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This list compares various in (J), organized by order of magnitude.

Below 1 J
+ List of orders of magnitude for ! Factor (joules) ! SI ! Value ! Item
10−35  Optical dipole potential measured in a tune-out experiment with ultracold metastable helium.
of a with a of 1 .
Average kinetic energy of translational motion of a at the lowest temperature reached (38 Calculated: KE = (3/2) × Boltzmann constant × Temperature )
10−28 6.6×10−28JEnergy of a typical photon (1 MHz) (4×10−9 )Calculated: E = hν = 6.626J-s × 1 Hz = 6.6J. In eV: 6.6J / 1.6J/eV = 4.1 eV.
(yJ)1.6×10−24JEnergy of a typical photon (2.45 GHz) (1×10−5 )Calculated: E = hν = 6.626J-s × 2.45 Hz = 1.62J. In eV: 1.62J / 1.6J/eV = 1.0 eV.
Average kinetic energy of translational motion of a molecule in the , the coldest place known outside of a laboratory, at a temperature of 1 Calculated: KE ≈ (3/2) × T × 1.38 = (3/2) × 1 × 1.38 ≈ 2.07J
10−22 2–3000×10−22JEnergy of light photons
10−21 (zJ)1.7×10−21J1kJ/mol, converted to energy per moleculeCalculated: 1J / 6.022 entities per mole = 1.7J per entity
2.1×10−21J in each degree of freedom of a molecule at 25 °C ( k T/2) (0.01 )Calculated: 1.381J/K × 298.15 K / 2 = 2.1J
2.856×10−21JBy Landauer's principle, the minimum amount of energy required at 25 °C to change one bit of information
3–7×10−21JEnergy of a van der Waals interaction between atoms (0.02–0.04 eV)Calculated: 2 to 4kJ/mol = 2J / 6.022 molecules/mol = 3.3J. In eV: 3.3J / 1.6J/eV = 0.02 eV. 4J / 6.022 molecules/mol = 6.7J. In eV: 6.7J / 1.6J/eV = 0.04 eV.
4.1×10−21JThe " k T" constant at 25 °C, a common rough approximation for the total of each molecule in a system (0.03 eV)
7–22×10−21JEnergy of a (0.04 to 0.13 eV)Calculated: 4 to 13kJ/mol. 4kJ/mol = 4J / 6.022 molecules/mol = 6.7J. In eV: 6.7J / 1.6 eV/J = 0.042 eV. 13kJ/mol = 13J / 6.022 molecules/mol = 2.2J. In eV: 13J / 6.022 molecules/mol / 1.6 eV/J = 0.13 eV.
10−20 4.5×10−20JUpper bound of the mass–energy of a in (0.28 eV)Calculated: 0.28 eV × 1.6J/eV = 4.5J
10−19 1 (eV) by definition. This value is exact as a result of the 2019 revision of SI units.
Energy range of in (≈1.6–3.1 eV)Calculated: E = hc/λ. E = 6.6 kg-m/s × 3 m/s / (780 m) = 2.5J. E_390 _nm = 6.6 kg-m/s × 3 m/s / (390 m) = 5.1J
3–14×10−19JEnergy of a (2–9 eV)Calculated: 50 kcal/mol × 4.184J/calorie / 6.0e23 molecules/mol = 3.47J. (3.47J / 1.60 eV/J = 2.2 eV.) and 200 kcal/mol × 4.184J/calorie / 6.0e23 molecules/mol = 1.389J. (7.64J / 1.60 eV/J = 8.68 eV.)
5–200×10−19JEnergy of light photons
10−18 (aJ)1.78×10−18JBond dissociation energy for the carbon monoxide (CO) triple bond, alternatively stated: 1072 kJ/mol; 11.11eV per molecule. This is the strongest chemical bond known.
Ground state ionization energy of (13.6 eV)
10−17 2–2000×10−17JEnergy range of photons
 
