Temat: Chondrite - Katalog OPAC zbiorów

Skocz do pozycji: 1.

Tytuł:: Średni ciężar atomowy chondrytu Sołtmany, chondrytów L6 i minerałów pozaziemskich
Mean atomic weight of Sołtmany chondrite, L6 chondrites and extraterrestrial minerals
Autorzy:: Szurgot, Marian
Powiązania:: https://bibliotekanauki.pl/articles/1033038.pdf
Data publikacji:: 2015
Wydawca:: Polskie Towarzystwo Meteorytowe
Tematy:: Girgenti chondrite
Holbrook chondrite
Jesenice chondrite
Leedey chondrite
Modoc chondrite
Sołtmany chondrite
chondrites
elemental composition
grain density
mean atomic weight
Opis:: Mean atomic weight Amean of Sołtmany (L6, S2, W0) ordinary chondrite, various L6 chondrites such as: Jesenice, Girgenti, Leedey, Bruderheim, Holbrook and Modoc, as well as LL, L and H chondrites has been determined using literature data on chemical composition of the meteorites. Relationship between mean atomic weight and Fe/Si atomic ratio for ordinary chondrites has been established. It was shown that Sołtmany’s Amean = 23.97 is close to mean atomic weight of L chondrites Amean = 23.70, and is close to mean atomic weight of L6 chondrites Amean = 24.06±0.16. It has been established that Sołtmany’s Fe/Si atomic ratio (Fe/Si = 0.588) is close to Fe/Si ratio for L6 chondrites (Fe/Si = 0.598). This means that Sołtmany belongs to L6 chondrites, as previously classified. Using discovered by the author (Szurgot, 2015) dependence between mean atomic weight and uncompressed density of planetary matter it was established that grain density of Sołtmany meteorite should be equal to 3.56±0.12 g/cm3, which is about 4% lower than previously estimated by porosity data. Mean atomic weight of extraterrestrial minerals present in ordinary chondrites and in Sołtmany meteorite have been also determined.
Źródło:: Acta Societatis Metheoriticae Polonorum; 2015, 6; 107-128
2080-5497
Pojawia się w:: Acta Societatis Metheoriticae Polonorum
Dostawca treści:: Biblioteka Nauki

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Tytuł:: Northwest Africa 7915: A New approved LL5 chondrite from Morocco
Autorzy:: Brawata, M.
Kryza, R.
Jakubowski, T.
Przylibski, T. A.
Ćwiąkalski, J.
Łuszczek, K.
Powiązania:: https://bibliotekanauki.pl/articles/411506.pdf
Data publikacji:: 2014
Wydawca:: Polskie Towarzystwo Meteorytowe
Tematy:: chondrite
NWA 7915
Morocco
chondrule
chondrite chemistry
chondrite weathering
Opis:: A 415 g single meteorite was purchased in 2010 by T. Jakubowski from a dealer in Morocco. The meteorite was isometric in shape, ca. 8 cm in size, with distinct regmaglypts on the original ablated surface, and covered mostly in primary crust with one broken surface. The weight of the sample studied was 69 g. The meteorite is composed of several types of chondrules including porphyritic-Ol-Px, barred-Ol, radial-Px, granular and cryptocrystalline with distinct and diffused (not sharp) boundaries, and opaque grains and aggregates, enclosed in a very fine-grained matrix. The average compositions of minerals are: olivine (both in chondrules and matrix) − Fo70.4Fa29.1Te0.5, pyroxenes, represented by Mg-Fe (Ca-poor) orthopyroxene (and minor clinopyroxene?) − En73.9Fs24.1Wo2.0, feldspars (small in the matrix and in barred chondrules), with An12-37, and Or~3-4, taenite − Fe 70.80, Ni 25.50 and Co 1.67 wt. %, troilite − Fe0.98S1.00, chromite (Fe2+ 0.96Mg0.12Mn0.01Zn0.01) (Cr1.52Al0.23Fe3+ 0.02Ti0.10Si0.02)O4; altered accessory minerals including apatite and iron-rich secondary phases have also been identified and analyzed. The meteorite is of petrologic type 5, as evidenced by the observed recrystallization of the matrix, relatively good preservation of the chondrule structures, homogeneous composition of olivine and pyroxene, and the presence of only secondary small feldspar grains. The shock stage, S2, is based on the presence of undulatory extinction and irregular fractures in olivine crystals. The weathering grade, W3, is confirmed by the observation that kamacite is totally altered into secondary iron phases, whereas Nirich taenite, and troilite are only partly weathered. The specimen shows many bulk- and mineral-chemical parameters corresponding, mostly, to the LL chondrite group (e.g., Fe/SiO2 0.49, SiO2/MgO 1.62, Fa in olivine 29.05). However, concentrations of several other elements, including REE, are not fully consistent with the average values for the LL ordinary chondrites. Apparently, the parent body of the studied NWA 7915 meteorite was depleted in Dy, Tm, and Yb, compared to typical LL-type ordinary chondrite parent bodies. Also, relatively high concentrations of other elements, including Ba and Sr, have been measured, which may result from terrestrial weathering in hot desert conditions. The meteorite has been classified as LL5 ordinary chondrite, S2, W3, and registered in the Meteoritical Society database as NWA 7915. The type specimen is deposited in the Mineralogical Museum of the University of Wrocław.
Źródło:: Meteorites; 2014, 3, No. 1-2; 45-58
2299-0313
2299-1220
Pojawia się w:: Meteorites
Dostawca treści:: Biblioteka Nauki

