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Posts tagged with "earth’s interior"

Lithosphere and Tectosphere

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Lithosphere is a new journal from GSA. Its focus is the tectonic processes that affect Earth's crust and upper mantle. One of the papers in the first issue (of February 2009) is “A fluid factory in solid Earth”. The text contains terms like “slab graveyards”, “superplumes” and “hot spots” - at a time when many geologists still wonder whether these things really exist.

But first a few words about the tectosphere. I find the tectosphere a useful term, if everybody could just agree on what they understand by tectosphere. The term has been in use for at least 20 years. It was a.o. used by Jordan in 1978. Here are a few, different, definitions: The tectosphere is the portions of Earth's mantle lying below cratons. The tectosphere is the region of the earth's crust occupied by the tectonic plates. It is the continental roots. It is the continental keels. The tectosphere is the part of the crust and uppermost mantle, that moves laterally as a plate. Oceanic tectosphere is identical with Lithosphere, but Continental tectosphere is considerably thicker, 400 km, or even more. Apart from that some people may confuse it with the tectonosphere (The tectonosphere seems to include all outer layers of the Earth down to the level where there is a hydrostatic gravitational equilibrium and is about 120 km thick - but that again, of course, is arguable).

Anyway here is how the authors of the mentioned paper understand the term:

“The tectosphere, also referred to as continental “keels,” is considered to be essentially rigid and cold, representing a chemically distinct raft supporting the bulk of the continental crust (Jordan, 1988). The tectosphere appears to be confined to continental cratonic regions, formed before 2.0 Ga, the origins of which are controversial.“

A cartoon (fig 3) illustrates how the Earth’s interior is seen by some geologists - I would like to stress that some of the elements in the cartoon still are more or less controversial, while others are covered by a greater consensus.


MOR is an abbreviation for mid-ocean ridge, and MORB for mid-ocean-ridge basalt. The green line to the far right shows how an ocean plate is subducted along an oblique Benioff zone down to about 660 km, this zone can be detected by earthquakes. The deepest earthquakes practically never occur lower than 700 km. The lower mantle may be a “plate graveyard” (in the recycled MORB area in the cartoon). Although earthquakes cease below 660 km, plate descent may continue through the middle mantle (there is still some disagreement on this point). I have mentioned the D“ layer in several posts (a.o. here).

If we assume that the subducted slab material reach the core-mantle boundary, horizontal movements must take place at the base of the mantle, and these movements have been referred to as “anti–plate tectonics”. They are in many respects analogous to lithospheric plate tectonic processes operating in near-surface regions.

From here vertically rising “superplumes” enters into the upper mantle, transforms to horizontal, and branches out into several “hot spots”. These hot spots cause the rifting of the continent and deliver the mantle fluid to the surface.

I recommend the paper. The full text (pdf) is free!

Reference:
M. Santosh, S. Maruyama and S. Omori
A fluid factory in solid Earth
Lithosphere 2009;1;29-33
doi:10.1130/L2.1

http://lithosphere.gsapubs.org/cgi/content/abstract/1/1/29
http://lithosphere.gsapubs.org/current.dtl





The Tails of Two Plumes

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Hans Christian Andersen once wrote a fairy tale about a little feather that grew into five hens (It's Quite True!). Mantle plumes may sound as another fairy tale - but is it?

The concept of mantle plumes was advanced in the 1970s to explain intra-plate or hot spot volcanism erupting far from any plate boundary. The concept is still being heavily discussed. Do mantle plumes exist? Where and how do they form? Are all, none, or some hotspot volcanoes associated with mantle plumes? What do they look like, anyway?

First a very brief description of the concept. Mantle plumes are plume-like upwelling currents of hot material from the core-mantle boundary (the D“ layer) - or maybe higher up from the junction of the upper and lower mantle - that finally erupts as hotspot volcanoes or flood basalts.

And what do they look like? One idea is a cavity plume with a large spherical head and a thin trailing tail. Another idea is a diapir plume with a thick tail.

The conditions required for the formation of these two types of plumes are different, and it may seem unlikely that both could coexist in a chemically more or less homogeneous mantle. But on the other hand maybe not so if they are formed in the layer just above the core-mantle boundary, also known as the D” layer (pronounced "dee double prime"). In recent years a better understanding of this layer is accumulating. The core-mantle boundary region is chemically heterogeneous, particularly where mantle plumes are thought to originate. The thickness of the layer also varies a lot from place to place - probably from 0 and 300 km thick.

