162 Planetary Geologic Mapping Across the Solar System
We invite abstracts that showcase planetary geologic maps, discuss mapping strategies, and leverage map-based investigations of planetary surfaces at multiple scales.
Tuesday, 21 October 2025
8:00 AM - 12:00 PM
HBGCC, 214B
Geologic Mapping of Asteroid (52246) Donaldjohanson as Observed by NASA’s Lucy Mission
Paper number: 162-13
Program: Technical Sessions
Time: 11:00 AM – 11:15 AM
Authors
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Jennifer Scully Presenting AuthorJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA
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Fiona Nichols-FlemingSmithsonain Center for Earth and Planetary Studies, Washington DC, DC
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Harrison AgrusaUniversité Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Nice
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John SpencerSouthwest Research Institute, Boulder, CO
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Neil Dello RussoJohns Hopkins University Applied Physics Laboratory, College Park, MD
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Hal WeaverJohns Hopkins University Applied Physics Laboratory, College Park, MD
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Harold LevisonSouthwest Research Institute, Boulder, CO
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Simone MarchiSouthwest Research Institute, Boulder, CO
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Keith NollGoddard Space Flight Center, Greenbelt, MD
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Stuart RobbinsSouthwest Research Institute, Boulder, CO
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Olivier BarnouinJohns Hopkins University Applied Physics Laboratory, Laurel, MD
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Stefano MottolaInstitute of Space Research (DLR), Berlin
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Edward BierhausLockheed Martin, Littleton, CO
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Audrey MartinCalifornia Institute of Technology, Pasadena, CA
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Jessica SunshineUniversity of Maryland, College Park, MD
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Emily CostelloUniversity of Hawaii, Honolulu, HI
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Masatoshi HirabayashiGeorgia Institute of Technology, Atlanta, GA
Abstract
NASA’s Lucy mission will study the Jupiter Trojan asteroids, which are thought to be a physically and compositionally diverse group of primitive planetesimals that originated in the outer Solar System from ~15-30 AU [1]. The Jupiter Trojans are thus early Solar System relics, which are one of the last accessible, stable, small-body groups yet to be explored by a spacecraft. Prior to the first Trojan encounter, (3548) Eurybates in August 2027, Lucy flew by two main-belt asteroids: asteroid (152830) Dinkinesh in November 2023 [2] and asteroid (52246) Donaldjohanson in April 2025 [3], both of which have never before been visited by a spacecraft.
Here we present the first geologic map of the observed portion of Donaldjohanson. The asteroid is about 8 km long, with a greater than 2 to 1 axis ratio, and appears to be an elongated contact binary composed of two lobes joined by a narrower neck. The primary datasets on which we base the geologic map are images from the L’LORRI camera [4] and the derived shape model [5]. We will present a geologic map that includes both lobes and the neck. We will discuss geologic units, linear features and point features, and an analysis of their distribution across the surface. We will also use geomorphic and structural analyses of these features to make inferences about the present-day near-subsurface structure and formation mechanism of Donaldjohanson.
The Lucy mission is funded through the NASA Discovery program on contract No. NNM16AA08C, and part of this work was funded by ROSES grant 24-LUCYL4PSP-0031.
References: [1] Levison, H., et al. (2021) PSJ, 2(5), 171. [2] Levison, H., et al. (2024) Nature, 629, 1015-1020. [3] Levison, H., et al. (2025) EPSC/DPS #408. [4] Weaver, H.A., et al. (2023) SSR, 219, 82. [5] Mottola, S., et al. (2025) EPSC/DPS #1022.
Geological Society of America Abstracts with Programs. Vol. 57, No. 6
doi: 10.1130/abs/2025AM-413845
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