The origin of water on Mars

By Jonathan I. Lunine, J. Chambers, A. Morbidelli, L. Leshin. 2002

163 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/42b5ec56c5b2834a65d78744264477f796d096ef

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. S. Raymond
2. A. Morbidelli
3. Kevin J. Walsh
4. S. Kenyon
5. B. Bromley
6. F. Selsis
7. K. Zahnle
8. H. Lammer

In Statistical and Nonlinear Physics

1. B. Bromley
2. S. Raymond
3. H. Lammer
4. Ernst Hauber
5. A. Morbidelli
6. S. Kenyon
7. O. Mousis
8. K. Zahnle

Citations in the corpus

• Outgassing History and Escape of the Martian Atmosphere and Water Inventory (2015, methodology): “Lunine et al. (2003) estimated the cumulative collision probability between small bodies and Mars and found that Mars’ initial water inventory may have equivalent to ∼0.06–0.27 times that of an Earth ocean (EO), corresponding to a martian surface pressure of ∼10–100 bar.”
• Emergence of a Habitable Planet (2007, background): “It is possible in Mars we are looking at a planet that is old enough to remember these times (Lunine et al. 2003; Halliday and Kleine 2006).”
• Terrestrial Planet Formation. I. The Transition from Oligarchic Growth to Chaotic Growth (2005, background): “…with the dynamical influence of Jupiter (e.g., Kominami & Ida 2004), the highly eccentric orbits of lower mass oligarchs have an important role in clearing the inner solar system (e.g., Goldreich, Lithwick & Sari 2004a; Kominami & Ida 2004) and delivering water to the Earth (Lunine et al. 2003).”
• Ventilation of CO2 from a reduced mantle and consequences for the early Martian greenhouse (2008, background): “Delivery of volatiles by chondritic meteorites and comets occurred principally in first 10 Ma (Lunine et al., 2003), whereas massive ventilation of volatiles from the interior would have occurred within the first 30–50 Ma (Elkins-Tanton et al.”
• Building Terrestrial Planets (2012, background): “The third possibility is that Earth accreted water from primitive planetesimals and/or planetary embryos originally from the outer asteroid belt (Lunine et al. 2007; Morbidelli et al. 2000; O’Brien et al. 2006; Raymond et al. 2004, 2005, 2006, 2007).”