Feasibility of Cloud Nine
I did some exploration into this idea and thought I'd share my results here. TL;DR at the bottom.
In this answer, I attempt to explore the feasibility of a Cloud Nine style airborne habitat.
I’ll look at:
- modeling atmospheric conditions for different altitudes;
- calculating buoyancy & lift;
- estimating the mass of the geodesic tensegrity superstructure;
- estimating the mass of the the envelope/membrane;
- optimal operating altitudes;
- building a model Cloud Nine;
- energy requirements, solar-thermal input, and losses to waste heat;
- and interior architecture for buildings and living structures.
First, I’ll describe some of the equations and methods I’ll use, then I’ll apply them to build a model Cloud Nine and inspect its feasibility.
Atmosphere Model
From NASA’s document on U.S. Standard Atmosphere, I get the following formula for modeling barometric pressure at various height regimes:
$$P=P_{b}\exp\left(\frac{-g_{0}M_{air}\left(h-h_{b}\right)}{RT_{b}}\right)$$
- $P_b$ = reference pressure [Pa]
- $T_b$ = reference temperature [K]
- $h$ = height at which pressure & density are calculated [m]
- $h_b$ = height of reference level (meters; hb = 11,000 m)
- $R$ = universal gas constant: 8.3144598 J/(mol·K)
- $g_0$ = gravitational acceleration: 9.80665 m/s^2
- $M_{air}$ = molar mass of Earth’s air: 0.0289644 kg/mol
Next, from the same source, I get the the following formula for modeling atmospheric density:
$$d=d_{b}\exp\left(\frac{-g_{0}M_{air}\left(h-h_{b}\right)}{RT_{b}}\right)$$
- $d_b$ = reference density [kg/m^3]
From the table supplied in the paper, I use the pressure & temperature reference values calculated for heights less than 11,000 m:
- $h_b$ = 11,000 m
- $P_b$ = 22,632.10 Pa
- $T_b$ = 216.65 K
- $d_b$ = 0.36391 kg/m^3
To model temperature, I use this approximation from NASA for temperatures at heights less than 11,000 m, adjusted for units in Kelvin:
$$T=288.19-0.00649h$$
(It's surprisingly accurate, compared against empirical data I was using before it.)
Buoyancy & Lift Equations
The buoyant force of an airship, regardless what mixture is used within the envelope, is the difference in densities between interior and exterior, multiplied by the volume of the balloon, multiplied by gravitational acceleration:
$$F_{b}=\left(d-d_{i}\right)\cdot V_{sphere}\cdot g_{0}$$
I calculate the external density, temperature, and pressure using my model atmosphere, and the internal density using the Ideal Gas Law:
$$P=\frac{d_i}{M_{air}}RT$$
Rearranging, we get:
$$d_{i}=\frac{PM_{air}}{RT}$$
where:
- $d_i$ = internal density [kg/m^3]
- $P$ = atmospheric pressure [Pa]
- $T$ = desired internal temperature [K]
- $M_{air}$ = mean molar mass of Earth’s air: 0.0289644 kg/mol
- $R$ = universal gas constant: 8.3144598 J/(mol·K)
From the equations, we can see that our options for increasing the density differential (thereby increasing buoyancy) are increasing either the pressure or temperature differentials. Building a multi-kilometer-wide pressure vessel sounds annoying compared to just heating the interior up, so I’ll go with the latter. This means I'll use the outside pressure from the atmosphere model for the internal pressure of the balloon.
Geodesic structural mass
The formula to calculate the various strut lengths of a geodesic sphere is actually pretty simple. You just need the chord factors, the number of strut members for each given factor, and the sphere radius. Chord factors are constants that pop out in unit space and remain identical no matter how you resize the structure or what your units are, like angles. Each chord factor is resized according to the sphere/dome radius, and multiplied by the number of struts per strut type (A-I). You can find those figures and also a handy calculator here. I’ll be using the values for a 6V geodesic sphere.

