BN: rocks
Showing posts with label rocks. Show all posts
Showing posts with label rocks. Show all posts

8 Jun 2020

The Basis of Rock Classification

Beginning in the 18th century, geologists struggled to develop a sensible way to classify rocks, for they realized, as did miners from centuries past, that not all rocks are the same. Classification schemes help us organize information and remember significant details about materials or objects, and they help us recognize similarities and differences among them. By the end of the 18th century, most geologists had accepted the genetic scheme for classifying rocks that we continue to use today. This scheme focuses on the origin (genesis) of rocks. Using this approach, geologists recognize three basic groups: (1) igneous rocks, which form by the freezing (solidification) of molten rock (figure above a); (2) sedimentary rocks, which form either by the cementing together of fragments (grains) broken off preexisting rocks or by the precipitation of mineral crystals out of water solutions at or near the Earth’s surface (figure above b); and (3) metamorphic rocks, which form when pre-existing rocks change character in response to a change in pressure and temperature conditions (figure above c). Metamorphic change occurs in the solid state, which means that it does not require melting. In the context of modern plate tectonics theory, different rock types form in different geologic settings (figure below).

A cross section illustrating various geologic settings in which rocks form.

Each of the three groups contains many different individual rock types, distinguished from one another by physical characteristics.

Describing grains in rock.

  • Grain size: The dimensions of individual “grains” (here used in a general sense to mean fragments or crystals) in a rock may be measured in millimetres or centimetres. Some grains are so small that they can’t be seen without a microscope, whereas others are as big as a fist or larger. Some grains are equant, meaning that they have the same dimensions in all directions; some are inequant, meaning that the dimensions are not the same in all directions (figure above a, b). In some rocks, all the grains are the same size, whereas other rocks contain a variety of grain sizes.
  • Composition: A rock is a mass of chemicals. The term rock composition refers to the proportions of different chemicals making up the rock. The proportion of chemicals, in turn, affects the proportion of different minerals  constituting the rock.
  •  Texture: This term refers to the arrangement of grains in a rock, that is, the way grains connect to one another and whether or not inequant grains are aligned parallel to each other.
  •  Layering: Some rock bodies appear to contain distinct layering, defined either by bands of different compositions or textures, or by the alignment of inequant grains so that they trend parallel to each other. Different types of  layering occur in different kinds of rocks. For example, the layering in sedimentary rocks is called bedding, whereas the layering in metamorphic rocks is called metamorphic foliation (figure below a, b).

Each distinct rock type has a name. Names come from a variety of sources. Some come from the dominant component making up the rock, some from the region where the rock was first discovered or is particularly abundant, some from a root word of Latin origin, and some from a traditional name used by people in an area where the rock is found.

Credits: Stephen Marshak (Essentials of Geology)

Studying Rock

The study of rocks begins by examining a rock in an outcrop. If the outcrop is big enough, such an examination will reveal relationships between the rock you’re interested in and the rocks around it, and will allow you to detect layering. Geologists carefully record observations about an outcrop, then break off a hand specimen, a fist-sized piece, that they can examine more closely with a hand lens (magnifying glass). Observation with a hand lens enables geologists to identify sand-sized or larger grains, and may enable them to describe the texture of the rock.

Geologists often must examine rock composition and texture in minute detail in order to identify a rock and develop a hypothesis for how it formed. To do this, they take a specimen back to the lab, make a very thin slice (about 0.03 mm thick, the thickness of a human hair) and mount it on a glass slide (figure above a–c). They study the resulting thin section with a petrographic microscope (petro comes from the Greek word for rock). A petrographic microscope differs from an ordinary microscope in that it illuminates the thin section with  transmitted polarized light. This means that the illuminating light beam first passes through a special polarity filter that makes all the light waves in the beam vibrate in the same plane, and then the light passes up through the thin section and then up through another polarizing filter. An observer looks through the thin section as if it were a window. When illuminated with transmitted polarized light, and viewed through two polarizing filters, each type of mineral grain displays a unique suite of colours (figure above d). The specific colour the observer sees depends on both the identity of the grain and its orientation with respect to the waves of polarized light.

