The Medusae Fossae Formation is a large geological formation of probable volcanic origin on the planet
Mars
Mars is the fourth planet from the Sun. It is also known as the "Red Planet", because of its orange-red appearance. Mars is a desert-like rocky planet with a tenuous carbon dioxide () atmosphere. At the average surface level the atmosph ...
.
It is named for the
Medusa
In Greek mythology, Medusa (; ), also called Gorgo () or the Gorgon, was one of the three Gorgons. Medusa is generally described as a woman with living snakes in place of hair; her appearance was so hideous that anyone who looked upon her wa ...
of Greek mythology. "Fossae" is Latin for "trenches".
The formation is a collection of soft, easily eroded deposits that extends discontinuously for more than 5,000 km along the
equator
The equator is the circle of latitude that divides Earth into the Northern Hemisphere, Northern and Southern Hemisphere, Southern Hemispheres of Earth, hemispheres. It is an imaginary line located at 0 degrees latitude, about in circumferen ...
of
Mars
Mars is the fourth planet from the Sun. It is also known as the "Red Planet", because of its orange-red appearance. Mars is a desert-like rocky planet with a tenuous carbon dioxide () atmosphere. At the average surface level the atmosph ...
. Its roughly-shaped regions extend from just south of
Olympus Mons
Olympus Mons (; ) is a large shield volcano on Mars. It is over high as measured by the Mars Orbiter Laser Altimeter (MOLA), about 2.5 times the elevation of Mount Everest above sea level. It is Mars's tallest volcano, its tallest planetary mou ...
to
Apollinaris Patera, with a smaller additional region closer to
Gale Crater
Gale is a crater, and probable dry lake, at in the northwestern part of the Aeolis quadrangle on Mars. It is in diameter and estimated to be about 3.5–3.8 billion years old. The crater was named after Walter Frederick Gale, an amateur a ...
.
The total area of the formation is equal to 20% the size of the continental United States.
It is divided into three subunits (members) that are all considered to be of
Amazonian age, the youngest era in martian geological history.
The formation straddles the
highland - lowland boundary near the
Tharsis and
Elysium
Elysium (), otherwise known as the Elysian Fields (, ''Ēlýsion pedíon''), Elysian Plains or Elysian Realm, is a conception of the afterlife that developed over time and was maintained by some Greek religious and philosophical sects and cult ...
volcanic areas, and extends across five quadrangles:
Amazonis,
Tharsis,
Memnonia,
Elysium
Elysium (), otherwise known as the Elysian Fields (, ''Ēlýsion pedíon''), Elysian Plains or Elysian Realm, is a conception of the afterlife that developed over time and was maintained by some Greek religious and philosophical sects and cult ...
, and
Aeolis
Aeolis (; ), or Aeolia (; ), was an area that comprised the west and northwestern region of Asia Minor (modern-day Turkey), mostly along the coast, and also several offshore islands (particularly Lesbos), where the Aeolian Greek city-states w ...
.
Origin and age
The origin of the formation is unknown, but many theories have been presented over the years.
In 2020, a group of researchers headed by Peter Mouginis-Mark has hypothesized that the formation could have been formed from pumice rafts from the volcano
Olympus Mons
Olympus Mons (; ) is a large shield volcano on Mars. It is over high as measured by the Mars Orbiter Laser Altimeter (MOLA), about 2.5 times the elevation of Mount Everest above sea level. It is Mars's tallest volcano, its tallest planetary mou ...
. In 2012, a group headed by Laura Kerber hypothesized that it could have been formed from ash from the volcanoes
Apollinaris Mons,
Arsia Mons, and possibly
Pavonis Mons.
An analysis of data from the
Mars Odyssey
''2001 Mars Odyssey'' is a robotic spacecraft orbiting the planet Mars. The project was developed by NASA, and contracted out to Lockheed Martin, with an expected cost for the entire mission of US$297 million. Its mission is to use spectro ...
Neutron Spectrometer revealed that the western lobe of the Medusae Fossae Formation contains some water. This means that this formation contains bulk water ice. During periods of high
obliquity
In astronomy, axial tilt, also known as obliquity, is the angle between an object's rotational axis and its orbital axis, which is the line perpendicular to its orbital plane; equivalently, it is the angle between its equatorial plane and orbital ...
(tilt) water ice was stable on the surface. By means of a re-analysis of data from
Mars Express
''Mars Express'' is a space exploration mission by the European Space Agency, European Space Agency (ESA) exploring the planet Mars and its moons since 2003, and the first planetary mission attempted by ESA.
''Mars Express'' consisted of two ...
