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Papers by charles cockell

Research paper thumbnail of Isolation of an Extremophilic Cyanobacterium Using Low Earth Orbit as a Selection Factor

A rock-dwelling community from cliffs in Beer, UK was exposed to 10 days of LEO as part of the BI... more A rock-dwelling community from cliffs in Beer, UK was exposed to 10 days of LEO as part of the BIOPAN VI mission. An extremophilic cyanobacterium, which was identified as a member of the order Chroococcales was isolated after exposure.

Research paper thumbnail of Geological Characteristics of Remote Field Sites Using Infrared Spectroscopy: Results from the 1999 Marsokhod Field Test

Journal of Geophysical Research Atmospheres

Research paper thumbnail of ensuremath Darwinensuremath<?iensuremath> -- an experimental astronomy mission to search for extrasolar planets

As a response to ESA call for mission concepts for its Cosmic Vision 2015?2025 plan, we propose a... more As a response to ESA call for mission concepts for its Cosmic Vision 2015?2025 plan, we propose a mission called ensuremath Darwinensuremath<?iensuremath>. Its primary goal is the study of terrestrial extrasolar planets and the search for life on them. In this paper, we describe different characteristics of the instrument.

Research paper thumbnail of Lunar Astrobiology

Research paper thumbnail of The genetics of a microbe-mineral interaction

Geochmica et Cosmochimica Acta

Microbial activity has been linked to volcanic rock weathering. It is thought that the process is... more Microbial activity has been linked to volcanic rock weathering. It is thought that the process is generally driven by the nutrient requirement of the microbial community and occurs as a result of the sequestration of bioessential elements. Although we know that metabolising bacteria influence rock weathering, the molecular processes invloved are unknown. For the first time, we have used DNA microarray technology to investigate the genes involved in weathering, in particular the sequestering of iron using the heavy metal resistant bacterium, Cupriavidus metallidurans CH34. Extensive studies have characterized the heavy metal resistant and iron uptake mechanisms of this bacterium.Microarray analysis demonstrated that siderophore genes were not differentially expressed when grown in MM284 (iron-limited) with basalt. This was in concurrence with siderophore measurements using the CAS assay. Instead, a large number of porins and membrane transporters in concomitantly with genes associate...

Research paper thumbnail of CLUPI: Close-UP Imager on the ExoMars Mission rover

Research paper thumbnail of CLUPI, a high-performance imaging system on the rover of the 2018 mission to discover biofabrics on Mars

The scientific objectives of the 2018 ExoMars rover mission are to search for traces of past or p... more The scientific objectives of the 2018 ExoMars rover mission are to search for traces of past or present life and to characterise the near-sub surface. Both objectives require study of the rock/regolith materials in terms of structure, textures, mineralogy, and elemental and organic composition. The 2018 ExoMars rover payload consists of a suite of complementary instruments designed to reach these objectives. CLUPI, the high-performance colour close up imager, on board the 2018 ExoMars Rover plays an important role in attaining the mission objectives: it is the equivalent of the hand lens that no geologist is without when undertaking field work. CLUPI is a powerful, highly integrated miniaturized (<700g) low-power robust imaging system, able to operate at very low temperatures (-120°C). CLUPI has a working distance from 10cm to infinite providing outstanding pictures with a color detector of 2652x1768. At 10cm, the resolution is 7 micrometer/pixel in color. The optical-mechanical ...

Research paper thumbnail of Kelly et al 2014 with figures

Research paper thumbnail of COSPAR poster text

Research paper thumbnail of SGM Actinobacteria poster

Research paper thumbnail of COSPAR poster post conference

Research paper thumbnail of Stone 6: Mars-analogue artificial sedimentary meteorites in space

Of the 34 meteorites from Mars, none are sedimentary although sediments exist in abundance on the... more Of the 34 meteorites from Mars, none are sedimentary although sediments exist in abundance on the planet. The STONE experiments aim at testing the survivability of different types of analogue martian sediments during entry into the Earth's atmosphere. The rocks are fixed into the heat shield of a FOTON re-entry vehicle around the ablation point and undergo entry speeds of about 7.6 km/s (meteorite entry speeds are slightly higher, at 12-15 km/s). Previous STONE experiments have proven the survivability of dolomite and sandstone through atmospheric passage (STONE 1 and STONE 5). The STONE 6 experiment included an Early Archaean chert (3.446 Ga) from the Pilbara containing cryptic traces of fossil life (microfossils, C isotopes) (N.B. this sample is a good sedimentary Noachian Mars analogue], a Devonian laminite (mudstone) from the Orkneys (Fig 1e), and an Eocene basalt from Austria. A culture of a modern endolithic microorganism, Chroococcidiopsis, was smeared on the back side an...

Research paper thumbnail of STONE 6: Artificial Sedimentary Meteorites in Space

The STONE 6 experiment demonstrated the survivability of carbonaceous and microfossiliferous mart... more The STONE 6 experiment demonstrated the survivability of carbonaceous and microfossiliferous martian analogue sediments during atmospheric re-entry. Doped endoliths died but their carbonised cells remained.

