Materials Map

Discover the materials research landscape. Find experts, partners, networks.

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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Materials Map under construction

The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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1.080 Topics available

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (2/2 displayed)

  • 2020Characterisation of iron oxide encrusted microbial fossils12citations
  • 2012Carbonate precipitation under bulk acidic conditions as a potential biosignature for searching life on Mars28citations

Places of action

Chart of shared publication
Gagen, Emma J.
1 / 2 shared
Rintoul, Llew
1 / 1 shared
Levett, Alan
1 / 1 shared
Vasconcelos, Paulo M.
1 / 1 shared
Diao, Hui
1 / 1 shared
Flemming, Roberta
1 / 1 shared
Gómez-Ortíz, David
1 / 1 shared
Banerjee, Neil R.
1 / 2 shared
Rodríguez, Nuria
1 / 4 shared
Preston, Louisa J.
1 / 1 shared
Izawa, Matthew R. M.
1 / 1 shared
Dyar, M. Darby
1 / 5 shared
Osinski, Gordon R.
1 / 1 shared
Sánchez-Román, Mónica
1 / 2 shared
Prieto-Ballesteros, Olga
1 / 2 shared
Amils, Ricardo
1 / 1 shared
Fernández-Remolar, David C.
1 / 2 shared
Huang, L.
1 / 3 shared
Chart of publication period
2020
2012

Co-Authors (by relevance)

  • Gagen, Emma J.
  • Rintoul, Llew
  • Levett, Alan
  • Vasconcelos, Paulo M.
  • Diao, Hui
  • Flemming, Roberta
  • Gómez-Ortíz, David
  • Banerjee, Neil R.
  • Rodríguez, Nuria
  • Preston, Louisa J.
  • Izawa, Matthew R. M.
  • Dyar, M. Darby
  • Osinski, Gordon R.
  • Sánchez-Román, Mónica
  • Prieto-Ballesteros, Olga
  • Amils, Ricardo
  • Fernández-Remolar, David C.
  • Huang, L.
OrganizationsLocationPeople

article

Carbonate precipitation under bulk acidic conditions as a potential biosignature for searching life on Mars

  • Flemming, Roberta
  • Gómez-Ortíz, David
  • Banerjee, Neil R.
  • Rodríguez, Nuria
  • Preston, Louisa J.
  • Izawa, Matthew R. M.
  • Dyar, M. Darby
  • Osinski, Gordon R.
  • Sánchez-Román, Mónica
  • Prieto-Ballesteros, Olga
  • Amils, Ricardo
  • Fernández-Remolar, David C.
  • Huang, L.
  • Southam, Gordon
Abstract

<p>Recent observations of carbonate minerals in ancient Martian rocks have been interpreted as evidence for the former presence of circumneutral solutions optimal for carbonate precipitation. Sampling from surface and subsurface regions of the low-pH system of Río Tinto has shown, unexpectedly, that carbonates can form under diverse macroscopic physicochemical conditions ranging from very low to neutral pH (1.5-7.0). A multi-technique approach demonstrates that carbonate minerals are closely associated with microbial activity. Carbonates occur in the form of micron-size carbonate precipitates under bacterial biofilms, mineralization of subsurface colonies, and possible biogenic microstructures including globules, platelets and dumbbell morphologies. We propose that carbonate precipitation in the low-pH environment of Río Tinto is a process enabled by microbially-mediated neutralization driven by the reduction of ferric iron coupled to the oxidation of biomolecules in microbially-maintained circumneutral oases, where the local pH (at the scale of cells or cell colonies) can be much different than in the macroscopic environment. Acidic conditions were likely predominant in vast regions of Mars over the last four billion years of planetary evolution. Ancient Martian microbial life inhabiting low-pH environments could have precipitated carbonates similar to those observed at Río Tinto. Preservation of carbonates at Río Tinto over geologically significant timescales suggests that similarly-formed carbonate minerals could also be preserved on Mars. Such carbonates could soon be observed by the Mars Science Laboratory, and by future missions to the red planet.</p>

Topics
  • impedance spectroscopy
  • mineral
  • surface
  • precipitate
  • precipitation
  • iron