| Europa Thermal Emission Imaging System | |
| Operator: | NASA |
| Manufacturer: | Arizona State University |
| Type: | infrared camera |
| Function: | study thermal anomalies |
| Spectral Band: | infrared |
| Spacecraft: | Europa Clipper |
| Sc Operator: | NASA |
| Launch: | October 10, 2024 (planned)[1] |
| Rocket: | Falcon Heavy |
The Europa Thermal Emission Imaging System (E-THEMIS) instrument is designed to scan the surface of Europa and identify areas of geologically recent resurfacing through the detection of subtle thermal anomalies. This 'heat detector' will provide high spatial resolution, multi-spectral thermal imaging of Europa to help detect active sites such as outflows and plumes. E-THEMIS will be launched on board the planned Europa Clipper astrobiology mission to Jupiter's moon Europa in 2024.
The E-THEMIS uses technology inherited from the THEMIS camera flown on board the 2001 Mars Odyssey orbiter, and the OSIRIS-REx OTES instruments.[2]
E-THEMIS will identify areas of geologically recent resurfacing through the detection of subtle thermal anomalies. E-THEMIS will be fabricated by Arizona State University with hardware contributions from Ball Aerospace Corporation,[3] and Raytheon Vision Systems. The Principal Investigator is Philip Christensen at Arizona State University.[2] One of the primary science objectives of the Europa Thermal Emission Imaging System (E-THEMIS) is to determine the regolith particle size, block abundance, and sub-surface layering for landing site assessment and surface process studies.[4] The E-THEMIS investigation is designed to characterize Europa's thermal behavior and identify any thermal anomalies due to recent or ongoing activity, which include multi-spectral infrared emission, at both day and night.[5] To accomplish this, E-THEMIS will obtain thermal infrared images in three spectral bands from 7 to 70 μm at multiple times of day.
Thermal anomalies on Europa may be manifestations of subsurface melting due to hot spots, shear heating on faults, and eruptions of liquid water, which can be imaged in the infrared spectrum.[5] Europa's water is suspected to lie 70km (40miles) below the moon's ice crust.
The specific objectives of the E-THEMIS investigation are: [6]
To achieve this, E-THEMIS will image the surface at a resolution of 5 × 22 m from 25 km altitude; it will have a precision of 0.2 K for 90 K surfaces and 0.1 K at 220 K, with an accuracy of 1-2.2 K from 220-90 K; and E-THEMIS will obtain images with up to 360 cross-track pixels with a 10.1 km wide image swath from 100 km.[6] The instrument can identify active vents, if existing, at the 1-10 meter scale. A radiation-hardened integrated circuit will be incorporated to meet the radiation requirements.
| Infrared wavelength bands | Spatial resolution from 100 km altitude | Temperature (K) | Absolute accuracy (K) | |
|---|---|---|---|---|
| 1 (7-14 μm) | 17 m × 24 m | 220 | 2.0 | |
| 2 (14-28 μm) | 25 m × 33 m | 130 | 2.2 | |
| 3 (28-70 μm) | 46 m × 52 m | 90 | 1.0 |