A short duration of chondrule formation in the solar nebula: evidence from 26Al in Semarkona ferromagnesian chondrules

By N. Kita, H. Nagahara, S. Togashi, Y. Morishita. 2000

223 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/7cbb5d23992ce214b431d386a7a7f818498d7944

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In Astronomy and Astrophysics

1. N. Dauphas
2. T. Kleine
3. B. Bourdon
4. F. DeMeo
5. C. Alexander
6. M. Chaussidon
7. Kevin J. Walsh
8. Clark R. Chapman

In Atmospheric Science

1. N. Dauphas
2. M. Chaussidon
3. T. Kleine
4. B. Bourdon
5. P. Caselli
6. Cecilia Ceccarelli
7. Kevin J. Walsh
8. F. Nimmo

Citations in the corpus

• A Perspective from Extinct Radionuclides on a Young Stellar Object: The Sun and Its Accretion Disk (2011, background): “…(solid curve) and 44 from carbonaceous chondrites (dashed curve); data from Hsu et al. 2003; Hutcheon & Hutchison 1989; Hutcheon et al. 2000; Kita et al. 2000, 2005b; Kunihiro et al. 2004; Kurahashi et al. 2008; Mostéfaoui et al. 2000; Nagashima et al. 2007, 2008; Rudraswami & Goswami 2007;…”
• Hf-W chronology of the accretion and early evolution of asteroids and terrestrial planets (2009, background): “Based on 26Al–26Mg and Pb–Pb ages it is well established that most chondrules formed 2–3 Myr after CAIs (Kita et al., 2000; Amelin et al., 2002; Kunihiro et al., 2004; Rudraswami and Goswami, 2007; Connelly et al., 2008a; Kurahashi et al., 2008; Rudraswami et al., 2008).”
• The Initial Abundance of 60Fe in the Solar System (2003, background): “Ion-microprobe studies of olivine phenocrysts in chondrules, submillimeter-sized once-molten spherules that are a major constituent of chondrites, gave no resolvable60Ni* in the unequilibrated ordinary chondrites Semarkona and Bishunpur (Kita et al. 2000; Choi et al. 1999).”
• Our astrochemical heritage (2012, background): “Since its discovery in meteorites, 26Al (Kita et al. 2000; Villeneuve et al. 2009) became one of the proofs, indeed highly debated for decades, that the Solar System was polluted with material ejected from a nearby type II supernova, whose progenitor mass is ∼25 M (Cameron and Truran 1977; Gounelle…”
• The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites (2017, unknown): “…Bollard et al. (2017); s. Al-Mg: Rudraswami et al. (2008); t. Al-Mg: Mostefaoui et al. (2002); u. Al-Mg: Villeneuve et al. (2009); v. Al-Mg: Kurahashi et al. (2008); w. Al-Mg: Kita et al. (2000); x. Hf-W: Budde et al. (2016); y. Al-Mg: Nagashima et al. (2015); z. Al-Mg: Hutcheon et al. (2009); aa.”
• A model for planetesimal meltdown by 26Al and its implications for meteorite parent bodies (2006, result): “The late accretion of chondritic parent bodies is, of course, consistent with the young ages of around t = 2 Myr reported for many chondrules (Kita et al. 2000; Huss et al. 2001; Amelin et al. 2002).”
• Chondrules and the Protoplanetary Disk (2011, unknown): “Sources of data: (1) McKeegan et al. (2000), (2) Kita et al. (2000), (3) Mostefaoui et al. (2002), (4) Amelin et al. (2004), (5) Bizzarro et al. (2004), (6) Kurahashi et al. (2004), (7) Amelin et al. (2002), (8) unpublished data of Amelin and coworkers cited by Kita et al. 2005.”
• The Compositional Structure of the Asteroid Belt (2015, background): “Kitamura, M. (1959) Photoelectric study of colors of asteroids and meteorites.”