Evidence for Mg-rich carbonates on Mars from a 3.9 μm absorption feature
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Organic matter is absent on both Mars and moon although they do contain carbon.
“However organic matter is absent on both Mars and moon although they do contain carbon [2]–[6].”
From Can Plants Grow on Mars and the Moon: A Growth Experiment on Mars and Moon Soil Simulants (2014) · cites this paper as [2]
There is no organic matter on Mars, as far as we know.
“There is no organic matter on Mars [2]–[6], as far as we now, so this would make the Mars simulant we used less suitable for experiments to investigate the potential of Mars soil, unless the experiment has as goal to test the potential of the soil after adding organic matter.”
From Can Plants Grow on Mars and the Moon: A Growth Experiment on Mars and Moon Soil Simulants (2014) · cites this paper as [2]
Cites
Early geochemical environment of Mars as determined from thermodynamics of phyllosilicates
Chevrier, V., Poulet, F., & Bibring, J.-P. (2007) · Nature · doi:10.1038/nature05961 · Cited by 208 · see citing works
Initial results from the Mini-TES experiment in Gusev crater from the Spirit rover
Christensen, P. R., Ruff, S. W., Fergason, R. L., Knudson, A. T., Anwar, S., Arvidson, R. E., Bandfield, J. L., Blaney, D. L., Budney, C., Calvin, W. M., et al. (2004) · Science · doi:10.1126/science.1100564 · Cited by 173 · see citing works
Wilson, S. A. (2006) · American Mineralogist · doi:10.2138/am.2006.2058 · Cited by 172 · see citing works
Thermal infrared emission spectroscopy of anhydrous carbonates
Lane, M. D., & Christensen, P. R. (1997) · Journal of Geophysical Research: Planets · doi:10.1029/97je02046 · Cited by 138 · cited 2× · see citing works
“0 lm (Farmer, 1974; Salisbury, 1991; Gaffey et al., 1993; Calvin et al., 1994; Lane and Christensen, 1997).”
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Hydrothermal formation of Clay-Carbonate alteration assemblages in the Nili Fossae region of Mars
Brown, A. J., Hook, S. J., Baldridge, A. M., Crowley, J. K., Bridges, N. T., Thomson, B. J., Marion, G. M., de Souza Filho, C. R., & Bishop, J. L. (2010) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2010.06.018 · Cited by 219 · see citing works
Can Plants Grow on Mars and the Moon: A Growth Experiment on Mars and Moon Soil Simulants
Wamelink, G. W. W., Frissel, J. Y., Krijnen, W. H. J., Verwoert, M. R., & Goedhart, P. W. (2014) · PLoS ONE · doi:10.1371/journal.pone.0103138 · Cited by 201 · see citing works
Orbital evidence for more widespread carbonate-bearing rocks on Mars
Wray, J. J., Murchie, S. L., Bishop, J. L., Ehlmann, B. L., Milliken, R. E., Wilhelm, M. B., Seelos, K. D., & Chojnacki, M. (2016) · Journal of Geophysical Research: Planets · doi:10.1002/2015je004972 · Cited by 161 · see citing works
Aerobic biomineralization of Mg-rich carbonates: Implications for natural environments
Sánchez-Román, M., Romanek, C. S., Fernández-Remolar, D. C., Sánchez-Navas, A., McKenzie, J. A., Pibernat, R. A., & Vasconcelos, C. (2011) · Chemical Geology · doi:10.1016/j.chemgeo.2010.11.020 · Cited by 141 · see citing works
Cosmic dust fluxes in the atmospheres of Earth, Mars, and Venus
Carrillo-Sánchez, J. D., Gómez-Martín, J. C., Bones, D. L., Nesvorný, D., Pokorný, P., Benna, M., Flynn, G. J., & Plane, J. M. C. (2020) · Icarus · doi:10.1016/j.icarus.2019.113395 · Cited by 116 · see citing works
Shirokova, L. S., Mavromatis, V., Bundeleva, I. A., Pokrovsky, O. S., Bénézeth, P., Gérard, E., Pearce, C. R., & Oelkers, E. H. (2013) · Aquatic Geochemistry · doi:10.1007/s10498-012-9174-3 · Cited by 109 · see citing works
Carbonate Detection With SuperCam in Igneous Rocks on the Floor of Jezero Crater, Mars
Clavé, E., Benzerara, K., Meslin, P. ‐., Forni, O., Royer, C., Mandon, L., Beck, P., Quantin‐Nataf, C., Beyssac, O., Cousin, A., et al. (2023) · Journal of Geophysical Research: Planets · doi:10.1029/2022je007463 · Cited by 93 · see citing works
Self-citationBishop, J. L., Perry, K. A., Darby Dyar, M., Bristow, T. F., Blake, D. F., Brown, A. J., & Peel, S. E. (2013) · Journal of Geophysical Research: Planets · doi:10.1002/jgre.20066 · Cited by 52 · see citing works
- Authors
- Palomba, E., Zinzi, A., Cloutis, E. A., D’Amore, M., Grassi, D., & Maturilli, A.
- Affiliations
- National Institute for Astrophysics (IT)
- University of L'Aquila (IT)
- The University of Winnipeg (CA)
- Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (DE)
- Corresponding author
- Palomba, Ernesto
- ORCID
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 2009-09
- Volume
- 203
- Issue
- 1
- Pages
- 58-65
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2062606692
- Cited by
- 59
- References
- 4
- Citations by year
- 2026: 1 · 2025: 2 · 2024: 1 · 2023: 3 · 2022: 7 · 2021: 4 · 2020: 3 · 2019: 3 · 2018: 2 · 2017: 5 · 2016: 6 · 2015: 2 · 2014: 3 · 2013: 5 · 2012: 1
- FWCI
- 1.94
- Type
- journal article
- Language
- en
- Open access
- green
- hal.science
- Licence
- Locations
- Icarus (publishedVersion)
- HAL (submittedVersion, other-oa)
- Trinity's Access to Research Output (TARA) (Trinity College Dublin) (submittedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Physical Sciences › Computer Science › Artificial Intelligence › Geochemistry and Geologic Mapping
- Keywords
- Mars, huntite, magnesite, Martian regolith, paleoclimate, carbonate weathering, Planetary Fourier Spectrometer, Mars Express, Mars mineralogy
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
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