Average kinetic energy of one human red blood cell.Calculated: 1/2 × 27 g × (3.5 miles per hour) = 3J
10−14 1×10−14J (vibration) transmitted to the by listening to a for one second.. "The eardrum is a ... membrane with an area of 65 mm2."Calculated: two eardrums ≈ 1 cm2. 1 W/m2 × 1 m2 × 1 s = 1J
> 2×10−14JEnergy of photons
Upper bound of the mass–energy of a
(2025). 9789810238872, World Scientific. .
Calculated: 170 eV × 1.6J/eV = 2.7J
Rest mass–energy of an (0.511 MeV)
10−13 1 (MeV)
Energy released by a single event of two fusing into (1.44 megaelectronvolt MeV)
Kinetic energy of produced by , used to trigger fission (14.1 MeV)
10−11 Average total energy released in the of one uranium-235 (215 MeV)
10−10 1.492×10−10JMass-energy equivalent of 1 Da (931.5 MeV)
Rest mass–energy of a (938.3 MeV)
Rest mass–energy of a (939.6 MeV)
1 (GeV)
Rest mass–energy of a
Rest mass–energy of an
Energy required to raise a grain of by 0.1mm (the thickness of a piece of paper).Calculated: 7 g × 9.8 m/s2 × 1 m
10−9 (nJ)10 GeV
Initial operating energy per beam of the Large Electron Positron Collider in 1989 (50 GeV)Calculated: 50 eV × 1.6J/eV = 8J
10−8 Mass–energy of a (80.4 GeV)
Mass–energy of a (91.2 GeV)
100 GeV
Mass–energy of the (125.1 GeV)
Operating energy per proton of the Super Proton Synchrotron accelerator in 1976Calculated: 400 eV × 1.6J/eV = 6.4J
10−7 ≡ 1
1 TeV (teraelectronvolt), about the kinetic energy of a flying
Energy per proton in the Large Hadron Collider in 2015 (6.5 TeV)Calculated: 6.5 eV per beam × 1.6J/eV = 1.04J
 
Energy released by a typical in 1 hour (1 μCi × 4.871 MeV × 1 hr)
Energy released by a P100 in 1 hour (2.4 V × 350 nA × 1 hr)
Use of a typical LED for 1 second (2.0 V × 20 mA × 1 s)
10−1 (dJ)Energy of an American half-dollar falling 1 metreCalculated: m×g×h = 11.34 kg × 9.8 m/s × 1 m = 1.1J

