Show simple item record

Isotopes of nitrogen on Mars: Atmospheric measurements by Curiosity's mass spectrometer

dc.contributor.authorWong, Michael H.en_US
dc.contributor.authorAtreya, Sushil K.en_US
dc.contributor.authorMahaffy, Paul N.en_US
dc.contributor.authorFranz, Heather B.en_US
dc.contributor.authorMalespin, Charlesen_US
dc.contributor.authorTrainer, Melissa G.en_US
dc.contributor.authorStern, Jennifer C.en_US
dc.contributor.authorConrad, Pamela G.en_US
dc.contributor.authorManning, Heidi L. K.en_US
dc.contributor.authorPepin, Robert O.en_US
dc.contributor.authorBecker, Richard H.en_US
dc.contributor.authorMcKay, Christopher P.en_US
dc.contributor.authorOwen, Tobias C.en_US
dc.contributor.authorNavarro‐gonzález, Rafaelen_US
dc.contributor.authorJones, John H.en_US
dc.contributor.authorJakosky, Bruce M.en_US
dc.contributor.authorSteele, Andrewen_US
dc.date.accessioned2014-01-08T20:34:55Z
dc.date.available2015-02-03T16:14:40Zen_US
dc.date.issued2013-12-16en_US
dc.identifier.citationWong, Michael H.; Atreya, Sushil K.; Mahaffy, Paul N.; Franz, Heather B.; Malespin, Charles; Trainer, Melissa G.; Stern, Jennifer C.; Conrad, Pamela G.; Manning, Heidi L. K.; Pepin, Robert O.; Becker, Richard H.; McKay, Christopher P.; Owen, Tobias C.; Navarro‐gonzález, Rafael ; Jones, John H.; Jakosky, Bruce M.; Steele, Andrew (2013). "Isotopes of nitrogen on Mars: Atmospheric measurements byâ Curiosity's mass spectrometer." Geophysical Research Letters 40(23): 6033-6037.en_US
dc.identifier.issn0094-8276en_US
dc.identifier.issn1944-8007en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/102173
dc.publisherUniv. of Ariz. Pressen_US
dc.publisherWiley Periodicals, Inc.en_US
dc.subject.otherPlanetary Atmospheresen_US
dc.subject.otherMarsen_US
dc.subject.otherNitrogen Isotopesen_US
dc.subject.otherMars Meteoritesen_US
dc.titleIsotopes of nitrogen on Mars: Atmospheric measurements by Curiosity's mass spectrometeren_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeological Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/102173/1/wong_readme.pdf
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/102173/2/wong2013_SM_v4b.pdf
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/102173/3/grl51166.pdf
dc.identifier.doi10.1002/2013GL057840en_US
dc.identifier.sourceGeophysical Research Lettersen_US
dc.identifier.citedreferenceNavarro‐González, R., et al. ( 2013 ), Possible detection of nitrates on Mars by the Sample Analysis at Mars (SAM) instrument, LPI Contrib., 1719, 2648.en_US
dc.identifier.citedreferenceFanale, F. P., W. B. Banerdt, R. S. Saunders, L. A. Johansen, and J. R. Salvail ( 1982 ), Seasonal carbon dioxide exchange between the regolith and atmosphere of Mars: Experimental and theoretical studies, J. Geophys. Res., 87, 10,215 – 10,225.en_US
dc.identifier.citedreferenceFox, J. L., and A. Hać ( 1997 ), The 15 N/ 14 N isotope fractionation in dissociative recombination of N 2 +, J. Geophys. Res., 102, 9191 – 9204.en_US
dc.identifier.citedreferenceFox, J. L., and A. Dalgarno ( 1983 ), Nitrogen escape from Mars, J. Geophys. Res., 88, 9027 – 9032.en_US
dc.identifier.citedreferenceFenton, L. K., P. E. Geissler, and R. M. Haberle ( 2007 ), Global warming and climate forcing by recent albedo changes on Mars, Nature, 446, 646 – 649.en_US
dc.identifier.citedreferenceGrotzinger, J. P., et al. ( 2012 ), Mars Science Laboratory mission and science investigation, Space Sci. Rev., 170, 5 – 56.en_US
dc.identifier.citedreferenceHoffman, J. H., R. R. Hodges, M. B. McElroy, T. M. Donahue, and M. Kolpin ( 1979 ), Composition and structure of the Venus atmosphere—Results from Pioneer Venus, Science, 205, 49 – 52.en_US
dc.identifier.citedreferenceJakosky, B. M. ( 1991 ), Mars volatile evolution: Evidence from stable isotopes, Icarus, 94, 14 – 31.en_US
