Breaking Degeneracies in Formation Histories by Measuring Refractory Content in Gas Giants
Relating planet formation to atmospheric composition has been a long-standing goal of the planetary science community. So far, most modeling studies have focused on predicting the enrichment of heavy elements and the C/O ratio in giant planet atmospheres.
Yayaati Chachan+3 more
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Geochemistry and petrogenesis of the Feshark intrusion (NE Isfahan city)
Introduction Granitic rocks are the most abundant rock types in various tectonic settings and they have originated from mantle-derived magmas and/or partial melting of crustal rocks.
Ali Kananian+4 more
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One of the outstanding goals of the planetary science community is to measure the present-day atmospheric composition of planets and link this back to formation.
Stefan Pelletier+13 more
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A Comparison of Presolar Isotopic Signatures in Laboratory-Studied Primitive Solar System Materials and Comet 67P/Churyumov-Gerasimenko: New Insights from Light Elements, Halogens, and Noble Gases. [PDF]
Hoppe P, Rubin M, Altwegg K.
europepmc +1 more source
Stability of hydrides in sub-Neptune exoplanets with thick hydrogen-rich atmospheres. [PDF]
Kim T+6 more
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Time of proto-Earth reservoir formation and volatile element depletion from <sup>53</sup>Mn-<sup>53</sup>Cr chronometry. [PDF]
Kruttasch PM, Mezger K.
europepmc +1 more source
Rare earth element nucleosynthetic anomalies and dust transport in the protoplanetary disk. [PDF]
Hu JY+11 more
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Enrichment of moderately volatile elements in first-generation planetesimals of the inner Solar System. [PDF]
Grewal DS+4 more
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The Ni isotopic composition of Ryugu reveals a common accretion region for carbonaceous chondrites. [PDF]
Spitzer F+90 more
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Long-chain alkanes preserved in a Martian mudstone. [PDF]
Freissinet C+21 more
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