According to a study just published in the GSA journal Geology (with FREE access!) under the title Tails of two plume types in one mantle the variable thickness of this layer at the base of the mantle can lead to the coexistence of the two mentioned distinct plume types.

The form of mantle plumes is governed by viscosity. A locally thick chemical layer leads to small viscosity variation instabilities and hence to diapir plumes. The diapir plume is characterised by a cylindrical stem with a diameter twice the thickness of the thermal boundary layer capped by a head only slightly larger in radius than the stem. A locally thin chemical layer allows for large viscosity variations across the active portion of the lower mantle thermal boundary layer and, hence, for cavity plume formation. The thin tail reflects the thickness of the lowest viscosity active part of the thermal boundary layer (i.e. the velocity boundary layer), which feeds the upwelling plume.

The authors expect weak hotspots (such as the Azores) to be associated with diapir plumes and strong hotspots (such as the Hawaii) to be associated with cavity plumes.

Reference:
Lenardic and Jellinek:
Tails of two plume types in one mantle
Geology 2009;37;127-130
doi:10.1130/G25229A.1

http://geology.gsapubs.org/cgi/content/abstract/37/2/127?rss=1


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Core-Mantle Boundary

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Can slabs of oceanic crust descend as deep as to the core-mantle boundary? Is cold mid-ocean-ridge basalt dense enough to sink so deep into the mantle?

Do mantle plumes exist? And if so, can they well up from as deep as the core-mantle boundary?

These and other core-mantle boundary related questions are occupying many earth scientists. They just want to know.

Most of our earlier knowledge of the Earth's interior came from studying seismic waves (after earthquakes). It became clear that the boundary between the core and the mantle was something special. S-waves (secondary wave or shear wave) stopped. They cannot propagate through liquids. Seismic velocity is linked to the density of the medium through which the waves travel. P-wave (primary wave) velocity in general increases with increasing density - In liquids, however, the speed will be less. The core is much denser than the mantle.

When it was discovered that a thin layer directly above the core-mantle boundary had some mysterious properties it had to get a name consistent with the naming of the earth’s layers in the middle of last century. It is now still referred to as the D" ("D double-prime" or "D prime prime"). The D" name originates from the mathematician Keith Bullen's designations for the Earth's layers. His system was to label each layer alphabetically, A through G, with the crust as 'A' and the inner core as 'G'. In his 1942 publication of his model, the entire lower mantle was the D layer. In 1950, Bullen found his "D" layer to actually be two different layers. The upper part of the D layer, about 1800 km thick, was renamed D’ (D prime) and the lower part (the bottom 200 km) was named D" (pronounced "dee double prime"). A layer that produces strange seismic properties.

Research into the mysteries of the D“ layer has advanced spectacularly since 2004, when Japanese researchers found that high temperatures and pressures like those existing in the D” layer transform perovskite, the major mineral in Earth's mantle. The publication in the journal Science of Post-Perovskite Phase Transition in MgSiO3 is seen as a turning point. Since then many papers on this topic have followed. The latest I have seen is Radiative conductivity in the Earth's lower mantle by Goncharov et al. in today’s (13 November 2008) issue of Nature.

The discovery of post-perovskovite has profound implications for the chemical, thermal, and dynamical structure of the lowermost mantle (the D” region). Several major seismological characteristics of the D” region can now be explained by the presence of post-perovskite, and the specific properties of the phase transition provide the first direct constraints on absolute temperature and temperature gradients in the lowermost mantle. A discussion of the current understanding of the core–mantle boundary region can be found in Discovery of Post-Perovskite and New Views on the Core–Mantle Boundary Region by Kei Hirose and Thorne Lay in Elements of June 2008 (DOI: 10.2113/GSELEMENTS.4.3.183 - start downloading of the full article as large pdf-file by clicking here).

The Mg2+ site in post-perovskite is smaller than in perovskite, resulting in a volume reduction of 1.0–1.5%. Unlike perovskite, the post-perovskite phase has a layered structure of the SiO6 octahedra, which may lead to a large contrast in some properties with perovskite.


