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  • 1975-1979  (10)
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Year
  • 1
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    Fluid inclusion studies of ore deposits in the Viburnum Trend, Southeast Missouri (1977)
    Society of Economic Geologists
    Details
    Publication Date: 1977-05-01
    Print ISSN: 0361-0128
    Electronic ISSN: 1554-0774
    Topics: Geosciences
    Published by Society of Economic Geologists
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    PAPER CURRENT
  • 2
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    Environment of ore deposition in the Creede mining district, San Juan Mountains, Colorado; Part III, Progress toward interpretation of the chemistry of the ore-forming fluid for the OH Vein (1977)
    Society of Economic Geologists
    Details
    Publication Date: 1977-02-01
    Print ISSN: 0361-0128
    Electronic ISSN: 1554-0774
    Topics: Geosciences
    Published by Society of Economic Geologists
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    PAPER CURRENT
  • 3
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    High-silica glass inclusions in olivine of Luna-24 samples (1977)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Description: Optical examination of nine polished grain mounts of Luna-24 drill-core material (0.09-0.50 mm size) revealed melt inclusions in olivine crystals. Two inclusions consist of clear glass with exceptionally high Si, yet contain no visible daughter minerals and have had no reaction effects with the olivine walls. Their compositions (one has SiO2 93.8, Al2O3 1.51, FeO 2.32, MgO 1.61, CaO 0.06, Na2O less than 0.05, K2O 0.11, total 99.41%; the other is similar) are unique and quite unlike the high-Si high-K melt of granitic composition that is found as inclusions in late-stage minerals of these (and the Apollo) samples, from silicate liquid immiscibility. The host olivines are Fo73 and Fo51. The origin of the melt in the inclusions and the lack of reaction effects are perplexing unsolved problems.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Geophysical Research Letters; 4; Oct. 197
    Format: text
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    NASA TECHNICAL REPORTS
  • 4
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    Melt inclusions in 75075 and 78505 - The problem of anomalous low -K inclusions in ilmenite revisited (1979)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Science Conference; Mar 19, 1979 - Mar 23, 1979; Houston, TX
    Format: text
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    NASA TECHNICAL REPORTS
  • 5
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    Anomalous low-K silicate melt inclusions in ilmenite from Apollo 17 basalts (1975)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: Primary silicate melt inclusions in ilmenite crystals in seven mare basalt samples were analyzed by electron microprobe, and analyses were made of their host and associated phases. Two distinct and restricted chemical composition ranges are drawn: high-K and low-K. The high-K samples are nearly identical with the granitic residual liquid, averaging a weight percentage of 6.27% K20, 76.3% SiO2, plus 82% normative quartz and orthoclase. It is noted that no low-K melt was found as a re-entrant or interstitial inclusion in any sample; only as isolated inclusions in illmenite.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 17, 1975 - Mar 21, 1975; Houston, TX
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    NASA TECHNICAL REPORTS
  • 6
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    Barred olivine 'chondrules' in lunar spinel troctolite 62295 (1977)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: Several objects have been found in sections of lunar igneous spinel troctolite 62295 that resemble certain meteoritic barred olivine chondrules. Each consists of an apparently spherical single crystal of Fo90 olivine, approximately 0.6-0.8 mm in diameter, containing a set of approximately 30-40 subparallel stringers of An95 plagioclase, whereas the stringers in ordinary meteoritic chondrules consist of glass. The olivine of the 62295 chondrules is also more magnesian, and is radially zoned, having a relatively iron-rich core and rim and an iron-poor intermediate zone. Several possible origins are proposed: impact-generated melt globules solidified in flight, spherical phenocrysts, and meteoritic chondrules, but none of these seems adequate to explain the detailed observations.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 14, 1977 - Mar 18, 1977; Houston, TX
    Format: text
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    NASA TECHNICAL REPORTS
  • 7
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    Compositional interrelationships of mare basalts from bulk chemical and melt inclusion studies (1976)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: Petrographic and electron microprobe data (355 new analyses) are presented on melt inclusions and their host phases found in a reexamination of the Apollo thin section collection. In addition, occurrences of early armalcolite and ilmenite are described and new data are presented on quench-pyroxene compositions and melt inclusions in chromian ulvospinel. Compositional differences between mare basalt types and their melt inclusions are illustrated with plots of compositions normalized to a terrestrial lava composition, that of the 1965 Makaopuhi lava lake. The plots emphasize the fact that mare basalts are not significantly differentiated relative to the compositions that are possible as defined by the melt inclusion data. Distribution coefficients for Fe and Mg partitioning between trapped melt and host olivine and ilmenite are calculated and show a range about probable equilibrium values. It is suggested that the crystallization sequence olivine-ilmenite-plagioclase-pyroxene defined by the melt inclusion data may be the actual sequence which obtained generally for Apollo 11 and 17 mare basalts just prior to eruption.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 15, 1976 - Mar 19, 1976; Houston, TX
    Format: text
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    NASA TECHNICAL REPORTS
  • 8
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    The problem of the origin of symplectites in olivine-bearing lunar rocks (1975)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: In a study of its origin in olivine-bearing lunar rocks, symplectite is grouped into the following types: (1) very abundant blebs in olivine phenocrysts, (2) scattered blebs in dunite, (3) scattered elongated masses along grain boundaries in troctolite, (4) scattered mosaic assemblages of coarser minerology along grain boundaries, (5) very abundant needle-like arrays, and (6) very abundant grains dispersed in rows. Four theories are proposed to explain the various symplectite distributions.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 17, 1975 - Mar 21, 1975; Houston, TX
    Format: text
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    NASA TECHNICAL REPORTS
  • 9
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    Shock glass veins in some lunar and meteoritic samples - Their nature and possible origin (1977)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: Glassy veinlets, 15 microns to 1 mm thick and now in part devitrified, cut through breccias 67915, 67936, and 67955 from Outhouse Rock, and similar veins have been found in several other lunar samples and in meteorites. The veins have features suggesting injection of extremely hot material, possibly at several thousands degrees of superheat, presumably from an impact event. The vein compositions are very similar but not identical to the bulk compositions of the host rocks. Two mechanisms of injection are considered feasible-injection of hot liquid and injection of hot particulate matter (resembling a 'fluidized bed'), but neither mechanism fully explains all details of the occurrences.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 14, 1977 - Mar 18, 1977; Houston, TX
    Format: text
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    NASA TECHNICAL REPORTS
  • 10
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    Compositional variation in late-stage differentiates in mare lavas, as indicated by silicate melt inclusions (1977)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: Questions regarding an interpretation of data from silicate melt inclusions are considered, taking into account the fragmental nature of the record, the possible effects of cooling rate on late-stage melt composition, and the crystallization of the trapped melt. New data related to 484 new analyses are provided in a separate table. Textural and mineralogical features and bulk chemical composition for an overall characterization of late-stage differentiates are discussed. A description is presented of a grouping and recognition of rock types on the basis of late-stage inclusion analyses. Attention is given to the bimodality of potassium values and the delineation of differentiation trends. It is found that many of the problems in interpretation and much of the scatter found in the composition of silicate melt inclusions in lunar samples can be attributed to the incomplete nature of the record and to crystallization after trapping.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 14, 1977 - Mar 18, 1977; Houston, TX
    Format: text
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    NASA TECHNICAL REPORTS
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