Astronomy:Gas-rich meteorites
Gas-rich meteorites are meteorites with high levels of primordial gases, such as helium, neon, argon, krypton, xenon and sometimes other elements.[1] Though these gases are present "in virtually all meteorites,"[2] the Fayetteville meteorite has ~2,000,000 x10−8 ccSTP/g helium,[3] or ~2% helium by volume equivalent. In comparison, background level is a few ppm. The identification of gas-rich meteorites is based on the presence of light noble gases in large amounts, at levels which cannot be explained without involving an additional component over and above the well-known noble gas components that are present in all meteorites.[3]
History
William Ramsay was the first to report helium in an iron meteorite, in 1895- not long after its first Earth sample, instead of via Solar observation.[4]
The use of decay products to date meteorites was suggested by Bauer in 1947,[5] and explicitly published by Gerling and Pavlova in 1951.[6] However, this soon resulted in wildly varying ages; it was realized excess helium (including helium-3, rare on Earth) was generated by radiation, too.[7]
The first explicit publication of a gas-rich meteorite was Staroe Pesyanoe (often shortened to Pesyanoe), by Gerling and Levskii in 1956. In family with the later Fayetteville, Pesyanoe's helium level is ~1 million x10−8 ccSTP/g.[8]
Reynolds' publication of a "general Xe anomaly",[9] including 129I decay products and more, touched off the subfield of xenology,[10][11][12][13] continuing to today.[14][15]
The first publication of presolar grains in the 1980s[16] was precipitated by workers searching for noble gases;[17] PSGs were not simply checked via their gas contents.[18][19]
Lines of inquiry
As unreactive components, they are tracers of processes throughout and predating the Solar System:
Material age can be determined by relative exposure to direct solar and cosmic radiation (by cosmic ray tracks), and indirect creation of resultant nuclides. This includes Ar-Ar dating, I-Xe dating, and U to its various decay products including helium.[20][21][22]
The parent body of a meteorite can be traced in part via comparison of trace elements.[23][24][25] That meteorites are fragments of asteroids, and conditions on such asteroids, were partially deduced from gas evidence.[26][27][28][29]
This includes meteorite pairing, the re-association of meteorites which had split before recovery.[30][31]
Meteorite, parent, and Solar System histories are indicated by tracer elements,[32][33][34] including thermometry, a record of material temperature.[35]
- Presolar activity.[36][19]
- A supernova thought to have preceded the Solar System.[37][36]
- The history of the Sun.[38][39][40][41] This record extends to billion-year timescales,[42][43] back to "very early in the life of the Sun".[44]
- The history of cosmic ray fluence. Meteorites do not show significant variation of cosmic rays over time.[45]
The Lost City Meteor was tracked, allowing an orbit determination back to the asteroid belt. Measurement of relatively short-half-life isotopes in the subsequent Lost City Meteorite then indicate radiation levels in that region of the Solar System.[46]
Gas study
The field of meteoritic gases follows progress in analytical methods.[47]
The first analyses were basic laboratory chemistry, such as acid dissolution. Various acids were necessary, due to mixtures of various soluble and insoluble minerals. Stepped etching gave higher levels of resolution and discrimination.
Pyrolysis was used, such as on highly acid resistant minerals. These two methods were alternately lauded and derided as "burning the haystack to find the needle."[48][49][50]
Meteoritical studies have tracked the progress of mass spectrometry,[51] a continual and rapid progression[52][53] comparable to or greater than Moore's Law.[54]
More recently, laser extraction[55][56][57]
Meteorites
[58] This meteoritics-related list is incomplete; you can help by expanding it.
Name | Classification | Date | Provenance | Ref |
---|---|---|---|---|
Pantar | H5 | 1938 | Fall | ,[59][60] |
Fayetteville | H4 | 1934 | Fall | ,[60][61][62] |
Gladstone | H4 | 1936 | Find | [63][64] |
Noblesville | H4 | 1991 | Fall | [65][66] |
Tsukuba | H5-6 | 1996 | Fall | [67][68] |
Weston | H4 | 1807 | Fall | ,[59][60][69] |
Willard | H3 | 1934 | Find | [70][64] |
Elm Creek | H4 | 1906 | Find | [60] |
Leighton | H5 | 1907 | Fall | [60][71] |
Djermaia | H | 1961 | Fall | [60] |
Acfer 111 | -H3 | 1990 | Find | [72][73] |
Ghubara | L5 | 1954 | Find | [74][75] |
St. Mesmin | L5 | 1866 | Fall | [76][77][69] |
(Staroe) Pesyanoe | Aubrite | 1933 | Fall | [78][62][79] |
Khor Temiki | Aubrite | 1932 | Fall | ,[80][69] |
Bustee | Aubrite | 1852 | Fall | [81][82] |
Jodzie | Howardite | 1877 | Fall | [83] |
Kapoeta | Howardite | 1942 | Fall | ,[84] 3,[85] |
South Oman | -EH | 1958 | Find | [86][87] |
Interplanetary dust, like c-chondrites and enstatites, contain hosts for these gases and often measurable gas contents.[88][89][90] So too do a fraction of micrometeorites.[91][92][93]
Gas
Gas components were first named by descriptors, then letter codes;[94][95] the letter taxonomy "has become increasingly complicated and confusing with time."[96][97]
By Element and Isotope
Primordial/trapped
Solar wind/solar flare
Cosmic ray/spallogenic
3He 83Kr 126Xe[7][99][100][101]
Radiogenic/fissile
3He 36Ar 40Ar 129Xe 132Xe 134Xe 136Xe 128Xe[102]
By Component
Planetary
"Planetary" gases (P, Q, P1) are depleted in light elements (He, Ne) compared to solar abundances (see below), or conversely, enriched in Kr, Xe.[103][104][105] This name originally implied an origin, the gas blend observed in terrestrial planets. Scientists wished to stop implying this,[106][105] but the habit was retained.[107][105]
Solar, subsolar
This gas component corresponds to the solar wind.[108][105] Solar flare gas can be distinguished by its greater depth,[109] and a slightly variant composition.[110] "Subsolar" is intermediary between solar and planetary.[111]
E
"Exotic" neon- aberrant 20Ne/22Ne values.[112][113]
H
"Heavy" isotopes of xenon,[114][97] primarily r-process isotopes, plus p-process. Thus, sometimes seen as "HL," anomalous heavy and light isotopes.
