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Diviner Lunar Radiometer Observations of Cold Traps in the Moon's South Polar Region

SCIENCE 330:6003 (2010) 479-482

Authors:

David A Paige, Matthew A Siegler, Jo Ann Zhang, Paul O Hayne, Emily J Foote, Kristen A Bennett, Ashwin R Vasavada, Benjamin T Greenhagen, John T Schofield, Daniel J McCleese, Marc C Foote, Eric DeJong, Bruce G Bills, Wayne Hartford, Bruce C Murray, Carlton C Allen, Kelly Snook, Laurence A Soderblom, Simon Calcutt, Fredric W Taylor, Neil E Bowles, Joshua L Bandfield, Richard Elphic, Rebecca Ghent, Timothy D Glotch, Michael B Wyatt, Paul G Lucey
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Element cycling and the evolution of the Earth System

GEOCHIMICA ET COSMOCHIMICA ACTA 74:12 (2010) A339-A339

Authors:

Y Godderis, Y Donnadieu, JZ Williams, C Roelandt, J Schott, D Pollard, RT Pierrehumbert, S Brantley
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Global Silicate Mineralogy of the Moon from the Diviner Lunar Radiometer

SCIENCE 329:5998 (2010) 1507-1509

Authors:

Benjamin T Greenhagen, Paul G Lucey, Michael B Wyatt, Timothy D Glotch, Carlton C Allen, Jessica A Arnold, Joshua L Bandfield, Neil E Bowles, Kerri L Donaldson Hanna, Paul O Hayne, Eugenie Song, Ian R Thomas, David A Paige
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Mapping Titan's HCN in the far infra-red: implications for photochemistry.

Faraday Discuss 147 (2010) 51-64

Authors:

NA Teanby, PGJ Irwin, R de Kok, CA Nixon

Abstract:

Observations of Titan's far infra-red spectra by the Cassini orbiter's Composite InfraRed Spectrometer have been used to determine the latitude distribution of HCN at 1 mbar by fitting the HCN and CO rotational lines in the 18-60 cm(-1) (160-550 microm) spectral range. Results confirm the north polar HCN enrichment previously observed using mid-IR data and support the conclusion that Titan's nitrile species are significantly more enriched than hydrocarbons species with similar predicted photochemical lifetimes. This suggests Titan's photochemical cycle includes an additional sink for nitrogen bearing species. The abundance of CO was also determined, and had a mean value of 55 +/- 6 ppm at 20 mbar. However, it was not possible to reliably determine the CO latitude variation due to unconstrained temperatures in the north polar lower stratosphere.
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Martian atmosphere as observed by VIRTIS-M on Rosetta spacecraft

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 115 (2010) ARTN E04004

Authors:

A Coradini, D Grassi, F Capaccioni, G Filacchione, F Tosi, E Ammannito, MC De Sanctis, V Formisano, P Wolkenberg, G Rinaldi, G Arnold, MA Barucci, G Bellucci, J Benkhoff, JP Bibring, A Blanco, D Bockelee-Morvan, MT Capria, R Carlson, U Carsenty, P Cerroni, L Colangeli, M Combes, M Combi, J Crovisier, P Drossart, T Encrenaz, S Erard, C Federico, U Fink, S Fonti, W-H Ip, PGJ Irwin, R Jaumann, E Kuehrt, Y Langevin, G Magni, T McCord, V Mennella, S Mottola, G Neukum, V Orofino, P Palumbo, G Piccioni, H Rauer, B Schmitt, D Tiphene, FW Taylor, GP Tozzi
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