A sophisticated lander for scientific exploration of Mars: scientific objectives and implementation of the Mars-96 Small Station.

A mission to Mars including two Small Stations, two Penetrators and an Orbiter was launched at Baikonur, Kazakhstan: on 16 November 1996. This was called the Mars-96 mission. The Small Stations ere expected to land in September 1997 (L, approximately 178 degrees), nominally to Amazonis-Arcadia region on locations (33 N, 169.4 W) and (37.6 N, 161.9W). The fourth stage of the Mars-96 launcher mal-functioned and hence the mission was lost. However, the state of the art concept of the Small Station can be applied to future Martian lander missions. Also, from the manufacturing and performance point of view, the Mars-96 Small Station could be built as such at low cost, and be fairly easily accommodated on almost any forthcoming Martian mission. This is primarily due to the very simple interface between the Small Station and the spacecraft. The Small Station is a sophisticated piece of equipment. With the total available power of approximately 400 m W the Station successfully supports an ambitious scientific program. The Station accommodates a panoramic camera, an alpha-proton-x-ray spectrometer, a seismometer, a magnetometer, an oxidant instrument, equipment for meteorological observations, and sensors for atmospheric measurement during the descent phase, including images taken by a descent phase camera. The total mass of the Small Station with pay-load on the Martian surface, including the airbags, is only 32 kg. Lander observations.on the surface of Mars combined data from Orbiter instruments will shed on the contemporary Mars and its evolution. As in the Mars-96 mission specific science goals could be exploration of the interior and surface of Mars, investigation of the structure and dynamics of the :atmosphere, the role of water and other materials containing volatiles and in situ studies of the atmospheric boundary layer processes. To achieve the scientific goals of the mission the lander should carry a versatile set of instruments. The Small Station accommodates devices far atmospheric measurements, geophysical I-and geochemical studies of the Martian surface and interior, and cameras for descent phase and panoramic; views. These instruments would be able to contribute remarkably to the process of solving some of the scientific puzzles of Mars. (C) 1998 Elsevier Science Ltd. All rights reserved.