1 to 105 J
+ List of orders of magnitude for ! Factor (joules) ! SI ! Value ! Item
100J≡ 1 N·m (newton–)
≡ 1 W·s (-second)
Kinetic energy produced as an extra small apple (~100 grams) falls 1 against Earth's Calculated: m×g×h = 1 kg × 9.8 m/s × 1 m = 1J
Energy required to heat 1 gram of dry, cool air by 1 degree
≈ 1 ft·lbf ()
≡ 1 thermochemical (small calorie)
≡ 1 International (Steam) Table calorie
Greisen-Zatsepin-Kuzmin theoretical upper limit for the energy of a coming from a distant sourceCalculated: 5 eV × 1.6J/ev = 8J
101 (daJ)Flash energy of a typical pocket camera electronic flash @
The most energetic cosmic ray ever detected. Most likely a single proton traveling only very slightly slower than the speed of light.
102 (hJ)1.25×102JKinetic energy of a regulation (standard) baseball (5.1 oz / 145 g) thrown at 93 mph / 150 km/h (MLB average pitch speed).
Energy delivered by a biphasic external electric shock (), usually during adult cardiopulmonary resuscitation for .
Energy of a lethal dose of
Kinetic energy of an average person jumping as high as they canKinetic energy at start of jump = potential energy at high point of jump. Using a mass of 70 kg and a high point of 40 cm => energy = m×g×h = 70 kg × 9.8 m/s × 40 m = 274J
Energy to melt 1 g of
Kinetic energy of 800 gram thrown at > 30 m/s by elite javelin throwersCalculated: 1/2 × 0.8 kg × (30 m/s) = 360J
Energy output of a typical studio strobe light in a single flash
Use of a 10-watt flashlight for 1 minute
A power of 1 applied for 1 second
Kinetic energy of 7.26 kg thrown at 14.7 m/s by the world record holder Calculated: 1/2 × 7.26 kg × (14.7 m/s) = 784J
8.01×102JAmount of work needed to lift a man with an average weight (81.7 kg) one meter above Earth (or any planet with Earth gravity)
103 (kJ)≈ 1 British thermal unit (BTU), depending on the
Total received from the by 1 at the altitude of Earth's orbit per second ()
Energy to vaporize 1 g of into steam
can crusher pinch powerlabs.org – The PowerLabs Solid State Can Crusher!, 2002
Kinetic energy of world-record men's (7.26 kg thrown at 30.7 m/s in 1986)Calculated: 1/2 × 7.26 kg × (30.7 m/s) = 3420J
≡ 1 W·h (-hour)
Energy released by explosion of 1 gram of 4.2J/ton of TNT-equivalent × (1 ton/1 grams) = 4.2J/gram of TNT-equivalent
≈ 1 food (large calorie)
Muzzle energy of an , e.g. firing a .458 Winchester Magnum
8.5×103JKinetic energy of a regulation baseball thrown at the speed of sound (343m/s = 767mph = 1,235km/h. Air, 20°C).
Energy in an alkaline AA battery
104 Energy released by the of 1 gram of or
Energy released by the metabolism of 1 gram of
Energy released by the of 1 gram of
Kinetic energy of 1 gram of matter moving at 10 km/sCalculated: E = 1/2 m×v = 1/2 × (1 kg) × (1 m/s) = 5J.
105  of an at highway speeds (1 to 5 tons at or )Calculated: Using car weights of 1 ton to 5 tons. E = 1/2 m×v = 1/2 × (1 kg) × (55 mph × 1600 m/mi / 3600 s/hr) = 3.0J. E = 1/2 × (5 kg) × (55 mph × 1600 m/mi / 3600 s/hr) = 15J.

