Does internal pressure always increase inwards with size

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Discussion Overview

The discussion revolves around the concept of internal pressure within large planetary bodies, particularly whether pressure consistently increases inward with size. Participants explore theoretical implications of self-supporting structures, the effects of gravity, and the nature of material properties in solid and liquid states.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants propose that internal pressure may not always increase with depth in large objects, suggesting that lateral forces could counteract vertical forces in solid structures.
  • Others argue that pressure typically increases with depth, assuming that variations in material properties are small compared to the overall size of the object.
  • A participant suggests that in solid bodies formed over long periods, layers of self-supporting material could reduce the transmission of pressure to lower layers, potentially leading to lower density than expected.
  • There is a discussion about the implications of rapid versus slow planetary formation on the material state and density of celestial bodies.
  • Some participants question the assumption of uniform material properties and elastic deformation in the context of planetary formation, suggesting that many bodies may behave more plastically.
  • One participant introduces the idea of concentric shells that do not contribute to internal pressure once they are self-supporting, challenging traditional assumptions about density based on size.
  • Another participant counters that planets are too massive to be self-supporting and emphasizes that empirical data from space probes confirm their mass and gravitational properties.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the behavior of internal pressure in large planetary bodies, with no consensus reached on the validity of the various models proposed.

Contextual Notes

Participants highlight limitations in assumptions regarding material properties, the effects of gravity, and the nature of planetary formation, which remain unresolved in the discussion.

curiouschris
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I was reading about states of planetary ice in the following article. http://www.sciencedaily.com/releases/2015/06/150622182455.htm when it struck me that perhaps we should not assume that pressure increases as we descend into a large object.

Like a cathedral ceiling a large cave does not exert pressure on the cavity within. This is because of the lateral forces supporting the structure.

Do we assume this does not happen inside large rocky objects? Clearly in a large liquid object this would occur but in a cool or frozen object could not the lateral forces negate the vertical forces meaning a ice planet does not experience the extremes of pressure discussed in the article?
 
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Pressure increases as you descent assuming that variatons from homogeniety as you descent are small compared with the overall size.
Sure - there could be a hollow Moon someplace but how likely is that?
How would the hollow space within form without balancing the inwards pressure from the upper surfaces?
(Cathedrals need scaffolding to hold them up while they form.)
 
Although I used a hollow object as in a cathedral or a cave. it was only to get across the idea of a self supporting structure.

My point is at some point the entire structure assuming it is not plastic will actually have layers of self supporting material which prevents or reduces the transmission of pressure to the lower layers.

Combine that with a decrease in gravity as you progress towards the centre and while I don't see hollow moons I certainly see objects where the density is greatly over estimated.
 
Last edited:
A.T. said:
In a solid sphere under its own gravity, there is a layer near the surface that will be stretched radially (PROBLEM 3):
https://books.google.de/books?id=tpY-VkwCkAIC&lpg=PP1&hl=de&pg=PA19#v=onepage&q&f=false

Yes. that problem makes the assumption I am talking about.

Lets assume that we are talking about heavenly bodies. Planets form over million and billions of years. if the formation is rapid the planet will not have enough time to cool, thus it will remain plastic and all the formulas will be approximately correct.

But bodies forming more slowly which radiate their heat and thus cool to a solid state will support new material added (and stretched radially) until it too cools and hardens enough to support new material added to its surface. Thus the cycle continues.

In this process you would end up with concentric layers of self supporting material which transfers little of its own weight to underlying layers. thus creating lower density objects than one would assume.

Clearly the Earth with its molten centre is not a sphere that fits this description. I am just saying the Earth may not be prototypical.
 
You are thinking of, say, concentric shells of material that do not touch with vacuum between them?
The addition of more concentric spheres outside would not contribute to the load on the lower spheres?
Likewise, a ball inside a house does not need to support the weight of the house.
 
curiouschris said:
Yes. that problem makes the assumption I am talking about.
They assume uniform material properties and elastic deformation. I doubt this applies to planet formation, which is more plastic.
 
Simon Bridge said:
You are thinking of, say, concentric shells of material that do not touch with vacuum between them?
No need for a vacuum although if the inner shell contracted for some reason a vacuum could form or gases or liquids leak in from other levels.

All I am saying is that once a shell is self supporting it no longer adds to the internal pressure. Therefore an assumption of internal pressures and hence density based on the size of an object may be incorrect.

It was just a thought.
 
A planet is far too massive to be self-supporting even it it were rigid, which it isn't (it is plastic). Indeed, that's part of the definition of "planet".

Moreover, since we'sent probes to all of the planets in the solar system, we've confirmed their mass by sensing their gravitational pull.
 

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