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The laws of thermodynamics

by simon

Thermodynamics are at the heart of our understanding of ecosystems and not an altogether difficult concept to grasp but one that isn’t widely taught to ecologists. Basically, all life on Earth, is derived from the Sun’s heat. This renewable energy source constantly bombards ecosystems with energy but they would overheat, if it wasn’t for the absorptive capacity of food webs.

The laws of nature that determine how this all works, were popularised by Einstein in the early 1900s.

The first law of thermodynamics states:

In a perfectly isolated system, energy can change from one form to another but can never be created or destroyed.

Energy contained within a system will never disappear, just alter from one state to another and redistribute itself in a different way.

The second law of thermodynamics states that

the total entropy of an isolated system can never decrease over time and is constant only if all processes are reversible. In other words, entropy forces energy to flow towards a state of greater chaos.

This last law is the most important.

There are two key principles to understand in this. The first is entropy. It’s a measure of the degree of disorder in molecules. Molecules that are inside biologically systems are highly ordered. A tree branch has minimum entropy because the carbon is locked up as a lattice. This cools the planet. When a log decays, you release molecules into the atmosphere and this energy heats the planet.

Plants are on the front line of energy capture, so their potential to emit waste energy and increase the entropy of Earth’s biosphere is huge. Left alone, plants would destabilise their own environment. Until that is, animals evolved. The ability of animals to move from place to place and absorb the free surplus energy created by plants, meant that ecosystems could reach a steady stable-state. That’s one way of saying, that the amount of heat reaching Earth from the Sun, and the amount of heat absorbed by ecosystems, roughly balanced.

This point was only reached quite recently, after a few hundred million years of animal evolution.

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