Victoria Rupes

Last updated
Victoria Rupes
Victoria Rupes EN1007706026M.jpg
Oblique MESSENGER NAC image
Feature typeRupes
Coordinates 50°54′N31°06′W / 50.9°N 31.1°W / 50.9; -31.1
Eponym Victoria , a ship used on Ferdinand Magellan's expedition

Victoria Rupes is an escarpment in the Victoria quadrangle of Mercury. The quadrangle was named after this escarpment, and the escarpment itself was named after the Victoria , a ship used on the famous expedition of Ferdinand Magellan. Its name was adopted by the International Astronomical Union (IAU) in 1976. [1]

The escarpment cuts across Enheduanna crater at its southern end and across an unnamed crater near its center.

Victoria Rupes trends north-south across the center of this MESSENGER image. Sor Juana crater is in the background. Victoria Rupes and Sor Juana crater EW0236531373G.jpg
Victoria Rupes trends north-south across the center of this MESSENGER image. Sor Juana crater is in the background.

Related Research Articles

<span class="mw-page-title-main">Cauchy (crater)</span> Crater on the Moon

Cauchy is a small lunar impact crater on the eastern Mare Tranquillitatis. It was named after French mathematician Augustin-Louis Cauchy. It is circular and symmetric, with a small interior floor at the midpoint of the sloping inner walls. Due to the high albedo of this bowl-shaped formation, it is particularly prominent at full Moon.

<span class="mw-page-title-main">Discovery Rupes</span> Long cliff on Mercury

Discovery Rupes is an escarpment on Mercury approximately 650 kilometers (400 mi) long and 2 kilometres (6,562 ft) high, located at latitude 56.3 S and longitude 38.3 W. It was formed by a thrust fault, thought to have occurred due to the shrinkage of the planet's core as it cooled over time. The scarp cuts through Rameau crater. It was discovered by Mariner 10.

<span class="mw-page-title-main">Rupes Cauchy</span>

Rupes Cauchy is a 120 km-long escarpment at 9.0°N 37.0°E on the surface of the Moon. It faces southwest, and rises about 200–300 m. It is located in the northeastern portion of the Mare Tranquillitatis, and is named after the nearby crater Cauchy.

<span class="mw-page-title-main">Antoniadi Dorsum</span>

Antoniadi Dorsum is a ridge on Mercury at 25.1°N 30.5°W, and it is approximately 359 km in length. In 1976, it was named by the International Astronomical Union after Eugène Michel Antoniadi.

<span class="mw-page-title-main">Beethoven (crater)</span> Crater on Mercury

Beethoven is a crater at latitude 20°S, longitude 124°W on Mercury. It is 630 km in diameter and was named after Ludwig van Beethoven. It is the eleventh largest named impact crater in the Solar System and the third largest on Mercury.

<span class="mw-page-title-main">Eminescu quadrangle</span> Quadrangle on Mercury

The Eminescu quadrangle (H-9) is one of fifteen quadrangles on Mercury. It runs from 216 to 288° longitude and from -25 to 25° latitude. Named after the Eminescu crater, it was mapped in detail for the first time after MESSENGER entered orbit around Mercury in 2011. It had not been mapped prior to that point because it was one of the six quadrangles that was not illuminated when Mariner 10 made its flybys in 1974 and 1975. These six quadrangles continued to be known by their albedo feature names, with this one known as the Solitudo Criophori quadrangle.

<span class="mw-page-title-main">Discovery quadrangle</span> Quadrangle on Mercury

The Discovery quadrangle lies within the heavily cratered part of Mercury in a region roughly antipodal to the 1550-km-wide Caloris Basin. Like the rest of the heavily cratered part of the planet, the quadrangle contains a spectrum of craters and basins ranging in size from those at the limit of resolution of the best photographs to those as much as 350 km across, and ranging in degree of freshness from pristine to severely degraded. Interspersed with the craters and basins both in space and time are plains deposits that are probably of several different origins. Because of its small size and very early segregation into core and crust, Mercury has seemingly been a dead planet for a long time—possibly longer than the Moon. Its geologic history, therefore, records with considerable clarity some of the earliest and most violent events that took place in the inner Solar System.

<span class="mw-page-title-main">Beagle Rupes</span> Rupes on Mercury

Beagle Rupes is an escarpment on Mercury, one of the highest and longest yet seen. It was discovered in 2008 when MESSENGER made its first flyby of the planet. It has an arcuate shape and is about 600 km long. The scarp is a surface manifestation of a thrust fault, which formed when the planet contracted as its interior cooled.

<span class="mw-page-title-main">Claritas Rupes</span> Geologic feature of Mars

Claritas Rupes is a scarp in the Phoenicis Lacus quadrangle of Mars, located at 26° South and 105.4° West. It is 924 km long and was named after an albedo feature at 25S, 110W. The term "Rupes" is used in planetary geology to refer to an escarpments or cliff on Mars and other planets. It is the Latin word for cliff.

<span class="mw-page-title-main">Leopardi (crater)</span> Crater on Mercury

Leopardi is a crater on Mercury. Its name was adopted by the International Astronomical Union in 1976. Leopardi is named for the Italian writer Giacomo Leopardi, who lived from 1798 to 1837.

<span class="mw-page-title-main">Belgica Rupes</span>

Belgica Rupes is an escarpment in the Debussy quadrangle of Mercury. The escarpment is approximately 425 km long and cuts across the crater Carleton. It was named after the RV Belgica, a Belgian ship used for an expedition to determine the position of the South Magnetic Pole in 1898, and the first ship to winter in Antarctica. Its name was adopted by the International Astronomical Union (IAU) in 2013.

<span class="mw-page-title-main">Vostok Rupes</span> Escarpment on Mercury

Vostok Rupes is an escarpment on Mercury. The scarp is a surface manifestation of a thrust fault, which formed when the planet contracted as its interior cooled.

<span class="mw-page-title-main">Villa-Lobos (crater)</span> Crater on Mercury

Villa-Lobos is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) on September 25, 2015. Villa-Lobos is named for the Brazilian composer Heitor Villa-Lobos.

<span class="mw-page-title-main">Seuss (crater)</span> Crater on Mercury

Seuss is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 2012. It is named for the American author and cartoonist Theodor Seuss Geisel, better known as Dr. Seuss.

The Rupes Toscanelli is an escarpment located on the Moon. The cliff is named after the nearby Toscanelli crater, which in turn was named after the Italian mathematician and astronomer Paolo dal Pozzo Toscanelli.

The Rupes Mercator is an escarpment located on the Moon. It is named after the neighboring Mercator crater, a name assigned to it in 1935 by the International Astronomical Union in honor of the Flemish geographer and mathematician Gérard Mercator.

The Rupes Liebig is an escarpment located on the Moon. The cliff is named after the nearby Liebig crater, which in turn was named after the German chemist Justus von Liebig (1803–1873).

References

  1. "Victoria Rupes". Gazetteer of Planetary Nomenclature. NASA . Retrieved 26 July 2020.