THE RESEARCH PROJECT CONTEMPLATES TWO ASPECTS, ONE TECHNOLOGICAL AND ANOTHER SCIENTIFIC. THE FIRST HAS AS ITS FINAL OBJECTIVE THE DEVELOPMENT OF THE C/D PHASES OF THE JANUS CHAMBER AND ALTIMETRO LASER GALA POWER SOURCES AND ALSO THE CONSTRUCTION OF A MECHANICAL MODULE COMPOSED OF A FILTER WHEEL AND THE ELECTRONIC CONTROL OF THE SAME FOR THE CAMERA. _x000D_ the COMMITTEE OF THE C/D Phase is coming with the IPDR, which will end in 2016 Summer, following the beginning of the development of the ENGLIAN MODEL PREVIED FOR JANUARY 2017. _x000D_ for the CONSTRUCTION OF PROTO-FLIGHT models, PFM and FS, PFM and FS, the adopted philosophia will be the one of PROTO-FLIGHT, and the dates ahead for the deliveries are FINAL 2018 for PFM and Measured 2019 for FS. Both INSTRUMENTS are within the SCIENTIFIC BACK OF THE JUICE MISSION (ESA) to the JUPITER SYSTEM TO STUDY THE PLANET (OUT THE INTERIOR HASTS YOUR Magnetosphere PASAN BY THE ANILS), the Galilean SATELITES WITH SPECIAL INTERESTS in Ganymede and Calixt, and the agreement as a whole and as a PLANETARY SYSTEM ARQUETY._x000D_ THE SCIENTIFIC VERtENT Is ORIENTIFIC TO THE CONTINUATION OF THE SCIENTIFIC EXPLOTATION OF THE DATA OF OSIRIS CHARARAS TO BORDO DE LA NAVE ROSETTA (MISION IS TO COMETA 67P/Churyumov-Gerasimenko). THE SPECIFIC OBJECTIVES ARE, TO THE EXTENT POSSIBLE, (I) TO DETERMINE THE INTERNAL STRUCTURE OF THE COMET BY STUDYING DATA FROM CONCERT, RSI AND OSIRIS; (II) ANALYSE THE NON-GRAVITATIONAL AND TORQUE FORCES ACTING ON THE NUCLEUS, (III) PROPOSE A SCENARIO TO EXPLAIN THE ACTIVITY, AND (IV) WITH THE INFORMATION OBTAINED IN (I)+(II)+(III) STUDY THE ROTATIONAL EVOLUTION OF THE NUCLEUS TO DERIVE INTERNAL PROPERTIES THAT WILL HELP REVEAL HOW THIS COMETARY NUCLEUS WAS FORMED. _x000D_ there are two SCIENTIFIC OBJECTIVES that are to be treated with the contract of two documents. THESE ARE: (I) INVESTIGATE THE SUPERFICIAL COMPOSITION OF SMALL BODIES OF THE SOLAR SYSTEM THROUGH SPECTROSCOPY AND SIMULATION OF SURFACE RENEWAL CAUSED BY IMPACTS, AND (II) EXTEND THE KNOWLEDGE ACQUIRED ON HOW THE ACTIVITY IN COMETS IS DEVELOPED (ESPECIALLY FROM DATA FROM THE ROSETTA MISSION (THAT)) TO OTHER BODIES SUCH AS THE ASTEROIDS SHOWING ACTIVITY, I.E., DUST EJECTION THAT MUST BE PRODUCED BY GAS SUBLIMATION AT SHORT HELIOCENTRIC DISTANCES, OR BY IMPACTS OF OTHER ASTEROIDS OR METEOROIDS ON THEM. _x000D_ the TWO ULTIMATE Decades OF EXOPLANET DISCOVERS HAVE REVELATED EXOPLANETS THAT ARE VERY COMMUNES AND VERY DIVERSES IN YOUR orbital, DINAMIC AND COMPOSIONAL PROPERTYS. NOW WE BEGIN TO INVESTIGATE THE CHEMICAL DIVERSITY OF EXOPLANETS, THEIR ATMOSPHERIC AND INTERNAL PROCESSES, AND THEIR FORMATION CONDITIONS. THE ADVANCES IN OUR UNDERSTANDING OF THE CHEMISTRY OF THE ATMOSPHERE OF THE EXOPLANETS AND THE IMPLICATIONS FOR THEIR FORMATION CONDITIONS ARE BEING VERY IMPORTANT. DURING THE DURATION OF THE PROJECT, WE WILL GENERATE FAMILIES OF ATMOSPHERES IN THERMOCHEMICAL AND PHOTOQUIMICO EQUILIBRIUM BASED ON DIFFERENT TYPES OF STARS, REGION OF TRANSITION BETWEEN CONVECTION AND TURBULENT DIFFUSION, FLOW CONDITIONS AT THE UPPER AND LOWER BORDERS, ETC. OF THIS CATALOGUE OF EXOPLANETARY ATMOSPHERES, AND THROUGH STATISTICAL ANALYSIS, WE INTEND TO ANSWER QUESTIONS SUCH AS WHAT PROPERTIES ARE FREQUENT OR EXCEPTIONAL IN THE EXOPLANETARY ATMOSPHERES? HOW MANY TYPES OF PLANETS CAN WE DISTINGUISH?ETC