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b | . The water content of Comet Tempel 1 was 38% by mass. [See Endnote 4 on page 282.] |
c | . “Hence, if comets like Hale-Bopp brought in the Earth’s water, they would have brought in a factor of 40,000 times more argon than is presently in the atmosphere.” T. D. Swindle and D. A. Kring, “Implications of Noble Gas Budgets for the Origin of Water on Earth and Mars,” Eleventh Annual V. M. Goldschmidt Conference, Abstract No. 3785 (Houston: Lunar and Planetary Institute, 20–24 May 2001). [To learn how comets probably collected argon, see Endnote 36 on page 285.] |
| D/H is the ratio of heavy hydrogen (also called deuterium, or D) to normal hydrogen (H). Drake and Righter give many other reasons why meteorites could not have provided much of Earth’s water. |
| After reading pages 260–310, you will see that the water in comets, asteroids, and meteoroids—as well as some water detected elsewhere in the inner solar system—came primarily from the subterranean water chambers. During the flood, this subterranean water mixed with Earth’s surface water, giving our surface water different isotope characteristics from water in comets, asteroids, and meteoroids. |