Energy Reports: Xinyu Miao, Haochun Zhang, Dong Zhang, Chenxu Zhang, Ziliang Huang
Energy Reports: Xinyu Miao, Haochun Zhang, Dong Zhang, Chenxu Zhang, Ziliang Huang
Energy Reports: Xinyu Miao, Haochun Zhang, Dong Zhang, Chenxu Zhang, Ziliang Huang
Energy Reports
journal homepage: www.elsevier.com/locate/egyr
Research paper
article info a b s t r a c t
Article history: Space nuclear reactors are the research foundation of space nuclear power and nuclear propulsion.
Received 2 August 2021 Thermoelectric conversion efficiency and mass of high-power nuclear reactors have always been
Received in revised form 27 December 2021 essential factors that restrict aerospace design. Supercritical nitrous oxide (S-N2 O) Brayton cycle is
Accepted 22 January 2022
becoming hot research due to its high-power conversion efficiency, low energy loss, compact and
Available online xxxx
simple system structure, making it widely used in space nuclear reactor application. The recompression
Keywords: cycle is proposed to improve the thermal efficiency of the S-N2 O cycle and effectively weaken the
Nuclear power spacecraft ‘‘pinch point’’ phenomenon that may occur in the regenerators. The thermodynamic of the S-N2 O
Supercritical N2 O-He Brayton cycle has been studied but has little research on the nitrous oxide (N2 O) and helium (He)
Recompression Brayton cycle mixtures as the working medium for the Brayton cycle. In this paper, physical properties were
Thermodynamic properties
studied on the mixture of supercritical nitrous oxide and helium (S-N2 O+He) as the working medium
Thermoelectric conversion efficiency
of the space power system based on a recompression Brayton cycle. Consider the thermodynamic
properties of the mixture at seven different temperature nodes, analyze the variation trend of
compressibility factor, specific heat, specific heat ratio, thermal conductivity, and dynamic viscosity
with temperature, respectively. Finally, determined the mixing ratio of the working medium at the
maximum thermoelectric conversion efficiency of the cycle and estimated the mass and specific mass
of the Brayton rotating unit.
© 2022 The Author(s). Published by Elsevier Ltd. This is an open access article under the CC BY-NC-ND
license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
1. Introduction shield, and pressure shell. A NEP system can be defined in six
subsystems: reactor, shield, thermoelectric conversion, heat re-
With the deepening exploration of space, spacecraft missions jection, power management and distribution (PMAD), and electric
have been farther and farther away from the earth in recent propulsion (EP). The thermoelectric conversion part of the space
years. Space nuclear power systems are favored due to the advan- nuclear power system is significant. Thermoelectric conversion
tages such as high-power density, stable performance, and long efficiency is related to the operational efficiency and safety of
working life. Space nuclear reactor power systems have simple the aircraft and has a significant influence on the structure and
lightweight structures, making them more suitable for deep space mass of the spacecraft. Thermoelectric conversion technologies
exploration missions and Mars and Lunar Outposts in the future
for a space nuclear power system include dynamic (Gryaznov,
(Liu et al., 2021). Space reactor power system can be operated
2000) and static methods (Mason and Schreiber, 2007). Static
continuously or intermittently, starting and shutting down mul-
conversion methods are designed for a specific situation by mod-
tiple times for more than 1000 years or even longer, with the
power ranging from 100 kWe to 1 MWe, to replace where the so- ular modes, but conversion efficiency is usually about 10% (Fang
lar energy options are not feasible or non-existent (El-Genk et al., et al., 2017). Dynamic conversion methods based on the Stirling,
2010). The nuclear power system of spacecraft can be divided Rankine, and Brayton cycles can provide high thermal efficiency
into two types: nuclear thermal propulsion (NTP) system and of 20% to 30% (Fang et al., 2017). The recompression Brayton cycle
nuclear electric propulsion (NEP) system. NTP consists of three is suitable for the space system (Yuan et al., 2021). Supercritical
highly integrated subsystems: a nuclear reactor, a rocket engine, fluids in power systems have been regarded as a potential techni-
propellant storage, and management subsystem. The reactor sub- cal choice for different types of power conversion systems (Antti
system consists of the core, control drums, actuators, reflector, et al., 2021). The Brayton cycle can be combined with the fourth-
generation nuclear energy system to meet the different power
∗ Corresponding author. requirements of spacecraft. The fourth-generation nuclear energy
E-mail address: zhc7@vip.163.com (H. Zhang). system generally operates with high temperature and pressure
https://doi.org/10.1016/j.egyr.2022.01.186
2352-4847/© 2022 The Author(s). Published by Elsevier Ltd. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-
nc-nd/4.0/).
