PH508: Spacecraft Power generation
Solar cells, fuel cells and RTGs.
Payload mass, mp = 5 tons ms1 = 140 tons (given in table) ms2 = 35 tons “ ms3 = 10 tons “ mf1 = 2160 tons “ mf2 = 420 tons “ mf3 = 100 tons “
mo1 =ms1 + mf1 + ms2 + mf2 + ms3 + mf3 + mp
=2870 tons
mo2 =ms2 + mf2 + ms3 + mf3 + mp
=570 tons
mo3 =ms3 + mf3 + mp
=115 tons
Homework – Week 15, Q2, part 1.
Now calculate ‘R’ for each stage
Recall:
∴
Homework – Week 15, Q2, part 1.
fioi
oii mm
mR
67.7110115
115
80.3420570
570
04.421602870
2870
3
2
1
R
R
R
Now we have R1, R2, and R3 can calculate the final rocket velocity, vfinal via:
Homework – Week 15, Q2, part 1.
1-
332211
s km 3.17
66.874.524.367.7ln25.480.3ln10.404.4ln32.2
lnlnln
RvRvRvv eeefinal
This wasn’t easy – my apologies. From definition of R we have:
Homework – Week 15, Q2, part 2.
6
25.410.432.2
16
25.410.432.2
25.410.432.2
321
332211
321
10886.810110
145565
7052865
10110
145565
7052865
ln16
10110
ln145565
ln7052865
ln16
10110
ln25.4145565
ln10.47052865
ln32.216
ln25.4ln10.4ln32.216
0.16lnlnln
10110
,145565
,7052865
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
p
eeefinal
p
p
p
p
p
p
mm
mm
mm
e
mm
mm
mm
mm
mm
mm
mm
mm
mm
RRR
RvRvRvv
mm
Rmm
Rmm
R
ANALYTICALLY INTRACTABLE!?!?
Homework – Week 15, Q2, part 2: graphical solution
Solve by plotting, vfinal versus mp
PH508: Spacecraft Power generation
Solar cells, fuel cells and RTGs.
The Glast Satellite, source NASA/Sonoma State University (Aurore Simonnet)
Solar Cells: I
These use solar radiant energy and convert it directly into electricity, via the photovoltaic effect.
An array is made up of thousands of individual cells (2 cm x 4 cm typically), connected in series to provide DC power (28 V typical, 120 V can be found today).
Power levels can be in range of a few Watts to 100’s of kW.
An individual cell is just a semiconductor p-n junction.
Solar cells: II
Solar Cells: IV
Solar cells: IISolar panels on ISS
Silicon was typical, today (Gallium Arsenide) GaAs has been used but is not universal.
Silicon is doped with boron to produce p-type (electron deficient) material and phosphorous for n-type (electron excess) material.
In dark conditions an equilibrium is reached where no significant current flows. If illuminated, by photons of sufficient energy, electron-hole pairs are created, these flow creating a potential difference across the device.
Solar cells: V
Solar cells: III
Schematic showing photoconduction of an electron
Solar cells: II
To cause the hole-electron production the photon energy has to exceed the band-gap energy. If photons have excess energy this can be deposited as heat.
We can define hf Eg where h is Planck’s constant, f is the frequency of the radiation and Eg is the band gap in Joules.
You can characterise a solar cell by its I-V curve. The best operating point is the maximum power point, given by Vmp and Imp
Solar cells: VI
Typical solar-cellI-V characteristic
Solar cells: VII
You can also define:◦ Open circuit voltage (i.e. no current drawn) Voc
◦ Short circuit current Isc◦ A fill factor (FF) which says how “square” the I-V
curve is. The “squarer” the better. FF is defined as:
FF = (Vmp Imp)/(Voc Isc)
The closer to 1 this is the “squarer” it is.
Solar cells: VIII
For a silicon cell Voc is typically 0.5 to 0.6 V, Isc depends on the illumination level, and FF can be 0.7 to 0.85.
To find the peak power, you draw output power vs. output voltage. A clear peak can be found, which defines Vmp and hence Imp can be determined.
If you heat a solar cell you will find its performance changes. Its efficiency falls as its temperature increases.
Solar cells: IX
There is a packing factor for a solar panel, which describes how much of its surface area is really solar cells, 0.9 is good. The rest is structure, edges, gaps etc. So the effective area is less than the actual surface area of a solar panel.
Solar panels need to be face on to the Sun for maximum efficiency. If they are tilted then a geometric correction has to be applied to give the cross-section projected orthogonal to the solar direction. If the angle between the normal to the surface of the panel and the solar direction is θ, then there is a factor cos θ that has to be applied when finding the effective surface area illuminated and hence the power output.
Solar cells: X
Typical bandgap energies for solar cell materials
Solar cells: XI
nnn
Solar cells: XII
Solar cells in orbit do suffer degradation with time. Due to:◦Accumulation of micrometeorite impact damage,◦Attack by atomic oxygen on the wiring◦Radiation damage to the semi-conductor.
