Trojan Asteroid Satellites, Rings, and Activity
Abstract
The Lucy mission will encounter five Jupiter Trojans during its mission with three of the five already known to be multiple systems. These include a near-equal-mass binary, a small and widely separated satellite, and one intermediate-size satellite system. This chapter reviews the current state of knowledge of Trojan asteroid satellites in the context of similar satellite systems in other small body populations. The prospects for the detection of additional satellites as well as other near-body phenomena are considered. The scientific utility of satellites makes their observation with Lucy an important scientific priority for the mission.
Copyright and License
This is a U.S. Government work and not under copyright protection in the US; foreign copyright protection may apply 2023. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Funding
The Lucy mission is funded through the NASA Discovery program on contract No. NNM16AA08C.
Conflict of Interest
The authors declare that they have no competing interests.
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Additional details
- ISSN
- 1572-9672
- National Aeronautics and Space Administration
- NNM16AA08C
- Caltech groups
- Division of Geological and Planetary Sciences