Article

Vishnu Basement Rocks

Photo of inner Grand Canyon and the Colorado River.
The inner gorge of the Grand Canyon and the Colorado River.

NPS Photo by Michael Quinn.

Introduction

Rock Type

Metamorphic and igneous rocks with vertical folds and foliation

Environment

Originally in volcanic island chains that collided with ancestral North America to form the southwest United States; rocks were metamorphosed and invaded by magmas in the deep crust.

Age (Ma; mega annum = million years ago)

Paleo- and Mesoproterozoic Eras (Precambrian)
1375–1840 Ma

The Vishnu Basement Rocks contains all the ancient crystalline rocks at the bottom of the Grand Canyon. Vishnu Basement Rocks is an informal term but is useful because the formal stratigraphic nomenclature does not encompass all of Grand Canyon’s metamorphic units and all individual igneous plutons.

The terminology uses “Vishnu” because the public is familiar with the Vishnu Schist and “basement” to indicate the type of rock assemblage and its position. These rocks span from 1,840 to 1,375 Ma (Table 2), a duration of 465 million years. A nominal age of about one and three quarter billion years ago (1.75 Ga) focuses attention on the tectonic collisions that added this tract onto the North American continent and is a general number for the age of the Vishnu Basement Rocks.

Two illustrations showing earth's crust with tectonic plates and surface features.

Figure 26. Tectonic evolution of the continent during the formation of the Vishnu Basement Rocks. A) The volcanic and sedimentary precursors of the Granite Gorge Metamorphic Suite were deposited on the flanks of volcanic island chains, and the granodiorite plutons formed as magma chambers underneath the islands. B) Later granite and pegmatite intrusions formed as the volcanic islands were added to the Wyoming Province, part of the growing North American continent.

The basement rocks are divided into five informal groupings reflecting distinct time periods and tectonic histories (Table 2). Of these groupings, only the Granite Gorge Metamorphic Suite and the Zoroaster Plutonic Complex have been formally defined in the geologic literature.

Best numeric ages of the Vishnu Basement Rocks

Group

Formation

Stratigraphic Age

Numeric Age (Ma)

Precision (Ma)

Youngest granite

Quartermaster granite

Mesoproterozoic

1,375

± 2

Later granites / dike swarms

Phantom granite

Paleoproterozoic

1,662

± 1

Cremation pegmatite

Paleoproterozoic

1,698

± 1

Zoroaster Plutonic Complex

Horn Creek granite

Paleoproterozoic

1,713

± 2

Ruby gabbro

Paleoproterozoic

1,716

± 0.5

Trinity granite

Paleoproterozoic

1,730

± 93

Diamond Creek granite

Paleoproterozoic

1,736

± 1

Zoroaster granite

Paleoproterozoic

1,740

± 2

Granite Gorge Metamorphic Suite

Vishnu Schist

Paleoproterozoic

1,750

± 2

Brahma Schist

Paleoproterozoic

1,750

± 2

Rama Schist

Paleoproterozoic

1,751

± 2

Oldest basement

Elves Chasm pluton

Paleoproterozoic

1,840

± 1

Table 2.
Ma = mega annum = million years ago

Elves Chasm Pluton

Tectonic Environment

An older crustal pluton (magma chamber) in one of the microcontinents that gradually united to form North America

Age (Ma; mega annum = million years ago)

1,840 Ma

The Elves Chasm pluton (1,840 Ma) is the oldest basement identified in Grand Canyon. It is only exposed in the vicinity of Elves Chasm near River Mile 115. The age of this rock reflects its crystallization age from magma. Since it is an intrusive rock, it must have intruded older rocks, but these rocks have not yet been identified.

Granite Gorge Metamorphic Suite

Tectonic Environment

Volcanic and sedimentary rocks were deposited on the Elves Chasm pluton; they were metamorphosed as they were buried up to 12-mile (20-km) depths during the Yavapai orogeny. This event was similar to the collision of Italy with Europe to form the Alps. The Yavapai orogeny added new continental crust onto the then-southern margin of North America.

Age (Ma; mega annum = million years ago)

1,750–1,751 Ma

An unconformity of 90 million years separates the Elves Chasm pluton from the overlying Granite Gorge Metamorphic Suite, which consists of the 1,751 Ma Rama Schist and the 1,750 Ma Vishnu and Brahma schists. The Brahma and Rama schists originated as volcanic rocks, and the Vishnu Schist as sedimentary rocks. These rocks were deposited in volcanic island arcs that were later welded to the growing continent in the Yavapai orogeny approximately 1,700 Ma. They were metamorphosed during the mountain building event when the folds and vertical foliation that characterize these units was developed.

These rocks were intruded at great depths by two main types of magma: an early group of granodiorite plutons, and a later group of granite plutons and pegmatite dikes.

