Boulder Migration in the Khonsu Region of Comet 67P/Churyumov–Gerasimenko

Bibliographic Details
Title: Boulder Migration in the Khonsu Region of Comet 67P/Churyumov–Gerasimenko
Authors: Xiang Tang, Xian Shi, Mohamed Ramy El-Maarry
Source: The Astrophysical Journal, Vol 979, Iss 1, p 91 (2025)
Publisher Information: IOP Publishing, 2025.
Publication Year: 2025
Collection: LCC:Astrophysics
Subject Terms: Comets, Comet surfaces, Coma dust, Comet volatiles, Astrophysics, QB460-466
More Details: The European Space Agency's Rosetta mission is the only space mission that has performed long-term monitoring of a comet at close distances. For over two years, Rosetta rendezvoused with comet 67P/Churyumov–Gerasimenko, which revealed diverse evolutionary processes of the cometary nucleus. One of the most striking events is the migration of a ∼30 m boulder in the southern hemisphere region of Khonsu. Previous works found the boulder's ∼140 m displacement occurred during the three months from 2015 August to October, and several triggering mechanisms were proposed, including outburst at the boulder site, seismic vibrations from nearby activities, or surface erosion of the slope beneath the boulder. In this work, we further analyze this impressive event by analyzing imaging data from Rosetta's OSIRIS camera. We constrained the boulder's migration time to within 14 hr and derived a detailed timeline of the boulder migration event and local dust activities. High-resolution thermophysical modeling shows significant dichotomy in the thermal history of the boulder's southern and northern sides, which could have triggered or facilitated its migration via its own volatile activity.
Document Type: article
File Description: electronic resource
Language: English
ISSN: 1538-4357
Relation: https://doaj.org/toc/1538-4357
DOI: 10.3847/1538-4357/ad9825
Access URL: https://doaj.org/article/ac3f30d7854b4a29b1663e16d902eea8
Accession Number: edsdoj.3f30d7854b4a29b1663e16d902eea8
Database: Directory of Open Access Journals
More Details
ISSN:15384357
DOI:10.3847/1538-4357/ad9825
Published in:The Astrophysical Journal
Language:English