The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition
Kaba meteorite as a reference material (one of a least metamorphosed and most primitive carbonaceous chondrites fell on Earth) was chosen for this study providing an adequate background for study of the protoplanetary disk or even the crystallization processes of the Early Solar System. Its olivine...
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De Gruyter
2021
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oai:doaj.org-article:404413282ff8467983d1cd1f246511f32021-12-05T14:10:40ZThe Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition2543-637610.1515/astro-2021-0006https://doaj.org/article/404413282ff8467983d1cd1f246511f32021-10-01T00:00:00Zhttps://doi.org/10.1515/astro-2021-0006https://doaj.org/toc/2543-6376Kaba meteorite as a reference material (one of a least metamorphosed and most primitive carbonaceous chondrites fell on Earth) was chosen for this study providing an adequate background for study of the protoplanetary disk or even the crystallization processes of the Early Solar System. Its olivine minerals (forsterite and fayalite) and their Mg/Fe ratio can help us to understand more about the planet formation mechanism and whether or not the metallic constitutes of the disk could be precursors for the type of planets in the Solar System. A multiple methodological approach such as a combination of the scanning electron microscope, optical microscope, Raman spectroscopy and electron microprobe of the olivine grains give the Fe/Mg ratio database. The analyses above confirmed that planet formation in the protoplanetary disk is driven by the mineralogical precursors of the crystallization process. On the other hand, four nebulae mentioned in this study provide the astronomical data confirming that the planet formation in the protoplanetary disk is dominated or even driven by the metallic constituents.Futó PéterVanyó JózsefSimonia IrakliSztakovics JánosNagy MihályGucsik ArnoldDöncző BoglárkaKertész ZsófiaNovák RichárdCsámer ÁrpádDe Gruyterarticlemeteoritescircumstellar environmentplanetmineralastrophysicsAstronomyQB1-991ENOpen Astronomy, Vol 30, Iss 1, Pp 45-55 (2021) |
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meteorites circumstellar environment planet mineral astrophysics Astronomy QB1-991 |
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meteorites circumstellar environment planet mineral astrophysics Astronomy QB1-991 Futó Péter Vanyó József Simonia Irakli Sztakovics János Nagy Mihály Gucsik Arnold Döncző Boglárka Kertész Zsófia Novák Richárd Csámer Árpád The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition |
| description |
Kaba meteorite as a reference material (one of a least metamorphosed and most primitive carbonaceous chondrites fell on Earth) was chosen for this study providing an adequate background for study of the protoplanetary disk or even the crystallization processes of the Early Solar System. Its olivine minerals (forsterite and fayalite) and their Mg/Fe ratio can help us to understand more about the planet formation mechanism and whether or not the metallic constitutes of the disk could be precursors for the type of planets in the Solar System. A multiple methodological approach such as a combination of the scanning electron microscope, optical microscope, Raman spectroscopy and electron microprobe of the olivine grains give the Fe/Mg ratio database. The analyses above confirmed that planet formation in the protoplanetary disk is driven by the mineralogical precursors of the crystallization process. On the other hand, four nebulae mentioned in this study provide the astronomical data confirming that the planet formation in the protoplanetary disk is dominated or even driven by the metallic constituents. |
| format |
article |
| author |
Futó Péter Vanyó József Simonia Irakli Sztakovics János Nagy Mihály Gucsik Arnold Döncző Boglárka Kertész Zsófia Novák Richárd Csámer Árpád |
| author_facet |
Futó Péter Vanyó József Simonia Irakli Sztakovics János Nagy Mihály Gucsik Arnold Döncző Boglárka Kertész Zsófia Novák Richárd Csámer Árpád |
| author_sort |
Futó Péter |
| title |
The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition |
| title_short |
The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition |
| title_full |
The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition |
| title_fullStr |
The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition |
| title_full_unstemmed |
The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition |
| title_sort |
mg/fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: a case study for the chondritic-like composition |
| publisher |
De Gruyter |
| publishDate |
2021 |
| url |
https://doaj.org/article/404413282ff8467983d1cd1f246511f3 |
| work_keys_str_mv |
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