Spaceflight Insider

Schiaparelli may be dead but TGO saves the ExoMars mission

Trace Gas Orbiter (TGO) releasing its lander, Schiaparelli, as it approached Mars.

Artist’s rendition of the Trace Gas Orbiter (TGO) releasing its lander, Schiaparelli, as it approached Mars. Image Credit: ESA/ATG medialab

More than one month has now passed since the arrival of Europe’s ExoMars mission at the Red Planet. Although the mission’s Schiaparelli module has crashed onto the Martian surface, the Trace Gas Orbiter (TGO) is in excellent shape and prepares for science operations.

ExoMars began its journey to Mars on March 14, 2016. Seven months later, on Oct. 16, the Schiaparelli module had been successfully separated from the TGO, heading for a risky descent toward Martian rocky surface three days later. Apparently, the lander’s backshell and parachute were ejected prematurely, and the braking thrusters fired while the lander was still at an altitude of 2.3 miles (3.7 kilometers); consequently, the estimated altitude error caused the crash. However, it is only a hypothesis as the full analysis of the failure is not yet complete and an independent inquiry board has been initiated to investigate the event.

“An independent inquiry board will look into the non-nominal landing sequence. We know that after the deployment of the parachute the three clusters of thrusters did only work for a few seconds and that Schiaparelli fell from an altitude of two to four kilometers, reaching the surface at more than 300 km/h (186 mph),” Markus Bauer, ESA Science and Robotic Exploration Communication Officer, told

Trace Gas Orbiter instruments

Artist’s impression of the ExoMars 2016 Trace Gas Orbiter (TGO) with its instrument packages labelled. Image Credit: ESA/ATG medialab

The TGO had a much easier task to accomplish than Schiaparelli. After the successful deployment of the lander, it was scheduled to be injected into Martian orbit on Oct. 19. The orbiter completed this milestone flawlessly and is now cruising toward a highly elliptical path that takes it from an altitude of between 143 and 193 miles (230 and 310 kilometers) to around 60,900 miles (98,000 kilometers) every four days and five hours.

“TGO works nominal as well as its instruments. It is a spacecraft in its own right, scientifically and operationally,” Bauer said. “Apart from delivering Schiaparelli successfully to Mars and relaying data from it, TGO and Schiaparelli are two separate missions, with different scopes. Schiaparelli was a technology test. The TGO is a full-fledged science and communication satellite in orbit of Mars,” he added.

The orbiter’s instruments are now being calibrated and the mission controllers are now conducting first test observations. This is required to make sure that the spacecraft is working properly ahead of the start of its science mission in March 2018. By then, the aerobraking will be finished and the TGO will be in a circular orbit at an altitude of about 248 miles (400 kilometers) above the surface of Mars.

When in a circular orbit, the TGO will then fully concentrate on its science tasks, mainly detecting and analyzing methane and other trace gases.

“Scientifically it is of interest whether Mars atmospheric trace gases emanate from a specific region on Mars and to understand their source. Of specific interest is the origin of methane. TGO will solve the mystery of the origin of methane,” Bauer noted.

Although the TGO’s main scientific goal is to search for evidence of methane and other trace atmospheric gases, the spacecraft will also relay communications of NASA rovers on the ground and will be instrumental for ESA’s future ExoMars rover, which will operate on Mars as of 2021.

The TGO was built by Thales Alenia Space. The orbiter’s dimensions are 11.5 ft × 6.5 ft × 6.5 ft (3.5 m × 2 m × 2 m) with solar wings spanning 57.4 feet (17.5 meters) and providing up to 2,000 W of power. It has a mass of approximately 4.3 metric tons. The TGO is equipped with four scientific instruments for the detection of trace gases: Nadir and Occultation for MArs Discovery (NOMAD), Atmospheric Chemistry Suite (ACS), Colour and Stereo Surface Imaging System (CaSSIS), and Fine Resolution Epithermal Neutron Detector (FREND).



Tomasz Nowakowski is the owner of Astro Watch, one of the premier astronomy and science-related blogs on the internet. Nowakowski reached out to SpaceFlight Insider in an effort to have the two space-related websites collaborate. Nowakowski's generous offer was gratefully received with the two organizations now working to better relay important developments as they pertain to space exploration.

Reader Comments

Where is the FRONT heat shield ? Are we sure that the front heat shield was ejected ?

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