"Why Everything Burns: The Science of Combustion and Energy"

After everything in this series — the chain reactions, the fluid dynamics, the spectroscopy, Faraday's candle — you might think combustion science is a solved problem. After all, humans have been burning things for 400,000 years. We've been studying the chemistry for 200 years. We can simulate combustion on computers.

We don't fully understand it.

Not in all the ways that matter for engineering and climate and fundamental chemistry.

## The soot problem

Soot — those tiny carbon particles that glow orange in a candle flame — is one of the most studied and least understood products of combustion.

We know soot begins as small aromatic molecules called **polycyclic aromatic hydrocarbons (PAHs)** that form in fuel-rich, oxygen-poor zones of the flame. These grow into clusters, then into nanoparticles, then into the fractal aggregates that make up visible soot.

But the growth kinetics are not well characterized. The exact pathways from the first ring-forming reactions to mature soot particles involve hundreds of possible reaction routes, many of which have rate constants we can only estimate. State-of-the-art combustion simulations use simplified soot models that are acknowledged to have substantial uncertainty.

This matters because **soot is the second most important climate forcer after CO₂** (by warming effect), it's a major health hazard (ultrafine particles penetrate deep into lung tissue), and understanding soot formation is critical to making cleaner diesel engines, gas turbines, and industrial furnaces.

> 🔬 **Quick experiment:** Hold a piece of white paper a few centimeters above a candle flame (well above — don't ignite it) and then bring it into the flame briefly. You'll see a black smudge of soot deposit. That smudge is nanoparticles of partially oxidized carbon — the same particles that, at a fine enough scale, lodge in lung tissue.

## Turbulent combustion modeling

Most practical combustion happens in turbulent regimes: gas turbine engines, diesel engines, furnaces, rocket engines. Turbulence dramatically increases mixing of fuel and oxidizer, which is why turbulent flames burn more completely and at higher intensity than laminar ones.

But turbulent combustion is extraordinarily difficult to model from first principles. The range of length scales involved — from the centimeter-scale flow structures down to the Kolmogorov microscale where molecular diffusion dominates — spans many orders of magnitude. You cannot resolve all of this in a simulation.

Current engineering models use turbulence closures — mathematical approximations — that work well for the conditions they were calibrated on, but fail in novel operating regimes (like the ultra-lean combustion needed for low-emission engines, or the extreme pressures in advanced rocket engines).

This is an active area of both fundamental research and commercial urgency — the aeronautics and automotive industries depend on combustion models that are better than current ones.

## The origin-of-life angle

Oxidation reactions — slow combustion — may have played a role in the origin of life. Some origin-of-life theories propose that the first self-replicating molecules formed in environments with strong redox gradients (differences in oxidation-reduction potential) — like hydrothermal vents, where chemically reduced fluids from the crust meet oxidized ocean water.

In this framing, life didn't *avoid* oxidation chemistry — it *exploited* it, using the free energy available from controlled oxidation as the thermodynamic driver for the first metabolic reactions.

We don't know if this is how life began. But combustion chemistry and the chemistry of life are far less separate than our cultural compartmentalization of "fire" and "biology" suggests.

## Combustion and climate — the transition problem

Hydrocarbon combustion has powered civilization for 200 years. It has also been the primary driver of the atmospheric CO₂ increase that is now measurably altering Earth's climate system.

The challenge of the coming decades is not simply "stop burning things." It's harder than that. Global energy demand is still rising. Hundreds of millions of people are transitioning to energy access for the first time. And while renewable electricity can replace combustion for many applications, there remain hard-to-electrify sectors: long-haul aviation, high-temperature industrial processes (cement, steel), and certain shipping routes.

These sectors are actively exploring **green hydrogen** combustion (burns to water, no CO₂), **synthetic fuels** (carbon-neutral hydrocarbon combustion using captured CO₂ and renewable electricity), and **ammonia combustion** (nitrogen-based fuel with no carbon at all, though NOₓ emissions remain a problem).

All of these alternatives involve combustion — just with different fuels. The combustion science challenges for each are nontrivial. Hydrogen combustion, for example, produces a different radical pool than hydrocarbon combustion, requires different nozzle designs, and has significantly different flame stability characteristics.

## What Faraday would study today

If Faraday were alive in 2026 and chose to pick up a "simple" combustion problem to study — the way he once picked up a candle — he might choose to study the chemistry of soot nucleation at the molecular scale. Or the coupling between turbulence and radical kinetics. Or the metabolic oxidation pathways in the mitochondria as a form of slow combustion.

The questions that remain are genuinely hard. They are not merely engineering questions — they sit at the intersection of chemistry, physics, fluid dynamics, atmospheric science, and biology.

**Fire is still not fully understood.** And that makes it, after 400,000 years, still one of the most interesting phenomena in the universe.

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*This series covered: what fire fundamentally is → the misconceptions → molecular-level chemistry → fluid dynamics of flame shape → spectroscopy of flame color → slow combustion in biology and materials → Faraday's classic candle experiments → the open questions of combustion science today.*

*The candle on your table is not simple. It never was.*

"What We Still Don't Know — The Open Questions of Combustion Science"

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