Research paper thumbnail of Simulation of the Martian atmosphere for exobiology experiments with special emphasis on the water content

Research paper thumbnail of Impact experiments in support of "Lithopanspermia": The route from Mars to Earth

Shock recovery experiments on a Martian analogue rock (gabbro) loaded with three types of microor... more Shock recovery experiments on a Martian analogue rock (gabbro) loaded with three types of microorganisms reveal that these organisms survive the impact and ejection phase on Mars at shock pressures up to about 50 GPa with exponentially decreasing survival rates.

Research paper thumbnail of Stöffler, D., Horneck, G., Ott, S., Hornemann U., Cockell, C. S., Moeller, R., Meyer, C., de Vera, J.-P., Fritz, F., and Artemieva, N. A. (2007) Experimental evidence for the impact ejection of viable microorganisms from Mars and Mars-like planets, Icarus 186, 585-588

Stöffler, D., Horneck, G., Ott, S., Hornemann U., Cockell, C. S., Moeller, R., Meyer, C., de Vera, J.-P., Fritz, F., and Artemieva, N. A. (2007) Experimental evidence for the impact ejection of viable microorganisms from Mars and Mars-like planets, Icarus 186, 585-588

Icarus

Research paper thumbnail of Testing the Survival of Microfossils During Entry Into the Earth's Atmosphere: The STONE 6 Experiment

Research paper thumbnail of A 500-year experiment

Astronomy & Geophysics, 2015

Research paper thumbnail of Impact Craters, Water and Microbial Life

Because of the lack of recent plate tectonics, the surface of Mars has abundant, well-preserved i... more Because of the lack of recent plate tectonics, the surface of Mars has abundant, well-preserved impact structures. Impact structures can localize water in a number of ways including: 1) circulation of water into hydrothermal systems, 2) ponding of water in the hydrologic depression of the crater. This ponding can occur because of excavation below the water table, filling of the

Research paper thumbnail of 11 Impact Craters, Water and Microbial Life

Because of the lack of recent plate tectonics, the surface of Mars has abundant, well-preserved i... more Because of the lack of recent plate tectonics, the surface of Mars has abundant, well-preserved impact structures. Impact structures can localize water in a number of ways including: 1) circulation of water into hydrothermal systems, 2) ponding of water in the hydrologic depression of the crater. This ponding can occur because of excavation below the water table, filling of the

Research paper thumbnail of Isolation of an Extremophilic Cyanobacterium Using Low Earth Orbit as a Selection Factor

A rock-dwelling community from cliffs in Beer, UK was exposed to 10 days of LEO as part of the BI... more A rock-dwelling community from cliffs in Beer, UK was exposed to 10 days of LEO as part of the BIOPAN VI mission. An extremophilic cyanobacterium, which was identified as a member of the order Chroococcales was isolated after exposure.

Research paper thumbnail of Geological Characteristics of Remote Field Sites Using Infrared Spectroscopy: Results from the 1999 Marsokhod Field Test

Journal of Geophysical Research Atmospheres

Research paper thumbnail of ensuremath Darwinensuremath<?iensuremath> -- an experimental astronomy mission to search for extrasolar planets

As a response to ESA call for mission concepts for its Cosmic Vision 2015?2025 plan, we propose a... more As a response to ESA call for mission concepts for its Cosmic Vision 2015?2025 plan, we propose a mission called ensuremath Darwinensuremath<?iensuremath>. Its primary goal is the study of terrestrial extrasolar planets and the search for life on them. In this paper, we describe different characteristics of the instrument.

Research paper thumbnail of Lunar Astrobiology

Research paper thumbnail of The genetics of a microbe-mineral interaction

Geochmica et Cosmochimica Acta

Microbial activity has been linked to volcanic rock weathering. It is thought that the process is... more Microbial activity has been linked to volcanic rock weathering. It is thought that the process is generally driven by the nutrient requirement of the microbial community and occurs as a result of the sequestration of bioessential elements. Although we know that metabolising bacteria influence rock weathering, the molecular processes invloved are unknown. For the first time, we have used DNA microarray technology to investigate the genes involved in weathering, in particular the sequestering of iron using the heavy metal resistant bacterium, Cupriavidus metallidurans CH34. Extensive studies have characterized the heavy metal resistant and iron uptake mechanisms of this bacterium.Microarray analysis demonstrated that siderophore genes were not differentially expressed when grown in MM284 (iron-limited) with basalt. This was in concurrence with siderophore measurements using the CAS assay. Instead, a large number of porins and membrane transporters in concomitantly with genes associate...

