The Lucy flyby of (52246) Donaldjohanson: A bilobed asteroid with tumbling rotation

The main belt asteroid (52246) Donaldjohanson (DJ) is a likely member of the Erigone asteroid family. This implies that DJ is a fragment of a larger parent body that was destroyed in a collision about 155 million years ago. We report observations taken during a flyby of DJ by the Lucy spacecraft. We found that DJ is composed of two heavily cratered lobes, connected by a smoother neck, with overall dimensions 8.8 kilometers (km) by 4.4 km by 3.1 km. The crater density is consistent with the Erigone family’s age, except for craters <0.4 km, which have been preferentially erased. DJ rotates slowly in a tumbling state, likely owing to spin-down by radiative forces. Surface spectra show iron-bearing phyllosilicates, indicating moderate aqueous evolution on the parent body.

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Journal
Science
Published
2026-06-18
DOI
https://doi.org/10.1126/science.aec0503
Primary Topic
Astro and Planetary Science
Type
article
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article

The Lucy flyby of (52246) Donaldjohanson: A bilobed asteroid with tumbling rotation

Matthew Montanaro, Amy A. Simon, Masatoshi Hirabayashi, Joshua P. Emery et al.
Science
Astro and Planetary Science
article

The Lucy flyby of (52246) Donaldjohanson: A bilobed asteroid with tumbling rotation

Matthew Montanaro, Amy A. Simon, Masatoshi Hirabayashi, Joshua P. Emery, Rich Burns, E. S. Costello, W. M. Grundy, J. F. Bell, W. F. Bottke, Thomas S. Statler, H. H. Kaplan, Julien Salmon, C. B. Olkin, O. S. Barnouin, Keith Noll, H. A. Weaver, David Vokrouhlický, S. Mottola, M. Pätzold, Michael E. Brown, Michael A. Vincent, D. Poland, P. R. Christensen, Sheila Gray, Fiona Nichols‐Fleming, J. Geeraert, Carly Howett, J. M. Sunshine, A. Verbiscer, J. W. Parker, S. A. Stern, Neil Dello Russo, Frank Preusker, Tod R. Lauer, Russell Carpenter, Richard P. Binzel, Harrison Agrusa, M. W. Buie, Brian A. Keeney, E. B. Bierhaus, Eric Sahr, Silvia Protopapa, S. Marchi, Brian H. May, J. R. Spencer, V. E. Hamilton, Coralie D. Adam, Dennis C. Reuter, J. E. C. Scully, Harold F. Levison, Ishita Solanki, S. J. Robbins, Mark Effertz, Katie Hegedus, Kevin Berry, Kristen Francis, Daniel Britt, David Kaufmann, Thomas Kennedy, John Andrews, Jim McAdams, Emma Birath, Katherine Kretke, Brian Sutter, Dale Stanbridge, Jon Pineau
article en

Abstract

The main belt asteroid (52246) Donaldjohanson (DJ) is a likely member of the Erigone asteroid family. This implies that DJ is a fragment of a larger parent body that was destroyed in a collision about 155 million years ago. We report observations taken during a flyby of DJ by the Lucy spacecraft. We found that DJ is composed of two heavily cratered lobes, connected by a smoother neck, with overall dimensions 8.8 kilometers (km) by 4.4 km by 3.1 km. The crater density is consistent with the Erigone family’s age, except for craters <0.4 km, which have been preferentially erased. DJ rotates slowly in a tumbling state, likely owing to spin-down by radiative forces. Surface spectra show iron-bearing phyllosilicates, indicating moderate aqueous evolution on the parent body.

ScienceVol. 392(6804)
University of Central Florida (US), University of Hawaiʻi at Mānoa (US), California Institute of Technology (US), Lockheed Martin (United States) (US), Southwest Research Institute (US), Planetary Science Institute (US), Goddard Space Flight Center (US), Georgia Institute of Technology (US), Jet Propulsion Laboratory (US), Rochester Institute of Technology (US), Northern Arizona University (US), Charles University (CZ), Lowell Observatory (US), Centre National d'Études Spatiales (FR), Czech Academy of Sciences, Astronomical Institute (CZ), Johns Hopkins University Applied Physics Laboratory (US), Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (DE), University of Oxford (GB), Planetary Systems (United States) (US), Rhenish Institute for Environmental Research (DE), Institute of Flight (US), Stellar Solutions (United States) (US), Observatoire de la Côte d’Azur (FR), National Air and Space Museum (US), NSF NOIRLab (US), BH Consulting (Ireland) (IE), American Institute of Aeronautics and Astronautics (US), University of Virginia (US), Arizona State University (US), Massachusetts Institute of Technology (US), University of Maryland, College Park (US)
Openalex Percentile: Top 6%
Astro and Planetary Science
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