ऊर्जा के परिमाण की कोटि का स्रोत देखें

इस सूची में विभिन्न प्रणालियों में निहित [[ऊर्जा]] ([[जूल]] में) को [[परिमाण की कोटि]] के क्रम में व्यवस्थित किया गया है।
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==10<sup>−34</sup> to 10<sup>−1</sup> J==
{| class="wikitable"
|+'''[[ऊर्जा]] के परिमाणों की कोटियाँ'''
!गुणक (जूल)
! एस आई प्री-फिक्स
!मान
!प्रणाली
|-
|10<sup>−34</sup>||&nbsp;||6.626×10<sup>−34</sup> J || १ हर्ट्ज आवृत्ति वाले एक [[फोटॉन]] की [[ऊर्जा]]<ref name="britannica">{{cite web|url=http://www.britannica.com/EBchecked/topic/462917/Plancks-constant|publisher=britannica.com|title=Planck's constant &#124; physics &#124; Britannica.com|accessdate=26 December 2016|archive-url=https://web.archive.org/web/20150503001457/http://www.britannica.com/EBchecked/topic/462917/Plancks-constant|archive-date=3 मई 2015|url-status=live}}</ref>
|-
|10<sup>−33</sup>||&nbsp;||2×10<sup>−33</sup> J || [[Thermodynamic temperature#The relationship of temperature, motions, Heat, and thermal energy|Average kinetic energy of translational motion]] of a [[molecule]] at the lowest temperature reached, [[Absolute zero#Very low temperatures|100 picokelvins]] {{As of|1999|lc=on}}<ref>Calculated:  KE_avg ≈ (3/2) * T * 1.38E-23 = (3/2) * 1E-10 * 1.38E-23 ≈ 2.07E-33 J</ref>
|-
|10<sup>−28</sup>
| &nbsp;
| 6.6×10<sup>−28</sup> J
| Energy of a typical [[AM radio]] photon (1&nbsp;MHz) (4×10<sup>−9</sup> [[electronvolt|eV]])<ref>Calculated:  E_photon = hv = 6.626e-34 J-s * 1e6 Hz = 6.6e-28 J.  In eV:  6.6e-28 J / 1.6e-19 J/eV = 4.1e-9 eV.</ref>
|-
|10<sup>−24</sup>{{Anchor|10-24}}|| [[Yocto-]] (yJ)
| 1.6×10<sup>−24</sup> J
| Energy of a typical [[microwave oven]] photon (2.45&nbsp;GHz) (1×10<sup>−5</sup> [[electronvolt|eV]])<ref>{{cite web|title=Frequency of a Microwave Oven|url=http://hypertextbook.com/facts/1998/HowardCheung.shtml|work=The Physics Factbook|accessdate=15 November 2011|archive-url=https://web.archive.org/web/20111126062634/http://hypertextbook.com/facts/1998/HowardCheung.shtml|archive-date=26 नवंबर 2011|url-status=dead}}</ref><ref>Calculated:  E_photon = hv = 6.626e-34 J-s * 2.45e8 Hz = 1.62e-24 J.  In eV:  1.62e-24 J / 1.6e-19 J/eV = 1.0e-5 eV.</ref>
|-
|10<sup>−23</sup>||&nbsp;||2×10<sup>−23</sup> J || [[Thermodynamic temperature#The relationship of temperature, motions, Heat, and thermal energy|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]]<ref>{{cite web|title=Boomerang Nebula boasts the coolest spot in the Universe|url=http://www.jpl.nasa.gov/news/releases/97/coldspot.html|publisher=JPL|accessdate=13 November 2011|archive-url=https://web.archive.org/web/20090827115717/http://jpl.nasa.gov/news/releases/97/coldspot.html|archive-date=27 अगस्त 2009|url-status=live}}</ref><ref>Calculated:  KE_avg ≈ (3/2) * T * 1.38E-23 = (3/2) * 1 * 1.38E-23 ≈ 2.07E-23 J</ref>
|-
| 10<sup>−22</sup>
| &nbsp;
| 2-3000×10<sup>−22</sup> J
| Energy of [[infrared]] light photons<ref name="NASA_spectrum"/>
|-
|rowspan=6|10<sup>−21</sup>{{Anchor|10-21}}
|rowspan=6| [[Zepto-]] (zJ)
|1.7×10<sup>−21</sup> J
| 1 kJ/mol, converted to energy per molecule<ref>Calculated:  1e3 J / 6.022e23 entities per mole = 1.7e-21 J per entity</ref>
|-
|2.1×10<sup>−21</sup> J
| [[Thermal energy]] in each [[Degrees of freedom (physics and chemistry)|degree of freedom]] of a molecule at 25&nbsp;°C ([[Boltzmann constant|k]]T/2) (0.01 [[electronvolt|eV]])<ref>Calculated:  1.381e-23 J/K * 298.15 K / 2 = 2.1e-21 J</ref>
|-
|2.856×10<sup>−21</sup> J
| By [[Landauer's principle]], the minimum amount of energy required at 25&nbsp;°C to change one bit of information
|-
|3–7×10<sup>−21</sup> J
| Energy of a [[van der Waals force|van der Waals interaction]] between atoms (0.02–0.04 eV)<ref name=ucla_chem125>{{cite web|title=Bond Lengths and Energies|url=http://www.doe-mbi.ucla.edu/CHEM125/bonds.html|work=Chem 125 notes|publisher=UCLA|accessdate=13 November 2011|archive-url=https://web.archive.org/web/20110823121639/http://www.doe-mbi.ucla.edu/CHEM125/bonds.html|archive-date=23 अगस्त 2011|url-status=dead}}</ref><ref>Calculated:  2 to 4 kJ/mol =  2e3 J / 6.022e23 molecules/mol = 3.3e-21 J.  In eV: 3.3e-21 J / 1.6e-19 J/eV = 0.02 eV.  4e3 J / 6.022e23 molecules/mol = 6.7e-21 J.  In eV:  6.7e-21 J / 1.6e-19 J/eV = 0.04 eV.</ref>
|-
|4.1×10<sup>−21</sup> J
| The "[[Boltzmann constant|k]]T" constant at 25&nbsp;°C, a common rough approximation for the total [[thermal energy]] of each molecule in a system (0.03 eV)<ref>{{cite web|last=Ansari|first=Anjum|title=Basic Physical Scales Relevant to Cells and Molecules|url=http://www.uic.edu/classes/phys/phys450/MARKO/N003.html|work=Physics 450|accessdate=13 November 2011|archive-url=https://web.archive.org/web/20120401213027/http://www.uic.edu/classes/phys/phys450/MARKO/N003.html|archive-date=1 अप्रैल 2012|url-status=live}}</ref>
|-
|7–22×10<sup>−21</sup> J
| Energy of a [[hydrogen bond]] (0.04 to 0.13 eV)<ref name=ucla_chem125/><ref>Calculated:  4 to 13 kJ/mol.  4 kJ/mol = 4e3 J / 6.022e23 molecules/mol = 6.7e-21 J.  In eV:  6.7e-21 J / 1.6e-19 eV/J = 0.042 eV. 13 kJ/mol = 13e3 J / 6.022e23 molecules/mol = 2.2e-20 J.  In eV:  13e3 J / 6.022e23 molecules/mol / 1.6e-19 eV/J = 0.13 eV.</ref>
|-
| 10<sup>−20</sup>
| &nbsp;
| 4.5×10<sup>−20</sup> J
| Upper bound of the [[mass-energy]] of a [[neutrino]] in [[particle physics]] (0.28 eV)<ref>{{Cite journal | last1 = Thomas | first1 = S. | last2 = Abdalla | first2 = F. | last3 = Lahav | first3 = O. | title = Upper Bound of 0.28 eV on Neutrino Masses from the Largest Photometric Redshift Survey | doi = 10.1103/PhysRevLett.105.031301 | journal = Physical Review Letters | volume = 105 | issue = 3 | year = 2010 | pmid =  20867754| pmc = |arxiv = 0911.5291 |bibcode = 2010PhRvL.105c1301T | pages=031301}}</ref><ref>Calculated:  0.28 eV * 1.6e-19 J/eV = 4.5e-20 J</ref>
|-
|rowspan=4|10<sup>−19</sup>
|rowspan=4|&nbsp;
|1.6×10<sup>−19</sup> J || ≈1 [[electronvolt]] (eV)<ref>{{cite web|title=CODATA Value: electron volt|url=http://physics.nist.gov/cgi-bin/cuu/Value?tevj|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20120103203213/http://physics.nist.gov/cgi-bin/cuu/Value?tevj|archive-date=3 जनवरी 2012|url-status=dead}}</ref>
|-
|3–5×10<sup>−19</sup> J || Energy range of [[photon]]s in [[visible light]]<ref>{{cite web|title=BASIC LAB KNOWLEDGE AND SKILLS|url=http://www.sci.sdsu.edu/classes/chemistry/chem467l/mardahl/basic.html|quote=Visible wavelengths are roughly from 390 nm to 780 nm|accessdate=5 November 2011|archive-url=https://web.archive.org/web/20130515121940/http://www.sci.sdsu.edu/classes/chemistry/chem467l/mardahl/basic.html|archive-date=15 मई 2013|url-status=dead}}</ref><ref>Calculated:  E = h * c / lambda.  E_780_nm = 6.6e-34 kg-m^2/s * 3e8 m/s / (780e-9 m) = 2.5e-19 J.  E_390 _nm = 6.6e-34 kg-m^2/s * 3e8 m/s / (390e-9 m) = 5.1e-19 J</ref>
|-
|3–14×10<sup>−19</sup> J
| Energy of a [[covalent bond]] (2–9 eV)<ref name=ucla_chem125/><ref>Calculated:  50 kcal/mol * 4.184 J/calorie / 6.0e22e23 molecules/mol = 3.47e-19 J.  (3.47e-19 J / 1.60e-19 eV/J = 2.2 eV.)  and 200 kcal/mol * 4.184 J/calorie / 6.0e22e23 molecules/mol = 1.389e-18 J.  (7.64e-19 J / 1.60e-19 eV/J = 8.68 eV.)</ref>
|-
| 5–200×10<sup>−19</sup> J
| Energy of [[ultraviolet]] light photons<ref name="NASA_spectrum"/>
|-
