Searching for extinct or extant life on Mars is part of the future NASA sur
veyor class missions. Looking for key organic compounds that are essential
for biochemistry as we know it or indicative of extraterrestrial organic in
flux is the primary goal of the Mars Organic Detector (MOD). MOD is able to
detect amino acids, amines and PAHs with at least 100 times higher sensiti
vity than the Viking GCMS experiment. MOD is not capable of identifying spe
cific organic molecules but can assess the organic inventory of amines and
PAHs on the planet. MOD can also quantify adsorbed and chemisorbed water an
d evolved carbon dioxide in a stepped heating cycle to determine specific c
arbon-bearing minerals. All that comes with no sample preparation and no we
t chemistry. The organics can be isolated from the carrier matrix by heatin
g the sample and recovering the volatile organics on a cold finger. This su
blimation technique can be used for extracting amino acids, amines and PAHs
under Mars ambient conditions. The detection of amino acids, amines and PA
Hs is based on a fluorescence detection scheme. The MOD concept has functio
ned as a laboratory breadboard since 1998. A number of natural samples incl
uding shells, clays, bones, lambda -DNA and E.-coli bacteria have been used
and organic molecules have been extracted successfully in each case. The f
irst prototype of MOD is operational as of early fall of 1999. MOD has been
selected for the definition phase of the NASA-MSR 2003 mission. (C) 2000 E
lsevier Science Ltd. All rights reserved.