Planetary Crusts: Their Composition, Origin and Evolution

By S. Taylor, S. McLennan. 2009

369 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/d4e9f078dfc47403a5644b52ab4acb4dfab1322a

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. P. King
2. E. Kite
3. G. Feulner
4. T. O. S. University
5. Research School of Earth Sciences
6. D. Geology
7. T. Yoshizaki
8. William F. McDonough Department of Earth Science

In Oceanography

1. E. Kite
2. G. Feulner
3. L. Rothschild

Citations in the corpus

• Sulfur on Mars (2010, background): “Dust, ubiquitous on Mars’s surface and in its atmosphere, has an average SO3 content of 6.8 wt% (2.7 wt% S), and soils have an average SO3 content of ~6.2 wt% (2.5 wt% S) (Taylor and McLennan 2009).”
• Is Mercury a volatile‐rich planet? (2012, background): “This value is likely representative of a combination of primary and secondary crustal material at Mercury’s surface [Denevi et al., 2009; Taylor and McLennan, 2008].”
• Sustainable life support on Mars – the potential roles of cyanobacteria (2015, background): “Martian regolith is also in large part composed of basaltic minerals; more generally, Mars’s surface seems to be mostly basaltic (McSween et al. 2009; Taylor & McLennan 2009).”
• The composition of Mars (2019, methodology): “We also estimated mineralogy and physical properties of the present-day Martian mantle (not the BSM), which is calculated using compositional models for the BSM (Table 4) and the Martian crust (Taylor and McLennan, 2009), and a crustal mass fraction of ∼5 % in the BSM.”
• The faint young Sun problem (2012, background): “greenhouse. In terms of warming, ammonia is the dominant greenhouse gas in this case, Modified after Sagan and Mullen [1972]. higher than today for the early and late Archean, respectively [Taylor and McLennan, 2009]. Thus even on the early Earth, flows of internal heat are at least two orders of magn”
• Geologic Constraints on Early Mars Climate (2018, background): “las impact (Taylor and McLennan 2009), and Mars’ geodynamo shut down before the”