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	<journal>
		<journal_title>eEarth Discussions</journal_title>
		<journal_url>www.electronic-earth-discuss.net</journal_url>
		<issn>1815-3836</issn>
		<eissn>1815-3844</eissn>
		<volume_number>2</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/eed-2-99-2007</doi>
	<article_url>http://www.electronic-earth-discuss.net/2/99/2007/</article_url>
	<abstract_html>http://www.electronic-earth-discuss.net/2/99/2007/eed-2-99-2007.html</abstract_html>
	<fulltext_pdf>http://www.electronic-earth-discuss.net/2/99/2007/eed-2-99-2007.pdf</fulltext_pdf>
	<start_page>99</start_page>
	<end_page>113</end_page>
	<publication_date>2007-07-10</publication_date>
	<article_title content_type="html">Noble gas signature of the late heavy bombardment in the Earth&apos;s atmosphere</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>B. Marty</name>
			<email>bmarty@crpg.cnrs-nancy.fr</email>
		</author>
		<author numeration="2" affiliations="2">
			<name>A. Meibom</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Centre de Recherches Pétrographiques et Géochimiques and Ecole Nationale Supérieure de Géologie, Nancy Universités, Nancy, France</affiliation>
		<affiliation numeration="2" content_type="html">Muséum National d&apos;Histoire Naturelle, Paris, France</affiliation>
	</affiliations>
	<abstract content_type="html">The Lunar cratering record is consistent with the occurrence of a late heavy
bombardment (LHB), which marked the end of terrestrial planet accretion 3.8
billion years ago. However, clear evidence of a LHB on Earth has not yet
been identified. Here it is shown that the LHB did indeed occur on Earth and
that we are breathing its aftermaths. The terrestrial atmosphere and
hydrosphere is enriched in noble gases relative to the abundance of
volatiles in the mantle. This enrichment is consistent with the mass
delivered to Earth during the LHB only if this material consisted of
~0.5% Kuiper-belt objects mixed in with a population of largely
chondritic (i.e. asteroidal) impactors. This places strong constraints on
dynamical models for early Solar System evolution.</abstract>
	<references>
		<reference numeration="1" content_type="text"> Anders, E.: Abiotic organic matter from comets and asteroids, Nature, 342, 255&amp;ndash;257, 1989. </reference>
		<reference numeration="2" content_type="text"> Ballentine, C. J., Marty, B., Lollar, B. S., and Cassidy, M.: Neon isotopes constrain convection and volatile origin in the Earth&apos;s mantle, Nature, 433, 33&amp;ndash;38, 2005. </reference>
		<reference numeration="3" content_type="text"> Bar-Nun, A., Herman, G., Laufer, D., and Rappaport, M. L.: Trapping and release of gases by water ice and implications for icy bodies, Icarus, 63, 317&amp;ndash;332, 1985. </reference>
		<reference numeration="4" content_type="text"> Bell, D. R. and Rossman, G. R.: Water in the Earth&apos;s mantle: the role of anhydrous minerals, Science, 255, 1391&amp;ndash;1397, 1992. </reference>
		<reference numeration="5" content_type="text"> Bockelée-Morvan, D., Crovisier, J., Mumma, M. J., and Weaver, H. A.: The composition of cometary volatiles, in: Comets 2, edited by: Festou, M. C., Keller, H. U., and Weaver, H. A., Univ. Arizona Press, 391&amp;ndash;423, 2004. </reference>
		<reference numeration="6" content_type="text"> Dauphas, N.: The dual origin of the terrestrial atmosphere, Icarus, 165, 326&amp;ndash;339, 2003. </reference>
		<reference numeration="7" content_type="text"> Delsemme, A. H. and Swings, P.: Gas hydrates in cometary nuclei and interstellar grains, Ann. Astrophys., 15, 1&amp;ndash;6, 1952. </reference>
		<reference numeration="8" content_type="text"> Frei, R. and Rosing, M. T.: Search for traces of the late heavy bombardment on Earth-Results from high precision chromium isotopes, Earth Planet. Sci. Lett., 236, 28&amp;ndash;40, 2005. </reference>