There is thus a factor for loss of efficiency with time – power output falls slowly with time.
Estimating this loss rate, and over-sizing the solar array at the Beginning of Life (BOL) so it over-produces power but produces the correct power at the End of Life (EOL). Solar panels at the BOL in Earth orbit can produce 30 – 50 W/kg of mass.
Current state-of-the-art Multi-Junction (MJ) solar cells have efficiencies approaching 50%.
Solar cells: XIII
Fuels Cells [F & S Chapter 10, p. 337] The basic idea is to generate electricity from
chemical reactions. They are used on the Shuttle, and were used in
the Mercury, Gemini and Apollo space missions. An oxidation reaction is used. It has a high energy
density (typical o/p Gemini: 33W/kg, Apollo: 25 W/kg, STS: 275 W/kg). This is available on demand and continuous when running (although the start up time of early cells was long). But you need to carry fuel (oxygen and hydrogen).
Fuel cells: I
A hydrogen/oxygen fuel cell is typical and produces water (a useful output).
In an ideal cell the voltage (Er) produced is given by:
Where ΔG is the Gibbs free energy in the reaction, n is the number of electrons transferred and F is the Faraday constant (9.65× 104 C/mol).
Fuel cells: II
nFGEr
In the hydrogen/oxygen cell the reaction transfers 2 electrons per molecule of water formed and ΔG = -273.2 kJ/mol at 25 °C. This gives 1.416 V. In reality this is the ideal potential, as there are losses in the system.
Early cells could take 24 hrs to start and 17 hrs to stop (Apollo), but for the Shuttle start up times is 15 min and shut down is immediate.
Fuel cells: III
Fuel cells: IV
v
Radioisotope Thermal Generators (RTGs) are used to generate power on space missions where solar energy is at a low flux or not available for long periods (mainly unmanned missions).
They generate heat. They then use the thermoelectric effect whereby a voltage is generated between two materials (semi-conductors or conductors) if a temperature difference is maintained between the two ends (think of a thermocouple).
Here the cold end is achieved by exposure to space. The hot end by waste heat from nuclear decay.
RTGs: I
RTGs: II
A practical device is shown in F&S page 340
Isotope Fuel form Decay product
Power density (W/g)
τ½ (years)
Polonium 210 Gd Po α 82 0.38
Plutonium 238 Pu O2 α 0.41 86.4
Curium 242 Cm2 O3 α 98 0.4
Strontium 90 SrO β 0.24 28.0
RTGs: III
Various radioactive materials for possible use in a RTG.
RTGsPellet of glowing 238PuO2 – generating 62 watts of heat
RTGs: IV
Cassini RTG – source, NASA
RTGsCassini’s RTG? Doesn’t look like a clean room!
RTGsMuch better…..New Horizons’ RTG (mission to Pluto)[Cassini flight spare, using 11 kg of Plutonium pellets]
When considering a design, care has to be made to ensure that in the event of an accident during launch, the radioactive material does not escape into the environment. Clean-up costs would be expensive in terms of money, and public support!
The power generated by a RTG is not constant with time, the material decays so there is less as time goes on and hence less power can be generated.
RTGs: V
You need:
Where Pt is power at time t, and P0 is the initial power at t = 0.
τ½ (years) is given in the table above.
RTGs: VI
tPP ot
2/1
693.0exp
So you have to calculate what power you need for the mission and start the mission (Beginning Of Life - BOL) with too much power. Then as the source decays, the RTG’s output falls and you plan it so you have just the right amount of power at the end of the mission lifetime (End Of Life – EOL)
RTGs: VII
Pros:◦ You are not reliant on the spacecraft pointing at
the Sun or not being in eclipse.◦ You are not dependent on radial distance from the
Sun◦ Power levels can be sustained for periods of years
(depending on τ½). Voyager’s RTG has been running for almost 30 years.
◦ Aside: Congress has just agreed to the start-up of plutonium production to fulfil NASA’s requirement for RTG material – at NASA’s expense it would seem!
RTGs: VIII
Cons:◦ Radiation is emitted and may affect instruments on the
spacecraft.◦ The material is radioactive and often highly poisonous – it
needs careful handing during construction and spacecraft integration at the launch.
◦ By definition the hotter the better, but this may not be good for spacecraft components so may need to shield the heat from the spacecraft interior.
◦ The public does not like the word radioactive and rockets do fail during launch, so extra care has to be taken in packaging the RTG to prevent disassembly during an explosion or crash.
RTGs: IX
Should now have an understanding of the different mechanisms available to power a spacecraft:◦ Solar Panels◦ Fuel Cells◦ RTGs
You should also understand the advantages and disadvantages of each.
The power source you choose is dependent on the mission requirements.
Conclusions