Possible physical and thermodynamical evidence for liquid water at the Phoenix landing site

By Nilton O. Renno, B. Bos, David C. Catling, B. Clark, L. Drube, D. Fisher, W. Goetz, S. Hviid, H. Keller, J. Kok and 13 more. 2009

194 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Physiology

View Paper: https://www.semanticscholar.org/paper/37d78c6bf855ae9491c486e3434511e86a8e4ce5

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. R. Haberle
2. A. Spiga
3. Mark T. Lemmon
4. Mark Richardson
5. Peter L Read
6. Nilton O. Renno
7. Germán Martínez
8. V. Chevrier

In Physiology

1. Michael D. Smith
2. Ashwin R. Vasavada
3. Germán Martínez
4. A. Spiga
5. Nilton O. Renno

Citations in the corpus

• THE MARTIAN ATMOSPHERIC BOUNDARY LAYER (2011, background): “[150] Recent studies suggest that electric fields in Martian dust storms produce energetic electrons [Delory et al., 2006], destroy water vapor, and lead to the formation of hydrogen peroxide, a potential sink of methane [Atreya et al., 2006; Kok and Renno, 2009].”
• The Modern Near-Surface Martian Climate: A Review of In-situ Meteorological Data from Viking to Curiosity (2017, background): “…al. 2008), is important because they can melt this ice at Mars’ present-day environmental conditions and produce liquid saline water (brine) (Clark 1978; Brass 1980; Clark and Van Hart 1981; Haberle et al. 2001; Chevrier and Altheide 2008; Rennó et al. 2009; McEwen et al. 2011; Ojha et al. 2015).”
• Formation of recurring slope lineae by liquid brines on present‐day Mars (2012, background): “Direct observations of possible liquids have been so far limited to a few droplets on the feet of the Phoenix lander [Rennó et al., 2009].”