icarus (New York, N.Y. 1962) (01-12-2018)“…•We produced a geologic map Ceres’ Kerwan quadrangle to determine regional geologic history.•Kerwan is the oldest, largest (∼284 km) undisputed impact crater…”
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Elemental composition and mineralogy of Vesta and Ceres: Distribution and origins of hydrogen-bearing species
Published in Icarus (New York, N.Y. 1962) (15-01-2019)“…•Surface elemental and mineral composition constrains origin of H-bearing species.•Physics-based smoothing enables direct comparison of elemental and mineral…”
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One Moon, Many Measurements 3: Spectral reflectance
Published in Icarus (New York, N.Y. 1962) (01-09-2013)“…•This is one of three companion papers entitled “One Moon, Many Measurements”.•Paper describes the features of the each instrument data aboard two lunar…”
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The unique geomorphology and physical properties of the Vestalia Terra plateau
Published in Icarus (New York, N.Y. 1962) (01-12-2014)“…•We produced a geologic map of the Av-9 Numisia quadrangle of asteroid Vesta.•Stratigraphic relationships show Vestalia Terra is one of Vesta’s oldest…”
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Geomorphology and structural geology of Saturnalia Fossae and adjacent structures in the northern hemisphere of Vesta
Published in Icarus (New York, N.Y. 1962) (01-12-2014)“…•A mapping study of a portion of the northern hemisphere of Vesta is presented.•Eight geomorphic units are classified, along with their relative age…”
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One Moon, many measurements 1: Radiance values
Published in Icarus (New York, N.Y. 1962) (01-09-2013)“…•Cross-calibration/validation succeeded for instruments on Kaguya and Chandrayaan-1.•Radiance values agree overall across spectral properties, but some…”
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Variations in surface adsorbed H2O on lunar soils and relevant minerals
Published in Icarus (New York, N.Y. 1962) (15-03-2024)“…Spectral variations due to the removal of surface adsorbed H2O at 3 and 6 μm in reflectance spectra on lunar soils and relevant minerals (olivine, pyroxene,…”
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Bright carbonate deposits as evidence of aqueous alteration on (1) Ceres
Published in Nature (London) (04-08-2016)“…High-resolution near-infrared observations of the Occator bright areas on the dwarf planet Ceres suggest that the bright material is mostly made up of…”
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Effects of varying environmental conditions on emissivity spectra of bulk lunar soils: Application to Diviner thermal infrared observations of the Moon
Published in Icarus (New York, N.Y. 1962) (01-02-2017)“…•Thermal infrared spectra of lunar soil samples are measured under varying conditions.•Emissivity spectra are most sensitive to atmospheric pressure and solar…”
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Pink Moon: The petrogenesis of pink spinel anorthosites and implications concerning Mg-suite magmatism
Published in Earth and planetary science letters (01-10-2014)“…NASA's Moon Mineralogy Mapper (M3) has identified and characterized a new lunar rock type termed pink spinel anorthosite (PSA) (Pieters et al., 2011)…”
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Distinctive space weathering on Vesta from regolith mixing processes
Published in Nature (London) (01-11-2012)“…Whereas space weathering of some airless bodies, such as the Moon, occurs through the accumulation on regolith of nanophase metallic particles, spectroscopic…”
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Mineralogical mapping of Coniraya quadrangle of the dwarf planet Ceres
Published in Icarus (New York, N.Y. 1962) (15-01-2019)“…•We present a method for thermal removal from Ceres spectra.•Most of the crater floors are devoid of volatiles due to the impact events.•Na-carbonates on…”
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Olivine in an unexpected location on Vesta’s surface
Published in Nature (London) (05-12-2013)“…Although olivine was expected to occur within the deep, south-pole basins of asteroid Vesta, which are thought to be excavated mantle rocks, spectral data from…”
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Geologic characteristics of the Luna 17/Lunokhod 1 and Chang'E-3/Yutu landing sites, Northwest Mare Imbrium of the Moon
Published in Planetary and space science (01-11-2015)“…We compared and assessed the results of measurements and observations by the Lunokhod 1 and Yutu rovers, both of which explored the northwestern part of Mare…”
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The unique geomorphology and structural geology of the Haulani crater of dwarf planet Ceres as revealed by geological mapping of equatorial quadrangle Ac-6 Haulani
Published in Icarus (New York, N.Y. 1962) (01-12-2018)“…The dwarf planet Ceres has been explored by NASA's Dawn spacecraft with the goal of characterizing its geology, mineralogy, topography, shape, and internal…”
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Geologic mapping of Vesta
Published in Planetary and space science (15-11-2014)“…We report on a preliminary global geologic map of Vesta, based on data from the Dawn spacecraft’s High-Altitude Mapping Orbit (HAMO) and informed by…”
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Mineralogical analysis of the Ac-H-6 Haulani quadrangle of the dwarf planet Ceres
Published in Icarus (New York, N.Y. 1962) (15-01-2019)“…•The most prominent surface feature in quadrangle Ac-H-6 is crater Haulani.•Negative visual to near-infrared spectral slopes are observed in crater…”
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Ammoniated phyllosilicates with a likely outer Solar System origin on Ceres
Published in Nature (London) (10-12-2015)“…Studies of the dwarf planet (1) Ceres using ground-based and orbiting telescopes have concluded that its closest meteoritic analogues are the volatile-rich CI…”
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Sublimation in bright spots on Ceres
Published in Nature (London) (10-12-2015)“…The dwarf planet (1) Ceres, the largest object in the main asteroid belt (1) with a mean diameter of about 950 kilometres, is located at a mean distance from…”
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Mineralogical analysis of the Oppia quadrangle of asteroid (4) Vesta: Evidence for occurrence of moderate-reflectance hydrated minerals
Published in Icarus (New York, N.Y. 1962) (01-10-2015)“…•The older northeastern part of Av-10 is dominated by howardite-like material.•The younger southwestern part (including Oppia) has a markedly eucritic…”
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