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Table 1 Parameters for calculation of thermal structure in Mars

From: Evolution of the rheological structure of Mars

 

North Pole*

Solis Planum

Crustal density ρc (kg/m3)

2900a

2900a

Crustal thickness hc (km)

35b

65c

Crustal thermal conductivity kc (W/m K)

2.5d

2.5d

Mantle density ρm (kg/m3)

3300

3300

K (ppm)

3659e

2540e

Th (ppm)

0.69e

0.42e

U (ppm)

0.18e

0.11e

Surface temperature T 0 (K)

155b

220f

Martian radius R m (km)

3390

Core radius R c (km)

1700g

Surface gravity g (ms−2)

3.71

Gas constant R (JK−1mol−1)

8.3144

  1. aRuiz (2014), b Phillips et al. (2008), c Neumann et al. (2004), d Kobranova (1989), e Hahn et al. (2011), f Kieffer et al. (1977), g Yoder et al. (2003)
  2. * HPE abundances are average values for Martian crust