|10<sup>−18</sup>{{Anchor|10-18}} || [[Atto-]] (aJ) || &nbsp; || &nbsp;
|-
| 10<sup>−17</sup>
| &nbsp;
| 2-2000×10<sup>−17</sup> J
| Energy range of [[X-ray]] photons<ref name="NASA_spectrum">{{cite web|title=Wavelength, Frequency, and Energy|url=http://imagine.gsfc.nasa.gov/docs/science/know_l1/spectrum_chart.html|work=Imagine the Universe|publisher=NASA|accessdate=15 November 2011|archive-url=https://web.archive.org/web/20111116000744/http://imagine.gsfc.nasa.gov/docs/science/know_l1/spectrum_chart.html|archive-date=16 नवंबर 2011|url-status=live}}</ref>
|-
| 10<sup>−16</sup> || &nbsp; || &nbsp; || &nbsp;
|-
| 10<sup>−15</sup>{{Anchor|10-15}} || [[Femto-]] (fJ) || 3 * 10<sup>−15</sup> J || Average kinetic energy of one human [[red blood cell]].<ref>{{cite journal | last1 = Phillips | first1 = Kevin | last2 = Jacques | first2 = Steven | last3 = McCarty | first3 = Owen | title = How much does a cell weigh? | url = https://physics.aps.org/synopsis-for/10.1103/PhysRevLett.109.118105 | journal = Physical Review Letters | volume = 109 | year = 2012 | publisher = American Physical Society | doi = 10.1103/PhysRevLett.109.118105 | quote = Roughly 27 picograms | access-date = 14 अगस्त 2017 | archive-url = https://web.archive.org/web/20170829202228/https://physics.aps.org/synopsis-for/10.1103/PhysRevLett.109.118105 | archive-date = 29 अगस्त 2017 | url-status = dead }}</ref><ref>{{cite web|title=Our Bodies' Velocities, By the Numbers|author=Bob Berman|accessdate=19 August 2016|url=http://discovermagazine.com/2014/julyaug/18-body-of-work|quote=The [...] blood [...] flow[s] at an average speed of 3 to 4 mph|archive-url=https://web.archive.org/web/20160821135131/http://discovermagazine.com/2014/julyaug/18-body-of-work|archive-date=21 अगस्त 2016|url-status=live}}</ref><ref>Calculated: 1/2 * 27e-12 g * (3.5 miles per hour)^2 = 3e-15 J</ref>
|-
|rowspan=4|10<sup>−14</sup>
|rowspan=4|&nbsp;
| 1×10<sup>−14</sup> J
| [[Sound energy]] (vibration) transmitted to the [[eardrums]] by listening to a [[whisper]] for one second.<ref>{{cite web|title=Physics of the Body|url=https://www3.nd.edu/~nsl/Lectures/mphysics/Medical%20Physics/Part%20I.%20Physics%20of%20the%20Body/Chapter%204.%20Acoustics%20of%20the%20Body/4.3%20Physics%20of%20the%20ear/Physics%20of%20the%20ear.pdf|publisher=Notre Dame|accessdate=19 August 2016|archive-url=https://web.archive.org/web/20161106160152/https://www3.nd.edu/~nsl/Lectures/mphysics/Medical%20Physics/Part%20I.%20Physics%20of%20the%20Body/Chapter%204.%20Acoustics%20of%20the%20Body/4.3%20Physics%20of%20the%20ear/Physics%20of%20the%20ear.pdf|archive-date=6 नवंबर 2016|url-status=dead}}. "The eardrum is a [...] membran[e] with an area of 65 mm<sup>2</sup>."</ref><ref>{{cite web|title=Intensity and the Decibel Scale|url=http://www.physicsclassroom.com/class/sound/Lesson-2/Intensity-and-the-Decibel-Scale|publisher=Physics Classroom|accessdate=19 August 2016|archive-url=https://web.archive.org/web/20160820014448/http://www.physicsclassroom.com/class/sound/Lesson-2/Intensity-and-the-Decibel-Scale|archive-date=20 अगस्त 2016|url-status=dead}}</ref><ref>Calculated: two eardrums ≈ 1 cm<sup>2</sup>.  1e-6 W/m<sup>2</sup> * 1e-4 m<sup>2</sup> * 1 s = 1e-14 J</ref>
|-
| > 2×10<sup>−14</sup> J
| Energy of [[gamma ray]] photons<ref name="NASA_spectrum"/>
|-
|2.7×10<sup>−14</sup> J || Upper bound of the [[mass-energy]] of a [[muon neutrino]]<ref>{{cite book|title=Neutrinos in physics and astrophysics: from 10–33 to 1028 cm: TASI 98 : Boulder, Colorado, USA, 1–26 June 1998|year=2000|publisher=World Scientific|isbn=978-981-02-3887-2|url=https://books.google.com/books?id=QC5zi1N-1KMC&pg=PA354&lpg=PA354&dq=muon+neutrino+mass+170kev&source=bl&ots=0NDArur2q5&sig=Pv64mojKL34XqBYpCa4_B_7zg2s&hl=en&ei=Laa9TuunHqOriAKoh4WFAw&sa=X&oi=book_result&ct=result&resnum=2&ved=0CCUQ6AEwATgK#v=onepage&q&f=false|author=Thomas J Bowles|authorlink=The Experimental Search for Finite Neutrino Mass|editor=P. Langacker|accessdate=11 November 2011|page=354|quote=an upper limit ov m_v_u < 170 keV|archive-url=https://web.archive.org/web/20161203195838/https://books.google.com/books?id=QC5zi1N-1KMC&pg=PA354&lpg=PA354&dq=muon+neutrino+mass+170kev&source=bl&ots=0NDArur2q5&sig=Pv64mojKL34XqBYpCa4_B_7zg2s&hl=en&ei=Laa9TuunHqOriAKoh4WFAw&sa=X&oi=book_result&ct=result&resnum=2&ved=0CCUQ6AEwATgK#v=onepage&q&f=false|archive-date=3 दिसंबर 2016|url-status=live}}</ref><ref>Calculated:  170e3 eV * 1.6e-19 J/eV = 2.7e-14 J</ref>
|-
|8.2×10<sup>−14</sup> J || Rest [[mass-energy]] of an [[electron]]<ref>{{cite web|title=electron mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?mec2|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20110805131300/http://physics.nist.gov/cgi-bin/cuu/Value?mec2|archive-date=5 अगस्त 2011|url-status=live}}</ref>
|-
|10<sup>−13</sup> || &nbsp; || 1.6×10<sup>−13</sup> J || 1 [[megaelectronvolt]] (MeV)<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=6&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215050/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=6&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
|10<sup>−12</sup>{{Anchor|10-12}} || [[Pico-]] (pJ) || 2.3×10<sup>−12</sup> J || Kinetic energy of [[Neutron#Fusion neutrons|neutrons produced by D-T fusion]], used to trigger fission (14.1 MeV)<ref>{{cite web|last=Muller|first=Richard A.|title=The Sun, Hydrogen Bombs, and the physics of fusion|url=http://muller.lbl.gov/teaching/physics10/old%20physics%2010/chapters%20%28old%29/7-fusion.htm|accessdate=5 November 2011|year=2002|quote=The neutron comes out with high energy of 14.1 MeV|archive-url=https://web.archive.org/web/20120402214226/http://muller.lbl.gov/teaching/physics10/old%20physics%2010/chapters%20(old)/7-fusion.htm|archive-date=2 अप्रैल 2012|url-status=dead}}</ref><ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=7&num=1.41&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215052/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=7&num=1.41&From=ev&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
|rowspan=1|10<sup>−11</sup>
|rowspan=1|&nbsp;
|3.4×10<sup>−11</sup> J || Average total energy [[nuclear explosions|released]] in the [[nuclear fission]] of one [[uranium-235]] [[atom]] (215 MeV)<ref name="Energy From Uranium Fission">{{cite web|title=Energy From Uranium Fission|url=http://hyperphysics.phy-astr.gsu.edu/hbase/nucene/u235chn.html#c3|work=HyperPhysics|accessdate=8 November 2011|archive-url=https://web.archive.org/web/20111028142620/http://hyperphysics.phy-astr.gsu.edu/hbase/nucene/u235chn.html#c3|archive-date=28 अक्तूबर 2011|url-status=dead}}</ref><ref name="Conversion from eV to J">{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=8&num=2.15&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215048/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=8&num=2.15&From=ev&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
|rowspan=6|10<sup>−10</sup>
|rowspan=6|&nbsp;
|1.5030×10<sup>−10</sup> J || Rest [[mass-energy]] of a [[proton]]<ref>{{cite web|title=proton mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?mpc2|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20120910055535/http://physics.nist.gov/cgi-bin/cuu/Value?mpc2|archive-date=10 सितंबर 2012|url-status=dead}}</ref>
|-