The brilliant colours and strange shapes in a thin section viewed in polarized light rival the beauty of an abstract painting or stained glass. By examining a thin section with a petrographic microscope, geologists can identify most of the minerals constituting the rock and can describe the way in which the grains connect to each other. They can make a record of the image by using a camera. A photograph taken through a petrographic microscope is called a photomicrograph.

High-Tech Analytical Equipment

An electron micro-probe uses a beam of electrons to analyse the chemical composition of minerals.

Beginning in the 1950s, high-tech electronic instruments became available that enabled geologists to examine rocks on an even finer scale than is possible with a petrographic microscope. Modern research laboratories typically boast instruments such as electron micro-probes, which can focus a beam of electrons on a small part of a grain to create a signal that defines the  chemical  composition of the mineral (figure above); mass spectrometers, which analyse the proportions of atoms with different atomic weights contained in a rock; and X-ray diffractometers, which identify minerals by measuring how X-ray beams interact with crystals. Such instruments, in conjunction with optical examination, can provide geologists with highly detailed  characterizations of rocks, which in turn help them understand how the rocks formed and where the rocks came from. This information enables geologists to use the study of rocks as a basis for deciphering Earth history.

Credits: Stephen Marshak (Essentials of Geology)

13 May 2020

Igneous Origin of Diamonds

Diamondsare a rare occurrence on the surface of the planet because it takes extremely hot and high pressure conditions to create them. Physical and chemical conditions where diamonds form only exist in the mantle, nearly 70 miles down or more. In that environment in the upper mantle, diamonds may be a common mineral! It takes incredible events, nothing that has ever been witnessed in historic times, to bring diamonds to the surface.

Kimberlite-Diamond-mantle-rock

Diamond deposits around the world (that have any economic significance) are associated with volcanic features calleddiatremes. A diatreme is a long, vertical pipe formed when gas-filled magma forces its way through the crust to explosively erupt at the surface.Kimberlite a special kind of intrusive igneous rock associated with some diatremes that sometimes contain diamonds, typical coarse grained an bluish in color.

Diamond-bearing kimberlite pipes are diatremes that originate in the mantle.
Diamonds are xenoliths carried up from deep sources in the mantle, and often occur in association with other gem minerals including garnet, spinel and diopside. Most "economically significant" diamond deposits occur in ancient rocks (Precambrian age), but have been discovered on all continents. Because diamonds are so hard, they survive torturously-long histories, recycled through sedimentary and metamorphic environments without being destroyed. As a result they have been found almost everywhere as very rare, isolated discoveries. Diamonds of microscopic size have been discovered in meteorites and asteroid impact sites, and some metamorphic rocks. They are most extensively mined from kimberlite pipes or from alluvial gravels derived downstream from diamond source areas. It should be noted that most diamonds are not of gem quality, but those that are not are used for industrial purposes.

Credits to Phil Stoffer at geologycafe.Com

Text and figures are used with permission.

12 May 2020

Siccar Point - the world's most important geological site and the birthplace of modern geology

Siccar Point is world-famous as the most important unconformity described by James Hutton (1726-1797) in support of his world-changing ideas on the origin and age of the Earth.

James Hutton unconformity with annotations - Siccar Point

In 1788, James Hutton first discovered Siccar Point, and understood its significance. It is by far the most spectacular of several unconformities that he discovered in Scotland, and very important in helping Hutton to explain his ideas about the processes of the Earth.At Siccar Point, gently sloping strata of 370-million-year-oldFamennian LateDevonianOld RedSandstone and a basal layer of conglomerate overlie near vertical layers of 435-million-year-old lowerSilurianLlandovery Epoch greywacke, with an interval of around 65 million years.

