Studying the composition and mineralogy of the Hermean surface with the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) for the BepiColombo …
Abstract Launched onboard the BepiColombo Mercury Planetary Orbiter (MPO) in October
2018, the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) is on its way to …
2018, the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) is on its way to …
Rationale for BepiColombo studies of Mercury's surface and composition
DA Rothery, M Massironi, G Alemanno, O Barraud… - Space science …, 2020 - Springer
BepiColombo has a larger and in many ways more capable suite of instruments relevant for
determination of the topographic, physical, chemical and mineralogical properties of …
determination of the topographic, physical, chemical and mineralogical properties of …
Deriving iron contents from past and future Venus surface spectra with new high-temperature laboratory emissivity data
J Helbert, A Maturilli, MD Dyar, G Alemanno - Science Advances, 2021 - science.org
In situ information on the surface composition of Venus is based on measurements of a
small number of landing sites. In the laboratory, we measured the emissivity of a range of …
small number of landing sites. In the laboratory, we measured the emissivity of a range of …
Thermal expansion of oldhamite, CaS: implication for the surface of Mercury
The temperature excursion variation of Mercury's surface may significantly change crystal
structure of surface-comprising minerals. The thermal stability of oldhamite (CaS) was …
structure of surface-comprising minerals. The thermal stability of oldhamite (CaS) was …
Laboratory Emissivity Spectra of Sulphide-Bearing Samples, New Constraints for the Surface of Mercury: Oldhamite in Mafic Aggregates
C Carli, S Ferrari, A Maturilli, G Serventi, M Sgavetti… - Minerals, 2024 - mdpi.com
Exploration of Mercury will continue in the near future with ESA/JAXA's BepiColombo
mission, which will increase the number and the type of datasets, and it will take advantage …
mission, which will increase the number and the type of datasets, and it will take advantage …
High temperature spectral emissivity of glass and crystal-bearing basalts
Temperature is a key parameter controlling the rheology of lava flows. However, the
unpredictable hazard of eruptions prevents direct measurements of hot volcanic bodies …
unpredictable hazard of eruptions prevents direct measurements of hot volcanic bodies …
Volume thermal expansion along the jadeite–diopside join
F Pandolfo, F Cámara, MC Domeneghetti… - Physics and Chemistry …, 2015 - Springer
An in situ single-crystal high-temperature X-ray diffraction study was performed on
clinopyroxene crystals along the jadeite,(NaAlSi 2 O 6 Jd)–diopside (CaMgSi 2 O 6 Di) join …
clinopyroxene crystals along the jadeite,(NaAlSi 2 O 6 Jd)–diopside (CaMgSi 2 O 6 Di) join …
Thermal infrared emissivity of felsic-rich to mafic-rich analogues of hot planetary regoliths
Abstract Inner Solar System bodies with absent or extremely tenuous atmospheres such as
Mercury and several high-eccentricity Near Earth Objects (NEOs) are subject to a wide …
Mercury and several high-eccentricity Near Earth Objects (NEOs) are subject to a wide …
A new calibration to determine the closure temperatures of Fe‐Mg ordering in augite from nakhlites
M Alvaro, MC Domeneghetti, AM Fioretti… - … & Planetary Science, 2015 - Wiley Online Library
Recently it has been shown that the relatively low closure temperature (Tc) of 500 (100)° C
calculated for augite from Miller Range nakhlite (MIL 03346, 13) using the available …
calculated for augite from Miller Range nakhlite (MIL 03346, 13) using the available …
Thermal expansion of minerals in the pyroxene system and examination of various thermal expansion models
GL Hovis, M Tribaudino, A Leaman, C Almer… - American …, 2021 - degruyter.com
To examine the effects of chemical composition on thermal expansion in the pyroxene
mineral group, X‑ray diffraction data have been collected from room temperature to~ 925° C …
mineral group, X‑ray diffraction data have been collected from room temperature to~ 925° C …