OrbHab>Spacesettlers
Re: Bruce Dunn's table of rocket-fuel densities at yarchive (was Resources are)
# 12383 byhitssquad@... on March 26, 2012, 5:16 p.m.
Member since 2021-10-03
--- In spacesettlers@yahoogroups.com, Ian Woollard wrote:
> On 22 March 2012 00:46, Al Globus wrote:
> > H2/O2 is the bets rocket fuel.
> Actually, no. The optimum for launch is a tripropellant system where the mixture varies over the launch.
Yes. More on fuel densities, from yarchive:
http://yarchive.net/space/rocket/fuels/fuel_table.html
Notice the difference between hydrogen at 20 degrees Kelvin vs. propane at 100 degrees Kelvin. The hydrogen, even though it has to be kept at a much lower temperature, has a density of only 70 kg/m^3, whereas the Propane, which can be brought down to 100 degrees Kelvin simply by putting it in contact with a liquid oxygen tank, has a density of 782 kg/m^3 -- more than 11x the density of liquid hydrogen.
From: Bruce Dunn
Newsgroups: sci.space.policy
Subject: Re: Kerosene vs Hydrogen fuelled SSTO rockets
Date: Sun, 09 Feb 1997 09:10:58 -0800
With respect to the subject of this thread, the choice of fuels for an SSTO isn't just between kerosene and hydrogen. A number of other fuels are quite reasonable alternatives. I reproduce below a cleaned-up version of a post I recently made in sci.space.tech on the subject:
A number of alternate fuels have been proposed for use with liquid oxygen. Here are some characteristics of these propellant combinations, in comparison with the standard fuels hydrogen and RP-1 (Rocket Propellant 1 = kerosene). I have only included fuels with an Isp greater than that of RP-1, and have ignored exotics like boranes. See the table notes at the end of the article for details of how the calculations were done.
Tank Fuel Bulk Vac.
Temp Formula MR Dens. Dens. Tc Isp
K O/F kg/m^3 kg/m^3 K 100:1
NON-HYDROCARBONS
hydrogen, NBP 20 H2 6.0 70 358 3610 455.9
UDMH, RT 298 C2H8N2 1.6 786 972 3710 365.4
ALKANES
methane, NBP 112 CH4 3.0 423 801 3589 368.3
ethane, NBP 184 C2H6 2.7 544 880 3671 364.6
propane, NBP 231 C3H8 2.7 582 905 3734 361.9
propane, 100K 100 C3H8 2.7 782 1014 3734 361.9
butane, NBP 273 C4H10 2.6 573 894 3734 360.9
RP-1, RT 298 C12H24 2.5 820 1026 3803 354.6
UNSATURATED HYDROCARBONS
ethylene, NBP 169 C2H4 2.3 569 874 3888 366.9
propylene, NBP 225 C3H6 2.3 611 903 3842 364
1,2-butadiene, NBP 284 C4H6 2.1 645 914 3982 363.5
1,3-butadiene, NBP 269 C4H6 2.1 614 893 3917 359.4
methylacetylene, NBP 250 C3H4 1.9 671 919 4034 366.9
Hydrogen has an excellent Isp but a rotten bulk density. RP-1 gives an excellent bulk density, but a much lower Isp. There are a number of alternate propellants shown in the table which fall somewhere between the two, having a slightly higher Isp than RP-1 but a lower bulk density.
UDMH (unsymmetrical dimethyl hydrazine) is normally used mixed with straight hydrazine (N2H4) and is normally burned with N2O4 as an oxidizer. It burns perfectly well however with liquid oxygen, and is a superior fuel provided one can tolerate its toxicity and cost.
The light alkanes are all readily available in industrial quantities, are good coolants. Going from RP-1 to methane gains 3.8 % in Isp, but costs about 22% in density. Other alkanes lie between the performance of methane and RP-1.
Propane at room temperature is a non-starter for pump fed engines, as its vapor pressure is too high for light weight tanks. Propane is unusual in that it will not freeze solid if put in tanks in thermal contact with LOX tanks; it has been proposed therefore to use sub-cooled propane. Calculations done here show both propane at its normal boiling point, and at 100 K, about 10 K above LOX temperature. Sub-cooled propane (at LOX temperatures or slightly above to account for imperfect chilling of propane by adjacent LOX tanks) is a winner, with a bulk density nearly the same as that of RP-1, and a superior Isp.
The light unsaturated compounds are also readily available in industrial quantities. These compounds may possibly give polymerization problems when used for engine cooling, but again, they may not (particular those which are very cold to start with may not warm up enough to cause problems). They don't seem to be superior enough to alkanes to make their use worth while, particularly considering that they generally have higher chamber temperatures than for alkanes with the same Isp.
