6.1. Defining the Thermal Load
The sun is an extremely powerful body of energy which will not only power the CubeSat’s electrical system but will also input radiation into nanosatellites “boundary conditions” as shown in
Figure 44 below.
The following estimates the value of direct solar flux from solar radiation [
10]:
The solar radiation intensity at any distance from the Sun can be found using the relationship:
This value of the solar constant ignores atmospheric attenuation. At an orbiting altitude of 600 km this value is assumed to be the same as at Earth’s surface.
Earth’s surface also reflects the incoming solar radiation from the Sun back into the atmosphere, known as Albedo Radiation. The albedo radiation is calculated using the following formula:
where a is the albedo, assumed to be 0.34 average for Earth. For open ocean, this value drops to 0.05 and rises to 0.6 for high cloud and icecaps. F is the visibility factor found from the following
Figure 45.
With an altitude of 600 km and Sun-synchronous orbit the Beta angle of this mission will be 0 degrees. The beta angle is the minimum angle between the orbit plane and the solar vector, which is permitted to vary between −90 to 90 degrees [
20]. The visibility factor is 1.05 as this value on
Figure 46 above corresponds to an altitude of 600 km and a Beta angle of 0 degrees. The beta angle can be calculated using the following formula (see
Figure 46) [
10]:
where:
,
,
,
The maximum albedo radiation would occur over high clouds and icecaps:
The Earth also emits planetary radiation which must be considered during CubeSat thermal design. The Earth emits infra-red radiation.
The observed values are as follows:
The value of planetary radiation at any altitude can be found at any altitude per the following formula:
In reality, this value of planetary radiation varies significantly throughout a day as shown on
Figure 47 below which presents experimental data of J values over a 3 h period from a spacecraft in LEO.
The intensity of incoming radiation from the Sun varies throughout Earth’s elliptical orbit and depends on the weather season on Earth. For example, in the Northern Hemisphere’s summer the intensity is 1372 W/m
2 and at the winter solstice the intensity reaches 1472 W/m
2. The intensity varies due to Earth’s elliptical orbit around the Sun, meaning the distance between the two bodies constantly alters. To estimate the Intensity of the radiation (solar constant) for any given day of the year the following formula may be implemented:
where
n is equal to the day number of the year, and
equals the current solar constant.
At an altitude of 600 km the environment is very radiative causing extreme temperature variations to the CubeSat’s components, particularly the outer surfaces. The background temperature of space at this altitude is 2.7 K. As stated earlier in the report, the pressure is of an extremely small magnitude at this orbit and is assumed to be negligible, assuming a vacuum. Temperatures of the outer surfaces of CubeSats are typically 100 degrees when facing the Sun’s radiation and −100 degrees when in Earth’s or CubeSat’s shadow.
This represents an extreme temperature range, at which the CubeSat’s subsystems would begin to fail towards the extremes, it is, therefore, necessary to regulate temperature to ensure components do not fail in such a harsh environment. The following table,
Table 27 details typically operational temperatures for key CubeSat subsystems.
The advantage of selecting a Sun-synchronous orbit is that the CubeSat’s orbit plane remains at a fixed angle relative to the Sun’s position [
10]. This is advantageous as every orbit the CubeSat completes is over locations on Earth which have the same local time, and as Earth is rotating too the craft can cover approximately the whole course of Earth in a day. This is very useful for the RAVAN payload as it can measure imbalance over all locations, highlighting hotspots and regions which produce more emissions which is extremely useful when developing climate control programs for greenhouse gas reduction [
9].
As the Beta angle for this mission is 0 degrees, the CubeSat will pass over the Sub-Solar Point of Earth. This location is where the Sun is directly overhead, has the most intense Albedo radiation value and has the longest eclipse time as the entirety of Earth’s diameter shadows it. As this angle increases, the Albedo load decreases as it is further from the SSP point, but as a trade off the CubeSat will be exposed to the Sun for a longer period of each orbit as the eclipse time reduces. When the beta angle reaches the maximum value of 90 degrees, there is no eclipse and the albedo load is negligible.
For an orbit between 0 and (−) 90 degrees, the eclipse fraction for the assumed circular orbit can be found using (
Figure 48 for illustration).
where:
Therefore, use is valid as 0 < 73.4.
