Los Pinos peridotite - full thin section

Click on image to enlarge.      Specimen: Michael Davis; Photo: Dan Snyder

Rounded, partially-resorbed olivine grains and interstitial pyroxene in peridotite of the  Los Pinos pluton, San Diego County, California. Macrophotograph in XPL. Imaged area 22mm by 42mm. See post of April 9, 2012 for description of rock body and higher-magnification photomicrographs.

Many thanks to Prof. Michael Davis, of the University of California at Riverside, for the specimen.

Montserate Mountain peridotite - full thin section.

Click on image to enlarge.          Sample: Michael Davis; Photo: Dan Snyder

Full thin section of igneous peridotite, Montserate Mountain, San Diego County, California. Macrophotograph in XPL. Imaged area 22mm by 38mm. See post of July 15, 2012 for detailed description of rock body and higher-magnification photomicrographs.

Many thanks to Prof. Michael Davis of the University of California at Riverside for the specimen. 

Cumulate olivine and interstitial pyroxene in igneous peridotite

Click on image to enlarge.          Specimen: Michael Davis          Photo: Dan Snyder

Olivine (left and right) with interstitial pyroxene (center). Note that opaque secondary mineral(s) occupying fractures in olivine do not extend through pyroxene. Montserate Mountain, San Diego County, California. XPL. Imaged area 1.3 mm x 2 mm.

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 Plane-polarized light image of same area shown above. Fractures appear to end at the olivine/pyroxene border. In the center of the image, the pyroxene is colored by parallel streaks of a red material, probably iddingsite, a late magmatic alteration product of olivine.

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Higher-magnification (10X objective) view of center of previous image. PPL.  Imaged area 0.54 mm by 0.8 mm.

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Higher-magnification (40X objective) view of center of previous image. PPL. Imaged area 0.13 mm by 0.2 mm.

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Optical Scan of remnants of hand specimen after removing material for billet for thin section. Imaged area 54 mm by 51 mm.

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Optical scan of outside of hand specimen minus billet material. Red material appears to be iddingsite. Imaged area 57 mm by 51 mm.



Many thanks to Prof. Michael Davis of the University of California at Riverside for the specimen.

Serpentinized Trinity peridotite

Click on image to enlarge.   Specimen: Michael Davis   Image: Dan Snyder

Optical scan of sawed surface of a small hand specimen of serpentinized Trinity peridotite. A 6-mm-thick slice of this specimen crumbled easily with the fingers, and thus the specimen was too fragile to use for a thin section. Olivine has largely been altered to yellowish-gray chrysotile serpentine, which also occupies some of the smaller fractures. Chrysotile has a waxy luster which, although not apparent in this image, shows up well on the hand specimen.  Dark linear features are earlier-formed fracture fillings of the antigorite or lizardite varieties of serpentine. Dark, rounded masses are relict or pseudomorphosed pyroxene. According to Quick (1981)*, the Trinity peridotite is highly serpentinized, except where glaciation has exposed large outcrops of relatively unserpentinized peridotite.  Eastern Klamath Mountains, northern California.  Imaged area 4.75 cm by 5.54 cm.

Excerpt from USGS Open File of02-490 s1

Hess (1989)* states the areal extent of the Trinity peridotite incorrectly as 3,700 sq. km. He cites Quick (1981) as the source. Quick, however does not give a figure for the areal extent of the peridotite outcrop. He states only that "Contiguous outcrops of ultramafic rocks occur over an area about 50 km wide and 75 km long." (Quick, 1981)**. It appears that Hess multiplied 50 by 75 and got 3,750, then dropped the 50 to avoid the impression of spurious accuracy. A glance at the map shows that this figure doesn't account for the various plutons lying within the contiguous area of peridotite, and that the actual areal extent of the peridotite itself is more like 1,500 sq. km.  I did a point count on graph paper, which resulted in an area of 1,237 sq. km.



* Hess, Paul C., 1989, Origins of Igneous Rocks, p. 80.

**Quick, James E., 1981. Petrology and petrogenesis of the Trinity Peridotite, an upper mantle diapir in the Eastern Klamath Mountains, northern California. Journal of Geophysical Research, v. 86, No. B12, p. 11,838.


Many thanks to Professor Michael Davis, of the University of California at Riverside, for the specimen.

The fibrous structure of chrysotile, the asbestiform variety of serpentine, can be seen clearly a thin chip of the mineral at 100x (10x objective) in a microscope. The dark strips at the top and bottom of the chip are remnants of the fracture wall to which it was anchored, and the dark horizontal strip in the center may be a cross-section of an antigorite vein occupying the center of the fracture. Plane polarized light. Length of chip ~0.5 mm.

Rounded olivine grains in peridotite of the Los Pinos pluton.

Click on image to enlarge.   Sample: Michael Davis   Image: Dan Snyder

   Rounded olivine grains surrounded by amphibole. The Los Pinos pluton is one of several gabbroic plutons intruding the Peninsular Ranges batholith in the southernmost part of California. "Olivine and amphibole...are the dominant phases and form up to 88% of the rock." (Walawender, 1976)*. Walawender describes the petrogenesis of the peridotite as an example of Bowen's classic reaction series. Olivine was first mineral to solidify from melt, along with minor plagioclase (not shown in this image). Outer parts of olivine grains were resorbed by melt as pyroxene (not shown) solidified. Amphibole solidfied last and occupied interstices between other minerals. Red material in large grain at center is iddingsite, occupying part of an irregular fracture.  Los Pinos Mountain, Peninsular ranges, San Diego County, California. XPL. Imaged area 2.7mm by 4mm.

See post of December 17, 2012 for a macrophotograph of the entire thin section.

Many thanks to Professor Michael Davis, of the University of California at Riverside, for the specimen.

Click on image to enlarge.   Sample: Michael Davis   Image: Dan Snyder

   PPL image of same area as above. Dark smudges in amphibole are made up of "aligned, rod-like, opaque minerals" (Walawender, 1976)*.


* Walawender, M. J, 1976. Petrology and Emplacement of the Los Pinos Pluton, southern California. Canadian Journal of Earth Sciences, v. 13, pp. 1288-1300.