Publicación:
Lower atmosphere and pressure evolution on Pluto from ground-based stellar occultations, 1988-2016

dc.contributor.author Meza, E es_PE
dc.contributor.author Sicardy, B es_PE
dc.contributor.author Assafin, M es_PE
dc.contributor.author Ortiz, JL es_PE
dc.contributor.author Bertrand, T es_PE
dc.contributor.author Lellouch, E es_PE
dc.contributor.author Desmars, J es_PE
dc.contributor.author Forget, F es_PE
dc.contributor.author Berard, D es_PE
dc.contributor.author Doressoundiram, A es_PE
dc.contributor.author Lecacheux, J es_PE
dc.contributor.author Gil-Hutton, R es_PE
dc.contributor.author Dhillon, V es_PE
dc.contributor.author Bendjoya, P es_PE
dc.contributor.author Littlefair, S es_PE
dc.contributor.author Marsh, T es_PE
dc.contributor.author Veillet, C es_PE
dc.contributor.author Bath, KL es_PE
dc.contributor.author Beisker, W es_PE
dc.contributor.author Bode, HJ es_PE
dc.contributor.author Kretlow, M es_PE
dc.contributor.author Guhl, K es_PE
dc.contributor.author Herald, D es_PE
dc.contributor.author Gault, D es_PE
dc.contributor.author Kerr, S es_PE
dc.contributor.author Rivet, JP es_PE
dc.contributor.author Pavlov, H es_PE
dc.contributor.author Farago, O es_PE
dc.contributor.author Klos, O es_PE
dc.contributor.author Frappa, E es_PE
dc.contributor.author Lavayssiere, M es_PE
dc.contributor.author Cole, AA es_PE
dc.contributor.author Rothe, W es_PE
dc.contributor.author Giles, AB es_PE
dc.contributor.author Greenhill, JG es_PE
dc.contributor.author Hill, KM es_PE
dc.contributor.author Buie, MW es_PE
dc.contributor.author Vernet, D es_PE
dc.contributor.author Olkin, CB es_PE
dc.contributor.author Young, EF es_PE
dc.contributor.author Young, LA es_PE
dc.contributor.author Wasserman, LH es_PE
dc.contributor.author Devogele, M es_PE
dc.contributor.author Roques, F es_PE
dc.contributor.author French, RG es_PE
dc.contributor.author Bianco, FB es_PE
dc.contributor.author Marchis, F es_PE
dc.contributor.author Brosch, N es_PE
dc.contributor.author Kaspi, S es_PE
dc.contributor.author Di Fabrizio, L es_PE
dc.contributor.author Polishook, D es_PE
dc.contributor.author Manulis, I es_PE
dc.contributor.author Larbi, MAM es_PE
dc.contributor.author Benkhaldoun, Z es_PE
dc.contributor.author Walzel, K es_PE
dc.contributor.author Daassou, A es_PE
dc.contributor.author El Azhari, Y es_PE
dc.contributor.author Moulane, Y es_PE
dc.contributor.author Broughton, J es_PE
dc.contributor.author Milner, J es_PE
dc.contributor.author Dobosz, T es_PE
dc.contributor.author Lorenzi, V es_PE
dc.contributor.author Bolt, G es_PE
dc.contributor.author Lade, B es_PE
dc.contributor.author Gilmore, A es_PE
dc.contributor.author Wortmann, G es_PE
dc.contributor.author Kilmartin, P es_PE
dc.contributor.author Allen, WH es_PE
dc.contributor.author Graham, PB es_PE
dc.contributor.author Loader, B es_PE
dc.contributor.author McKay, G es_PE
dc.contributor.author Talbot, J es_PE
dc.contributor.author Parker, S es_PE
dc.contributor.author Magazzu, A es_PE
dc.contributor.author Molinari, E es_PE
dc.contributor.author Gazeas, K es_PE
dc.contributor.author Eberle, A es_PE
dc.contributor.author Tzouganatos, L es_PE
dc.contributor.author Oliveira, JM es_PE
dc.contributor.author Carbognani, A es_PE
dc.contributor.author Bonnoli, G es_PE
dc.contributor.author Marchini, A es_PE
dc.contributor.author Leto, G es_PE
dc.contributor.author Sanchez, RZ es_PE
dc.contributor.author Mancini, L es_PE
dc.contributor.author Kattentidt, B es_PE
dc.contributor.author Dohrmann, M es_PE
dc.contributor.author Hampf, D es_PE
dc.contributor.author Ohlert, J es_PE
dc.contributor.author Krannich, G es_PE
dc.contributor.author Murawsky, G es_PE
dc.contributor.author Jelinek, M es_PE
dc.contributor.author Gahrken, B es_PE
dc.contributor.author Gloistein, D es_PE
dc.contributor.author Alonso, S es_PE
dc.contributor.author Widemann, T es_PE
dc.contributor.author Roman, A es_PE
dc.contributor.author Communal, JE es_PE
dc.contributor.author Jabet, F es_PE
dc.contributor.author deVisscher, S es_PE
dc.contributor.author Serot, J es_PE
dc.contributor.author Janik, T es_PE
dc.contributor.author Cunniffe, R es_PE
dc.contributor.author Moravec, Z es_PE
dc.contributor.author Machado, P es_PE
dc.contributor.author Selva, A es_PE
dc.contributor.author Perello, C es_PE
dc.contributor.author Colas, F es_PE
dc.contributor.author Rovira, J es_PE
dc.contributor.author Conti, M es_PE
dc.contributor.author Papini, R es_PE
dc.contributor.author Salvaggio, F es_PE
dc.contributor.author Noschese, A es_PE
dc.contributor.author Querel, R es_PE
dc.contributor.author Tsamis, V es_PE
dc.contributor.author Tigani, K es_PE
dc.contributor.author Barroy, P es_PE
dc.contributor.author Irzyk, M es_PE
dc.contributor.author Neel, D es_PE
dc.contributor.author Vachier, F es_PE