G
"Giant", after asymptotic giant branch (while A and B had been taken[112][113]); contains their s-process isotopes.[115]
See also
- Activated carbon
- Clathrate
- Cryopump
- Getter
- Hydrogen embrittlement
- Ion implantation
- Molecular sieve and Molecular distillation
- Outgassing
References
- ↑ Suess, H. E.; Wänke, H.; Wlotzka, F. (1964-05-01). "On the origin of gas-rich meteorites". Geochimica et Cosmochimica Acta 28 (5): 595–607. doi:10.1016/0016-7037(64)90080-8. Bibcode: 1964GeCoA..28..595S.
- ↑ Swindle, T. (1988). Trapped noble gases in meteorites. Tucson: University of Arizona Press. p. 535. in Meteorites and the early solar system, J. F. Kerridge & M. S. Matthews Eds.
- ↑ 3.0 3.1 Goswami, J.; Lal, D.; Wilkening, L. (1983). "Gas-Rich meteorites: Probes for particle environment and dynamical processes in the inner solar system". Space Science Reviews 37 (1–2): 111–59. doi:10.1007/BF00213959. Bibcode: 1984SSRv...37..111G.
- ↑ Ramsay, W. (4 Jul 1895). "Argon and Helium in Meteoritic Iron". Nature 52 (1340): 224–25. doi:10.1038/052224a0. Bibcode: 1895Natur..52..224R.
- ↑ Bauer, C. (15 August 1947). "Production of Helium in Meteorites by Cosmic Radiation". Physical Review 72 (4): 354. doi:10.1103/PhysRev.72.354. Bibcode: 1947PhRv...72..354B.
- ↑ Gerling, E.; Pavlova, T. (1951). "Determination of the geological age of two stony meteorites by the argon method". Doklady Akademii Nauk SSSR 77: 85–97.
- ↑ 7.0 7.1 Paneth, F.; Reasbeck, P.; Mayne, K. (Aug 1953). "Production by cosmic rays of helium-3 in meteorites". Nature 172 (4370): 200–01. doi:10.1038/172200a0. PMID 13087152. Bibcode: 1953Natur.172..200P.
- ↑ Gerling, E.; Levskii, L. (1956). "On the origin of the rare gases in stony meteorites". Doklady Akademii Nauk SSSR 110: 750.
- ↑ Reynolds, J. (15 May 1963). "Xenology". Journal of Geophysical Research 68 (10): 2939–56. doi:10.1029/JZ068i010p02939. Bibcode: 1963JGR....68.2939R.
- ↑ Fleischer, R.; Price, P.; Walker, R. (1975). "6.5 Study of Nucleosynthesis and the Early History of the Solar System by Extinct Isotopes". Nuclear Tracks in Solids: Principles and Applications. University of California Press. ISBN 9780520026650. https://archive.org/details/bub_gb_yfTBvben3GoC.
- ↑ Hintenberger, H. (Jul 1972). "Xenon in irdischer und in extraterrestrischer Materie (Xenologie)". Naturwissenschaften 59 (7): 285–91. doi:10.1007/BF00593352. Bibcode: 1972NW.....59..285H.
- ↑ Kuroda, P. (Jan 1976). "Xenology: The enigma of xenon in carbonaceous chondrite". Geochemical Journal 10 (3): 121–36. doi:10.2343/geochemj.10.121. Bibcode: 1976GeocJ..10..121K.
- ↑ Staudacher, T. Allègre C. (Oct 1982). "Terrestrial xenology". Earth and Planetary Science Letters 60 (3): 389–406. doi:10.1016/0012-821X(82)90075-9. Bibcode: 1982E&PSL..60..389S.
- ↑ Tolstikhin, I.; Marty, B.; Porcelli, D.; Hofmann, A. (Jul 2014). "Evolution of volatile species in the earth's mantle: A view from xenology". Geochimica et Cosmochimica Acta 136: 229–46. doi:10.1016/j.gca.2013.08.034. Bibcode: 2014GeCoA.136..229T.