Standing on the angular unconformity at Siccar Point (click to enlarge). Photo: Chris Rowan, 2009
As above, with annotations. Photo: Chris Rowan, 2009

Hutton used Siccar Point to demonstrate the cycle of deposition, folding, erosion and further deposition that the unconformity represents. He understood the implication of unconformities in the evidence that they provided for the enormity of geological time and the antiquity of planet Earth, in contrast to the biblical teaching of the creation of the Earth.

How the unconformity at Siccar Point formed.

At this range, it is easy to spot that the contact between the two units is sharp, but it is not completely flat. Furthermore, the lowest part of the overlying Old Red Sandstone contains fragments of rock that are considerably larger than sand; some are at least as large as your fist, and many of the fragments in this basal conglomerate are bits of the underlying Silurian greywacke. These are all signs that the greywackes were exposed at the surface, being eroded, for a considerable period of time before the Old Red Sandstone was laid down on top of them.

The irregular topography and basal conglomerate show that this is an erosional contact. Photo: Chris Rowan, 2009

The Siccar Point which is a rocky promontory in the county of Berwickshire on the east coast of Scotland.

8 May 2020

30+ Thin Section Photos That Will Develop Your Interest in Petrography

The art of getting ready thin sections has been critical to expertise the core samples that scientists are observing. Thin segment samples permit scientists to look at minerals in rocks, their crystal shape and texture at a microscopic stage.

Want to revise how do geologists examine rock? Follow this hyperlink to see our blog on "Studying Rock".

In this blog, we're taking you into the adventure of thin phase snap shots that were captured and given by means of college students and younger professionals from Finland, Ireland, Denmark, Czech Republic and Plymouth (UK).

Again our purpose is to encourage students and professionals' research by promoting "learning and scope" of Geology through our blogs. Help us to help others in learning and understanding geology. See this link that how you can contribute to Learning Geology.

Note: We are using following thin section photos by having permission from their owners. If you like to use these photos, leave us a message or email ushere.

1. A beautiful heart shaped hornblende in XPL (cross polarized light) view.It is a thin section ofbasalt with some secondary mineralization in the vesicles. Plagioclase is present in the form of black and white matrix and large phenocryst (with some zoning). Alignment of plagioclase grains is indicative of the "flow" of magma.

Photo Credits: Astaley

2. Thin Section of a Biotite and Muscovite, XPL view

Photo Courtesy: Laura

3. Thin Section of a Plagioclase (orthoclase) and Pyroxene, XPL

Photo Courtesy: Laura

4. Eclogite in Thin Section, XPL

Photo Courtesy: Laura

5. Cummulate Rock with Pyroxene and plagioclase, XPL

Photo Courtesy: Laura

6. Blueschist, XPL

Photo Courtesy: Laura

7. Agglomerate in a Thin Section, XPL view

       Agglomeratesare pyroclastic igneous rocks that consist almost wholly of angular or rounded lava fragments of varying size and shape. Fragments are usually poorly sorted in a tuffaceous matrix, or appear in lithified volcanic ash. (Britannica.com)

Photo Courtesy: Laura
8. Thin Section of a Pigeonite and Olivine, XPL

Photo Courtesy: Laura

nine. Olivine phenocryst in Basaltic Lapilli, XPL

Photo Courtesy: Laura

10. Thin Section of a Gabbro, XPL

Showing minerals; Pyroxene and Olivine, plagioclase and others. Learn more about Gabbrohere.

Photo Courtesy: Laura

 11. Another beautiful skinny section of a Gabbro, XPL

Photo Courtesy: Laura
12. Thin Section of a Greenschist, XPL

Photo Courtesy: Laura

thirteen. Thin Section showing intrusion of rocks from magma chamber into united states rocks, XPL

Photo Courtesy: Jack Lewis Donnelly

14. Thin Section of a Sillimanite - a mineral discovered in rocks formed with the aid of the metamorphism of a mudstone. (XPL view)

Photo Courtesy: Jack Lewis Donnelly
15. Microgeode in ultrabasic vulcanite (a rare copper telluride mineral), 30 µm thin section, PPL and XPL

Photo Courtesy: Petr Hyks
Photo Courtesy: Petr Hyks

See unique photohere

16. Muscovite & biotite (30 µm thin section, PPL and XPL)

Photo Courtesy:Petr Hyks

Photo Courtesy:Petr Hyks

Same photo in XPL view. See unique photohere

17. Quartz and epidote (30 µm thin section, PPL and XPL)

Photo Courtesy:Petr Hyks
Photo Courtesy:Petr Hyks

See originalhere.

