Orders Of Magnitude (energy)
This list compares various energies in joules (J), organized by order of magnitude.
Factor (Joules) | SI prefix | Value | Item |
---|---|---|---|
10−33 | 2×10−33 J | average kinetic energy of translational motion of a molecule at the lowest temperature reached, 100 picokelvins as of 2003 | |
10−28 | 6.6×10−28 J | energy of a typical AM radio photon (1 MHz) (4×10−9 eV) | |
10−24 | yocto- (yJ) | 1.6×10−24 J | energy of a typical microwave oven photon (2.45 GHz) (1×10−5 eV) |
10−23 | 2×10−23 J | average kinetic energy of translational motion of a molecule in the Boomerang Nebula, the coldest place known outside of a laboratory, at a temperature of 1 kelvin | |
10−22 | 2-3000×10−22 J | energy of infrared light photons | |
10−21 | zepto- (zJ) | 1.7×10−21 J | 1 kJ/mol, converted to energy per molecule |
2.1×10−21 J | thermal energy in each degree of freedom of a molecule at 25 °C (kT/2) (0.01 eV) | ||
2.85×10−21 J | By Landauer's principle, the minimum amount of energy required at 25 °C to change one bit of information. | ||
3-7×10−21 J | energy of a van der Waals interaction between atoms (0.02-0.04 eV) | ||
4.1×10−21 J | "kT" at 25 °C, a common rough approximation for the total thermal energy of each molecule in a system (0.03 eV) | ||
7-22×10−21 J | energy of a hydrogen bond (0.04 to 0.13 eV) | ||
10−20 | 4.5×10−20 J | upper bound of the mass-energy of a neutrino in particle physics (0.28 eV) | |
10−19 | 1.6×10−19 J | ≈1 electronvolt (eV) | |
3–5×10−19 J | energy range of photons in visible light | ||
3-14×10−19 J | energy of a covalent bond (2-9 eV) | ||
5-200×10−19 J | energy of ultraviolet light photons | ||
10−18 | atto- (aJ) | ||
10−17 | 2-2000×10−17 J | energy range of X-ray photons | |
10−16 | |||
10−15 | femto- (fJ) | ||
10−14 | > 2×10−14 J | energy of gamma ray photons | |
2.7×10−14 J | upper bound of the mass-energy of a muon neutrino | ||
8.2×10−14 J | rest mass-energy of an electron | ||
10−13 | 1.6×10−13 J | 1 megaelectronvolt (MeV) | |
10−12 | pico- (pJ) | 2.3×10−12 J | kinetic energy of neutrons produced by D-T fusion, used to trigger fission (14.1 MeV) |
10−11 | 3.4×10−11 J | average total energy released in the nuclear fission of one uranium-235 atom (215 MeV) | |
10−10 | 1.503×10−10 J | rest mass-energy of a proton | |
1.505×10−10 J | rest mass-energy of a neutron | ||
1.6×10−10 J | 1 gigaelectronvolt (GeV) | ||
3.0×10−10 J | rest mass-energy of a deuteron | ||
6.0×10−10 J | rest mass-energy of an alpha particle | ||
10−9 | nano- (nJ) | 1.6×10−9 J | 10 GeV |
8×10−9 J | initial operating energy per beam of the CERN Large Electron Positron Collider in 1989 (50 GeV) | ||
10−8 | 1.3×10−8 J | mass-energy of a W boson (80.4 GeV) | |
1.5×10−8 J | mass-energy of a Z boson (91.2 GeV) | ||
1.6×10−8 J | 100 GeV | ||
6.4×10−8 J | operating energy per proton of the CERN Super Proton Synchrotron accelerator in 1976 | ||
10−7 | 1×10−7 J | ≡ 1 erg | |
1.6×10−7 J | 1 TeV (teraelectronvolt), about the kinetic energy of a flying mosquito | ||
5.6×10−7 J | energy per proton beam in the CERN Large Hadron Collider in 2011 (3.5 TeV) | ||
10−6 | micro- (µJ) | ||
10−5 | |||
10−4 | |||
10−3 | milli- (mJ) | ||
10−2 | centi- (cJ) | ||
10−1 | deci- (dJ) | 1×10−1 J | energy of an American half-dollar falling 1 metre |
100 | J | 1 J | ≡ 1 N·m (newton–metre) |
1 J | ≡ 1 W·s (watt-second) | ||
1 J | kinetic energy produced as an extra small apple (~100 grams) falls 1 meter against Earth's gravity | ||