total strut length [m] = sphere radius [m] * chord factor * NOF strut members
total combined length [m] = sum( total strut length [A - I] [m] )
Alternatively, using math from this paper, you can calculate the total combined strut length of a geodesic icosahedron, $L_{total}$, using the following equations:
$$S_{PCF}=2\sum_{a=1}^{f}\sum_{b=1}^{a}f_{PCF}\left(a,b\right)$$
$$f_{PCF}\left(a,b\right)=2\sin\left(\frac{1}{2}\operatorname{arccot}\left(t\left(a\right)+\left(\frac{a}{2}-b\right)\left(\frac{a}{2}-b+1\right)t\left(a\right)^{-1}\right)\right)$$
$$t\left(a\right)=\frac{1}{2}\sqrt{\left(f-a\right)\left(f-3a\right)+f^{2}\cot^{2}\left(\frac{\arctan\left(2\right)}{2}\right)}$$
$$L_{total}=20S_{PCF}\cdot r_{sphere}$$
where:
- $f$ = chord frequency (1, 2, 3,...)
- $r_{sphere}$ = radius of the sphere
To estimate the mass of the total structure, take the total combined length of all the strut types (A-I) and, treating them as cylindrical spars of a certain radius, compute their volume and multiply by the chosen material’s density.
volume [m^3] = pi * strut radius^2 [m^2] * combined length [m]
mass [kg] = volume [m^3] * density [kg/m^3]
Cloud Nine is a tensegrity structure with “floating compression” members. The calculation I’ve just shown is for the mass of the compression members. What I’m missing is the mass of the tension members, e.g., cables. I’m not sure how to find the lengths of those mathematically, but, as a rough approximation, we can just double the result of the mass of the compression members. It’s likely way off because, for certain ultimate stresses, tension members are usually less massive than compression members (think cables versus I-beams). It usually takes more to pull something apart than to crumple it up. The way I see it, doubling the compression member mass is a very conservative estimate. As we’ll see later, we have a lot of lift-mass to play with, anyway.
Envelope/Membrane Mass
Finding envelope mass is as simple as multiplying the surface area by the thickness of the membrane, getting an approximate volume, then by material density.
envelope mass [kg] = surface area [m^2] * thickness [m] * material density [kg/m^3]
I could calculate the volume of a spherical shell instead, which would be more accurate, but for large-scale objects like Cloud Nine with paper-thin skins, the difference is beyond negligible.
Optimal Altitude for Flight
For populated, non-pressurized Cloud Nines, I figure the maximum altitude will be around the highest elevation humans tolerate living at. The highest-elevation urban settlement in the world is La Rinconada, Peru, with 30,000 residents at 16,700 ft (5,100 m), living at half standard pressure. Cloud Nine appears to function even better at higher altitudes than this, but for the sake of comfort, I’ll stop there. The optimal altitude for maximum buoyancy is probably where the ratio of air density to ambient temperature is greatest (when we are constrained to a steady-state internal temperature).
Basically, there comes a point along increasing altitude where density begins falling faster than temperature, and we start losing buoyancy. At best guess, I'd say that point could be as high as 40 km.
Building a model Cloud Nine
Using the equations above, let’s construct a Cloud Nine tensegrity sphere with the following properties:
- Sphere diameter: 2,000 m (1.24 mi)
- Height above sea level: 5.1 km, elevation of La Rinconada, Peru
- Internal temperature: 300 K (80 F)
The atmospheric conditions at 5,100 m are:
- Pressure: 57,380 Pa
- Temperature: 255.1 K
- Density: 0.923 kg/m^3
Our 2 km wide Cloud Nine has an internal density of 0.67 kg/m^3, creates a density differential of 0.26 kg/m^3, and exhibits a buoyant force of over 10.5B N, or a “lift-mass” of over 1B kg or 1M metric tonnes. The mass of the supporting superstructure needs to be less than that to maintain buoyancy at 5.1 km altitude. Indeed, it needs to be a lot less than that to support the mass of a whole “village”. Let’s look at that.
Running through the geodesic strut calculations, we arrive at a total material length of 215,780 m of struts. If we use Aluminum alloy 6061, with density 2,700 kg/m^3, as our construction material (known for its low density and being a common “aircraft aluminum”, see here), and if each strut is 20 cm in diameter, then we calculate a total mass of ~18,300 metric tonnes for the compression members.
