INTRODUCTION TO
LANDING SITE SAFETY ISSUES
M. Golombek
JPL
Mars Exploration Rover
Landing Site Selection Workshop II
October 17-18, 2001
Pasadena, CA
ELEVATION
Below –1.3 km Elevation
MER A 5°N-15°S
MER B 10°N-10°S
SURFACE
PROPERTIES
Thermal Inertia >125-170 SI Units
>-95°C at 1 m Above Surface, I/Alb - 220/0.12 to 260/0.28
Reflectivity >0.05 – Radar Reflective Surface
Initially RMS Slopes <6°;
Then <15°
HAZARD FREE IN
MDIM
Smooth, Flat Looking in MDIM, Avoid Bumps, Hills, etc.
Avoid All Obvious Fresh Craters >5-10 km Dia
SLOPES
1 km Scale, Slopes <2° <35 m Relief MOLA
Topo/Slopes
Non-Accelerating
Roll
100 m Scale, Slopes <5° <10 m Relief MOLA Pulse Spread
Radar Spoofing,
Mesa Failure Scenario
5 m Scale, Slopes <15° <1.34 m Relief MOC
Stereo, Photoclin
Bounce Velocity
(vertical & horizontal), Lander Stability
Rover Deployment
<20% Rock Coverage
Impact Hazards (Rocks >0.5 m height)
Rover Egress
May Constrain to Even Lower Rock Abundances
SURFACE
PROPERTIES
Load Bearing and Trafficable Surface
Coat Rocks and Solar Panels
SLOPES
GARVIN – Pulse Spread
Look for Relief of <10 m over 150 m MOLA
Footprint; PS <2 m
SHEPHARD
Look for Slopes over 150 m, Inferences for 5 m Scale
KIRK and McEwen
Look for 15° Slopes or Relief of 1.34 m over 5 m
NOWICKI – TES Rock Abundance
Look for >20%
PELKEY – TES Thermal Inertia
Inferences for Surface Properties
Duricrust
RUFF - Albedo
Dust
SUMMARY OF
SAFETY EVALUATIONS - Golombek