Compositional Variations in Sedimentary Deposits in Gale Crater as Observed by ChemCam Passive and Active Spectra

Research output: Contribution to journalJournal articleResearchpeer-review

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Compositional Variations in Sedimentary Deposits in Gale Crater as Observed by ChemCam Passive and Active Spectra. / Manelski, H. T.; Sheppard, R. Y.; Fraeman, A. A.; Wiens, R. C.; Johnson, J. R.; Rampe, E. B.; Frydenvang, J.; Lanza, N. L.; Gasnault, O.

In: Journal of Geophysical Research: Planets, Vol. 128, No. 3, e2022JE007706, 2023.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Manelski, HT, Sheppard, RY, Fraeman, AA, Wiens, RC, Johnson, JR, Rampe, EB, Frydenvang, J, Lanza, NL & Gasnault, O 2023, 'Compositional Variations in Sedimentary Deposits in Gale Crater as Observed by ChemCam Passive and Active Spectra', Journal of Geophysical Research: Planets, vol. 128, no. 3, e2022JE007706. https://doi.org/10.1029/2022JE007706

APA

Manelski, H. T., Sheppard, R. Y., Fraeman, A. A., Wiens, R. C., Johnson, J. R., Rampe, E. B., Frydenvang, J., Lanza, N. L., & Gasnault, O. (2023). Compositional Variations in Sedimentary Deposits in Gale Crater as Observed by ChemCam Passive and Active Spectra. Journal of Geophysical Research: Planets, 128(3), [e2022JE007706]. https://doi.org/10.1029/2022JE007706

Vancouver

Manelski HT, Sheppard RY, Fraeman AA, Wiens RC, Johnson JR, Rampe EB et al. Compositional Variations in Sedimentary Deposits in Gale Crater as Observed by ChemCam Passive and Active Spectra. Journal of Geophysical Research: Planets. 2023;128(3). e2022JE007706. https://doi.org/10.1029/2022JE007706

Author

Manelski, H. T. ; Sheppard, R. Y. ; Fraeman, A. A. ; Wiens, R. C. ; Johnson, J. R. ; Rampe, E. B. ; Frydenvang, J. ; Lanza, N. L. ; Gasnault, O. / Compositional Variations in Sedimentary Deposits in Gale Crater as Observed by ChemCam Passive and Active Spectra. In: Journal of Geophysical Research: Planets. 2023 ; Vol. 128, No. 3.

Bibtex

@article{6ccadbd958e840f294504a4ff95192d6,
title = "Compositional Variations in Sedimentary Deposits in Gale Crater as Observed by ChemCam Passive and Active Spectra",
abstract = "During the first 2934 sols of the Curiosity rover's mission 33,468 passive visible/near-infrared (NIR) reflectance spectra were taken of the surface by the mast-mounted Chemistry and Camera (ChemCam) instrument on a range of target types. ChemCam spectra of bedrock targets from the Murray and Carolyn Shoemaker formations on Mt. Sharp were investigated using principal component analysis and various spectral parameters including the band depth at 535 nm and the slope between 840 and 750 nm. Four end-member spectra were identified. Passive spectra were compared to Laser Induced Breakdown Spectroscopy (LIBS) data to search for correlations between spectral properties and elemental abundances. The correlation coefficient between FeOT reported by LIBS and BD535 from passive spectra was used to search for regions where iron may have been added to the bedrock through oxidation of ferrous-bearing fluids but no correlations were found. Rocks in the Blunts Point-Sutton Island transition that have unique spectral properties compared to surrounding rocks, that is flat NIR slopes and weak 535 nm absorptions, are associated with higher Mn and Mg in the LIBS spectra of bedrock. Additionally, calcium-sulfate cements, previously identified by Ca and S enrichments in the LIBS spectra of bedrock, were also shown to be associated with spectral trends seen in Blunts Point. A shift toward a steeper NIR slope is seen in the Hutton interval, indicative of changing depositional conditions or increased diagenesis.",
author = "Manelski, {H. T.} and Sheppard, {R. Y.} and Fraeman, {A. A.} and Wiens, {R. C.} and Johnson, {J. R.} and Rampe, {E. B.} and J. Frydenvang and Lanza, {N. L.} and O. Gasnault",
year = "2023",
doi = "10.1029/2022JE007706",
language = "English",
volume = "128",
journal = "Journal of Geophysical Research: Planets",
issn = "2169-9100",
publisher = "American Geophysical Union",
number = "3",