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Tytuł:: Nowy chondryt zwyczajny L6, S1, W1: Northwest Africa 11779
A new ordinary chondrite L6, S1, W1: Northwest Africa 11779
Autorzy:: Przylibski, Tadeusz A.
Łuszczek, Katarzyna
Kryza, Ryszard
Powiązania:: https://bibliotekanauki.pl/articles/1033133.pdf
Data publikacji:: 2019
Wydawca:: Polskie Towarzystwo Meteorytowe
Tematy:: L6 chondrite
NWA chondrite
bulk chemistry
chemistry of minerals
meteorite
ordinary chondrite
Opis:: Based on petrological, mineralogical and geochemical research authors classified new meteorite Northwest Africa 11779 as the ordinary chondrite L6, S1, W1. Chemical composition of olivine crystals (Fa 24.9 mol.%) and of pyroxene crystals (Fs 19.4 mol.%) proved that this meteorite belongs to L chondrites. However, bulk chemical composition of NWA 11779 is not typical for L chondrites. Nevertheless, all analyzed elements (except Mo, Sn and Nb) are in abundances reported for L chondrites, some of elements have concentration closed to average abundances for L chondrites. The content of chosen, characteristic lithophile, siderophile and chalkophile elements in NWA 11779 chondrite is in most cases in accord with its typical abundance in L chondrites. Presence of poorly defined chondrules, secondary feldspar crystals larger than 50 µm in size, absence of glass within chondrules, coarse recrystallized matrix (with olivine crystals of 0.5 mm in diameter and pyroxene crystals of 0.3 mm in diameter) as well as carbon content below 0.2 wt% proved that studied meteorite belongs to the petrologic type 6. The only difference from characteristic features of petrologic type 6 in case of NWA 11779 chondrite is presence of ca. 10% of monoclinic Ca-poor pyroxenes. Undulatory extinction by olivine and absence of other shock features in this chondrite allow to determine the shock level as S1. Weathering grade of NWA 11779 was identified as W1 based on weathering of only FeNi alloy grains. The outer part of metallic grains as well as contact zones of FeNi and FeS are changed due to weathering. Between 10 and 20% of FeNi alloy grains are oxidized to iron oxides and hydroxides. These secondary products of weathering replace outer zone of FeNi grains and fill the small cracks, creating a few thin veins.
Źródło:: Acta Societatis Metheoriticae Polonorum; 2019, 10; 121-139
2080-5497
Pojawia się w:: Acta Societatis Metheoriticae Polonorum
Dostawca treści:: Biblioteka Nauki

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Skocz do pozycji: 4.