		<reference numeration="9" content_type="text"> Gomes, R., Levison, H. F., Tsiganis, K., and Morbidelli, A.: Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets, Nature, 435, 466&amp;ndash;469, 2005. </reference>
		<reference numeration="10" content_type="text"> Hartmann, W. K., Ryder, G., Dones, L., and Grinspoon, D.: The time-dependent intense bombardment of the primordial Earth/Moon system, in: Origin anf the Earth and Moon, edited by: Canup, R. M. and Righter, K., Univ. Arizona Press, Tucson, 493&amp;ndash;512, 2000. </reference>
		<reference numeration="11" content_type="text"> Hersant, F., Gautier, D., and Hure, J. M.: A two-dimensional model for the primordial nebula constrained by D/H measurements in the solar system: Implications for the formation of giant planets, Astrophys. J., 554, 391&amp;ndash;407, 2001. </reference>
		<reference numeration="12" content_type="text"> Iro, N., Gautier, D., Hersant, F., Bockelee-Morvan, D., and Lunine, J. I.: An interpretation of the nitrogen deficiency in comets, Icarus, 161, 511&amp;ndash;532, 2003. </reference>
		<reference numeration="13" content_type="text"> Jambon, A. and Zimmermann, J. L.: Water in Oceanic Basalts &amp;ndash; Evidence for Dehydration of Recycled Crust, Earth Planet. Sci. Lett., 101, 323&amp;ndash;331, 1990. </reference>
		<reference numeration="14" content_type="text"> Keppler, H. and Bolfan-Casanova, N.: Thermodynamics of water solubility and partitioning, in: Water in Nominally Anhydrous Minerals, Rev. Mineral. Geochem., 62, 193&amp;ndash;230, 2006. </reference>
		<reference numeration="15" content_type="text"> Lunine, J. I. and Stevenson, D. J.: Thermodynamics of clathrate hydrate at low and high pressures with application to the outer solar system, Astrophys. J., 58, 493&amp;ndash;531, 1985. </reference>
		<reference numeration="16" content_type="text"> Marty, B.: Nitrogen content of the mantle inferred from N&lt;sub&gt;2&lt;/sub&gt;-Ar correlation in oceanic basalts, Nature, 377, 326&amp;ndash;329, 1985. </reference>
		<reference numeration="17" content_type="text"> Marty, B. and Dauphas, N.: The nitrogen record of crust-mantle interaction from Archean to Present, Earth Planet. Sci. Lett., 206, 397&amp;ndash;410, 2003. </reference>
		<reference numeration="18" content_type="text"> Marty, B. and Zimmermann, L.: Volatiles (He, C, N, Ar) in mid-ocean ridge basalts: Assessment of shallow-level fractionation and characterization of source composition, Geochim. Cosmochim. Acta, 63, 3619&amp;ndash;3633, 1999. </reference>
		<reference numeration="19" content_type="text"> McDonough, W. F., Sun, S. S., Ringwood, A. E., Jagoutz, E., and Hofmann, A. W.: Potassium, rubidium and cesium in the Earth and Moon and the evolution of the mantle of the Earth, Geochim. Cosmochim. Acta, 56, 1001&amp;ndash;1012, 1992. </reference>
		<reference numeration="20" content_type="text"> McKeegan, K. D., Aleon, J., Bradley, J., et al.: Isotopic compositions of cometary matter returned by Stardust, Science, 314, 1724&amp;ndash;1728, 2006. </reference>
		<reference numeration="21" content_type="text"> Miller, S. L.: A production of amino acids under possible primitive Earth conditions, Science, 117, 528&amp;ndash;530, 1953. </reference>
		<reference numeration="22" content_type="text"> Mojzsis, S., Arrhenius, G., McKeegan, K. D., et al.: Evidence for life on Earth before 3800 million years ago, Nature, 384, 55&amp;ndash;59, 1996. </reference>
		<reference numeration="23" content_type="text"> Morbidelli, A., Levison, H. F., Tsiganis, K., and Gomes, R.: Chaotic capture of Jupiter&apos;s Trojan asteroids in the early Solar System, Nature, 435, 462&amp;ndash;465, 2005. </reference>