Research paper thumbnail of CLUPI: Close-UP Imager on the ExoMars Mission rover

Research paper thumbnail of CLUPI, a high-performance imaging system on the rover of the 2018 mission to discover biofabrics on Mars

The scientific objectives of the 2018 ExoMars rover mission are to search for traces of past or p... more The scientific objectives of the 2018 ExoMars rover mission are to search for traces of past or present life and to characterise the near-sub surface. Both objectives require study of the rock/regolith materials in terms of structure, textures, mineralogy, and elemental and organic composition. The 2018 ExoMars rover payload consists of a suite of complementary instruments designed to reach these objectives. CLUPI, the high-performance colour close up imager, on board the 2018 ExoMars Rover plays an important role in attaining the mission objectives: it is the equivalent of the hand lens that no geologist is without when undertaking field work. CLUPI is a powerful, highly integrated miniaturized (<700g) low-power robust imaging system, able to operate at very low temperatures (-120°C). CLUPI has a working distance from 10cm to infinite providing outstanding pictures with a color detector of 2652x1768. At 10cm, the resolution is 7 micrometer/pixel in color. The optical-mechanical ...

Research paper thumbnail of Kelly et al 2014 with figures

Research paper thumbnail of COSPAR poster text

Research paper thumbnail of SGM Actinobacteria poster

Research paper thumbnail of COSPAR poster post conference

Research paper thumbnail of Stone 6: Mars-analogue artificial sedimentary meteorites in space

Of the 34 meteorites from Mars, none are sedimentary although sediments exist in abundance on the... more Of the 34 meteorites from Mars, none are sedimentary although sediments exist in abundance on the planet. The STONE experiments aim at testing the survivability of different types of analogue martian sediments during entry into the Earth's atmosphere. The rocks are fixed into the heat shield of a FOTON re-entry vehicle around the ablation point and undergo entry speeds of about 7.6 km/s (meteorite entry speeds are slightly higher, at 12-15 km/s). Previous STONE experiments have proven the survivability of dolomite and sandstone through atmospheric passage (STONE 1 and STONE 5). The STONE 6 experiment included an Early Archaean chert (3.446 Ga) from the Pilbara containing cryptic traces of fossil life (microfossils, C isotopes) (N.B. this sample is a good sedimentary Noachian Mars analogue], a Devonian laminite (mudstone) from the Orkneys (Fig 1e), and an Eocene basalt from Austria. A culture of a modern endolithic microorganism, Chroococcidiopsis, was smeared on the back side an...

Research paper thumbnail of STONE 6: Artificial Sedimentary Meteorites in Space

The STONE 6 experiment demonstrated the survivability of carbonaceous and microfossiliferous mart... more The STONE 6 experiment demonstrated the survivability of carbonaceous and microfossiliferous martian analogue sediments during atmospheric re-entry. Doped endoliths died but their carbonised cells remained.

Research paper thumbnail of Simulation of the Martian atmosphere for exobiology experiments with special emphasis on the water content

Research paper thumbnail of Impact experiments in support of "Lithopanspermia": The route from Mars to Earth

Shock recovery experiments on a Martian analogue rock (gabbro) loaded with three types of microor... more Shock recovery experiments on a Martian analogue rock (gabbro) loaded with three types of microorganisms reveal that these organisms survive the impact and ejection phase on Mars at shock pressures up to about 50 GPa with exponentially decreasing survival rates.

Research paper thumbnail of Stöffler, D., Horneck, G., Ott, S., Hornemann U., Cockell, C. S., Moeller, R., Meyer, C., de Vera, J.-P., Fritz, F., and Artemieva, N. A. (2007) Experimental evidence for the impact ejection of viable microorganisms from Mars and Mars-like planets, Icarus 186, 585-588

Stöffler, D., Horneck, G., Ott, S., Hornemann U., Cockell, C. S., Moeller, R., Meyer, C., de Vera, J.-P., Fritz, F., and Artemieva, N. A. (2007) Experimental evidence for the impact ejection of viable microorganisms from Mars and Mars-like planets, Icarus 186, 585-588

Icarus

Research paper thumbnail of Testing the Survival of Microfossils During Entry Into the Earth's Atmosphere: The STONE 6 Experiment

Research paper thumbnail of A 500-year experiment

Astronomy & Geophysics, 2015

Research paper thumbnail of Impact Craters, Water and Microbial Life

Because of the lack of recent plate tectonics, the surface of Mars has abundant, well-preserved i... more Because of the lack of recent plate tectonics, the surface of Mars has abundant, well-preserved impact structures. Impact structures can localize water in a number of ways including: 1) circulation of water into hydrothermal systems, 2) ponding of water in the hydrologic depression of the crater. This ponding can occur because of excavation below the water table, filling of the

Research paper thumbnail of 11 Impact Craters, Water and Microbial Life

Because of the lack of recent plate tectonics, the surface of Mars has abundant, well-preserved i... more Because of the lack of recent plate tectonics, the surface of Mars has abundant, well-preserved impact structures. Impact structures can localize water in a number of ways including: 1) circulation of water into hydrothermal systems, 2) ponding of water in the hydrologic depression of the crater. This ponding can occur because of excavation below the water table, filling of the