|1.505×10<sup>−10</sup> J || Rest [[mass-energy]] of a [[neutron]]<ref>{{cite web|title=neutron mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?mnc2|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20120819065453/http://physics.nist.gov/cgi-bin/cuu/Value?mnc2|archive-date=19 अगस्त 2012|url-status=dead}}</ref>
|-
|1.6×10<sup>−10</sup> J || 1 [[gigaelectronvolt]] (GeV)<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215041/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
|3×10<sup>−10</sup> J || Rest [[mass-energy]] of a [[deuteron]]<ref>{{cite web|title=deuteron mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?mdc2|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20110805130134/http://physics.nist.gov/cgi-bin/cuu/Value?mdc2|archive-date=5 अगस्त 2011|url-status=dead}}</ref>
|-
|6×10<sup>−10</sup> J || Rest [[mass-energy]] of an [[alpha particle]]<ref>{{cite web|title=alpha particle mass energy equivalent|url=http://physics.nist.gov/cgi-bin/cuu/Value?malc2|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20110805132512/http://physics.nist.gov/cgi-bin/cuu/Value?malc2|archive-date=5 अगस्त 2011|url-status=dead}}</ref>
|-
|7×10<sup>−10</sup> J || Energy required to raise a grain of [[sand]] by 0.1mm (the thickness of a piece of paper).<ref>Calculated: 7e-4 g * 9.8 m/s<sup>2</sup> * 1e-4 m</ref>
|-
|rowspan=2|10<sup>−9</sup>{{Anchor|10-9
}}
|rowspan=2| [[Nano-]] (nJ)
| 1.6×10<sup>−9</sup> J || 10 GeV<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=10&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215055/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=10&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
| 8×10<sup>−9</sup> J || Initial operating energy per beam of the [[CERN]] [[Large Electron Positron Collider]] in 1989 (50 GeV)<ref>{{cite web|last=Myers|first=Stephen|title=The LEP Collider|url=http://sl-div.web.cern.ch/sl-div/history/lep_doc.html|publisher=CERN|accessdate=14 November 2011|quote=the LEP machine energy is about 50 GeV per beam|archive-url=https://web.archive.org/web/20140618030149/https://sl-div.web.cern.ch/sl-div/history/lep_doc.html|archive-date=18 जून 2014|url-status=dead}}</ref><ref>Calculated:  50e9 eV * 1.6e-19 J/eV = 8e-9 J</ref>
|-
|rowspan=5|10<sup>−8</sup>
|rowspan=5|&nbsp;
| 1.3×10<sup>−8</sup> J || [[Mass-energy]] of a [[W boson]] (80.4 GeV)<ref>{{cite web|title=W|url=http://pdglive.lbl.gov/Rsummary.brl?nodein=S043|work=PDG Live|publisher=Particle Data Group|accessdate=4 November 2011|archive-url=https://archive.today/20120717002128/http://pdglive.lbl.gov/Rsummary.brl?nodein=S043|archive-date=17 जुलाई 2012|url-status=dead}}</ref><ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=80.4&From=ev&To=j&Action=Convert+value+and+show+factor&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215108/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=80.4&From=ev&To=j&Action=Convert+value+and+show+factor&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
| 1.5×10<sup>−8</sup> J || [[Mass-energy]] of a [[Z boson]] (91.2 GeV)<ref name="Amsler2008">{{Cite journal | last1 = Amsler | first1 = C. | last2 = Doser | first2 = M. | last3 = Antonelli | first3 = M. | last4 = Asner | first4 = D. | last5 = Babu | first5 = K. | last6 = Baer | first6 = H. | last7 = Band | first7 = H. | last8 = Barnett | first8 = R. | last9 = Bergren | first9 = E. | last10 = Beringer | first10 = J. | last11 = Bernardi | first11 = G. | last12 = Bertl | first12 = W. | last13 = Bichsel | first13 = H. | last14 = Biebel | first14 = O. | last15 = Bloch | first15 = P. | last16 = Blucher | first16 = E. | last17 = Blusk | first17 = S. | last18 = Cahn | first18 = R. N. | last19 = Carena | first19 = M. | last20 = Caso | first20 = C. | last21 = Ceccucci | first21 = A. | last22 = Chakraborty | first22 = D. | last23 = Chen | first23 = M. -C. | last24 = Chivukula | first24 = R. S. | last25 = Cowan | first25 = G. | last26 = Dahl | first26 = O. | last27 = d'Ambrosio | first27 = G. | last28 = Damour | first28 = T. | last29 = De Gouvêa | first29 = A. | last30 = Degrand | first30 = T. | title = Review of Particle Physics⁎ | doi = 10.1016/j.physletb.2008.07.018 | journal = Physics Letters B | volume = 667 | pages = 1–6 | year = 2008 | pmid =  | pmc =  | url = http://pdglive.lbl.gov/Rsummary.brl?nodein=S044&fsizein=1 | bibcode = 2008PhLB..667....1A | access-date = 14 अगस्त 2017 | archive-url = https://archive.today/20120712165412/http://pdglive.lbl.gov/Rsummary.brl?nodein=S044&fsizein=1 | archive-date = 12 जुलाई 2012 | url-status = dead }}</ref><ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=91.2&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215045/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=9&num=91.2&From=ev&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
| 1.6×10<sup>−8</sup> J || 100 GeV<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=11&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215036/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=11&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
| 2×10<sup>−8</sup> J || [[Mass-energy]] of the [[Higgs Boson]] (125.1 GeV)<ref>{{cite arXiv|last1=ATLAS |last2=CMS |authorlink1=ATLAS experiment|authorlink2=Compact Muon Solenoid|eprint=1503.07589 |title= Combined Measurement of the Higgs Boson Mass in pp Collisions at √s=7 and 8 TeV with the ATLAS and CMS Experiments|date=26 March 2015 |version= }}</ref>
|-
| 6.4×10<sup>−8</sup> J || Operating energy per proton of the [[CERN]] [[Super Proton Synchrotron]] accelerator in 1976<ref>{{cite web|last=Adams|first=John|title=400 GeV Proton Synchrotron|url=http://sl-div.web.cern.ch/sl-div/history/sps_doc.html|work=Excertp from the CERN Annual Report 1976|publisher=CERN|accessdate=14 November 2011|quote=A circulating proton beam of 400 GeV energy was first achieved in the SPS on 17 June 1976|archive-url=https://web.archive.org/web/20111026162037/http://sl-div.web.cern.ch/sl-div/history/sps_doc.html|archive-date=26 अक्तूबर 2011|url-status=dead}}</ref><ref>Calculated:  400e9 eV * 1.6e-19 J/eV = 6.4e-8 J</ref>
|-
|rowspan=2|10<sup>−7</sup>
|rowspan=2|&nbsp;
| 1×10<sup>−7</sup> J   || ≡ 1 [[erg]]<ref name=NIST_SI_units/>
|-
| 1.6×10<sup>−7</sup> J || 1 TeV (teraelectronvolt),<ref>{{cite web|title=Conversion from eV to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=12&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202212059/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=12&num=1&From=ev&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref> about the kinetic energy of a flying [[mosquito]]<ref>{{cite web|title=Chocolate bar yardstick|url=http://www.cernlove.org/blog/2010/04/chocolate-bar-yardstick/|accessdate=24 January 2014|quote=A TeV is actually a very tiny amount of energy. A popular analogy is to a flying mosquito.|archive-url=https://web.archive.org/web/20140226141339/http://www.cernlove.org/blog/2010/04/chocolate-bar-yardstick/|archive-date=26 फ़रवरी 2014|url-status=dead}}</ref>
|-
|10<sup>−6</sup>{{Anchor|10-6}} || [[Micro-]] (µJ) || 1.04×10<sup>−6</sup> J || Energy per proton in the [[CERN]] [[Large Hadron Collider]] in 2015 (6.5 TeV)<ref>{{cite web|title=First successful beam at record energy of 6.5 TeV|url=http://home.web.cern.ch/about/updates/2015/04/first-successful-beam-record-energy-65-tev|accessdate=28 April 2015|archive-url=https://web.archive.org/web/20150426052457/http://home.web.cern.ch/about/updates/2015/04/first-successful-beam-record-energy-65-tev|archive-date=26 अप्रैल 2015|url-status=dead}}</ref><ref>Calculated:  6.5e12 eV per beam * 1.6e-19 J/eV = 1.04e-6 J</ref>
