Projects per year
Abstract
Europa is an attractive target for future lander missions due to its dynamic
surface and potentially habitable sub-surface environment. Seismology has
the potential to provide powerful new constraints on the internal structure
using natural sources such as faults or meteorite impacts. Here we predict
how many meteorite impacts are likely to be detected using a single seismic
station on Europa to inform future mission planning efforts. To this end, we
derive: (1) the current small impactor flux on Europa from Jupiter impact
rate observations and models; (2) a crater diameter versus impactor energy
scaling relation for icy moons by merging previous experiments and simulations;
and (3) scaling relations for seismic signal amplitudes as a function
of distance from the impact site for a given crater size, based on analogue
explosive data obtained on Earth’s ice sheets. Finally, seismic amplitudes are
compared to predicted noise levels and seismometer performance to deter
mine detection rates. We predict detection of 0.002–20 small local impacts
per year based on P-waves travelling directly through the ice crust. Larger
regional and global-scale impact events, detected through mantle-refracted
waves, are predicted to be extremely rare (10-8–1 detections per year), so
are unlikely to be detected by a short duration mission. Estimated ranges
include uncertainties from internal seismic attenuation, impactor flux, and
seismic amplitude scaling. Internal attenuation is the most significant unknown
and produces extreme uncertainties in the mantle-refracted P-wave
amplitudes. Our nominal best-guess attenuation model predicts 0.002–5 local
direct P detections and 6x10-6–0.2 mantle-refracted detections per year.
Given that a plausible Europa landed mission will only last around 30 days,
we conclude that impacts should not be relied upon for a seismic exploration
of Europa. For future seismic exploration, faulting due to stresses in the
rigid outer ice shell is likely to be a much more viable mechanism for probing
Europa’s interior.
Original language | English |
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Pages (from-to) | 39-55 |
Number of pages | 17 |
Journal | Icarus |
Volume | 277 |
Early online date | 3 May 2016 |
DOIs | |
Publication status | Published - 1 Oct 2016 |
Keywords
- Europa
- cratering
- impact processes
- geophysics
- interiors
Fingerprint
Dive into the research topics of 'Europa’s small impactor flux and seismic detection predictions'. Together they form a unique fingerprint.Projects
- 6 Finished
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Short Period Seismology with the InSight Microseismometer
Teanby, N. A. (Principal Investigator)
1/11/15 → 30/06/18
Project: Research
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Research into planetary formation at Bristol.
Elliott, T. (Principal Investigator)
1/04/15 → 28/02/19
Project: Research
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Microseismometer for InSight: Pre-launch Science Support
Teanby, N. A. (Principal Investigator)
1/07/13 → 1/07/16
Project: Research