The Absolute Chronology and Thermal Processing of Solids in the Solar Protoplanetary Disk

By J. Connelly, M. Bizzarro, A. Krot, Å. Nordlund, D. Wielandt, M. Ivanova. Science, 2012

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View Paper: https://www.semanticscholar.org/paper/0c751fd277de6a40af066a2348f27bd211772217

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In Astronomy and Astrophysics

Citations in the corpus

The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites (2017, background): “This is corroborated by Pb-Pb dating (Amelin et al. 2002; Connelly et al. 2017), although it is currently debated whether some fraction of chondrules formed contemporaneously with CAIs, i.e. at time t = 0 (Connelly et al. 2012).”
Astrophysics with Extraterrestrial Materials (2016, methodology): “In particular, application of the Pb-Pb and 26Al systems shows that CAIs are the oldest objects to have formed in the solar nebula, predating other meteoritic materials by as much as 3–5 Myr (Amelin et al. 2002, Brennecka et al. 2010, Connelly et al. 2012).”
Differentiated Planetesimals and the Parent Bodies of Chondrites (2013, background): “Such an early accretion time is broadly consistent with the fact that among chondrite groups, CV chondrites contain chondrules with some of the oldest crystallization ages (Bizzarro et al. 2004, Connelly et al. 2012, Kleine et al. 2009).”
Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, background): “However, the existence of a distinct time gap between the CAI and chondrule forming events is disputed by Connelly et al. (2012).”
26Al‐26Mg isotope systematics of the first solids in the early solar system (2013, neutral): “The relative Pb-Pb ages between several CAIs (Amelin et al. 2010; Connelly et al. 2012) and D’Orbigny (Amelin 2008; Brennecka and Wadhwa 2012) are approximately 3.8 Ma, which is approximately 1 Ma shorter than the Al-Mg age of the quenched angrites.”
Future climate forcing potentially without precedent in the last 420 million years (2017, background): “Radiative forcing from CO2 change can be calculated using equation (6).”
The Non-carbonaceous–Carbonaceous Meteorite Dichotomy (2020, background): “For most elements nucleosynthetic anomalies are most prominent in Ca-Al-rich inclusions (CAIs), the solar system’s oldest dated solids (Amelin et al. 2010; Connelly et al. 2012).”
Correlated accretion ages and ε54Cr of meteorite parent bodies and the evolution of the solar nebula (2014, background): “The 54Cr anomalies in five chondrules in carbonaceous chondrite (Allende) vary between 0.24 and 0.87e with an analytical error of 0.09e (Connelly et al. 2012).”
Chelyabinsk Airburst, Damage Assessment, Meteorite Recovery, and Characterization (2013, background): “The Chelyabinsk (LL) parent body experienced a substantial thermal and/or collision resetting event 115 ± 21 million years after the formation of the solar system (25), not experienced by most other LL chondrites, possibly due to a major impact event near its site of origin on the parent body.”
Water delivery and giant impacts in the 'Grand Tack' scenario (2014, neutral): “…planet formation extends from the condensation of the ﬁrst solids (cid:2) 4.567–4.568 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 4.1–3.8 Gyr ago (Tera et al., 1974; Chapman et al., 2007;…”
The Compositional Structure of the Asteroid Belt (2015, background): “, 2008) and the Pb-Pb systems (Amelin and Krot, 2007; Amelin et al., 2002; Connelly et al., 2012; Krot et al., 2005) to date chondrules.”
SPECTRAL PROPERTIES OF COOL STARS: EXTENDED ABUNDANCE ANALYSIS OF 1,617 PLANET-SEARCH STARS (2016, background): “Sodium Planetesimal formation mechanisms and timescales are still poorly understood, though 14 recent progress has been made on both (Moriarty & Fischer 2015; Leinhardt & Stewart 2012; Connelly et al. 2012).”