106 to 1011 J
+ List of orders of magnitude for ! Factor (joules) ! SI ! Value ! Item
106 (MJ) of a 2 vehicle at 32 metres per second (115 km/h or 72 mph)Calculated: KE = 1/2 × 2 kg × (32 m/s) = 1.0J
Approximate of a snack such as a (280 food calories)
= 1 kWh (kilowatt-hour) (used for electricity)
Energy released by explosion of 1 kilogram of
6.1×106JKinetic energy of the 4 kg APFSDS penetrator after being fired from a 120mm KE-W A1 cartridge with a nominal muzzle velocity of 1740 m/s.
Recommended food energy intake per day for a moderately active woman (2000 food calories)Calculated: 2000 food calories = 2.0 cal × 4.184J/cal = 8.4J
9.1×106JKinetic energy of a regulation baseball thrown at Earth's escape velocity (First cosmic velocity ≈ 11.186 km/s = 25,020 mph = 40,270 km/h).
107 1×107JKinetic energy of the armor-piercing round fired by the ISU-152 assault gunCalculated: 1/2 × m × v = 1/2 × 48.78 kg × (655 m/s) = 1.0J.
Recommended food energy intake per day for a moderately active man (2600 food calories)Calculated: 2600 food calories = 2.6 cal × 4.184J/cal = 1.1J
Kinetic energy of a 23 lb projectile fired by the Navy's mach 8 railgun.
3.7×107J$1 of electricity at a cost of $0.10/kWh (the US average retail cost in 2009)Calculated J per dollar: 1 million BTU/$28.90 = 1 BTU / 28.90 dollars × 1.055J/BTU = 3.65J/dollarCalculated cost per kWh: 1 kWh × 3.60J/kWh / 3.65J/dollar = 0.0986 dollar/kWh
4×107JEnergy from the combustion of 1 cubic meter of
4.2×107JCaloric energy consumed by on a daily basis during Olympic training
6.3×107JTheoretical minimum energy required to accelerate 1 kg of matter to from Earth's surface (ignoring atmosphere)
9×107JTotal mass-energy of 1 microgram of matter (25 kWh)
108 Kinetic energy of a 55 tonne aircraft at typical landing speed (59 m/s or 115 knots)
≈ 1 , depending on the temperature
≈ 1 Tour de France, or ~90 hours ridden at 5 W/kg by a 65 kg riderCalculated: 90 hr × 3600 seconds/hr × 5 W/kg × 65 kg = 1.1J
≈ Energy from burning 16 kilograms of oil (using 135 kg per barrel of light crude)
109 (GJ)Energy in an average bolt (thunder)
Magnetic stored energy in the world's largest toroidal superconducting magnet for the at , Geneva
Inflight 100-ton Boeing 757-200 at 300 knots (154 m/s)
Theoretical minimum amount of energy required to melt a tonne of steel (380 )Calculated: 380 kW-h × 3.6J/kW-h = 1.37J
Energy of an ordinary gasoline tank of a car. thepartsbin.com – Volvo Fuel Tank: Compare at The Parts Bin, 6 May 2012
Unit of energy in ,E_\text{P} = \sqrt{\frac{\hbar c^5}{G}} roughly the diesel tank energy of a mid-sized truck.
2.49×109JApproximate kinetic energy carried by American Airlines Flight 11 at the moment of impact with WTC 1 on September 11, 2001.
Inflight 125-ton Boeing 767-200 flying at 373 knots (192 m/s)
Approximate average amount of energy expended by a human heart over an 80-year lifetimeCalculated: 1.3J/s × 80 years × 3.16 s/year = 3.3J
3.6×109J= 1 MW·h (megawatt-hour)
Energy released by explosion of 1 .
Average annual energy usage of a standard Calculated: 1239 kWh × 3.6J/kWh = 4.5J
≈ 1 bboe (barrel of oil equivalent) Energy Units , by Arthur Smith, 21 January 2005
1010 Kinetic energy of an Airbus A380 at cruising speed (560 tonnes at 511 knots or 263 m/s)
≈ 1 toe (ton of oil equivalent)
Yield energy of a Massive Ordnance Air Blast bomb, the second most powerful non-nuclear weapon ever designedCalculated: 11 tons of TNT-equivalent × 4.184J/ton of TNT-equivalent = 4.6J
Energy consumed by the average U.S. automobile in the year 2000Calculated: 581 gallons × 125J/gal = 7.26J
≈ 1 MW·d (-day), used in the context of power plants (24 MW·h)Calculated: 1 watts × 86400 seconds/day = 8.6J
Total energy released in the of one gram of uranium-235Calculated: 3.44J/U-235-fission × 1 kg / (235 amu per U-235-fission × 1.66 amu/kg) = 8.82J
9×1010JTotal mass-energy of 1 milligram of matter (25 MW·h)
1011 1.1×1011JKinetic energy of a regulation baseball thrown at lightning speed (120 km/s = 270,000 mph = 435,000 km/h).
Approximate food energy consumed by an average human in an 80-year lifetime.Calculated: 2000 kcal/day × 365 days/year × 80 years = 2.4J