dc.identifier.citedreferenceJakosky, B. M., and R. J. Phillips ( 2001 ), Mars' volatile and climate history, Nature, 412, 237 – 244.en_US
dc.identifier.citedreferenceJakosky, B. M., R. O. Pepin, R. E. Johnson, and J. L. Fox ( 1994 ), Mars atmospheric loss and isotopic fractionation by solar‐wind‐induced sputtering and photochemical escape, Icarus, 111, 271 – 288.en_US
dc.identifier.citedreferenceMahaffy, P. R., et al. ( 2012 ), The sample analysis at Mars investigation and instrument suite, Space Sci. Rev., 170, 401 – 478.en_US
dc.identifier.citedreferenceMahaffy, P. R., et al. ( 2013 ), Abundance and isotopic composition of gases in the Martian atmosphere from the Curiosity rover, Science, 341 ( 263 ), 263 – 266.en_US
dc.identifier.citedreferenceMalin, M. C., M. A. Caplinger, and S. D. Davis ( 2001 ), Observational evidence for an active surface reservoir of solid carbon dioxide on Mars, Science, 294, 2146 – 2148.en_US
dc.identifier.citedreferenceManning, C. V., C. P. McKay, and K. J. Zahnle ( 2008 ), The nitrogen cycle on Mars: Impact decomposition of near‐surface nitrates as a source for a nitrogen steady state, Icarus, 197, 60 – 64.en_US
dc.identifier.citedreferenceMarti, K., and K. J. Mathew ( 2000 ), Ancient Martian nitrogen, Geophys. Res. Lett., 27, 1463 – 1466.en_US
dc.identifier.citedreferenceMarti, K., J. S. Kim, A. N. Thakur, T. J. McCoy, and K. Keil ( 1995 ), Signatures of the Martian atmosphere in glass of the Zagami meteorite, Science, 267, 1981 – 1984.en_US
dc.identifier.citedreferenceMarty, B., M. Chaussidon, R. C. Wiens, A. J. G. Jurewicz, and D. S. Burnett ( 2011 ), A 15 N‐poor isotopic composition for the solar system as shown by Genesis solar wind samples, Science, 332, 1533 – 1536.en_US
dc.identifier.citedreferenceMcElroy, M. B., Y. L. Yung, and A. O. Nier ( 1976 ), Isotopic composition of nitrogen: Implications for the past history of Mars atmosphere, Science, 194, 70 – 72.en_US
dc.identifier.citedreferenceNier, A. O., and M. B. McElroy ( 1977 ), Composition and structure of Mars' upper atmosphere: Results from the neutral mass spectrometers on Viking 1 and 2, J. Geophys. Res., 82, 4341 – 4349.en_US
dc.identifier.citedreferenceNiemann, H. B., et al. ( 2005 ), The abundances of constituents of Titan's atmosphere from the GCMS instrument on the Huygens probe, Nature, 438, 779 – 784.en_US
dc.identifier.citedreferenceNyquist, L. E., D. D. Bogard, C.‐Y. Shih, A. Greshake, D. Stöffler, and O. Eugster ( 2001 ), Ages and geologic histories of Martian meteorites, Space Sci. Rev., 96, 105 – 164.en_US
dc.identifier.citedreferenceOwen, T. C. ( 1992 ), The composition and early history of the atmosphere of Mars, in Mars, edited by H. H. Kieffer et al., pp. 818 – 834, Univ. of Ariz. Press, Tucson, Ariz.en_US
dc.identifier.citedreferenceOwen, T., K. Biemann, D. R. Rushneck, J. E. Biller, D. W. Howarth, and A. L. Lafleur ( 1977 ), The composition of the atmosphere at the surface of Mars, J. Geophys. Res., 82, 4635 – 4639.en_US
dc.identifier.citedreferenceOwen, T., P. R. Mahaffy, H. B. Niemann, S. Atreya, and M. H. Wong ( 2001 ), Protosolar nitrogen, Astrophys. J., 553, L77 – L79.en_US
dc.identifier.citedreferenceOyama, V. I., and B. J. Berdahl ( 1977 ), The Viking gas exchange experiment results from Chryse and Utopia surface samples, J. Geophys. Res., 82, 4669 – 4676.en_US
dc.identifier.citedreferenceSchwenzer, S. P., S. Herrmann, R. K. Mohapatra, and U. Ott ( 2007 ), Noble gases in mineral separates from three shergottites: Shergotty, Zagami, and EETA79001, Meteorit. Planet. Sci., 42, 387 – 412.en_US
dc.identifier.citedreferenceStern, J. C., et al. ( 2013 ), Detection of reduced nitrogen compounds at rocknest using the Sample Analysis at Mars (SAM) instrument on the Mars Science Laboratory (MSL), LPI Contrib., 1719, 2790.en_US
