Nabokov (crater)

Last updated
Nabokov
Nabokov crater MESSENGER WAC.jpg
MESSENGER WAC mosaic of Nabakov
Feature typePeak-ring impact basin
Location Derain quadrangle, Mercury
Coordinates 14°34′S55°46′E / 14.56°S 55.76°E / -14.56; 55.76
Diameter166 km (103 mi)
Eponym Vladimir Nabokov
Enhanced color image of Nabokov Nabokov crater MESSENGER WAC IGF to RGB.jpg
Enhanced color image of Nabokov

Nabokov is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) on April 24, 2012. Nabokov is named for the Russian and American author Vladimir Nabokov. [1]

Nabokov is one of 110 peak ring basins on Mercury. [2] To the west is another peak-ring basin, Holst, of similar size. To the north of Nabokov is Martins crater, and to the northeast is Barney. Nabokov lies on the east side of the ancient Lennon-Picasso Basin. About 137 km to the northeast of Barney is the highest point on Mercury (over 4 km above the global average), the highest part of scarps that are remnants of the rim of the Lennon-Picasso Basin.

Related Research Articles

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

Bach is a double-ringed impact basin within the Bach quadrangle of Mercury. It was named by the IAU in 1976.

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

Michelangelo is a 230 km diameter impact basin in the Michelangelo quadrangle of Mercury, which is named after this crater. The crater itself was named by the IAU in 1979 after the Italian painter, sculptor and architect Michelangelo.

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

Mozart is a crater on Mercury, named by the IAU in 1976 after Austrian composer Wolfgang Amadeus Mozart.

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

Homer is a crater on Mercury. It is one of 110 peak ring basins on Mercury. It is Tolstojan in age.

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

Polygnotus is a crater on Mercury, named by the IAU in 1976, after ancient Greek painter Polygnotus.

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

Praxiteles is a crater on Mercury. It is one of 110 peak ring basins on Mercury.

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

Moody is an impact crater on Mercury.

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

Munkácsy, named after Mihály Munkácsy, is a crater on Mercury. Munkácsy originally had a double-ring basin structure, but most of the inner ring was buried when the basin was flooded with volcanic lava. Only a few remnants of the ring poke up through the lava, although low ridges in the lava seem to trace out much of the rest of the ring's circumference. Munkácsy is one of 110 peak ring basins on Mercury.

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

Izquierdo is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 2009, for the Mexican painter María Izquierdo. The floor of Izquierdo is smooth, the result of having been partially filled with volcanic lava. Circular outlines of the rims of “ghost craters” – smaller, older craters that have been largely buried by the lavas that infilled the basin – are visible in a few places on Izquierdo's floor. The remnants of a buried inner ring are also barely discernible in spots, and it is one of 110 peak ring basins on Mercury. There have been more recent impacts into the floor of Izquierdo, resulting in some small, sharply defined craters.

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

Scarlatti is a pit-floored crater on Mercury, which was discovered in 1974 by the Mariner 10 spacecraft. It has a prominent peak ring, and it is one of 110 peak ring basins on Mercury. The crater floor is covered by the smooth plains material. The crater displays an arcuate collapse feature along the northeastern peak ring. The size of the pit, which was first noticed in MESSENGER images obtained in January 2008, is 38 × 12 km. Such a feature may have resulted from collapse of a magma chamber underlying the central peak ring complex of the crater. The collapse feature is an analog of Earth's volcanic calderas. Scarlatti is thought to have the same age as the Caloris basin.

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

Lange is a crater on Mercury. It was named by the IAU in 2009 after American photographer Dorothea Lange.

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

Ahmad Baba is a crater on Mercury. It has a diameter of 127 kilometers. Its name was adopted by the International Astronomical Union (IAU) in 1979.

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

Aksakov is a crater on Mercury. It has a diameter of 174 kilometers. Its name was adopted by the International Astronomical Union (IAU) on April 24, 2012. Aksakov is named for the Russian author Sergey Aksakov, who lived from 1791 to 1859 C.E.

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

Ma Chih-Yuan is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Ma Chih-Yuan is named for the Chinese playwright Ma Zhiyuan, who lived in the 13th century CE.

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

Mark Twain is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976. Mark Twain is named for the American author Mark Twain, who lived from 1835 to 1910.

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

Holst is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) on April 24, 2012.

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

Barney is a small crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 2013. Barney is named for the American-French playwright, poet, and novelist Natalie Clifford Barney.

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

Joplin is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 2012, after the American composer Scott Joplin.

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

Larrocha is an impact crater on Mercury. It has a diameter of 196 km (122 mi), and it is one of 110 peak ring basins on Mercury. It is located in the Victoria quadrangle at 43.29°N 69.83°W.

References

  1. "Nabokov". Gazetteer of Planetary Nomenclature. IAU/NASA/USGS . Retrieved 20 January 2020.
  2. Chapman, C. R., Baker, D. M. H., Barnouin, O. S., Fassett, C. I., Marchie, S., Merline, W. J., Ostrach, L. R., Prockter, L. M., and Strom, R. G., 2018. Impact Cratering of Mercury. In Mercury: The View After MESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 9.