Claire Newman

ORCID: 0000-0001-9990-8817
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About
Contact & Profiles
Research Areas
  • Planetary Science and Exploration
  • Astro and Planetary Science
  • Space Exploration and Technology
  • Aeolian processes and effects
  • Space Science and Extraterrestrial Life
  • Spaceflight effects on biology
  • Geology and Paleoclimatology Research
  • Atmospheric and Environmental Gas Dynamics
  • Methane Hydrates and Related Phenomena
  • Scientific Research and Discoveries
  • Solar and Space Plasma Dynamics
  • Geomagnetism and Paleomagnetism Studies
  • Spacecraft and Cryogenic Technologies
  • Meteorological Phenomena and Simulations
  • Space exploration and regulation
  • Geophysics and Gravity Measurements
  • Biocrusts and Microbial Ecology
  • Isotope Analysis in Ecology
  • Aerospace Engineering and Energy Systems
  • Marine and environmental studies
  • Atmospheric aerosols and clouds
  • Spacecraft Design and Technology
  • Air Quality Monitoring and Forecasting
  • Ionosphere and magnetosphere dynamics
  • Particle Dynamics in Fluid Flows

Aeolis Research (United States)
2016-2025

University of Wyoming
2024

Goddard Space Flight Center
2023

Jet Propulsion Laboratory
2005-2023

University of the Basque Country
2023

California Institute of Technology
2005-2022

Southwest Research Institute
2022

Observatoire de Paris
2022

The King's College
2018

Ashima Group (United States)
2009-2017

The Curiosity rover discovered fine-grained sedimentary rocks, which are inferred to represent an ancient lake and preserve evidence of environment that would have been suited support a martian biosphere founded on chemolithoautotrophy. This aqueous was characterized by neutral pH, low salinity, variable redox states both iron sulfur species. Carbon, hydrogen, oxygen, sulfur, nitrogen, phosphorus were measured directly as key biogenic elements; inference, is assumed available. probably had...

10.1126/science.1242777 article EN Science 2013-12-10
Donald M. Hassler C. Zeitlin R. F. Wimmer‐Schweingruber Bent Ehresmann Scot Rafkin and 95 more J. L. Eigenbrode D. E. Brinza Gerald Weigle Stephan Böttcher Eckart Böhm Söenke Burmeister Jingnan Guo Jan Köhler César Martı́n G. Reitz Francis A. Cucinotta Myung‐Hee Y. Kim David Grinspoon M. A. Bullock Arik Posner Javier Gómez‐Elvira A. R. Vasavada J. P. Grotzinger MSL Science Team Osku Kemppinen David A. Cremers J. F. Bell Lauren Edgar Jack D. Farmer Austin Godber M. Wadhwa Danika Wellington Ian McEwan Claire Newman M. I. Richardson Antoine Charpentier Laurent Péret P. L. King J. G. Blank M. E. Schmidt Shuai Li R. E. Milliken Kevin M. Robertson V. Z. Sun Michael B. Baker Christopher S. Edwards B. L. Ehlmann K. A. Farley J. L. Griffes Hayden Miller Megan Newcombe C. Pilorget M. S. Rice K. L. Siebach Katie Stack Edward M. Stolper Claude Brunet V. Hipkin Richard Léveillé Geneviève Marchand Pablo Sobrón Sánchez Laurent Favot George D. Cody A. Steele Lorenzo Flückiger David Lees Ara Nefian Mildred Martin M. Gailhanou Francès Westall Guy Israël Christophe Agard Julien Baroukh Christophe Donny Alain Gaboriaud Philippe Guillemot Vivian Lafaille Eric Lorigny Alexis Paillet R. Pérez M. Saccoccio Charles Yana Carlos Armiens‐Aparicio Javier Caride Rodríguez Isaías Carrasco Blázquez Felipe Gómez Sebastian Hettrich Alain Lepinette Malvitte Mercedes Marín Jiménez Jesús Martínez‐Frías Javier Martín-Soler Javier Martín‐Torres Antonio Molina Jurado Luis Mora‐Sotomayor G. M. Muñoz Sara Navarro López Verónica Peinado-González Jorge Pla-García J. A. Rodríguez‐Manfredi Julio José Romeral-Planelló

The Radiation Assessment Detector (RAD) on the Mars Science Laboratory’s Curiosity rover began making detailed measurements of cosmic ray and energetic particle radiation environment surface 7 August 2012. We report discuss absorbed dose equivalent from galactic rays solar particles martian for ~300 days observations during current maximum. These provide insight into hazards associated with a human mission to an anchor point which model subsurface environment, implications microbial survival...

