ScienceMarch 30, 2026

Heat Transfer Calculator Guide: Conduction, Convection & Radiation

By The hakaru Team·Last updated March 2026

Quick Answer

  • *Heat transfers through three modes: conduction (direct contact), convection (fluid motion), and radiation (electromagnetic waves).
  • *Conduction rate is governed by Fourier's law: Q = k × A × ΔT / d, where k is thermal conductivity.
  • *Copper conducts heat 15,400× better than air (401 vs 0.026 W/m·K) — material choice drives everything.
  • *Radiation scales with T&sup4;, making it the dominant mode above roughly 500°C.

The Three Modes of Heat Transfer

Every heat transfer problem involves one or more of three fundamental mechanisms. Understanding which mode dominates your scenario determines which formula to use and which variables matter most.

ModeMechanismRequires Medium?Governing Law
ConductionMolecular vibration & electron transportYes (solid, liquid, or gas)Fourier's law
ConvectionBulk fluid motionYes (liquid or gas only)Newton's law of cooling
RadiationElectromagnetic wavesNo (works in vacuum)Stefan-Boltzmann law

According to the ASHRAE Handbook of Fundamentals (2025 edition), a typical residential wall loses heat through all three modes simultaneously: conduction through the wall material, convection from air films on both surfaces, and radiation between the wall and surrounding surfaces.

Conduction: Heat Through Solids

Conduction is heat transfer through direct molecular contact. In metals, free electrons carry most of the thermal energy. In non-metals, it's lattice vibrations (phonons). The governing equation is Fourier's law:

Q = k × A × (T<sub>hot</sub> – T<sub>cold</sub>) / d

Where:

  • Q = heat transfer rate (watts)
  • k = thermal conductivity (W/m·K)
  • A = cross-sectional area perpendicular to heat flow (m²)
  • ΔT = temperature difference (K or °C)
  • d = thickness of material (m)

Thermal Conductivity of Common Materials

Materialk (W/m·K)Category
Copper401Excellent conductor
Aluminum237Good conductor
Carbon steel50Moderate conductor
Stainless steel16Poor metal conductor
Glass1.0Insulator
Concrete0.8Insulator
Wood (oak)0.17Good insulator
Fiberglass insulation0.04Excellent insulator
Still air0.026Excellent insulator
Aerogel0.015Best known insulator

Notice the enormous range. Copper conducts heat over 10,000 times better than fiberglass insulation. This is why material selection dominates conduction problems. According to data from the Engineering Toolbox, the thermal conductivity values above are at approximately 25°C — conductivity varies with temperature, sometimes significantly.

Convection: Heat Through Fluid Motion

Convection occurs when a fluid (liquid or gas) moves past a surface at a different temperature. The governing equation is Newton's law of cooling:

Q = h × A × (T<sub>surface</sub> – T<sub>fluid</sub>)

Where his the convective heat transfer coefficient (W/m²·K). Unlike thermal conductivity, h is not a material property — it depends on fluid velocity, geometry, and flow regime.

ScenarioTypical h (W/m²·K)
Natural convection in air5–25
Forced convection in air25–250
Natural convection in water100–900
Forced convection in water250–10,000
Boiling water2,500–25,000
Condensing steam5,000–100,000

The jump from air to water is striking. Water's convective coefficient is roughly 10–100 times higher than air's for equivalent flow conditions. This is why water-cooled systems (from car engines to data center cooling) are so much more effective than air cooling. According to ASHRAE, liquid cooling in data centers can handle 3,000–4,000 watts per rackcompared to roughly 10–15 kW for air-cooled systems.

Natural vs Forced Convection

Natural (free) convection occurs when temperature differences create density gradients that drive fluid motion — hot air rises, cold air sinks. Forced convection uses an external mechanism (fan, pump, wind) to move the fluid. Forced convection is always more effective because higher fluid velocities increase h.

Radiation: Heat Without Contact

All objects above absolute zero emit thermal radiation. Unlike conduction and convection, radiation requires no medium — it's how the Sun heats the Earth across 150 million kilometers of vacuum.

