Pb–Pb dating constraints on the accretion and cooling history of chondrites

By A. Bouvier, J. Blichert‐Toft, F. Moynier, J. Vervoort, F. Albarède. 2007

166 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/92380f65d5d1dfa63d246400a5b15dded635120e

How researchers see this paper

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In Astronomy and Astrophysics

1. A. Morbidelli
2. T. Kleine
3. S. Raymond
4. B. Bourdon
5. Kevin J. Walsh
6. D. Nesvorný
7. C. Burkhardt
8. H. Palme

In Geophysics

1. B. Bourdon
2. T. Kleine
3. A. Morbidelli
4. C. Burkhardt
5. H. Palme
6. A. Halliday
7. F. Nimmo
8. S. Raymond

Citations in the corpus

• Hf-W thermochronometry: Closure temperature and constraints on the accretion and cooling history of the H chondrite parent body (2008, background): “First, the thermal evolution and structure of their parent bodies has already been studied with several chronometers (Wasserburg et al., 1969; Podosek and Brannon, 1991; Gopel et al., 1994; Trieloff et al., 2003; Amelin et al., 2005; Bouvier et al., 2007 ).”
• Chronology of the Solar System’s Oldest Solids (2008, background): “…and long-lived radioisotope chronometers, a number of studies have recently proposed an upward revision of the age of the solar system with estimates ranging from ∼4568 to ∼4571 Myr (Lugmair & Shukolyukov 1998; Nyquist et al. 2003; Baker et al. 2005; Bouvier et al. 2007; Burkhardt et al. 2007).”
• Hf–W mineral isochron for Ca,Al-rich inclusions: Age of the solar system and the timing of core formation in planetesimals (2008, methodology): “5 Ma Pb–Pb age for CAIs that has been determined from (207)Pb–(206)Pb data for selected fractions of CAIs from Allende and Murchison and Efremovka CAIs E60 and E49 (Bouvier et al., 2007).”
• STATISTICAL STUDY OF THE EARLY SOLAR SYSTEM'S INSTABILITY WITH FOUR, FIVE, AND SIX GIANT PLANETS (2012, background): “A protoplanetary nebula typically disperses in ∼3-10 Myr after the birth of the star (Haisch et al. 2001), which for the Sun was probably contemporary to the formation of the first Solar System solids, 4.568 Gyr ago (Bouvier et al. 2007, Burkhardt et al. 2008).”
• Building Terrestrial Planets (2012, background): “ zero” in every region of the proto-planetary disk, where “time zero” is usually identified with the formation time of the first solids, the calcium-aluminium inclusions (CAIs, dated at 4.568 Gy ago; Bouvier et al. 2007; Burkhardt et al. 2008). Sufficient clumping of small particles to form planetes”
• U-Pb chronology of the Solar System's oldest solids with variable 238 U/ 235 U (2010, result): “…relationships have been the subject of many recent studies (Amelin et al. 2002, Bizzarro et al. 2004, Thrane et al. 2006, Amelin and Krot 2007, Bouvier et al. 2007, Connelly et al. 2008a, Jacobsen et al. 2008, Burkhardt et al. 2008, Bouvier and Wadhwa 2009, Krot et al. 2009, Nyquist et al.…”
• Hf-W chronology of the accretion and early evolution of asteroids and terrestrial planets (2009, background): “One problem with this approach is that the absolute age of CAIs is not known with sufficient precision, with Pb–Pb ages ranging from 4567.11 ± 0.16 Myr (Amelin et al., 2002, 2006) to 4568.5 ± 0.5 Myr (Bouvier et al., 2007).”