18. October 2018
European-Japanese mission to investigate the smallest planet in the Solar System

Bepi­Colom­bo mis­sion: The long voy­age to Mer­cury

Artist impression of BepiColombo in front of Mercury
Artist im­pres­sion of Bepi­Colom­bo in front of Mer­cury
Image 1/5, Credit: ESA/ATG medialab; Merkur: NASA/JPL.

Artist impression of BepiColombo in front of Mercury

The mis­sion will reach Mer­cury af­ter a sev­en-year-long jour­ney. The so­lar pan­els of the Mer­cury Trans­fer Mod­ule have a span of about 30 me­tres. In the cen­tre of the for­ma­tion, with the small­er so­lar pan­el, is the Mer­cury Plan­e­tary Or­biter. Above that is the Mer­cury Mag­ne­to­spher­ic Or­biter, con­tribut­ed by the Japanese space agen­cy JAXA for the Bepi­Colom­bo mis­sion.
BepiColombo at the European spaceport in Kourou
Bepi­Colom­bo at the Eu­ro­pean space­port in Kourou (French Guiana)
Image 2/5, Credit: ESA/CNES/Arianespace/Optique vidéo du CSG - S. Martin.

BepiColombo at the European spaceport in Kourou (French Guiana)

Bepi­Colom­bo con­sists of the Mer­cury Mag­ne­to­spher­ic Or­biter (top), the Mer­cury Plan­e­tary Or­biter (mid­dle) and the Mer­cury Trans­fer Mod­ule (bot­tom).
False colour image of Mercury
False colour im­age of Mer­cury
Image 3/5, Credit: NASA/JHU Applied Physics Lab/Carnegie Inst. Washington.

False colour image of Mercury

NASA's MES­SEN­GER probe col­lect­ed nu­mer­ous da­ta from Mer­cury, most­ly from the north­ern hemi­sphere of the plan­et. The sur­face of Mer­cury is dis­played here in false colour to make its min­er­alog­i­cal com­po­nents more vis­i­ble. The rocks of Mer­cury’s sur­face have dif­fer­ent re­flec­tion prop­er­ties, which on­ly be­come vis­i­ble through the com­bi­na­tion of im­ages tak­en with dif­fer­ent colour fil­ters. Clear­ly vis­i­ble is the vol­canic rock-filled Caloris basin with a di­am­e­ter of 1,500 kilo­me­tres. This makes it one of the largest im­pact craters on the plan­ets and moons in the So­lar Sys­tem.
The MERTIS spectrometer
The MER­TIS spec­trom­e­ter for ESA’s Bepi­Colom­bo mis­sion
Image 4/5, Credit: DLR/G. Peter

The MERTIS spectrometer for ESA’s BepiColombo mission

MER­TIS is an imag­ing spec­trom­e­ter com­bined with a ra­diome­ter. The in­stru­ment is char­ac­terised by its com­pact de­sign mea­sur­ing 18 by 18 by 13 cen­time­tres, a weight of on­ly 3.3 kilo­grams and its low pow­er con­sump­tion. The sen­sors built in­to MER­TIS are unique: The imag­ing chan­nel us­es a so-called un­cooled mi­crobolome­ter - the first to be space-qual­i­fied in Eu­rope. The ra­diome­ter us­es a sen­sor mea­sur­ing on­ly three by one mil­lime­tres, which has been made from sil­i­con and al­so serves as a slit for the spec­trom­e­ter. Us­ing MER­TIS, the min­er­alog­i­cal com­po­si­tion of Mer­cury’s sur­face as well as the rock-form­ing min­er­als will be in­ves­ti­gat­ed. At the same time, the in­te­grat­ed mi­cro-ra­diome­ter will mea­sure the tem­per­a­ture and ther­mal con­duc­tiv­i­ty of Mer­cury. From the da­ta, the sci­en­tists hope to learn about the for­ma­tion and evo­lu­tion of the plan­et.
The BELA laser altimeter
The BELA laser al­time­ter on ESA’s Bepi­Colom­bo mis­sion
Image 5/5, Credit: University of Bern.

