This paper discusses a modularised design for a Mars Global Terrain Database. The design provides for elevation data with respect to a triaxial ellipsoidal reference datum developed for Mars by USGS. Terrain data is recorded for 1-second of arc almost square grid elements over the surface of Mars. A 2000-Gigabyte column-gridded relation called Terrain contains the surface terrain data. Data for Terrain is expected in 1999-2000 from the Mars Global Surveyor satellite currently in initial polar orbit around Mars. Each tuple of Terrain contains data for a N-S column-grid of 900 1-second grid elements. There is thus a set of tuples per 1-degree rectangle, with the number of tuples per set decreasing with the cosine of latitude. Surface resolution is 16.5 meters or better. The design constrains tuple sizes in Terrain to permit efficient blocking and manipulation of the records of the underlying storage file. Terrain contains a virtual-attribute function for geodetic computations relating to the triaxial ellipsoidal reference datum. The database also relates Mars feature-type relations to Terrain. Terrain's gridded structure is transparent to users writing SQL expressions to retrieve Terrain data on the basis of specific features. Many different distinct feature-type relations can be included. At least two of these participate in recursive relationships. The design also allows attachment of additional feature-type relations in a modular manner, correctly related to Terrain, without affecting the contents of Terrain. The design is intended to enable efficient exploration of the planet at all levels of scale.
438J. BRADLEY data. Remote-sensed photogrammetric data, obtained with telescopic lenses, is excellent for high-resolution planimetric mapping. However, it can be employed only in a limited manner, involving sophisticated triangulation methods, for generating corresponding elevation data for topographic mapping and imaging, or for a digital terrain model or database, unless supplemented by coincident altimeter readings [1,7].MGS is in a sun-synchronous polar orbit [6], so that an imaginary line from planet to sun always lies in (or makes a zero angle with) the plane of the MGS orbit. As a result, MGS always traverses (in a N-S direction) the planet's daytime face at midday at all (nadir) points of the surface. This enables photogrammetric data to be obtained at uniform lighting and shading angle. Since Mars rotates under the orbital plane both daily and annually, MGS will take a Martian year (about two Earth years) to complete an accurate survey of the entire planet. The initial polar orbit is highly elliptical, and a tight near-circular orbit, enabling the survey to begin, is expected in late 1998. Complete survey data should be available late in 2000. From this survey, detailed surface elevation, color, and some composition data will become available for the entire planet.This means that it will shortly be possible to construct a very high resolution Mars Global Terrain Database (MGTDB). Such a database would not h...