Abstract
The Mars Aerial Platform (MAP) concept uses superpressure balloons deployed at a constant atmospheric density, nominally set at 6 km above mean Mars elevation. Three balloons deployed in the northern, southern, and equatorial zones would traverse more than 500,000 km during a nominal lifetime of 100 sols, covering some 80% of the major terrains of Mars. The payload of imaging system, thermal emission spectrometer, and neutron spectrometer would provide geologic, geomorphic, compositional, and volatile-content data at scales which are order of magnitude greater than previous and planned missions. Tracking balloon positions would provide the first in situ measurements of atmospheric motion. In all, these data would provide unprecedented insight into the complex history of Mars, the present climate regime, and potential resources, including water.
Original language | English (US) |
---|---|
Title of host publication | 34th Aerospace Sciences Meeting and Exhibit |
Publisher | American Institute of Aeronautics and Astronautics Inc, AIAA |
ISBN (Print) | 9780000000002 |
State | Published - 1996 |
Event | 34th Aerospace Sciences Meeting and Exhibit, 1996 - Reno, United States Duration: Jan 15 1996 → Jan 18 1996 |
Other
Other | 34th Aerospace Sciences Meeting and Exhibit, 1996 |
---|---|
Country/Territory | United States |
City | Reno |
Period | 1/15/96 → 1/18/96 |
ASJC Scopus subject areas
- Space and Planetary Science
- Aerospace Engineering