1 J | energy required to heat 1 gram of dry, cool air by 1 degree Celsius | ||
1.4 J | ≈ 1 ft·lbf (foot-pound force) | ||
4.184 J | ≡ 1 thermochemical calorie (small calorie) | ||
4.1868 J | ≡ 1 International (Steam) Table calorie | ||
8 J | Greisen-Zatsepin-Kuzmin theoretical upper limit for the energy of a cosmic ray coming from a distant source | ||
101 | deca- (daJ) | 1×101 J | flash energy of a typical pocket camera photoflash capacitor (100-400 µF @ 330 V) |
5×101 J | most energetic cosmic ray ever detected, in 1991 | ||
102 | hecto- (hJ) | 3×102 J | energy of a lethal dose of X-rays |
3×102 J | kinetic energy of an average person jumping as high as they can | ||
> 3.6×102 J | kinetic energy of 800 g standard men's javelin thrown at > 30 m/s by elite javelin throwers | ||
5-20×102 J | energy output of a typical photography studio strobe light in a single flash | ||
6.0×102 J | kinetic energy of 2 kg standard men's discus thrown at 24.4 m/s by the world record holder Jürgen Schult | ||
6×102 J | use of a 10-watt flashlight for 1 minute | ||
7.5×102 J | a power of 1 horsepower applied for 1 second | ||
7.8×102 J | kinetic energy of 7.26 kg standard men's shot thrown at 14.7 m/s by the world record holder Randy Barnes | ||
103 | kilo- (kJ) | 1.1×103 J | ≈ 1 British thermal unit (BTU), depending on the temperature |
1.4×103 J | total solar radiation received from the Sun by 1 square meter at the altitude of Earth's orbit per second (solar constant) | ||
1.8×103 J | kinetic energy of M16 rifle bullet (5.56x45mm NATO M855, 4.1 g fired at 930 m/s) | ||
3×103 J | Lorentz force can crusher pinch | ||
3.4×103 J | kinetic energy of world-record men's hammer throw (7.26 kg thrown at 30.7 m/s in 1986) | ||
3.6×103 J | ≡ 1 W·h (watt-hour) | ||
4.2×103 J | energy released by explosion of 1 gram of TNT | ||
4.2×103 J | ≈ 1 food Calorie (large calorie) | ||
~7×103 J | muzzle energy of an elephant gun, e.g. firing a .458 Winchester Magnum | ||
9×103 J | energy in an alkaline AA battery | ||
104 | 1.7×104 J | energy released by the metabolism of 1 gram of carbohydrates or protein | |
3.8×104 J | energy released by the metabolism of 1 gram of fat | ||
4-5×104 J | energy released by the combustion of 1 gram of gasoline | ||
5×104 J | kinetic energy of 1 gram of matter moving at 10 km/s | ||
105 | 3×105 J—15×105 J | kinetic energy of an automobile at highway speeds (1 to 5 tons at 89 km/h or 55 mph) | |
5×105 J | kinetic energy of 1 gram of a meteor hitting Earth | ||
106 | mega- (MJ) | 1×106 J | kinetic energy of a 2 tonne vehicle at 32 metres per second (72 miles per hour) |
1.2×106 J | approximate food energy of a snack such as a Snickers bar (280 food calories) | ||
3.6×106 J | = 1 kW·h (kilowatt-hour) (used for electricity) | ||
8.4×106 J | recommended food energy intake per day for a moderately active woman (2000 food calories) | ||
107 | 1×107 J | kinetic energy of the armor-piercing round fired by the assault guns of the ISU-152 tank | |
1.1×107 J | recommended food energy intake per day for a moderately active man (2600 food calories) | ||
3.7×107 J | $1 of electricity at a cost of $0.10/kWh (the US average retail cost in 2009) | ||
4×107 J | energy from the combustion of 1 cubic meter of natural gas | ||
4.2×107 J | caloric energy consumed by Olympian Michael Phelps on a daily basis during Olympic training | ||
6.3×107 J | theoretical minimum energy required to accelerate 1 kg of matter to escape velocity from Earth's surface (ignoring atmosphere) | ||