Assuming the tension members weigh just as much (which they likely don’t, but let’s be generous), we double that figure to get ~36,600 metric tonnes for the geodesic tensegrity skeleton. (There are many options to explore for the compression and tension member materials--way too many.)
Most blimps use Kevlar as a membrane material for its properties of low density and high tensile strength. According to this table, Kevlar has a density of 1,440 kg/m^3. According to this Goodyear study, most blimps have a Kevlar membrane thickness between 0.5 mm and 4 mm. I’ll use the lowest value, choosing 0.5 mm. Doing the math, we get an envelope mass of ~9,000 metric tonnes. Choosing 2 mm would bring the mass up to around the mass of the tensegrity superstructure itself at ~36,000 tonnes.
The total mass of the geodesic tensegrity sphere + Kevlar envelope is around ~47,000 metric tonnes. A tiny divet into our lift-mass budget of over 1M tonnes. Our Cloud Nine can lift over 22.5 times its own structure’s mass, or over 23 Lexington-class battlecruisers. If each inhabitant on average requires 10 tonnes of material (ballpark figure), then the sphere can carry over 100,000 people. Definitely a village’s worth.
Losses to Black-Body Radiation
To find the power requirements of the internal heat engines I find the energy lost via transmittance through the Kevlar membrane, which represents the energy that needs to be added back into the system to maintain a steady-state temperature condition. For that, I look at the thermal transmittance of the entire Cloud Nine. The paper-thin Kevlar envelope has a thermal conductivity of 0.04 W/(m•K) (source). Dividing by our chosen membrane thickness of 0.5 mm gives us its thermal transmittance U-factor of 80 W/(m^2•K). Cloud Nine will leak heat like nobody’s business.
I figure the envelope could be painted with a dark material, further insulated with a foam layer, or both to bring that value down to that of at least single-glazed glass at 5.7 W/(m^2•K).
thermal transmittance [W] = surface area [m^2] * U-factor [W/(m^2*K)] * (internal temp - external temp [K])
Crunching the numbers, we get a transmittance over the entire sphere’s surface of 3.22 GW. Yup, gigawatts. That’s how much power needs to be pumped back in to maintain our 300 K internal temperature. It shouldn’t be all that surprising considering the sheer quantity of air inside the sphere. Our insulation could be better than that of darkened glass. A well-insulated roof has a thermal transmittance of only 0.15 W/(m^2•K), which would drop the energy requirement into the megawatt range.
Gains from Solar Flux
The original Cloud Nine concept was made buoyant entirely by heat energy from the Sun. Let’s see how close I can get. According to this paper, Kevlar has a thermal absorptivity coefficient of 0.47. To find the solar energy absorbed, we multiply the solar irradiance times the surface area normal to the light rays times the (dimensionless) absorptivity coefficient.
solar input [W] = solar irradiance [W/m^2] * cross-sectional area [m^2] * absorptivity
Solar irradiance at sea level on a clear day is usually about 1,000 W/m^2, and that value only gets larger as you go higher due to there being less air between you and the top of the atmosphere to attenuate the Sun’s rays. I’ll just use 1,000 W/m^2 as a constant. Cranking the analytical engine, we get an input energy of ~1.5 GW when the Sun is out. Close to half of the 3.22 GW requirement for maintaining a 300 K internal temperature. We get some irradiance on the bottom of the sphere, too, reflected up from Earth’s surface, but for simplicity's sake I’ll ignore that.
We could improve the absorptivity of the envelope with a coat of paint, a different membrane material, or an additional layer of some high-absorption substance. With an improvement in insulation, the gains in efficiency could drastically reduce the power requirements and the mass of the heat engines.
Out of curiosity, I rearranged the thermal transmittance equation to find the steady-state temperature with solar irradiance alone. I calculate the Sun will heat our Cloud Nine sphere up to ~275.7 K. Plugging that into the buoyancy equations as our new internal temperature, we can find the new free lift-mass after subtracting the structure mass: ~780,000 metric tonnes. Cloud Nine can hover at 5.1 km altitude while carrying almost 18 Lexington-class battlecruisers without any energy input from onboard heat sources.