10.1126/science.1244797 article EN Science 2013-12-10

Samples from the Rocknest aeolian deposit were heated to ~835°C under helium flow and evolved gases analyzed by Curiosity’s Sample Analysis at Mars instrument suite. H 2 O, SO , CO O major released. Water abundance (1.5 3 weight percent) release temperature suggest that is bound within an amorphous component of sample. Decomposition fine-grained Fe or Mg carbonate likely source much . Evolved coincident with Cl, suggesting oxygen produced thermal decomposition oxychloride compound. Elevated...

10.1126/science.1238937 article EN Science 2013-09-26
P. R. Mahaffy Christopher R. Webster S. K. Atreya H. B. Franz Michael Wong and 95 more P. G. Conrad D. N. Harpold John J. Jones L. A. Leshin H. L. K. Manning Tobias Owen R. O. Pepin S. W. Squyres M. G. Trainer Osku Kemppinen Nathan Bridges J. R. Johnson M. E. Minitti David A. Cremers J. F. Bell Lauren Edgar Jack D. Farmer Austin Godber M. Wadhwa Danika Wellington Ian McEwan Claire Newman M. I. Richardson Antoine Charpentier Laurent Péret P. L. King J. G. Blank Gerald Weigle M. E. Schmidt Shuai Li R. E. Milliken Kevin M. Robertson V. Z. Sun Michael B. Baker Christopher Edwards Bethany Ehlmann Kenneth Farley J. L. Griffes J. P. Grotzinger Hayden Miller Megan Newcombe C. Pilorget M. S. Rice Kirsten Siebach Katie Stack Edward M. Stolper Claude Brunet V. Hipkin Richard Léveillé Geneviève Marchand Pablo Sobrón Sánchez Laurent Favot George D. Cody A. Steele Lorenzo Flückiger David Lees Ara Nefian Mildred Martin M. Gailhanou Francès Westall Guy Israël Christophe Agard Julien Baroukh Christophe Donny Alain Gaboriaud Philippe Guillemot Vivian Lafaille Eric Lorigny Alexis Paillet R. Pérez M. Saccoccio Charles Yana Carlos Armiens‐Aparicio Javier Caride Rodríguez Isaías Carrasco Blázquez Felipe Gómez Javier Gómez‐Elvira Sebastian Hettrich Alain Lepinette Malvitte Mercedes Marín Jiménez Jesús Martínez‐Frías Javier Martín-Soler Javier Martín‐Torres Antonio Molina Jurado Luis Mora‐Sotomayor G. M. Muñoz Sara Navarro López Verónica Peinado-González Jorge Pla-García J. A. Rodríguez‐Manfredi Julio José Romeral-Planelló Sara Alejandra Sans Fuentes Eduardo Sebastian Martinez J. Torres Roser Urqui-O'Callaghan

Volume mixing and isotope ratios secured with repeated atmospheric measurements taken the Sample Analysis at Mars instrument suite on Curiosity rover are: carbon dioxide (CO2), 0.960(±0.007); argon-40 ((40)Ar), 0.0193(±0.0001); nitrogen (N2), 0.0189(±0.0003); oxygen, 1.45(±0.09) × 10(-3); monoxide, < 1.0 (40)Ar/(36)Ar, 1.9(±0.3) 10(3). The (40)Ar/N2 ratio is 1.7 times greater (40)Ar/(36)Ar 1.6 lower than values reported by Viking Lander mass spectrometer in 1976, whereas other are generally...

10.1126/science.1237966 article EN Science 2013-07-18

H 2 O, CO , SO O S, HCl, chlorinated hydrocarbons, NO, and other trace gases were evolved during pyrolysis of two mudstone samples acquired by the Curiosity rover at Yellowknife Bay within Gale crater, Mars. O/OH-bearing phases included 2:1 phyllosilicate(s), bassanite, akaganeite, amorphous materials. Thermal decomposition carbonates combustion organic materials are candidate sources for . Concurrent evolution hydrocarbons suggests presence oxychlorine phase(s). Sulfides likely...