|-
| 10<sup>−5</sup> || &nbsp; || &nbsp; || &nbsp;
|-
| 10<sup>−4</sup> || &nbsp; || &nbsp; || &nbsp;
|-
| 10<sup>−3</sup>{{Anchor|10-3}} || [[Milli-]] (mJ) || &nbsp; || &nbsp;
|-
| 10<sup>−2</sup>{{Anchor|10-2
}} || [[Centi-]] (cJ) || &nbsp; || &nbsp;
|-
|rowspan=1|10<sup>−1</sup>{{Anchor|10-1}}
|rowspan=1| [[Deci-]] (dJ)
| 1.1×10<sup>−1</sup> J || Energy of an [[Half dollar (United States coin)|American half-dollar]] falling 1 metre<ref>{{cite web |url=http://www.usmint.gov/about_the_mint/?action=coin_specifications |title=Coin specifications |publisher=United States Mint |accessdate=2 November 2011 |quote=11.340 g |archive-url=https://web.archive.org/web/20150218061037/http://www.usmint.gov/about_the_mint/?action=coin_specifications |archive-date=18 फ़रवरी 2015 |url-status=live }}</ref><ref>Calculated:  m*g*h = 11.34e-3 kg * 9.8 m/s^2 * 1 m = 1.1e-1 J</ref>
|}

==1 to 10<sup>6</sup> J==
{| class="wikitable"
|-
|rowspan=8|10<sup>0</sup>
|rowspan=8| J
| 1 J || ≡ 1 N·m ([[Newton (unit)|Newton]]–[[metre]])
|-
| 1 J || ≡ 1&nbsp;W·s ([[Watt]]-second)
|-
| 1 J || Kinetic energy produced as an extra small apple (~100 grams<ref>{{cite web|url=http://www.nal.usda.gov/fnic/foodcomp/search/ |title=Apples, raw, with skin (NDB No. 09003) |work=USDA Nutrient Database |publisher=USDA |accessdate=8 December 2011 |url-status=dead |archiveurl=https://web.archive.org/web/20150303184216/http://www.nal.usda.gov/fnic/foodcomp/search/ |archivedate= 3 March 2015 |df= }}</ref>) falls 1 [[meter]] against Earth's [[gravity]]<ref>Calculated:  m*g*h = 1e-1 kg * 9.8 m/s^2 * 1 m = 1 J</ref>
|-
| 1 J || Energy required to heat 1 gram of dry, cool [[Earth's atmosphere|air]] by 1-degree [[Celsius]]<ref>{{cite web|title=Specific Heat of Dry Air|url=http://www.engineeringtoolbox.com/air-specific-heat-capacity-d_705.html|publisher=Engineering Toolbox|accessdate=2 November 2011|archive-url=https://web.archive.org/web/20111105034342/http://www.engineeringtoolbox.com/air-specific-heat-capacity-d_705.html|archive-date=5 नवंबर 2011|url-status=dead}}</ref>
|-
| 1.4 J || ≈ 1&nbsp;ft·lbf ([[foot-pound force]])<ref name=NIST_SI_units>{{cite web|title=Appendix B8—Factors for Units Listed Alphabetically|url=http://physics.nist.gov/Pubs/SP811/appenB8.html|work=NIST Guide for the Use of the International System of Units (SI)|publisher=NIST|quote=1.355818|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20160129233551/http://physics.nist.gov/Pubs/SP811/appenB8.html|archive-date=29 जनवरी 2016|url-status=live}}</ref>
|-
| 4.184 J || ≡ 1 thermochemical [[calorie]] (small calorie)<ref name=NIST_SI_units/>
|-
| 4.1868 J || ≡ 1 International (Steam) Table calorie<ref>{{cite web|title=Footnotes|url=http://physics.nist.gov/Pubs/SP811/footnotes.html#f09|work=NIST Guide to the SI|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20111107224559/http://physics.nist.gov/Pubs/SP811/footnotes.html#f09|archive-date=7 नवंबर 2011|url-status=dead}}</ref>
|-
| 8 J || [[Greisen-Zatsepin-Kuzmin limit|Greisen-Zatsepin-Kuzmin]] theoretical upper limit for the energy of a [[cosmic ray]] coming from a distant source<ref>{{cite web|title=Physical Motivations|url=http://www.dfg.unito.it/euso/physical-motivation.html|work=ULTRA Home Page (EUSO project)|publisher=Dipartimento di Fisica di Torino|accessdate=12 November 2011|archive-url=https://web.archive.org/web/20120209054727/http://www.dfg.unito.it/euso/physical-motivation.html|archive-date=9 फ़रवरी 2012|url-status=dead}}</ref><ref>Calculated:  5e19 eV * 1.6e-19 J/ev = 8 J</ref>
|-
|rowspan=1|10<sup>1</sup>{{Anchor|101}}
|rowspan=1| [[Deca-]] (daJ)
| 5×10<sup>1</sup> J || The [[Ultra-high-energy cosmic ray|most energetic cosmic ray]] ever detected<ref>{{cite web|title=The Fly's Eye (1981–1993)|url=http://www.cosmic-ray.org/reading/flyseye.html#SEC10|publisher=HiRes|accessdate=14 November 2011|archive-url=https://web.archive.org/web/20090815102123/http://www.cosmic-ray.org/reading/flyseye.html#SEC10|archive-date=15 अगस्त 2009|url-status=dead}}</ref> was most likely a [[Oh-My-God Particle|single proton]] traveling only slightly slower than the speed of light.<ref>
{{Cite journal
 | author=Bird, D. J.
 | date=March 1995
 | title=Detection of a cosmic ray with measured energy well beyond the expected spectral cutoff due to cosmic microwave radiation
 | url=http://adsabs.harvard.edu/abs/1995ApJ...441..144B
 | publisher=Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 441, no. 1, p. 144-150
 |accessdate=14 February 2014
 | bibcode=1995ApJ...441..144B
}}</ref>
|-
| colspan="2" rowspan="11" |10<sup>2</sup>{{Anchor|100|102}}
| 1×10<sup>2</sup> J || Flash energy of a typical pocket camera electronic flash [[capacitor]] {{nowrap|(100–400 µF}} @ {{nowrap|330 V)}}<ref>{{cite web|title=Notes on the Troubleshooting and Repair of Electronic Flash Units and Strobe Lights and Design Guidelines, Useful Circuits, and Schematics|url=http://www.repairfaq.org/sam/strbfaq.htm|accessdate=8 December 2011|quote=The energy storage capacitor for pocket cameras is typically 100 to 400 uF at 330 V (charged to 300 V) with a typical flash energy of 10 W-s.|archive-url=https://web.archive.org/web/20111219072154/http://www.repairfaq.org/sam/strbfaq.htm|archive-date=19 दिसंबर 2011|url-status=dead}}</ref><ref name="ev_pwrsh">{{cite web|title=Teardown: Digital Camera Canon PowerShot &#124;|url=http://electroelvis.com/2012/09/02/teardown-digital-camera-canon-powershot/|date=2 September 2012|accessdate=6 June 2013|publisher=electroelvis.com|archive-url=https://web.archive.org/web/20130801014811/http://electroelvis.com/2012/09/02/teardown-digital-camera-canon-powershot/|archive-date=1 अगस्त 2013|url-status=dead}}</ref>
|-
|3×10<sup>2</sup> J || Energy of a lethal dose of [[X-ray]]s<ref>{{cite web|title=Ionizing Radiation|url=http://chemed.chem.purdue.edu/genchem/topicreview/bp/ch23/radiation.php|work=General Chemistry Topic Review:  Nuclear Chemistry|publisher=Bodner Research Web|accessdate=5 November 2011|archive-url=https://web.archive.org/web/20120109191204/http://chemed.chem.purdue.edu/genchem/topicreview/bp/ch23/radiation.php|archive-date=9 जनवरी 2012|url-status=dead}}</ref>
|-
|3×10<sup>2</sup> J || Kinetic energy of an average person jumping as high as they can<ref>{{cite web|title=Vertical Jump Test|url=http://www.topendsports.com/testing/tests/vertjump.htm|publisher=Topend Sports|accessdate=12 December 2011|quote=41–50 cm (males) 31–40 cm (females)|archive-url=https://web.archive.org/web/20111224055703/http://www.topendsports.com/testing/tests/vertjump.htm|archive-date=24 दिसंबर 2011|url-status=live}}</ref><ref>{{cite web|title=Mass of an Adult|url=http://hypertextbook.com/facts/2003/AlexSchlessingerman.shtml|work=The Physics Factbook|accessdate=13 December 2011|quote=70 kg|archive-url=https://web.archive.org/web/20150506084852/http://hypertextbook.com/facts/2003/AlexSchlessingerman.shtml|archive-date=6 मई 2015|url-status=live}}</ref><ref>Kinetic energy at start of jump = potential energy at high point of jump. Using a mass of 70 kg and a high point of 40&nbsp;cm => energy = m*g*h = 70&nbsp;kg * 9.8 m/s^2 * 40e-2 m = 274 J</ref>