		<reference numeration="24" content_type="text"> Moreira, M., Kunz, J., and Allègre, C. J.: Rare gas systematics in Popping Rock: Isotopic and elemental compositions in the upper mantle, Science, 279, 1178&amp;ndash;1181, 1998. </reference>
		<reference numeration="25" content_type="text"> Notesco, G. and Bar-Nun, A.: A ~25 K temperature fo formation for the submicron ice grains which formed comets, Icarus, 175, 546&amp;ndash;550, 2005. </reference>
		<reference numeration="26" content_type="text"> Owen, T., Bar-Nun, A., and Kleinfeld, I.: Possible cometary origin of heavy noble gases in the atmospheres of Venus, Earth and Mars, Nature, 358, 43&amp;ndash;46, 1992. </reference>
		<reference numeration="27" content_type="text"> Owen, T., Mahaffy, P., Niemann, H. B., et al.: A low-temperature origin for the planetesimals that formed Jupiter, Nature, 402, 269&amp;ndash;270, 1999. </reference>
		<reference numeration="28" content_type="text"> Pepin, R. O.: On the origin and early evolution of terrestrial planetary atmospheres and meteoritic volatiles, Icarus, 92, 1&amp;ndash;79, 1991. </reference>
		<reference numeration="29" content_type="text"> Porcelli, D. and Pepin, R. O.: Rare gas constraints on Early Earth history, in: Origin of the Earth and Moon, edited by: Canup, R. M. and Righter, K., Univ. Arizona Press, Tucson, 435&amp;ndash;458, 2000. </reference>
		<reference numeration="30" content_type="text"> Rosing, M. T.: C-13-depleted carbon microparticles in &amp;gt;3700-Ma sea-floor sedimentary rocks from west Greenland, Science, 283, 674&amp;ndash;676, 1999. </reference>
		<reference numeration="31" content_type="text"> Ryder, G., Koeberl, C., and Mojzsis, S. J.: Heavy bombardment of the Earth at $\sim $3.85 Ga: The search for petrographic and geochemichal evidence, in: Origin and the Earth and Moon, edited by: Canup, R. M. and Righter, K., Univ. Arizona Press, Tucson, 475&amp;ndash;492, 2000. </reference>
		<reference numeration="32" content_type="text"> Saal, A. E., Hauri, E. H., Langmuir, C. H., and Perfit, M. R.: Vapour undersaturation in primitive mid-ocean-ridge basalt and the volatile content of Earth&apos;s upper mantle, Nature, 419, 451&amp;ndash;455, 2002. </reference>
		<reference numeration="33" content_type="text"> Schoenberg, R., Kamber, B. S., Collerson, K. D., and Moorbath, S.: Tungsten isotope evidence from 3.8-Gyr metamorphosed sediments for early bombardment of the Earth, Nature, 418, 403&amp;ndash;405, 2002. </reference>
		<reference numeration="34" content_type="text"> Tolstikhin, I. N. and Marty, B.: The evolution of terrestrial volatiles: a view from helium, neon, argon and nitrogen isotope modelling, Chem. Geol., 147, 27&amp;ndash;52, 1998. </reference>
		<reference numeration="35" content_type="text"> Trieloff, M. and Kunz, J.: Isotope systematics of noble gases in the Earth&apos;s mantle: possible sources of primordial isotopes and implications for mantle structure, Phys. Earth Planet. Int., 148, 13&amp;ndash;38, 2005. </reference>
		<reference numeration="36" content_type="text"> Tsiganis, K., Gomes, R., Morbidelli, A., and Levison, H. F.: Origin of the orbital architecture of the giant planets of the Solar System, Nature, 435, 459&amp;ndash;461, 2005. </reference>
		<reference numeration="37" content_type="text"> Yokochi, R. and Marty, B.: A determination of the neon isotopic composition of the deep mantle, Earth Planet. Sci. Lett., 225, 77&amp;ndash;88, 2004. </reference>
		<reference numeration="38" content_type="text"> Yokochi, R. and Marty, B.: Geochemical constraints on mantle dynamics in the Hadean, Earth Planet. Sci. Lett., 238, 17&amp;ndash;30, 2005. </reference>
		<reference numeration="39" content_type="text"> Zahnle, K. J.: Earth&apos;s earliest atmosphere, Elements, 2, 217&amp;ndash;222, 2006. </reference>
	</references>
</article>

