1996
DOI: 10.1093/mnras/283.2.551
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The flux of meteorites to the Earth over the last 50 000 years

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Cited by 132 publications
(113 citation statements)
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“…The accretion of cosmic material might seem at first a reasonable hypothesis for planetary mass growth. All bodies in the solar system formed by the aggregation of gas and dust in the primitive solar nebula, and extraterrestrial material is constantly falling on Earth (Bland et al, 1996;PeuckerEhrenbrink, 1996;Karner et al, 2003;Yada et al, 2004;Zolensky, 2006), sometimes with very dramatic effects (Alvarez et al, 1980;French, 1998;Chapman, 2004). However, during the formation of the solar system, the growing planets cleaned their orbits of residual material and, when the Sun reached the necessary mass to trigger nuclear fusion reactions, the solar wind expelled what remained of the original cloud (Taylor, 2001;Righter and O'Brien, 2011).…”
Section: P Sudiro: the Earth Expansion Theorymentioning
confidence: 99%
“…The accretion of cosmic material might seem at first a reasonable hypothesis for planetary mass growth. All bodies in the solar system formed by the aggregation of gas and dust in the primitive solar nebula, and extraterrestrial material is constantly falling on Earth (Bland et al, 1996;PeuckerEhrenbrink, 1996;Karner et al, 2003;Yada et al, 2004;Zolensky, 2006), sometimes with very dramatic effects (Alvarez et al, 1980;French, 1998;Chapman, 2004). However, during the formation of the solar system, the growing planets cleaned their orbits of residual material and, when the Sun reached the necessary mass to trigger nuclear fusion reactions, the solar wind expelled what remained of the original cloud (Taylor, 2001;Righter and O'Brien, 2011).…”
Section: P Sudiro: the Earth Expansion Theorymentioning
confidence: 99%
“…Wlotzka et al 1995) had used a petrographic weathering estimate, however, Bland et al (1998) introduced the idea of using Mössbauer spectroscopy, where the relative amounts of Fe in different valence states could be measured. Bland et al (1996) further showed that meteorites of different composition weather at different rates, a fact known qualitatively to many meteoriticists, but difficult to quantify. Mössbauer provides that quantitation, and Bland et al (1996) showed that H chondrites, which contain more metallic iron, weather at faster rates than L chondrites.…”
Section: Desert Meteoritesmentioning
confidence: 99%
“…If the high pairing were the case, any estimates of infall rates would be too high, as our calculations of infall rates rely on an estimate of the total number of meteorites collected in our to scale our observed age distributions to the whole population. We can compare the estimates of infall rate from different areas and the results summarized by Bland et al (1996) in Table 5. Here we can see that the estimates from Allan Hills are not in disagreement with other estimates.…”
Section: Antarctic Meteoritesmentioning
confidence: 99%
“…They have been used to estimate the meteorite accretion rate (e.g., Bland et al 1996a), identify multiple fragments of single preatmospheric bodies (Benoit et al 2000), assess the role and rate of weathering processes (Bland et al 1996b), understand meteorite concentration mechanisms (e.g., Zolensky et al 1990), and constrain the environmental and geological history of the locations where they are found Folco et al 2006). A recent review of meteorite terrestrial ages and their significance is given by Jull (2006).…”
Section: Introductionmentioning
confidence: 99%