18. Olivine (30 µm thin section, PPL and XPL)

Photo Courtesy: Petr Hyks

See this photohere on Petr Hyks' website

19. Zircons in biotite (30 µm thin section, PPL views, showing extinction)

                          Photo Courtesy:Petr Hyks

See this photo here on Petr's website

20. Zircon in biotite (30 µm thin section, XPL)

Photo Courtesy:Petr Hyks

See this photo here on Petr's website

21. Kyanite surrounded by muscovite (30 µm thin section, PPL and XPL)

Photo Courtesy: Petr Hyks

See these photos on Petr's pagehere and here

22. Zircon crystal in chloritized biotite (30 µm thin section, PPL and XPL)

Photo Courtesy:Petr Hyks

See these photos on Petr's pagehere and here Petr Hyks is 21 year old geology student from Masaryk University in Brno (Czech Republic). He has uploaded 5000+ photos about geology, astronomy and meteorology on his Flickr page. Follow this link to visit his website. Thank you Petr for contributing to Learning Geology and helping others to learn geology through your thin section photos. 🙂 Now following 10 thin section photos are from a geology student of University of Helsinki, Finland.

23. Thin Section of Olivine Diabase in XPL and PPL view.

Photo Courtesy: GeoAmethyst

24. Thin Section of Basalt in XPL view

        Having minerals: Olivine (in center) plagioclase, pyroxene and other accessory minerals

Photo Courtesy:GeoAmethyst

25. Thin Section of a Trachyte, XPL view

    Trachyte is an igneous volcanic rock with aphanitic to porphyritic texture. It is volcanic equivalent of Syenite. Major or essential minerals are alkali feldspar with less amount of plagioclase, quartz or feldspathiod.

Photo Courtesy:GeoAmethyst

26. Thin Section of a Harzburgite, XPL view

      Harzburgite is an ultramafic igneous rock. It chiefly contains plagioclase (under 10%) , olivine, orthopyroxene (enstatite), clinopyroxene (diopside) and biotite. There could be a small amount of talc, carbonate, tremolite, cummingtonite, chlorite, serpentine and titanite.

Photo Courtesy:GeoAmethyst

27.  Another thin section of Harzburgite, XPL view

Photo Courtesy:GeoAmethyst

28.  Thin Section of Pyroxenite (an ultramafic igneous rock), XPL view

Photo Courtesy:GeoAmethyst

29. Thin Section of Trachyte showing Sandine mineral in center, XPL view

Photo Courtesy:GeoAmethyst
30.  Thin Section of Andesite, XPL view

       It is an extrusive igneous, of intermediate composition, with aphanitic to porphyritic texture.              Here this thin section is showing chiefly hornblende and plagioclase.

Photo Courtesy:GeoAmethyst

31. Thin Section of Alkali Basalt (silica undersaturated) in XPL view.

Photo Courtesy:GeoAmethyst

32. Thin Section showing small clinopyroxene grains within orthopyroxene

Photo Courtesy:GeoAmethyst

Like this article? Leave a comment down or send us your valuable suggestion or feedback here  to help us in improving this article.

Useful Websites:  1. Polarized light Microscopy (Image Gallery)

2.How to make a thin section

3. Petrographic thin section preparation

4. Guide to Thin Section Microscopy

5. Index of Minerals in Thin Section

6. Optical Petrography website by an Italian Geologist

7.Carbonate Thin Section Images and Exercises

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Anies Baswedan

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