<p><strong>TL;DR</strong>: 1000 K (according to differentiated model of Pluto)</p>
<hr />
<p>According to the density value of Pluto, astronomers proposed three types of structural models:</p>
<ol>
<li>Undifferentiated or &quot;cold&quot; model: rocks mixed with water-ice</li>
<li>Differentiated or &quot;hot&quot; model: rocky core and water-ice mantle</li>
<li>Rocky core only (temperature high enough to boil off water-ice.</li>
</ol>
<p>There are two types of rocks to consider i.e. CI rock- carbonaceous chondrite(<span class="math-container">$\rho$</span> = 2.66g/cm3) for undifferentiated models which is <span class="math-container">$\approx$</span>13% by wt. eposomite(MgSO<sub>4</sub>) and Prinn-Frigley rock(<span class="math-container">$\rho$</span> = 3.262 g/cm3) for differentiated models which is sulfide-rich rocks like troilite(FeS).</p>
<p>McKinnon and Parmentier(1986); McKinnon and Mueller(1988) correctly predicted the structural model of Pluto to be differentiated one. During initial formation of Pluto, radiogenic heating was the only source of heat, hot enough to melt the outside part of the undifferentiated core consisting of hydrated CI-rocks to form liquid matter of what is known today as water-ice in the mantle (water-ice melting temperature was 251 K at 0.21 GPa). During that time, 80% of core was at above 500 K . The anhydrous silicate core at the center was still rigid resisting the outside flow (the temperature of core was 500 K). Convection through heating allowed steady-state heat flow to form water-ice in the mantle, some of which erupted into the surface. Although the gravitational potential energy was modest, the process become self-accelerating.</p>
<p>This process was also accelerated by the &quot;accretion process&quot; due to a large-body impact that resulted in the formation of Charon. This collision heated up the core by 100 K and also resulted in several differentiation of Pluto that made the surface level ice layer mixed with organic compounds.</p>
<p><em>Present day scenario:</em> Pluto is a rock-rich world with rock mass fraction <span class="math-container">$\gtrsim$</span> 60%. <strong>Core temperature is 1000 K</strong>, surrounded by 250-300 km thick mantle shell of predominately water-ice and mixed liquid rock. Surface temperature is 40 K. Core pressure is 1.1-1.4 GPa. Rock fraction (rock/rock+H2O+ice) for differentiated Pluto is 0.69-0.79(mainly PF-rock). There is also an extra thermal boundary layer between the ice-mantle and the ice-rock layer just outside the core. There might also be an organic layer in between the core and mantle but it hasn't been proven yet. The water-ice mantle is differentiated into several layers based on its transitions. You can check the details and calculation in ref.2</p>
<p><a href="https://i.sstatic.net/c9zwv.png" rel="noreferrer"><img src="https://i.sstatic.net/c9zwv.png" alt="enter image description here" /></a></p>
<p>Fig. 1: Temperature of Pluto at several Pressure value</p>
<p><a href="https://i.sstatic.net/E3wE2.png" rel="noreferrer"><img src="https://i.sstatic.net/E3wE2.png" alt="enter image description here" /></a></p>
<p>Fig. 2: Temperature of the mantle and outside layer</p>
<p><a href="https://i.sstatic.net/JaALL.png" rel="noreferrer"><img src="https://i.sstatic.net/JaALL.png" alt="enter image description here" /></a></p>
<p>Fig.3: Differentiated model of Pluto</p>
<p>References:</p>
<ol>
<li><a href="http://articles.adsabs.harvard.edu//full/1988LPI....19..764M/0000764.000.html" rel="noreferrer">http://articles.adsabs.harvard.edu//full/1988LPI....19..764M/0000764.000.html</a></li>
<li>Pluto and Charon, Alan Stern, David James Tholen, University of Arizona Press, 1997</li>
<li><a href="https://arxiv.org/ftp/arxiv/papers/1510/1510.06604.pdf" rel="noreferrer">https://arxiv.org/ftp/arxiv/papers/1510/1510.06604.pdf</a> (This paper discusses the possibility that Pluto might have an iron core)</li>
</ol>

CC BY-SA 4.0
2020-12-03T11:44:20.987Z
2020-12-03T11:44:20.987Z
Nilay Ghosh
<p>The surface is freezing-nitrogen cold, but it's typical for the temperature to increase towards the core. What's the temperature of the <em>core</em> of Pluto? Is the <s>planet</s> icy and rocky all the way through? I wonder at the possibility if that frozen ice ball could have any internal heat at all?</p>

CC BY-SA 4.0
2020-11-27T13:56:43.340Z
Remember, Pluto isn't very big. Its mass is < 0.18 the mass of our Moon, and its radius about 0.67 the Moons radius. And of course it gets much less solar heating.
PM 2Ring
CC BY-SA 4.0
2020-11-27T21:32:11.677Z
The core of the moon is about 1400C https://www.space.com/18175-moon-temperature.html You might expect Pluto's to be above vacuum temp. But at 0.2 of Earth rather than 1.2, & with much less heating, proportionately lower. I remember reading that when the sun explodes Earth's core will have only cooled a few degrees, so there will still be seismic activity. Because the mantle acts as a great insulator, & the core is very dense & hot to start with. But that will vary with the cube of radius..
CriglCragl
CC BY-SA 4.0
2020-11-28T03:43:48.327Z
[Life inside Pluto? Hot birth may have created internal ocean on dwarf planet](https://theconversation.com/life-inside-pluto-hot-birth-may-have-created-internal-ocean-on-dwarf-planet-140976) They don't mention a temperature and the cited paper is paywalled.
Keith McClary
CC BY-SA 4.0
2020-11-28T04:14:11.533Z
A couple more speculative papers: https://arxiv.org/pdf/1510.06604.pdf , https://www.popsci.com/pluto-ocean-insulation/
Keith McClary
CC BY-SA 4.0
2020-11-28T06:56:14.053Z
@CriglCragl The Sun cannot explode because it by far hasn't enough mass to go supernova. You probably mean the ejection of its planetary nebula, becoming a white dwarf.
Greenhorn
CC BY-SA 4.0
2020-12-03T12:55:03.610Z
@CriglCragl I though the moon's core was hotter but that's still quite hot
user random numbers
<temperature><pluto><core>
What's the temperature of Pluto's core?
user random numbers
# What's the temperature of Pluto's core?

