title: Preservation of extraterrestrial 3He in 480-Ma-old marine limestones.
abstract: We have measured the helium abundance and isotopic composition of a suite of Lower Ordovician marine limestones and associated fossil meteorites from Kinnekulle, Sweden. Limestone 3He/4He ratios as high as 11.5 times the atmospheric value in fused samples and up to 23 times atmospheric in a single step-heat fraction indicate the presence of extraterrestrial helium, and demonstrate that at least a fraction of the extraterrestrial 3He carried by interplanetary dust particles must be retained against diffusive and diagenetic losses for up to 480 Ma. The carrier phase has not been identified but is not magnetic. Extrapolation of high-temperature 3He diffusivities in these sediments is consistent with strong retention of extraterrestrial 3He under ambient Earth-surface conditions. Combination of the observed helium concentrations with sedimentation rates estimated from conodont biostratigraphy suggest that the flux of extraterrestrial 3He in the Early Ordovician was about 0.5 x 10(-12) cm3 STP cm-2 ka-1, ignoring potential post-deposition helium loss. This value is indistinguishable from the average 3He flux estimated for the Cenozoic Era. In contrast, previous studies of fossil meteorites, Ir abundances, and Os isotopic ratios in the limestone suggest that the total accretion rate of extraterrestrial material during the studied interval was at least an order of magnitude higher than the Cenozoic average. This disparity may reflect significant post-depositional loss of 3He from IDPs within these old limestones; if so, the match between the Ordovician flux and the Cenozoic average would be fortuitous. Alternatively, the size distribution of infalling objects during the Early Ordovician may have been enriched only in extraterrestrial material too large to retain 3He during atmospheric entry heating (> approximately 30 micrometers). The fossil meteorites themselves also preserve extraterrestrial helium. Meteorite 3He concentrations of 2 to 9 x 10(-12) cm3 STP g-1 are several orders of magnitude lower than found in most modern meteorites, suggesting very substantial helium loss (probably >99.9%) from these chemically altered objects. The Meteorites carry 3He concentrations only a factor of a few higher than the host limestones. The meteorites themselves cannot be the source of the extraterrestrial 3He observed in the limestones.
authors.affiliation: Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA. desmond@gps.caltech.edu
authors.forename: D B
authors.initials: DB
authors.lastname: Patterson
authors.forename: K A
authors.initials: KA
authors.lastname: Farley
authors.forename: B
authors.initials: B
authors.lastname: Schmitz
mesh_terms: D002119:Calcium Carbonate / Q000032:analysis* / Q000737:chemistry; D019443:Cosmic Dust; D018534:Earth, Planet; D019419:Evolution, Planetary; D005118:Extraterrestrial Environment; D019015:Geologic Sediments / Q000737:chemistry; D006371:Helium / Q000032:analysis / Q000737:chemistry*; D007554:Isotopes; D008094:Lithium / Q000737:chemistry; D019110:Meteoroids; D009792:Oceans and Seas; D013548:Sweden
chemical_list: D019443:Cosmic Dust; D007554:Isotopes; D006371:Helium; D008094:Lithium; D002119:Calcium Carbonate