Radiation Safety. Amplified.
Join us on Linkedin
Follow us on YouTube
Subscribe to our Blog

CANBERRA Equipment Lands on Mars!

About the size of a small toaster, the Radiation Assessment Detector will look skyward and use a stack of silicon detectors and a crystal of cesium iodide to measure galactic cosmic rays and solar particles that pass through the Martian atmosphere. Image credit: NASA/JPL-Caltech/SwRI

The NASA Mars Science Laboratory (MSL) mission to Mars was launched in the fall of 2011 with the aim to determine the planet's habitability. On August 5th 2012 the MARS Rover Curiosity made an awesome landing on the planet Mars. Curiosity carries a total of 10 scientific instruments. The CANBERRA Detectors are incorporated in the Radiation Assessment Detector (RAD) .

The Radiation Assessment Detector (RAD) will be one of the first instruments sent to Mars specifically to prepare for future human exploration. The size of a small toaster or six-pack of soda, RAD will measure and identify all high-energy radiation on the Martian surface, such as protons, energetic ions of various elements, neutrons, and gamma rays. That includes not only direct radiation from space, but also secondary radiation produced by the interaction of space radiation with the martian atmosphere and surface rocks and soils.

To prepare for future human exploration, RAD will collect data that will allow scientists to calculate the equivalent dose (a measure of the effect radiation has on humans) to which people would be exposed on the surface of Mars. RAD will also assess the hazard presented by radiation to potential microbial life, past and present, both on and beneath the martian surface. In addition, RAD will investigate how radiation has affected the chemical and isotopic composition of martian rocks and soils. (Isotopes are atoms of the same element having the same number of protons but a different number of neutrons.)

A stack of paper-thin, silicon detectors and a small block of cesium iodide measure high-energy charged particles coming through the Martian atmosphere. As the particles pass through the detectors, they lose energy, producing electron or light pulses. An internal signal processor analyzes the pulses to identify each high-energy particle and determine its energy. In addition to identifying neutrons, gamma rays, protons, and alpha particles (subatomic fragments consisting of 2 protons and 2 neutrons, identical to helium nuclei), RAD will identify heavy ions up to iron on the periodic table. The RAD will be lightweight and energy efficient so as to use as little of the Mars Science Laboratory's available mass and energy resources as possible.
Visit MSL for Scientists for technical information about RAD

CANBERRA produced a total of 4 different models to go aboard and a total of 72 devices. The model called ABC Detector has 1200mm² active area segmented into 6 junctions. The models called D, E and F are single-junction detectors with 200 to 300mm² active areas and specific shapes. The devices showed extremely good leakage currents. Less than 100pA at room temperature for the 300mm² devices. The applied anti-reflective coating proved a quantum efficiency above 80%. At this very moment the first flight detectors are being tested.

This type of instrument and/or detectors is also envisaged to be used for the Ionizing Radiation Sensor (IRAS) on ESA's ExoMars mission.