First water map of Mars could help NASA choose where to land in the future
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While the idea of sending humans to Mars was once confined to science fiction, NASA hopes it could become a reality by the late 2030s.
But one of the key questions we need to resolve before we set off for the Red Planet, is where to land.
Now, scientists from the European Space Agency (ESA) have created the first water map of Mars, based on data from its Mars Express Observatory and NASA’s Mars Reconnaissance Orbiter.
The team hopes the map will change the way we think about Mars’ watery past and help in the decision of where to land on the Red Planet in the future.
Scientists from the European Space Agency (ESA) have created the first water map of Mars, based on data from its Mars Express Observatory and NASA’s Mars Reconnaissance Orbiter
The map shows the locations and abundances of aqueous minerals on Mars.
These minerals are from rocks that have been chemically altered by water in the past and have typically been transformed into clays and salts.
While you might think that these aqueous minerals would be few and far between, the big surprise is their prevalence on Mars, with the map revealing hundreds of thousands of such areas.
‘This work has now established that when you are studying the ancient terrains in detail, not seeing these minerals is actually the oddity,’ said Dr John Carter from the Institut d’Astrophysique Spatiale.
The big question is now whether this water was persistent, or confined to shorter, more intense episodes.
ESA hopes the map will serve as a better tool for answering this question.
‘I think we have collectively oversimplified Mars,’ said Dr Carter.
Scientists have previously tended to think that only a few types of clay minerals were created on Mars during its wet period.
Then, as water gradually dried up, salts were produced across the planet.
However, the new map shows that the process was likely much more complicated than this.
While many of the salts probably did form later than the clays, the map shows that there are exceptions.
Data from NASA’s Mars Reconnaissance Orbiter Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument showed the Jezero crater displays a rich variety of hydrated minerals
ESA’s Mars Express Observatoire pour la Mineralogie, l’Eau, les Glaces et l’Activité (OMEGA) instrument is better suited for higher spectral resolution mapping and provided global coverage of Mars
‘The evolution from lots of water to no water is not as clear cut as we thought, the water didn’t just stop overnight,’ Dr Carter explained.
‘We see a huge diversity of geological contexts, so that no one process, or simple timeline can explain the evolution of the mineralogy of Mars.
‘That’s the first result of our study. The second is that if you exclude life processes on Earth, Mars exhibits a diversity of mineralogy in geological settings just as Earth does.’
To create the map, ESA used data from various instruments.
For example, data from NASA’s Mars Reconnaissance Orbiter Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument showed the Jezero crater displays a rich variety of hydrated minerals.
Meanwhile, ESA’s Mars Express Observatoire pour la Mineralogie, l’Eau, les Glaces et l’Activité (OMEGA) instrument is better suited for higher spectral resolution mapping and provided global coverage of Mars.
The researchers hope the map will prove useful for NASA as it chooses where to land on Mars in the future.
The news comes ahead of NASA’s Artemis I mission, which is set to launch on August 29, paving the way for future missions to the moon and Mars.
‘Artemis I will be an uncrewed flight test that will provide a foundation for human deep space exploration, and demonstrate our commitment and capability to extend human existence to the Moon and beyond,’ NASA explained.
If the Artemis missions are a success, NASA aims to launch astronauts to Mars by the late 2030s or early 2040s.