}

RIS

TY - JOUR

T1 - Compositional Variations in Sedimentary Deposits in Gale Crater as Observed by ChemCam Passive and Active Spectra

AU - Manelski, H. T.

AU - Sheppard, R. Y.

AU - Fraeman, A. A.

AU - Wiens, R. C.

AU - Johnson, J. R.

AU - Rampe, E. B.

AU - Frydenvang, J.

AU - Lanza, N. L.

AU - Gasnault, O.

PY - 2023

Y1 - 2023

N2 - During the first 2934 sols of the Curiosity rover's mission 33,468 passive visible/near-infrared (NIR) reflectance spectra were taken of the surface by the mast-mounted Chemistry and Camera (ChemCam) instrument on a range of target types. ChemCam spectra of bedrock targets from the Murray and Carolyn Shoemaker formations on Mt. Sharp were investigated using principal component analysis and various spectral parameters including the band depth at 535 nm and the slope between 840 and 750 nm. Four end-member spectra were identified. Passive spectra were compared to Laser Induced Breakdown Spectroscopy (LIBS) data to search for correlations between spectral properties and elemental abundances. The correlation coefficient between FeOT reported by LIBS and BD535 from passive spectra was used to search for regions where iron may have been added to the bedrock through oxidation of ferrous-bearing fluids but no correlations were found. Rocks in the Blunts Point-Sutton Island transition that have unique spectral properties compared to surrounding rocks, that is flat NIR slopes and weak 535 nm absorptions, are associated with higher Mn and Mg in the LIBS spectra of bedrock. Additionally, calcium-sulfate cements, previously identified by Ca and S enrichments in the LIBS spectra of bedrock, were also shown to be associated with spectral trends seen in Blunts Point. A shift toward a steeper NIR slope is seen in the Hutton interval, indicative of changing depositional conditions or increased diagenesis.

AB - During the first 2934 sols of the Curiosity rover's mission 33,468 passive visible/near-infrared (NIR) reflectance spectra were taken of the surface by the mast-mounted Chemistry and Camera (ChemCam) instrument on a range of target types. ChemCam spectra of bedrock targets from the Murray and Carolyn Shoemaker formations on Mt. Sharp were investigated using principal component analysis and various spectral parameters including the band depth at 535 nm and the slope between 840 and 750 nm. Four end-member spectra were identified. Passive spectra were compared to Laser Induced Breakdown Spectroscopy (LIBS) data to search for correlations between spectral properties and elemental abundances. The correlation coefficient between FeOT reported by LIBS and BD535 from passive spectra was used to search for regions where iron may have been added to the bedrock through oxidation of ferrous-bearing fluids but no correlations were found. Rocks in the Blunts Point-Sutton Island transition that have unique spectral properties compared to surrounding rocks, that is flat NIR slopes and weak 535 nm absorptions, are associated with higher Mn and Mg in the LIBS spectra of bedrock. Additionally, calcium-sulfate cements, previously identified by Ca and S enrichments in the LIBS spectra of bedrock, were also shown to be associated with spectral trends seen in Blunts Point. A shift toward a steeper NIR slope is seen in the Hutton interval, indicative of changing depositional conditions or increased diagenesis.

U2 - 10.1029/2022JE007706

DO - 10.1029/2022JE007706

M3 - Journal article

VL - 128

JO - Journal of Geophysical Research: Planets

JF - Journal of Geophysical Research: Planets

SN - 2169-9100

IS - 3

M1 - e2022JE007706

ER -

ID: 338786805