Tytuł:: Nowy chondryt zwyczajny H5, S2, W1: Northwest Africa 11778
A new ordinary chondrite H5, S2, W1: Northwest Africa 11778
Autorzy:: Przylibski, Tadeusz
Łuszczek, Katarzyna
Kryza, Ryszard
Blutstein, Konrad
Powiązania:: https://bibliotekanauki.pl/articles/1033153.pdf
Data publikacji:: 2020
Wydawca:: Polskie Towarzystwo Meteorytowe
Tematy:: H5 chondrite
NWA chondrite
bulk chemistry
chemistry of minerals
meteorite
ordinary chondrite
Opis:: Based on petrological, mineralogical and geochemical analyses, the authors classified the new meteorite Northwest Africa 11778 as an ordinary chondrite H5, S2, W1. It is a single stone with mass 767.5 g and with well-preserved black fusion crust with brown shade (Fig. 1). This meteorite was found in Sahara Desert and it was purchased by Wroclaw University of Science and Technology, Faculty of Geoengineering, Mining and Geology from Moroccan dealer in Zagora in June 2013. The most characteristic component of analyzed chondrite are different types of chondrules (barred olivine – BO, porphyritic olivine – PO, granular olivine – GO, radial pyroxene – RP, porphyritic olivine-pyroxene – POP, cryptocrystalline – C) (Fig. 2), which constitute 75% of meteorite. Their size is in range 0.2–1.2 mm, with average chondrule size ca. 0.6 mm. Bigger porphyritic olivine chondrules with diameter up to 1.5 mm rarely occur. The chemical composition of olivine crystals (Fa 18 mol%) and pyroxene crystals (Fs 16.2 mol%) proves this meteorite to be an H chondrite (Tab. 1, Fig. 4–5, App. 1–2). The averaged concentration of major elements in the classified meteorite is comparable to their mean content in H chondrites (Fig. 8). The meteorite NWA 11778 contains only slightly less Mg and Al than average H chondrites (Tab. 2). Among the other analysed elements, values distinctly out of the range of typical concentrations for H chondrites are characteristic of Hg and Eu (lower concentration in the NWA 11778 meteorite) (Tab. 3, Fig. 8–9). The presence of chondrules with predominantly sharp boundaries (Fig. 2), secondary feldspar crystals with sizes of up to 50 mm, chiefly crystalline mesostasis and only secondarily – devitrified glass in chondrules, and transparent crystalline matrix (with olivine crystals up to 0.26 mm and pyroxenes up to 0.30 mm in size), as well as common occurrence of untwinned rhombic pyroxenes prove the classified meteorite to belong to petrological type 5. It is additionally confirmed by mean Ni content in troilite below 0.5 wt% (0.04 wt%) (Tab. 1, App. 4) and carbon content below 0.2 wt% (0.07 wt%) (Tab. 2). Undulatory extinction in some olivine and pyroxene crystals and the presence of irregular fractures in the NWA 11778 chondrite enables specifying its shock level as S2. The weathering grade adopted for the NWA 11778 chondrite was W1, as visible weathering changes cover only the marginal parts of FeNi alloy grains. As a result of the weathering of 10–20% of FeNi grains, iron oxides and hydroxides are formed. These secondary weathering Fe3+ compounds also fill cracks, forming veins running between chondrules within matrix (Fig. 3).
Źródło:: Acta Societatis Metheoriticae Polonorum; 2020, 11; 77-97
2080-5497
Pojawia się w:: Acta Societatis Metheoriticae Polonorum
Dostawca treści:: Biblioteka Nauki

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Skocz do pozycji: 5.

Tytuł:: Mineralogy and petrology of two ordinary chondrites and their correlation with other meteorites
Autorzy:: Owocki, Krzysztof
Pilski, Andrzej
Powiązania:: https://bibliotekanauki.pl/articles/2086510.pdf
Data publikacji:: 2009
Wydawca:: Polskie Towarzystwo Mineralogiczne
Tematy:: ordinary chondrite
type 6 chondrite
shock metamorphism
Dhofar
Opis:: Two ordinary chondrites are compared and classified using transmitted and reflected light microscopy and electron microprobe analyses. Both meteorites were confiscated by the Polish Customs Service at the border with Belarus. The first meteorite (called in this paper Terespol-1) is a L/LL6 chondrite, its classification being supported by the equilibrated compositions of olivine and orthopyroxene and the presence of large recrystallized feldspars (< 150 μm). The specimen examined experienced weak shock metamorphism (S3) and moderate weathering (although metal in the inner part of the meteorite seems to be unaffected by oxidization). The other meteorite (called in this paper Terespol-2) is a LL6 chondrite which experienced weak shock metamorphism (S3) and is unaffected by weathering. The Terespol-2 meteorite shares its classification with the Dhofar 1401 chondrite but the lack of data prevents further correlation. Both meteorites have been correlated with known findings from the Meteoritical Bulletin database and an attempt is made to identify their place of origin (fall event). Results indicate that Terespol-1 is most closely related to the Dhofar 1316 chondrite and we suggest that both meteorites at least came from the same parent body.
Źródło:: Mineralogia; 2009, 40, 1/4; 107--116
1899-8291
1899-8526
Pojawia się w:: Mineralogia
Dostawca treści:: Biblioteka Nauki

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Skocz do pozycji: 6.

