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- W2070954477 abstract "Determining the source of Earth's oceans is a longstanding problem in planetary science. Possible sources of water include water ice or water of hydration of silicate minerals in the original material from which the bulk Earth accreted and water brought in by late‐arriving planetesimals during the heavy bombardment period (4.5–3.8 Gyr ago) [ Chyba , 1989, 1991]. Comets are an attractive source of water because their origin in the outer solar system is consistent with the long timescale for heavy bombardment. However, the high deuterium/hydrogen (D/H) ratio of the three comets that have been studied, Halley, Hyakutake, and Hale‐Bopp, indicates that Earth must have had a source with a low‐D/H ratio as well. Here we suggest that solar wind‐implanted hydrogen on interplanetary dust particles (IDPs) provided the necessary low‐D/H component of Earth's water inventory." @default.
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- W2070954477 date "1999-12-01" @default.
- W2070954477 modified "2023-09-27" @default.
- W2070954477 title "Irradiated interplanetary dust particles as a possible solution for the deuterium/hydrogen paradox of Earth's oceans" @default.
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- W2070954477 doi "https://doi.org/10.1029/1999je001120" @default.
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