Terrestrial planet and asteroid belt formation by Jupiter–Saturn chaotic excitationOPEN ACCESS
Patryk Sofia Lykawka & Takashi Ito Scientific Reports, Volume 13, Article number: 4708 LINK (OPEN ACCESS)PDF (OPEN ACCESS) “The terrestrial planets formed by accretion of asteroid-like objects within the inner solar system’s protoplanetary disk. Previous…
Characterization of a 2700 KM long bolide airburst chain, Phoebe Regio, Venus.
E.G. Antropova, C.H.G. Braga, R.E. Ernst, H. El Bilali, J.W. Head, B.A. Ivanov Planetary and Space ScienceAvailable online 7 February 2023 LINK “Detailed geological mapping of Phoebe Regio on Venus, located near 10°S, 282°W, at…
Experiments on the reactivity of basaltic minerals and glasses in Venus surface conditions using the Glenn Extreme Environment RigOPEN ACCESS
Brandon G. Radoman-Shaw, Ralph P. Harvey, Gustavo Costa, Nathan S. Jacobson, Amir Avishai, Leah M. Nakley, Daniel Vento MAPSFirst published: 14 September 2022 LINK (OPEN ACCESS)PDF (OPEN ACCESS) “Climate models for Venus rely heavily on…
Chemical Differentiation of Planets: A Core IssueOPEN ACCESS
Hervé Toulhoat, Viacheslav Zgonnik The Astrophysical Journal, Volume 924, Number 2Published: 14 January 2022 LINK (OPEN ACCESS)PDF (OPEN ACCESS) “By plotting empirical chemical element abundances on Earth relative to the Sun and normalized to silicon…
A pebble accretion model for the formation of the terrestrial planets in the Solar SystemOPEN ACCESS
Anders Johansen, Thomas Ronnet, Martin Bizzarro, Martin Schiller, Michiel Lambrechts, Åke Nordlund, Helmut Lammer Science Advances, 17 Feb 2021:Vol. 7, no. 8, eabc0444DOI: 10.1126/sciadv.abc0444 LINK (OPEN ACCESS)PDF (OPEN ACCESS) “Pebbles of millimeter sizes are abundant…
What is the Oxygen Isotope Composition of Venus? The Scientific Case for Sample Return from Earth’s “Sister” PlanetOPEN ACCESS
Richard C. Greenwood & Mahesh Anand Space Science Reviews, Volume 216, Article number: 52 (2020) LINK (OPEN ACCESS)PDF (OPEN ACCESS) “Venus is Earth’s closest planetary neighbour and both bodies are of similar size and mass….
40Ar/39Ar and (U-Th)/He model age signatures of elusive Mercurian and Venusian meteorites.
Jourdan, F. and Eroglu, E. Meteoritics & Planetary Science. doi: 10.1111/maps.12838 LINK “No meteorites from Mercury and Venus have been conclusively identified so far. In this study, we develop an original approach based on extensive…
Ground-based IR observation of oxygen isotope ratios in the Venus atmosphere
N. Iwagami, G.L. Hashimoto, S. Ohtsuki, S. Takagi, S. Robert Planetary and Space Science available online 12 November 2014 LINK Correlation plot of δ17O and δ18O in Earth-Moon, Mars and Venus
