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List of quadrangles on Mercury

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The surface of the planetMercury has been divided into fifteenquadrangles, designated H-1 to H-15 (the 'H' stands forHermes, the Greek equivalent of Mercury).[1] The quadrangles are named for prominent surface features visible within each area.[1] The quadrangles were initially named foralbedo features, as these were the most prominent features visible before mapping was carried out by spacecraft. The mapping carried out with the images obtained by theMariner 10 flybys in 1974 and 1975 led to nine of the quadrangles being renamed for newly mapped prominent features.[1] The remaining six quadrangles were completely unmapped byMariner 10 and were still referred to by their albedo feature names. Following the arrival ofMESSENGER in orbit in 2011, these six quadrangles were mapped and renamed.[2] The base mosaic used in the new maps was produced with orbital images by the MESSENGER Team and released by NASA’s Planetary Data System on March 8, 2013. This global mosaic includes complete coverage of Mercury’s surface.

Name[3]NumberNamesakeAlbedo feature name[4]Area[5]Mariner 10 mapCurrent map[3]Notes
BorealisH-1Borealis Planitia[6]BoreaNorth pole to 67° latitudeProvisionally called "Goethe", but renamed by the International Astronomical Union in 1976 (IAU, 1977)[5]
VictoriaH-2Victoria RupesAurora0 to 90° longitude, 21 to 66° latitude
ShakespeareH-3Shakespeare craterCaduceata90 to 180° longitude, 21 to 66° latitude
RaditladiH-4Raditladi craterLiguria270 to 180° longitude, 21 to 66° latitudenone
HokusaiH-5Hokusai craterApollonia360 to 270° longitude, 21 to 66° latitudenone
KuiperH-6Kuiper craterTricrena0 to 72° longitude, −22 to 22° latitude
BeethovenH-7Beethoven craterSolitudo Lycaonis72 to 144° longitude, −22 to 22° latitude
TolstojH-8Tolstoj craterPhaethontias144 to 216° longitude, −22 to 22° latitudeProvisionally called "Tir", but renamed by the International Astronomical Union in 1976 (IAU, 1977)[5]
EminescuH-9Eminescu craterSolitudo Criophori216 to 288° longitude, −22 to 22° latitudenone
DerainH-10Derain craterPieria288 to 360° longitude, −22 to 22° latitudenone
DiscoveryH-11Discovery Rupes[6]Solitudo Hermae Trismegisti0 to 90° longitude, −21 to −66° latitude
MichelangeloH-12Michelangelo craterSolitudo Promethei90 to 180° longitude, −21 to −66° latitude
NerudaH-13Neruda craterSolitudo Persephones180 to 270° longitude, −21 to −66° latitudenone
DebussyH-14Debussy craterCyllene270 to 360° longitude, −21 to −66° latitudenone
BachH-15Bach craterAustraliaSouth pole to −67° latitude

Schema of the quadrangles

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Relationship of the quadrangles to each other on the surface of Mercury:[5]

See also

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References

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  1. ^abcStrom, Robert G.; Sprague, Ann L. (2003).Exploring Mercury: The Iron Planet. p. 79.ISBN 9781852337315.
  2. ^"IAU Information Bulletin"(PDF) (108). International Astronomical Union. July 2011: 23. Archived fromthe original(PDF) on 2022-01-08. Retrieved2013-09-19.{{cite journal}}:Cite journal requires|journal= (help)
  3. ^ab"1:5 Million-Scale Maps of Mercury". Gazetteer of Planetary Nomenclature (USGS/IAU/NASA).Archived from the original on 2013-02-17. Retrieved2021-10-24.
  4. ^"SP-423 Atlas of Mercury". NASA. p. 21.Archived from the original on 2011-01-04. Retrieved2013-09-19.
  5. ^abcdSchaber, Gerald G.; John F. McCauley (1980).Geologic Map of the Tolstoj (H-8) Quadrangle of Mercury(PDF). U.S. Geological Survey. USGS Miscellaneous Investigations Series Map I–1199, as part of the Atlas of Mercury, 1:5,000,000 Geologic Series.Archived(PDF) from the original on 2022-10-09. Retrieved2007-11-12.
  6. ^ab"SP-423 Atlas of Mercury". NASA.Archived from the original on 2007-11-10. Retrieved2007-11-12.
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