Tytuł:: Mineralogy and petrology of two ordinary chondrites and their correlation with other meteorites
Autorzy:: Owocki, K.
Pilski, A.
Powiązania:: https://bibliotekanauki.pl/articles/2086559.pdf
Data publikacji:: 2009
Wydawca:: Polskie Towarzystwo Mineralogiczne
Tematy:: ordinary chondrite
type 6 chondrite
shock metamorphism
Dhofar
Opis:: Two ordinary chondrites are compared and classified using transmitted and reflected light microscopy and electron microprobe analyses. Both meteorites were confiscated by the Polish Customs Service at the border with Belarus. The first meteorite (called in this paper Terespol-1) is a L/LL6 chondrite, its classification being supported by the equilibrated compositions of olivine and orthopyroxene and the presence of large recrystallized feldspars (< 150 μm). The specimen examined experienced weak shock metamorphism (S3) and moderate weathering (although metal in the inner part of the meteorite seems to be unaffected by oxidization). The other meteorite (called in this paper Terespol-2) is a LL6 chondrite which experienced weak shock metamorphism (S3) and is unaffected by weathering. The Terespol-2 meteorite shares its classification with the Dhofar 1401 chondrite but the lack of data prevents further correlation. Both meteorites have been correlated with known findings from the Meteoritical Bulletin database and an attempt is made to identify their place of origin (fall event). Results indicate that Terespol-1 is most closely related to the Dhofar 1316 chondrite and we suggest that both meteorites at least came from the same parent body.
Źródło:: Mineralogia; 2009, 40, 1/4; 107--116
1899-8291
1899-8526
Pojawia się w:: Mineralogia
Dostawca treści:: Biblioteka Nauki

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Skocz do pozycji: 7.

