The delta is in the Eberswalde Crater in the southern highlands of Mars. The 40-mile-diameter (65 kilometers) crater is visible as a semicircle on the right of the image and was formed more than 3.7 billion years ago when an asteroid hit the planet.
The rim of the crater is intact only on its right-hand side. The rest appears only faintly or is not visible at all. A later impact created the 87-mile-diameter (140 km) Holden Crater that dominates the center and left side of the image. The expulsion of large amounts of material from that impact buried parts of Eberswalde.
However, within the visible part of Eberswalde, the delta and its feeder channels are well preserved, as seen near the top right of the crater. The delta covers an area of 44 square miles (115 square km). Small, meandering feeder channels are visible toward the top of the crater, which would have filled it to form a lake.
After the deposition of the delta sediments in the crater’s ancient lake, fresher sediments accumulated to cover up a major part of both the channels and the delta. These secondary sediments, presumably deposited by the wind, were later eroded in the delta area, exposing an inverted relief of the delta structure.
This delta structure, first identified with NASA’s Mars Global Surveyor spacecraft, is characteristic of the presence of a lake in the crater at that time. Such features provide a clear indication that liquid water flowed across the surface of Mars in the planet’s early history.
Both Eberswalde Crater and Holden Crater were on the list of four possible destinations for the next NASA Mars rover to be launched late this year. The main objective of the Mars Science Laboratory mission is the search for present or previously habitable environments on Mars. ESA’s Mars Express mission has been helping in the search for the best landing site.
Eberswalde was proposed because its delta indicates the long-lasting presence of liquid water in the past, and Holden Crater was a candidate because of its mineral diversity and many structures that again suggest past liquid water. Another candidate, Mawrth Vallis, exposes some of the oldest clay-rich layers on Mars. However, in July, Gale Crater, the final entry on the list, was selected as the mission’s landing site, given its high mineral and structural diversity related to water.
Eberswalde, Holden, and Mawrth Vallis will get to hold on to their secrets for a while longer.
The delta is in the Eberswalde Crater in the southern highlands of Mars. The 40-mile-diameter (65 kilometers) crater is visible as a semicircle on the right of the image and was formed more than 3.7 billion years ago when an asteroid hit the planet.
The rim of the crater is intact only on its right-hand side. The rest appears only faintly or is not visible at all. A later impact created the 87-mile-diameter (140 km) Holden Crater that dominates the center and left side of the image. The expulsion of large amounts of material from that impact buried parts of Eberswalde.
However, within the visible part of Eberswalde, the delta and its feeder channels are well preserved, as seen near the top right of the crater. The delta covers an area of 44 square miles (115 square km). Small, meandering feeder channels are visible toward the top of the crater, which would have filled it to form a lake.
After the deposition of the delta sediments in the crater’s ancient lake, fresher sediments accumulated to cover up a major part of both the channels and the delta. These secondary sediments, presumably deposited by the wind, were later eroded in the delta area, exposing an inverted relief of the delta structure.
This delta structure, first identified with NASA’s Mars Global Surveyor spacecraft, is characteristic of the presence of a lake in the crater at that time. Such features provide a clear indication that liquid water flowed across the surface of Mars in the planet’s early history.
Both Eberswalde Crater and Holden Crater were on the list of four possible destinations for the next NASA Mars rover to be launched late this year. The main objective of the Mars Science Laboratory mission is the search for present or previously habitable environments on Mars. ESA’s Mars Express mission has been helping in the search for the best landing site.
Eberswalde was proposed because its delta indicates the long-lasting presence of liquid water in the past, and Holden Crater was a candidate because of its mineral diversity and many structures that again suggest past liquid water. Another candidate, Mawrth Vallis, exposes some of the oldest clay-rich layers on Mars. However, in July, Gale Crater, the final entry on the list, was selected as the mission’s landing site, given its high mineral and structural diversity related to water.
Eberswalde, Holden, and Mawrth Vallis will get to hold on to their secrets for a while longer.