1012 to 1017 J
+ List of orders of magnitude for ! Factor (joules) ! SI ! Value ! Item
1012 (TJ)1.85×1012JGravitational potential energy of the Twin Towers, combined, accumulated throughout their construction and released during the collapse of the complex.Equation for calculating potential assumes that the towers' center of mass is located halfway along the building's height of ~416 meters.
3.4×1012JMaximum fuel energy of an Airbus A330-300 (97,530 liters of Jet A-1)Calculated: 97530 liters × 0.804 kg/L × 43.15 MJ/kg = 3.38J
3.6×1012J1 GW·h (-hour)Calculated: 1 watts × 3600 seconds/hour
4×1012JElectricity generated by one 20-kg fuel bundle assuming ~29% thermal efficiency of reactorCalculated: 7500 watt-days/tonne × (0.020 tonnes per bundle) × 86400 seconds/day = 1.3J of burnup energy. Electricity = burnup × ~29% efficiency = 3.8J
4.2×1012JChemical energy released by the detonation of 1 Calculated: 4.2J/ton of TNT-equivalent × 1 tons/megaton = 4.2J/megaton of TNT-equivalent
Energy contained in jet fuel in a Boeing 747-100B aircraft at max fuel capacity (183,380 liters of Jet A-1)Calculated: 183380 liters × 0.804 kg/L × 43.15 MJ/kg = 6.36J
1013 Energy of the maximum fuel an Airbus A380 can carry (320,000 liters of Jet A-1)Calculated: 320,000 L × 0.804 kg/L × 43.15  MJ/kg = 11.1J
Orbital kinetic energy of the International Space Station (417 tonnes at 7.7 km/s)Calculated: E = 1/2 m.v2 = 1/2 × 417000 kg × (7700m/s)2 = 1.2J
1.20×1013JOrbital kinetic energy of the Parker Solar Probe as it dives deep into the Sun's gravity well in December 2024, reaching a peak velocity of 430,000 mph.
Yield of the atomic bomb dropped on in World War II (15 kilotons)Calculated: 15 kt = 15 grams of TNT-equivalent × 4.2J/gram TNT-equivalent = 6.3J
Theoretical total mass–energy of 1 gram of matter (25 GW·h)
1014 1.8×1014JEnergy released by annihilation of 1 gram of and matter (50 GW·h)
Total energy released by the Chelyabinsk meteor.
Energy released by an average per day
1015 (PJ)Energy released by a severe
Yearly consumption in as of 2008Calculated: 288.6 kWh × 3.60J/kWh = 1.04J
Energy released by explosion of 1 Calculated: 4.2J/ton of TNT-equivalent × 1 tons/megaton = 4.2J/megaton of TNT-equivalent
1016 Estimated impact energy released in forming
Yearly electricity consumption in as of 2010Calculated: 3.02 kWh × 3.60J/kWh = 1.09J
6.3×1016JYield of , the most powerful nuclear weapon tested by the United States
7.9×1016JKinetic energy of a regulation baseball thrown at 99% the speed of light (KE = mc^2 × γ-1, where the Lorentz factor γ ≈ 7.09).
Mass–energy of 1 kilogram of matterCalculated: E = mc = 1 kg × (2.998 m/s) = 8.99J
1017 Seismic energy released by the 2004 Indian Ocean earthquake
Total energy from the that strikes the face of the each secondThe Earth has a cross section of 1.274×1014 and the is 1361 per square meter. Note, however, that because portions of Earth reflect light well, the actual energy absorbed is about 1.2*10^17 watts, from an average albedo of 0.3.
Yield of the , the most powerful ever tested (50 megatons)Calculated: 50 tons TNT-equivalent × 4.2J/ton TNT-equivalent = 2.1J
2.552×1017JTotal energy of the 2022 Hunga Tonga–Hunga Haʻapai eruptionCalculated to be 61 megatons of TNT, equivalent to 2.552J
Yearly electricity consumption of as of 2008Calculated: 115.6 kWh × 3.60J/kWh = 4.16J
Energy needed to accelerate one ton of mass to 0.1c (~30,000 km/s)
Estimated energy released by the eruption of the Indonesian volcano, Krakatoa, in 1883
(1989). 9780231066679, Columbia University Press. .
Calculated: 200 tons of TNT equivalent × 4.2J/ton of TNT equivalent = 8.4JThis value appears to be referred only to the third explosion on 27 August, 10.02 a.m.

According to reports, the third explosion was by far the largest; it is associated to the biggest sound in the recorded history, the highest tsunami during the eruption and the most powerful shock waves rounded the world several times. 200 Megatons of TNT are often referred as the total energy released by the entire eruption, but it's plausible that are rather the energy released by the single third explosion, considering the effects.[4][5]