However, once the period for orbit has been calculated, a much more concise method can be implied to determine the time spent in eclipse and the time spent in direct solar radiation. The period is found using the following equation:
Assuming the satellite orbits in a circular motion, and Earth’s shadow causing eclipse is cylindrically shaped, the following formula can be employed to find the time spent in eclipse.
where α equals:
During the CubeSat’s 96 min 30 s orbit, approximately 35 min and 38 s will be spent in the shade cooling due to net heat dissipation as the CubeSat will only be exposed to a very small amount of radiation as no direct sunlight will contact the body and the body would attempt to reach thermal equilibrium with the 3 K background space temperature. However, for the remaining 60 min and 52 s the CubeSat will be exposed to intense solar radiation which will raise component temperatures potentially causing mission failure. It is vital to select materials and develop temperature regulation system to prevent this from occurring.
Heating of the CubeSat will occur through 3 thermodynamic transfer mechanisms, conduction, convection, and radiation. Convection can be classed as negligible for this system, as the atmosphere is extremely thin meaning very little particle mass is available to drive this process.
Per the Zeroth Law, energy will always flow from a region of high temperature to a region of low temperature to reach equilibrium. This heat transfer is expressed mathematically in Fourier’s Law as shown below:
To make Fourier’s Law more suited to its application, the geometrical and material properties of the CubeSat can be factored into the equation by replacing
with the resistance factor
. This gives the following equation:
Using this equation, Fourier’s Law can be written as:
Heat transfer due to Radiation is extremely significant in space craft design. No medium (i.e., atmosphere) is required for this process to occur as energy is transferred in the form of electromagnetic radiation. A body which has a non-zero temperature will always emit radiation, the magnitude will depend upon the bodies geometry, material composition, relative position to other thermally heated bodies and the bodies surface temperature. The following equation numerically analyses the significance of these stated factors to allow the rate of Radiation emission from a body to be calculated:
This incoming radiation can be absorbed, reflected, and transmitted. All energy must be conserved in any interaction therefore:
Most CubeSat bodies used on CubeSats, for example the Compass-1 craft, are opaque to thermal radiation, therefore transmission can be neglected.
To achieve a thermal balance for the CubeSat to prevent net heating and failure of components, the amount of incoming heat must equal the amount of heat exiting the CubeSat system. Radiation is the most significant source of heat incoming to the body, and radiation is the main driving force causing heat exhaustion from the system.
where:
The external surfaces of the CubeSat act as the interface to energy exchange with the environment, and are exposed to radiation such as solar, Albedo and IR. It is key to achieving a net energy balance to select material with suitable properties to ensure this occurs.
Table 28 shows material properties for Al 6061-T6, used for the CubeSat structure, GaAs solar cells as well as black paint. As the coating is extremely thin is paint is assumed to have a negligible weight. The paint is Nextel velvet coating manufactured by 3 M. It has been certified for space exploration and extreme temperature ranges beyond which the CubeSat will experience.
The larger surfaces, with dimensions 100 mm by 300 mm, of the CubeSat are composed of 70% GaAs solar cells and 30% Al 6061-T6. The smaller “upper” and “lower” surfaces of the CubeSat are Al 6061-T6 coated with black Nextel Velvet coating. The average material property for each face can be calculated using:
For the larger sides covered with 70% GaAs solar cells and 30% Al 6061-T6 the combined absorptivity and emissivity is shown below:
To accommodate for the propulsion system, one of the smaller 100 mm by 100 mm faces will be made from aluminum and will not be coated in black paint, and the emissivity and absorptivity are standard values shown in the table; however, for the aluminum face covered in black paint:
For the 100 mm × 300 mm faces exposed to background space, it is desirable to have as high an emissivity as possible. This will ensure the maximum amount of heat is released to limit the internal temperature to as safe a maximum as possible. The Earth-facing CubeSat panel will be manufactured from 6061-T6 aluminum
The results are summarized in
Table 29, with the Surface Number designations matching those shown below:
To ensure steady-state operation, a basic energy balance can be applied to the system factoring solar radiation, Albedo, Earth infra-red, and radiation from the body to space:
It is assumed therefore can be assumed to also be equal to zero.
The equation shown above can be rearranged to solve the equilibrium temperature for the hottest worst-case scenario:
The worst case hot temperature for the CubeSat’s components giving during the heating phase is given by:
Applying the materials shown in the face identification table, the worst case hot temperature is found to be 315.018 K (42.018 °C). This matches extremely close to temperatures published in literature. For example, Compass-1 encountered a theoretical hot-case temperature of 320.8 K (47.8 °C) at an altitude of 600 km. A temperature difference of 5.782 °C represents an extremely accurate estimation, the difference in these temperatures is accounted for by differences in material selection, for example compass-1’s bottom face was assumed to be 70% solar cells and 30% aluminum whereas this CubeSat’s bottom face was purely 6061-T6 aluminum. The difference in absorptivity of these materials will account for this difference, as more flux enters in the higher absorptivity Solar and Black paint configuration causing a relative temperature increase compared to aluminum.
