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Barnard Regio

Ancient dark region on Ganymede, split by bright sulci.

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Barnard Regio

NASA/ JPL / USGS · Public domain

Barnard Regio is a dark, irregular patch on Ganymede, one of Jupiter’s moons. It is made up of several ancient, dark areas that are crossed by many younger, brighter grooves called sulci.

Barnard Regio 1
Barnard Regio 1. Image: NASA/ JPL / USGS · Public domain · Wikimedia Commons

The dark regions on Ganymede, known as regiones, are named by the International Astronomical Union after astronomers who helped discover Jupiter’s moons. Barnard Regio honors Edward Emerson Barnard, the American astronomer who found Amalthea—Jupiter’s fifth-largest moon, its largest minor moon, and the first Jovian moon discovered since Galileo spotted the four Galilean moons almost 300 years earlier. The IAU approved the name in 1979.

Barnard Regio geologic map
Barnard Regio geologic map. Image: NASA / JPL / USGS · Public domain · Wikimedia Commons

Location and geography

This region covers most of the equatorial area on the side of Ganymede that always faces Jupiter. Like all dark areas on the moon, Barnard Regio is thought to be among the oldest parts of the surface. It is rugged and covered with ancient dark material, likely accumulated from dark fragments brought by impacting asteroids and comets.

PIA02279 Barnard Regio
PIA02279 Barnard Regio. Image: NASA / JPL · Public domain · Wikimedia Commons

To the north, Phrygia Sulcus separates Barnard Regio from Perrine Regio. An unnamed narrow sulcus divides it from Nicholson Regio to the south. Dardanus Sulcus cuts through the southern half from north to south, splitting it in two. The more complex and chaotic Mysia Sulci run from the northeast to the southwest, breaking the region into many separate segments that look like islands.

A few craters lie inside and around Barnard Regio, but only a handful have names. Within the region, three craters are named: the bright ray crater Ishkur, and two fainter ones, Danel and Isimu. Craters without rays are generally older than those with rays. To the north sits the major ray crater Tros; to the west, the prominent dome crater Serapis; to the northwest, the bright crater chain Nanshe Catena; and to the east, the rayless crater Misharu and the dark-ray crater Kittu.

Barnard Regio lies within the Dardanus quadrangle (Jg6) and the Misharu quadrangle (Jg10) of Ganymede. A small part crosses into the Nabu quadrangle (Jg11) to the southwest. The region also contains the spot where Ganymede’s prime meridian—the line of 0° longitude that always points toward Jupiter because the moon rotates synchronously—meets its equator.

Relationship to other regiones

A 2020 study by Hirata, Suetsugu, and Ohtsuki suggests that Ganymede may have been hit by a huge impactor about 4 billion years ago.

Did You Know?

Frequently Asked Questions

What is Barnard Regio?

Barnard Regio is a dark, irregularly shaped terrain feature on the surface of Ganymede, one of Jupiter's four largest moons. It is composed of several ancient, dark patches that have been fractured and crossed by numerous younger, brighter grooves called sulci.

Which spacecraft have photographed Barnard Regio?

Imagery of the region has been returned by Voyager 1, Galileo, Cassini, New Horizons, and Juno. The IAU formally approved the name in 1979 under its convention of titling Ganymede's dark regiones after astronomers linked to the discovery of Jovian satellites.

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Sources

Compiled from Wikipedia and the sources listed below. Text from Wikipedia is available under CC BY-SA 4.0; this entry is adapted from it.

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