X. Miao, H. Zhang, D. Zhang et al. Energy Reports 8 (2022) 2480–2489
Similarly, the data for the normalized third virial coefficient are Where ρ is the density of the mixture(kg/m3 ), Rg is the gas
correlated as Jean and Mohamed (2008): constant of the mixture, and presented below:
0.0237 8314
[ ( )
C = v ∗2 0.0757 + −0.0826 − 3.6 × 10−5 θ + 0.059
Rg = (13)
θ M
Where M is the average molar mass of the mixture and presented
]
× tanh (0.84θ) (5) below (Zhang et al., 2021):
The B, C for mixture can be presented as Brewer and Vaughn M = x1 M1 + (1 − x1 )M2 (14)
(1969):
2.2.3. Dynamic viscosity
B = x21 B11 + 2x1 x2 B12 + x22 B22
The dynamic viscosity of the mixture is shown as Jean and
B12 = v12
∗
ΨB T /Tcr ,12
( )
Mohamed (2008):
(6)
B11 = v11
∗
ΨB T /Tcr ,11 1 0.291 × v ∗
( )
µmix = µ0 + (1 − )µ∗ × ψµ ( ρ) (15)
2.3 M
B22 = v22 ΨB T /Tcr ,22
∗
( )
The critical viscosity of the mixture, µ∗ is calculated using Eq. (16)
C = x31 C111 + 3x21 x2 C112 + 3x1 x22 C122 + x32 C222 by Mason and Uribe (1996),
) 13 √ as:
C112 = C12 C2
( MT ∗
(7) µ = 0.204 × 10
∗ −7
)1 (0.291 × v ∗ )2/3 (16)
C1 C22 3
(
C122 =
ψµ (ρ ) = 0.221ρ + 1.062ρ 2 − 0.509ρ 3 + 0.225ρ 4
Where Bii is the second virial coefficient for a pure gas (mol/m3 ),
The average critical specific volume v∗ and average critical
Bij is the second virial interaction coefficient (mol/m3 ) i ̸ = j, Ciii
temperatures T ∗ are calculated as Jean and Mohamed (2008):
is the third virial coefficient of pure gas (mol2 /m6 ), Cijj is the
third virial interaction coefficient (mol2 /m6 ) i ̸ = j, v*ii is the v ∗ = x1 v11 + x2 v22 (17)
characteristic molar volume of pure gas (m3 /mol) v*ii = v* =
x2 V11 T11 + x222 V22 T22 + 2x1 x2 V12 T12
Rg∗ (Tcr /Pcr ), v*ij is the characteristic interaction molar volume T ∗ = 11 (18)
(m3 /mol) i ̸ = j, v∗12 is the average specific volume of the mixture, x1 V11 + x2 V22
1 and 2 respectively stand for He and N2 O. xi is the molar fraction The viscosity of the gas mixture is calculated using the pro-
of component i in the gas mixture. posed by Sutherland and Wassiljewa:
Tcr,12 is the average critical temperature of mixture and pre- µ01 µ02
sented as Prausnitz (1959): µ0 = x2 + (19)
1 + φ12 x 1 + φ21 x1
x
1 2
4b √
Tcr ,12 = Tcr ,1 Tcr ,2 (8) The interaction coefficient φij are calculated by Mason and Uribe
(1 + b)
(1996):
v11
∗
µ0 2M1 M2 5 M2
b=
v22
∗ φ12 = 1 ×( + )
µ12 (M1 + M2 )2 3A12 M1
(20)
2.2.1. Enthalpy and specific heat µ0 2M1 M2 5 M1
φ21 = 2 × ( + )
In this paper, Cp and Cv of the working medium are consid- µ12 (M1 + M2 )2 3A12 M2
ered as strength parameters (unrelated to the total amount of In these equations, the A12 is the ratio collision integrals, A12 =
(2,2)
substance) and Cp , Cv can be calculated by the weighted aver- Ω / Ω (1,1) , and the interaction viscosity is shown below (Jean
age of the mass fraction. Therefore, the calculation formulas for and Mohamed, 2008):
the thermal parameters of N2 O-He mixed working medium are
shown as Zhang et al. (2021): µ12 = Aµ (T − Tµ )n (21)
Table 1
Constant value of the empirical formula for N2 O physical properties calculation.
T (K) 298–1400 1400–6000
A 27.67988 60.30274
B 51.14898 1.034566
C −30.64454 −0.192997
D 6.847911 0.012540
E −0.157906 −6.860254
Cp◦ = A + Bt + Ct 2 + Dt 3 + E /t 2
(39)
Cv◦ = A − Rg + Bt + Ct 2 + Dt 3 + E /t 2
3.1.3. Thermophysical properties of N2 O-He Fig. 5. Effect of He mole fraction on heat capacity of the mixture, Cp .
The properties of the mixture depending on the properties of
the pure gas substance. Python software was used to program
and iteratively calculate the parameters related to the working 3.4. Specific heat ratio, γ
medium properties of the mixtures.