10.1126/science.1245267 article EN Science 2013-12-10

Observations by the Mars Science Laboratory Mast Camera (Mastcam) in Gale crater reveal isolated outcrops of cemented pebbles (2 to 40 millimeters diameter) and sand grains with textures typical fluvial sedimentary conglomerates. Rounded conglomerates indicate substantial abrasion. ChemCam emission spectra at one outcrop show a predominantly feldspathic composition, consistent minimal aqueous alteration sediments. Sediment was mobilized ancient water flows that likely exceeded threshold...

10.1126/science.1237317 article EN Science 2013-05-30

A new planetary atmospheric numerical model, “planetWRF,” has been developed by modifying the Weather Research and Forecasting (WRF) model. The model generalized map projection, multiscale, nesting capabilities, blurring distinction between global mesoscale models enabling investigation of coupling processes on all scales, including global. can also be run in one, two, or three dimensions. conversion dynamical core for application altering projection grid boundary conditions as well physics...

10.1029/2006je002825 article EN Journal of Geophysical Research Atmospheres 2007-09-01

Sedimentary rocks examined by the Curiosity rover at Yellowknife Bay, Mars, were derived from sources that evolved an approximately average martian crustal composition to one influenced alkaline basalts. No evidence of chemical weathering is preserved, indicating arid, possibly cold, paleoclimates and rapid erosion deposition. The absence predicted geochemical variations indicates magnetite phyllosilicates formed diagenesis under low-temperature, circumneutral pH, rock-dominated aqueous...

10.1126/science.1244734 article EN Science 2013-12-10

The ChemCam instrument, which provides insight into martian soil chemistry at the submillimeter scale, identified two principal types along Curiosity rover traverse: a fine-grained mafic type and locally derived, coarse-grained felsic type. component is representative of widespread soils similar in composition to dust. It possesses ubiquitous hydrogen signature spectra, corresponding hydration amorphous phases found by CheMin instrument. This likely accounts for an important fraction global...

10.1126/science.1238670 article EN Science 2013-09-26
J. C. Stern B. Sutter Caroline Freissinet R. Navarro‐González Christopher P. McKay and 95 more P. D. Archer A. Buch Anna Brunner Patrice Coll J. L. Eigenbrode Alberto González Fairén H. B. Franz D. P. Glavin Srishti Kashyap A. C. McAdam D. W. Ming A. Steele Cyril Szopa J. J. Wray Javier Martín‐Torres María‐Paz Zorzano P. G. Conrad P. R. Mahaffy Osku Kemppinen N. T. Bridges J. R. Johnson M. E. Minitti David A. Cremers J. F. Bell L. A. Edgar Jack D. Farmer Austin Godber M. Wadhwa Danika Wellington Ian McEwan Claire Newman M. I. Richardson Antoine Charpentier Laurent Péret P. L. King J. G. Blank Gerald Weigle M. E. Schmidt Shuai Li R. E. Milliken Kevin M. Robertson V. Z. Sun Michael B. Baker Christopher S. Edwards B. L. Ehlmann K. A. Farley J. Shechet J. P. Grotzinger Hayden Miller Megan Newcombe C. Pilorget M. S. Rice K. L. Siebach Katie Stack Edward M. Stolper C. Brunet V. Hipkin Richard Léveillé Geneviève Marchand Pablo Sobrón Sánchez Laurent Favot George D. Cody A. Steele Lorenzo Flückiger David Lees Ara Nefian Mildred Martin Francès Westall G. Israël Christophe Agard Julien Baroukh Christophe Donny Philippe Guillemot Vivian Lafaille Eric Lorigny Alexis Paillet R. Pérez M. Saccoccio Charles Yana Carlos Armiens‐Aparicio Javier Caride Rodríguez Isaías Carrasco Blázquez Felipe Gómez Javier Gómez‐Elvira Sebastian Hettrich Alain Lepinette Malvitte Mercedes Marín Jiménez Jesús Martínez‐Frías Javier Martín-Soler F. Javier Martín - Torres Antonio Molina Jurado Luis Mora‐Sotomayor G. M. Muñoz Sara Navarro López Verónica Peinado-González

Significance We present data supporting the presence of an indigenous source fixed nitrogen on surface Mars in form nitrate. This may indicate first stage development a primitive cycle ancient and would have provided biochemically accessible nitrogen.

10.1073/pnas.1420932112 article EN Proceedings of the National Academy of Sciences 2015-03-23

Abstract Mars Science Laboratory Curiosity rover observations of the 2018/Mars year 34 global/planet‐encircling dust storm represent first in situ measurements a global with dedicated meteorological sensors since Viking Landers. The team planned and executed science campaign lasting approximately 100 Martian sols to study involving an enhanced cadence environmental monitoring using rover's sensors, cameras, spectrometers. Mast Camera 880‐nm optical depth reached 8.5, Rover Environmental...