Numeric Ages of the Granite Gorge Metamorphic Suite

Formation

Stratigraphic Age

Numeric Age(Ma)

Precision(Ma)

Vishnu Schist

Paleoproterozoic

1,750

± 2

Brahma Schist

Paleoproterozoic

1,750

± 2

Rama Schist

Paleoproterozoic

1,751

± 2

Ma = mega annum = million years ago

Zoroaster Plutonic Complex

Tectonic Environment

Granodiorite magma chambers similar to modern ones under the Cascade volcanoes of the Pacific Northwest. The Zoroaster magmas formed during plate tectonic collisions during the Yavapai orogeny.

Age (Ma; mega annum = million years ago)

1,713–1,740 Ma

Most of the granodiorite intrusions in the Vishnu Basement Rocks are part of the Zoroaster Plutonic Complex. These plutons formed during the Yavapai orogeny and were likely related to the magma chambers that fed the volcanic arcs above subduction zones and range in age from 1,740 to 1,713 Ma.

Numeric Ages of the Zoroaster Plutonic Complex

Formation

Stratigraphic Age

Numeric Age (Ma)

Precision (Ma)

Horn Creek granite

Paleoproterozoic

1,713

± 2

Ruby gabbro

Paleoproterozoic

1,716

± 0.5

Trinity granite

Paleoproterozoic

1,730

± 93

Diamond Creek granite

Paleoproterozoic

1,736

± 1

Zoroaster granite

Paleoproterozoic

1,740

± 2

Ma = mega annum = million years ago

Later Granites and Dike Swarms

Tectonic Environment

The last crustal melts from the waning Yavapai orogeny

Age (Ma; mega annum = million years ago)

1,662–1,698 Ma

Later granites and dike swarms (Figure 27 and 28) formed more than 12 mile (20 km) below the surface due to crustal melting during the plate collisions that thickened and metamorphosed the crust during the Yavapai orogeny. These plutons and dikes can be differentiated from plutons in the Zoroaster Plutonic Complex by cross-cutting relationships and differences in composition. They are also slightly younger in age, ranging from 1,698–1,662 Ma.

Numeric Ages of the Later Granites and Dike Swarms

Formation

Stratigraphic Age

Numeric Age(Ma)

Precision(Ma)

Phantom granite

Paleoproterozoic

1,662

± 1

Cremation pegmatite

Paleoproterozoic

1,698

± 1

Ma = mega annum = million years ago

Photo of rock cliffs on a river bank.

Figure 27. Vishnu Basement Rocks include both metamorphic rocks of the Rama, Brahma, and Vishnu schists (dark in this photo) and granitic intrusions of several types and ages (lighter colors). This picture shows the Cremation pegmatite swarm near Phantom Ranch; one of these intrusions has been dated as 1,698 ± 1 million years old.
Photo by Laurie Crossey.

Photo of a rock outcrop with bands of dark and light minerals.

Figure 28. Granite intrusions of different sizes and compositions intruded the metavolcanic and metasedimentary rocks at great depths in the Vishnu mountains. This image shows granite from the later magmas filling a fracture network in the schist.
Photo by Laurie Crossey.

Youngest Granite

Tectonic Environment

Younger granites derived from crustal melting were widespread in the Southwest US, probably formed as other continental fragments collided with the growing North American continent far to the south of what is now the Grand Canyon region.

Age (Ma; mega annum = million years ago)

1,375 Ma

The Quartermaster pluton in the western Grand Canyon is substantially younger than the rest of the Vishnu Basement Rocks at 1,375 Ma. It is part of a belt of similar-age plutons that extends from southern California to Labrador that formed during a period of crustal melting due to later plate collisions.

Numeric Ages

The many reliable radiometric age determinations of the Vishnu Basement Rocks were obtained using the U-Pb method on the mineral zircon.

These radiometric age determinations are all highly precise, with analytical errors that are within ± 2 Ma, except for the 1,730 Ma Trinity Granite, which has an error of ± 93 Ma (Table 2). This imprecise age is due to mixed zircon populations in this granite that, with newer methods, could now be improved.

The dates we report for the Vishnu Basement Rocks have not been revised much in the past two decades. Additional research efforts are needed to further unravel their complex history. For example, the Vishnu Schist contains zircon grains whose ages were not reset during metamorphism, and can be used to determine the age of the sediment source. The oldest zircon grains are as old as 3.8 Ga, with many grains dated at about 2.4 and 1.8 Ga. A next step is to pinpoint the potential source regions outside Grand Canyon from which these grains were derived.

The igneous and metamorphic rocks of Vishnu Basement formed beneath the now-eroded Vishnu mountains. The erosional demise of those mountains to sea level was complete by the time the Grand Canyon Supergroup was deposited atop the Great Nonconformity erosion surface.

Learn More

Tiny image of the cover of a report titled Telling Time at Grand Canyon National Park.

To learn more about the age of Grand Canyon’s rocks, please see:

Karlstrom, K., L. Crossey, A. Mathis, and C. Bowman. 2021. Telling time at Grand Canyon National Park: 2020 update. Natural Resource Report NPS/GRCA/NRR—2021/2246. National Park Service, Fort Collins, Colorado. https://doi.org/10.36967/nrr-2285173. [IRMA Portal]

Photos and Illustrations

Part of a series of articles titled Telling Time at Grand Canyon National Park.

Grand Canyon National Park

Last updated: January 30, 2024