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Stellar Occultation Observations to Constrain the Stratosphere of Uranus for Aerocapture Background on Uranus: Voyager 2 (V2) UV stellar and solar occultations at Uranus detected a warm stratosphere and extremely hot thermosphere [1, 2], far in excess of solar irradiance [3, 4] and internal heating [5, 6]. New theories to explain similar heating at Jupiter [7] and Saturn [8] cannot be tested at Uranus due to a dearth of reliable measurements.
In [9, 10], we reprocessed 26 archival Earth-based stellar occultations by Uranus (1977-1996), finding stratospheric temperatures (~200 K) warmer than the original (~100 K), but in stark tension with V2 (~300-500 K). In [10], we built a physics-based, 1-D atmospheric model (see Fig 1) that finds a nearly isothermal stratosphere and a dynamic heat sink in the lower thermosphere.

Aerocapture: Aerocapture is spacecraft maneuver that uses a single deep dip to enter orbit. It could decrease cruise time and launch mass for a Uranus mission, but the greatest impediment is uncertain stratospheric densities of Uranus [11].

Aims: 1) Observe and process many high S/N Uranus stellar occultations in the next decade; 2) constrain stratospheric densities for aerocapture; 3) better understand the energy balance; 4) determine stratospheric changes since 1996.

Upcoming Occultations: We will present our observing plan for the 2025 April Uranus occultation (K mag 8) and discuss the best-in-a-century 2031 event (K mag 4). We will discuss other events in the early 2030s [12] [13], predicted constraints on density, and simulations of aerocapture for UOP. We will discuss the Shadow Chaser, a small satellite concept for observing occultations from Earth orbit [12].

Conclusions: New stellar occultations can vastly improve profiles of the stratosphere of Uranus; this is critical for understanding energy circulation and constraining densities for using aerocapture on UOP.

References:

[1] Herbert, F. et al. (1987). JGR.

[2] Stevens, M. et al. (1993). Icarus.

[3] Marley, M. & McKay, C. (1999). Icarus,

[4] Li, C. et al. (2018). JQRST.

[5] Pearl, J. et al. (1990). Icarus.

[6] Melin, H (2020). Nat Astron.

[7] O’Donoghue, J. et al. (2021) Nature.

[8] Mueller-Wodarg, I. et al. (2019) GRL.

[9] Saunders, W. et al. (2023). PSJ.

[10] Saunders, W. et al. (2024). PSJ.

[11] Report of the Aerocapture Demonstration Relevance Assessment Team (2023).

[12] Saunders, W. et al. (2022). P&SS.

[13] French, R. & Souami, D. (2023) PSJ.
Document ID
20240015651
Acquisition Source
Langley Research Center
Document Type
Presentation
External Source(s)
Authors
William Saunders
(Analytical Mechanics Associates (United States) Hampton, Virginia, United States)
Kunio Sayanagi
(Langley Research Center Hampton, United States)
Michael Person ORCID
(Massachusetts Institute of Technology Cambridge, United States)
Paul Withers
(Boston University Boston, United States)
Richard French ORCID
(Wellesley College Wellesley, United States)
Cindy Young
(Langley Research Center Hampton, United States)
Justin Garland
(Analytical Mechanics Associates (United States) Hampton, Virginia, United States)
Soumyo Dutta
(Langley Research Center Hampton, United States)
Rohan Deshmukh
(Analytical Mechanics Associates (United States) Hampton, Virginia, United States)
Date Acquired
December 6, 2024
Publication Date
December 9, 2024
Publication Information
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: American Geophysical Union (AGU24) Meeting
Location: Washington, DC
Country: US
Start Date: December 9, 2024
End Date: December 13, 2024
Sponsors: American Geophysical Union
Funding Number(s)
CONTRACT_GRANT: RSES.C3.13.00486
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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