Mineralogy and magnetism of Fe-Cr spinel series minerals from podiform chromitites and dunites from Tąpadła (Sudetic ophiolite, SW Poland) and their relationship to palaeomagnetic results of the dunites
Abstract:S U M M A R YThis paper presents the mineralogy and magnetic properties of two varieties of chromitite, sampled in the same exposure of a serpentinite massif regarded to be a fragment of the Sudetic ophiolite. The varieties differ mineralogically and magnetically. One of them, labelled TaA and altered to a low degree according to scanning electron microscope (SEM) and microprobe results, comprises an unaltered Al-Cr spinel core, some secondary chromite and less abundant Cr-magnetite. It has a high magnetic sus… Show more
“…Cr‐rich spinel can entirely constitute the NRM (Figure 4) or it can dominate the NRM while coexisting with magnetite (Figure 5). In particular, Cr‐rich spinel often records T c of 200–350°C both in terrestrial (e.g., Hounslow, 1996; Kądziałko‐Hofmokl et al, 2008; Kumar & Bhalla, 1984a; Murthy & Krishnamacharyulu, 1994; O'Driscoll & Petronis, 2009; Xu et al, 1997; Yu et al, 2001) and in extraterrestrial (e.g., Yu & Gee, 2005) materials. In this study, Group B spinel shows maximum unblocking temperatures of 200–280°C.…”
In comparison to the six spinel end-members in the spinel prism, magnetic information on the intermediate spinel compositions is relatively poorly established. To investigate magnetic properties of intermediate compositions of Cr-rich spinel, we collected 12 samples that might contain potentially magnetic Cr-rich spinel. On the basis of chemical composition analysis and physical magnetic behavior, magnetic Group A Fe-rich spinel (i.e., magnetite), magnetic Group B Cr-rich spinel, and paramagnetic Group C Cr-Al-rich spinel were identified. Magnetite is solely responsible for the natural remanent magnetization (NRM) in severely serpentinized samples from intraoceanic island arcs, orogenic exposures of ultramafics, and back-arc continental lithosphere settings. Magnetic Group B Cr-rich spinel shows maximum unblocking temperatures of 200-280°C. Such temperatures permit Cr-rich spinel to contribute to magnetic anomalies up to about 8-12 km in terrestrial lithosphere settings, given a normal geothermal gradient of 25 K/km. The existence of magnetic Cr-rich spinel requires certain compositional conditions including a cation ratio of [Cr]/[Fe 2+ + Fe 3+ ] from 1.33 to 1.56 as well as a low oxide ratio of (Al 2 O 3 + MgO)/ (Cr 2 O 3 + FeO + Fe 2 O 3) less than 10%. It is evident that compositions of spinels are related with the degree of serpentinization as Group A spinel is observed along the fractures between/among olivine grains in heavily serpentinized rocks. Spinels in Groups B and C seem to experience less severe metasomatic or hydrothermal alteration during serpentinization. Distribution of magnetic Cr-rich spinel along the fractures of silicates (mostly olivine) may support a chemical origin of the NRM. Thus, Cr-rich spinel is a potential NRM carrier and a source of magnetic anomalies in ultramafic complexes.
“…Cr‐rich spinel can entirely constitute the NRM (Figure 4) or it can dominate the NRM while coexisting with magnetite (Figure 5). In particular, Cr‐rich spinel often records T c of 200–350°C both in terrestrial (e.g., Hounslow, 1996; Kądziałko‐Hofmokl et al, 2008; Kumar & Bhalla, 1984a; Murthy & Krishnamacharyulu, 1994; O'Driscoll & Petronis, 2009; Xu et al, 1997; Yu et al, 2001) and in extraterrestrial (e.g., Yu & Gee, 2005) materials. In this study, Group B spinel shows maximum unblocking temperatures of 200–280°C.…”
In comparison to the six spinel end-members in the spinel prism, magnetic information on the intermediate spinel compositions is relatively poorly established. To investigate magnetic properties of intermediate compositions of Cr-rich spinel, we collected 12 samples that might contain potentially magnetic Cr-rich spinel. On the basis of chemical composition analysis and physical magnetic behavior, magnetic Group A Fe-rich spinel (i.e., magnetite), magnetic Group B Cr-rich spinel, and paramagnetic Group C Cr-Al-rich spinel were identified. Magnetite is solely responsible for the natural remanent magnetization (NRM) in severely serpentinized samples from intraoceanic island arcs, orogenic exposures of ultramafics, and back-arc continental lithosphere settings. Magnetic Group B Cr-rich spinel shows maximum unblocking temperatures of 200-280°C. Such temperatures permit Cr-rich spinel to contribute to magnetic anomalies up to about 8-12 km in terrestrial lithosphere settings, given a normal geothermal gradient of 25 K/km. The existence of magnetic Cr-rich spinel requires certain compositional conditions including a cation ratio of [Cr]/[Fe 2+ + Fe 3+ ] from 1.33 to 1.56 as well as a low oxide ratio of (Al 2 O 3 + MgO)/ (Cr 2 O 3 + FeO + Fe 2 O 3) less than 10%. It is evident that compositions of spinels are related with the degree of serpentinization as Group A spinel is observed along the fractures between/among olivine grains in heavily serpentinized rocks. Spinels in Groups B and C seem to experience less severe metasomatic or hydrothermal alteration during serpentinization. Distribution of magnetic Cr-rich spinel along the fractures of silicates (mostly olivine) may support a chemical origin of the NRM. Thus, Cr-rich spinel is a potential NRM carrier and a source of magnetic anomalies in ultramafic complexes.
“…This limit (n = 0.6) has therefore been applied to define the superior compositional boundary of ferritchromite in terms of Cr content ( Figure 1a). Kądziałko-Hofmokl et al (2008) defined the Cr-magnetite according to its magnetic properties, that is, a ferritchromite with a magnetic behavior close to that of magnetite in terms of saturation magnetization and T c . Yet, Cr-magnetite is still not defined in terms of its chemical composition, and a better constraint on this transition and the associated n value is needed.…”
Section: The Chromium-iron Spinel Systemmentioning
Rock magnetism methods can be judiciously used to recognize and understand some metamorphic processes. Serpentinization reactions, for example, generate a significant amount of magnetite that magnetic methods allow to efficiently identify and quantify (O'Hanley, 1996, p. 277). However, other magnetic phases
“…Previous studies of synthetics indicate that Cr‐Fe spinels can have a range of Curie temperatures [ Robbins et al , ]. Altered phases in nature commonly have Curie temperatures that range from 120 to 450°C [ Kądziałko‐Hofmokl et al , ]. Therefore, these particles are ideal for the inverse microconglomerate test because they should have been reset by the peak metamorphic temperatures experienced by the JH sediments.…”
We introduce a new paleomagnetic test, applicable to metamorphosed terrains, that assesses the recording fidelity of a metasediment. Magnetic mineral carriers with unblocking temperatures lower than the peak metamorphic temperature should record a common remagnetization direction, whereas those with higher unblocking temperatures should be randomly distributed if a primary magnetization has been preserved on a sedimentary grain scale. We call this an inverse microconglomerate test. Application to metasediments of the Jack Hills (JH), Western Australia, reveals that the chrome mica fuchsite records a well‐grouped secondary magnetization at unblocking temperatures between ∼270 and 340°C, in contrast to the random distribution of in situ directions held by zircons isolated at unblocking temperatures >550°C. This positive test further supports JH zircons as hosts of primary Hadean magnetizations. More generally, the new test can aid in understanding the timing of peak metamorphism and deformation in complex terrains.
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