Engineering Calculator

Semi-empiricalASTM C740Real-time

Lockheed Equation Calculator

Predict MLI thermal performance using the most widely adopted semi-empirical correlation. Input your boundary conditions and get real-time heat flux predictions.

Interactive Calculator

Input Parameters

Enter your MLI system conditions below. The calculator computes total heat flux and breaks it into conduction, radiation, and gas conduction components.

Boundary Conditions

Quick presets:

MLI Configuration

Material & Atmosphere

Results

Total heat flux q (mW/m2)
Solid conduction
Radiation
Mean temperature Tm
Apparent emissivity

Equation Reference

The Lockheed Correlation

Standard (High Vacuum)

q = (Cs * N^2.56 * Tm * dT) / Ns + (Cr * e * (Th^4.67 - Tc^4.67)) / Ns

Valid for vacuum < 10-3 Pa. Separates heat flux into solid conduction and radiation components.

Extended (With Gas)

q_gas = Cg * P * (Th^0.52 - Tc^0.52) / Ns

For non-ideal vacuum. Adds gas conduction term scaled by interstitial pressure.

Correlation Parameters

Gask (300K) mW/(m·K)CgExpSource
N225.914,6000.52Lockheed empirical
He155.748,9000.26Lockheed empirical
H2186.648,9000.26Lockheed (same as He)
Air26.414,6000.52~ N2 (78% N2 + 21% O2)
CH434.4~20,0000.52Estimated from k ratio
CO216.6~9,3000.52Estimated from k ratio
Ar17.7~10,0000.52Estimated from k ratio
H2O (gas)35.8 *~10,1000.52Estimated; * condensation risk
Mixed (air)~26~14,6000.52Typical seal-failure composition

Note: Cg values marked "~" are estimated by scaling from Lockheed's empirical N2 data using thermal conductivity ratios at 300K (NIST REFPROP / Marcia L. Huber). Only N2, He, and H2 have direct Lockheed empirical data. Estimated values should be validated against test data for critical applications.

H2O Warning: Water vapor condenses/deposits on cryogenic surfaces below ~200K, forming ice layers with thermal conductivity of 150-400 mW/(m·K) — orders of magnitude higher than vapor. This phase-change effect cannot be captured by the linear Cg*P model. (The Aerospace Corp., SPIE 2025)

Mixed Gas Effects

In real MLI systems, the interstitial gas is rarely pure. Typical residual gas compositions after seal failure or during pump-down:

ScenarioDominant GasesEffective kKey Risk
Normal high vacuumH2O, CO2, H2 (trace)negligibleOutgassing from materials
Seal failure (air in)N2 (78%), O2 (21%), Ar (1%)~26 mW/(m·K)Rapid k_eff increase
He leak (from leak check)He + airdominated by HeHe has 6x higher k than air
LH2 systemH2 permeation + Hevery highH2 permeates through metals
LNG systemCH4 + N2moderate-highCH4 from cargo evaporation
Humid air ingressAir + H2O vapor~26 + condensationIce deposition on cold layers

Data sources: Gas thermal conductivities from NIST REFPROP (Marcia L. Huber); Lockheed empirical Cg from NASA/TM-2015-000199; Sun et al. MLI multi-gas experiments (Processes 2023, MDPI); NETZSCH GHP 456 measurements (2026); The Aerospace Corp. water vapor study (SPIE 2025, DOI: 10.1117/12.3065462); LNG tanker MLI data (MATEC ICCHMT 2018).

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