The BELA laser altimeter on ESA’s BepiColombo mission

BELA is the first Eu­ro­pean-made laser al­time­ter for a plan­e­tary mis­sion. It pro­vides in­for­ma­tion about the glob­al shape, ro­ta­tion and to­pog­ra­phy of Mer­cury. In Mer­cury or­bit, a neodymi­um-doped yt­tri­um-alu­mini­um-gar­net laser will trans­mit 10 laser puls­es per sec­ond to­wards Mer­cury via the trans­mit­ter (left in the pic­ture) at a height of less than 1000 kilo­me­tres and, af­ter a few mil­lisec­onds, will re­ceive the sig­nal re­flect­ed from the sur­face in the fo­cal point of the BELA tele­scope (right in the pic­ture). The tele­scope has a di­am­e­ter of 20 cen­time­tres and the en­tire sys­tem in­clud­ing elec­tron­ics has a mass of 15 kilo­grams. The high­er a land­scape point is lo­cat­ed, the short­er the time re­quired for the laser pulse to trav­el to the sur­face and from there to BELA’s sen­sor. From the du­ra­tion of mil­lions of laser puls­es, a 3D mod­el of the en­tire sur­face of Mer­cury will emerge in the course of the mis­sion. In ad­di­tion, re­searchers can use the shape of the re­flect­ed puls­es to de­ter­mine the sur­face rough­ness to bet­ter un­der­stand the phys­i­cal and ge­o­log­i­cal pro­cess­es shap­ing the plan­et. By de­ter­min­ing the ro­ta­tion and tides, con­clu­sions can al­so be drawn about the in­ter­nal struc­ture and de­vel­op­ment of Mer­cury.
  • The BepiColombo mission lifted off from the European spaceport in French Guiana at 03:45 Central European Summer time on 20 October 2018, on board an Ariane 5 launch vehicle.
  • The mission consists of two orbiters that, among other things, will investigate the surface and composition of the planet and analyse its magnetosphere
  • The spacecraft's long cosmic journey will last approximately seven years
  • Focus: space, space science

The European-Japanese planetary mission BepiColombo lifted off from the European spaceport in French Guiana at 03:45 Central European Summer time on 20 October 2018 (22:45 on 19 October local time), on board an Ariane 5 launch vehicle. "Not only is the mission designed to investigate the planet Mercury, it will also deliver new insights into the Solar System," explains Walther Pelzer, Executive Board Member for the Space Administration at the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR). "Once again, by rising to this immense challenge, Japan is proving to be a dependable aerospace partner for Europe." The spacecraft's cosmic journey through the inner Solar System will last approximately seven years.

Two spacecraft will investigate Mercury together

BepiColombo is the most comprehensive European project to explore a planet in the Solar System to date. The mission consists of two orbiters that will circle Mercury – the Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (MMO). While MPO is designed to investigate the surface and composition of the planet, MMO will analyse its magnetosphere. Other mission objectives include investigating the solar wind, the inner structure and the planetary environment of Mercury, as well as its interaction with the environment nearest to the Sun. The scientists hope that this will also deliver new insights into the formation of the Solar System.

During the voyage, both orbiters will travel on board the Mercury Composite Spacecraft (MCS), which will supply them with power and, thanks to a special shield – the MMO Sunshield and Interface Structure (MOSIF) – protect them from the extreme temperatures that vary between 430 degrees Celsius on the planet’s day side and minus 180 degrees Celsius on the night side.

MERTIS and BELA – Use of sensors under extreme conditions

Of the 16 instruments on board the two spacecraft, three were primarily developed in Germany: BELA (BepiColombo Laser Altimeter), MPO-MAG (MPO Magnetometer) and MERTIS (Mercury Radiometer and Thermal Infrared Spectrometer). MERTIS is an infrared imaging spectrometer and radiometer with two radiation sensors that will operate in the wavelength region of seven to 40 micrometres. Once in orbit, MERTIS will study the surface and interior of Mercury aboard MPO. With a spatial resolution of 500 metres, it will identify rock-forming minerals on the surface in the mid-infrared range.

Knowledge of the mineralogical composition allows scientists to make statements about the evolution of the planet. In addition, an integrated micro-radiometer will provide data on the surface temperature and thermal conductivity of Mercury. Thanks to an innovative instrument concept, MERTIS is extremely compact and energy-efficient. "Both MERTIS sensors are unique," says the DLR experiment manager Jörn Helbert and adds: "The imaging channel uses a so-called uncooled microbolometer – the first to be space-qualified in Europe – using a sensor measuring only three by one millimetre, which was made from one piece of silicon and also serves as a slit for the spectrometer. These are just two of a number of innovative technologies developed specifically for this experiment." The team is headed by scientists from the University of Münster and the DLR Institute of Planetary Research. The experiment is managed by the DLR Institute of Optical Sensor Systems, which designed and developed MERTIS. The operation is carried out under the direction of the DLR Institute of Planetary Research, while the scientific evaluation of the data is carried out with the University of Münster.