Alternative material choices can be made for the structure, for example changing the background space faces to aluminum to observe the impact upon the hot-case temperature. For example, converting the background space-facing surfaces with aluminum instead of 30% aluminum and 70% black paint yields a maximum hot-case steady-state temperature of 500.682 K (227.682 °C) which would lead to critical failure of the CubeSat components. This highlights the critical importance of material selection for the external CubeSat faces.
During the eclipse phase the CubeSat will experience extremely low temperatures; due to the fact the only heat input is infra-red radiation from Earth with a value of 198 Wm
−2 [
10]. No electrical power is generated during this phase, as no solar flux is incident, making it an extremely difficult environment for the CubeSat to survive.
By altering the original setup to have a 70% black paint, 30% aluminum structure from pure aluminum 6061-T6 the steady-state hot-case temperature is 321.1187 K (48.11 °C).
The minimum Cold Case steady-state temperature is given by:
Inputting the original material set-up, the cold case steady-state temperature is found to be 102.813 K (−170.187 °C). This temperature extreme cause complete shutdown of the electrical system, leading to mission failure. If Earth-facing material was altered to 70% black paint and 30% 6061-T6 aluminum the cold case temperature is found to be 172.951 K (−100.0489 °C). The selection of the black paint covered face is critical to the success of the shuttle mission. The reduction in the cold case temperature is vital; however, a heating system would still require integration into the CubeSat to ensure temperatures do not exceed the critical values of the CubeSat’s electrical components [
10].
Steady-state analysis does not provide an accurate method of temperature estimation, particularly for the cold case. As the CubeSat would enter the eclipse phase with internally stored energy within the CubeSat’s material mass from the hot-case heating action due to incoming flux from the Sun and Earth. An accurate estimation of the cold case temperature would be given by conducting a transient analysis upon the CubeSat’s eclipse orbit. This would ensure the initial temperature reached from heating, and the material mass and geometry of the CubeSat gave a much more accurate estimation of the CubeSat’s eclipse cold case minimum temperature. A transient study would also map the temperature drop as a function of time [
65]. It would therefore be possible to program the electrical systems heater to switch on a certain critical time in the eclipse phase, just before the minimum operating temperature of the electrical system was reached to conserve stored power in the battery. A transient load case is ideally modelled in a software CAD analysis package, for example SolidWorks, which is explored in
Section 6.2 [
65].
It should however be considered that a thermal load will be placed upon the CubeSat due to heat generated by resistance in electrical components. The worst case hot scenario factoring in heat dissipation is given by [
10]
From the electrical system the average power consumption of constantly active components throughout the cycle was found to be 2.665 W. Given an average efficiency of 70% [
21] the heat dissipation in the device is assumed to be 30% of the 2.665 W power draw, which is equal to a dissipated heat of 0.7995 W.
Inputting this power dissipation into the starting material composition model yields a maximum hot-case steady-state equilibrium temperature of 324.021 K (51.021 °C). This is a significant increase upon the hot-case scenario for the same material analysis of 9.003 °C. Although a relatively small value given the extreme temperature range observed, this increase pushes the steady-state hot-case temperature much higher than operating capabilities [
10], for example the batteries maximum operating temperature of 20 °C. This re-iterates the need for the implementation of multi-layer insulation [
10].
By altering Earth-facing side’s material to 70% black paint, and 30% 6061-T6 Aluminum, the maximum temperature observed due factoring heat dissipation is 322.2 K, which is very similar to the value calculated for compass-1 assuming a 1 W heat dissipation, of 326 K.
Electrical heat dissipation is advantageous during the eclipse phase, as it will raise the average temperature inside the CubeSat, bringing the steady-state temperature closer towards that which would be suitable for electrical components to remain operational, approximately −5 °C [
21]. By including heat dissipation to the best case cold scenario, where black paint is attached to Earth-facing side, the cold case temperature is given by:
The best case thermal load is 179.514 K. This is extremely similar for that calculated for the compass-1 craft of 176.3 K [
10]. Even with the addition of electrical heat dissipation a heater will be required to keep electrical components operational.