- ↑ Diehl, R.; Hartmann, D.; Prantzos, N. (2018). "2.2.4 Extinct Radioactivity and Immediate Pre-Solar Nucleosynthesis". Astrophysics with Radioactive Isotopes (2nd ed.). Springer. ISBN 978-3319919294.
- ↑ Lewis, R.; Ming, T.; Wacker, J.; Anders, E.; Steel, E. (Mar 1987). "Interstellar diamonds in meteorites". Nature 326 (6109): 160–62. doi:10.1038/326160a0. Bibcode: 1987Natur.326..160L.
- ↑ Zinner, E.; Ming, T.; Anders, E. (24 Dec 1987). "Large isotopic anomalies of Si, C, N and noble gases in interstellar silicon carbide from the Murray meteorite". Nature 330 (6150): 730–32. doi:10.1038/330730a0. Bibcode: 1987Natur.330..730Z.
- ↑ Ott, U. (Jul 1993). "Interstellar grains in meteorites". Nature 364 (6432): 25–33. doi:10.1038/364025a0. Bibcode: 1993Natur.364...25O.
- ↑ 19.0 19.1 Anders, E. (1988). Circumstellar material in meteorites: noble gases, carbon and nitrogen. Tucson: University of Arizona Press. p. 927. ISBN 978-0816510634. in Meteorites and the Early Solar System, Kerridge, J., Matthews, M. eds.
- ↑ Martin, G. (1953). "Recent studies of iron meteorites. IV The origin of meteoritic helium and the age of meteorites". Geochimica et Cosmochimica Acta 3 (6): 288–309. doi:10.1016/0016-7037(53)90037-4. Bibcode: 1953GeCoA...3..288M.
- ↑ Gerling, E.; Pavlova, T. (1951). "Determination of the geological age of two stony meteorites by the argon method". Doklady Akademii Nauk SSSR 77: 85–97.
- ↑ Wasserburg, G.; Hayden, R. (1955). "Age of meteorites by the Ar40-K40 method". Physical Review 97 (1): 86–87. doi:10.1103/PhysRev.97.86. Bibcode: 1955PhRv...97...86W. https://authors.library.caltech.edu/5266/1/WASpr55.pdf.
- ↑ Wieler, R.; Baur, H.; Pedroni, A.; Signer, P.; Pellas, P. (1989). "Exposure history of the regolithic chondrite Fayetteville: I. Solar-gas-rich matrix". Geochimica et Cosmochimica Acta 53 (6): 1441–59. doi:10.1016/0016-7037(89)90076-8. Bibcode: 1989GeCoA..53.1441W.
- ↑ Nier, A.; Schlutter, D. (1990). "H and N isotopes in stratospheric particles". Meteoritics 25: 263–67. doi:10.1111/j.1945-5100.1990.tb00710.x.
- ↑ Bogard, D. (1995). "Impact ages of meteorites: A synthesis". Meteoritics 30 (3): 244–68. doi:10.1111/j.1945-5100.1995.tb01124.x. Bibcode: 1995Metic..30..244B.
- ↑ Lal, D. Rajan R. (19 Jul 1969). "Observations on Space Irradiation of Individual Crystals of Gas-rich Meteorites". Nature 223 (5203): 269–71. doi:10.1038/223269a0. Bibcode: 1969Natur.223..269L.
- ↑ MacDougall, Rajan R. Price P. (11 Jan 1974). "Gas-rich meteorites: possible evidence for origin on a regolith". Science 183 (4120): 73–4. doi:10.1126/science.183.4120.73. PMID 17743149. Bibcode: 1974Sci...183...73M.
- ↑ Anders, E. (1978). "Most Stony Meteorites Come from the Asteroid Belt". Asteroids: An Exploration Assessment, NASA Conference Publication 2053. NASA. p. 57.
- ↑ Obase, T.; Nakashima, D. (12 Jul 2019). "Past Solar Wind Fluxes at the Locations of Gas-Rich Meteorite Parent Bodies Based on Noble Gas Studies: Implications to the Past Heliocentric Distances". Proc. 82nd Annual Meeting of the Meteoritical Society 82 (2157): 6270. Bibcode: 2019LPICo2157.6270O.
- ↑ Schultz, L.; Kruse, H.. "He, Ne, and Ar in meteorites. A detailed compilation". Meteoritics 24: 155–72. doi:10.1111/j.1945-5100.1989.tb00958.x.
- ↑ Bogard, D; Johnson, P (Aug 1983). "Martian Gases in an Antarctic Meteorite?". Science 221 (4611): 651–54. doi:10.1126/science.221.4611.651. PMID 17787734. Bibcode: 1983Sci...221..651B.
- ↑ Padia, J.; Rao, M. (1989). "Neon isotope studies of Fayetteville and Kapoeta meteorites and clues to ancient solar activity". Geochimica et Cosmochimica Acta 53 (6): 1461–67. doi:10.1016/0016-7037(89)90078-1. Bibcode: 1989GeCoA..53.1461P.
