Beagle 2: the exobiological lander of Mars Express

planned to touch down in the Isidis Planitia region of Mars (265.0°W, 11.6°N). Once safely deployed on the surface, Beagle 2 will conduct an intensive and exhaustive programme of surface operations for about 180 sols (equivalent to about 6 months on Earth). The principal objective is the detection of extinct and/or extant life, or at least to establish if the conditions at the landing site were ever suitable for life to have evolved in the planet’s history. To achieve this goal, a systematic set of experiments using a complementary suite of instruments will perform in situ geochemical, mineralogical and petrological analysis of selected rocks and soils. Studies of the martian environment will also be conducted via chemical analysis of the atmosphere, local geomorphological assessment of the landing site and measurement/monitoring of dynamic environmental processes, including transient events such as ‘dust devils’. Further studies, unique to Beagle 2, include analysis of the subsurface regime using a ground penetration tool and the first attempt at in situ isotopic dating of rocks on another planet. The complete experiment package weighs less than 9 kg and requires less than 40 W of power. With a probe mass limit of 69 kg, imposed by mission constraints, and a landed mass of 33 kg, Beagle 2 thus aims to fly the highest mass ratio of payload-to-support systems of any mission to Mars. This is achievable only by adopting an integrated design approach and employing minimal or zero redundancy.

[1]  H. J. Moore,et al.  Overview of the Mars Pathfinder mission and assessment of landing site predictions. , 1997, Science.

[2]  M. Schidlowski,et al.  Application of Stable Carbon Isotopes to Early Biochemical Evolution on Earth , 1987 .

[3]  Tobias Owen,et al.  The composition and early history of the atmosphere of Mars , 1992 .

[4]  C. Pillinger,et al.  Organic materials in a martian meteorite , 1989, Nature.

[5]  C. Pillinger,et al.  Mars, Modulus and MAGIC. The measurement of stable isotopic compositions at a planetary surface , 1998 .

[6]  R. Wiens,et al.  The case for a Martian origin of the shergottites. II - Trapped and indigenous gas components in EETA 79001 glass , 1986 .

[7]  E. Gibson,et al.  Low-Temperature Carbonate Concretions in the Martian Meteorite ALH84001: Evidence from Stable Isotopes and Mineralogy , 1997, Science.

[8]  H. McSween SNC meteorites: Clues to Martian petrologic evolution? , 1985 .

[9]  J. Muller,et al.  Selection of the landing site in Isidis Planitia of Mars probe Beagle 2 , 2003 .

[10]  Larry W. Esposito,et al.  Meteorological observations on Martian surface: met-packages of Mars-96 Small Stations and Penetrators , 1998 .

[11]  C. Pillinger,et al.  A search for nitrates in Martian meteorites , 1995 .

[12]  Harry Y. McSween,et al.  What we have learned about Mars from SNC meteorites , 1994 .

[13]  Harry Y. McSween,et al.  A possible high-temperature origin for the carbonates in the martian meteorite ALH84001 , 1996, Nature.

[14]  L. Leshin,et al.  Oxygen Isotopic Constraints on the Genesis of Carbonates from Martian Meteorite ALH84001 , 1998 .

[15]  C. Pillinger,et al.  The oxygen‐isotopic composition of Earth and Mars , 1999 .

[16]  I. Lyon,et al.  Correlated chemical and isotopic zoning in carbonates in the martian meteorite ALH84001 , 1998 .

[17]  C. Pillinger,et al.  Distribution of sulphides and oxidised sulphur components in SNC meteorites , 1989 .

[18]  C P McKay,et al.  A coupled soil-atmosphere model of H2O2 on Mars. , 1994, Icarus.

[19]  Richard V. Morris,et al.  Mineralogical analysis of Martian soil and rock by a miniaturized backscattering Mössbauer spectrometer , 1996 .

[20]  R. J. Reid,et al.  Results from the Mars Pathfinder camera. , 1997, Science.

[21]  Ian Wright,et al.  Modulus—An experiment to measure precise stable isotope ratios on cometary materials , 1998 .

[22]  D. R. Rushneck,et al.  The composition of the atmosphere at the surface of Mars , 1977 .

[23]  C. A. Wood,et al.  SNC meteorites - Igneous rocks from Mars , 1982 .

[24]  R. Zare,et al.  Search for Past Life on Mars: Possible Relic Biogenic Activity in Martian Meteorite ALH84001 , 1996, Science.

[25]  A. Brack,et al.  Exobiology in the Solar System and the Search for Life on Mars , 1999 .

[26]  I. P. Wright,et al.  Record of fluid–rock interactions on Mars from the meteorite ALH84001 , 1994, Nature.

[27]  G. Klingelhöfer In‐situ analysis of planetary surfaces by Mössbauer spectroscopy , 1998 .

[28]  D. Bogard,et al.  Martian Gases in an Antarctic Meteorite? , 1983, Science.

[29]  Anthony J. Tuzzolino,et al.  Applications of PVDF dust sensor systems in space , 1996 .

[30]  H. Kochan,et al.  Small Sample Acquisition/Distribution Tool , 1997 .

[31]  M. Grady,et al.  Martian atmospheric carbon dioxide and weathering products in SNC meteorites , 1985 .

[32]  Michael E. Zolensky,et al.  Aqueous alteration of the Nakhla meteorite , 1991 .

[33]  C. Stoker,et al.  Organic degradation under simulated Martian conditions. , 1997, Journal of geophysical research.

[34]  C. McKay,et al.  The Chemical Reactivity of the Martian Soil and Implications for Future Missions , 1994 .

[35]  Robert O. Pepin,et al.  The case for a martian origin of the shergottites: nitrogen and noble gases in EETA 79001 , 1984 .

[36]  C. Pillinger,et al.  Chassigny and the nakhlites: Carbon-bearing components and their relationship to martian environmental conditions , 1992 .

[37]  R. Pepin Meteorites: Evidence of Martian origins , 1985, Nature.

[38]  D P Glavin,et al.  A search for endogenous amino acids in martian meteorite ALH84001. , 1998, Science.

[39]  R. Clayton,et al.  Water in SNC meteorites: evidence for a martian hydrosphere. , 1992, Science.

[40]  C. Pillinger,et al.  Carbon, oxygen and nitrogen isotopic compositions of possible martian weathering products in EETA 79001 , 1988 .

[41]  Michael E. Zolensky,et al.  Calcium carbonate and sulfate of possible extraterrestrial origin in the EETA 79001 meteorite , 1988 .

[42]  D. Mittlefehldt,et al.  ALH84001, a cumulate orthopyroxenite member of the martian meteorite clan , 1994 .

[43]  H Y McSween,et al.  The chemical composition of Martian soil and rocks returned by the mobile alpha proton X-ray spectrometer: preliminary results from the X-ray mode. , 1997, Science.

[44]  J. Ryan,et al.  Possible dust devils, vortices on Mars , 1983 .

[45]  J. Bada,et al.  A search for endogenous amino acids in the Martian meteorite EETA79001. , 1995, Geochimica et cosmochimica acta.