Exobiology and Future Mars Missions
نویسندگان
چکیده
Nitrogen is an essential element for the evolution of life as we know it, because it is found in avariety of biologically important molecules. Therefore, N is an important element to study from anexobiological perspective. In particular, “fixed nitrogen” is the biologically useful form of nitrogen.Fixed nitrogen is generally defined as “3, NH;, NO,, or N that is chemically bound to eitherinorganic or organic molecules, and releasable by hydrolysis to NH3 or NH:. On Earth, the vastmajority of nitrogen exists as N2 in the atmosphere, and not in the fixed form. On early Marsthe same situation probably existed. The partial pressure of N2 on early Mars is thought to havebeen 18 mb, significantly less than that of early Earth. Dinitrogen can be fixed abiotically byseveral mechanisms. These mechanisms include thermal shock from meteoritic infall and lightning,which could produce NOat a rate of 1015 molecules J-l in a primitive Martian atmosphere(1 bar total pressure; COz:N2=33), as well as the interaction of light and sand containing Ti02which produces NHJ that would be rapidly destroyed by photolysis and reaction with OH radicals.These mechanisms could have been operative on primitive Mars. Any NO produced under theseconditions reacts with H forming HNO. In the Martian ocean HNO would react to form N20,,N30; , and their conjugate acids. These species would decay leaving a nitrogen pool in the oceansof NO, and NO,. In addition, there may have been organic nitrogen compounds available in theenvironment. These compounds then would have formed sediment, which may have been buriedby volcanic lava to a depth at which gaseous products would be produced and released to theatmosphere. If this burial process did not occur, or was insufficient to produce enough heat andpressure, then any nitrogen that was fixed would remain buried on Mars, and not recycled. Wouldthe relatively low abundance of nitrogen, compared to primitive Earth, have an impact on theorigin and early evolution of a living system on Mars? Data gathered in our laboratory suggestthat the low abundance of nitrogen alone may not significantly deter the origin and early evolutionof a nitrogen utilizing organism. However, the conditions on current Mars with respect to nitrogenI Iare quite different, and organisms may not be able to utilize all of the available nitrogen.
منابع مشابه
Site selection for Mars exobiology.
The selection of sites on Mars that have a high priority for exobiological research is fundamental for planning future exploration. The most immediate need is to identify targets for high resolution orbital imaging during the Mars Observer and Mars '94/'96 missions that can be used to refine site priorities for surface exploration. We present an objective approach to site selection whereby in...
متن کاملCarl Woese, Dick Young, and the roots of astrobiology
The beginning of the space age in the late 1950s gave rise to innovative and interdisciplinary research concepts and perspectives, including the concept of "exobiology" as a way to approach the fundamental aspects of biology through a study of life outside of the Earth, if it existed. This concept was embodied by NASA into its formal Exobiology Program and into the philosophy of the program bot...
متن کاملContents — K through L Martian Global - scale Seasonal CO 2 Change : Comparison of Geodetic Observations and Numerical Simulations
The Micro-End Effectors (MEE) system was developed by The Hong Kong Polytechnic University covers all as-pects of planetary explorations. All sampling tools can be divided into six catalogues: 1) Surface sampling2) Subsurface sampling3) Surface coring4) Subsurface coring5) Zero gravity sampling6) Rind Grinding It is designed for long hauled missions with low payload. e.g...
متن کاملMars Atmospheric Characterization Using Advanced 2-μm Orbiting Lidar
Mars atmospheric characterization is critical for exploring the planet. Future Mars missions require landing massive payloads to the surface with high accuracy. The accuracy of entry, descent and landing (EDL) of a payload is a major technical challenge for future Mars missions. Mars EDL depends on atmospheric conditions such as density, wind and dust as well as surface topography. A Mars orbit...
متن کاملBiological contamination studies of lunar landing sites: implications for future planetary protection and life detection on the Moon and Mars
Chemical and microbiological studies of the impact of terrestrial contamination of the lunar surface during the Apollo missions could provide valuable data to help refine future Mars surface exploration plans and planetary protection requirements for a human mission to Mars. NASA and ESA have outlined new visions for solar system exploration that will include a series of lunar robotic missions ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2003