NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Survivability of Microbes in Mars Wind Blown Dust EnvironmentAlthough the probability of Earth microbes growing (dividing) in the Martian environment is extremely low, the probability of their survival on the Martian surface is unknown. During the course of landed missions to Mars terrestrial microbes may reach the surface of Mars via inadequately sterilized spacecraft landers, rovers, or through accidental impact of orbiters. This investigation studied the potential for Earth microbes to survive in the windblown dust on the surface of Mars. The rationale for the study comes from the fact that Mars regularly has huge dust storms that engulf the planet, shading the surface from solar UV radiation. These storms serve as a mechanism for global transfer of dust particles. If live organisms were to be transported to the surface of Mars they could be picked up with the dust during a dust storm and transported across the planet. Washed, dried spores of Bacillus subtilis strain HA 101 were aseptically mixed with sterile sieved (size range of 1-5microns) Mars soil standard (obtained from NASA Johnson Space Center, Houston, Texas, USA), or Fe-montmorillonite such that the number of microbes equals 5 x 10(exp 6)/g dry wt soil. The microbe soil mixture was placed in a spherical 8 L Mars simulation chamber equipped with a variable speed rotor, gas ports and an Oriel deuterium UV lamp emitting light of wave lengths 180-400 nm. The chamber was sealed, flushed with a simulated Martian atmosphere (96.9% CO2, 3% O2, 0.1% H2O), and the pressure brought to 10 torr. The lamp and rotor were switched on to begin the experiment. Periodically samples were collected from the chamber, and the numbers of microbial survivors g soil was determined using plate counts and the most probable number method (MPN). The data indicate that Bacillus subtilis spores dispersed with Mars analog soil in a Mars atmosphere (wind blown dust) survive exposure to 5.13 KJ m-2 UV radiation, suggesting that Mars wind blown dust has potential to the protect microbes from solar UV radiation.
Document ID
20010064200
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Mancinelli, Rocco L.
(Search for Extraterrestrial Intelligence Inst. Moffett Field, CA United States)
Klovstad, Melisa R.
(Search for Extraterrestrial Intelligence Inst. Moffett Field, CA United States)
Fonda, Mark L.
(NASA Ames Research Center Moffett Field, CA United States)
DeVincenzi, Donald
Date Acquired
August 20, 2013
Publication Date
January 1, 2000
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: 35th ESLAB Symposium
Location: Noordwijk
Country: Netherlands
Start Date: October 1, 2000
Sponsors: European Space Agency. European Space Research and Technology Center, ESTEC
Funding Number(s)
PROJECT: RTOP 274-52-00-37
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Available Downloads

There are no available downloads for this record.
No Preview Available