6.2. Thermal Load Case Testing (SolidWorks)
To conduct thermal modelling of the CubeSat’s orbit, it is firstly necessary to create a simplistic steady-state model [
9]. The generated CAD geometry will be a shelled rectangular body with a wall thickness of 1.27 mm to replicate the thickness of the Pumpkin Monocoque. A steady-state model does not require an accurate estimation of thickness and geometry, as this simplistic calculation generates an equilibrium temperature based on the heat balance equation
[
9].
A steady-state analysis can incorporate surface to ambient or surface to surface radiation in the SolidWorks program. Selecting the ambient option will replicate the load conditions, dissipating heat to the surrounding background space environment.
Once the two components were modelled it is necessary to assign material properties to the bodies. The material properties, listed in
Table 30, are extremely important for an accurate analysis. To provide comparable results to the first-hand calculations, the weighted emissivities and absorptivities are applied [
9]. For a steady-state calculation, material density and thickness does not factor; however, it will be important during the transient calculations, as the rate of heat loss and absorption will depend on the material geometry.
This 3U CubeSat geometry,
Figure 49 was then loaded into the thermal analysis window of SolidWorks. A standard mesh was then applied to the geometry with a coarse mesh size of 13.8 mm shown in
Figure 50. This value was found to be suitable via a mesh convergence study, as by default SolidWorks only produces results when convergence is lower than a 0.1% value [
58].
Thermal loads are then applied to the model, simplistically modelling a thermal load case similar to that encountered during the worst case hot phase in orbit. It is firstly assumed that both faces housing the Clyde-Space XTJ solar cells are perpendicularly incident to the incoming solar flux, which has an intensity of 1369 Wm
−2 illustrated in
Figure 51. In reality, it is highly unlikely that this loading scenario would be encountered [
9].
The incoming albedo and Earth’s infra-red radiation were applied to the bottom face, as shown in the figure below (
Figure 52). It is assumed that the Albedo and IR incoming fluxes are perpendicular to this face, which is the lower face, positioned towards Earth during orbit. The value of incoming applied Albedo is 488.733 W and Earth’s infra-red 197.96 W. These values are found in the first-principle calculations based on an orbit height of 600 km.
To create a steady-state heat transfer scenario, it is also necessary to model the heat exhaustion from the “cool” faces coincident with the background temperature of space of 3 K experiencing no heating effect due to the incoming flux. This heat removal from the system,
will allow SolidWorks to define a steady-state equilibrium temperature for the CubeSat in the worst case thermal load scenario [
9].
The initial chosen material for the heat expulsion faces is 70% black paint coating and 30% aluminum, which has an averaged emissivity of 0.654. The material selection for these faces will be altered to pure aluminum 6061-T6 to observe the effect upon the equilibrium temperature once the initial temperature has been determined by the SolidWorks Thermal simulation solver. Identical thermal loading was then applied to the 100 × 100 mm end faces of the CubeSat, as it is assumed these faces only interact with the background space temperature to dissipate heat from the CubeSat body (
Figure 53). The view factor for the radiation to background space is assumed equal to 1 [
9].
The CubeSat geometry was then designated an Aluminum 6061-T6 material in SolidWorks. The material selection for the steady-state analysis has no impact upon the results, only the surface area impacts upon the results. The initial results presented a temperature gradient across the CubeSat which would be expected according to theory. The panel’s incident with the incoming solar flux is at the highest temperature, a value of 547.6 K. The panels enduring no incoming solar flux are at the lowest temperature which also matches established theory. Temperatures on the “cold” faces drop as low as 427.7 K shown in
Figure 54.
Although the temperature gradient throughout the CubeSat matches that of theory, the magnitude of the steady-state temperature is much higher than that stated in literature [
9]. Steady-state analysis upon the 1U Compass-1, also orbiting at 600 km polar orbit, calculated a steady-state temperature range of 318.3 K to 326.516 K [
9]. The average internal temperature of compass-1’s orbit in the Sun phase is 322.408 K whereas the author’s analysis produced an average value of 510.15 K. This represents a 1.5823 magnitude difference between the values illustrated by
Figure 55.
It is, therefore, necessary to reconsider the loading scenario to produce a steady-state temperature range matching that presented in validated theory. The loading case has been significantly altered from the initial testing and may have a significant impact upon the proposed design. The preliminary design had solar flux incident upon two faces, this assumption has been altered to have solar flux incident on the singular top face. This would significantly impact the power system, as the theoretical power generation would be halved to 5.39 W. It was previously assumed heat was only radiated from the 3 cold faces; however, heat would be radiated from the top face as the Sun is an extreme distance away, and the side face incident has no solar flux as this faces background space. Heat would not be dissipated from the bottom face assumed perpendicular to Earth, as the expected temperature range of this body would be extremely similar to that of Earth, approximately 20 °C.
