page_title: Isidis Planitia
hierarchical_section_title: Isidis Planitia
caption_attribution_description: Isidis basin (Mars) topography
context_page_description: Isidis Planitia is a plain located inside a giant impact basin on Mars, centered at 12.9°N 87.0°E; Isidis Planitia is partly in the Syrtis Major quadrangle and partly in the Amenthes quadrangle. It is the third biggest obvious impact structure on the planet after the Hellas and Argyre basins – it is about 1,500 km in diameter.
  Isidis was likely the last major basin to be formed on Mars, having formed approximately 3.9 billion years ago during the Noachian Period. Due to dust coverage, it typically appears bright in telescopic views, and was mapped as a classical albedo feature, Isidis Regio, visible by telescope in the pre-spacecraft era.
  A study reported in Icarus described the complex geologic history of parts of Isidis, especially areas near the Deuteronilus contact. This contact is the supposed edge of a vast Martian ocean. The researchers found evidence of a Late Hesperian/Early Amazonian Sea in the area. The sea would have quickly frozen over. Eskers formed under the ice.
  Just to the west of Isidis is Syrtis Major Planum, a low-relief shield volcano that is a prominent dark albedo feature of Mars, which formed after the basin.
context_section_description: Isidis Planitia is a plain located inside a giant impact basin on Mars, centered at 12.9°N 87.0°E; Isidis Planitia is partly in the Syrtis Major quadrangle and partly in the Amenthes quadrangle. It is the third biggest obvious impact structure on the planet after the Hellas and Argyre basins – it is about 1,500 km (930 mi) in diameter.
  Isidis was likely the last major basin to be formed on Mars, having formed approximately 3.9 billion years ago during the Noachian Period. Due to dust coverage, it typically appears bright in telescopic views, and was mapped as a classical albedo feature, Isidis Regio, visible by telescope in the pre-spacecraft era.
  A study reported in Icarus described the complex geologic history of parts of Isidis, especially areas near the Deuteronilus contact.  This contact is the supposed edge of a vast Martian ocean.  The researchers found evidence of a Late Hesperian/Early Amazonian Sea in the area.  The sea would have quickly frozen over.  Eskers formed under the ice.
  Just to the west of Isidis is Syrtis Major Planum, a low-relief shield volcano that is a prominent dark albedo feature of Mars, which formed after the basin. The westernmost extent s bounded by a subregion, Northeast Syrtis with diverse geology.
  Around the Isidis basin magnesium carbonate was found by MRO. This mineral indicates that water was present and that it was not acidic, pH conditions more favorable for the evolution of life.
  The name "Isidis Planitia" follows the earlier name Isidis Regio ("Isis' Region").  Isis is the Egyptian goddess of heaven and fertility.
caption: Topography of Isidis Planitia
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