1018 to 1023 J
+ List of orders of magnitude for ! Factor (joules) ! SI ! Value ! Item
1018 (EJ)Worldwide nuclear-powered electricity output in 2023.
1019 1×1019JThermal energy released by the 1991 Pinatubo eruption
1.1×1019JSeismic energy released by the 1960 Valdivia Earthquake
1.2×1019JExplosive yield of global nuclear arsenal (2.86 Gigatons)
Yearly electricity consumption in the as of 2009Calculated: 3.741 kWh × 3.600J/kWh = 1.347J
Yearly electricity production in the as of 2009Calculated: 3.953 kWh × 3.600J/kWh = 1.423J
Energy released in 1 day by an average in producing rain (400 times greater than the wind energy)
Yearly electricity consumption of the world Calculated: 17.8 kWh × 3.60J/kWh = 6.41J
Yearly electricity generation of the world Calculated: 18.95 kWh × 3.60J/kWh = 6.82J
1020 1.4×1020JTotal energy released in the 1815 Mount Tambora eruption
2.33×1020JKinetic energy of a carbonaceous chondrite meteor 1 km in diameter striking Earth's surface at 20 km/s. Such an impact occurs every ~500,000 years.
2.4×1020JTotal latent heat energy released by Hurricane Katrina
Total world annual energy consumption in 2010Calculated: 12002.4 tonnes of oil equivalent × 42J/tonne of oil equivalent = 5.0J
6.2×1020JWorld generation in 2023 (620 EJ). "2023 saw a second consecutive record year for global primary energy consumption as it grew by 2%, reaching 620 EJ."
Estimated global resources for generating electricity 2005Final number is computed. Energy Outlook 2007 shows 15.9% of world energy is nuclear. IAEA estimates conventional uranium stock, at today's prices is sufficient for 85 years. Convert billion kilowatt-hours to joules then: 6.25×1019×0.159×85 = 8.01×1020.
1021 (ZJ)Estimated energy contained in the world's reserves as of 2010Calculated: "6608.9 trillion cubic feet" => 6608.9 billion cubic feet × 0.025 million tonnes of oil equivalent/billion cubic feet × 1 tonnes of oil equivalent/million tonnes of oil equivalent × 42J/tonne of oil equivalent = 6.9J
7.0×1021JThermal energy released by the Toba eruption
Estimated energy contained in the world's reserves as of 2010Calculated: "188.8 thousand million tonnes" => 188.8 tonnes of oil × 42J/tonne of oil = 7.9J
Annual net uptake of thermal energy by the global ocean during 2003-2018Calculated per reference: 0.58W·m−2 is 9.3J·yr−1 in the global domain
1022 1.2×1022JSeismic energy of a magnitude 11 earthquake on Earth (M 11)
Total energy from the Sun that strikes the face of the Earth each dayCalculated: 1.27 m × 1370 W/m × 86400 s/day = 1.5J
1.94×1022JImpact event that formed the , the largest impact structure in
Estimated energy contained in the world's reserves as of 2010Calculated: 860938 million tonnes of coal => 860938 tonnes of coal × (1/1.5 tonne of oil equivalent / tonne of coal) × 42J/tonne of oil equivalent = 2.4J
Identified global uranium-238 resources using fast reactor technology
Estimated energy contained in the world's reserves as of 2010Calculated: natural gas + petroleum + coal = 6.9J + 7.9J + 2.4J = 3.9J
8.03×1022JTotal energy of the 2004 Indian Ocean earthquake
1023 1.5×1023JTotal energy of the 1960 Valdivia earthquake
Total global uranium-238 resources using fast reactor technology
The energy released in the formation of the in the Yucatán Peninsula

Over 1024 J
+ List of orders of magnitude for ! Factor (joules) ! SI ! Value ! Item
1024 (YJ)2.31×1024JTotal energy of the
2.69×1024JRotational energy of Venus, which has a sidereal period of (-)243 Earth days.Clarification of calculation:

Rotational energy = (defined equal to) 1/2 * Moment of Inertia Factor * Mass * Radius^2 * Angular Velocity^2

The inertial factor has been normalized, and takes on a value between 0 and 1. In this case it is 0.337(24).