Power Station Requirements
Our power requirement during the day, when the Sun lifts some of our energy burdens, is 3.22 - 1.5 GW = ~1.72 GW. At night, depending on how well-insulated the structure is, the requirement may be the full 3.22 GW -- or it may be a fraction of that. Over 3 GW is the power output of a good-sized nuclear power station, so it’s probably worth the extra mass to cake on extra insulation, especially since it’s such a small proportion of our total lift-mass budget.
If we increase the insulation to that of a well-insulated roof, our power requirements drop to ~85 MW, far smaller than what we receive from solar energy. With that kind of insulation, we could warm up during the day and cool down at night while losing very little internal temperature and altitude, day by day, ad infinitum. 85 MW is about 40 Hoover dams, close to the output of some of the smallest nuclear reactors which usually bottom-out at a shameful 50 MW. If the nuclear reactor mass can be made as little 5-10 kg per kW, then the entire powerplant could weigh as little as 423-847 metric tonnes. If instead it is as high as 500 kg per kW, then the powerplant would weigh ~42,000 metric tons, about half an aircraft carrier or about as much as the geodesic tensegrity structure itself. We would still have much of the original 1M tonnes to work with for other structures.
With current battery technology as heavy as it is, storing excess power to any meaningful extent seems out of the question.
There may be the possibility of cladding the envelope with a thin solar array to more efficiently draw solar energy. Using figures from Space Future, “current best” aerospace solar cell arrays can reach 4,600 W/kg with a density of 30 g/m^2. Assuming protection against the environment reduces that by an order of magnitude, 460 W/kg, and assuming half the sphere is clad in the solar cell film, I get a total mass of ~200,000 kg and an input of ~87 MW. Not tremendous, but nothing to sneeze at either.
Another potential option is outrigging large mirrors or reflective foils to focus more sunlight onto collectors for internal heating, or outrigging wind turbines to collect wind power. With such a large cross-sectional area, space-based microwave beam power seems like an enticing option, and if fusion power could be realized and built small enough, that could potentially work too.
Interior Architecture
This section is a little less rigorous and is mainly just me guessing. We have approximately 1M tonnes to work with, mass enough for basically any number of people and structures. I assume we want to take advantage of how the tensegrity structure spreads tension forces over the surface of the sphere and hang everything inside on guy wires. There are plenty of material options for the necessary tensile strength. Structures and levels might be suspended like suspension bridges, with additional supports guarding against bad oscillations/resonances, shearing, and torques.
Conclusion
Cloud Nine seems possible.
I've calculated that a 2,000 m diameter tensegrity sphere, made of 20 cm diameter Aluminum 6061 spars and tension cables, enveloped in a 0.5 mm Kevlar membrane, masses ~47,000 metric tonnes. With an internal temperature of 300 K (80 F), at an altitude of 5.1 km, the sphere displaces over 1 million metric tonnes of air.
The sphere absorbs 1.5 GW of solar energy and naturally heats to an internal temperature of 275.7 K. With no energy input, the sphere can hover at 5.1 km altitude while carrying 780,000 metric tonnes of cargo, structures, and people. When heated to an internal temperature of 300 K, a well-insulated sphere radiates as little as 85 MW of power, requiring that much power during the nighttime to stay aloft. Conceivably, it wouldn't need any power input if the sphere were allowed to drop in altitude by a kilometer or two at night; however, a small nuclear reactor massing between 420 and 42,000 metric tons could supply the power, depending on W/kg assumptions. Conversely, a poorly-insulated sphere radiates as much as 3.22 GW and would require a major power station to stay aloft.
What I'm missing from my analysis is an estimate of the stresses across the structure. Samuel, another user, calculated the forces of a buoyant geodesic sphere in their answer, but not a tensegrity sphere. Reading through the other answers and comments, I’m not entirely sure where the major loads would be or how to estimate their magnitude. The general consensus that I've seen is that high-tensile strength materials would be enough. Fuller believed so, and he made his calculations in the 1950s with the materials available at the time.
From my geodesic strut calculations, the longest struts would be over 400 m in length, nearly 4x the size of the largest wind turbine blades. A larger geodesic chord number with a greater number of, yet on average smaller, struts might be needed, increasing the mass of the geodesic tensegrity skeleton, but offering less load on the compression members.