Mission “BepiColombo”: Instrument MERTIS is flying to Mercury

On December 1, ESA's BepiColombo mission successfully completed its fifth of a total of six flybys of the target planet Mercury. For the first time, images of the planet closest to the sun were captured in the mid-infrared range, providing new insights into the planet's properties.

The instrument responsible for these unique images: the MERTIS (Mercury Radiometer and Thermal Infrared Spectrometer) measuring instrument on board BepiColombo. The built-in reflective infrared optics of MERTIS were developed by researchers at the Fraunhofer Institute for Applied Optics and Precision Engineering IOF. The high-precision optics make it possible to analyze the surface of Mercury in the thermal infrared range and reveal previously hidden details.

The latest images now reveal new information on areas with different temperatures and material properties that provide clues to the mineralogical composition of the planet's surface. "We have never been this close to understanding the global surface mineralogy of Mercury," says Solmaz Adeli from the DLR Institute of Planetary Research in Berlin (Source).

BepiColombo is scheduled to reach Mercury's orbit in 2026. During this phase, MERTIS will create a global map of the mineralogical distribution on Mercury's surface - with a resolution of up to 500 meters.

Further information:

Press release on the website of ESA

On its long journey towards Mercury, the European-Japanese space probe BepiColombo cruised past Venus on October 15,20201 at a mere distance of 10,720 km. On board: the Mercury Radiometer and Thermal Infrared Spectrometer - MERTIS for short - developed at Fraunhofer IOF.

BepiColombo was slowed down by the gravity of Venus by a special flight maneuver on its journey to Mercury. This prevented the probe from plunging into the sun. On this occasion some of the instruments were tested while zooming by Venus.

MERTIS will later take a look at the surface of Mercury. But when passing Venus, the spectrometer can only see a thick cloud cover. The surface below remains veiled. But the analysis of these clouds can also be enlightening: It provides information about the elements of which they are composed. Researchers hope to be able to detect even organic compounds under certain circumstances.

After the visit to Venus, BepiColombo and MERTIS will continue on to Mercury. The probe is scheduled to arrive in 2025.

We wish you a good journey and are looking forward to the data that MERTIS will deliver from Venus!

On the morning of October 20, 2018, the European-Japanese space probe “BepiColombo” was launched from the Kourou spaceport in French Guiana towards Mercury. The mission, a seven-year voyage, is intended to unlock the secrets of Mercury, the planet closest to the sun. On board is a thermal infrared spectrometer developed by the Fraunhofer Institute for Applied Optics and Precision Engineering IOF to analyze Mercury's surface. In December 2025, the space probe will reach Mercury's target orbit and then provide information about how our solar system was created and shaped, as researchers hope.

On Saturday morning, Central European Time, the space probe “BepiColombo” was launched to the smallest and most unknown planet in our solar system. According to the European Space Agency ESA, this is the most challenging interplanetary mission in their history. The preparations for the approximately 1.3 billion euro mission took almost 20 years. One of the reasons for this is the inhospitable conditions near Mercury: A number of new technologies had to be developed to enable the probe to survive in what ESA calls “hellish surroundings”. ESA researchers hope that the mission will provide them with information about the origin of our solar system. Due to its closeness to the Sun, Mercury is of special significance.

There are a total of eleven cameras and instruments on board the satellite, four of which were developed with the help of German research institutes. For example, an infrared spectrometer called “MERTIS” is being used to characterize the minerals and elements on Mercury’s surface. MERTIS (Mercury Radiometer and Thermal Infrared Spectrometer) is a joint project of the Institute of Planetology (IfP) of the Westfälische Wilhelms-Universität (WWU) Münster and two institutes of the German Aerospace Center (DLR) in Berlin-Adlershof as well as a number of industrial partners, including OHB System AG.

Reflective infrared optics were produced for MERTIS at the Fraunhofer Institute for Applied Optics and Precision Engineering IOF (Jena). The enormous temperature differences of Mercury’s surface, which range from minus 170 to plus 430 degrees Celsius, posed a particular challenge during development. For this purpose, the optics were built from gold-coated spherical and aspherical metal mirrors and a spherical grating. These mirrors guarantee maximum stability and shape accuracy and have to withstand the stresses during rocket launch and continuous operation under space conditions.

Mirrors and gratings were manufactured at Fraunhofer IOF on special machines by ultra-precision turning with diamond tools and then installed into the assembly according to the design specifications. The mirror assembly meets the highest requirements with respect to shape accuracy and roughness of the mirror surfaces and is optimized regarding minimal deformation caused by dynamic and thermal loads as well as gravity. Fraunhofer IOF has many years of expertise in the production of high-precision metal mirror systems for applications in astronomy, aerospace and laser technology. The entire value chain from design, mirror production, coating to assembly, including system optimization, is provided from a single source.