The specific heat ratio, γ , is shown in Fig. 6. The range of
γ is from 1.15 to 1.7. The Cp of He is not easily affected by
3.2. Compressibility factor, Z temperature, but the Cp of N2 O is greatly affected by temperature.
In the low region of xHe , the γ of mixture has a more significant
When Z = 1, the mixed gas obeys the ideal gas law; Z < 1, the variation with temperature. The γ is increased with the increase
gas is compressed easily; Z > 1, the gas is compressed difficultly. of xHe . When the xHe > 0.6, the γ change trend tends to be
The compressibility factor of the mixture, Z, is shown in Fig. 4. gentle. When T = 315.00 K, the corresponding line of γ has
The compressibility factor of the mixture gas is changed from a bit different from other lines because near the critical point
0.75 to 1.15. When T = 315.00 K–600.00 K, Z of the mixture properties of N2 O changed drastically.
increase slowly with the increase in the mole fraction of He,
xHe . When T = 800.00 K–1400.00 K, Z is decreases with the 3.5. Thermal conductivity, λ
increases of xHe . For the mixture, if xHe < 0.3, Z decreases with the
The thermal conductivity, λ, is shown in Fig. 7. Thermal con-
temperature decrease; if xHe > 0.3, Z decreases with the increase
ductivity is sensitive to temperature changes. The thermal con-
of temperature. When T = 800.00 K, Z ≈ 1.0, nearly has no
ductivity of pure N2 O at 1200.00 K is 2.8 times that at 400.00 K.
change with xHe . The thermal conductivity of He is much higher than that of N2 O.
Therefore, with the increase of xHe , the thermal conductivity
3.3. Specific heat, Cp of the gas mixture increases, and the higher temperature, the
greater the λ rise. The 315.00 K thermal conductivity line is
slightly different from other lines because 315.00 K is close to
The heat capacity of the mixture, Cp , is shown in Fig. 5. In the critical point of N2 O.
Fig. 5, the Cp is increased with the increase of xHe . At high xHe ,
the Cp has little change with temperature, the lines approximately 3.6. Dynamic viscosity, µ
overlap; at low xHe , lower temperature more minor smaller Cp .
With the same xHe , Cp increases slower by temperature, and the The dynamic viscosity, µ, is shown in Fig. 8. Due to the
lines have small change in high temperature. molecular interaction of the working medium, the viscosity of the
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X. Miao, H. Zhang, D. Zhang et al. Energy Reports 8 (2022) 2480–2489
Fig. 6. Effect of He mole fraction on specific heat ratio, γ . Fig. 9. Effect of He mole fraction on Prandtl number, Pr.
Table 2
The selected Brayton cycle parameters (Zhang, 2019; Feng et al., 2020;
Mohammadi et al., 2019; Meng et al., 2021).
Parameters Description Values
p3 (MPa) Main compressor inlet pressure 7.40
T2 (K) Reactor outlet temperature 1200.00
T6 (K) Cooler outlet temperature 315.00
m (kg/s) Mass flow rate 5.00
x∗ Split ratio 0.30
π Pressure ratio 3.00
ηMC Main compressor efficiency 0.85
ηRC Re-compressor efficiency 0.85
ηT Turbine efficiency 0.88
εHTR Effectiveness of High-temperature recuperator 0.86
εLTR Effectiveness of Low-temperature recuperator 0.86
Fig. 7. Effect of He mole fraction on thermal conductivity, λ. The Prandtl number, Pr, is shown in Fig. 9. The Prandtl number
of mixtures is always lower than those of pure gases in the
mixtures and very significant with the mixture composition and
temperature. The Prandtl number of He is between 0.5–0.7, and
N2 O is between 0.7–1.5. When T = 315.00 K–325.00 K, the
Prandtl number increases rapidly with increasing Helium mole
fraction xHe . At the same time, when T > 400.00 K and xHe < 0.5,
the Prandtl number of the mixture gradually decreases, then but
when xHe > 0.5, the Prandtl number almost changes little. The
Prandtl number is an important parameter that affects the heat
transfer coefficient of the working fluid and has an essential effect
on the cycle.
Fig. 10. Effect of He mole fraction on system thermal efficiency, ηth . Fig. 12. Effect of He mole fraction on specific mass of Brayton Rotating unit,
αBRU .
4. Conclusion
Table 3
Comparison of CO2 , N2 O, He, and 85% N2 O - 15% He recompression Brayton cycle.
Operating parameters CO2 N2 O 85% N2 O and 15% He He
Tmin (K) Tmax (K) Pmin (MPa) ηth (%) ηth (%) ηth (%) ηth (%)
315 1200 7.4 41.6 43.0 48.1 43.2
315 1200 8.4 39.9 40.9 45.3 41.2
315 1000 7.4 40.4 41.8 47.1 41.7
315 1000 8.4 38.2 39.7 44.5 39.4
325 1200 7.4 38.3 39.2 47.5 39.8
325 1200 8.4 36.1 36.9 44.8 37.5
325 1000 7.4 34.5 40.0 46.4 36.3
325 1000 8.4 31.2 37.5 43.6 33.3
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Declaration of competing interest Power Systems with Nuclear Fission Reactor Heat Sources. Cleveland State
University, Ann Arbor, USA.
The authors declare that they have no known competing finan- Khatoon, S., Kim, M.H., 2019. Potential improvement and comparative assess-
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