The Stefan-Boltzmann law governs radiative heat exchange:

Q = ε × σ × A × (T⊂1</sub>&sup4; – T<sub>2</sub>&sup4;)

Where:

  • ε = emissivity of the surface (0 to 1)
  • σ = Stefan-Boltzmann constant (5.67 × 10&sup8; W/m²·K&sup4;)
  • T = absolute temperatures in Kelvin

The T&sup4; dependence is the key feature. Doubling the absolute temperature increases radiation by a factor of 16. This is why radiation is negligible in everyday low-temperature scenarios but dominates in furnaces, rocket engines, and astrophysics. According to NASA, the Space Shuttle's thermal protection tiles needed to handle surface temperatures exceeding 1,650°C during re-entry, where radiation was the primary heat transfer mode.

Emissivity Values

SurfaceEmissivity (ε)
Polished aluminum0.04–0.06
Polished copper0.03–0.05
Oxidized steel0.7–0.8
Black paint0.95–0.98
Human skin0.95–0.97
Water0.95–0.96
Snow/ice0.82–0.90

Polished metals reflect most thermal radiation (low emissivity), which is why emergency blankets use aluminized mylar — they reflect up to 97% of radiated body heat back to the person.

Composite Walls and Thermal Resistance

Real walls have multiple layers (drywall, insulation, sheathing, siding). Each layer adds thermal resistance. The concept mirrors electrical resistance in series:

R<sub>total</sub> = R<sub>1</sub> + R<sub>2</sub> + R<sub>3</sub> + ...

Where R = d/k for each layer. Then: Q = A × ΔT / R<sub>total</sub>

The U.S. Department of Energy recommends wall insulation values between R-13 and R-23 depending on climate zone. According to the DOE's 2025 energy efficiency data, proper insulation reduces heating and cooling energy use by up to 40% in residential buildings.

Real-World Applications

Building Energy Efficiency

HVAC engineers calculate heat loss through walls, windows, and roofs to size heating and cooling equipment. According to the U.S. Energy Information Administration (EIA), space heating and cooling account for 43% of total energy usein U.S. homes — making heat transfer calculations directly tied to energy costs.

Electronics Cooling

Modern CPUs generate thermal design powers (TDP) of 65–350 watts in a package smaller than a matchbook. Heat must transfer from the silicon die through thermal paste, a heat spreader, and finally a heatsink to the air. According to Intel's thermal design guides, the junction-to-ambient thermal resistance must stay below roughly 0.3°C/W for high-performance desktop processors.

Industrial Heat Exchangers

Shell-and-tube heat exchangers transfer heat between two fluids without mixing them. They're used in power plants, chemical processing, and HVAC systems. The global heat exchanger market was valued at $18.4 billion in 2024 according to Grand View Research, reflecting the critical role of heat transfer engineering in industry.

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Frequently Asked Questions

What are the three modes of heat transfer?

The three modes are conduction (heat transfer through direct molecular contact in solids or stationary fluids), convection (heat transfer through fluid motion — either natural or forced), and radiation (heat transfer through electromagnetic waves that requires no medium). Most real-world systems involve all three modes simultaneously.

What is thermal conductivity and what are common values?

Thermal conductivity (k) measures how well a material conducts heat, in watts per meter-kelvin (W/m·K). Copper has a k of 401 W/m·K (excellent conductor), aluminum is 237, steel is 50, glass is about 1, wood is 0.12–0.17 (poor conductor), and air is just 0.026 (good insulator).

What is the difference between conduction and convection?

Conduction transfers heat through direct contact between molecules without bulk material movement. Convection transfers heat through the movement of fluid (liquid or gas). A pot on a stove illustrates both: heat conducts through the metal pot bottom, then convection currents circulate hot water upward and cool water downward.

How do I calculate heat loss through a wall?

Use Fourier's law: Q = k × A × (T_hot – T_cold) / d, where k is the wall material's thermal conductivity, A is the wall area, T values are the surface temperatures, and d is the wall thickness. For composite walls with multiple layers, calculate the total thermal resistance (R = d/k for each layer) and use Q = A × ΔT / R_total.

What is the Stefan-Boltzmann law?

The Stefan-Boltzmann law calculates radiative heat transfer: Q = ε × σ × A × (T₁&sup4; – T₂&sup4;), where ε is the surface emissivity (0 to 1), σ is the Stefan-Boltzmann constant (5.67 × 10⁻&sup8; W/m²·K&sup4;), A is the surface area, and T values are absolute temperatures in Kelvin.