Scenario for the D” region. The D” seismic discontinuity is caused by the perovskite (Pv) to post-perovskite (PPv) phase transition. Post-perovskite may transform back to perovskite in the bottom thermal boundary layer with a steep temperature gradient. The large low-shear-velocity provinces (LLSVP) underneath upwellings (forming plumes) possibly represent large accumulations of dense MORB-enriched materials. The solid residue formed by partial melting in the ultralow-velocity zone (ULVZ - thin reddish zone on image) might also be involved in upwelling plumes. Such thin (20-40 km) ULVZ-layers are mainly (but not only) found under the Pacific Ocean and under Africa.

http://www.eurekalert.org/pub_releases/2008-11/ci-eht111008.php
http://www.cems.umn.edu/research/wentzcovitch/highlights/science_now_040324.htm
http://olivine.ethz.ch/~artem/NewMinerals.html
http://www.ucsc.edu/news_events/press_releases/text.asp?pid=978
http://www.nature.com/ngeo/journal/v1/n1/full/ngeo.2007.44.html (full paper in HTML)

For my (increasing number of) Scandinavian readers there is review in Norwegian at Geoportalen - http://www.geoportalen.no/planetenjorden/jordensindre/revolusjon/ . The article here by Reidar G. Trønnes, Natural History Museum, Universitty of Oslo, on the Earth’s Interior is somewhat easier to consume, and is well illustrated.

Maybe I ought to add that some of the topics discussed in the (review) papers are still controversial.




Iron in Earth's Inner Core

First a few words about iron crystals.

In contrast to most metals, which come in only one crystalline form, iron (Fe) can have two standard forms:

• Body centred cubic (bcc) iron, also called alpha iron or the ferritic phase, and
• Face centred cubic (fcc) iron, also called gamma iron or the austenitic phase.

Both structures are built from cubes with atoms at each corner. The bcc crystal structure has Fe atoms also at the centre of each cube, whereas the fcc structure has additional atoms in the sides of each cube.

At ambient conditions, pure iron is body-centred cubic (bcc). Above approximately 920°C, it becomes face centred cubic (fcc). At higher pressures the atoms may get even closer packed together into a crystal form of iron known as hexagonal close-packed (hcp), in which the atoms are arranged in planes like racked pool balls, each atom touching six others, and the planes of hexagons are stacked up, with alternating planes slightly offset, to give the three-dimensional structure.

At high temperature, an iron atom in the hcp structure is surrounded by 12 identical neighbours. An iron atom in the bcc structure is surrounded by eight atoms at a distance slightly shorter than that in the hcp structure and by six atoms located at a slightly larger distance compared to the nearest neighbour separation in the hcp structure.

And now to Earth’s inner core.

The Earth's inner core - a spherical body in the centre of Earth with a radius of about 1200 km - is a solid ball mainly of iron, but maybe with a bit of nickel as well. It has even been suggested (some ten years ago) that Earth's inner core may be a single crystal of (hcp-)iron.

Seismic observations have shown that elastic waves pass more rapidly through this core in directions that are parallel to the earth’s axis of rotation than in directions parallel to the equator. In the single crystal theory this is explained by a single hcp iron crystal, because hexagonal crystals have a unique directionality.

In 2003, however, Swedish researchers published strong theoretical proof that the earth’s core assumes the body centred cubic (bcc) crystal structure, a structure that despite its high degree of symmetry evinces a surprisingly high level of elastic anisotropy, that is, its elastic properties are contingent on direction. This theory about the crystal structure directly contradicted the then prevailing view, but since then the theory has found both experimental and theoretical support. The body-centred cubic crystal structure forms a cube with atoms in each corner and a further atom in the middle of this cube. It is oriented in such a way that its great diagonal is directed along the earth’s axis of rotation, which makes it possible for the iron to evince wave propagations with the velocities observed (seismic waves propagate by 3 to 4% faster in the direction of Earth’s spin axis than in the direction aligned with the equatorial plane).

In a new study published in Science of 8 February 2008 the same Swedish researchers present further evidence and an explanation based on computer simulations.

Why is the crystal structure important? Well, the earth’s heat balance, like its magnetic field, is dependent on the amount of heat that is stored in the inner core of the earth. These conditions, in turn, are dependent on the crystal structure of the iron in the inner core.

Another matter is that it recently was suggested that the inner core consists of two parts. The central part seems to react differently from the rest of the core on seismic waves. Such a different behaviour could maybe be explained in terms of two iron phases, one of which (bcc) is anisotropic and the other (hcp) isotropic.

Reference:
Article: Anatoly B. Belonoshko, Natalia V. Skorodumova, Anders Rosengren, Börje Johansson, Elastic Anisotropy of Earth's Inner Core, Science 8 February 2008: Vol. 319. no. 5864, pp. 797 - 800 DOI: 10.1126/science.1150302

http://www.sciencemag.org/cgi/content/short/319/5864/797
http://www.physorg.com/news121692398.html
http://www.scientificblogging.com/news_releases/magnetic_mystery_at_the_earths_core
http://www.nature.com/nature/journal/v424/n6952/abs/nature01954.html



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