The alteration in the thermal load case has provided a temperature range much closer to that stated in literature. The temperature range for this thermal load scenario has been reduced to a minimum of 313 K (40 °C) and a maximum of 338.9 K (65.9 °C) illustrated by
Figure 56. This gives an average steady-state heating phase temperature of 325.95 K (52.95 °C). This is an extremely similar value to the average steady-state heating phase value of compass-1, which is 322.408 K (49.408 °C) [
10]. Assuming theory to be the correct value, the percentage error between the values is 1.09% which is an acceptable error as an error below 5% is deemed negligible [
59].
The significant difference in upper temperature limit on the face incident with solar flux is due to the difference in area exposed to the incoming solar flux between the two models. As compass-1 is a 1U CubeSat, the area of one face exposed to incoming solar flux is 100 mm × 100 mm (0.01 m
2) [
1] whereas the 3U has a total exposed surface of 100 mm × 300 mm (0.3 m
2). As the solar flux is assumed perpendicular to this face, triple the amount of radiation is incident. An error arises when comparing results generated in SolidWorks to those generated in first-principle calculations. This is because SolidWorks does not account for the absorptivity of faces incident with thermal load and assumes full ideal absorption, whereas the first-principle accounts for absorptivity of the incident faces, for a weighted load into the system based on material properties. In SolidWorks, the model’s material could be changed to rubber, for example, and this would have no bearing upon the results, highlighting the need for the future development of a transient model [
9].
The range of temperatures exerted during the hot phase is unacceptable as many of the electrical systems components would fail under the calculated thermal load [
9]. For example, this temperature would lie outside the safe operating range of the CubeSat’s selected battery, causing potential catastrophic failure for the imminent eclipse phase when stored power is required to operate vital sub-systems. It is, therefore, necessary to introduce an additional thermal passive control system, for example multi-layer insulation, to help shield incoming critical components from incoming radiation [
9].
A following thermal study was conducted, investigating the impact of the “eclipse phase” upon the internal temperatures of the CubeSat.
Initially the original material parameters used in the first-principle steady-state calculations were applied. A flux of (198 Wm−2) was applied to Earth-facing edge, with radiation to background space assumed for the other remaining 5 faces.
The minimum temperature, illustrated in
Figure 57 observed during this analysis was 183.3 K (−89.7 °C). When compared to the first-principle calculations result of 172.951 K (−100.0489 °C), the values are found to have approximately 10% difference. This is due to the slight differences in radiation emittance from the CubeSat body, as the first-principle calculations assume no emittance from the solar cell-mounted face incident with solar flux, whereas the SolidWorks analysis has been configured to assume heat loss from this face. When comparing the results to published literature [
9] compass-1 encountered theoretical cold case temperatures of 167.7 K. The negligible difference in calculated results compared to those presented in literature highlights the accuracy of the developed thermal load case.
To validate first-principle results incorporating a thermal load due to heat dissipation, a study was developed to replicate each respective hot and cold case in SolidWorks thermal solver. The finalized hot-case analysis mirrored the initial hot analysis, with the addition of a 0.7995 W applied to the “top face” to replicate a worst-case heat transfer scenario [
9].
The minimum observed temperature is 321.2 K and the maximum observed temperature is 339.5 K directly upon the face incident with the incoming solar flux, which is to be expected as the highest incoming rate of energy is located at this geometry, shown in
Figure 58. The average observed temperature throughout the structure is 330.35 K (57.35 °C) which represents an approximate temperature increase of (4.5 °C) which is to be expected due to the additional thermal load placed upon the structure [
9]. The calculated value is extremely close to the 326 K experienced by compass-1 under an extremely similar thermal load, validating the accuracy and reliability of the generated results [
9] The addition of a thermal heat dissipation load has further increased temperatures inside the structure, increasing the need for a thermal management system to be incorporated to bring this temperature to a safe operating level.
The cold case power dissipation simulation also provided extremely similar results to those published in literature. Due to the addition, the of internal heat dissipation the lowest observed temperature is (−80.1 °C), shown in
Figure 59, This represents a (9 °C) increase upon the temperature previously observed during cold phase testing. This temperature increase, however, is relatively irrelevant as the average temperature in the structure is still well below the required (−5 °C) minimum operating temperature for the electrical system. It is, therefore, critical to mission success that an adequate heater is installed feeding off the power systems battery reserves built up during the hot phase by the solar cells.