The origins of volatiles in the terrestrial planets

By A. Halliday. 2013

231 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/629661d4a1ef0435e04c46d7a33336c56b1d08dc

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. M. Gudel
2. H. Lammer
3. A. Izidoro
4. L. Noack
5. M. Godolt
6. E. Pilat-Lohinger
7. J. Tucker
8. J. Orman

In Geophysics

1. E. Hauri
2. L. Noack
3. M. Godolt
4. E. Pilat-Lohinger
5. J. Tucker
6. J. Orman
7. A. Izidoro
8. M. Gudel

Citations in the corpus

• Water in the Moon's interior: Truth and consequences (2015, background): “…objects during the last stages of accretion, as neither the Earth nor the Moon have the bulk composition of carbonaceous chondrites that are thought to have delivered water and other volatiles to both bodies (Marty, 2012; Halliday, 2013; Saal et al., 2013; Tartèse et al., 2013; Füri et al., 2014).”
• Origins of volatile elements (H, C, N, noble gases) on Earth and Mars in light of recent results from the ROSETTA cometary mission (2016, unknown): “Dauphas and Morbidelli (2014; “DM”) obtained an inventory comparable to the one of Halliday (2013) from global calibration of volatiles to refractory (Ce, Nb) elements, and obtained a total bulk Earth water content of about 3 ocean masses (MOcean equivalent to 230 ppm H2O for bulk Earth).”
• Evidence for multiple magma ocean outgassing and atmospheric loss episodes from mantle noble gases (2013, background): “However, the late veneer contribution was not sufficiently large to overprint the volatile characteristics acquired during the main stages of Earth’s accretion (Halliday, 2013).”
• Atmospheric mass loss during planet formation: The importance of planetesimal impacts (2014, unknown): “Earth, Venus and Mars all display similar geochemical abundance patterns of near chondritic light noble gasses, but relative depletion of in Xe, C and N (e.g. Halliday 2013).”
• Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn's rapid gas accretion (2017, background): “Estimates range from less than one ocean (Panero, 2016) to a few (Halliday, 2013) to more than ten oceans (Marty, 2012), where an “ocean” of water is defined as the amount of water on Earth’s surface (≈ 1.5 × 1024 g).”
• Origin and evolution of the atmospheres of early Venus, Earth and Mars (2018, background): “…to resolve the missing nitrogen conundrum, whereby the abundance of nitrogen in the bulk silicate Earth appears to be significantly lower than that of other volatile elements, but only if this calculation uses N2/Ar ratios and assumes nitrogen behaves like a noble gas (Halliday 2013; Marty 2012).”
• The Nitrogen Budget of Earth (2015, background): “s for the N budget of the silicate Earth. There is signicant disagreement between estimates, necessitating a more comprehensive approach. All values are 1018 kg N Reservoir Amount Reference BSE 2.78 Halliday (2013) Mantle 5 Marty (2012) 8:4 5:2 Goldblatt et al. (2009) Continental Crust 2:1 1:1 Goldb”