3.8×1024JRadiative heat energy released from the 's surface each year
Total energy from the that strikes the face of the each yearCalculated: 1.27 m × 1370 W/m × 86400 s/day = 5.5J
1025 4×1025JTotal energy of the in 1859
1026 Estimated energy of early
3.2×1026JBolometric energy of 's superflare in March 2016 (10^33.5 erg). In one year, potentially five similar superflares erupts from the surface of the red dwarf.
Total radiative energy output of the each second
Estimated energy released by the impact that created the on Mercury
1×1027JUpper limit of the most energetic possible (X1000)
5.19×1027JThermal input necessary to evaporate all surface water on Earth. Note that the evaporated water still remains on Earth, merely in vapor form.
4.2×1027JKinetic energy of a regulation baseball thrown at the speed of the Oh-My-God particle, itself a cosmic ray proton with the kinetic energy of a baseball thrown at 60mph (~50J).
Kinetic energy of the in its orbit around the Earth (counting only its velocity relative to the Earth)Calculated: KE = 1/2 × m × v. v = 1.023 m/s. m = 7.349 kg. KE = 1/2 × (7.349 kg) × (1.023 m/s) = 3.845J.
7×1028JTotal energy of the from V1355 Orionis
Rotational energy of the Calculated: E_rotational = 1/2 × I × w = 1/2 × (8.0 kg m) × (2×pi/(23.9345 hour period × 3600 seconds/hour)) = 2.1J
Rough estimate of the gravitational binding energy of Mercury.
1031 2×1031JThe Theia Impact, the most energetic event ever in Earth's history
Total energy output of the each dayCalculated: 3.8J/s × 86400 s/day = 3.3J
Gravitational binding energy of the Earth
3.10×1032JYearly energy output of Sirius B, the ultra-dense and Earth-sized white dwarf companion of , the Dog Star. It has a surface temperature of about 25,200 K.
kinetic energy at perihelion in its orbit around the SunKE = 1/2 × 5.9722×10^24 kg × (30.29 km/s)^2 = 2.74×10^33 J
Total energy output of the each yearCalculated: 3.8J/s × 86400 s/day × 365.25 days/year = 1.2J
1035 3.5×1035JThe most energetic to date (V2487 Ophiuchi)
1038 7.53×1038JBaryonic (ordinary) mass-energy contained in a volume of one cubic light-year, on average.
1039   2–5×1039 J

Energy of the giant flare (starquake) released by SGR 1806-20
Theoretical total mass–energy of the
1040   1.61×1040JBaryonic mass-energy contained in a volume of one cubic parsec, on average.
1041 Gravitational binding energy of the U = \frac{(3/5)GM^2}{r}Chandrasekhar, S. 1939, An Introduction to the Study of Stellar Structure (Chicago: U. of Chicago; reprinted in New York: Dover), section 9, eqs. 90–92, p. 51 (Dover edition)Lang, K. R. 1980, Astrophysical Formulae (Berlin: Springer Verlag), p. 272
Theoretical total mass–energy of the
1043 5×1043JTotal energy of all gamma rays in a typical if collimated "the gamma-ray energy release, corrected for geometry, is narrowly clustered around 5 × 10 erg"Calculated: 5 erg × 1J/erg = 5J
>1043 JTotal energy in a typical fast blue optical transient (FBOT)
1044 ~1044 JAverage value of a Tidal Disruption Event (TDE) in / bands
~1044 JEstimated kinetic energy released by FBOT CSS161010
Total energy released in a typical , sometimes referred to as a foe.
Approximate lifetime energy output of the .
Total energy of a typical gamma-ray burst if collimated
1045 ~1045 JEstimated energy released in a and pair instability supernova
1045 JEnergy released by the energetic supernova, SN 2016aps
Energy released by hypernova ASASSN-15lh
2.3×1045 JEnergy released by the energetic supernova PS1-10adiBoth ASSASN-15lh and PS1-10adi are indicated as supernovae and probably they are; actually, other mechanisms are proposed to explain them, more or less in accordance to the characteristics of supernovae
>1045 JEstimated energy of a magnetorotational hypernova
Total (energy in gamma rays+relativistic kinetic energy) of hyper-energetic if collimated
>1046JEstimated energy in theoretical
~1046JUpper limit of the total energy of a supernova
1.5×1046JTotal energy of the most energetic optical non- transient, AT2021lwx
1047 1045-47 JEstimated energy of stellar mass rotational black holes by vacuum polarization in an electromagnetic field
1047 JTotal energy of a very energetic and relativistic jetted Tidal Disruption Event (TDE)
~1047 JUpper limit of collimated- corrected total of a gamma-ray burst
Theoretical total mass–energy of the
Mass–energy emitted as gravitational waves during the merger of two , originally about 30 Solar masses each, as observed by (GW150914)
Mass–energy emitted as gravitational waves during the most energetic black hole merger observed until 2020 (GW170729)If GW190521 is a merging, the present one remains the largest. See note 246247
GRB 080916C – formerly the most powerful gamma-ray burst (GRB) ever recorded – total/trueIt is important to specify that the energetic reduction for beaming (invoked to explain so much energetics and jet breaks) is expected in the "Fireball model", which is the traditional one; other main models explain both Long and Short GRBs with binary systems, such as "Induced Gravitational Collapse", "Binary-Driven Hypernovae" which refer to the "Fireshell" one, in which cases the beaming isn't assumpted and the isotropic energy is a real value of energy due to the rotational energy of the stellar black hole and vacuum polarization in an electromagnetic field, which are able to explain energetics up and over 1047 J isotropic energy output estimated at 8.8 × 1047 joules (8.8 × 1054 erg), or 4.9 times the Sun's mass turned to energy
1048 1048 JEstimated energy of a supermassive Population III star supernova, denominated "General Relativistic Instability Supernova."
~1.2×1048 J

