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Now, before the year-long aerobraking phase begins on 15 March, the science teams once again have the opportunity to make important calibration measurements, focusing mainly on tests to check the pointing and tracking of the instruments, but this time from the new orbit.

The spacecraft’s new one-day orbit takes it from 37 150 km at its farthest and to within about 200 km of the planet’s surface at its closest approach, which will also allow some of the closest images of the mission to be obtained.

TGO’s two spectrometer suites will make some preliminary calibration observations on 28 February and 1 March while the spacecraft’s instruments are facing towards Mars, with the main campaign taking place 5–7 March, covering two complete orbits of the planet.

During the main campaign, the spectrometers will be able to test another operational mode, such as scanning towards the horizon at sunlight scattered by the atmosphere.

By looking at how the sunlight is influenced by the atmosphere, scientists will be able to analyse the atmospheric constituents of Mars – TGO’s main science goal.

Indeed, TGO is tasked with making a detailed inventory of the atmosphere, particularly those gases that are present only in trace amounts. Of high interest is methane, which on Earth is produced primarily by biological activity or geological processes such as some hydrothermal reactions. 

The spacecraft will also seek out water or ice just below the surface, and will provide colour and stereo context images of surface features, including those that may be related to possible trace gas sources.

During the upcoming observations, and in addition to pointing directly at the planet’s surface, the camera will also take important dark sky and star field calibration measurements.

Meanwhile TGO’s neutron detector will be on throughout the two orbits in order to calibrate the background flux.

“It’s great we have the opportunity to squeeze in these important observations during this very busy time preparing for the year-long aerobraking phase,” says Håkan Svedhem, ESA’s TGO project scientist. “While the aerobraking is taking place, the science teams will be able to use these essential calibration measurements to best prepare for the start of the main mission when we arrive in our science orbit next year.”