10.1029/2018gl080839 article EN public-domain Geophysical Research Letters 2018-12-05

Abstract NASA’s Dragonfly mission will send a rotorcraft lander to the surface of Titan in mid-2030s. Dragonfly's science themes include investigation Titan’s prebiotic chemistry, habitability, and potential chemical biosignatures from both water-based “life as we know it” (as might occur interior mantle ocean, cryovolcanic flows, and/or impact melt deposits) “life, but not that use liquid hydrocarbons solvent (within lakes, seas, aquifers). Consideration these solvents simultaneously led...

10.3847/psj/abfdcf article EN cc-by The Planetary Science Journal 2021-07-19

Abstract The Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) spacecraft landed successfully on Mars imaged the surface to characterize surficial geology. Here we report geology subsurface structure of landing site aid in situ geophysical investigations. InSight a degraded impact crater Elysium Planitia smooth sandy, granule- pebble-rich with few rocks. Superposed craters are common eolian bedforms sparse. During landing, pulsed retrorockets modified...

10.1038/s41467-020-14679-1 article EN cc-by Nature Communications 2020-02-24

Abstract The first samples collected by the Mars 2020 mission represent units exposed on Jezero Crater floor, from potentially oldest Séítah formation outcrops to youngest rocks of heavily cratered Máaz formation. Surface investigations reveal landscape‐to‐microscopic textural, mineralogical, and geochemical evidence for igneous lithologies, some possibly emplaced as lava flows. contain major rock‐forming minerals such pyroxene, olivine, feldspar, accessory including oxides phosphates,...

10.1029/2022je007474 article EN cc-by-nc Journal of Geophysical Research Planets 2023-02-09

A dust transport scheme has been developed for a general circulation model of the Martian atmosphere. This enables radiatively active transport, with atmospheric state responding to changes in distribution via heating, as well being determined by conditions. The includes lifting, advection winds, mixing, and gravitational sedimentation. Parameterizations lifting initiated (1) near‐surface wind stress (2) convective vortices known devils are considered. Two parameterizations defined each...

10.1029/2002je001910 article EN Journal of Geophysical Research Atmospheres 2002-12-01
Edward M. Stolper M. B. Baker Megan Newcombe M. E. Schmidt A. H. Treiman and 95 more A. Cousin M. D. Dyar M. R. Fisk R. Gellert P. L. King L. A. Leshin S. Maurice S. M. McLennan M. E. Minitti G. M. Perrett Scott K. Rowland V. Sautter R. C. Wiens Osku Kemppinen Nathan Bridges J. R. Johnson David A. Cremers J. F. Bell Lauren Edgar Jack D. Farmer Austin Godber M. Wadhwa Danika Wellington Ian McEwan Claire Newman M. I. Richardson Antoine Charpentier Laurent Péret J. G. Blank Gerald Weigle Shuai Li R. E. Milliken Kevin M. Robertson V. Z. Sun Christopher S. Edwards Bethany Ehlmann Kenneth Farley Jennifer Griffes J. P. Grotzinger Hayden Miller Cedric Pilorget M. S. Rice Kirsten Siebach Katie Stack C. Brunet Victoria Hipkin Richard Léveillé Geneviève Marchand Pablo Sobrón Sánchez Laurent Favot George D. Cody A. Steele Lorenzo Flückiger David Lees Ara Nefian Mildred Martin M. Gailhanou Francès Westall Guy Israël Christophe Agard Julien Baroukh Christophe Donny Alain Gaboriaud Philippe Guillemot Vivian Lafaille Eric Lorigny Alexis Paillet R. Pérez M. Saccoccio Charles Yana Carlos Armiens‐Aparicio Javier Caride Rodríguez Isaías Carrasco Blázquez Felipe Gómez Javier Gómez‐Elvira Sebastian Hettrich Alain Lepinette Malvitte Mercedes Marín Jiménez Jesús Martínez‐Frías Javier Martín-Soler Javier Martín‐Torres Antonio Molina Jurado Luis Mora‐Sotomayor G. M. Muñoz Sara Navarro López Verónica Peinado-González Jorge Pla‐García J. A. Rodríguez‐Manfredi Julio José Romeral-Planelló Sara Alejandra Sans Fuentes Eduardo Sebastián J. Torres Roser Urqui-O'Callaghan María‐Paz Zorzano Steve Chipera

"Jake_M," the first rock analyzed by Alpha Particle X-ray Spectrometer instrument on Curiosity rover, differs substantially in chemical composition from other known martian igneous rocks: It is alkaline (>15% normative nepheline) and relatively fractionated. Jake_M compositionally similar to terrestrial mugearites, a type typically found at ocean islands continental rifts. By analogy with these comparable rocks, could have been produced extensive fractional crystallization of primary or...

