How Mars Lost Its Water to Space

How Mars Lost Its Water to Space

Mars was once a warm, wet world.

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Between 3.7 and 4 billion years ago, rivers and lakes covered the surface, protected by a strong magnetic field.

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Without protection, the solar wind began stripping away the atmosphere.

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Today, we know water escapes through processes like photodissociation, where sunlight breaks water molecules into hydrogen and oxygen.

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Dust storms also play a role, lifting water vapor high into the atmosphere where it is more easily lost.

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While much water has vanished, some remains trapped in polar ice caps, underground permafrost, and rocks.

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Missions like MAVEN help scientists track this history by studying isotope ratios, which act as a 'fingerprint' of lost water.

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Understanding Mars helps us learn how planets evolve and what makes a world capable of supporting life.

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Comprehension Questions

What primary factor originally protected the ancient Martian atmosphere?

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Correct Choice

A strong global magnetic field

What is the primary mechanism for the long-term depletion of water on Mars?

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Correct Choice

The escape of hydrogen into space

How do dust storms affect the loss of water on Mars?

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Correct Choice

They transport water vapor to high altitudes where it is more vulnerable to escape

What do scientists use as a 'fingerprint' to measure how much water Mars has lost?

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Correct Choice

The ratio of hydrogen to deuterium

Where is most of the remaining water on Mars located today?

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Correct Choice

In polar ice caps, subsurface permafrost, and hydrated rocks

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