(Asked by: username_0 on 2020-11-27)

The surface is freezing-nitrogen cold, but it's typical for the temperature to increase towards the core. What's the temperature of the *core* of Pluto? Is the ~~planet~~ icy and rocky all the way through? I wonder at the possibility if that frozen ice ball could have any internal heat at all?

**Tags:** temperature, pluto, core
> **Comments:**
> **username_1**: Remember, Pluto isn't very big. Its mass is < 0.18 the mass of our Moon, and its radius about 0.67 the Moons radius. And of course it gets much less solar heating.  
> **username_2**: The core of the moon is about 1400C https://www.space.com/18175-moon-temperature.html You might expect Pluto's to be above vacuum temp. But at 0.2 of Earth rather than 1.2, & with much less heating, proportionately lower. I remember reading that when the sun explodes Earth's core will have only cooled a few degrees, so there will still be seismic activity. Because the mantle acts as a great insulator, & the core is very dense & hot to start with. But that will vary with the cube of radius..  
> **username_3**: [Life inside Pluto? Hot birth may have created internal ocean on dwarf planet](https://theconversation.com/life-inside-pluto-hot-birth-may-have-created-internal-ocean-on-dwarf-planet-140976) They don't mention a temperature and the cited paper is paywalled.  
> **username_3**: A couple more speculative papers: https://arxiv.org/pdf/1510.06604.pdf , https://www.popsci.com/pluto-ocean-insulation/  
> **username_4**: @CriglCragl The Sun cannot explode because it by far hasn't enough mass to go supernova. You probably mean the ejection of its planetary nebula, becoming a white dwarf.  
> **username_0**: @CriglCragl I though the moon's core was hotter but that's still quite hot  

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## 1 answers

### Answer by username_5 on 2020-12-03. Score: 9 | Accepted answer

**TL;DR**: 1000 K (according to differentiated model of Pluto)

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According to the density value of Pluto, astronomers proposed three types of structural models:

1. Undifferentiated or "cold" model: rocks mixed with water-ice
2. Differentiated or "hot" model: rocky core and water-ice mantle
3. Rocky core only (temperature high enough to boil off water-ice.

There are two types of rocks to consider i.e. CI rock- carbonaceous chondrite($\rho$ = 2.66g/cm3) for undifferentiated models which is $\approx$13% by wt. eposomite(MgSO4) and Prinn-Frigley rock($\rho$ = 3.262 g/cm3) for differentiated models which is sulfide-rich rocks like troilite(FeS).

McKinnon and Parmentier(1986); McKinnon and Mueller(1988) correctly predicted the structural model of Pluto to be differentiated one. During initial formation of Pluto, radiogenic heating was the only source of heat, hot enough to melt the outside part of the undifferentiated core consisting of hydrated CI-rocks to form liquid matter of what is known today as water-ice in the mantle (water-ice melting temperature was 251 K at 0.21 GPa). During that time, 80% of core was at above 500 K . The anhydrous silicate core at the center was still rigid resisting the outside flow (the temperature of core was 500 K). Convection through heating allowed steady-state heat flow to form water-ice in the mantle, some of which erupted into the surface. Although the gravitational potential energy was modest, the process become self-accelerating.

This process was also accelerated by the "accretion process" due to a large-body impact that resulted in the formation of Charon. This collision heated up the core by 100 K and also resulted in several differentiation of Pluto that made the surface level ice layer mixed with organic compounds.

*Present day scenario:* Pluto is a rock-rich world with rock mass fraction $\gtrsim$ 60%. **Core temperature is 1000 K**, surrounded by 250-300 km thick mantle shell of predominately water-ice and mixed liquid rock. Surface temperature is 40 K. Core pressure is 1.1-1.4 GPa. Rock fraction (rock/rock+H2O+ice) for differentiated Pluto is 0.69-0.79(mainly PF-rock). There is also an extra thermal boundary layer between the ice-mantle and the ice-rock layer just outside the core. There might also be an organic layer in between the core and mantle but it hasn't been proven yet. The water-ice mantle is differentiated into several layers based on its transitions. You can check the details and calculation in ref.2

[![enter image description here](https://i.sstatic.net/c9zwv.png)](https://i.sstatic.net/c9zwv.png)

Fig. 1: Temperature of Pluto at several Pressure value

[![enter image description here](https://i.sstatic.net/E3wE2.png)](https://i.sstatic.net/E3wE2.png)

Fig. 2: Temperature of the mantle and outside layer

[![enter image description here](https://i.sstatic.net/JaALL.png)](https://i.sstatic.net/JaALL.png)

Fig.3: Differentiated model of Pluto

References:

1. <http://articles.adsabs.harvard.edu//full/1988LPI....19..764M/0000764.000.html>
2. Pluto and Charon, Alan Stern, David James Tholen, University of Arizona Press, 1997
3. <https://arxiv.org/ftp/arxiv/papers/1510/1510.06604.pdf> (This paper discusses the possibility that Pluto might have an iron core)


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