10.1126/science.1239463 article EN Science 2013-09-26

Research Article| May 01, 2013 Growth and form of the mound in Gale Crater, Mars: Slope wind enhanced erosion transport Edwin S. Kite; Kite 1Geological Planetary Sciences, California Institute Technology, Pasadena, 91125, USA Search for other works by this author on: GSW Google Scholar Kevin W. Lewis; Lewis 2Department Geosciences, Princeton University, Princeton, New Jersey 08544, Michael P. Lamb; Lamb Claire E. Newman; Newman 3Ashima Research, Mark I. Richardson Author Article Information...

10.1130/g33909.1 article EN Geology 2013-03-27

In the first 100 Martian solar days (sols) of Mars Science Laboratory mission, Rover Environmental Monitoring Station (REMS) measured seasonally evolving diurnal cycles ultraviolet radiation, atmospheric pressure, air temperature, ground relative humidity, and wind within Gale Crater on Mars.As an introduction to several REMS-based articles in this issue, we provide overview design performance REMS sensors discuss our approach mitigating some difficulties encountered following landing,...

10.1002/2013je004576 article EN Journal of Geophysical Research Planets 2014-05-22
Christopher R. Webster P. R. Mahaffy Sushil K. Atreya Gregory J. Flesch K. A. Farley and 95 more Osku Kemppinen Nathan Bridges J. R. Johnson M. E. Minitti David A. Cremers J. F. Bell Lauren Edgar Jack D. Farmer Austin Godber M. Wadhwa Danika Wellington Ian McEwan Claire Newman M. I. Richardson Antoine Charpentier Laurent Péret P. L. King J. G. Blank Gerald Weigle M. E. Schmidt Shuai Li R. E. Milliken Kevin M. Robertson V. Z. Sun Michael B. Baker Christopher Edwards Bethany Ehlmann Kenneth Farley Jennifer Griffes J. P. Grotzinger Hayden Miller Megan Newcombe C. Pilorget M. S. Rice K. L. Siebach Katie Stack Edward M. Stolper C. Brunet Victoria Hipkin Richard Léveillé Geneviève Marchand Pablo Sobrón Sánchez Laurent Favot George D. Cody A. Steele Lorenzo Flückiger David Lees Ara Nefian Mildred Martin M. Gailhanou Francès Westall G. Israël Christophe Agard Julien Baroukh Christophe Donny Alain Gaboriaud Philippe Guillemot Vivian Lafaille Eric Lorigny Alexis Paillet R. Pérez M. Saccoccio Charles Yana Carlos Armiens‐Aparicio Javier Caride Rodríguez Isaías Carrasco Blázquez Felipe Gómez Javier Gómez Elvira Sebastian Hettrich Alain Lepinette Malvitte Mercedes Marín Jiménez Jesús Martínez‐Frías Javier Martín Soler Javier Martín‐Torres Antonio Molina Jurado Luis Mora‐Sotomayor G. M. Muñoz Sara Navarro López Verónica Peinado-González Jorge Pla-García J. A. Rodríguez‐Manfredi Julio José Romeral-Planelló Sara Alejandra Sans Fuentes Eduardo Sebastian Martinez J. Torres Roser Urqui-O'Callaghan María‐Paz Zorzano Steve Chipera Jean-Luc Lacour Patrick Mauchien Jean‐Baptiste Sirven H. L. K. Manning Alberto González Fairén Alexander Hayes Jonathan Joseph

By analogy with Earth, methane in the Martian atmosphere is a potential signature of ongoing or past biological activity. During decade, Earth-based telescopic observations reported "plumes" tens parts per billion by volume (ppbv), and those from Mars orbit showed localized patches, prompting speculation sources subsurface bacteria nonbiological sources. From situ measurements made Tunable Laser Spectrometer (TLS) on Curiosity using distinctive spectral pattern specific to methane, we report...

10.1126/science.1242902 article EN Science 2013-09-20
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