|-
|3.3×10<sup>2</sup> J || [[Enthalpy of fusion|Energy to melt]] 1&nbsp;g of [[ice]]<ref>{{cite web|title=Latent Heat of Melting of some common Materials|url=http://www.engineeringtoolbox.com/latent-heat-melting-solids-d_96.html|3=|publisher=Engineering Toolbox|accessdate=10 June 2013|quote=334 kJ/kg|archive-url=https://web.archive.org/web/20130707160839/http://www.engineeringtoolbox.com/latent-heat-melting-solids-d_96.html|archive-date=7 जुलाई 2013|url-status=dead}}</ref>
|-
|> 3.6×10<sup>2</sup> J || Kinetic energy of 800&nbsp;g<ref>{{cite web|title=Javelin Throw – Introduction|url=http://www.iaaf.org/community/athletics/trackfield/newsid=9427.html|publisher=IAAF|accessdate=12 December 2011|archive-url=https://web.archive.org/web/20120606232418/http://www.iaaf.org/community/athletics/trackfield/newsid%3D9427.html|archive-date=6 जून 2012|url-status=live}}</ref> [[Javelin Throw|standard men's javelin]] thrown at > 30&nbsp;m/s<ref>{{cite web|last=Young|first=Michael|title=Developing Event Specific Strength for the Javelin Throw|url=http://www.indianathrower.com/documents/javelinthrowbiomechanics.pdf|accessdate=13 December 2011|quote=For elite athletes, the velocity of a javelin release has been measured in excess of 30m/s|archive-url=https://web.archive.org/web/20110813094040/http://www.indianathrower.com/documents/javelinthrowbiomechanics.pdf|archive-date=13 अगस्त 2011|url-status=dead}}</ref> by elite javelin throwers<ref>Calculated:  1/2 * 0.8 kg * (30 m/s)^2 = 360 J</ref>
|-
|5–20×10<sup>2</sup> J || Energy output of a typical [[photography]] studio [[xenon flash lamp|strobe light]] in a single flash<ref>{{cite web|last=Greenspun|first=Philip|title=Studio Photography|url=http://photo.net/learn/studio/primer|accessdate=13 December 2011|quote=Most serious studio photographers start with about 2000 watts-seconds|archive-url=https://web.archive.org/web/20070929104533/http://photo.net/learn/studio/primer|archive-date=29 सितंबर 2007|url-status=dead}}</ref>
|-
|6×10<sup>2</sup> J || Kinetic energy of 2&nbsp;kg<ref>{{cite web|title=Discus Throw – Introduction|url=http://www.iaaf.org/community/athletics/trackfield/newsid=9437.html|publisher=IAAF|accessdate=12 December 2011|archive-url=https://web.archive.org/web/20111122203019/http://www.iaaf.org/community/athletics/trackfield/newsid=9437.html|archive-date=22 नवंबर 2011|url-status=live}}</ref> [[Discus Throw|standard men's discus]] thrown at 24.4&nbsp;m/s{{Citation needed|date=November 2011}} by the world record holder [[Jürgen Schult]]<ref>Calculated:  1/2 * 2 kg * (24.4 m/s)^2 = 595.4 J</ref>
|-
|6×10<sup>2</sup> J || Use of a 10-watt flashlight for 1-minute
|-
|7.5×10<sup>2</sup> J || A power of 1 [[horsepower]] applied for 1 second<ref name=NIST_SI_units/>
|-
|7.8×10<sup>2</sup> J || Kinetic energy of 7.26&nbsp;kg<ref>{{cite web|title=Shot Put – Introduction|url=http://www.iaaf.org/community/athletics/trackfield/newsid=9444.html|publisher=IAAF|accessdate=12 December 2011|archive-url=https://web.archive.org/web/20121025121004/http://www.iaaf.org/community/athletics/trackfield/newsid=9444.html|archive-date=25 अक्तूबर 2012|url-status=live}}</ref> [[Shot Put|standard men's shot]] thrown at 14.7&nbsp;m/s{{Citation needed|date=November 2011}} by the world record holder [[Randy Barnes]]<ref>Calculated:  1/2 * 7.26 kg * (14.7 m/s)^2 = 784 J</ref>
|-
|8.01×10<sup>2</sup> J
|Amount of work needed to lift a man with an average weight (81.7&nbsp;kg) one meter above earth (or any planet with earth gravity)
|-
|rowspan=11|10<sup>3</sup>{{Anchor|103
}}
|rowspan=11| [[Kilo-]] (kJ)
|1.1×10<sup>3</sup> J || ≈ 1 [[British thermal unit]] (BTU), depending on the [[temperature]]<ref name=NIST_SI_units/>
|-
|1.4×10<sup>3</sup> J || Total [[solar radiation]] received from the [[Sun]] by 1 [[square meter]] at the altitude of Earth's orbit per second ([[solar constant]])<ref>{{Cite journal | last1 = Kopp | first1 = G. | last2 = Lean | first2 = J. L. | doi = 10.1029/2010GL045777 | title = A new, lower value of total solar irradiance: Evidence and climate significance | journal = Geophysical Research Letters | volume = 38 | pages = n/a | year = 2011 | pmid =  | pmc =  | url = http://onlinelibrary.wiley.com/doi/10.1029/2010GL045777/pdf | format = PDF | bibcode = 2011GeoRL..38.1706K | access-date = 14 अगस्त 2017 | archive-url = https://web.archive.org/web/20170726161617/http://onlinelibrary.wiley.com/doi/10.1029/2010GL045777/pdf | archive-date = 26 जुलाई 2017 | url-status = live }}</ref>
|-
|1.8×10<sup>3</sup> J || Kinetic energy of [[M16 rifle]] [[bullet]] ([[5.56×45mm NATO]] [[M855]], 4.1&nbsp;g fired at 930&nbsp;m/s)<ref>{{cite web|title=Intermediate power ammunition for automatic assault rifles|url=http://world.guns.ru/ammunition/intermediate-cartridges-e.html|work=Modern Firearms|publisher=World Guns|accessdate=12 December 2011|archive-url=https://web.archive.org/web/20130810184827/http://world.guns.ru/ammunition/intermediate-cartridges-e.html|archive-date=10 अगस्त 2013|url-status=dead}}</ref>
<!-- Don't need so many of these bullet entries:
|-
|~1.4×10<sup>3</sup> J || Kinetic energy of a [[5.45x39mm]] [[AK-74]] [[bullet]] (3.6 g fired at 880&nbsp;m/s)<ref>{{cite web|title=Intermediate power ammunition for automatic assault rifles|url=http://world.guns.ru/ammunition/intermediate-cartridges-e.html|work=Modern Firearms|publisher=World Guns|accessdate=12 December 2011}}</ref>
|-
|1.7×10<sup>3</sup> J || Kinetic energy of a 3.56 g [[.223 Remington]] M193 [[M16 rifle|M16]] [[bullet]] fired at 975&nbsp;m/s
|-
|3.3×10<sup>3</sup> J || Kinetic energy of a 9.33 g [[7.62×51mm NATO]] [[rifle]] [[Cartridge (firearms)|cartridge]] fired at {{nowrap|838 m/s}}
-->
|-
|2.3×10<sup>3</sup> J || [[Enthalpy of vaporization|Energy to vaporize]] 1&nbsp;g of [[water]] into steam<ref>{{cite web|title=Fluids - Latent Heat of Evaporation|url=http://www.engineeringtoolbox.com/fluids-evaporation-latent-heat-d_147.html|3=|publisher=Engineering Toolbox|accessdate=10 June 2013|quote=2257 kJ/kg|archive-url=https://web.archive.org/web/20130704053756/http://www.engineeringtoolbox.com/fluids-evaporation-latent-heat-d_147.html|archive-date=4 जुलाई 2013|url-status=dead}}</ref>
|-
|3×10<sup>3</sup> J   || [[Lorentz force]] [[Pinch (plasma physics)#Crushing cans with the pinch effect|can crusher pinch]]<ref>[http://www.powerlabs.org/pssecc.htm powerlabs.org – The PowerLabs Solid State Can Crusher!] {{Webarchive|url=https://web.archive.org/web/20170820105856/http://www.powerlabs.org/pssecc.htm |date=20 अगस्त 2017 }}, 2002</ref>
|-
|3.4×10<sup>3</sup> J || Kinetic energy of world-record men's [[hammer throw]] (7.26&nbsp;kg<ref>{{cite web|title=Hammer Throw – Introduction|url=http://www.iaaf.org/community/athletics/trackfield/newsid=9418.html|publisher=IAAF|accessdate=12 December 2011|archive-url=https://web.archive.org/web/20111122194630/http://www.iaaf.org/community/athletics/trackfield/newsid=9418.html|archive-date=22 नवंबर 2011|url-status=live}}</ref> thrown at 30.7&nbsp;m/s<ref>{{cite web|last=Otto|first=Ralf M.|title=HAMMER THROW WR PHOTOSEQUENCE – YURIY SEDYKH|url=http://hammerthrow.org/wp-content/uploads/photosequences/otto_sedykh_wr.pdf|format=pdf|accessdate=4 November 2011|quote=The total release velocity is 30.7 m/sec|archive-url=https://web.archive.org/web/20140813044843/http://hammerthrow.org/wp-content/uploads/photosequences/otto_sedykh_wr.pdf|archive-date=13 अगस्त 2014|url-status=dead}}</ref> in 1986)<ref>Calculated:  1/2 * 7.26 kg * (30.7 m/s)^2 = 3420 J</ref>
