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On an extended spaceflight in Starship, the liquid propellant and oxidizer will tend towards the same temperature. The tanks can be refrigerated by boiling off contents, but your mileage may vary doing that. The tanks might be warmed by rotating the ship. But you are still stuck with both tanks being the same temperature inside.

Attached is a phase diagram of oxygen and methane. There is a narrow temperature gap between solidified Methane and tank-rupturing Oxygen pressure. Of course, the boiled O2 could just be vented. But where's the fun in launching liquid O2 just to boil it off?

I can see Starship running out of Helium, cold cranking those turbines as Mars looms ahead.

These diagram graphics are from Engineering Toolbox. I’ve edited them so the horizontal axes (temperature) line up. It appears there is only a 12 °C gap between the freezing point of methane and the temperature where the vapor pressure of oxygen exceeds the safe working pressure of the Starship tank wall (6 bar).

enter image description here

It would be tricky to maintain tank temperature within this band using only passive means. The shiny side of Starship is uninsulated and low emissivity. The heat shield side is heavily insulated and high emissivity. I suspect that cooling the tanks would be easy since the shaded side would try equilibrate with the cosmic background radiation temperature (2.7 K). But it would be difficult to acquire heat from the sunny side due to the low emissivity of stainless steel on the shiny part of the hull, and the high insulation of the heat shield on the other side of the hull.

Woody
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    It looks like you have something severely wrong with your oxygen plot. Oxygen's critical point is at about 50 bar, but you have it somewhere in the neighborhood of 10^5 bar. You have its triple point far too high as well. Oxygen's boiling point and methane's melting point are nearly the same at 1 bar. – Christopher James Huff Oct 22 '21 at 00:09
  • There are shared bulkheads with thermal insulation, for instance the second stage of Saturn V – Uwe Oct 22 '21 at 00:25
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    Your basic premise is true, but to a vastly lesser point than your diagram seems to think. At 1 bar, Oxygen boils at -183C, and Methane freezes at -182C. That's not very horridly incompatible!! The diagram makes a LOT more sense if you use a phase diagram for Oxygen that uses the same vertical scale as the Scale of the Methane diagram! – CuteKItty_pleaseStopBArking Oct 22 '21 at 01:17
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    Thanks for pointing out the error. Very sloppy of me. I have edited the original posting, including Engineering Toolbox data. I was wrong that there was "no overlap" in liquid state between oxygen and methane. I corrected this to a "narrow overlap". I can't figure out how to edit the original question. It should be, "There is a narrow overlap in temperature/pressure in which oxygen and methane are both liquid. Is this a problem for using this fuel duo for interplanetary travel, particularly in the Starship as presently conceived?" – Woody Oct 23 '21 at 02:51
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    "The shiny side of Starship is uninsulated and very low emissivity".. Ok, as what did you take the emissivity of the 304L stainless that StarShip is made of? Asking because the emissivity of stainless can vary from 0,004 to 0.93, depending on the metal specific formulation, the surface roughness, surface contaminants, and the exact level of polishing applied. Frankly, I have no idea of the emissivity of Starship, but as its reflectivity is only mediocre(it's best described as somewhat shiny grey), the emissivity cannot be very far from 0.5 either. – CuteKItty_pleaseStopBArking Oct 23 '21 at 05:11
  • Very good points. The surface treatment of metals has a large effect on the emissivity, so surface treatment becomes a engineering decision for thermoregulation. – Woody Oct 23 '21 at 18:48
  • The visual appearance of a surface correlates poorly with its emissivity because visible light is a small part of the Black Body spectrum. For instance, soil and snow both have emissivity >0.90. I suspect off-the-roll 304 has the emissivity of polished SS, about 0.08. It could be much higher after being “weathered” in the solar wind. https://www.engineeringtoolbox.com/emissivity-coefficients-d_447.html . If the surface is engineered, it could likely have emissivity above 0.90. – Woody Oct 23 '21 at 18:48
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    I can just see Starship running out of Helium Hard to run out of something you don't launch with! Operational starships will use autogenous pressurization for their tanks and RCS, heating the propellants if necessary to produce boil-off and increase pressure rather than relying on helium or any other pressurant. Mars' atmosphere does have some He, but it's better not to need to re-tank an additional fluid (also, it's getting very expensive even here on earth) – CBHacking Oct 24 '21 at 23:25
  • Can i suggest you rephrase this question, or even scrap it completely and redo? The main question title contains a since-proven incorrect fact. – CuteKItty_pleaseStopBArking Oct 25 '21 at 01:13
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    nice fixing of both title and content. – CuteKItty_pleaseStopBArking Oct 28 '21 at 12:48
  • Re: StarShip running out of Helium on re-start. I understood the engine start procedure used helium to spool up the pump impellers before the pre-burners ignited. If they don't use Helium for re-starts, how do they crank over the pumps? The propellant tanks can be pressurized (to 6 bar) with boil-off, but this is unlikely enough pressure for the re-starting job since the pre-burner pump impeller chamber usually operates at 512 bar.. – Woody Oct 30 '21 at 00:14

2 Answers2

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Starship will be re-tanked in Earth Orbit. During this time it will be possible to cool the propellants via boil off and orientation of the ship relative to the Sun and the Earth. The main tanks can be topped off from a tanker immediately before departure. The trans Mars injection will use virtually all of the propellants in the main tanks and any residue will be vented to space leaving two separate full header tanks that do not share a common bulkhead.

The propellants in the header tanks will be used to land on Mars. cryocoolers and A boil off margin can be allowed during the re-tanking operation using ISRU on Mars. After launch from Mars the main tanks will again be vented into space leaving the header tanks full.

Slarty
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  • Thanks for the great answer. I was not aware of the mission propellant use profile. Can you share a reference so I can learn more? – Woody Oct 26 '21 at 16:23
  • Unfortunately I am not able to provide a reference at the moment. This was from memory based on extensive discussions from these threads: https://forum.nasaspaceflight.com/index.php?board=72.0 I will see if I can find it – Slarty Oct 27 '21 at 16:26
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NASA solved that problem of differing boiling/cooling points when they designed Saturn V. They used an insulated core wall to hold differing materials. enter image description here

LazyReader
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