chevron_left Universe: In thermodynamics, this refers to the system plus the surroundings chevron_right

Universe: In thermodynamics, this refers to the system plus the surroundings
Anna Kowalski
share
visibility52
calendar_month2025-12-01

The Thermodynamic Universe: More Than Stars and Galaxies

Understanding energy flow by defining everything that exists: the system, the surroundings, and the universe they create together.
Summary: In the science of thermodynamics, the word "universe" has a special, precise meaning. It doesn't refer to outer space, but to the complete picture of any energy interaction. To understand this, we break reality into two parts: the system (the specific part we are studying, like a cup of coffee or a car engine) and the surroundings (everything else that can exchange energy with it, like the air in the room or the road). The universe is simply the system plus the surroundings. This powerful idea helps us track where energy comes from and where it goes, governed by fundamental laws like the conservation of energy[1] and the increase in entropy[2]. Whether you're watching ice melt or charging a phone, you're observing the thermodynamic universe in action.

Defining the Players: System, Surroundings, and Universe

Imagine you are a scientist trying to solve a mystery. The first step is to decide what you are investigating. In thermodynamics, this is called defining the system. It's like drawing an imaginary boundary around the object or process you want to understand. Everything inside this boundary is the system. Everything outside this boundary is the surroundings. Together, they form the thermodynamic universe for your experiment.

Key Formula: The relationship is beautifully simple: $\text{Universe} = \text{System} + \text{Surroundings}$. This equation is the foundation for analyzing all energy changes.

Systems can be classified based on how they interact with their surroundings across the boundary:

System TypeCan Exchange Matter?Can Exchange Energy?Everyday Example
Open SystemYesYesA boiling pot of water (steam leaves, heat enters).
Closed SystemNoYesA sealed, insulated water bottle (water stays, but it can get warm or cold).
Isolated SystemNoNoA theoretical "perfect" thermos (nothing gets in or out). The universe itself is considered the only truly isolated system.

The choice of system boundary is up to the scientist. For example, if you are studying an ice cube melting on a plate, your system could be just the ice cube (an open system, as water melts away). The surroundings are the plate and the air. The "universe" is both. This framework lets us focus on where the energy is moving.

The Laws Governing the Thermodynamic Universe

The concept of a thermodynamic universe is crucial because it is the stage upon which the fundamental laws of thermodynamics play out. These laws describe absolute rules for energy and disorder.

The First Law: Conservation of Energy in the Universe. This law states that energy cannot be created or destroyed; it can only change forms or be transferred. For the thermodynamic universe (system + surroundings), the total energy always remains constant. If the system gains energy, the surroundings must lose exactly that same amount, and vice versa.

Mathematically, we often write the First Law for a system as: $\Delta U = Q - W$. Here, $\Delta U$ is the change in the system's internal energy, $Q$ is the heat added to the system from the surroundings, and $W$ is the work done by the system on the surroundings. This equation explicitly shows the energy exchange across the boundary.

The Second Law: The Direction of Change and Entropy. This law introduces the concept of entropy, a measure of disorder or randomness. It states that for any spontaneous process, the total entropy of the thermodynamic universe always increases.

Second Law Formula: For any real process, $\Delta S_{universe} = \Delta S_{system} + \Delta S_{surroundings} > 0$. This "greater than zero" is what gives time its arrow—ice melts in warm air but doesn't spontaneously form from a puddle in the same warm air.

The Second Law explains why some processes are one-way. When you drop a hot rock into a cool lake (system: rock, surroundings: lake), heat flows from the rock to the lake until temperatures equalize. The entropy of the rock decreases as it cools, but the entropy of the lake increases by a larger amount. The total entropy of the universe increases.

Tracking Energy Flow in Everyday Events

Let's apply the "system + surroundings = universe" model to familiar situations to see how energy is accounted for.

Example 1: A Campfire on a Cold Night.

  • System: The burning wood and flames.
  • Surroundings: The cold air, the ground, and you sitting nearby.
  • Universe: All of the above.

