Abstract
To assess the habitability of the icy environments in the solar system, for example, on Mars, Europa, and Enceladus, the scientific analysis of material embedded in or underneath their ice layers is very important. We consider self-steering robotic ice melting probes to be the best method to cleanly access these environments, that is, in compliance with planetary protection standards. The required technologies are currently developed and tested.
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Notes
- 1.
In this chapter, we will use the term “water” also for salt water or brine.
- 2.
The reader may forgive this bias, but the IceMole solves many of the discussed challenges in a unique and seminal way, and reliable information about the current development status of other ice melting probes is difficult to obtain.
- 3.
where the Sun is at zenith.
- 4.
“SUSI” is the abbreviation for “Sonde Under Shelf Ice.”
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Dachwald, B., Ulamec, S., Biele, J. (2013). Clean In Situ Subsurface Exploration of Icy Environments in the Solar System. In: de Vera, JP., Seckbach, J. (eds) Habitability of Other Planets and Satellites. Cellular Origin, Life in Extreme Habitats and Astrobiology, vol 28. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-6546-7_20
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