The age of the Solar System redefined by the oldest Pb–Pb age of a meteoritic inclusion
By A. Bouvier, M. Wadhwa. 2010
366 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/141c1d36907c6d26ad7dc1edbb5a01bb7c482746
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Citations in the corpus
- 26Al‐26Mg isotope systematics of the first solids in the early solar system (2013, unknown): “Another is b = 0.514 according to the evaporation experiments of CAI-like melt (Davis et al. 2005), which has been used for several internal isochron studies of igneous CAIs (e.g., Bouvier and Wadhwa 2010; Kita et al. 2012).”
- Evolution of protoplanetary disk inferred from 26Al chronology of individual chondrules (2012, methodology): “3 Myr (Bouvier and Wadhwa 2010), the Gujba chondrules formed 6.”
- HETEROGENEOUS DISTRIBUTION OF 26Al AT THE BIRTH OF THE SOLAR SYSTEM (2010, background): “The uranium–lead absolute chronology (Amelin et al. 2002; Amelin and Krot 2007; Bouvier and Wadhwa 2010; Bouvier et al. 2011a) and aluminum–magnesium relative chronology (Kita et al.”
- U-Pb chronology of the Solar System's oldest solids with variable 238 U/ 235 U (2010, methodology): “The CAIs from both age groups have well preserved 26 Al26 Mg systems (Amelin et al. 2002, Jacobsen et al. 2008, Bouvier and Wadhwa 2010) that yield initial 26 Al/ 27 Al close to the canonical value and suggest simultaneous formation.”
- Correlated accretion ages and ε54Cr of meteorite parent bodies and the evolution of the solar nebula (2014, methodology): “Bouvier and Wadhwa (2010) reported an internal isochron age of 4568.2 (+0.2/ 0.4) Ma for a CAI in NWA 2364 using an estimated 238U/235U ratio (137.81 ~ 137.83).”
- Stellar magnetism: empirical trends with age and rotation (2014, unknown): “…(2014); 64: Morin et al. (2008b); 65: Morin et al. (2010); 66: Schmitt, Fleming & Giampapa (1995); 67: Morin et al. (2008a); 68: Peres et al. (2000); 69: Bouvier & Wadhwa (2010); 70: Donati et al. (2010a); 71: Johnstone et al. (2014); 72: Siess, Dufour & Forestini (2000); 73: Gregory et al.…”
- Early life on land and the first terrestrial ecosystems (2013, background): “The oldest materials yet found in the Solar System occur in meteorites and are ~4,570 Ma (Mega annum, million years) of age (Bouvier and Wadhwa 2010), which may serve as a starting point for the condensation of the first solids in our Solar System.”
- Astrophysics with Extraterrestrial Materials (2016, background): “The Solar System formed 4.6 Gyr ago from an interstellar molecular cloud consisting of gas and dust produced throughout the previous ∼8 Gyr of galactic history.”
- Magma oceans in the inner solar system (2012, background): “…range of times of Moon-forming impact (constrained by ages above) b d e f g h i j k l m n o a c Selected age of first solids in solar system (Bouvier & Wadhwa 2010) 4.5682 Gya Lunar formation and differentiation (time of the giant impact) Core formation in iron meteorite parent…”
- Chronology of the angrite parent body and implications for core formation in protoplanets (2012, methodology): “3: (i) CAI SJ101 with a Pb–Pb age of 4567.2 ± 0.5 Ma, calculated using its measured U isotopic composition (Amelin et al., 2010); and (ii) CAI 2364 B-1 from the CV chondrite NWA 2364, for which Bouvier and Wadhwa (2010) reported a Pb–Pb age of 4568.22 ± 0.17 Ma.”
- A Perspective from Extinct Radionuclides on a Young Stellar Object: The Sun and Its Accretion Disk (2011, background): “Bouvier & Wadhwa (2010) did not measure directly the U isotopic composition in the CAI that they analyzed; instead, they estimated it on the basis of the observed chemical composition and obtained an age of Myr.”
- Water delivery and giant impacts in the 'Grand Tack' scenario (2014, unknown): “568 Gyr ago (Amelin et al., 2002; Bouvier and Wadhwa, 2010; Connelly et al., 2012) until the end of heavy bombardment of the inner Solar System around 4.”