- ↑ Marti, K. (5 Dec 1969). "Solar-type xenon: a new isotopic composition of xenon in the pesyanoe meteorite". Science 166 (3910): 1263–5. doi:10.1126/science.166.3910.1263. PMID 17759945. Bibcode: 1969Sci...166.1263M.
- ↑ Begemann, F. (1972). "Ar37/Ar39 activity ratios in meteorites and the spatial consistency of the cosmic radiation". Journal of Geophysical Research 77: 3650–59. doi:10.1029/JB077i020p03650.
- ↑ Okazaki, R.; Nagao, K. (Apr 2017). "Primordial and cosmogenic noble gases in the Sutter's Mill CM chondrite". Meteoritics & Planetary Science 52 (4): 669–89. doi:10.1111/maps.12819. Bibcode: 2017M&PS...52..669O.
- ↑ 36.0 36.1 Alaerts, L.; Lewis, R.; Matsuda, J; Anders, E. (1980). "Isotopic anomalies of noble gases in meteorites and their origins-Presolar components in the Murchison C2 chondrite". Geochimica et Cosmochimica Acta 44 (2): 189–209. doi:10.1016/0016-7037(80)90131-3. Bibcode: 1980GeCoA..44..189A.
- ↑ Clayton, D (Oct 1979). "Supernovae and the origin of the solar system". Space Science Reviews 24 (2): 147–226. doi:10.1007/BF00167709. Bibcode: 1979SSRv...24..147C.
- ↑ The Ancient Sun: Fossil record in the Earth, Moon and Meteorites. New York: Pergamon Press. 1980. ISBN 978-0080263243.
- ↑ Pepin, R. O.; McKay, D. S. (1986). Workshop On Past And Present Solar Radiation: The Record in Meteoritic and Lunar Regolith Material. Houston: Lunar And Planetary Institute.
- ↑ The Sun in Time. Tucson: University of Arizona Press. 1991. ISBN 978-0-8165-1297-3.
- ↑ Koop, L.; Heck, P. (2018). "High early solar activity inferred from helium and neon excesses in the oldest meteorite inclusions". Nature Astronomy 2 (9): 709–13. doi:10.1038/s41550-018-0527-8. Bibcode: 2018NatAs...2..709K.
- ↑ Heber, V.; Baur, H.; Wieler, R. (Nov 2001). Solar Krypton and Xenon in gas-rich meteorites: New insights into a unique archive of solar wind. American Institute of Physics. p. 387. ISBN 0-7354-0042-3. in Solar and Galactic Composition: A Joint SOHO/ACE Workshop, R. F. Wimmer-Schweingruber, ed.
- ↑ Pepin, R. Palma R. Schlutter D. (Feb 2010). "Noble gases in interplanetary dust particles, II: Excess helium-3 in cluster particles and modeling constraints on interplanetary dust particle exposures to cosmic-ray irradiation". Meteoritics & Planetary Science 36 (11): 1515–34. doi:10.1111/j.1945-5100.2001.tb01843.x.
- ↑ Wieler, R.; Pedroni, A.; Leya, I. (4 Feb 2010). "Cosmogenic neon in mineral separates from Kapoeta: No evidence for an irradiation of its parent body regolith by an early active Sun". Meteoritics & Planetary Science 35 (2): 251–57. doi:10.1111/j.1945-5100.2000.tb01774.x.
- ↑ Smith, T.; Cook, D.; Merchel, S.; Pavetich, S.; Rugel, G.; Scharf, A.; Leya, I. (Dec 2019). "The constancy of galactic cosmic rays as recorded by cosmogenic nuclides in iron meteorites". Meteoritics & Planetary Science 54 (12): 2951–76. doi:10.1111/maps.13417. Bibcode: 2019M&PS...54.2951S.
- ↑ Begemann, F. (10 Jul 1972). "Argon 37/argon 39 activity ratios in meteorites and the spatial constancy of the cosmic radiation". Journal of Geophysical Research 77 (20): 3650–59. doi:10.1029/JB077i020p03650. Bibcode: 1972JGR....77.3650B.
- ↑ Begemann, F. (1996). "Noble gases and meteorites". Meteoritics & Planetary Science 31 (2): 171–76. doi:10.1111/j.1945-5100.1996.tb02012.x.
- ↑ Wieler, R.; Busemann, H.; Franchi, I. (2006). Trapping and Modification Processes of Noble Gases and Nitrogen in Meteorites and Their Parent Bodies. Tucson: University of Arizona Press. p. 499. ISBN 9780816525621. in Meteorites and the Early Solar System II, Lauretta, D. McSween, H. eds.
- ↑ Manavi. "Stardust from meteorites". Case Western Reserve University. https://caslabs.case.edu/ansmet/2014/01/21/stardust-from-meteorites/.
- ↑ Dauphas, N.; Schauble, E. (2016). "Mass Fractionation Laws, Mass-Independent Effects, and Isotopic Anomalies". Annu. Rev. Earth Planet. Sci. 44: 709–83. doi:10.1146/annurev-earth-060115-012157. Bibcode: 2016AREPS..44..709D.
