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Compositional Analysis of (52246) Donaldjohanson from the Lucy FlybyThe NASA Lucy mission was designed to provide the first reconnaissance of Jupiter Trojan asteroids. These primitive bodies hold important clues to the origin and evolution of the Solar System. The Lucy spacecraft is currently en route to its encounters with Trojan asteroids in the L4 swarm in 2027 and 2028, and the L5 swarm in 2033 [1]. On its way through the Main Belt, Lucy flew past the asteroid (52246) Donaldjohanson on April 20, 2025. The main purpose of the flyby was to support mission preparation for the primary science targets, the Trojan asteroids. The Linear Etalon Imaging Spectral Array (LEISA) mapping spectrometer [2,3], part of the L’Ralph instrument, collected multiple spectral datasets during the encounter with Donaldjohanson. LEISA covers the spectral range 0.97 – 3.95 μm with a variable spectral resolving power ranging from ~50 to 160 (Δλ<10 nm).

Several primitive asteroid families have been identified in the inner Main Belt. These families are of interest for their potential to deliver primitive material into near-Earth space, and potentially even sourcing the carbonaceous meteorites that fall to Earth. Donaldjohanson is a member of one of these families, the Erigone collisional family. The collisional disruption of the Erigone family occurred ~155 Myr ago [4]. Ground-based observations have revealed that the Erigone family consists of primitive C-complex asteroids, the majority of which show evidence for a 0.7-μm absorption due to Fe-bearing phyllosilicates [5] and spectral slopes that are neutral to slightly red [6]. The only ground-based near-infrared data published of Donaldjohanson itself [7] are too noisy for a reliable interpretation. We will report on the Lucy near-infrared spectral observations of Donaldjohanson, with a focus on a search for absorption features due to materials seen in ground-based spectra of Erigone family members and found in analog carbonaceous meteorites, including hydrated silicates and organic molecules. The spatially resolved LEISA data also enable assessment of any potential spectral heterogeneity on Donaldjohanson.
Document ID
20250004683
Acquisition Source
Goddard Space Flight Center
Document Type
Abstract
Authors
Joshua P Emery ORCID
(Northern Arizona University Flagstaff, United States)
Amy A Simon
(Goddard Space Flight Center Greenbelt, United States)
Hannah H Kaplan
(Goddard Space Flight Center Greenbelt, United States)
William M Grundy
(Lowell Observatory Flagstaff, Arizona, United States)
Jessica M Sunshine
(University of Maryland, College Park College Park, United States)
Silvia Protopapa ORCID
(Southwest Research Institute San Antonio, United States)
Dennis C Reuter
(Goddard Space Flight Center Greenbelt, United States)
Allen Lunsford
(American University Washington D.C., District of Columbia, United States)
Matt Montanaro
(Rochester Institute of Technology Rochester, United States)
Gerald E Weigle
(BigHeadEndian, LLC Boulder, CO, United States)
Ishita Solanki
(Southwest Research Institute Boulder, CO, United States)
Richard P Binzel ORCID
(Massachusetts Institute of Technology Cambridge, United States)
John R Spencer
(Southwest Research Institute San Antonio, United States)
Keith Noll
(Goddard Space Flight Center Greenbelt, United States)
Simone Marchi
(Southwest Research Institute San Antonio, United States)
Harold F Levison
(Southwest Research Institute San Antonio, United States)
Date Acquired
May 7, 2025
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: Europlanet Science Congress - Division for Planetary Sciences (EPSC-DPS) Joint Meeting
Location: Helsinki
Country: FI
Start Date: September 7, 2025
End Date: September 12, 2025
Sponsors: American Astronomical Society, euroPLANET
Funding Number(s)
WBS: 577236.07.01.02.01
CONTRACT_GRANT: NNM16AA08C
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
External Peer Committee
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