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Mars Express

NSSDCA/COSPAR ID: 2003-022A

Description

Mars Express is a European Space Agency (ESA) mission to Mars. It consists of an orbiter, the Mars Express Orbiter, and a lander, Beagle 2. The scientific objectives of the Mars Express Orbiter are to obtain global high-resolution photo-geology (10 m resolution), mineralogical mapping (100 m resolution) and mapping of the atmospheric composition, study the subsurface structure, the global atmospheric circulation, and the interaction between the atmosphere and the subsurface, and the atmosphere and the interplanetary medium. The Beagle 2 lander objectives were to characterize the landing site geology, mineralogy, and geochemistry, the physical properties of the atmosphere and surface layers, collect data on martian meteorology and climatology, and search for possible signatures of life.

Spacecraft and Subsystems

The Mars Express Orbiter is a cube-shaped spacecraft with two solar panel wings extending from opposite sides. The launch mass of 1123 kg includes a main bus with a 113 kg of payload, the 60 kg lander, and 457 kg of propellant. The main body is 1.5 m x 1.8 m x 1.4 m in size, with an aluminum honeycomb strucure covered by an aluminum skin. The solar panels measure about 12 m tip-to-tip. A 1.8 m diameter high-gain antenna is mounted on one face, pointing in the same direction as the solar panels. Two 20 m long wire dipole antennas extend from opposite side faces perpendicular to the solar panels as part of the radar sounder. A 4 m tubular monopole low-gain antenna extends from the upper face. The body is built around the main propulsion system, which consists of a bi-propellant 400 N main engine. The two 267-liter propellant tanks have a total capacity of 595 kg. Approximately 370 kg are needed for the nominal mission. Pressurized helium from a 35 liter tank is used to force fuel into the engine. Trajectory corrections will be made using a set of eight 10 N thrusters, one attached to each corner of the spacecraft bus. Attitude control (3-axis stabilization) is achieved using two 3-axis inertial measurement units, a set of two star cameras and two Sun sensors, gyroscopes, accelerometers, and four 12-Nms reaction wheels. Pointing accuracy is .04 degrees with respect to the inertial reference frame and 0.8 degrees with respect to the Mars orbital frame. Thermal control is maintained through the use of radiators, multi-layer insulation, and actively controlled heaters. The spacecraft configuration is optimized for a Soyuz/Fregat, but is fully compatible with a Delta II launch vehicle if necessary.

Spacecraft power is provided by the solar panels which contain 11.42 square meters of silicon cells. The originally planned power was to be 660 W at 1.5 AU but a faulty connection has reduced the amount of power available by 30%, to about 460 W. This loss of power is not expected to significantly impact the science return of the mission. Power is stored in three lithium-ion batteries with a total capacity of 64.8 Ah for use during eclipses. The power is fully regulated at 28 V, the peak power requirement at Mars is 450 W. Telecommunications are via the high-gain parabolic antenna and two omnidirectional low-gain S-band antennas. These provide X-band (7.1 GHz) and S-band (2.1 GHz) uplink and downlink. Two Mars lander relay UHF antennas are mounted on the top face for communication with the Beagle 2. The spacecraft is run by two Control and Data management Units with a 10 gigabit solid state mass memory for storage of data and housekeeping information for transmission.

The science payload consists of seven experiments. The high resolution stereoscopic camera (HRSC) is mounted inside the spacecraft body, aimed through the top face of the spacecraft, which is nadir pointing during Mars operations. A visible and near-infrared spectrometer (OMEGA), infrared spectrometer (PFS) and ultraviolet spectrometer (SPICAM) are also mounted inside pointing out the top face. The neutral and charged particle sensors (ASPERA) are mounted on the top face. The subsurface radar and altimeter is mounted in the body and is nadir pointing, and also incorporates the two 20 m antennas. The radio science experiment (MaRS) uses the communications subsystem. The total mass budgeted for the science payload is 116 kg.

Beagle 2

The Beagle 2 is a lander initially mounted on the top deck of the Mars Express Orbiter. It was released from Mars Express on 19 December and reached Mars on 25 December. However no signals have been received from the lander and the mission was declared lost. For more information on the Beagle 2 lander, see:

http://nssdc.gsfc.nasa.gov/nmc/spacecraftDisplay.do?id=2003-022C

Mission profile

Launch took place on a Soyuz/Fregat from Baikonur Cosmodrome on 2 June 2003 at 23:45 local time (17:45 UT, 1:45 p.m. EDT), with the Mars Express and Fregat booster put into a 200 km Earth parking orbit. The Fregat was fired again at 19:14 UT to put the spacecraft into a Mars transfer orbit, and the Fregat and Mars Express separated at approximately 19:17 UT. The solar panels have been deployed and a trajectory correction maneuver will be performed on 4 June to aim Mars Express towards Mars and allow the Fregat booster to coast into interplanetary space. Mars Express arrived at Mars after a 400 million km journey and a course correction in September, in December 2003. The Beagle 2 lander was released on 19 December at 8:31 UTC (9:31 CET) on a ballistic cruise towards the surface. On 20 December, Mars Express fired a short thruster burst to put it into position to orbit the planet. The Mars Express Orbiter fired its main engine for 37 minutes on 25 December at 2:47 UT (9:47 p.m. EST, 24 December) and went into a highly elliptical 250 km x 150,000 km initial capture orbit with an inclination of 25 degrees. The orbit was adjusted by four more main engine firings starting on 30 December to the desired 258 km x 11,560 km near polar (86.3 degree inclination) orbit with a period of 7.5 hours. Near periapsis the top deck will be pointed down towards the martian surface and near apoapsis the high gain antenna will be pointed towards Earth for uplink and downlink. After 440 days the apoapsis was lowered to 10,107 km and periapsis raised to 298 km to give an orbital period of 6.7 hours. Aerobraking can be used to modify the orbit if there are any problems with the main engine. Nominal mission duration was planned to be 1 martian year (687 Earth days) but it was been extended multiple times. The orbit was changed in January 2009 to maintain illumination conditions. As of September 2015, the orbiter continues to operate.

The Beagle 2 coasted for five days after release and entered the martian atmosphere on the morning of 25 December. Landing was expected to occur at about 02:54 UT on 25 December (9:54 p.m. EST 24 December). No signals have been received and the lander was declared lost.

The overall Mars Express budget excluding the lander is 150 million Euros (roughly $150 million U.S.)

Alternate Names

  • Mars Express Orbiter
  • Beagle 2

Facts in Brief

Launch Date: 2003-06-02
Launch Vehicle: Soyuz
Launch Site: Tyuratam (Baikonur Cosmodrome), Kazakhstan
Mass: 666.0 kg
Nominal Power: 460.0 W

Discipline

  • Planetary Science

Additional Information

Questions or comments about this spacecraft can be directed to: Dr. David R. Williams.

 

Personnel

NameRoleOriginal AffiliationE-mail
Mr. Augustin ChicarroProject ScientistESA-European Space Research and Technology Centre 
Dr. Rudolf J. SchmidtProject ManagerESA-European Space Research and Technology Centrerschmidt@estec.esa.nl

Selected References

Bridges, J. C., et al., Selection of the landing site in Isidis Planitia of Mars probe Beagle 2, J. Geophys. Res., 108, No. E1, Jan. 2003.

Schmidt, R., Mars Express - ESA's first mission to planet Mars, Space Technol., 20, No. 5-6, 219-224, 2001.

Wright, I. P., et al., Scientific objectives of the Beagle 2 lander, Acta Astronaut., 52, No. 2-6, 219-225, 2003.

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