The chemical energy stored in the wood (system) is converted into heat and light. This energy flows into the surroundings, warming the air and you. The First Law is obeyed: the chemical energy lost by the system equals the thermal and radiant energy gained by the surroundings. The Second Law is also obeyed: the highly ordered molecules in wood become dispersed gases and ash (more disorder), and the concentrated heat spreads out into the vast surroundings, greatly increasing the universe's total entropy.

Example 2: Charging a Smartphone Battery.

  • System: The smartphone battery.
  • Surroundings: The electrical outlet, the charger, and the room air.
  • Universe: All of the above.

Electrical work is done on the system (battery) by the surroundings (outlet). The battery's internal energy increases (it stores chemical potential energy). However, the process isn't 100% efficient. Some energy is lost as waste heat to the surroundings, making the charger warm. The First Law balances: Electrical energy in = Stored chemical energy + Waste heat. The Second Law dictates that even though we are "ordering" energy into the battery, the waste heat generated increases the entropy of the air more than the decrease in entropy from charging the battery, so the universe's entropy still increases.

Example 3: Photosynthesis in a Leaf.

  • System: The leaf (specifically, the chloroplasts inside its cells).
  • Surroundings: Sunlight, carbon dioxide from the air, water from the roots, and the rest of the plant.
  • Universe: All of the above.

This seems like it creates order (sugars from $CO_2$ and water), which might appear to decrease entropy. But we must consider the entire universe. The system (leaf) uses extremely high-energy, ordered photons from the sun. When sunlight is absorbed, it is converted to much lower-energy, disordered heat that radiates back into space. The massive increase in entropy from the sun's energy being degraded far outweighs the small local decrease in entropy from making sugar molecules. The total entropy of the universe increases, satisfying the Second Law.

Important Questions

Q: Is the "thermodynamic universe" the same as the "cosmological universe"?

A: Not exactly, but they are related. The cosmological universe (all of space, time, matter, and energy) is often modeled as an isolated thermodynamic system—or even the ultimate isolated system—because, by definition, there is nothing outside of it to exchange energy or matter with. So, the cosmological universe is the largest possible example of a thermodynamic universe where "system + surroundings" equals "everything that exists."

Q: Can the entropy of a system ever decrease?

A: Yes, but only if it causes an even larger increase in entropy elsewhere in the surroundings. For example, when your refrigerator cools food (decreasing the entropy inside the fridge), it must exhaust heat into your kitchen. The heating of the kitchen air increases its entropy. The key is that the total entropy change of the universe (fridge + kitchen) is positive. Localized order can be created, but always at the cost of greater disorder overall.

Q: Why is the "isolated system" mostly theoretical?

A: In practice, it's almost impossible to create a perfect isolated system because some tiny amount of energy (like heat or light) will always leak across any boundary. Even the best insulated thermos will let a little heat through over time. However, it's a very useful ideal model for simplifying calculations and thought experiments, much like a "frictionless surface" in physics.

Conclusion: The thermodynamic definition of the universe as system plus surroundings is a master key for unlocking how energy works in our world. It provides a clear, logical framework for analyzing everything from simple cooling to complex life processes. By drawing an imaginary boundary to define our system, we can precisely track energy transfers with the First Law and understand the inevitable trend toward disorder described by the Second Law. This concept reminds us that no process happens in isolation; every change in the part we study is mirrored by an opposite change in the environment. Learning to think in terms of this complete "universe" is a fundamental step in mastering the science of energy.

Footnote

[1] Conservation of Energy (First Law of Thermodynamics): A fundamental principle stating that the total energy of an isolated system remains constant; it is said to be conserved over time. Energy can neither be created nor destroyed, but only transformed from one form to another or transferred from one object to another.

[2] Entropy: A thermodynamic property that is a measure of the molecular disorder or randomness of a system. The Second Law of Thermodynamics states that the total entropy of the universe always increases for a spontaneous process.

[3] Spontaneous Process: A process that occurs without needing an ongoing external influence. It has a natural tendency to happen under a given set of conditions (e.g., heat flowing from hot to cold).

[4] Internal Energy (U): The total energy contained within a system. It is the sum of the kinetic and potential energies of all the particles (atoms and molecules) that make up the system.

Did you like this article?

home
grid_view
add
explore
account_circle