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IRTF/SpeX observations of Pluto's near-infrared reflectance spectrum during 2013 show vibrational absorption features of CO and N$_2$ ices at 1.58 and 2.15 {\mu}m, respectively, that are weaker than had been observed during the preceding…

Earth and Planetary Astrophysics · Physics 2015-06-18 W. M. Grundy , C. B. Olkin , L. A. Young , B. J. Holler

The New Horizons spacecraft, which flew by Pluto on July 14, 2015, revealed the presence of haze in Pluto's atmosphere that were formed by CH4/N2 photochemistry at high altitudes in Pluto's atmosphere, as on Titan and Triton. In order to…

Earth and Planetary Astrophysics · Physics 2017-03-08 Tanguy Bertrand , François Forget

We apply scintillation theory to stellar signal fluctuations in the high-resolution, high signal/noise, dual-wavelength data from the MMT observation of the 2007 March 18 occultation of P445.3 by Pluto. A well-defined high wavenumber cutoff…

Earth and Planetary Astrophysics · Physics 2015-05-13 W. B. Hubbard , D. W. McCarthy , C. A. Kulesa , S. D. Benecchi , M. J. Person , J. L. Elliot , A. A. S. Gulbis

The surprising discovery by the Rosetta spacecraft of molecular oxygen (O$_2$) in the coma of comet 67P/Churyumov-Gerasimenko (Bieler et al. 2015) challenged our understanding of the inventory of this volatile species on and inside bodies…

Earth and Planetary Astrophysics · Physics 2017-08-02 J. A. Kammer , S. A. Stern , G. R. Gladstone , L. A. Young , C. B. Olkin , A. Steffl , H. A. Weaver , K. Ennico

The rotational lightcurves of the Pluto-Charon system were previously believed to be solely attributed to their surfaces. However, a proposed scenario of haze cooling \citep{2017Natur.551..352Z} suggests that the atmospheric haze of Pluto…

Earth and Planetary Astrophysics · Physics 2023-09-20 Linfeng Wan , Xi Zhang , Jason D. Hofgartner

Context. The equatorial region of Cthulhu as revealed by New Horizons appears to be generally dark and largely devoid of volatiles because its surface albedo is low. Localized bright patches, however, which are interpreted as CH4 frost, are…

Earth and Planetary Astrophysics · Physics 2026-01-09 L. Lange , T. Bertrand , V. Belissa , S. Capry , L. A. Young , A. Falco

The seasonal evolution of Saturn's polar atmospheric temperatures and hydrocarbon composition is derived from a decade of Cassini Composite Infrared Spectrometer (CIRS) 7-16 $\mu$m thermal infrared spectroscopy. We construct a…

A stellar occultation by Neptune's main satellite, Triton, was observed on 5 October 2017 from Europe, North Africa, and the USA. We derived 90 light curves from this event, 42 of which yielded a central flash detection. We aimed at…

Earth and Planetary Astrophysics · Physics 2022-04-20 J. Marques Oliveira , B. Sicardy , A. R. Gomes-Júnior , J. L. Ortiz , D. F. Strobel , T. Bertrand , F. Forget , E. Lellouch , J. Desmars , D. Bérard , A. Doressoundiram , J. Lecacheux , R. Leiva , E. Meza , F. Roques , D. Souami , T. Widemann , P. Santos-Sanz , N. Morales , R. Duffard , E. Fernández-Valenzuela , A. J. Castro-Tirado , F. Braga-Ribas , B. E. Morgado , M. Assafin , J. I. B. Camargo , R. Vieira-Martins , G. Benedetti-Rossi , S. Santos-Filho , M. V. Banda-Huarca , F. Quispe-Huaynasi , C. L. Pereira , F. L. Rommel , G. Margoti , A. Dias-Oliveira , F. Colas , J. Berthier , S. Renner , R. Hueso , S. Pérez-Hoyos , A. Sánchez-Lavega , J. F. Rojas , W. Beisker , M. Kretlow , D. Herald , D. Gault , K. -L. Bath , H. -J. Bode , E. Bredner , K. Guhl , T. V. Haymes , E. Hummel , B. Kattentidt , O. Klös , A. Pratt , B. Thome , C. Avdellidou , K. Gazeas , E. Karampotsiou , L. Tzouganatos , E. Kardasis , A. A. Christou , E. M. Xilouris , I. Alikakos , A. Gourzelas , A. Liakos , V. Charmandaris , M. Jelínek , J. Štrobl , A. Eberle , K. Rapp , B. Gährken , B. Klemt , S. Kowollik , R. Bitzer , M. Miller , G. Herzogenrath , D. Frangenberg , L. Brandis , I. Pütz , V. Perdelwitz , G. M. Piehler , P. Riepe , K. von Poschinger , P. Baruffetti , D. Cenadelli , J. -M. Christille , F. Ciabattari , R. Di Luca , D. Alboresi , G. Leto , R. Zanmar Sanchez , P. Bruno , G. Occhipinti , L. Morrone , L. Cupolino , A. Noschese , A. Vecchione , C. Scalia , R. Lo Savio , G. Giardina , S. Kamoun , R. Barbosa , R. Behrend , M. Spano , E. Bouchet , M. Cottier , L. Falco , S. Gallego , L. Tortorelli , S. Sposetti , J. Sussenbach , F. Van Den Abbeel , P. André , M. Llibre , F. Pailler , J. Ardissone , M. Boutet , J. Sanchez , M. Bretton , A. Cailleau , V. Pic , L. Granier , R. Chauvet , M. Conjat , J. L. Dauvergne , O. Dechambre , P. Delay , M. Delcroix , L. Rousselot , J. Ferreira , P. Machado , P. Tanga , J. -P. Rivet , E. Frappa , M. Irzyk , F. Jabet , M. Kaschinski , A. Klotz , Y. Rieugnie , A. N. Klotz , O. Labrevoir , D. Lavandier , D. Walliang , A. Leroy , S. Bouley , S. Lisciandra , J. -F. Coliac , F. Metz , D. Erpelding , P. Nougayrède , T. Midavaine , M. Miniou , S. Moindrot , P. Morel , B. Reginato , E. Reginato , J. Rudelle , B. Tregon , R. Tanguy , J. David , W. Thuillot , D. Hestroffer , G. Vaudescal , D. Baba Aissa , Z. Grigahcene , D. Briggs , S. Broadbent , P. Denyer , N. J. Haigh , N. Quinn , G. Thurston , S. J. Fossey , C. Arena , M. Jennings , J. Talbot , S. Alonso , A. Román Reche , V. Casanova , E. Briggs , R. Iglesias-Marzoa , J. Abril Ibáñez , M. C. Díaz Martín , H. González , J. L. Maestre García , J. Marchant , I. Ordonez-Etxeberria , P. Martorell , J. Salamero , F. Organero , L. Ana , F. Fonseca , V. Peris , O. Brevia , A. Selva , C. Perello , V. Cabedo , R. Gonçalves , M. Ferreira , F. Marques Dias , A. Daassou , K. Barkaoui , Z. Benkhaldoun , M. Guennoun , J. Chouqar , E. Jehin , C. Rinner , J. Lloyd , M. El Moutamid , C. Lamarche , J. T. Pollock , D. B. Caton , V. Kouprianov , B. W. Timerson , G. Blanchard , B. Payet , A. Peyrot , J. -P. Teng-Chuen-Yu , J. Françoise , B. Mondon , T. Payet , C. Boissel , M. Castets , W. B. Hubbard , R. Hill , H. J. Reitsema , O. Mousis , L. Ball , G. Neilsen , S. Hutcheon , K. Lay , P. Anderson , M. Moy , M. Jonsen , I. Pink , R. Walters , B. Downs