'
MARSIS radar, Thomas Watters found evidence about the existence of large underground water deposits in Medusae Fossae up to 3.7 km thick and covered by hundreds of meters of dust.
Combining several gravity models of Mars with the
MOLA topographic dataset allowed calculation of the density of the deposit; the value is 1.765 ± 0.105 g/cm
3, similar to the density of terrestrial
ignimbrite
Ignimbrite is a type of volcanic rock, consisting of hardened tuff. Ignimbrites form from the deposits of pyroclastic flows, which are a hot suspension of particles and gases flowing rapidly from a volcano, driven by being denser than the surrou ...
s.
This rules out significant amounts of ice in the bulk composition. In combination with the deposit's high content of sulfur and chlorine, it implies an explosive volcanic origin. The total volume of the deposit is 1.4 million km
3; such a large deposit might have been emplaced in periodic eruptions over an interval of 500 million years.
Appearance and composition
In some places, the formation appears as a smooth and gently undulating surface, while in others it is wind-sculpted into ridges and grooves.
Radar imaging has suggested that the region may contain either extremely porous rock (for example volcanic ash) or deep layers of glacier-like ice deposits amounting to about the same quantity as is stored in Mars' south polar cap. Further evidence for a fine-grained composition is the fact that the area gives almost no radar return.
File:Medusae Fossae Remnant.jpg, Plateau and rootless cones (HiRISE)
File:ESP 036510 1735layers.jpg, Mounds with layers, east of Gale Crater in Aeolis quadrangle
The Aeolis quadrangle is one of a series of list of quadrangles on Mars, 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Aeolis quadrangle is also referred to as MC-23 (Mars Chart-2 ...
File:Wikiesp036510 1735layersmedussa.jpg, Layers and mounds, east of Gale Crater
File:Wikiesp036510 1735moundsmedussa.jpg, Layers and a field of small mounds, east of Gale Crater
File:Wikiesp036510 1735layersmound.jpg, Mound showing layers at the base, east of Gale Crater
File:ESP 038302 1735medusaelayers.jpg, Surface features along a scarp in Memnonia quadrangle
The Memnonia quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Memnonia quadrangle is also referred to as MC-16 (Mars Chart-16).
The quadrangle i ...
(HiRISE)
Inverted relief

The lower portion (member) of Medusae Fossae Formation contains many patterns and shapes that are thought to be the remains of streams. It is believed that streams formed valleys that were filled and became resistant to erosion by cementation of minerals or by the gathering of a coarse covering layer to form an
inverted relief. These inverted stream beds are sometimes called sinuous ridges or raised curvilinear features. They have been divided into six classes: flat-crested, narrow-crested, round-crested, branching, non-branching, and multilevel. They may be a kilometer or so in length. Their height ranges from a meter to greater than 10 meters, while the width of the narrow ones is less than 10 meters.
Yardangs and dust
Comparisons of elemental composition suggest that the Medusae Fossae Formation has been a source of Mars' ubiquitous surface dust.
In July 2018, researchers reported that it may be the largest single source of
dust
Dust is made of particle size, fine particles of solid matter. On Earth, it generally consists of particles in the atmosphere that come from various sources such as soil lifted by wind (an aeolian processes, aeolian process), Types of volcan ...
on the planet.
The surface of the formation has been eroded by the wind into a series of linear ridges called
yardangs. These ridges generally point in direction of the
prevailing winds
In meteorology, prevailing wind in a region of the Earth's surface is a surface wind that blows predominantly from a particular Wind direction, direction. The dominant winds are the trends in direction of wind with the highest speed over a partic ...
that carved them, and demonstrate the erosive power of Martian winds. The easily eroded nature of the Medusae Fossae Formation suggests that it is composed of weakly cemented particles, and was most likely formed by the deposition of wind-blown dust or
volcanic ash
Volcanic ash consists of fragments of rock, mineral crystals, and volcanic glass, produced during volcanic eruptions and measuring less than 2 mm (0.079 inches) in diameter. The term volcanic ash is also often loosely used to r ...
. Yardangs are parts of rock that have been sand blasted into long, skinny ridges by bouncing sand particles blowing in the wind. Layers are seen in parts of the formation. A resistant caprock on the top of yardangs has been observed in Viking,
Mars Global Surveyor
''Mars Global Surveyor'' (MGS) was an American Robotic spacecraft, robotic space probe developed by NASA's Jet Propulsion Laboratory. It launched November 1996 and collected data from 1997 to 2006. MGS was a global mapping mission that examined ...