Approximate energy released in the most energetic black hole merging to date (GW190521), which originated the first intermediate-mass black hole ever detectedAssuming the uncertainties about the masses of the objects, the values of the LIGO Data are taken in consideration; so we have a newborn black hole with about 142 solar masses and the conversion in gravitational waves of about 7 solar massesA research claims that this is instead a merging with approximately 8 times more probability than the black hole case; if so, the existence and the collision of boson stars there would be confirmed together. Furthermore, the energy released and the distance would be reduced.[6]

See the following note for the link of the research

1.2–3×1048 JGRB 221009A – the most powerful gamma-ray burst (GRB) ever recorded – total/true isotropic energy output estimated at 1.2–3 × 1048 joules (1.2–3 × 1055 erg)
1050 ≳1050 JUpper limit of isotropic energy (Eiso) of Population III stars Gamma-Ray Bursts (GRBs).
1053 >1053 JMechanical energy of very energetic so-called " tsunamis"To determinate this value, the maximum energy of 1047 J for gamma-ray burts is taken in consideration; then six orders of magnitude are added, equivalent to ten million of years, the time frame in which the quasar tsunami will exceed the GRBs energetics over 1 million of times, according to the Nahum Arav's statement in the previous note
Total mechanical or in the powerful AGN outburst in the RBS 797
7.65×1053JMass-energy of Sagittarius A*, Milky Way's central supermassive black hole
1054Total mechanical or in the powerful AGN outburst in the Hercules A (3C 348)
Total mechanical or in the powerful AGN outburst in the MS 0735.6+7421, Ophiucus Supercluster Explosion and supermassive black holes mergings
1057 ~1057 JEstimated rotational energy of M87 SMBH and total energy of the most luminous over time-scales
~2×1057 JEstimated of the of
7.3×1057 JMass-energy equivalent of the ultramassive black hole TON 618, an extremely luminous quasar / active galactic nucleus (AGN).
1058 ~1058 JEstimated total energy (in shockwaves, turbulence, gases heating up, gravitational force) of mergings
Visible mass–energy in our , the
Total mass–energy of our , the , including and
1.4×1059JMass-energy of the (M31), ~0.8 trillion .
Total mass–energy of the Virgo Supercluster including , the which contains the
Rough estimate of total mass–energy of ordinary matter (atoms; baryons) present in the observable universe.Details of calculation: WMAP 10 year survey's estimate of mass-energy density * volume of Observable Universe * percentage of which is ordinary matter: 9.9e-30 * 3.566e+80 * 0.046 * c^2 = 1.46e+70 Joules.
1071 3.177×1071JRough estimate of total mass-energy within our observable universe, accounting for all forms of matter and energy.

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