[en] Combining stellar occultation observations probing Pluto's atmosphere from 1988 to 2013, and models of energy balance between Pluto's surface and atmosphere, we find the preferred models are consistent with Pluto retaining a collisional atmosphere throughout its 248-year orbit. The occultation results show an increasing atmospheric pressure with time in the current epoch, a trend present only in models with a high thermal inertia and a permanent N<SUB>2</SUB> ice cap at Pluto's north rotational pole.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Olkin, C. B.; Southwest Research Institute, Boulder 80503, USA
Young, L. A.; Southwest Research Institute, Boulder 80503, USA
Borncamp, D.; Southwest Research Institute, Boulder 80503, USA
Pickles, A.; Las Cumbres Observatory Global Telescope Network, Goleta 93117, USA
Sicardy, B.; Observatoire de Paris, Meudon, France
Assafin, M.; Universidade Federal do Rio de Janeiro, Observatorio do Valongo, Rio de Janeiro, Brazil
Bianco, F. B.; Center for Cosmology and Particle Physics, New York University, NY 10003, USA
Buie, M. W.; Southwest Research Institute, Boulder 80503, USA
de Oliveira, A. Dias; Observatoire de Paris, Meudon, France
Gillon, Michaël ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Origines Cosmologiques et Astrophysiques (OrCa)
French, R. G.; Wellesley College, Wellesley, 02481, USA
Ramos Gomes, A.; Universidade Federal do Rio de Janeiro, Observatorio do Valongo, Rio de Janeiro, Brazil
Jehin, Emmanuel ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Origines Cosmologiques et Astrophysiques (OrCa)
Morales, N.; Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
Opitom, Cyrielle ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Origines Cosmologiques et Astrophysiques (OrCa)
Ortiz, J. L.; Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
Maury, A.; San Pedro de Atacama Celestial Explorations (S.P.A.C.E.), San Pedro de Atacama, Chile
Norbury, M.; Las Cumbres Observatory Global Telescope Network, Goleta 93117, USA
Braga-Ribas, F.; Observatório Nacional/MCTI, Rio de Janeiro, Brazil
Smith, R.; Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK
Wasserman, L. H.; Lowell Observatory, Flagstaff 86001, USA
Young, E. F.; Southwest Research Institute, Boulder 80503, USA
Zacharias, M.; United States Naval Observatory, Washington, DC 20392, USA
Zacharias, N.; United States Naval Observatory, Washington, DC 20392, USA)
Assafin M., et al. Precise predictions of stellar occultations by Pluto, Charon, Nix, and Hydra for 2008-2015. Astron. Astrophys. 2010, 515(A32):1-14.
Brown T.M., et al. Las cumbres observatory global telescope network. Publ. Astron. Soc. Pac. 2013, 125:1031-1055.
Dobrovolskis A.R., Harris A.W. The obliquity of Pluto. Icarus 1983, 55:231-235.
Elliot J.L., Young L.A. Analysis of stellar occultation data for planetary atmospheres. I. Model fitting, with application to Pluto. Astron. J. 1992, 103:991-1015.
Elliot J.L., et al. The prediction and observation of the 1997 July 18 stellar occultation by Triton: More evidence for distortion and increasing pressure in Triton's atmosphere. Icarus 2000, 148:347-369.
Elliot J.L., et al. The recent expansion of Pluto's atmosphere. Nature 2003, 424:165-168.
Eshleman V.R. Pluto's atmosphere: Models based on refraction, inversion, and vapor-pressure equilibrium. Icarus 1989, 80:439-443.
Lellouch E., Stansberry J., Emery J., Grundy W., Cruikshank D.P. Thermal properties of Pluto's and Charon's surfaces from Spitzer observations. Icarus 2011, 214:701-716.
Millis R.L., et al. Pluto's radius and atmosphere: Results from the entire 9 June 1988 occultation data set. Icarus 1993, 105:282-297.
Olkin C.B., et al. The thermal structure of Triton's atmosphere: Results from the 1993 and 1995 occultations. Icarus 1997, 129:178-201.
Owen, et al. Surface ices and the atmospheric composition of Pluto. Science 1993, 261:745-748.
Sicardy B., et al. Large changes in Pluto's atmosphere as revealed by recent stellar occultations. Nature 2003, 424:168-170.
Spencer J.R., Moore J.M. The influence of thermal inertia on temperatures and frost stability on Triton. Icarus 1992, 99:261-272.
Spencer J.R., Stansberry J.A., Trafton L.M., Young E.F., Binzel R.P., Croft S.K. Volatile transport, seasonal cycles, and atmospheric dynamics on Pluto. Pluto and Charon 1997, 435. Univ. of AZ Press. S.A. Stern, D.J. Tholen (Eds.).
Stansberry J.A., Lunine J.I., Hubbard W.B., Yelle R.V., Hunten D.M. Mirages and the nature of Pluto's atmosphere. Icarus 1994, 111:503-513.
Stern S.A., Trafton L. Constraints on bulk composition, seasonal variation, and global dynamics of Pluto's atmosphere. Icarus 1984, 57:231-240.
Stern S.A., et al. The New Horizons Pluto Kuiper belt mission: An overview with historical context. Space Sci. Rev. 2008, 140.
Young L.A. Pluto's Seasons: New predictions for New Horizons. Astrophys. J. 2013, 766:L22-L28.
Young E.Y., et al. Vertical structure in Pluto's atmosphere from the 2006 June 12 stellar occultation. Astron. J. 2008, 136:1757-1769.
Young L.A., et al. New Horizons: Anticipated scientific investigations at the Pluto system. Space Sci. Rev. 2008, 140:93-127.
Zalucha A., Michaels T. A 3D general circulation model for Pluto and Triton with fixed volatile abundance and simplified surface forcing. Icarus 2013, 223:819-831.