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Areography

Areography, also known as the geography of Mars, is a subfield of planetary science that entails the delineation and characterization of regions on Mars.[1][2][3] Areography is mainly focused on what is called physical geography on Earth; that is the distribution of physical features across Mars and their cartographic representations. In April 2023, The New York Times reported an updated global map of Mars based on images from the Hope spacecraft.[4] A related, but much more detailed, global Mars map was released by NASA on 16 April 2023.[5]

Fretted terrain of Ismenius Lacus showing flat floored valleys and cliffs. Photo taken with Mars Orbiter Camera (MOC) on the Mars Global Surveyor.

Fretted terrain of Ismenius Lacus showing flat floored valleys and cliffs. Photo taken with Mars Orbiter Camera (MOC) on the Mars Global Surveyor.

Enlargement of the photo on the left showing cliff. Photo taken with high resolution camera of Mars Global Surveyor (MGS).

Enlargement of the photo on the left showing cliff. Photo taken with high resolution camera of Mars Global Surveyor (MGS).

View of lobate debris apron along a slope. Image located in Arcadia quadrangle.

View of lobate debris apron along a slope. Image located in Arcadia quadrangle.

Place where a lobate debris apron begins. Note stripes which indicate movement. Image located in Ismenius Lacus quadrangle.

Place where a lobate debris apron begins. Note stripes which indicate movement. Image located in Ismenius Lacus quadrangle.

Nomenclature[edit]

Early nomenclature[edit]

Although better remembered for mapping the Moon starting in 1830, Johann Heinrich Mädler and Wilhelm Beer were the first "areographers". They started off by establishing once and for all that most of the surface features were permanent, and pinned down Mars's rotation period. In 1840, Mädler combined ten years of observations and drew the first map of Mars ever made. Rather than giving names to the various markings they mapped, Beer and Mädler simply designated them with letters; Meridian Bay (Sinus Meridiani) was thus feature "a".


Over the next twenty years or so, as instruments improved and the number of observers also increased, various Martian features acquired a hodge-podge of names. To give a couple of examples, Solis Lacus was known as the "Oculus" (the Eye), and Syrtis Major was usually known as the "Hourglass Sea" or the "Scorpion". In 1858, it was also dubbed the "Atlantic Canale" by the Jesuit astronomer Angelo Secchi. Secchi commented that it "seems to play the role of the Atlantic which, on Earth, separates the Old Continent from the New;" this was the first time the fateful canale, which in Italian can mean either "channel" or "canal", had been applied to Mars.


In 1867, Richard Anthony Proctor drew up a map of Mars. It was based, somewhat crudely, on the Rev. William Rutter Dawes' earlier drawings of 1865, then the best ones available. Proctor explained his system of nomenclature by saying, "I have applied to the different features the names of those observers who have studied the physical peculiarities presented by Mars." Here are some of his names, paired with those later used by Schiaparelli in his Martian map created between 1877 and 1886.[23] Schiaparelli's names were generally adopted and are the names actually used today:

Sheehan, William, Archived 2017-09-11 at the Wayback Machine (Full text online) The University of Arizona Press, Tucson. 1996.

"The Planet Mars: A History of Observation and Discovery"

Google Maps for Mars, with various surface features and interesting places pointed out

Google Mars

Arizona State University

Mars/themis Maps

– Maps of Mars

Mars Maps

MEC-1 Prototype

Historical Globes of the Red Planet

– 3D Map of Mars

3D Map of Mars

Presents distances and altitudes of features/NASA

The Origin of Mars Crater Names

Interactive 3D map of Mars created by CTX