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Erratum: "Inward Radial Mixing of Interstellar Water Ices in the Solar Protoplanetary Disk" (2016, ApJL, 827, L1)

The bulk D/H value of the CM chondrite Paris(i.e.,(167±0.2)×10−6)reported in the published article is incorrect(Vacheret al.2016). The D/HSMOWvalue used for the D/H calculation was 149×10−6(i.e., D/H ratio of the Bulk Silicate Earth; Lécuyeret al.1998)instead of 155.76×10−6(i.e., D/H ratio of the...

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Published in:Astrophysical journal. Letters 2017-02, Vol.836 (1), p.L16
Main Authors: Vacher, Lionel G., Marrocchi, Yves, Verdier-Paoletti, Maximilien J., Villeneuve, Johan, Gounelle, Matthieu
Format: Article
Language:English
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Summary:The bulk D/H value of the CM chondrite Paris(i.e.,(167±0.2)×10−6)reported in the published article is incorrect(Vacheret al.2016). The D/HSMOWvalue used for the D/H calculation was 149×10−6(i.e., D/H ratio of the Bulk Silicate Earth; Lécuyeret al.1998)instead of 155.76×10−6(i.e., D/H ratio of the Standard Mean Ocean Water). It implies that(i)all the bulk D/H valuesof Paris displayed in the Letter must be replaced by 174.5×10−6and(ii)our previous estimation of the contribution interstellarwater ice in Paris should be reevaluated to 20.6%(instead of 19%; page 5). However, the histogram distribution of bulk D/H ratiosof CM chondrites(Figure 1)is correct, and the new bulk D/H value of Paris does not change the interpretations of the Letter.
ISSN:2041-8205
2041-8213
DOI:10.3847/2041-8213/836/1/L16