, and
HiRISE
High Resolution Imaging Science Experiment is a camera on board the '' Mars Reconnaissance Orbiter'' which has been orbiting and studying Mars since 2006. The 65 kg (143 lb), US$40 million instrument was built under the direction ...
photos. Images from spacecraft show that they have different degrees of hardness probably because of significant variations in the physical properties, composition, particle size, and/or
cementation. Very few
impact craters
An impact crater is a depression in the surface of a solid astronomical body formed by the hypervelocity impact of a smaller object. In contrast to volcanic craters, which result from explosion or internal collapse, impact craters typically ...
are visible throughout the area so the surface is relatively young.
File:Medusae Fossae Formation.jpg, Yardangs in the Medusae Fossae (THEMIS
In Greek mythology and religion, Themis (; ) is the goddess and personification of justice, divine order, law, and custom. She is one of the twelve Titan children of Gaia and Uranus, and the second wife of Zeus. She is associated with oracles a ...
)
File:Apollinarisandmedusae.JPG, Yardangs in Aeolis
Aeolis (; ), or Aeolia (; ), was an area that comprised the west and northwestern region of Asia Minor (modern-day Turkey), mostly along the coast, and also several offshore islands (particularly Lesbos), where the Aeolian Greek city-states w ...
(HiRISE
High Resolution Imaging Science Experiment is a camera on board the '' Mars Reconnaissance Orbiter'' which has been orbiting and studying Mars since 2006. The 65 kg (143 lb), US$40 million instrument was built under the direction ...
)
File:WikiESP 039563 1730yardangs.jpg, Yardangs in Arsinoes Chaos (HiRISE)
File:WikiESP 039563 1730yardangsclose.jpg, Close-up, arrows point to transverse aeolian sand ridges (HiRISE)
File:23664medussa.jpg, Yardangs in Amazonis (HiRISE)
File:Yardangs in Medusae.jpg, Yardangs with caprock labeled, in Aeolis
Aeolis (; ), or Aeolia (; ), was an area that comprised the west and northwestern region of Asia Minor (modern-day Turkey), mostly along the coast, and also several offshore islands (particularly Lesbos), where the Aeolian Greek city-states w ...
(HiRISE)
File:WikiESP 035558 1830yardang.jpg, Yardangs near Gordii Dorsum, in the north of the formation (HiRISE)
File:35558 1830yardangs.jpg, Yardangs near Gordii Dorsum (enlargement of the previous image)
File:35558 1830yardangsclose.jpg, Yardangs near Gordii Dorsum (enlargement of the previous image)
File:WikiESP 036429 1925yardangscrater.jpg, Yardangs near a crater in Amazonis, in the middle of the region
File:Wikiesp036510 1735layersyardang.jpg, Yardangs showing layers, east of Gale Crater in Aeolis
Aeolis (; ), or Aeolia (; ), was an area that comprised the west and northwestern region of Asia Minor (modern-day Turkey), mostly along the coast, and also several offshore islands (particularly Lesbos), where the Aeolian Greek city-states w ...
(HiRISE)
File:46913 1800yardangs.jpg, Yardangs, in a crater in Amazonis quadrangle (HiRISE)
See also
*
Aeolis quadrangle
The Aeolis quadrangle is one of a series of list of quadrangles on Mars, 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Aeolis quadrangle is also referred to as MC-23 (Mars Chart-2 ...
*
Amazonis Planitia
Amazonis Planitia (, Latin ''Amāzŏnis'') is one of the smoothest plains on Mars. It is located between the Tharsis and Elysium volcanic provinces, to the west of Olympus Mons, in the Amazonis and Memnonia quadrangles, centered at . Th ...
*
Amazonis quadrangle
*
Geology of Mars
The geology of Mars is the scientific study of the surface, crust, and interior of the planet Mars. It emphasizes the composition, structure, history, and physical processes that shape the planet. It is analogous to the field of terrestrial geo ...
*
Groundwater on Mars
300px, The preservation and cementation of aeolian dune Endurance_(crater).html" ;"title="stratigraphy in Burns Cliff in Endurance (crater)">Endurance Crater are thought to have been controlled by flow of shallow groundwater.
Rain and snow we ...
*
Impact crater
An impact crater is a depression (geology), depression in the surface of a solid astronomical body formed by the hypervelocity impact event, impact of a smaller object. In contrast to volcanic craters, which result from explosion or internal c ...
*
Yardangs on Mars
External links
Graphical image of the geographical extent of the Medusae Fossae Formation Nature Communications
References
{{Portal bar, Solar System
Surface features of Mars
Amazonis quadrangle
Valleys and canyons on Mars