Difference between revisions of "Mars Quadrangles"
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The surface of Mars has been divided into thirty cartographic quadrangles by the United States Geological Survey. The maps below were produced by the [[Mars Global Surveyor]]'s [[w:Mars_Orbiter_Laser_Altimeter|Mars Orbiter Laser Altimeter]]; redder colors indicate higher elevations. The maps of the equatorial quadrangles use a [[w:Mercator_projection|Mercator projection]], while those of the mid-latitude quadrangles use a [[w:Lambert_conformal_conic_projection|Lambert conformal conic projection]], and the maps of the polar quadrangles use a polar [[w:Stereographic_projection_in_cartography|stereographic projection]]. | The surface of Mars has been divided into thirty cartographic quadrangles by the United States Geological Survey. The maps below were produced by the [[Mars Global Surveyor]]'s [[w:Mars_Orbiter_Laser_Altimeter|Mars Orbiter Laser Altimeter]]; redder colors indicate higher elevations. The maps of the equatorial quadrangles use a [[w:Mercator_projection|Mercator projection]], while those of the mid-latitude quadrangles use a [[w:Lambert_conformal_conic_projection|Lambert conformal conic projection]], and the maps of the polar quadrangles use a polar [[w:Stereographic_projection_in_cartography|stereographic projection]]. | ||
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See the [[Mars atlas|Mars Atlas]] for a general view of Mars. | See the [[Mars atlas|Mars Atlas]] for a general view of Mars. |
Revision as of 11:28, 18 January 2020
The surface of Mars has been divided into thirty cartographic quadrangles by the United States Geological Survey. The maps below were produced by the Mars Global Surveyor's Mars Orbiter Laser Altimeter; redder colors indicate higher elevations. The maps of the equatorial quadrangles use a Mercator projection, while those of the mid-latitude quadrangles use a Lambert conformal conic projection, and the maps of the polar quadrangles use a polar stereographic projection.
See the Mars Atlas for a general view of Mars.
Number | Name | Latitudes | Longitudes | Features | Map |
---|---|---|---|---|---|
MC-01 | Mare Boreum | 65–90° N | 180° W – 180° E | Features | |
MC-02 | Diacria | 30–65° N | 120–180° W | Features | |
MC-03 | Arcadia | 30–65° N | 60–120° W | Features | |
MC-04 | Mare Acidalium | 30–65° N | 0–60° W | Features | |
MC-05 | Ismenius Lacus | 30–65° N | 0–60° E | Features | |
MC-06 | Casius | 30–65° N | 60–120° E | Features | |
MC-07 | Cebrenia | 30–65° N | 120–180° E | Hecates Tholus | |
MC-08 | Amazonis | 0–30° N | 135–180° W | Features | |
MC-09 | Tharsis | 0–30° N | 90–135° W | Olympus Mons, | |
MC-10 | Lunae Palus | 0–30° N | 45–90° W | Features | |
MC-11 | Oxia Palus | 0–30° N | 0–45° W | Features | |
MC-12 | Arabia | 0–30° N | 0–45° E | Features | |
MC-13 | Syrtis Major | 0–30° N | 45–90° E | Jezero Crater | |
MC-14 | Amenthes | 0–30° N | 90–135° E | Features | |
MC-15 | Elysium | 0–30° N | 135–180° E | Elysium Mons | |
MC-16 | Memnonia | 0–30° S | 135–180° W | Features | |
MC-17 | Phoenicis Lacus | 0–30° S | 90–135° W | Arsia Mons | |
MC-18 | Coprates | 0–30° S | 45–90° W | Valles Marienis | |
MC-19 | Margaritifer Sinus | 0–30° S | 0–45° W | Features | |
MC-20 | Sinus Sabaeus | 0–30° S | 0–45° E | Features | |
MC-21 | Iapygia | 0–30° S | 45–90° E | Features | |
MC-22 | Mare Tyrrhenum | 0–30° S | 90–135° E | Features | |
MC-23 | Aeolis | 0–30° S | 135–180° E | Gale Crater, | |
MC-24 | Phaethontis | 30–65° S | 120–180° W | Features | |
MC-25 | Thaumasia | 30–65° S | 60–120° W | Features | |
MC-26 | Argyre | 30–65° S | 0–60° W | Argyre basin | |
MC-27 | Noachis | 30–65° S | 0–60° E | Features | |
MC-28 | Hellas | 30–65° S | 60–120° E | Hellas basin | |
MC-29 | Eridania | 30–65° S | 120–180° E | Features | |
MC-30 | Mare Australe | 65–90° S | 180° W – 180° E | Features |