Tytuł:: Chondryty węgliste CI oraz podobne do CI
CI and CI-like carbonaceous chondrites
Autorzy:: Blutstein, Konrad
Powiązania:: https://bibliotekanauki.pl/articles/30146491.pdf
Data publikacji:: 2024-04
Wydawca:: Polskie Towarzystwo Meteorytowe
Tematy:: carbonaceous chondrite
meteorite
CI chondrite
CY chondrite
chondryt węglisty
meteoryt
chondryt CI
chondryt CY
Opis:: Carbonaceous chondrites of the CI group represent the most primitive matter in the Solar System available for study. Currently, only 9 meteorites have been classified as CI group carbonaceous chondrites, with the classification of two of them being questioned. In the literature, there is a suggestion to consider these two meteorites, along with others that share similarities, as a separate CY group. Additionally, the Tagish Lake meteorite is considered CI2, although this classification has not gained widespread acceptance. Based on a limited number of scientific sources regarding the elemental composition of CI group carbonaceous chondrites and CI-like chondrites, it has been observed that Alais, Ivuna, and Orgueil chondrites have the most similar elemental composition. The composition of the Tonk chondrite differs slightly but still falls within the typical range for CI group chondrites. The chemical composition of the Revelstoke meteorite significantly deviates from the average composition of CI group chondrites; however, the small mass of this meteorite (1 g) and a lack of sufficient data may affect the results. Among CI-like chondrites, the best match in chemical composition to CI chondrites is found for the Tagish Lake chondrite. Conversely, the Belgica 7904 chondrite, previously considered a member of the potential CY group, unequivocally does not belong to CI or CY group based on its chemical composition. While potential CY chondrites exhibit significant cadmium depletion, the possibility of coincidental convergence on this matter cannot be excluded. From a mining perspective, parent bodies of CI group carbonaceous chondrites may serve as a potential source of water and, consequently, hydrogen, holding significant importance as potential fuel. Asteroid 1508 Kemi, which is a potential parent body of CI carbonaceous chondrites, may contain about 3.39·1012 Mg of water, including about 3.76·1011 Mg of hydrogen.
Chondryty węgliste z grupy CI stanowią najbardziej pierwotną materię w Układzie Słonecznym dostępną do badań. Obecnie tylko 9 meteorytów zostało sklasyfikowanych jako chondryty węgliste grupy CI, z czego dla dwóch z nich klasyfikacja ta jest kwestionowana. W literaturze sugeruje się, aby te dwa meteoryty, wraz z innymi podobnymi, uznać za osobną grupę CY. Dodatkowo, meteoryt Tagish Lake jest rozważany jako CI2, chociaż ta klasyfikacja nie zdobyła powszechnej akceptacji. Na podstawie ograniczonej ilości źródeł literaturowych dotyczących składu pierwiastkowego chondrytów grupy CI oraz chondrytów podobnych do CI, stwierdzono, że chondryty Alais, Ivuna oraz Orgueil mają najbardziej zbliżony skład pierwiastkowy. Skład chondrytu Tonk różni się nieznacznie, ale wciąż mieści się w zakresie typowym dla chondrytów grupy CI. Skład chemiczny meteorytu Revelstoke znacząco odbiega od średniego składu chondrytów grupy CI, jednak niewielka masa tego meteorytu (1 g) i brak dostatecznej ilości danych mogą wpływać na wyniki. Spośród chondrytów podobnych do CI, najlepsze dopasowanie składu chemicznego do grupy CI wykazuje chondryt Tagish Lake. Natomiast najgorsze dopasowanie charakteryzuje chondryt Belgica 7904, uważany za członka potencjalnej grupy CY, jednak na podstawie składu chemicznego jednoznacznie można stwierdzić, że nie należy do grupy CI lub CY. Chociaż potencjalne chondryty CY wykazują znaczne zubożenie w kadm, nie można wykluczyć przypadkowej zbieżności w tej kwestii. Z perspektywy górniczej, ciała macierzyste chondrytów węglistych grupy CI mogą stanowić potencjalne źródło wody, a co za tym idzie, również wodoru, mającego istotne znaczenie jako potencjalne paliwo. Planetoida 1508 Kemi będąca potencjalnym ciałem macierzystym chondrytów węglistych grupy CI może zawierać około 3,39·1012 Mg wody, w tym około 3,76·1011 Mg wodoru.
Źródło:: Acta Societatis Metheoriticae Polonorum; 2024, 15; 7-26
2080-5497
Pojawia się w:: Acta Societatis Metheoriticae Polonorum
Dostawca treści:: Biblioteka Nauki

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Skocz do pozycji: 8.

Tytuł:: Wyniki badań mineralogicznych i petrologicznych nowych okazów meteorytu Pułtusk w 150 rocznicę spadku
Results of mineralogical and petrological research of new samples on the Pułtusk meteorite at the 150th anniversary of the fall
Autorzy:: Przylibski, T. A.
Łuszczek, K.
Powiązania:: https://bibliotekanauki.pl/articles/2075816.pdf
Data publikacji:: 2018
Wydawca:: Państwowy Instytut Geologiczny – Państwowy Instytut Badawczy
Tematy:: Pułtusk
meteoryt
chondryt
zwyczajny chondryt
chondryt H5
meteorite
chondrite
ordinary chondrite
H5 chondrite
Opis:: One of the largest observed stone meteorite shower in the history of mankind on Earth took place on Thursday evening on January 30, 1868, about seven o’clock near Pułtusk in Poland. Despite the 150th anniversary of the fall of chondrite officially classified as Pułtusk H5 with a shock stage S3 there is still little published data on the chemical composition of minerals of this chondrite as well as its petrological characteristics in the literature. The authors carried out mineralogical and petrological research that will help a little to fill this gap in knowledge about the Pułtusk chondrite. Meteorite specimens found by Piotr Kuś in 2015 and investigated by the authors are undoubtedly part of the Pułtusk fall of January 30, 1868. They can be classified as ordinary chondrite H5, S2,W2. The authors stated that the studied rock is characterized by a varied shock level -from S1 to S2/3, as well as it contains chondrules of the chromite-plagioclase unequilibrated rock. In the composition of the examined fragment of Pułtusk chondrite, the authors identified silicates: olivine, diopside, bronzite and clinohyperstene, and oligoclase, oxides: chromite (and spinel), sulfides: troilite, FeNi alloy mineral phases: kamacite and taenite, as well as phosphates: merrilite and apatite. The chemical composition of olivine crystals as well as low- and high-Ca pyroxenes crystals and plagioclase crystals (about the composition of oligoclase) confirms that the examined specimen comes from the Pułtusk fall and it is a rock that should be classified as a petrographic type H5.
Źródło:: Przegląd Geologiczny; 2018, 66, 6; 368--378
0033-2151
Pojawia się w:: Przegląd Geologiczny
Dostawca treści:: Biblioteka Nauki

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Skocz do pozycji: 9.

