Chapter 11: Problem 15
What may have caused the thick atmosphere that Mars is believed to have had in the distant past to have disappeared?
Short Answer
Expert verified
Mars lost its thick atmosphere due to solar wind stripping and lower gravity, facilitated by the absence of a magnetic field.
Step by step solution
01
Understanding Martian Atmosphere Loss
Mars once had a thick atmosphere composed mainly of carbon dioxide. Scientists believe that the planet's atmosphere has thinned over billions of years, leaving it much less substantial than it once was.
02
Investigating Possible Causes
Several factors could have contributed to the loss of Mars' atmosphere: solar wind stripping, lack of a magnetic field, and lower gravity compared to Earth. Mars' smaller size and mass suggest it has a weaker gravitational pull, making it easier for atmospheric particles to escape into space.
03
Solar Wind Stripping Explanation
Mars lacks a significant magnetic field, which on Earth protects the atmosphere from solar winds. Without this protection, charged particles from the solar wind can strip away atmospheric particles over time, gradually thinning it.
04
Analyzing the Role of the Core
The cooling of Mars' core is believed to have stopped its magnetic dynamo, which is responsible for generating the magnetic field. Without a magnetic field, the atmosphere couldn't be shielded from solar winds effectively.
05
Conclusion
Mars' atmosphere likely disappeared because of a combination of factors: the lack of a strong magnetic field led to increased solar wind stripping, and the lower gravity made it easier for atmosphere molecules to escape into space.
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Solar Wind
Solar wind is a stream of charged particles—mainly electrons and protons—emitted by the sun. These particles travel through space at high speeds and have substantial effects on planetary atmospheres. For planets without a strong magnetic field, the solar wind can become a major player in atmospheric loss. The high-speed particles collide with atmospheric molecules, imparting enough energy to help them escape into space. Over time, continuous exposure to solar wind can lead to significant thinning of a planet's atmosphere.
On Earth, our strong magnetic field deflects much of this solar wind, providing a protective shield. This crucial protection helps maintain our atmosphere's integrity. Mars, however, lacks such a defense, making its atmosphere vulnerable to the relentless assault from solar winds.
On Earth, our strong magnetic field deflects much of this solar wind, providing a protective shield. This crucial protection helps maintain our atmosphere's integrity. Mars, however, lacks such a defense, making its atmosphere vulnerable to the relentless assault from solar winds.
Magnetic Field
A magnetic field acts as an invisible force field that protects a planet's atmosphere from various space phenomena, particularly the solar wind. Earth's magnetic field, generated by the movement of molten iron in its core, deflects many of the charged particles of solar wind, thus helping to retain its atmosphere.
Mars, on the other hand, currently has no global magnetic field. It is believed that Mars once had a magnetic field, but it disappeared as the planet's core cooled and solidified, ceasing to generate a protective shield.
Mars, on the other hand, currently has no global magnetic field. It is believed that Mars once had a magnetic field, but it disappeared as the planet's core cooled and solidified, ceasing to generate a protective shield.
- Without this shield, Mars' atmosphere was exposed to the full brunt of solar winds.
- The magnetic field not only protects; it also helps stabilize many aspects of a planet's environment.
Atmospheric Loss
Atmospheric loss refers to the gradual thinning and disappearance of a planet's atmosphere over time. Several factors contribute to this, including solar wind stripping, lack of a magnetic field, and the planet’s gravitational strength.
On Mars, atmospheric loss has been particularly pronounced due to its lack of a magnetic field and its smaller size compared to Earth. This smaller size results in lower gravity, which does not tightly hold onto gas molecules.
On Mars, atmospheric loss has been particularly pronounced due to its lack of a magnetic field and its smaller size compared to Earth. This smaller size results in lower gravity, which does not tightly hold onto gas molecules.
- Solar wind stripping is another key factor; it involves the solar wind's charged particles removing atmospheric gases.
- This process can take billions of years but results in a much thinner atmosphere than originally existed.
Mars Gravity
Gravity is the force that keeps a planet’s atmosphere from drifting into space. The strength of a planet's gravity depends on its size and mass. Larger and more massive planets have stronger gravitational fields, which can more effectively hold onto an atmosphere.
Mars is smaller and less massive than Earth, resulting in a weaker gravity. This makes it easier for gas molecules in Mars' atmosphere to escape into space.
Combined with factors like the lack of a magnetic field, Mars' lower gravity contributes to its inability to retain a thick atmosphere.
Mars is smaller and less massive than Earth, resulting in a weaker gravity. This makes it easier for gas molecules in Mars' atmosphere to escape into space.
Combined with factors like the lack of a magnetic field, Mars' lower gravity contributes to its inability to retain a thick atmosphere.
- Lower gravity allows atmospheric particles to overcome the pull of the planet more easily.
- This factor, along with solar wind stripping, accelerates the process of atmospheric loss.