Table Notes:
Isp calculations were performed on a partial equilibrium basis, assuming that recombination reactions stop at the nozzle throat (an approximation of real world behavior). Isp values are theoretical values for 100:1 expansion into vacuum, and assume a chamber pressure of 20 MPa (approximately 2900 psi). These conditions are representative of a high pressure, high expansion ratio engine that might be used for an SSTO.
Fuel storage temperature is generally at Normal Boiling Point (NBP) which is the temperature at which a fuel will equilibrate at if tanks are vented to the atmosphere during filling. Exceptions are RP-1 and UDMH at Room Temperature (298 K), and one calculation in which propane is chilled to 100 K, about 10 K above its freezing temperature.
Mixture ratios (MR) are expressed as the mass of oxidizer divided by the mass of the fuel (O/F). The MRs given are the optimum for maximal Isp, except for H2 which is calculated at a mixture ratio of 6:1, rather than the more optimal 4.4 which would give a higher Isp, but a much poorer bulk density.
Fuel densities are the density in the fuel tanks. Bulk density is the overall density of the propellant combination, with the stated mixture ratio and oxygen at a density of 1140 kg/m^3.
Tc is the chamber temperature - it is higher for unsaturated hydrocarbons than for alkanes, as the former have energy locked up in the structure of their molecules which adds to the energy available from oxidation.
RP-1 is shown with a molecular formula of C12H24 ; this is an approximation to something like the average molecular formula (RP-1 has an H to C ratio of approximately 2, and an average molecular weight somewhere near that of hexadecane, C12H26)
Dr. Bruce Dunn
General Astronautics Canada, Vancouver B.C.
http://www.genastro.com/ | 800-577-1117 | 604-876-7640
Reliable, low-cost transportation to low Earth orbit and beyond

# 12384 byian.woollard@... on March 27, 2012, 1:03 a.m.
Member since 2021-10-03
Yes, there's more about this and more on his website:
On 26 March 2012 18:16, hitssquad wrote:
> --- In spacesettlers@yahoogroups.com, Ian Woollard wrote:
> > On 22 March 2012 00:46, Al Globus wrote:
> > > H2/O2 is the bets rocket fuel.
> > Actually, no. The optimum for launch is a tripropellant system where the
> mixture varies over the launch.
>
> The reason is that hydrogen has poor density, so the tankage, pumps and
> pipe mass is very high for any given thrust level; so you are better off
> running with dense fuel early on
>
> Yes. More on fuel densities, from yarchive:
> http://yarchive.net/space/rocket/fuels/fuel_table.html
>
> Notice the difference between hydrogen at 20 degrees Kelvin vs. propane at
> 100 degrees Kelvin. The hydrogen, even though it has to be kept at a much
> lower temperature, has a density of only 70 kg/m^3, whereas the Propane,
> which can be brought down to 100 degrees Kelvin simply by putting it in
> contact with a liquid oxygen tank, has a density of 782 kg/m^3 -- more than
> 11x the density of liquid hydrogen.
>
> From: Bruce Dunn
> Newsgroups: sci.space.policy
> Subject: Re: Kerosene vs Hydrogen fuelled SSTO rockets
> Date: Sun, 09 Feb 1997 09:10:58 -0800
>
> With respect to the subject of this thread, the choice of fuels for an
> SSTO isn't just between kerosene and hydrogen. A number of other fuels are
> quite reasonable alternatives. I reproduce below a cleaned-up version of a
> post I recently made in sci.space.tech on the subject:
>
> A number of alternate fuels have been proposed for use with liquid oxygen.
> Here are some characteristics of these propellant combinations, in
> comparison with the standard fuels hydrogen and RP-1 (Rocket Propellant 1 > kerosene). I have only included fuels with an Isp greater than that of
> RP-1, and have ignored exotics like boranes. See the table notes at the
> end of the article for details of how the calculations were done.
>
> Tank Fuel Bulk Vac.