Tytuł:: Średni ciężar atomowy, średnia objętość i promień atomu chondrytu Creston (L5/6)
Mean atomic weight, mean volume and radius of atom of Creston (L5/6) chondrite
Autorzy:: Szurgot, Marian
Powiązania:: https://bibliotekanauki.pl/articles/30146488.pdf
Data publikacji:: 2024-04
Wydawca:: Polskie Towarzystwo Meteorytowe
Tematy:: Creston chondrite
Ensisheim chondrite
Jezersko chondrite
mean atomic weight
mean volume of atom
mean radius of atom
Opis:: Mean atomic weight Amean, mean volume and mean radius of atom of Creston ordinary chondrite (L5/6 S4 W0) felt in 2015 in Creston near Paso Robles, California has been calculated using literature data on chemical composition of the meteorite (Jenniskens et al. 2019). The aim of the studies was to determine Amean, Vatom, and Ratom values for this new meteorite, and compare the data with the values obtained for two other ordinary chondrites: Ensisheim (LL6), and Jezersko (H4). Calculations were conducted for the whole rock, for silicates, and for Fe, Ni metal of Creston, and Ensisheim chondrites. It was shown that the mean atomic weight of the whole rock of Creston chondrite Amean = 24.06. Creston’s silicates revealed the value: Ameansi = 21.92, and Creston’s Fe,Ni metal: Ameanmet = 56.25. It was calculated that the average volume of the Creston’s atom Vatom = 1.111·10–29 m3 (sample CR05), and 1.115·10–29 m3 (sample CR06). Average radius of Creston’s atom: Ratom = 138.5 pm, mean radius of atom of Creston silicates: Ratomsi = 138 pm, and mean radius of atom of Creston metal: Ratommet = 142 pm.
Źródło:: Acta Societatis Metheoriticae Polonorum; 2024, 15; 116-128
2080-5497
Pojawia się w:: Acta Societatis Metheoriticae Polonorum
Dostawca treści:: Biblioteka Nauki

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Skocz do pozycji: 10.

Tytuł:: Bulk chemical composition of Sołtmany chondrite
Autorzy:: Przylibski, T. A.
Łuszczek, K.
Powiązania:: https://bibliotekanauki.pl/articles/411498.pdf
Data publikacji:: 2012
Wydawca:: Polskie Towarzystwo Meteorytowe
Tematy:: meteorite
ordinary chondrite
L-chondrite
bulk composition
meteorite fall
observed fall
Opis:: The authors examined the bulk chemical composition of the Sołtmany chondrite which fell on April 30th, 2011 in Northern Poland. Based on the analysis of 47 elements, it was concluded that Sołtmany is representative of L-type of ordinary chondrites. However, compared to the average values observed in other L-type ordinary chondrites, Sołtmany displays higher content of Ni, P, Cd, Pb, and As. The Ni and P content closely resembles typical values for H-type ordinary chondrites. Furthermore, Sołtmany displays other distinct properties including very low Zn content and lower contents of Mo and Zr than the average values found in other L-type ordinary chondrites. Consistent with other L-type ordinary chondrites, the absolute content of REE in Sołtmany is higher than that of CI-type carbonaceous chondrites while the REE trend lines for both Sołtmany and CI-chondrites are similar. Due to similar times of year of when both falls took place and the proximity of their strewn fields, the chemical composition of Sołtmany was compared with that of Jesenice, an L6 ordinary chondrite which fell on April 9th, 2009 in Europe. The analysis led to a conclusion that Sołtmany and Jesenice are not launch-paired. Nevertheless, even though they do not represent fragments of the same meteoroid, their origin on a common parent body (an asteroid – planetesimal) cannot be conclusively ruled out on the sole basis of their bulk chemical composition.
Źródło:: Meteorites; 2012, 2, No. 1-2; 31-37
2299-0313
2299-1220
Pojawia się w:: Meteorites
Dostawca treści:: Biblioteka Nauki

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