Determining a Planet's Age Based on Mountain Ranges

In summary, the conversation discusses the idea that as planets age and their cores cool and shrink, there is a decrease in tectonic activity and an increase in mountain ranges due to plate tension on the surface. However, it is now known that the heat generated by radioactive decay in the core is what causes tectonic activity, not shrinkage, and this has no effect on the surface of the Earth. This theory was once thought to be true for Mars and the Moon before they cooled and solidified.
  • #1
Mattius_
8
0
Just thought of this, probably no validity to it, but just a thought.

Most planets start with hot cores, they eventually cool, and shrink. Their cooling and shrinking results in more plate tension on the surface because of the shrinkage. This would create more mountain ranges on planets. So, if a planet has many mountain ranges, than someone may surmise that it has cooled and shrunk, and thus, aged. :smile:
 
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  • #2
It seems to me that as a planet ages and its core cools off, tectonic activity would decrease. The mantle wouldn't be as active, and eventually the plates would lose their momentum and fuse. Erosion would then take care of the rest and homogenize the planet's surface.
 
  • #3
Mattius_ said:
Just thought of this, probably no validity to it, but just a thought.

Most planets start with hot cores, they eventually cool, and shrink. Their cooling and shrinking results in more plate tension on the surface because of the shrinkage. This would create more mountain ranges on planets. So, if a planet has many mountain ranges, than someone may surmise that it has cooled and shrunk, and thus, aged. :smile:


This was the commonly held theory about mountain formation before the 1920s. However, radioactive decay of isotopes in the Earth's core generates heat and it is this which keeps the core molten and makes the tectonic plates move around as they do. Shrinkage had absolutely no effect whatsoever on the present Earth's surface.

I assume the same was true for Mars and the Moon before they cooled down and solidified.
 

Related to Determining a Planet's Age Based on Mountain Ranges

1. How can mountain ranges help determine a planet's age?

Mountain ranges are formed by tectonic activity, which is the movement and collision of large plates beneath a planet's surface. By studying the formation and erosion patterns of these mountain ranges, scientists can estimate the age of the planet's crust and its overall age.

2. What tools and techniques are used to determine the age of mountain ranges?

Scientists use a variety of techniques, such as radiometric dating, paleomagnetism, and stratigraphy, to determine the age of mountain ranges. These methods involve analyzing the rocks and minerals within the mountains to determine their composition, structure, and relative age.

3. Can the age of a planet's mountain ranges change over time?

Yes, the age of a planet's mountain ranges can change over time due to erosion, tectonic activity, and other geological processes. This is why it is important for scientists to continually study and monitor these mountain ranges to accurately determine their age.

4. How do scientists account for different rates of erosion when determining a planet's age based on mountain ranges?

Scientists use a variety of methods to account for different rates of erosion, such as comparing the erosion rates of different mountain ranges within the same area or using computer simulations to model the effects of erosion on mountain ranges over time. These methods can help to refine age estimates and account for variations in erosion rates.

5. Can determining a planet's age based on mountain ranges be applied to all planets in our solar system?

No, the methods used to determine a planet's age based on mountain ranges may not be applicable to all planets in our solar system. Each planet has its own unique geological history and processes, making it necessary for scientists to develop specific methods for each planet. Additionally, some planets may have different types of surface features that cannot be used to determine their age, such as ice-covered worlds or gas giants.

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