|-
|3.6×10<sup>3</sup> J || ≡ 1&nbsp;W·h ([[Watt]]-hour)<ref name=NIST_SI_units/>
|-
|4.2×10<sup>3</sup> J || Energy released by explosion of 1 gram of [[trinitrotoluene|TNT]]<ref name=NIST_SI_units/><ref name="ReferenceA">4.2e9 J/ton of TNT-equivalent * (1 ton/1e6 grams) = 4.2e3 J/gram of TNT-equivalent</ref>
|-
|4.2×10<sup>3</sup> J || ≈ 1 food [[Calorie]] (large calorie)
|-
|~7×10<sup>3</sup> J || Muzzle energy of an [[elephant gun]], e.g. firing a [[.458 Winchester Magnum]]<ref name="accurate458">{{cite web|title=.458 Winchester Magnum|url=http://www.accuratepowder.com/data/PerCaliber2Guide/Rifle/Standarddata(Rifle)/458Cal(11.63mm)/458%20Winchester%20Magnum%20pages%20339%20and%20340.pdf|format=pdf|work=Accurate Powder|publisher=Western Powders Inc|accessdate=7 September 2010|archive-url=https://web.archive.org/web/20070928011847/http://www.accuratepowder.com/data/PerCaliber2Guide/Rifle/Standarddata(Rifle)/458Cal(11.63mm)/458%20Winchester%20Magnum%20pages%20339%20and%20340.pdf|archive-date=28 सितंबर 2007|url-status=live}}</ref>
|-
|9×10<sup>3</sup> J || Energy in an alkaline AA battery<ref>{{cite web|title=Battery energy storage in various battery sizes|url=http://www.allaboutbatteries.com/Energy-tables.html|publisher=AllAboutBatteries.com|accessdate=15 December 2011|archive-url=https://web.archive.org/web/20111204090808/http://www.allaboutbatteries.com/Energy-tables.html|archive-date=4 दिसंबर 2011|url-status=dead}}</ref>
|-
|rowspan=4|10<sup>4</sup>
|rowspan=4| &nbsp;
| 1.7×10<sup>4</sup> J || Energy released by the [[metabolism]] of 1 gram of [[carbohydrates]]<ref>{{cite web|title=Energy Density of Carbohydrates|url=http://hypertextbook.com/facts/2007/AnuragPanda.shtml|work=The Physics Factbook|accessdate=5 November 2011|archive-url=https://web.archive.org/web/20111126055006/http://hypertextbook.com/facts/2007/AnuragPanda.shtml|archive-date=26 नवंबर 2011|url-status=dead}}</ref> or [[protein]]<ref>{{cite web|title=Energy Density of Protein|url=http://hypertextbook.com/facts/2003/DavidDukhan.shtml|work=The Physics Factbook|accessdate=5 November 2011|archive-url=https://web.archive.org/web/20111126061719/http://hypertextbook.com/facts/2003/DavidDukhan.shtml|archive-date=26 नवंबर 2011|url-status=dead}}</ref>
|-
| 3.8×10<sup>4</sup> J || Energy released by the metabolism of 1 gram of [[fat]]<ref>{{cite web|title=Energy Density of Fats|url=http://hypertextbook.com/facts/2004/PingZhang.shtml|work=The Physics Factbook|accessdate=5 November 2011|archive-url=https://web.archive.org/web/20111126060720/http://hypertextbook.com/facts/2004/PingZhang.shtml|archive-date=26 नवंबर 2011|url-status=dead}}</ref>
|-
| 4–5×10<sup>4</sup> J || Energy released by the [[combustion]] of 1 gram of [[gasoline]]<ref name=gascomb>{{cite web|title=Energy Density of Gasoline|url=http://hypertextbook.com/facts/2003/ArthurGolnik.shtml|work=The Physics Factbook|accessdate=5 November 2011|archive-url=https://web.archive.org/web/20111126061300/http://hypertextbook.com/facts/2003/ArthurGolnik.shtml|archive-date=26 नवंबर 2011|url-status=dead}}</ref>
|-
| 5×10<sup>4</sup> J || Kinetic energy of 1 gram of matter moving at 10&nbsp;km/s<ref>Calculated:  E = 1/2 m*v^2 = 1/2 * (1e-3 kg) * (1e4 m/s)^2 = 5e4 J.</ref>
|-
|rowspan=2|10<sup>5</sup>
|rowspan=2| &nbsp;
| {{nowrap|3×10<sup>5</sup> J}}—{{nowrap|15×10<sup>5</sup> J}} || [[Kinetic energy]] of an [[automobile]] at highway speeds (1 to 5 tons<ref name=car_weights>{{cite web|title=List of Car Weights|url=http://cars.lovetoknow.com/List_of_Car_Weights|publisher=LoveToKnow|accessdate=13 December 2011|quote=3000 to 12000 pounds|archive-url=https://web.archive.org/web/20111204043323/http://cars.lovetoknow.com/List_of_Car_Weights|archive-date=4 दिसंबर 2011|url-status=dead}}</ref> at {{nowrap|89 km/h}} or {{nowrap|55 mph}})<ref>Calculated:  Using car weights of 1 ton to 5 tons. E = 1/2 m*v^2 = 1/2 * (1e3 kg) * (55 mph * 1600 m/mi / 3600 s/hr) = 3.0e5 J.  E = 1/2 * (5e3 kg) * (55 mph * 1600 m/mi / 3600 s/hr) = 15e5 J.</ref>
|-
| 5×10<sup>5</sup> J
| Kinetic energy of 1 gram of a [[meteor]] hitting Earth<ref>{{cite web|last=Muller|first=Richard A.|title=Kinetic Energy in a meteor|url=http://muller.lbl.gov/teaching/Physics10/old%20physics%2010/physics%2010%20notes/meteorKE.html|work=Old Physics 10 notes|access-date=14 अगस्त 2017|archive-url=https://web.archive.org/web/20120402214238/http://muller.lbl.gov/teaching/Physics10/old%20physics%2010/physics%2010%20notes/meteorKE.html|archive-date=2 अप्रैल 2012|url-status=dead}}</ref>
|-
|rowspan=5|10<sup>6</sup>{{Anchor|106}}
|rowspan=5| [[Mega-]] (MJ)
|1×10<sup>6</sup> J || [[Kinetic energy]] of a 2 [[tonne]]<ref name=car_weights/> vehicle at 32 metres per second (115&nbsp;km/h or 72&nbsp;mph)<ref>Calculated:  KE = 1/2 * 2e3 kg * (32 m/s)^2 = 1.0e6 J</ref>
|-
|1.2×10<sup>6</sup> J || Approximate [[food energy]] of a snack such as a [[Snickers bar]] (280 food calories)<ref>{{cite web|url=http://www.nal.usda.gov/fnic/foodcomp/search/ |title=Candies, MARS SNACKFOOD US, SNICKERS Bar (NDB No. 19155) |work=USDA Nutrient Database |publisher=USDA |accessdate=14 November 2011 |url-status=dead |archiveurl=https://web.archive.org/web/20150303184216/http://www.nal.usda.gov/fnic/foodcomp/search/ |archivedate= 3 March 2015 |df= }}</ref>
|-
|3.6×10<sup>6</sup> J || = 1 kWh (kilowatt-hour) (used for electricity)<ref name=NIST_SI_units/>
|-
|4.2×10<sup>6</sup> J || Energy released by explosion of 1 kilogram of [[trinitrotoluene|TNT]]<ref name=NIST_SI_units/><ref name="ReferenceA"/>
|-
|8.4×10<sup>6</sup> J || Recommended food energy intake per day for a moderately active woman (2000 food calories)<ref name=nih_balance>{{cite web|title=How to Balance the Food You Eat and Your Physical Activity and Prevent Obesity|url=http://www.nhlbi.nih.gov/health/public/heart/obesity/wecan/healthy-weight-basics/balance.htm|work=Healthy Weight Basics|publisher=National Heart Lung and Blood Institutde|accessdate=14 November 2011|archive-url=https://web.archive.org/web/20111108061015/http://www.nhlbi.nih.gov/health/public/heart/obesity/wecan/healthy-weight-basics/balance.htm|archive-date=8 नवंबर 2011|url-status=live}}</ref><ref>Calculated:  2000 food calories = 2.0e6 cal * 4.184 J/cal = 8.4e6 J</ref>
|}

==10<sup>7</sup> to 10<sup>12</sup> J==
{| class="wikitable"
|-
|rowspan=6|10<sup>7</sup>
|rowspan=6|&nbsp;
| 1×10<sup>7</sup> J
| Kinetic energy of the armor-piercing round fired by the assault guns of the [[ISU-152]] tank<ref>Calculated:  1/2 * m * v^2 = 1/2 * 48.78 kg * (655 m/s)^2 = 1.0e7 J.</ref><!-- Need a source for the muzzle velocity and round weight -->{{Citation needed|date=January 2012}}
|-
| 1.1×10<sup>7</sup> J || Recommended food energy intake per day for a moderately active man (2600 food calories)<ref name=nih_balance/><ref>Calculated:  2600 food calories = 2.6e6 cal * 4.184 J/cal = 1.1e7 J</ref>
|-
| 3.7×10<sup>7</sup> J
