The Mercury Planetary Orbiter, One Step Closer to Takeoff

February 27, 2013

Space

The Mercury Planetar Orbiter a Step Closer to its 2015 Launch

The Mercury Planetary Orbiter, part of ESA’s BepiColombo mission to Mercury, placed in the Phenix thermal vacuum facility on 17 January 2012 in preparation for its ‘bake-out’. After 23 days of sustained heating to remove potential contaminants the test was completed and the chamber reopened on 14 February 2013. ESA-Anneke Le Floc’h

The Mercury Planetary Orbiter is one step closer to its 2015 launch, completing a “bake-out” where the sides and top of the chamber were kept heated to around 50°C, while the underside remained cooled by liquid nitrogen.

The faint aroma of hot metal filled the surrounding cleanroom as the hatch to ESA’s newest test facility was slid aside, concluding a 23-day ‘bake-out’ of the largest segment of ESA’s mission to Mercury.

Ending on the early hours of 14 February, this test ensured ESA’s Mercury Planetary Orbiter – MPO, part of the multi-module BepiColombo mission – was cleaned of potential contaminants in advance of its 2015 mission to the inner Solar System.

The bake-out took place at ESA’s technical heart, ESTEC in Noordwijk, the Netherlands, which includes a dedicated test center equipped to simulate all aspects of the space environment.

MPO will fly to the innermost planet with Japan’s Mercury Magnetosphere Orbiter, riding together on ESA’s propulsion module. But not before getting cooked first.

“Being close to Mercury and experiencing high temperatures, the release of molecules from spacecraft materials is expected to occur at higher quantities than for normal satellites,” explains Jan van Casteren, BepiColombo Project Manager.

“Such molecules are a contamination threat if they condense on sensitive surfaces, so we need to minimize outgassing in order to protect our delicate scientific instrumentation on the spacecraft.”

So an initial bake-out of the various spacecraft segments is essential for cleaning purposes – in this case MPO’s ‘Proto-Flight Model’, incorporating its propulsion system and heat pipes that regulate its temperature.

A new test facility called Phenix hosted the bake-out, a 4.5 m-diameter stainless steel vacuum chamber 11.8 m long, with an inner box called the ‘thermal tent’ whose six copper walls can be heated up to 100°C or cooled via piped liquid nitrogen down to –190°C, all independent from each other.

“This test was different from more typical thermal vacuum testing because, while the sides and top of the chamber were kept heated to around 50°C, the underside remained cooled by liquid nitrogen throughout,” explains Mark Wagner, Head of ESTEC’s Test Facilities & Test Methods Section.

“This creates a ‘cold trap’ where the contaminants baked off from the satellite solidify for collection. But sustaining this environment required 1500 liters of liquid nitrogen per hour – on average three tankers were calling at ESTEC daily to top up our supply.”

The test was monitored 24 hours per day on a triple shift system, with care being taken to maintain the temperatures precisely and ensure a continuous flow of data.

Outgassing production was monitored throughout the test, and the bake-out results are now being analyzed. A non-trivial amount of contaminants are expected to have been produced – ‘spoonfuls’ of material.

Now Phenix itself is being thoroughly cleaned, ready for its next customer.

“Phenix was put in place to extend the range of thermal vacuum test services on offer to ESTEC Test Center customers,” explains Mark. “It is able to accommodate large subsystems or entire spacecraft.”

Phenix was cleared for use last December, after which preparations began immediately for BepiColombo testing.

“The chamber will be kept busy for much of the rest of this year accommodating a forthcoming batch of Galileo satellites,” Mark concludes.

“This will be more traditional testing – simulating the temperature extremes the Galileo satellites must endure throughout their 12-year working lifetimes.”

Source: European Space Agency

Image: ESA-Anneke Le Floc’h

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