Barrels of Oil Equivalent to Erg

One BOE equals approximately 6.118 gigajoules, 1,700 kWh, or 5.8 million BTU. That is roughly the energy a US household uses in electricity over six weeks. The figure is a defined convention — actual crude oil barrels vary by 5–10% depending on whether it is light sweet crude or heavy sour crude.

Because modern energy companies produce oil, natural gas, and natural gas liquids. Reporting everything in BOE allows investors to compare total energy reserves across companies on one scale. Roughly 6,000 cubic feet of natural gas equals 1 BOE. Without this conversion, comparing an oil-heavy company to a gas-heavy one would be apples-to-oranges.

Global oil consumption in 2024 was approximately 102 million barrels per day — or about 102 million BOE/day just from oil. Including natural gas and coal, total world primary energy consumption is roughly 580 million BOE/day equivalent. The US alone accounts for about 20 million barrels per day.

A physical barrel of crude oil is 42 US gallons (~159 liters) of liquid petroleum. A BOE is a standardized energy unit pegged to the average energy content of that barrel (6.118 GJ). Light crudes like Brent may actually yield slightly more energy per barrel, while heavy crudes yield less. The BOE smooths out these differences for accounting purposes.

A typical EV driven 20,000 km/year consumes about 3,500 kWh, which is roughly 2 BOE of energy. A petrol car covering the same distance burns about 1,500 liters of fuel — approximately 9.5 BOE. The EV uses roughly one-fifth the primary energy, largely because electric motors are 85–95% efficient while combustion engines waste 60–75% as heat.

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.