dc.contributor.author Godard, JP es_PE
dc.contributor.author Lanoiselee, D es_PE
dc.contributor.author Sogorb, P es_PE
dc.contributor.author Verilhac, D es_PE
dc.contributor.author Harnisch, M es_PE
dc.contributor.author Bretton, M es_PE
dc.contributor.author Signoret, F es_PE
dc.contributor.author Ciabattari, F es_PE
dc.contributor.author Naves, R es_PE
dc.contributor.author Boutet, M es_PE
dc.contributor.author De Queiroz, J es_PE
dc.contributor.author Renner, S es_PE
dc.contributor.author Lindner, P es_PE
dc.contributor.author Lindner, K es_PE
dc.contributor.author Enskonatus, P es_PE
dc.contributor.author Jansen, R es_PE
dc.contributor.author Dangl, G es_PE
dc.contributor.author Tordai, T es_PE
dc.contributor.author Eichler, H es_PE
dc.contributor.author Hattenbach, J es_PE
dc.contributor.author Peterson, C es_PE
dc.contributor.author Molnar, LA es_PE
dc.contributor.author Howell, RR es_PE
dc.contributor.author Leiva, R es_PE
dc.contributor.author Braga-Ribas, F es_PE
dc.contributor.author Benedetti-Rossi, G es_PE
dc.contributor.author Pennell, A es_PE
dc.contributor.author Camargo, JIB es_PE
dc.contributor.author Dias-Oliveira, A es_PE
dc.contributor.author Morgado, B es_PE
dc.contributor.author Gomes, AR es_PE
dc.contributor.author Vieira-Martins, R es_PE
dc.contributor.author Behrend, R es_PE
dc.contributor.author Tirado, AC es_PE
dc.contributor.author Duffard, R es_PE
dc.contributor.author Morales, N es_PE
dc.contributor.author Santos-Sanz, P es_PE
dc.contributor.author Todd, S es_PE
dc.contributor.author Ivanov, VD es_PE
dc.contributor.author Opitom, C es_PE
dc.contributor.author Gillon, M es_PE
dc.contributor.author Abe, L es_PE
dc.contributor.author Jehin, E es_PE
dc.contributor.author Manfroid, J es_PE
dc.contributor.author Pollock, J es_PE
dc.contributor.author Reichart, DE es_PE
dc.contributor.author Haislip, JB es_PE
dc.contributor.author Ivarsen, KM es_PE
dc.contributor.author LaCluyze, AP es_PE
dc.contributor.author Maury, A es_PE
dc.date.accessioned 2024-05-30T23:13:38Z
dc.date.available 2024-05-30T23:13:38Z
dc.date.issued 2019
dc.description This article is dedicated to the memory of H.-J. Bode, J. G. Greenhill and O. Faragó for their long-standing support and participation to occultation campaigns. The work leading to these results has received funding from the European Research Council under the European Community’s H2020 2014-2020 ERC Grant Agreement n° 669416 “Lucky Star”. E.M. thanks support from Concytec-Fondecyt-PE and GA, FC-UNI for providing support during the 2012 July 18 occultation.
dc.description.abstract Context. The tenuous nitrogen (N2) atmosphere on Pluto undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has recently (July 2015) been observed by the New Horizons spacecraft. Aims. The main goals of this study are (i) to construct a well calibrated record of the seasonal evolution of surface pressure on Pluto and (ii) to constrain the structure of the lower atmosphere using a central flash observed in 2015. Methods. Eleven stellar occultations by Pluto observed between 2002 and 2016 are used to retrieve atmospheric profiles (density, pressure, temperature) between altitude levels of ~5 and ~380 km (i.e. pressures from ~ 10 μbar to 10 nbar). Results. (i) Pressure has suffered a monotonic increase from 1988 to 2016, that is compared to a seasonal volatile transport model, from which tight constraints on a combination of albedo and emissivity of N2 ice are derived. (ii) A central flash observed on 2015 June 29 is consistent with New Horizons REX profiles, provided that (a) large diurnal temperature variations (not expected by current models) occur over Sputnik Planitia; and/or (b) hazes with tangential optical depth of ~0.3 are present at 4–7 km altitude levels; and/or (c) the nominal REX density values are overestimated by an implausibly large factor of ~20%; and/or (d) higher terrains block part of the flash in the Charon facing hemisphere.
dc.description.sponsorship Consejo Nacional de Ciencia, Tecnología e Innovación Tecnológica - Concytec
dc.identifier.doi https://doi.org/10.1051/0004-6361/201834281
dc.identifier.isi 467559100001
dc.identifier.uri https://hdl.handle.net/20.500.12390/1008
dc.language.iso eng
dc.publisher Astronomy & Astrophysics
dc.relation.ispartof Astronomy & Astrophysics
dc.rights info:eu-repo/semantics/openAccess
dc.rights.uri https://creativecommons.org/licenses/by/4.0/
dc.subject photometric
dc.subject observational|data analysis es_PE
dc.subject atmospheres es_PE
dc.subject.ocde https://purl.org/pe-repo/ocde/ford#1.03.00
dc.title Lower atmosphere and pressure evolution on Pluto from ground-based stellar occultations, 1988-2016
dc.type info:eu-repo/semantics/article
dspace.entity.type Publication
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