The EELS system is a mobile instrument platform conceived to explore internal terrain structures, assess habitability and ultimately search for evidence of life. It is designed to be adaptable to traverse ocean-world-inspired terrain, fluidized media, enclosed labyrinthian environments and liquids.
Cassini data indicates that Enceladus has a liquid ocean under its icy crust. The plumes erupting from its surface are conduits directly to liquid water, potentially making this the easiest path to a habitable liquid ocean. There are many hypothesized environmental conditions informed by proposed crevasse eruption models. These crevasse envelopes have driven every aspect of the EELS architecture to make it adaptable to the challenges it may face on this journey from the surface to the ocean. The adaptability of the system opens other destinations such as Martian polar caps, and descending crevasses in ice sheets on Earth. The current effort includes working with earth scientists to identify high-priority, high-impact terrestrial scientific investigations that will also demonstrate the capabilities of EELS in a planetary analogue environment.
The EELS architecture is a snake-like, self-propelled robot and made of multiple, identical, segments containing both the actuation and propulsion mechanisms as well as the power and communication electronics to drive them. EELS uses first-of-a-kind rotating propulsion units that act as tracks, gripping mechanisms and propeller units underwater, enabling the robot to access a plume vent exit and follow it to its ocean source.
A mobility system designed to explore internal and enclosed dynamic terrain structures in order to assess habitability and evidence for life.
This system can further Ocean World exploration by its diverse adaptability to various types of terrains. EELS allows for deeper exploration into areas that were once unattainable.
Point of Contact: Kalind Carpenter
Sponsored By: JPL Internal Research Programs funded