UPSC MainsGEOLOGY-PAPER-II202020 Marks
Q10.

Critically discuss the petrogenesis of anorthosites. Comment on the tectonic significance on the distribution of anorthosites.

How to Approach

This question requires a detailed understanding of igneous petrology, specifically focusing on the origin and evolution of anorthosites. The answer should begin by defining anorthosites and outlining their mineralogical composition. Then, it should delve into the various petrogenetic models proposed for their formation, including magmatic, impact, and metamorphic origins. Finally, the answer must critically evaluate the tectonic settings associated with anorthosite occurrences, linking their distribution to plate boundaries and other geological features. A structured approach, covering formation mechanisms and tectonic significance separately, is recommended.

Model Answer

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Introduction

Anorthosites are intrusive igneous rocks composed almost entirely of plagioclase feldspar, typically labradorite or bytownite. These relatively rare rocks are of significant petrological interest due to their unusual composition and their implications for understanding the processes occurring in the Earth’s crust and mantle. Their occurrence is often linked to specific tectonic environments, providing insights into the evolution of continental crust. The study of anorthosites has been crucial in understanding the early differentiation of the lunar crust, as the lunar highlands are predominantly composed of anorthositic rocks. This answer will critically discuss the petrogenesis of anorthosites and comment on the tectonic significance of their distribution.

Petrogenesis of Anorthosites

The origin of anorthosites has been a long-standing debate in igneous petrology. Several models have been proposed, each attempting to explain the extreme plagioclase composition of these rocks. These models can be broadly categorized into magmatic, impact, and metamorphic origins.

1. Magmatic Models

Magmatic models are the most widely accepted explanations for anorthosite formation. These models propose that anorthosites form through various processes involving the differentiation of mantle-derived magmas.

  • Fractional Crystallization: This model suggests that anorthosites form as a result of extensive fractional crystallization of a basaltic magma. As the magma cools, plagioclase crystals preferentially crystallize and are removed from the melt, leading to a residual magma enriched in other elements. This process, repeated over time, can produce anorthositic compositions. However, this model struggles to explain the large volumes of anorthosites observed.
  • Accumulation of Plagioclase Crystals: This model proposes that anorthosites form through the accumulation of plagioclase crystals that have crystallized in a magma chamber. These crystals can settle to the bottom of the chamber due to their density, forming layers of anorthosite. This process is often associated with convection currents within the magma chamber.
  • Liquid Immiscibility: This model suggests that anorthosites form through the separation of a plagioclase-rich liquid from a more mafic magma. This immiscibility is thought to occur under specific conditions of temperature, pressure, and composition.
  • In-situ Crystallization: This model, gaining prominence, suggests that large anorthositic massifs form through the prolonged, in-situ crystallization of a large magma chamber within the lower crust. This allows for the accumulation of plagioclase without significant transport.

2. Impact Models

Impact models propose that anorthosites can form as a result of large meteorite impacts. The impact event generates intense heat and pressure, which can melt the target rocks and produce anorthositic melts.

  • Impact Melting: The impact of a large meteorite can melt a significant volume of crustal rocks, creating a melt sheet that can differentiate to form anorthosites. This model is supported by the presence of impact breccias and shocked minerals in some anorthosite occurrences.

3. Metamorphic Models

Metamorphic models suggest that anorthosites can form through the metamorphism of pre-existing rocks, such as gabbros or diorites. This metamorphism can lead to the recrystallization of plagioclase and the formation of anorthositic textures.

  • Anatexis: Partial melting of plagioclase-rich rocks under high-grade metamorphic conditions can produce anorthositic melts.

Tectonic Significance of Anorthosite Distribution

The distribution of anorthosites is not random; it is strongly correlated with specific tectonic settings. This correlation provides valuable insights into the geological processes that control their formation.

  • Archean Cratons: Many of the largest and most well-studied anorthosite massifs are found within Archean cratons, such as the Bushveld Complex in South Africa, the Stillwater Complex in Montana, USA, and the Nain Plutonic Suite in Labrador, Canada. These cratons represent stable continental interiors that have undergone prolonged periods of crustal evolution. The anorthosites are thought to have formed during periods of mantle plume activity and crustal thickening.
  • Proterozoic Orogenic Belts: Anorthosites are also found in Proterozoic orogenic belts, which are regions of intense deformation and magmatism. These anorthosites are often associated with continental collisions and subduction zones.
  • Rift Zones: Some anorthosites are found in rift zones, which are regions of continental extension. These anorthosites are thought to have formed as a result of decompression melting of the mantle.
  • Lunar Highlands: The lunar highlands are dominated by anorthosites, formed early in the Moon’s history through the crystallization of a global magma ocean. This provides a unique context for understanding anorthosite petrogenesis.
Tectonic Setting Anorthosite Examples Petrogenetic Model
Archean Cratons Bushveld Complex (South Africa), Stillwater Complex (USA) Fractional Crystallization, Accumulation
Proterozoic Orogenic Belts Grenville Province (North America) Magmatic Differentiation, Metamorphism
Rift Zones East African Rift Valley Decompression Melting
Lunar Highlands Various lunar craters and maria Crystallization from Magma Ocean

Conclusion

In conclusion, the petrogenesis of anorthosites is complex and likely involves a combination of magmatic, impact, and metamorphic processes. While magmatic models, particularly those involving fractional crystallization and accumulation, are currently favored, the specific mechanisms responsible for their formation likely vary depending on the tectonic setting. The distribution of anorthosites is strongly linked to Archean cratons, Proterozoic orogenic belts, and rift zones, highlighting their importance in understanding the evolution of the Earth’s crust and mantle. Further research, integrating geochemical, isotopic, and geochronological data, is needed to refine our understanding of these fascinating rocks.

Answer Length

This is a comprehensive model answer for learning purposes and may exceed the word limit. In the exam, always adhere to the prescribed word count.

Additional Resources

Key Definitions

Plagioclase Feldspar
A series of solid solution minerals ranging continuously between albite (NaAlSi3O8) and anorthite (CaAl2Si2O8). It is a major constituent of many igneous and metamorphic rocks.
Magma Ocean
A layer of molten rock beneath the surface of a planetary body, typically formed during the early stages of planetary formation or after a giant impact event.

Key Statistics

The Bushveld Complex in South Africa, one of the largest layered igneous intrusions in the world, contains an estimated 75% of the world’s known platinum group element (PGE) reserves, often associated with its anorthositic layers.

Source: US Geological Survey, Mineral Commodity Summaries 2023 (Knowledge Cutoff: 2023)

Approximately 83% of the lunar highlands are composed of anorthosite, indicating a significant early differentiation event.

Source: Taylor, S. R. (1975). Lunar science: A post-Apollo view. Pergamon Press. (Knowledge Cutoff: 1975)

Examples

The Nain Plutonic Suite, Canada

This suite represents one of the largest coherent anorthosite intrusions on Earth, covering an area of approximately 60,000 square kilometers. It provides a prime example of in-situ crystallization of anorthositic magma.

Frequently Asked Questions

What is the significance of anorthosites in lunar geology?

Anorthosites are the dominant rock type in the lunar highlands, suggesting that the early lunar crust was formed by the crystallization of a global magma ocean. Their study provides insights into the early evolution of the Moon.