108 | 1×108 J | kinetic energy of a 55 tonne aircraft at typical landing speed (59 m/s or 115 knots) | |
1.1×108 J | ≈ 1 therm, depending on the temperature | ||
1.1×108 J | ≈ 1 Tour de France, or ~90 hours ridden at 5 W/kg by a 65 kg rider | ||
7.3×108 J | ≈ energy from burning 16 kilograms of oil (using 135 kg per barrel of light crude) | ||
109 | giga- (GJ) | 1 .. 10×109 J | energy in an average lightning bolt (thunder) |
1.1×109 J | magnetic stored energy in the world's largest toroidal superconducting magnet for the ATLAS experiment at CERN, Geneva | ||
1.4x109 J | theoretical minimum amount of energy required to melt a tonne of steel (380 kW·h) | ||
2.0x109 J | Energy of an ordinary 61 liter gasoline tank of a car. | ||
2.0×109 J | Planck energy, the unit of energy in Planck units | ||
3.3×109 J | approximate average amount of energy expended by a human heart muscle over an 80-year lifetime | ||
4.5×109 J | average annual energy usage of a standard refrigerator | ||
6.1×109 J | ≈ 1 bboe (barrel of oil equivalent) | ||
1010 | 2.3×1010 J | kinetic energy of an Airbus A380 at cruising speed (560 tonnes at 562 knots or 289 m/s) | |
4.2×1010 J | ≈ 1 toe (ton of oil equivalent) | ||
5×1010 J | yield energy of a Massive Ordnance Air Blast bomb, the second most powerful non-nuclear weapon ever designed | ||
7.3×1010 J | energy consumed by the average U.S. automobile in the year 2000 | ||
8.6×1010 J | ≈ 1 MW·d (megawatt-day), used in the context of power plants | ||
8.8×1010 J | total energy released in the nuclear fission of one gram of uranium-235 | ||
1011 | |||
1012 | tera- (TJ) | 3.4×1012 J | max fuel energy of an Airbus A330-300 (97,530 liters of Jet A-1) |
3.6×1012 J | 1 GW·h (gigawatt-hour) | ||
4×1012 J | electricity generated by one 20-kg CANDU fuel bundle assuming ~29% thermal efficiency of reactor | ||
6.4×1012 J | energy contained in jet fuel in a Boeing 747-100B aircraft at max fuel capacity (183,380 liters of Jet A-1) | ||
1013 | 1.1×1013 J | energy of the maximum fuel an Airbus A380 can carry (320,000 liters of Jet A-1) | |
1.2×1013 J | orbital kinetic energy of the International Space Station (417 tonnes at 7.7 km/s) | ||
8.8×1013 J | yield of the Fat Man atomic bomb used in World War II (21 kilotons) | ||
9.0×1013 J | theoretical total mass-energy of 1 gram of matter | ||
1014 | 6×1014 J | energy released by an average hurricane in 1 second | |
1015 | peta- (PJ) | > 1015 J | energy released by a severe thunderstorm |
1.0×1015 J | yearly electricity consumption in Greenland as of 2008 | ||
4.2×1015 J | energy released by explosion of 1 megaton of TNT | ||
1016 | 1×1016 J | estimated impact energy released in forming Meteor Crater | |
1.1×1016 J | yearly electricity consumption in Mongolia as of 2010 | ||
9.0×1016 J | mass-energy in 1 kilogram of antimatter (or matter) | ||
1017 | 1×1017 J | energy released on the Earth's surface by the magnitude 9.1-9.3 2004 Indian Ocean earthquake | |
1.7×1017 J | total energy from the Sun that strikes the face of the Earth each second | ||
2.1×1017 J | yield of the Tsar Bomba, the largest nuclear weapon ever tested (50 megatons) | ||
4.2×1017 J | yearly electricity consumption of Norway as of 2008 | ||
8×1017 J | estimated energy released by the eruption of the Indonesian volcano, Krakatoa, in 1883 | ||
1018 | exa- (EJ) | 1.4×1018 J | yearly electricity consumption of South Korea as of 2009 |
1019 | 1.4×1019 J | yearly electricity consumption in the U.S. as of 2009 | |
