List of quadrangles on Mercury
Template:SHORTDESC: The surface of the planet Mercury has been divided into fifteen quadrangles, designated H-1 to H-15 (the 'H' stands for Hermes, the Greek equivalent of Mercury).[1] The quadrangles are named for prominent surface features visible within each area.[1] The quadrangles were initially named for albedo 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 the Mariner 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 by Mariner 10 and were still referred to by their albedo feature names. Following the arrival of MESSENGER 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] | Number | Namesake | Albedo feature name[4] | Area[5] | Mariner 10 map | Current map[3] | Notes |
|---|---|---|---|---|---|---|---|
| Borealis | H-1 | Borealis Planitia[6] | Borea | North pole to 67° latitude | File:H-1 Borealis quadrangle.jpg | Provisionally called "Goethe", but renamed by the International Astronomical Union in 1976 (IAU, 1977)[5] | |
| Victoria | H-2 | Victoria Rupes | Aurora | 0 to 90° longitude, 21 to 66° latitude | File:Mercury, Aurora region.jpg | File:H-2 Victoria quadrangle.jpg | |
| Shakespeare | H-3 | Shakespeare crater | Caduceata | 90 to 180° longitude, 21 to 66° latitude | File:Mercury, Caduceata region.jpg | File:H-3 Shakespeare quadrangle.jpg | |
| Raditladi | H-4 | Raditladi crater | Liguria | 270 to 180° longitude, 21 to 66° latitude | none | File:H-4 Raditladi quadrangle.jpg | |
| Hokusai | H-5 | Hokusai crater | Apollonia | 360 to 270° longitude, 21 to 66° latitude | none | File:H-5 Hokusai quadrangle.jpg | |
| Kuiper | H-6 | Kuiper crater | Tricrena | 0 to 72° longitude, −22 to 22° latitude | File:Mercury h06 Kuiper quadrangle.png | File:H-6 Kuiper quadrangle.jpg | |
| Beethoven | H-7 | Beethoven crater | Solitudo Lycaonis | 72 to 144° longitude, −22 to 22° latitude | File:Mercury h07 Beethoven quadrangle.png | File:H-7 Beethoven quadrangle.jpg | |
| Tolstoj | H-8 | Tolstoj crater | Phaethontias | 144 to 216° longitude, −22 to 22° latitude | File:Mercury h08 Tolstoj quadrangle.png | File:H-8 Tolstoj quadrangle.jpg | Provisionally called "Tir", but renamed by the International Astronomical Union in 1976 (IAU, 1977)[5] |
| Eminescu | H-9 | Eminescu crater | Solitudo Criophori | 216 to 288° longitude, −22 to 22° latitude | none | File:H-9 Eminescu quadrangle.jpg | |
| Derain | H-10 | Derain crater | Pieria | 288 to 360° longitude, −22 to 22° latitude | none | File:H-10 Derain quadrangle.jpg | |
| Discovery | H-11 | Discovery Rupes[6] | Solitudo Hermae Trismegisti | 0 to 90° longitude, −21 to −66° latitude | File:Mercury h11 Discovery quadrangle.png | File:H-11 Discovery quadrangle.jpg | |
| Michelangelo | H-12 | Michelangelo crater | Solitudo Promethei | 90 to 180° longitude, −21 to −66° latitude | File:Mercury h12 Michelangelo quadrangle.png | File:H-12 Michelangelo quadrangle.jpg | |
| Neruda | H-13 | Neruda crater | Solitudo Persephones | 180 to 270° longitude, −21 to −66° latitude | none | File:H-13 Neruda quadrangle.jpg | |
| Debussy | H-14 | Debussy crater | Cyllene | 270 to 360° longitude, −21 to −66° latitude | none | File:H-14 Debussy quadrangle.jpg | |
| Bach | H-15 | Bach crater | Australia | South pole to −67° latitude | File:Mercury, Australia region.jpg | File:H-15 Bach quadrangle.jpg |
Schema of the quadrangles
[edit | edit source]Relationship of the quadrangles to each other on the surface of Mercury:[5]

See also
[edit | edit source]References
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