Did the terrestrial planets of the Solar System form by pebble accretion?OPEN ACCESS
Alessandro Morbidelli, Thorsten Kleine, Francis Nimmo In press as a Frontier paper in Earth and Planetary Science Letters PDF (OPEN ACCESS) “The dominant accretion process leading to the formation of the terrestrial planets of the…
Large Carbonaceous Chondrite Parent Bodies Favored by Abundance–Volatility Modeling: A Possible Chemical Signature of Pebble AccretionOPEN ACCESS
Jeremy W. Boyce, Francis M. McCubbin, Nicole Lunning and Tyler Anderson The Planetary Science Journal, Volume 5, Number 2 LINK (OPEN ACCESS)PDF (OPEN ACCESS) “Primitive meteorite groups such as the Vigarano, Mighei, and Karoonda carbonaceous…
Making the Solar SystemOPEN ACCESS
John Chambers Accepted for publication in the Astrophysical Journal PDF (OPEN ACCESS) Update (16 February 2023): The Astrophysical Journal, Volume 944, Number 2LINK (OPEN ACCESS)PDF (OPEN ACCESS) “We model the early stages of planet formation…
Rapid formation of massive planetary cores in a pressure bumpOPEN ACCESS
T.C.H. Lau, J. Dra̧żkowska, S.M. Stammler, T. Birnstiel, C.P. Dullemond Astronomy & Astrophysics, manuscript no. 44864corrReceived: 01 September 2022 / Accepted: 08 November 2022 PDF (OPEN ACCESS) “Context. Models of planetary core growth by either…
Solar System evolution and terrestrial planet accretion determined by Zr isotopic signatures of meteoritesOPEN ACCESS
Jan Render, Gregory A. Brennecka, Christoph Burkhardt, Thorsten Kleine Earth and Planetary Science LettersVolume 595, 1 October 2022, 117748 LINK (OPEN ACCESS) “Highlights • We present new Zr isotope data for a comprehensive suite of…
Anatomy of rocky planets formed by rapid pebble accretion II. Differentiation by accretion energy and thermal blanketingOPEN ACCESS
Anders Johansen, Thomas Ronnet, Martin Schiller, Zhengbin Deng, Martin Bizzarro Version accepted for Astronomy & Astrophysics PDF (OPEN ACCESS) “We explore the heating and differentiation of rocky planets that grow by rapid pebble accretion. Our…
Anatomy of rocky planets formed by rapid pebble accretion I. How icy pebbles determine the core fraction and FeO contentsOPEN ACCESS
Anders Johansen, Thomas Ronnet, Martin Schiller, Zhengbin Deng, Martin Bizzarro Version accepted for Astronomy & Astrophysics PDF (OPEN ACCESS) “We present a series of papers dedicated to modelling the accretion and differentiation of rocky planets…
Core segregation during pebble accretion
Peter Olson, Zachary Sharp, Susmita Garai Earth and Planetary Science LettersVolume 587, 1 June 2022, 117537 LINK “Highlights • Pebble accretion builds terrestrial protoplanets in a few million years.• Core segregation is synchronized to the…
Effects of pebble accretion on the growth and composition of planetesimals in the inner Solar SystemOPEN ACCESS
J. Mah, R. Brasser, A. Bouvier, S. J. Mojzsis accepted for publication in MNRAS PDF (OPEN ACCESS) “Recent work has shown that aside from the classical view of collisions by increasingly massive planetesimals, the accretion…
Terrestrial planet formation from lost inner solar system materialOPEN ACCESS
Christoph Burkhardt, Fridolin Spitzer, Alessandro Morbidelli, Gerrit Budde, Jan H. Render, Thomas S. Kruijer and Thorsten Kleine Science Advances, 22 Dec 2021, Vol 7, Issue 52 LINK (OPEN ACCESS)PDF (OPEN ACCESS) “Two fundamentally different processes…
The Effect of a Strong Pressure Bump in the Sun’s Natal Disk: Terrestrial Planet Formation via Planetesimal Accretion Rather than Pebble Accretion
André Izidoro, Bertram Bitsch, and Rajdeep Dasgupta The Astrophysical Journal, Volume 915, Number 1 LINK “Mass-independent isotopic anomalies of carbonaceous and noncarbonaceous meteorites show a clear dichotomy suggesting an efficient separation of the inner and…
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…
Magnetization of Large C-Type Asteroids: A Detectable Consequence of Pebble Accretion?
S. W. Courville, O’Rourke J. G., Castillo-Rogez J. C., Oran R., Weiss B. P. et al. 52nd Lunar and Planetary Science Conference (2021), Abstract #2355 PDF “The theory of pebble accretion implies that large planetesimals…
The formation of Jupiter by hybrid pebble–planetesimal accretionOPEN ACCESS
Yann Alibert, Julia Venturini, Ravit Helled, Sareh Ataiee, Remo Burn, Luc Senecal, Willy Benz, Lucio Mayer, Christoph Mordasini, Sascha P. Quanz & Maria Schönbächler Nature Astronomy (2018) PDF (OPEN ACCESS) LINK “The standard model for…
Forming Chondrites in a Solar Nebula with Magnetically Induced Turbulence
Yasuhiro Hasegawa, Neal J. Turner, Joseph Masiero, Shigeru Wakita, Yuji Matsumoto, Shoichi Oshino Updated (16 March 2016): abstract Yasuhiro Hasegawa et al 2016 ApJ 820 L12 PDF (open access) abstract “Chondritic meteorites provide valuable opportunities…
The growth of planets by pebble accretion in evolving protoplanetary discs
Bertram Bitsch, Michiel Lambrechts and Anders Johansen A&A Volume 582, October 2015, A112 Published online: 20 October 2015 DOI: http://dx.doi.org/10.1051/0004-6361/201526463 LINK
Evidence for Pebbles in Comets
K.A. Kretke, H.F. Levison Icarus In Press, Accepted Manuscript, Available online 20 August 2015 PDF (full text) abstract
Growing the gas-giant planets by the gradual accumulation of pebbles
Harold F. Levison Katherine A. Kretke Martin J. Duncan Nature 524, 322–324 (19 August 2015) | doi:10.1038/nature14675 LINK