1.4×1019J | yearly electricity production in the U.S. as of 2009 | ||
5×1019 J | energy released in 1 day by an average hurricane in producing rain (400 times greater than the wind energy) | ||
6.4×1019 J | yearly electricity consumption of the world as of 2008 | ||
6.8×1019 J | yearly electricity generation of the world as of 2008 | ||
1020 | 5.0x1020 J | total world annual energy consumption in 2010 | |
8.0×1020 J | estimated global uranium resources for generating electricity 2005 | ||
1021 | zetta- (ZJ) | 6.9×1021 J | estimated energy contained in the world's natural gas reserves as of 2010 |
7.9×1021 J | estimated energy contained in the world's petroleum reserves as of 2010 | ||
1022 | 1.5×1022J | total energy from the Sun that strikes the face of the Earth each day | |
2.4×1022 J | estimated energy contained in the world's coal reserves as of 2010 | ||
2.9×1022 J | identified global uranium-238 resources using fast reactor technology | ||
3.9×1022 J | estimated energy contained in the world's fossil fuel reserves as of 2010 | ||
4×1022 J | estimated total energy released by the magnitude 9.1-9.3 2004 Indian Ocean Earthquake | ||
1023 | 1×1023 J | Amount of energy added to climate by anthropogenic greenhouse gasses | |
2.2×1023 J | total global uranium-238 resources using fast reactor technology | ||
5×1023 J | approximate energy released in the formation of the Chicxulub Crater in the Yucatán Peninsula | ||
1024 | yotta- (YJ) | 5.5×1024 J | total energy from the Sun that strikes the face of the Earth each year |
1025 | |||
1026 | 1.3×1026 J | conservative estimate of the energy released by the impact that created the Caloris basin on Mercury | |
3.8×1026 J | total energy output of the Sun each second | ||
1027 | |||
1028 | 3.8×1028 J | kinetic energy of the Moon in its orbit around the Earth (counting only its velocity relative to the Earth) | |
1029 | 2.1×1029 J | rotational energy of the Earth | |
1030 | 1.8×1030 J | gravitational binding energy of Mercury | |
1031 | 3.3×1031 J | total energy output of the Sun each day | |
1032 | 2×1032 J | gravitational binding energy of the Earth | |
1033 | 2.7×1033 J | Earth's kinetic energy in its orbit | |
1034 | 1.2×1034 J | total energy output of the Sun each year | |
1039 | 6.6×1039 J | theoretical total mass-energy of the Moon | |
1041 | 5.4×1041 J | theoretical total mass-energy of the Earth | |
6.9×1041 J | gravitational binding energy of the Sun | ||
1043 | 5×1043 J | total energy of all gamma rays in a typical gamma-ray burst | |
1044 | 1-2×1044 J | estimated energy released in a supernova, sometimes referred to as a foe | |
1046 | 1×1046 J | estimated energy released in a hypernova | |
1047 | 1.8×1047 J | theoretical total mass-energy of the Sun | |
1058 | 4×1058 J | visible mass-energy in our galaxy, the Milky Way | |
1059 | 1×1059 J | total mass-energy of the galaxy, including dark matter and dark energy | |
1062 | 1-2×1062 J | total mass-energy of the Local Supercluster, including dark matter | |
1069 | 4×1069 J | estimated total mass-energy of the observable universe |
Read more about Orders Of Magnitude (energy): SI Multiples
Famous quotes containing the words orders and/or magnitude:
“Really, if the lower orders dont set us a good example, what on earth is the use of them? They seem, as a class, to have absolutely no sense of moral responsibility.”
—Oscar Wilde (18541900)
“He all their ammunition
And feats of war defeats
With plain heroic magnitude of mind
And celestial vigour armed;”
—John Milton (16081674)