- ↑ Merrill, G. (Jun 1909). "The composition of stony meteorites compared with that of terrestrial igneous rocks, and considered with reference to their efficacy in world-making". American Journal of Science 27 (162): 469–74. doi:10.2475/ajs.s4-27.162.469. Bibcode: 1909AmJS...27..469M. https://zenodo.org/record/2101871.
- ↑ Gilmour, J.; Lyon, I.; Johnston, W.; Turner, G. (Mar 1994). "RELAX: An ultrasensitive; resonance ionization mass spectrometer for xenon". Review of Scientific Instruments 65 (3): 617–25. doi:10.1063/1.1145127. Bibcode: 1994RScI...65..617G.
- ↑ Baur, H. (1999). "A noble gas mass spectrometer compressor source with two orders of magnitude improvement in sensitivity". EOS, Trans. Am. Geophys. Union 46: F1118.
- ↑ Thompson, Bruce (15 Nov 2012). "Driving High Sensitivity in Biomolecular MS". Genetic Engineering & Biotechnology News 32 (20).
- ↑ Takaoka, N.; Nagao, K.; Miura, Y. (1991). Noble Gas Study of Unique Meteorite Yamato-74063 by Laser Extraction. NIPR (Japan). p. 92. in 16th Symposium on Antarctic Meteorites, Jun 5-7 1991
- ↑ Osawa, T.; Nagao, K.; Nakamura, T.; Takaoka, N. (2000). "Noble gas measurement in individual micrometeorites using laser gas-extraction system". Antarctic Meteorite Research 13: 322–41. Bibcode: 2000AMR....13..322O.
- ↑ Avice, G.; Bekaert, D.; Chennaoui Aoudjehane, H.; Marty, B. (9 Feb 2018). "Noble gases and nitrogen in Tissint reveal the composition of the Mars atmosphere". Geochemical Perspectives Letters 6: 11–16. doi:10.7185/geochemlet.1802.
- ↑ Padia, J.; Rao, M. (Jun 1989). "Neon isotope studies of Fayetteville and Kapoeta meteorites and clues to ancient solar activity". Geochimica et Cosmochimica Acta 53 (6): 1461–67. doi:10.1016/0016-7037(89)90078-1. Bibcode: 1989GeCoA..53.1461P.
- ↑ 59.0 59.1 Eugster, O. (2003). "Cosmic-ray Exposure Ages of Meteorites and Lunar Rocks and Their Significance". Geochemistry 63 (1): 3–30. doi:10.1078/0009-2819-00021. Bibcode: 2003ChEG...63....3E.
- ↑ 60.0 60.1 60.2 60.3 60.4 60.5 Graf, Thomas; Marti, Kurt (1995). "Collisional history of H chondrites". Journal of Geophysical Research 100 (E10): 21247. doi:10.1029/95JE01903. Bibcode: 1995JGR...10021247G.
- ↑ Padia, J., Rao, M. "Neon isotope studies of Fayetteville and Kapoeta meteorites and clues to ancient solar activity ". (Jun 1989). Geochimica et Cosmochimica Acta. 53(6): 1461-67.
- ↑ 62.0 62.1 Mueller, O., Zahringer, J. "Chemische Unterschiede bei urdelgashaltigen Steinmeteoriten". (1966). Earth Planet. Sci. Lett. (1): 25.
- ↑ Miura, Y.; Nagao, K. (1992). "Noble gases and 81Kr-Kr exposure ages of non-Antarctic ordinary chondrites: An attempt to measure terrestrial ages of Antarctic meteorites". in Yanai, K.. Sixteenth Symposium on Antarctic Meteorites, held June 5–7, 1991, at the National Institute of Polar Research, Tokyo. National Institute of Polar Research (Japan). pp. 298–309. Bibcode: 1992AMR.....5..298M. https://core.ac.uk/download/pdf/51484034.pdf. Retrieved 2020-02-04.
- ↑ 64.0 64.1 Osawa, T.; Nagao, K. (2006). "Noble gases in solar-gas-rich and solar-gas-free polymict breccias". Antarctic Meteorite Research 19: 58–78. Bibcode: 2006AMR....19...58T.
- ↑ Lipschutz, M.; Wolf, S.; Vogt, S. (Sep 1993). "Consortium study of the unusual H chondrite regolith breccia, Noblesville". Meteoritics 28 (4): 528–537. doi:10.1111/j.1945-5100.1993.tb00276.x. Bibcode: 1993Metic..28..528L.
- ↑ Murer, C.; Baur, H.; Signer, P.; Wieler, R. (Mar 1997). "Helium, neon, and argon abundances in the solar wind: In vacuo etching of meteoritic iron-nickel". Geochimica et Cosmochimica Acta 61 (6): 1303–14. doi:10.1016/S0016-7037(97)83772-6. Bibcode: 1997GeCoA..61.1303M.
- ↑ Jabeen, I.; Kusakabe, M.; Nagao, K.; Nakamura, T. (1998). "Tsukuba meteorite: H chondrite, or a new parent body?". Meteoritics & Planetary Science 33: 77.
