47 citations · 72 across the 6 of their papers we have counts for
8 papers · 1 filter
Non-equilibrium condensation of the first Solar System solids
Sebastien Charnoz, Jérome Aleon, Marc Chaussidon +3
Primitive meteorites (chondrites) consist of an out-of-equilibrium assemblage of minerals formed during the assembling of our Solar Nebula. The conditions under which their precurs…
A chemical perspective on planet formation in reduced systems
Urja Zaveri, Haiyang S. Wang, Paolo A. Sossi
Relative abundances of refractory elements in planets are commonly assumed to reflect those of their host stars. However, because elements are classified according to their behavio…
Hydrodynamic outflows of proto-lunar disk volatiles
Kaveh Pahlevan, Andrew N. Youdin, Paolo A. Sossi
Volatile elements - those that vaporize at low temperatures - are depleted in lunar rocks relative to terrestrial rocks. This systematic chemical depletion is evidence for vaporiza…
Proto-planetary disk composition-dependent element volatility in the context of rocky planet formation
Rob J. Spaargaren, Oliver Herbort, Haiyang S. Wang +2
The compositions of the Solar System terrestrial bodies are fractionated from that of the Sun, where elemental depletions in the bulk rocky bodies correlate with element volatility…
Interior Controls on the Habitability of Rocky Planets
Cedric Gillmann, Kaustubh Hakim, Diogo Lourenco +2
No matter how fascinating and exotic other terrestrial planets are revealed to be, nothing generates more excitement than announcements regarding their habitability. From the obser…
A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO. Radial velocities lead to the detection of transits with low signal-to-noise ratio
M. Damasso, J. Rodrigues, A. Castro-González +52
We followed-up with ESPRESSO the K0V star HIP 29442 (TOI-469), already known to host a validated sub-Neptune companion TOI-469.01. We aim to verify the planetary nature of TOI-469.…