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Haze in Pluto's atmosphere: Results from SOFIA and ground-based observations of the 2015 June 29 Pluto occultation

Person, Michael J. and Pasachoff, Jay M. (2019) Haze in Pluto's atmosphere: Results from SOFIA and ground-based observations of the 2015 June 29 Pluto occultation. Icarus . ISSN 0019-1035. (In Press) https://resolver.caltech.edu/CaltechAUTHORS:20191202-094234104

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Abstract

On UT 29 June 2015, the occultation by Pluto of a bright star (r′ = 11.9) was observed from the Stratospheric Observatory for Infrared Astronomy (SOFIA) and several ground-based stations in New Zealand and Australia. Pre-event astrometry allowed for an in-flight update to the SOFIA team with the result that SOFIA was deep within the central flash zone (~22 km from center). Analysis of the combined data leads to the result that Pluto's middle atmosphere is essentially unchanged from 2011 and 2013 (Person et al. 2013; Bosh et al. 2015); there has been no significant expansion or contraction of the atmosphere. Additionally, our multi-wavelength observations allow us to conclude that a haze component in the atmosphere is required to reproduce the light curves obtained. This haze scenario has implications for understanding the photochemistry of Pluto's atmosphere.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1016/j.icarus.2019.113572DOIArticle
ORCID:
AuthorORCID
Pasachoff, Jay M.0000-0002-4372-4928
Additional Information:© 2019 Published by Elsevier Inc. Received 22 October 2019, Accepted 21 November 2019, Available online 30 November 2019. These critical observations with SOFIA would not have been possible if not for more than 30 years of tireless work and genius by the late Professor Dr. Hans-Peter Röser of the University of Stuttgart and by the late SOFIA Chief Engineer Mr. Nans Kunz of the NASA Ames Research Center. The SOFIA portion of these observations would not have occurred without the scientific and management support of then SMO Deputy Director of Science William Reach and then SMO Director Erick Young. We also thank NASA SOFIA Program Manager Eddie Zavala and the entire SOFIA team for their support. We thank Dick French, Georgi Mandushev, Tom Allen, Lauren Biddle, Lisa Prato, and Gail Schaefer for assistance during the prediction phase of this project. JVC would like to thank Ken Bower—“for teaching me the general art of flight planning, and doing an amazing job absorbing the peculiarities of occultation flight planning in two long days before the check flight”; and Navigator Jeff “Elvis” Wilson for smoothly translating our needs into “pilot-speak” with a former bombardier's flair. The FPI+ team thanks Karsten Schindler of DSI for his ground-based observations of the star field prior to the event, allowing accurate planning of the FPI+ settings. This work is based, in part, on observations made with the NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA). SOFIA is jointly operated by the Universities Space Research Association, Inc. (USRA), under NASA contract NAS2-97001, and the Deutsches SOFIA Institut (DSI) under DLR contract 50 OK 0901 to the University of Stuttgart. Additional financial support for this work was provided by NASA through award #SOF 03-0028 issued by USRA. Data were acquired using the Mt. John Observatory Optical Craftsman 61 cm telescope, operated by the AAVSO and the University of Canterbury. We are grateful to Nigel Frost and Arne Henden for support at MJO, and to H. Roe for the loan of his near IR camera (Xeva-CL). Some of the data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. Laird Close, Katie Morzinski, and Jared Males graciously helped with observations. Support for this work was provided by NASA SSO grants NNX15AJ82G to Lowell Observatory, NNX10AB27G to MIT, and NNX12AJ29G to Williams College. AAS acknowledges support from the National Research Foundation of South Africa.
Funders:
Funding AgencyGrant Number
NASANAS2-97001
Deutsches Zentrum für Luft- und Raumfahrt (DLR)50 OK 0901
Universities Space Research Association (USRA)SOF 03-0028
W. M. Keck FoundationUNSPECIFIED
NASANNX15AJ82G
NASANNX10AB27G
NASANNX12AJ29G
National Research Foundation (South Africa)UNSPECIFIED
Subject Keywords:Pluto; Atmosphere; Atmospheres; Structure; Occultations
Record Number:CaltechAUTHORS:20191202-094234104
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191202-094234104
Official Citation:Michael J. Person, Amanda S. Bosh, Carlos A. Zuluaga, Amanda A. Sickafoose, Stephen E. Levine, Jay M. Pasachoff, Bryce A. Babcock, Edward W. Dunham, Ian S. McLean, Jürgen Wolf, Fumio Abe, E.E. Becklin, Thomas A. Bida, Len P. Bright, Tim Brothers, Grant Christie, Rebecca F. Durst, Alan C. Gilmore, Ryan T. Hamilton, Hugh C. Harris, Chris Johnson, Pamela M. Kilmartin, Molly Kosiarek, Karina Leppik, Sarah E. Logsdon, Robert Lucas, Shevill Mathers, C.J.K. Morley, Peter Nelson, Haydn Ngan, Enrico Pfüller, Tim Natusch, Stephanie Sallum, Maureen L. Savage, Christina H. Seeger, Ho Chit Siu, Chris Stockdale, Daisuke Suzuki, Thanawuth Thanathibodee, Trudy Tilleman, Paul J. Tristram, William D. Vacca, Jeffrey Van Cleve, Carolle Varughese, Luke W. Weisenbach, Elizabeth Widen, Manuel Wiedemann, Haze in Pluto's atmosphere: Results from SOFIA and ground-based observations of the 2015 June 29 Pluto occultation, Icarus, 2019, 113572, ISSN 0019-1035, https://doi.org/10.1016/j.icarus.2019.113572. (http://www.sciencedirect.com/science/article/pii/S0019103519307377)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:100134
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:02 Dec 2019 17:53
Last Modified:02 Dec 2019 17:53

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