Packing for Mars

October 22, 2014, European Space Agency
Technicians in ESA’s ultra-clean microbiology laboratory, part of ESTEC's Life, Physical Sciences and Microgravity Laboratory, follow strict Planetary Protection procedures as they prepare the COMARS+ temperature sensor to be put into storage until it can be integrated into the heat shield of ExoMars 2016's Schiaparelli lander. Credit: ESA

Like surgeons in an operating room, the technicians work gowned and masked in ESA's ultraclean microbiology laboratory, ensuring a high-tech sensor will not contaminate the Red Planet with terrestrial microbes.

This temperature sensor is destined to land on Mars as part of ESA's Schiaparelli module in late 2016.

Schiaparelli will hitch a ride to the Red Planet with the ExoMars Trace Gas Orbiter, set for launch on a Russian Proton rocket at the start of 2016. By proving Europe's capability to land safely, the door will be opened for ESA's ExoMars rover two years later.

Schiaparelli will also do useful science in its own right during its estimated two to eight martian days of surface life.

First, sensors embedded in the heatshield will record details of its plunge through the alien atmosphere.

Then, a battery-powered suite of will measure the electrical activity and transparency of the surface atmosphere, its wind speed and direction, along with air pressure and temperature.

Produced by Germany's DLR space agency with France's CNES space agency, the heatshield package was delivered to ESA's technical centre, ESTEC, in Noordwijk, the Netherlands, earlier this year.

It must be stored until it can be integrated into the lander's heatshield, but first the ExoMars team had to be certain the sensor had not picked up any microscopic hitchhikers along the way.

Anything headed to Mars is subject to strict 'Planetary Protection' to ensure that the pristine environment is not contaminated by terrestrial microbes, which could mask possible evidence of alien life or result in a false-positive detection of life.

The ExoMars Trace Gas Orbiter (TGO), along with an Entry, Descent and Landing Demonstrator Module (EDM), form the first mission in the ExoMars programme. The Orbiter and EDM are scheduled to arrive at Mars in 2016. The ExoMars Orbiter will accomodate a suite of instruments to carry out a series of scientific investigations, including the search for evidence of methane and other trace gases in the Martian atmosphere. The ExoMars EDM constitutes a technology platform whose main goal is to enable Europe to acquire the capability to land on Mars. Although designed to demonstrate entry, descent and landing technologies, the EDM also offers limited, but useful, science capabilities. Credit: ESA/AOES Medialab

ESTEC's cleanroom, part of its Life, Physical Sciences and Microgravity Laboratory, is designed for such demanding work. Its rigorously filtered air contains millions of times fewer particles than the outside atmosphere: fewer than a dozen particles larger than 0.1 micrometres – each equivalent to a single speck of dust – per cubic metre of air.

Technicians donned sterile 'bunny suits' before they could have contact with the sensor, entering the 35 sq m cleanroom through an air shower.

Like all ExoMars hardware, the sensor was itself built in cleanroom conditions, but the technicians were still required to make 'bioburden' checks, drawing swabs across equipment surfaces that could be then put onto culture plates to identify any contamination.

ESA’s ultra-clean microbiology laboratory is part of the Agency's Life, Physical Sciences and Microgravity Laboratory, based in Noordwijk, the Netherlands. The air on the other side of the glass is an ISO class 1 cleanroom, its rigorously filtered air containing at rest millions of times fewer particles than the outside atmosphere: fewer than a dozen particles larger than 0.1 micrometres, such as a speck of dust,  per cubic metre of air. This makes it suitable for Planetary Protection procedures, such as examining temperature sensors destined to end up on the surface of Mars aboard the ExoMars 2016 Schiaparelli lander. Credit: ESA–A. Le Floc'h

In the event, it gained a clean bill of health, which meant it could then be placed into a sterile, antistatic bag for storage within the lab's protected environment.

It joins other Schiaparelli flight equipment already in storage, including the Descent Camera that will record the later stages of landing.

Explore further: Europe shortlists four sites for 2019 Mars mission

Related Stories

NASA radio delivered for Europe's 2016 Mars orbiter

July 8, 2014

(Phys.org) —The first of two NASA Electra radios that will fly aboard the European Space Agency's next mission to Mars has been delivered for installation onto the ESA ExoMars Trace Gas Orbiter (TGO).

ExoMars orbiter core module completed

February 4, 2014

(Phys.org) —The ExoMars Trace Gas Orbiter module consisting of the spacecraft structure, thermal control and propulsion systems was handed over by OHB System to Thales Alenia Space France at a ceremony held in Bremen, Germany, ...

ExoMars lander module named Schiaparelli

November 11, 2013

The entry, descent and landing demonstrator module that will fly on the 2016 ExoMars mission has been named 'Schiaparelli' in honour of the Italian astronomer Giovanni Schiaparelli, who famously mapped the Red Planet's surface ...

Entry, descent and surface science for 2016 ExoMars mission

June 10, 2011

ESA and NASA have announced the scientific investigations selected for their 2016 ExoMars lander demonstrator. They will probe the atmosphere during the descent, and return the first ever data on electrical fields at the ...

ExoMars 2016 set to complete construction

June 18, 2013

ESA's mission to Mars in 2016 has entered the final stage of construction with the signature of a contract today with Thales Alenia Space at the Paris Air & Space Show.

Recommended for you

Superflares from young red dwarf stars imperil planets

October 18, 2018

The word "HAZMAT" describes substances that pose a risk to the environment, or even to life itself. Imagine the term being applied to entire planets, where violent flares from the host star may make worlds uninhabitable by ...

Blazar's brightness cycle confirmed by NASA's Fermi mission

October 18, 2018

A two-year cycle in the gamma-ray brightness of a blazar, a galaxy powered by a supermassive black hole, has been confirmed by 10 years of observations from NASA's Fermi Gamma-ray Space Telescope. The findings were announced ...

Astronomers catch red dwarf star in a superflare outburst

October 18, 2018

New observations by two Arizona State University astronomers using the Hubble Space Telescope have caught a red dwarf star in a violent outburst, or superflare. The blast of radiation was more powerful than any such outburst ...

Magnetic fields may be the key to black hole activity

October 17, 2018

Collimated jets provide astronomers with some of the most powerful evidence that a supermassive black hole lurks in the heart of most galaxies. Some of these black holes appear to be active, gobbling up material from their ...

0 comments

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.