> Temp Formula MR Dens. Dens. Tc Isp
> K O/F kg/m^3 kg/m^3 K 100:1
>
> NON-HYDROCARBONS
> hydrogen, NBP 20 H2 6.0 70 358 3610 455.9
> UDMH, RT 298 C2H8N2 1.6 786 972 3710 365.4
>
> ALKANES
> methane, NBP 112 CH4 3.0 423 801 3589 368.3
> ethane, NBP 184 C2H6 2.7 544 880 3671 364.6
> propane, NBP 231 C3H8 2.7 582 905 3734 361.9
> propane, 100K 100 C3H8 2.7 782 1014 3734 361.9
> butane, NBP 273 C4H10 2.6 573 894 3734 360.9
> RP-1, RT 298 C12H24 2.5 820 1026 3803 354.6
>
> UNSATURATED HYDROCARBONS
> ethylene, NBP 169 C2H4 2.3 569 874 3888 366.9
> propylene, NBP 225 C3H6 2.3 611 903 3842 364
> 1,2-butadiene, NBP 284 C4H6 2.1 645 914 3982 363.5
> 1,3-butadiene, NBP 269 C4H6 2.1 614 893 3917 359.4
> methylacetylene, NBP 250 C3H4 1.9 671 919 4034 366.9
>
> Hydrogen has an excellent Isp but a rotten bulk density. RP-1 gives an
> excellent bulk density, but a much lower Isp. There are a number of
> alternate propellants shown in the table which fall somewhere between the
> two, having a slightly higher Isp than RP-1 but a lower bulk density.
>
> UDMH (unsymmetrical dimethyl hydrazine) is normally used mixed with
> straight hydrazine (N2H4) and is normally burned with N2O4 as an oxidizer.
> It burns perfectly well however with liquid oxygen, and is a superior fuel
> provided one can tolerate its toxicity and cost.
>
> The light alkanes are all readily available in industrial quantities, are
> good coolants. Going from RP-1 to methane gains 3.8 % in Isp, but costs
> about 22% in density. Other alkanes lie between the performance of methane
> and RP-1.
>
> Propane at room temperature is a non-starter for pump fed engines, as its
> vapor pressure is too high for light weight tanks. Propane is unusual in
> that it will not freeze solid if put in tanks in thermal contact with LOX
> tanks; it has been proposed therefore to use sub-cooled propane.
> Calculations done here show both propane at its normal boiling point, and
> at 100 K, about 10 K above LOX temperature. Sub-cooled propane (at LOX
> temperatures or slightly above to account for imperfect chilling of propane
> by adjacent LOX tanks) is a winner, with a bulk density nearly the same as
> that of RP-1, and a superior Isp.
>
> The light unsaturated compounds are also readily available in industrial
> quantities. These compounds may possibly give polymerization problems when
> used for engine cooling, but again, they may not (particular those which
> are very cold to start with may not warm up enough to cause problems). They
> don't seem to be superior enough to alkanes to make their use worth while,
> particularly considering that they generally have higher chamber
> temperatures than for alkanes with the same Isp.
>
> Table Notes:
>
> Isp calculations were performed on a partial equilibrium basis, assuming
> that recombination reactions stop at the nozzle throat (an approximation of
> real world behavior). Isp values are theoretical values for 100:1 expansion
> into vacuum, and assume a chamber pressure of 20 MPa (approximately 2900
> psi). These conditions are representative of a high pressure, high
> expansion ratio engine that might be used for an SSTO.
>
> Fuel storage temperature is generally at Normal Boiling Point (NBP) which
> is the temperature at which a fuel will equilibrate at if tanks are vented
> to the atmosphere during filling. Exceptions are RP-1 and UDMH at Room
> Temperature (298 K), and one calculation in which propane is chilled to 100
> K, about 10 K above its freezing temperature.
>
> Mixture ratios (MR) are expressed as the mass of oxidizer divided by the
> mass of the fuel (O/F). The MRs given are the optimum for maximal Isp,
> except for H2 which is calculated at a mixture ratio of 6:1, rather than
> the more optimal 4.4 which would give a higher Isp, but a much poorer bulk
> density.
>
> Fuel densities are the density in the fuel tanks. Bulk density is the
> overall density of the propellant combination, with the stated mixture
> ratio and oxygen at a density of 1140 kg/m^3.
>
> Tc is the chamber temperature - it is higher for unsaturated hydrocarbons
> than for alkanes, as the former have energy locked up in the structure of
> their molecules which adds to the energy available from oxidation.
>
> RP-1 is shown with a molecular formula of C12H24 ; this is an
> approximation to something like the average molecular formula (RP-1 has an
> H to C ratio of approximately 2, and an average molecular weight somewhere
> near that of hexadecane, C12H26)
>
> --
> Dr. Bruce Dunn
> General Astronautics Canada, Vancouver B.C.
> http://www.genastro.com/ | 800-577-1117 | 604-876-7640
> Reliable, low-cost transportation to low Earth orbit and beyond
>
--
-Ian Woollard