Difference between revisions of "Interior of Mars"

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==Overview of Layers==
 
==Overview of Layers==
Mars probably has a 24 to 72 km thick crust.  This crust is very light and seems to be highly fractured.  The crust of Mars is likely highly enriched with radioactive metals, which results in less heating lower down.<ref>https://www.eurekalert.org/news-releases/714311</ref> <ref>https://www.eurekalert.org/news-releases/876661</ref>
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Mars' crust is between 24 and 72 km thick.  This crust is very light and seems to be highly fractured.  The crust of Mars seems to contain half the radioactive materials on Mars, with proportionally less radioactive metals in the core than Earth, which results in less heating lower down.<ref>https://www.eurekalert.org/news-releases/714311</ref> <ref>https://www.eurekalert.org/news-releases/876661</ref>
  
It has a very deep lithosphere which is close to 500 km thick.  Like Earth, as you go deeper the mantle becomes less rigid, and softer.  The mantle has only one layer rather than Earth's two layers.
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It has a very deep lithosphere which is close to 500 km thick.  Like Earth, as you go deeper the mantle becomes less rigid and softer.  The mantle has only one layer, rather than Earth's two layers.
  
The core of Mars is liquid, and larger than expected~1830 km.  The core is less dense, likely it has more [[sulfur]], oxygen and even hydrogen than Earth's core.  These other elements make the Marian core les conductive than Earth's, which is consistent with Mars' extremely weak magnetic field. <ref>https://science.sciencemag.org/content/373/6553/443</ref>
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The core of Mars is liquid, and larger than expected at ~1830 km.  The core is less dense.  Likely it has more [[sulfur]], [[oxygen]] and even [[hydrogen]] than Earth's core.  These other elements make the Marian core les conductive than Earth's, which is consistent with Mars' extremely weak [[Magnetosphere|magnetic field]]. <ref>https://science.sciencemag.org/content/373/6553/443</ref>
  
 
==References==
 
==References==
 
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Revision as of 05:19, 2 August 2021

Until the InSight Mission we only had guesses of what the interior of Mars was like. However, with InSight, we are beginning to get limited data of the interior of Mars. Our information will greatly increase when we have several seismographs on Mars, since we will then have more than one 'view' of Martian earthquakes.

Overview of Layers

Mars' crust is between 24 and 72 km thick. This crust is very light and seems to be highly fractured. The crust of Mars seems to contain half the radioactive materials on Mars, with proportionally less radioactive metals in the core than Earth, which results in less heating lower down.[1] [2]

It has a very deep lithosphere which is close to 500 km thick. Like Earth, as you go deeper the mantle becomes less rigid and softer. The mantle has only one layer, rather than Earth's two layers.

The core of Mars is liquid, and larger than expected at ~1830 km. The core is less dense. Likely it has more sulfur, oxygen and even hydrogen than Earth's core. These other elements make the Marian core les conductive than Earth's, which is consistent with Mars' extremely weak magnetic field. [3]

References