dc.identifier.citedreferenceTrainer, M. G., et al. ( 2013 ), Change in the 40 Ar/N of the Mars Atmosphere from Viking to MSL: A possible indication of climate change on Mars, presented at 2013 Fall Meeting, P31C‐03, AGU, San Francisco, Calif.en_US
dc.identifier.citedreferenceWebster, C. R. et al. ( 2013 ), Isotope ratios of H, C, and O in CO 2 and H 2 O of the Martian atmosphere, Science, 341, 260 – 263.en_US
dc.identifier.citedreferenceWiens, R. C., R. H. Becker, and R. O. Pepin ( 1986 ), The case for a Martian origin of the shergottites. II. Trapped and indigenous gas components in EETA 79001 glass, Earth Planet. Sci. Lett., 77, 149 – 158.en_US
dc.identifier.citedreferenceWong, M. H., P. R. Mahaffy, S. K. Atreya, H. B. Niemann, and T. C. Owen ( 2004 ), Updated Galileo probe mass spectrometer measurements of carbon, oxygen, nitrogen, and sulfur on Jupiter, Icarus, 171, 153 – 170.en_US
dc.identifier.citedreferenceWong, M. H., et al. ( 2013 ), MSL/SAM measurements of nitrogen and argon isotopes in the Mars atmosphere, LPI Contrib., 1719, 1712. LPSC E‐Poster at http://www.lpi.usra.edu/meetings/lpsc2013/eposter/1712.pdf.en_US
dc.identifier.citedreferenceYork, D., N. M. Evensen, and M. L. Martínez ( 2004 ), Unified equations for the slope, intercept, and standard errors of the best straight line, Am. J. Phys., 72, 367 – 375.en_US
dc.identifier.citedreferenceZent, A. P., R. C. Quinn, and B. M. Jakosky ( 1994 ), Fractionation of nitrogen isotopes on Mars: The role of the regolith as a buffer, Icarus, 112, 537 – 540.en_US
dc.identifier.citedreferenceAtreya, S. K., S. W. Squyres, P. R. Mahaffy, L. A. Leshin, H. B. Franz, M. G. Trainer, M. H. Wong, C. P. McKay, R. Navarro‐González, and MSL Science Team ( 2013 ), MSL/SAM measurements of non‐condensable volatiles in the atmosphere of Mars—Possibility of seasonal variations, LPI Contrib., 1719, 2130.en_US
dc.identifier.citedreferenceAvice, G. ( 2012 ), Analyse géochimique d'une nouvelle météorite martienne: Tissint, Master's thesis, École Nationale Supérieure de Géologie, Vandœuvre‐lès‐Nancy, France.en_US
dc.identifier.citedreferenceBallou, E. V., P. C. Wood, T. Wydeven, M. E. Lehwalt, and R. E. Mack ( 1978 ), Chemical interpretation of Viking Lander 1 life detection experiment, Nature, 271, 644 – 645.en_US
dc.identifier.citedreferenceBecker, R. H., and R. O. Pepin ( 1984 ), The case for a Martian origin of the shergottites—Nitrogen and noble gases in EETA 79001, Earth Planet. Sci. Lett., 69, 225 – 242.en_US
dc.identifier.citedreferenceBogard, D. D., and P. Johnson ( 1983 ), Martian gases in an Antarctic meteorite?, Science, 221, 651 – 654.en_US
dc.identifier.citedreferenceChassefière, E., and F. Leblanc ( 2004 ), Mars atmospheric escape and evolution; interaction with the solar wind, Planet. Space Sci., 52, 1039 – 1058.en_US
dc.identifier.citedreferenceChennaoui Aoudjehane, H., et al. ( 2012 ), Tissint Martian meteorite: A fresh look at the interior, surface, and atmosphere of Mars, Science, 338, 785 – 788.en_US
dc.identifier.citedreferenceCoplen, T. B., et al. ( 2002 ), Isotope‐abundance variations of selected elements (IUPAC technical report), Pure Appl. Chem., 74, 1987 – 2017.en_US
dc.identifier.citedreferenceDahmen, G., T. L. Wilson, and F. Matteucci ( 1995 ), The nitrogen isotope abundance in the galaxy. 1: The galactic disk gradient, Astron. Astrophys., 295, 194 – 198.en_US
dc.identifier.citedreferenceFanale, F. P., and B. M. Jakosky ( 1982 ), Regolith‐atmosphere exchange of water and carbon dioxide on Mars—Effects on atmospheric history and climate change, Planet. Space Sci., 30, 819 – 831.en_US
dc.identifier.citedreferenceFanale, F. P., S. E. Postawko, J. B. Pollack, M. H. Carr, and R. O. Pepin ( 1992 ), Mars—Epochal climate change and volatile history, in Mars, edited by H. H. Kieffer et al., pp. 1135 – 1179, Univ. of Ariz. Press, Tucson, Ariz.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.