- ↑ Nakashima, D.; Nakamura, T.; Sekiya, M.; Takaoka, N. (2002). "Cosmic-ray exposure age and heliocentric distance of the parent body of H chondrites Y75029 and Tsukuba". Antarctic Meteorite Research 15: 97–113.
- ↑ 69.0 69.1 69.2 Schultz, L., Kruse, H. "Helium, Neon, and Argon in Meteorites: A Data Compilation". Max-Planck-Institut fur Chemie, Mainz. (1983).
- ↑ Inada, A.; Nagao, K. (2003). "Noble gases and cosmic-ray x host of Willard (b) H-chondrite: A breccia with". Meteoritics & Planetary Science 38: 5170.
- ↑ Quijano-Rico, M.; Wanke, H. (1969). Millman, P. M.. ed. Meteorite Research: Proceedings of a Symposium on Meteorite Research Held in Vienna, Austria, 7–13 August 1968. Springer Science & Business Media. p. 134. ISBN 978-90-277-0132-9.
- ↑ Romstedt, J.; Pedroni, A. (Jul 1993). "Irradiation History of ACFER 111, Inferred from Nuclear Tracks and Rare Gases". Meteoritics 28 (3): 424. Bibcode: 1993Metic..28R.424R.
- ↑ Pedroni, A.; Begemann, F. (1994). "On unfractionated solar noble gas in the H3-6 meteorite Acfer 111". Meteoritics 29 (5): 632. doi:10.1111/j.1945-5100.1994.tb00776.x.
- ↑ Levskii, L. (1979). "Rare gases in carbonaceous chondrites". Meteoritika 38: 27–36. Bibcode: 1979Metik..38...27L.
- ↑ Meier, M.; Schmitz, B.; Alwmark, C. (2014). "He and Ne in individual chromite grains from the regolith breccia Ghubara (L5):Exploring the history of the L chondrite parent body regolith". Meteoritics & Planetary Science 49 (4): 576–94. doi:10.1111/maps.12275. Bibcode: 2014M&PS...49..576M.
- ↑ Heymann, D.; Mazor, E. (1 Oct 1966). "St. Mesmin, A gas-rich amphoteric chondrite". Journal of Geophysical Research 71 (19): 4695–97. doi:10.1029/JZ071i019p04695. Bibcode: 1966JGR....71.4695H.
- ↑ Schultz, L.; Signer, P. (Dec 1974). "Rare gasses in the St. Mesmin chondrite". Meteoritics 9: 402–03. Bibcode: 1974Metic...9..402S.
- ↑ Gerling, E.; Levskii, L. (1956). "On the origin of the rare gases in stony meteorites". Doklady Akademii Nauk SSSR 110: 750.
- ↑ Murty, S.; Marti, K. (Sep 1990). "Search for solar-type nitrogen in the gas-rich Pesyanoe meteorite". Meteoritics 25 (3): 227–30. doi:10.1111/j.1945-5100.1990.tb01000.x. Bibcode: 1990Metic..25..227M.
- ↑ Ashworth, J.; Barber, D. (1975). "Electron petrography of shock effects in a gas-rich enstatite-achondrite". Contributions to Mineralogy and Petrology 49 (2): 149–62. doi:10.1007/BF00373858. Bibcode: 1975CoMP...49..149A.
- ↑ Poupeau, G.; Berdot, J. (Apr 1972). "Irradiations ancienne et recente des aubrites". Earth and Planetary Science Letters 14 (3): 381–396. doi:10.1016/0012-821X(72)90139-2. Bibcode: 1972E&PSL..14..381P.
- ↑ Poupeau, G.; Kirsten, T.; Steinbrunn, F.; Storzer, D. (Dec 1974). "The records of solar wind and solar flares in aubrites". Earth and Planetary Science Letters 24 (2): 229–41. doi:10.1016/0012-821X(74)90101-0. Bibcode: 1974E&PSL..24..229P.
- ↑ Mazor, E.; Anders, E. (Sep 1967). "Primordial gases in the Jodzie howardite and the origin of gas-rich meteorites". Geochimica et Cosmochimica Acta 31 (9): 1441–56. doi:10.1016/0016-7037(67)90020-8. Bibcode: 1967GeCoA..31.1441M.
- ↑ Pellas, P.; Poupeau, G.; Lorin, J.; Reeves, H.; Audouze, J. (1969). "Primitive Low-energy Particle Irradiation of Meteoritic Crystals". Nature 223 (5203): 272–74. doi:10.1038/223272a0. Bibcode: 1969Natur.223..272P.
- ↑ Swindle, T.; Garrison, D.; Goswami, J.; Hohenberg, C.; Nichols, R.; Olinger, C. (1990). "Noble gases in the howardites Bholghati and Kapoeta". Geochimica et Cosmochimica Acta 54 (8): 2183–94. doi:10.1016/0016-7037(90)90044-L. Bibcode: 1990GeCoA..54.2183S.
- ↑ Crabb, J.; Anders, E. (1981). "Noble gases in E-chondrites". Geochimica et Cosmochimica Acta 45 (12): 2443–64. doi:10.1016/0016-7037(81)90097-1. Bibcode: 1981GeCoA..45.2443C.
