Features Of Early Martian Environment And Presence Of Water Drive Search For Life Forms

Compiled by Helmut Lammer, PhD, Senior Editor of Astrobiology, from the Austrian Academy of Sciences, this special paper collection features a report by Pham et al. that presents a semi-analytical model to evaluate the influence of impacts on the evolution of the carbon dioxide-based martian atmosphere. The results of this study indicate that impacts alone cannot satisfactorily explain the loss of significant atmospheric mass since the Late Noachian (~ 3.7 – 4 Ga).

In other words, if the martian atmosphere was much denser at about 4 Ga than at present, impact erosion was most likely not responsible for the removal of the atmosphere at that time. Terada et al. present a 3-D model to assess the effects of exposure to solar energy and winds on ion escape on early Mars 4.5 Ga, and to demonstrate how ion erosion could have led to the loss of water that might have been present on Mars. Two reports, by Horváth et al. and Fendrihan et al., explore the existence and survival of two types of bacteria under martian surface and environmental conditions, and the types of habitats that might have existed to support these life forms.

"The results of Pham et al. and Terada et al. indicate that Mars should have lost its denser initial CO₂ atmosphere very early," says Dr. Lammer, PhD, "and may have been cold and dry during most of its history. Leblanc and colleagues propose a new concept in exploratory missions with Mars Environment and Magnetic Orbiter (MEMO), which would gather data to help scientists understand how the martian surface, atmosphere, and magnetic field have evolved, and how those questions raised by Terada et al. and Pham et al. can be investigated."

This Special Paper Collection is available free online at http://www.liebertpub.com/ast