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Updated: Nov 6, 2025

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The Formation of Bilobate Comet Shapes through Sublimative Torques
Taylor K Safrit1, Jordan K Steckloff1,2,3, Amanda S Bosh1
1Massachussetts Institute of Technology, Cambridge, MA.
Summary
Most short-period comets have a unique bilobate shape due to sublimation-driven rotational disruption. This process, unique to comets, explains their distinctive two-lobed structure as they migrate through the solar system.
Area of Science:
- Planetary Science
- Cometary Science
- Solar System Dynamics
Background:
- Approximately 70% of short-period comet nuclei, primarily Jupiter-family comets (JFCs), exhibit bilobate shapes, unlike asteroids of comparable size.
- This prevalence of bilobate shapes in comets suggests a unique formation mechanism distinct from asteroid shape evolution.
Purpose of the Study:
- To investigate the formation mechanism behind the bilobate shapes observed in Jupiter-family comet nuclei.
- To determine if sublimative activity during cometary migration can naturally produce these distinctive shapes.
Main Methods:
- Modeling the torques generated by volatile sublimation during the dynamical migration of comet nuclei.
- Simulating the rotational disruption and subsequent reformation of comet nuclei with known material properties.
Main Results:
- Sublimative activity during migration can spin comet nuclei to the point of rotational disruption.
- The rubble-pile nature of comet nuclei causes them to reform into bilobate shapes after disruption.
- JFCs likely underwent rotational disruption events before entering the Jupiter family, explaining their common bilobate morphology.
Conclusions:
- The bilobate shapes of JFC nuclei are a natural consequence of sublimation-induced rotational disruption during their migration.
- These shapes likely formed recently in cometary history (within the last 1-10 million years), not during initial solar system formation.
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