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Featured researches published by Amanda Zangari.


The Astronomical Journal | 2013

The 2011 June 23 stellar occultation by Pluto: Airborne and ground observations

Edward W. Dunham; Amanda Bosh; Stephen E. Levine; Amanda A. S. Gulbis; Amanda Zangari; Carlos Zuluaga; Jay M. Pasachoff; B. A. Babcock; S. Pandey; D. Amrhein; S. Sallum; D. J. Tholen; P. Collins; T. Bida; B. Taylor; Leonard P. Bright; Jürgen Wolf; A. W. Meyer; E. Pfueller; M. Wiedemann; H.-P. Roeser; R. Lucas; M. Kakkala; J. Ciotti; S. Plunkett; N. Hiraoka; William M. J. Best; E. J. Pilger; Marco Micheli; A. Springmann

On 2011 June 23, stellar occultations by both Pluto (this work) and Charon (future analysis) were observed from numerous ground stations as well as the Stratospheric Observatory for Infrared Astronomy (SOFIA). This first airborne occultation observation since 1995 with the Kuiper Airborne Observatory resulted in the best occultation chords recorded for the event, in three visible wavelength bands. The data obtained from SOFIA are combined with chords obtained from the ground at the IRTF, the U.S. Naval Observatory Flagstaff Station, and Leeward Community College to give the detailed state of the Pluto-Charon system at the time of the event with a focus on Plutos atmosphere. The data show a return to the distinct upper and lower atmospheric regions with a knee or kink in the light curve separating them as was observed in 1988, rather than the smoothly transitioning bowl-shaped light curves of recent years. The upper atmosphere is analyzed by fitting a model to all of the light curves, resulting in a half-light radius of 1288 ± 1 km. The lower atmosphere is analyzed using two different methods to provide results under the differing assumptions of particulate haze and a strong thermal gradient as causes for the lower atmospheric diminution of flux. These results are compared with those from past occultations to provide a picture of Plutos evolving atmosphere. Regardless of which lower atmospheric structure is assumed, results indicate that this part of the atmosphere evolves on short timescales with results changing the light curve structures between 1988 and 2006, and then reverting these changes in 2011 though at significantly higher pressures. Throughout these changes, the upper atmosphere remains remarkably stable in structure, again except for the overall pressure changes. No evidence of onset of atmospheric collapse predicted by frost migration models is seen, and the atmosphere appears to be remaining at a stable pressure level, suggesting it should persist at this full level through New Horizons flyby in 2015.


Icarus | 2015

29 November 2011 stellar occultation by 2060 Chiron: Symmetric jet-like features

Jessica D. Ruprecht; Amanda Bosh; Federica B. Bianco; Benjamin J. Fulton; Amanda A. S. Gulbis; Schelte John Bus; Amanda Zangari


Icarus | 2015

The state of Pluto’s atmosphere in 2012–2013☆☆☆☆☆☆

Amanda Bosh; Stephen E. Levine; Carlos Zuluaga; Amanda Zangari; Amanda A. S. Gulbis; G.H. Schaefer; Edward W. Dunham; B. A. Babcock; A.B. Davis; Jay M. Pasachoff; P. Rojo; Elise Servajean; F. Förster; T. Oswalt; Daniel P. Batcheldor; D. Bell; P. Bird; D. Fey; T. Fulwider; E. Geisert; D. Hastings; C. Keuhler; T. Mizusawa; P. Solenski; B. Watson


Icarus | 2015

A meta-analysis of coordinate systems and bibliography of their use on Pluto from Charon’s discovery to the present day

Amanda Zangari


Archive | 2010

Pluto's Atmosphere from the July 2010 Stellar Occultation

Michael James Person; James L. Elliot; Amanda Bosh; Amanda A. S. Gulbis; Rebecca M. Jensen-Clem; Melissa Fitch Lockhart; Amanda Zangari; Carlos Zuluaga; Stephen E. Levine; Jay M. Pasachoff; S. P. Souza; Min-Hao Lu; C. Malamut; Patricio Michel Rojo; Charles D. Bailyn; Rachel K. D. MacDonald; Kevin Ivarsen; Daniel E. Reichart; Aaron Patrick Lacluyze; Melissa C. Nysewander; Joshua B. Haislip


Archive | 2011

Constraints On The Size Of KBO (50000) Quaoar From A Single-chord Stellar Occultation

Michael James Person; James L. Elliot; Amanda Bosh; Amanda Zangari; Carlos Zuluaga; Stephanie Sallum; Stephen E. Levine; Leonard P. Bright; Scott S. Sheppard; Trudy Tilleman


Archive | 2010

Size and Albedo of the Kuiper Belt Object 55636

James L. Elliot; Michael James Person; Carlos Zuluaga; Amanda Bosh; Elisabeth R. Adams; Amanda A. S. Gulbis; Stephen E. Levine; Melissa Fitch Lockhart; Amanda Zangari; Bruce A. Babcock; K. M. DuPre; Jay M. Pasachoff; S. P. Souza; Wayne Rosing; N. Secrest


American Astronomical Society | 2013

THE 2011 JUNE 23 STELLAR OCCULTATION BY PLUTO: AIRBORNE AND GROUND OBSERVATIONS

Amanda Bosh; Stephen E. Levine; Amanda A. S. Gulbis; Amanda Zangari; Carlos Zuluaga; Stephanie Sallum; A. Springmann


Archive | 2011

First Small-Body Occultation Attempts from the Stratospheric Observatory for Infrared Astronomy

E W Dunham; T Bida; A S Bosh; P Collins; S E Levine; G Mandushev; B Taylor; T Tilleman; Amanda Zangari


Archive | 2011

A Search for Satellites of Kuiper Belt Object 55636 from the 2009 October 9 Occultation

Rebecca M. Jensen-Clem; James L. Elliot; Michael James Person; Carlos Zuluaga; Amanda Bosh; Elisabeth R. Adams; Amanda A. S. Gulbis; Stephen E. Levine; Melissa Fitch Lockhart; Amanda Zangari; Bruce A. Babcock; K. M. DuPre; Jay M. Pasachoff; S. P. Souza; Wayne Rosing; N. Secrest; Leonard P. Bright; Edward W. Dunham; M. Kakkala; Trudy Tilleman; Stanley I. Rapoport; L. Zambrano-Marin; Jürgen Wolf; Katie M. Morzinski

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Amanda Bosh

Massachusetts Institute of Technology

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Carlos Zuluaga

Massachusetts Institute of Technology

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Amanda A. S. Gulbis

Massachusetts Institute of Technology

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Michael James Person

Massachusetts Institute of Technology

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Melissa Fitch Lockhart

Massachusetts Institute of Technology

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