| $1 of electricity at a cost of $0.10/kWh (the US average retail cost in 2009)<ref>{{cite web|title=Table 3.3 Consumer Price Estimates for Energy by Source, 1970–2009|url=http://www.eia.gov/totalenergy/data/annual/showtext.cfm?t=ptb0303|work=Annual Energy Review|publisher=US Energy Information Administration|accessdate=17 December 2011|date=19 October 2011|quote=$28.90 per million BTU|archive-url=https://web.archive.org/web/20111114114034/http://www.eia.gov/totalenergy/data/annual/showtext.cfm?t=ptb0303|archive-date=14 नवंबर 2011|url-status=live}}</ref><ref>Calculated J per dollar:  1 million BTU/$28.90 = 1e6 BTU / 28.90 dollars * 1.055e3 J/BTU  = 3.65e7 J/dollar</ref><ref>Calculated cost per kWh:  1 kWh * 3.60e6 J/kWh / 3.65e7 J/dollar = 0.0986 dollar/kWh</ref>
|-
| 4×10<sup>7</sup> J
| Energy from the combustion of 1 cubic meter of [[natural gas]]<ref>{{cite web|title=Energy in a Cubic Meter of Natural Gas|url=http://hypertextbook.com/facts/2002/JanyTran.shtml|work=The Physics Factbook|accessdate=15 December 2011|archive-url=https://web.archive.org/web/20111126053851/http://hypertextbook.com/facts/2002/JanyTran.shtml|archive-date=26 नवंबर 2011|url-status=dead}}</ref>
|-
| 4.2×10<sup>7</sup> J
| Caloric energy consumed by [[Olympic Games|Olympian]] [[Michael Phelps]] on a daily basis during Olympic training<ref>{{cite web|title=The Olympic Diet of Michael Phelps|url=http://www.webmd.com/diet/news/20080813/the-olympic-diet-of-michael-phelps|work=WebMD|accessdate=28 December 2011|archive-url=https://web.archive.org/web/20111226210631/http://www.webmd.com/diet/news/20080813/the-olympic-diet-of-michael-phelps|archive-date=26 दिसंबर 2011|url-status=live}}</ref>
|-
| 6.3×10<sup>7</sup> J
| Theoretical minimum energy required to accelerate 1&nbsp;kg of matter to [[escape velocity]] from Earth's surface (ignoring atmosphere)<ref>{{cite web|last=Cline|first=James E. D.|title=Energy to Space|url=http://home.earthlink.net/~jedcline/ets.html|accessdate=13 November 2011|quote=6.27E7 Joules / Kg|archive-url=https://web.archive.org/web/20110925162612/http://home.earthlink.net/~jedcline/ets.html|archive-date=25 सितंबर 2011|url-status=live}}</ref>
|-
|rowspan=4|10<sup>8</sup>
|rowspan=4| &nbsp;
| 1×10<sup>8</sup> J || Kinetic energy of a 55 tonne aircraft at typical landing speed (59&nbsp;m/s or 115 knots){{Citation needed|date=November 2011}}
|-
|1.1×10<sup>8</sup> J || ≈ 1 [[therm]], depending on the temperature<ref name=NIST_SI_units/>
|-
|1.1×10<sup>8</sup> J || ≈ 1 [[Tour de France]], or ~90 hours<ref>{{cite web|title=Tour de France Winners, Podium, Times|url=http://bikeraceinfo.com/tdf/tdfindex.html|publisher=Bike Race Info|accessdate=10 December 2011|archive-url=https://web.archive.org/web/20111207202120/http://bikeraceinfo.com/tdf/tdfindex.html|archive-date=7 दिसंबर 2011|url-status=dead}}</ref> ridden at 5&nbsp;W/kg<ref>{{cite web|title=Watts/kg|url=http://www.flammerouge.je/content/3_factsheets/constant/wattkilobench.htm|publisher=Flamme Rouge|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20120102133701/http://www.flammerouge.je/content/3_factsheets/constant/wattkilobench.htm|archive-date=2 जनवरी 2012|url-status=dead}}</ref> by a 65&nbsp;kg rider<ref>Calculated:  90 hr * 3600 seconds/hr * 5 W/kg * 65 kg = 1.1e8 J</ref>
|-
|7.3×10<sup>8</sup> J || ≈ Energy from burning 16 kilograms of oil (using 135&nbsp;kg per barrel of light crude){{Citation needed|date=December 2011}}<!-- 6120 MJ is 1 bboe which is 135 kg light crude of about 0.85 density - therefore 16&nbsp;kg produces 725 MJ -->
|-
|rowspan=10|10<sup>9</sup>{{Anchor|109}}
|rowspan=10| [[Giga-]] (GJ)
|1–10×10<sup>9</sup> J  || Energy in an average [[lightning]] bolt<ref>{{cite web|last=Smith|first=Chris|title=How do Thunderstorms Work?|url=http://www.thenakedscientists.com/HTML/articles/article/howdothunderstormswork-2/|publisher=The Naked Scientists|accessdate=15 November 2011|quote=It discharges about 1–10 billion joules of energy|archive-url=https://web.archive.org/web/20120127132309/http://www.thenakedscientists.com/HTML/articles/article/howdothunderstormswork-2/|archive-date=27 जनवरी 2012|url-status=dead}}</ref> (thunder)<!--search hint-->
|-
|1.1×10<sup>9</sup> J || Magnetic stored energy in the world's largest toroidal [[superconducting magnet]] for the [[ATLAS experiment]] at [[CERN]], Geneva<ref>{{cite web|title=Powering up ATLAS's mega magnet|url=http://user.web.cern.ch/public/en/Spotlight/SpotlightATLAS-en.html|work=Spotlight on...|publisher=CERN|accessdate=10 December 2011|quote=magnetic energy of 1.1 Gigajoules|archive-url=https://web.archive.org/web/20111130024727/http://user.web.cern.ch/public/en/Spotlight/SpotlightATLAS-en.html|archive-date=30 नवंबर 2011|url-status=dead}}</ref>
|-
|1.2×10<sup>9</sup> J || Inflight 100-ton [[Boeing 757|Boeing 757-200]] at 300 [[knot]]s (154&nbsp;m/s)
|-
|1.4x10<sup>9</sup> J || Theoretical minimum amount of energy required to melt a tonne of steel (380 [[kWh]])<ref>{{cite web|title=ITP Metal Casting: Melting Efficiency Improvement|url=http://www1.eere.energy.gov/industry/metalcasting/pdfs/umr22_fs.pdf|work=ITP Metal Casting|publisher=U.S. Department of Energy|accessdate=14 November 2011|format=PDF|quote=377 kWh/mt|archive-url=https://web.archive.org/web/20090628213117/http://www1.eere.energy.gov/industry/metalcasting/pdfs/umr22_fs.pdf|archive-date=28 जून 2009|url-status=live}}</ref><ref>Calculated: 380 kW-h * 3.6e6 J/kW-h = 1.37e9 J</ref>
|-
| 2x10<sup>9</sup> J || Energy of an ordinary {{nowrap|61 liter}} gasoline tank of a car.<!-- m = p * V ; Q = (J/m) * m ; mass = density * volume ; energy = energy_density * mass ; 4.5*10^7 * 719.7 * 0.061 = 2.0*10^9 --><!-- gasoline J/kg --><ref name=gascomb/><!-- gasoline kg/m<sup>3</sup> --><ref>{{cite web | title = Lead-Free Gasoline Material Safety Data Sheet | author = Bell Fuels | publisher = [[NOAA]] | url = http://www.sefsc.noaa.gov/HTMLdocs/Gasoline.htm | accessdate = 6 July 2008 | archive-url = https://web.archive.org/web/20020820074636/http://www.sefsc.noaa.gov/HTMLdocs/Gasoline.htm | archive-date = 20 अगस्त 2002 | url-status = dead }}</ref><!-- tank volume 0.061 m<sup>3</sup> (Volvo 240) --><ref>[http://www.thepartsbin.com/guides/volvo/fuel_tank.html thepartsbin.com – Volvo Fuel Tank: Compare at The Parts Bin]{{Dead link|date=जून 2020 |bot=InternetArchiveBot }}, 6 May 2012</ref>
|-
|2×10<sup>9</sup> J || [[Planck energy]], the unit of energy in [[Planck units]]<ref><math>E_p = \sqrt{\frac{\hbar c^5}{G}} </math></ref>
|-
|3×10<sup>9</sup> J || Inflight 125-ton [[Boeing 767|Boeing 767-200]] flying at 373 [[knot]]s (192&nbsp;m/s)
|-
|3.3×10<sup>9</sup> J || Approximate average amount of energy expended by a human heart [[muscle]] over an 80-year lifetime<ref>{{cite web|title=Power of a Human Heart|url=http://hypertextbook.com/facts/2003/IradaMuslumova.shtml|work=The Physics Factbook|accessdate=10 December 2011|quote=The mechanical power of the human heart is ~1.3 watts|archive-url=https://web.archive.org/web/20111126054217/http://hypertextbook.com/facts/2003/IradaMuslumova.shtml|archive-date=26 नवंबर 2011|url-status=dead}}</ref><ref>Calculated:  1.3 J/s * 80 years * 3.16e7 s/year = 3.3e9 J</ref>
|-
|4.2×10<sup>9</sup> J || Energy released by explosion of 1 [[TNT equivalent|ton of TNT]].
