Link Budget for Artemis II. Updated: 2026-07-09 12:20:28. See: https://www.sarcnet.org/files/link_budget.py
 
1. Constants:
 
LineParameterValueUnitsComments
1.01 c299792458m/sSpeed of light constant
1.02 k1.380e-23W/Hz/KBoltzmann's constant
 
2. Artemis spacecraft data:
 
LineParameterValueUnitsComments
2.01 f2216509018HzReceived Frequency of the Artemis downlink derived from the Bochum video
2.02 l = c/f0.13525mReceived Wavelength of the Artemis downlink derived from the Bochum video
 
3. AMSAT-DL Bochum 20m Radio Telescope data:
 
LineParameterValueUnitsComments
3.01 GTdB = 30.0-(2.3-(f/1e9))*(32.6-30.0)/(2.4-2.3)27.8dB/KG/T for Bochum (dB) extrapolated for f from the AMSAT-DL website
3.02 GT = lin(GTdB)606.6/KG/T for Bochum extrapolated for f from the AMSAT-DL website
 
4. Estimate the Artemis downlink Equivalent Isotropic Radiated Power (EIRP) derived from Bochum video data:
 
LineParameterValueUnitsComments
4.01 r184034000mRange to Artemis derived from the Bochum video
4.02 PsdB-80dBThe signal peak (dB) derived from the Bochum video
4.03 PndB-95dBThe noise floor (dB) derived from the Bochum video
4.04 SNNRdB = PsdB - PndB15.0dBSignal plus Noise to Noise Ratio (dB) derived from the Bochum video
4.05 SNNR = lin(SNNRdB)31.6Signal plus Noise to Noise Ratio derived from the Bochum video
4.06 FSPL = (l/(4*pi*r))**23.4e-21Free Space Path Loss derived from the Bochum video
4.07 FSPLdB = dB(FSPL)-204.7Free Space Path Loss (dB) derived from the Bochum video
4.08 B8000000HzBandwidth of receiver derived from the Bochum video
4.09 Pt = 0.5*(SNNR-1)*k*B/(FSPL*GT)815WEstimate of Artemis transmitted EIRP
4.10 PtdB = dB(Pt)29.1dBWEstimate of Artemis transmitted EIRP (dBW)
 
5. System Dish calculations:
 
LineParameterValueUnitsComments
5.01 FD0.35Focus to Diameter ratio of the dish
5.02 dt5degreesDelta theta: Increment for all numerical integrations
5.03 d11.8mDiameter of the dish reflector
5.04 d20.12mDiameter of the feed antenna
5.05 e_mesh0.0018mMesh RMS surface error of the dish
5.06 a_mesh0.0030mMesh hole size of the dish
5.07 r_mesh0.0002mMesh wire radius (thickness / 2) of the dish
5.08 psi = dt*round(degrees(2*atan(1/(4*FD)))/dt)70degreesHalf-angle of Dish Rim at the focus point
5.09 theta_b = dt*round(degrees(2*atan(d2/d1/(4*FD)))/dt)5degreesHalf-angle of Feed Antenna at the focus point
5.10 cot_squared_psi_on_2 = (1/tan(radians(psi)/2))**22.040cot squared psi on 2
5.11 n_ill_numerator = 2*cot_squared_psi_on_2*integral(sqrt_p_tan_theta_on_2,0,psi,dt)**20.200Illumination efficiency numerator
5.12 n_ill_denominator = integral(p_sin_theta,0,psi,dt)0.257Illumination efficiency denominator
5.13 n_spill_numerator = integral(p_sin_theta,0,psi,dt)0.257Spillover efficiency numerator
5.14 n_spill_denominator = integral(p_sin_theta,0,180, dt)0.267Spillover efficiency denominator
5.15 n_block_numerator = integral(sqrt_p_tan_theta_on_2,theta_b,psi,dt)**20.048Blocking efficiency numerator
5.16 n_block_denominator = integral(sqrt_p_tan_theta_on_2,0,psi,dt)**20.049Blocking efficiency denominator
5.17 n_ill = n_ill_numerator/n_ill_denominator0.779Illumination efficiency of the dish
5.18 n_spill = n_spill_numerator/n_spill_denominator0.965Spillover efficiency of the dish
5.19 n_block = n_block_numerator/n_block_denominator0.983Blocking efficiency of the dish
5.20 n_ruze = exp(-(4*pi*e_mesh/l)**2)0.972Ruze efficiency of the dish
5.21 n_mesh = 1-((2*a_mesh/l)*log(a_mesh/(2*pi*r_mesh)))**20.999Mesh efficiency of the dish
5.22 n = n_ill*n_spill*n_block*n_ruze*n_mesh0.72Aperture efficiency of the dish
5.23 A = n*pi*(d1**2)/41.83m^2Effective area of the dish
 
6. System Gains and Noise Figures:
 
LineParameterValueUnitsComments
6.01 GlnadB15.0dBLNA Gain (dB)
6.02 Glna = lin(GlnadB)31.6LNA Gain
6.03 NFlnadB0.35dBLNA Noise Figure (dB) from TQP3M9037 datasheet
6.04 NFlna = lin(NFlnadB)1.08LNA Noise Figure from TQP3M9037 datasheet
6.05 GfildB-0.37dBFilter Gain (dB)
6.06 Gfil = lin(GfildB)0.92Filter Gain
6.07 NFsdrdB3.00dBSDR Noise Figure (dB) from AD9363 datasheet
6.08 NFsdr = lin(NFsdrdB)2.00SDR Noise Figure from AD9363 datasheet
 
7. System Noise Temperatures:
 
LineParameterValueUnitsComments
7.01 T0290.0KStandard reference temperature
7.02 Ts36.0KSky Noise Temperature from ITU-R P.372-14 (Worst case)
7.03 Tg = T0290.0KGround Noise Temperature from ITU-R P.372-14 (Worst case)
7.04 Tlna = T0*(NFlna-1)24.3KLNA Noise Temperature
7.05 Tfil = T0*((1/Gfil)-1)26.1KFilter Noise Temperature
7.06 Tsdr = T0*(NFsdr-1)288.6KSDR Noise Temperature
7.07 Tr = Tlna + Tfil/Glna + Tsdr/(Glna*Gfil)35.1KReceiver Noise Temperature
7.08 Ta = (n_spill*Ts)+((1-n_spill)*Tg)45.0KAntenna Noise Temperature
7.09 Tsys = Ta + Tr80.1KSystem Noise Temperature
7.10 TsysdB = dB(Tsys)19.0dB/KSystem Noise Temperature (dB/K)
 
8. System Figure of Merit:
 
LineParameterValueUnitsComments
8.01 GdB = dB(4*pi*A/(l**2))31.0dBGain of the dish (dB)
8.02 G = lin(GdB)1253.9Gain of the dish
8.03 GT = G/Tsys15.7/KG/T of the system
8.04 GTdB = GdB-TsysdB11.9dB/KG/T of the system (dB/K)
 
9. Estimate the SNNR of the Artemis downlink from the Moon:
 
LineParameterValueUnitsComments
9.01 r405696000mMax range to moon
9.02 FSPL = (l/(4*pi*r))**27.0e-22Free Space Path Loss
9.03 FSPLdB = dB(FSPL)-211.5Free Space Path Loss
9.04 B4000000HzBandwidth of receiver
9.05 SNNR = 2*(Pt*FSPL*GT/(k*B))+11.3SNNR
9.06 SNNRdB = dB(SNNR)1.22dBSNNR (dB)