- ↑ Pepin, R.; Becker, R.; Rider, P. (1995). "Xenon and krypton isotopes in extraterrestrial regolith soils and in the solar wind". Geochimica et Cosmochimica Acta 59 (23): 4997–5022. doi:10.1016/0016-7037(96)80916-1. Bibcode: 1995GeCoA..59.4997P.
- ↑ Merrihue, C. (1964). "Rare Gas Evidence For Cosmic Dust In Modern Pacific Red Clay". Ann. N.Y. Acad. Sci. 119 (1): 351–67. doi:10.1111/j.1749-6632.1965.tb47445.x.
- ↑ Tilles, D. (21 May 1965). "Atmospheric noble gases;; Solar-Wind bombardment of extraterrestrial dust as a possible source mechanism". Science 148 (3673): 1085–88. doi:10.1126/science.148.3673.1085. PMID 17820112. Bibcode: 1965Sci...148.1085T.
- ↑ Nier, A.; Schlutter, D. (Dec 1990). "Helium and neon isotopes in stratospheric particles". Meteoritics 25 (4): 263–67. doi:10.1111/j.1945-5100.1990.tb00710.x. Bibcode: 1990Metic..25..263N.
- ↑ Olinger, C.; Maurette, M.; Walker, R.; Hohenberg, C. (1990). "Neon measurements of individual Greenland sediment particles: proof of an extraterrestrial origin". Earth Planet. Sci. Lett. 100: 77–93. doi:10.1016/0012-821X(90)90177-Y.
- ↑ Osawa, T.; Nakamura, T.; Nagao, K. (2003). "Noble gas isotopes and mineral assemblages of Antarctic micrometeorites collected at the meteorite ice field around the Yamato mountains". Meteoritics & Planetary Science 38 (11): 1627–40. doi:10.1111/j.1945-5100.2003.tb00005.x. Bibcode: 2003M&PS...38.1627O.
- ↑ Heck, P.; Schmitz, B.; Baur, H.; Wieler, R. (March 2008). "Noble gases in fossil micrometeorites and meteorites from 470 Myr old sediments from southern Sweden, and new evidence for the L-chondrite parent body breakup event". Meteoritics & Planetary Science 43 (3): 517–28. doi:10.1111/j.1945-5100.2008.tb00669.x. Bibcode: 2008M&PS...43..517H.
- ↑ Pepin, R. (1967). "Trapped neon in meteorites". Earth and Planetary Science Letters 12 (1): 13–18. doi:10.1016/0012-821X(67)90165-3. Bibcode: 1967E&PSL...2...13P.
- ↑ 95.0 95.1 Nakamura, T.; Nagao, K. Metzler; K.; Takaoka, N. (Jan 1999). "Heterogeneous distribution of solar and cosmogenic noble gases in CM chondrites and implications for the formation of CM parent bodies". Geochimica et Cosmochimica Acta 63 (2): 257–73. doi:10.1016/S0016-7037(98)00278-6. Bibcode: 1999GeCoA..63..257N.
- ↑ Sabu, D.; Manuel, O. (1980). "The neon alphabet game". 2. New York: Pergamon Press. pp. 879–899. Bibcode: 1980LPSC...11..879S. http://pdfs.semanticscholar.org/56a7/135a9f842d9e17b29ea1dd5c532773111faa.pdf. Retrieved 2020-02-04.
- ↑ 97.0 97.1 Huss, G.; Lewis, R. (Jan 1995). "Presolar diamond, SiC, and graphite in primitive chondrites: Abundances as a function of meteorite class and petrologic type". Geochimica et Cosmochimica Acta 59 (1): 115–60. doi:10.1016/0016-7037(94)00376-W. Bibcode: 1995GeCoA..59..115H.
- ↑ Pepin, R.; Signer, P. (16 Jul 1965). "Primordial Rare Gases in Meteorites". Science 149 (3681): 253–65. doi:10.1126/science.149.3681.253. PMID 17838092. Bibcode: 1965Sci...149..253P.
- ↑ Eberhardt, P.; Eugster, O.; Geiss, J.; Marti, K. (1965). "Rare Gas Measurements in 30 Stone Meteorites". Z. Naturforsch. 21: 414–26. Bibcode: 1966ZNatA..21..414E.
- ↑ Vogt, S.; Herzog, G.; Reedy, R. (Aug 1990). "Cosmogenic nuclides in extraterrestrial materials". Reviews of Geophysics 28 (3): 253–75. doi:10.1029/RG028i003p00253. Bibcode: 1990RvGeo..28..253V.
- ↑ Leya, I; Lange, H.; Neumann, S.; Wieler, R.; Michel, R. (Mar 2000). "The production of cosmogenic nuclides in stony meteoroids by galactic cosmic-ray particles". Meteoritics & Planetary Science 35 (2): 259–86. doi:10.1111/j.1945-5100.2000.tb01775.x. Bibcode: 2000M&PS...35..259L.
- ↑ Fish, R.; Goles, G. (6 Oct 1962). "Ambient Xenon: A Key To The History Of Meteorites". Nature 196 (4849): 27–31. doi:10.1038/196027a0. Bibcode: 1962Natur.196...27F.