Relatively long-period nonsynchronized planets---such as warm Jupiters---potentially retain the primordial rotation, eccentricity, and obliquity that might encapsulate information on planetary climate and formation processes. To date, there…

Earth and Planetary Astrophysics · Physics 2019-03-20 Kazumasa Ohno , Xi Zhang

The New Horizons spacecraft will achieve a wide range of measurement objectives at the Pluto system, including color and panchromatic maps, 1.25-2.50 micron spectral images for studying surface compositions, and measurements of Pluto's…

Results are presented from a 3-D Pluto general circulation model (GCM) that includes conductive heating and cooling, non-local thermodynamic equilibrium (non-LTE) heating by methane at 2.3 and 3.3 microns, non-LTE cooling by cooling by…

Earth and Planetary Astrophysics · Physics 2016-03-29 Angela M. Zalucha

Context. During the last 30 years the surface of Pluto has been characterized, and its variability has been monitored, through continuous near-infrared spectroscopic observations. But in the visible range only few data are available. Aims.…

Earth and Planetary Astrophysics · Physics 2016-01-13 V. Lorenzi , N. Pinilla-Alonso , J. Licandro , D. P. Cruikshank , W. M. Grundy , R. P. Binzel , J. P. Emery

The presence of N2 in the surface environment of Pluto is critical in creating Pluto's richness of features and processes. Here, we propose that the nitrogen atoms in the N2 observed on Pluto were accreted in that chemical form during the…

Earth and Planetary Astrophysics · Physics 2018-05-29 Christopher R. Glein , J. Hunter Waite

The discovery of Pluto in 1930 presaged the discoveries of both the Kuiper Belt and ice dwarf planets, which are the third class of planets in our solar system. From the 1970s to the 19990s numerous fascinating attributes of the Pluto…

Earth and Planetary Astrophysics · Physics 2018-10-17 S. Alan Stern , William Grundy , William B. McKinnon , Harold A. Weaver , Leslie A. Young

We investigate the effects of varying Saturn's orbit on the atmospheric circulation and surface methane distribution of Titan. Using a new general circulation model of Titan's atmosphere, we simulate its climate under four characteristic…

Earth and Planetary Astrophysics · Physics 2014-12-30 Juan M. Lora , Jonathan I. Lunine , Joellen L. Russell , Alexander G. Hayes

Neptune's moon Triton shares many similarities with Pluto, including volatile cycles of N2, CH4 and CO, and represents a benchmark case for the study of surface-atmosphere interactions on volatile-rich KBOs. Within the context of New…

Plutinos are Kuiper-belt objects that share the 3:2 Neptune resonance with Pluto. The long-term stability of Plutino orbits depends on their eccentricity. Plutinos with eccentricities close to Pluto (fractional eccentricity difference…

Astrophysics · Physics 2009-10-31 Qingjuan Yu , Scott Tremaine

Clouds on Titan result from the condensation of methane and ethane and, as on other planets, are primarily structured by circulation of the atmosphere. At present, cloud activity mainly occurs in the southern (summer) hemisphere, arising…