Probing the internal structure of the asteriod Didymoon with a passive seismic investigation. (15th September 2017)

• Record Type: Journal Article
• Authors: Murdoch, N.; Hempel, S.; Pou, L.; Cadu, A.; Garcia, R.F.; Mimoun, D.; Margerin, L.; Karatekin, O.
• Is Part Of: Planetary and space science. Volume 144(2017)
• Page Start: 89
• Page End: 105
• Publication Date: 2017-09-15
• Subjects: Asteroid -- Geophysics -- Tidal forces -- Seismology; Space sciences -- Periodicals; Atmosphere, Upper -- Periodicals; Sciences spatiales -- Périodiques; Haute atmosphère -- Périodiques; 523
• DOI: 10.1016/j.pss.2017.05.005
• Languages: English
• ISSNs: 0032-0633

Abstract

Abstract: Understanding the internal structure of an asteroid has important implications for interpreting its evolutionary history, for understanding its continuing geological evolution, and also for asteroid deflection and in-situ space resource utilisation. Given the strong evidence that asteroids are seismically active, an in-situ passive seismic experiment could provide information about the asteroid surface and interior properties. Here, we discuss the natural seismic activity that may be present on Didymoon, the secondary component of asteroid (65803) Didymos. Our analysis of the tidal stresses in Didymoon shows that tidal quakes are likely to occur if the secondary has an eccentric orbit. Failure occurs most easily at the asteroid poles and close to the surface for both homogeneous and layered internal structures. Simulations of seismic wave propagation in Didymoon show that the seismic moment of even small meteoroid impacts can generate clearly observable body and surface waves if the asteroid's internal structure is homogeneous. The presence of a regolith layer over a consolidated core can result in the seismic energy becoming trapped in the regolith due to the strong impedance contrast at the regolith-core boundary. The inclusion of macro-porosity (voids) further complexifies the wavefield due to increased scattering. The most prominent seismic waves are always found to be those traveling along the surface of the asteroid and those focusing in the antipodal point of the seismic source. We find also that the waveforms and ground acceleration spectra allow discrimination between the different internal structure models. Although the science return of a passive seismic experiment would be enhanced by having multiple seismic stations, one single seismic station can already vastly improve our knowledge about the seismic environment and sub-surface structure of an asteroid. We describe several seismic measurement techniques that could be applied in order to study the asteroid internal structure with one three-component seismic station. Highlights: We discuss the natural seismic activity on the secondary component of asteroid (65803) Didymos. Tidal stress analyses show that tidal quakes may occur, if the secondary has an eccentric orbit. Tidally-induced failure occurs most easily at the asteroid poles and close to the surface. Seismic wave propagation is simulated for homogenous, layered and macro-porous structures. Waveforms and ground acceleration spectra allow discrimination between internal structure models.