- ↑ Merrihue, C.; Pepin, R.; Reynolds, J. (1962). "Rare Gases in the Chondrite Pantar". Journal of Geophysical Research 67 (5): 2017–21. doi:10.1029/JZ067i005p02017. Bibcode: 1962JGR....67.2017M.
- ↑ Zahnle, K. (1993). Planetary Noble Gases. Tucson: University of Arizona Press. p. 1305. ISBN 0816513341. in Protostars and Planets III, Levy, E.; Lunine, Jonathan I.; eds.
- ↑ 105.0 105.1 105.2 105.3 Huss, G.; Lewis, R.; hemkin, S (1996). "The "normal planetary" noble gas component in primitive chondrites: Compositions, carrier, and metamorphic history". Geochimica et Cosmochimica Acta 60 (17): 3311–40. doi:10.1016/0016-7037(96)00168-8. Bibcode: 1996GeCoA..60.3311H.
- ↑ Heymann, D. (1970). The Noble Gases. New York: Gordon and Breach. p. 29. ISBN 9780677149509. in Handbook of Elemental Abundances in Meteorites, Mason, B. ed.
- ↑ Lewis, R.; Srinavasan, B.; Anders, E. (1975). "Host phase of a strange xenon component in Allende meteorite". Science 190 (4221): 1251–62. doi:10.1126/science.190.4221.1251.
- ↑ Mazor, E.; Heymann, D.; Anders, E. (1970). "Noble gases in carbonaceous chondrites". Geochimica et Cosmochimica Acta 34 (7): 781–824. doi:10.1016/0016-7037(70)90031-1. Bibcode: 1970GeCoA..34..781M.
- ↑ Murer, C.; Bauer, H.; Wieler, R. (1995). "Light noble gas abundances in the solar wind trapped by chondritic material". Meteoritics 30: 554.
- ↑ Bochsler, P.; Kallenbach, R. (Sep 1994). "Fractionation of N Isotopes in SEPs". Meteoritics 29: 653–58. doi:10.1111/j.1945-5100.1994.tb00780.x.
- ↑ Busemann, H.; Eugster, O.; Baur, H.; Wieler, R. (Mar 2003). "The ingredients of the "Subsolar" noble gas component". Abstract no. 1674. Bibcode: 2003LPI....34.1674B. https://www.lpi.usra.edu/meetings/lpsc2003/pdf/1674.pdf. Retrieved 2020-02-04.
- ↑ 112.0 112.1 Pepin, R. (Jan 1967). "Trapped neon in meteorites". Earth and Planetary Science Letters 2 (1): 13–18. doi:10.1016/0012-821X(67)90165-3. Bibcode: 1967E&PSL...2...13P.
- ↑ 113.0 113.1 Black, D.; Pepin, R. (1969). "Trapped neon in meteorites — II". Earth and Planetary Science Letters 6 (5): 395–405. doi:10.1016/0012-821X(69)90190-3. Bibcode: 1969E&PSL...6..395B.
- ↑ Reynolds, J.; Turner, G. (Aug 1964). "Rare gases in the chondrite Renazzo". Journal of Geophysical Research 69 (15): 3263–81. doi:10.1029/JZ069i015p03263. Bibcode: 1964JGR....69.3263R.
- ↑ Gallino, R.; Bussot, M.; Picchiot, G.; Raiteri, C. (22 Nov 1990). "On the astrophysical interpretation of isotope anomalies in meteoritic SiC grains". Nature 348 (6299): 298–302. doi:10.1038/348298a0. Bibcode: 1990Natur.348..298G.
- Handbook of Elemental Abundances in Meteorites, Mason, B. ed. 1970 Gordon and Breach New York ISBN:9780677149509 Chapter 2: The Noble Gases, Heymann, D., p. 29
- Mazor, E. Heymann, D. Anders, E. Noble gases in carbonaceous chondrites. 1970 Geochimica et Cosmochimica Acta vol. 34 p. 781-824
- Goswami, J. Lal, D. Wilkening, L. Gas-Rich meteorites: Probes for particle environment and dynamical processes in the inner solar system 1983 Space Science Reviews vol. 37 p. 111-59
- The Sun in Time, Sonett, C. Giampapa, M. Mathews, M. eds. 1991 University of Arizona Press Tucson ISBN:978-0-8165-1297-3
- Ozima, M. Podosek, F. Noble Gases in Geochemistry, 2nd ed. 2002 Cambridge University Press Cambridge ISBN:9780521803663
- Noble Gases in Geochemistry and Cosmochemistry, Porcelli, D. Ballentine, C. Wieler, R. eds. 2002 Mineralogical Society of America Washington, DC
- Treatise on Geochemistry vol.1 2003 1.14 Noble Gases, Podosek, F. p. 381-403
- Meteorites and the Early Solar System II, Lauretta, D. McSween, H. eds. 2006 University of Arizona Press Tucson ISBN:9780816525621
- Geochemical Perspectives Jul 2013 vol. 2 issue 2 Special issue, Noble Gas Constraints on the Origin and Evolution of Earth's Volatiles ISSN 2223-7755
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