Joule to Erg

Joule was the first to prove experimentally that heat and mechanical work are the same thing — he measured the temperature rise of water churned by a falling weight. That 1845 brewery-funded experiment settled a centuries-old debate and earned the SI energy unit his name in 1889, well before units were named after Einstein or Feynman.

Exactly 3,600,000 joules. A kilowatt-hour is simply 1,000 watts sustained for 3,600 seconds. Utilities chose kWh because quoting home energy use in megajoules (e.g., "your fridge used 129.6 MJ this month") would confuse most customers.

Lifting a medium apple one meter off the ground takes roughly 1 J. Clicking a computer mouse uses about 1.5 mJ (0.0015 J), a heartbeat expends ~1 J, and a single typed keystroke on a mechanical keyboard is around 10–40 mJ. A joule is a surprisingly tiny amount of energy at human scale.

A joule measures total energy; a watt measures the rate of energy flow (power). One watt equals one joule per second. A 60 W lightbulb consumes 60 joules every second — leave it on for an hour and it uses 216,000 J (0.06 kWh). Think of joules as liters of water and watts as the flow rate of the tap.

One thermochemical calorie equals exactly 4.184 joules. The "calorie" on food labels is actually a kilocalorie (4,184 J). So a 2,000-Calorie daily diet supplies about 8.4 million joules — enough energy to lift a small car roughly 850 meters straight up, if your body were 100% efficient (it is not).

Astrophysics literature built decades of reference data in CGS units before SI became dominant. Key constants like solar luminosity (3.828 × 10³³ erg/s) and supernova energy (10⁵¹ erg, called a "foe") are baked into textbooks and databases. Switching to SI would require rewriting thousands of reference values, so the field maintains CGS by convention.

A core-collapse supernova releases roughly 3 × 10⁵³ ergs total, of which about 99% escapes as neutrinos. The visible light and kinetic energy of the ejected shell account for about 10⁵¹ ergs — a unit so common in astrophysics it has its own name: one "foe" (ten to the Fifty-One Ergs). In joules, that is 10⁴⁴ J, or the Sun's total output over 10 billion years.

An erg per second is the CGS unit of power, equivalent to 10⁻⁷ watts. Astronomers quote stellar luminosities in ergs per second because the numbers align well with astrophysical scales: the Sun emits 3.846 × 10³³ erg/s, and supernovae peak at ~10⁴³ erg/s. Using watts would give the same exponents minus seven — less tidy for a field that already juggles 40-digit numbers daily.

CGS (centimeter-gram-second) is a metric system that predates SI, formalised in the 1870s. It derives mechanical units from cm, g, and s: force in dynes (g·cm/s²) and energy in ergs (dyne·cm). CGS was standard in physics until the mid-20th century, and its Gaussian variant remains preferred in electromagnetism and astrophysics because Maxwell's equations take a simpler form.

One erg is 10⁻⁷ joules — roughly the kinetic energy of a mosquito in flight or the energy of a single grain of sand falling one centimeter. You would need about 10 million ergs to equal one joule, or 42 billion ergs to match the energy in a single dietary Calorie. The erg is useful precisely because atomic and astronomical quantities span so many orders of magnitude.