Mole Hill (Virginia)

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View facing east from Mole Hill Road Mole Hill VA 1.jpg
View facing east from Mole Hill Road
View facing northwest from Swope Road Mole Hill VA 2.jpg
View facing northwest from Swope Road

Mole Hill is a rounded hill composed of basalt, a volcanic rock, formed during the Eocene epoch of the Paleogene period. It is the eroded remnant of what was an active volcano approximately 47 million years ago, making it one of the youngest volcanoes on the east coast of North America. It is located west of Harrisonburg, Virginia, in Rockingham County. [1]

Contents

Description

Mole Hill is an isolated, rounded, tree-covered monadnock in an otherwise relatively flat valley, surrounded by farmland. The peak of Mole Hill is approximately 1,893 feet (577 meters) above sea level. [2]

The basalt outcropping at the crest of the hill is "dark greenish gray to grayish black, medium grained, and moderately porphyritic. It is an olivine-spinel basalt with abundant large pale green pyroxene and minor yellow-brown olivine phenocrysts." [3] The basalt intrudes through the Ordovician Beekmantown Group of carbonate rocks.

Age

The basalt at Mole Hill (and other igneous dikes in the area) was originally thought to be of Paleozoic age by relative age dating using cross-cutting relationships. [1] In 1969, Fullagar and Bottino used K-Ar and Rb-Sr radiometric dating techniques to date rocks that they thought were temporally related to the Devonian Tioga Bentonite, but discovered that the rocks were actually a much younger age of approximately 47 million years, placing them in the Eocene. [4]

Trimble Knob, located in Highland County, is geologically similar to Mole Hill and thought to be contemporaneous with it, along with other intrusive igneous rocks near Ugly Mountain in Pendleton County, West Virginia. [1]

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Gabbro is a phaneritic (coarse-grained), mafic intrusive igneous rock formed from the slow cooling of magnesium-rich and iron-rich magma into a holocrystalline mass deep beneath the Earth's surface. Slow-cooling, coarse-grained gabbro is chemically equivalent to rapid-cooling, fine-grained basalt. Much of the Earth's oceanic crust is made of gabbro, formed at mid-ocean ridges. Gabbro is also found as plutons associated with continental volcanism. Due to its variant nature, the term gabbro may be applied loosely to a wide range of intrusive rocks, many of which are merely "gabbroic". By rough analogy, gabbro is to basalt as granite is to rhyolite.

<span class="mw-page-title-main">Mafic</span> Silicate mineral or igneous rock that is rich in magnesium and iron

A mafic mineral or rock is a silicate mineral or igneous rock rich in magnesium and iron. Most mafic minerals are dark in color, and common rock-forming mafic minerals include olivine, pyroxene, amphibole, and biotite. Common mafic rocks include basalt, diabase and gabbro. Mafic rocks often also contain calcium-rich varieties of plagioclase feldspar. Mafic materials can also be described as ferromagnesian.

<span class="mw-page-title-main">Basalt</span> Magnesium- and iron-rich extrusive igneous rock

Basalt is an aphanitic (fine-grained) extrusive igneous rock formed from the rapid cooling of low-viscosity lava rich in magnesium and iron exposed at or very near the surface of a rocky planet or moon. More than 90% of all volcanic rock on Earth is basalt. Rapid-cooling, fine-grained basalt is chemically equivalent to slow-cooling, coarse-grained gabbro. The eruption of basalt lava is observed by geologists at about 20 volcanoes per year. Basalt is also an important rock type on other planetary bodies in the Solar System. For example, the bulk of the plains of Venus, which cover ~80% of the surface, are basaltic; the lunar maria are plains of flood-basaltic lava flows; and basalt is a common rock on the surface of Mars.

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<span class="mw-page-title-main">Dunite</span> Ultramafic and ultrabasic rock from Earths mantle which is made of the mineral olivine

Dunite, also known as olivinite, is an intrusive igneous rock of ultramafic composition and with phaneritic (coarse-grained) texture. The mineral assemblage is greater than 90% olivine, with minor amounts of other minerals such as pyroxene, chromite, magnetite, and pyrope. Dunite is the olivine-rich endmember of the peridotite group of mantle-derived rocks.

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Nephelinite is a fine-grained or aphanitic igneous rock made up almost entirely of nepheline and clinopyroxene. If olivine is present, the rock may be classified as an olivine nephelinite. Nephelinite is dark in color and may resemble basalt in hand specimen. However, basalt consists mostly of clinopyroxene (augite) and calcic plagioclase.

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References

  1. 1 2 3 Jonathan L. Tso; Ronald R. McDowell; Katharine Lee Avary; David L. Matchen & Gerald P. Wilkes (2004). "Middle Eocene Igneous Rocks in the Valley and Ridge of Virginia and West Virginia". Circular 1264. United States Geological Survey.
  2. "Mole Hill Topo Map, Rockingham County VA (Bridgewater Area)". TopoZone. Retrieved 2018-06-11.
  3. Gathright, Thomas M; Frischmann, Peter S (1986). Geology of the Harrisonburg and Bridgewater quadrangles, Virginia. Commonwealth of Virginia, Dept. of Mines, Minerals, and Energy, Division of Mineral Resources. OCLC   758391284.
  4. Fullagar, Paul D.; Bottino, Michael L. (1969). "Tertiary Felsite Intrusions in the Valley and Ridge Province, Virginia". Geological Society of America Bulletin. 80 (9): 1853. doi:10.1130/0016-7606(1969)80[1853:TFIITV]2.0.CO;2.
38°26′55″N78°57′12″W / 38.44861°N 78.95333°W / 38.44861; -78.95333