The BELA laser altimeter provides information about the global shape, rotation and topography of the planet closest to the Sun. Every second it sends 10 laser pulses towards Mercury and receives the signal reflected from the surface in a fraction of a second. The higher a landscape point is located, the shorter the time required for the laser pulse to travel to the surface and from there to BELA’s sensor. From the duration of millions of laser pulses, a 3D model of the entire surface of Mercury will emerge in the course of the mission. "In addition, we can use the shape of the reflected pulses to determine the surface roughness, which helps us better understand the physical and geological processes shaping the planet," explains Hauke Hußmann, scientific project manager of BELA. Sophisticated protective measurements and comprehensive heat and light protection prevent the instrument from overheating or radiation damage to occur due to the extreme temperatures on the planet. BELA was developed and built by DLR in collaboration with the University of Bern, the Max Planck Institute for Solar System Research, the Instituto de Astrofísica de Andalucía and industry. The operation and scientific evaluation of the data takes place under the direction of the DLR Institute of Planetary Research.

The MPO-MAG experiment is a high-resolution digital magnetometer. As already discovered by the Mariner 10 probe, Mercury is surrounded by a magnetic field with a strength that corresponds to one percent of the Earth's magnetic field. In MPO-MAG, two sensors are used on one of the MPO's arms to investigate Mercury's magnetic field. One of the goals is also the exploration of the internal structure of Mercury. Karl-Heinz Glaßmeier from the Institute for Geophysics and Extraterrestrial Physics (IGEP) of the Technical University of Braunschweig is scientifically responsible.

The long journey through space

It will take BepiColombo approximately seven years to reach Mercury. During this time, the spacecraft will perform several swing-by manoeuvres past Earth and Venus and even six at Mercury itself before being directed into its final orbital trajectory at its destination planet. During these swing-by manoeuvres, the spacecraft uses the gravitational force of celestial bodies to gather momentum for its continued travel through space, or, and also, to decelerate. For an orbit to be achieved, the probe must not only greatly reduce its velocity at Mercury, but also counteract the Sun's enormous gravitational pull. MERTIS will already be performing measurements during the swing-bys of Earth and Venus. Once it has arrived at Mercury, BepiColombo will collect data for approximately one year.

Mercury – Our 'unknown' neighbour in the Solar System

Mercury is more than just the smallest planet. With a diameter of 4878 kilometres it is barely larger than our own satellite. It is also the least researched of the Solar System's Earth-like planets. Above all, this is due to the fact that it is the closest neighbour to the Sun, which blasts the surface with radiation six times higher than on Earth, causing temperatures to rise to as high as 430 degrees Celsius during the day, before cooling down to even minus 180 degrees Celsius at night. Only two spacecraft have visited Mercury in the past: NASA's Mariner 10 performed three fly-bys past Mercury in 1974 and 1975, while the NASA probe MESSENGER performed three fly-bys and circled our neighbour while approaching the northern hemisphere of our planetary neighbour on an exploratory mission between 2011 and 2015. BepiColombo will complement the Messenger mission perfectly, as the southern hemisphere can now be captured accurately as well. At the same time, completely new investigations will be carried out. No instruments on MESSENGER observed the planet in the mid-infrared range. Therefore, MERTIS will supply a completely new dataset.

Close European-Japanese cooperation

ESA is responsible for the overall mission, and the agency was also responsible for developing and building the Mercury Planetary Orbiter. The Japanese space agency JAXA contributed the Mercury Magnetospheric Orbiter. The German part of the BepiColombo mission was coordinated and largely financed by DLR Space Administration using funds provided by the German Federal Ministry for Economic Affairs and Energy (BMWi). The two instruments BELA and MERTIS, which were largely developed by the DLR Institutes of Planetary Research and Optical Sensor Systems in Berlin-Adlershof, were essentially financed from means provided by DLR Research and Technology. The mission also received support from the Max Planck Institute for Solar System Research (MPS) in Göttingen, the University of Münster and TU Braunschweig. A European industrial consortium led by the firm Airbus Defence and Space is contributing the industrial part of the spacecraft.

Contact
  • Diana Gonzalez
    Ger­man Aerospace Cen­ter (DLR)
    Ger­man Space Agen­cy at DLR
    Cor­po­rate Com­mu­ni­ca­tions
    Telephone: +49 228 447-388
    Königswinterer Straße 522-524
    53227 Bonn
    Contact
  • Heiner Witte
    Ger­man Aerospace Cen­ter (DLR)

    Space Ad­min­is­tra­tion, Space Sci­ence
    Telephone: +49 228 447-344
    Fax: +49 228 447-745
    Linder Höhe
    51147 Köln
  • Julia Heil
    Ger­man Aerospace Cen­ter (DLR)
    Cor­po­rate Com­mu­ni­ca­tions
    Telephone: +49 2203 601-5263

    Contact
  • Ulrich Köhler
    Ger­man Aerospace Cen­ter (DLR)
    In­sti­tute of Plan­e­tary Re­search
    Rutherfordstraße 2
    12489 Berlin
    Contact

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