|-
|4.5×10<sup>9</sup> J || Average annual energy usage of a standard [[refrigerator]]<ref>{{cite web|title=U.S. Household Electricity Uses: A/C, Heating, Appliances|url=http://www.eia.gov/emeu/reps/enduse/er01_us.html|work=U.S.  HOUSEHOLD ELECTRICITY REPORT|publisher=EIA|accessdate=13 December 2011|quote=For refrigerators in 2001, the average UEC was 1,239 kWh|archive-url=https://web.archive.org/web/20111223072447/http://www.eia.gov/emeu/reps/enduse/er01_us.html|archive-date=23 दिसंबर 2011|url-status=live}}</ref><ref>Calculated:  1239 kWh * 3.6e6 J/kWh = 4.5e9 J</ref>
|-
|6.1×10<sup>9</sup> J || ≈ 1 bboe ([[barrel of oil equivalent]])<ref name="oe">'''[http://www.altenergyaction.org/mambo/index.php?option=com_content&task=view&id=9 Energy Units] {{Webarchive|url=https://web.archive.org/web/20161010120259/http://www.altenergyaction.org/mambo/index.php?option=com_content&task=view&id=9 |date=10 अक्तूबर 2016 }}''', by Arthur Smith, 21 January 2005</ref>
|-
|rowspan=6|10<sup>10</sup>
|rowspan=6| &nbsp;
|2.3×10<sup>10</sup> J || Kinetic energy of an [[Airbus A380]] at cruising speed (560 tonnes at 562 knots or 289&nbsp;m/s){{Citation needed|date=December 2011}}
|-
|4.2×10<sup>10</sup> J || ≈ 1 toe ([[ton of oil equivalent]])<ref name="oe"/>
|-
|5×10<sup>10</sup> J || Yield energy of a [[Massive Ordnance Air Blast]] bomb, the second most powerful non-nuclear weapon ever designed<ref>{{cite web|title=Top 10 Biggest Explosions|url=http://listverse.com/2011/11/28/top-10-biggest-explosions/|publisher=Listverse|accessdate=10 December 2011|quote=a yield of 11 tons of TNT|archive-url=https://web.archive.org/web/20111205214358/http://listverse.com/2011/11/28/top-10-biggest-explosions/|archive-date=5 दिसंबर 2011|url-status=dead}}</ref><ref>Calculated:  11 tons of TNT-equivalent * 4.184e9 J/ton of TNT-equivalent = 4.6e10 J</ref>
|-
|7.3×10<sup>10</sup> J || Energy consumed by the average U.S. automobile in the year 2000<ref>{{cite web|title=Emission Facts: Average Annual Emissions and Fuel Consumption for Passenger Cars and Light Trucks|url=http://www.epa.gov/otaq/consumer/f00013.htm|publisher=EPA|accessdate=12 December 2011|quote="581 gallons of gasoline"|archive-url=https://web.archive.org/web/20111202221408/http://www.epa.gov/otaq/consumer/f00013.htm|archive-date=2 दिसंबर 2011|url-status=live}}</ref><ref>{{cite web|title=200 Mile-Per-Gallon Cars?|url=http://www.uwgb.edu/dutchs/pseudosc/200mpgcar.htm|accessdate=12 December 2011|quote=a gallon of gas ... 125 million joules of energy|archive-url=https://web.archive.org/web/20111219011152/http://www.uwgb.edu/dutchs/pseudosc/200mpgcar.htm|archive-date=19 दिसंबर 2011|url-status=dead}}</ref><ref>Calculated:  581 gallons * 125e6 J/gal = 7.26e10 J</ref>
|-
|8.6×10<sup>10</sup> J || ≈ 1 MW·d ([[megawatt]]-day), used in the context of power plants<ref>Calculated:  1e6 Watts * 86400 seconds/day = 8.6e10 J</ref>
|-
|8.8×10<sup>10</sup> J || Total energy [[nuclear explosions|released]] in the [[nuclear fission]] of one gram of [[uranium-235]]<ref name="Energy From Uranium Fission"/><ref name="Conversion from eV to J"/><ref>Calculated:  3.44e-10 J/U-235-fission * 1e-3 kg / (235 amu per U-235-fission * 1.66e-27 amu/kg) = 8.82e-10 J</ref>
|-
|10<sup>11</sup> || &nbsp; || 2.4×10<sup>11</sup> J || Approximate food energy consumed by an average human in an 80-year lifetime.<ref>Calculated:  2000 kcal/day * 365 days/year * 80 years = 2.4e11 J</ref>
|-
|rowspan=4|10<sup>12</sup>{{Anchor|1012}}
|rowspan=4| [[Tera-]] (TJ)
|3.4×10<sup>12</sup> J
| Maximum fuel energy of an [[Airbus A330]]-300 (97,530 liters<ref>{{cite web|title=A330-300 Dimensions & key data|url=http://www.airbus.com/aircraftfamilies/passengeraircraft/a330family/a330-300/specifications/|publisher=Airbus|accessdate=12 December 2011|quote=97530 litres|archive-url=https://www.webcitation.org/6DrfekJmD?url=http://www.airbus.com/aircraftfamilies/passengeraircraft/a330family/a330-300/specifications/|archive-date=22 जनवरी 2013|url-status=live}}</ref> of [[Jet A-1]]<ref name=bp_jet_a1>{{cite web|url=http://www.bp.com/liveassets/bp_internet/aviation/air_bp/STAGING/local_assets/downloads_pdfs/a/air_bp_products_handbook_04004_1.pdf |title=Archived copy |accessdate=2011-08-19 |url-status=dead |archiveurl=https://web.archive.org/web/20110608075828/http://www.bp.com/liveassets/bp_internet/aviation/air_bp/STAGING/local_assets/downloads_pdfs/a/air_bp_products_handbook_04004_1.pdf |archivedate= 8 June 2011 |df= }}</ref>)<ref>Calculated: 97530 liters * 0.804&nbsp;kg/L * 43.15&nbsp;MJ/kg = 3.38e12 J</ref>
|-
|3.6×10<sup>12</sup> J
| 1 GW·h ([[gigawatt]]-hour)<ref>Calculated: 1e9 Watts * 3600 seconds/hour</ref>
|-
|4×10<sup>12</sup> J
| Electricity generated by one 20-kg [[CANDU]] fuel bundle assuming ~29%<ref>{{cite web|last=Weston|first=Kenneth|title=Chapter 10.  Nuclear Power Plants|url=http://www.personal.utulsa.edu/~kenneth-weston/chapter10.pdf|work=Energy Conversion|accessdate=13 December 2011|format=pdf|quote=The thermal efficiency of a CANDU plant is only about 29%|archive-url=https://web.archive.org/web/20111005120238/http://www.personal.utulsa.edu/~kenneth-weston/chapter10.pdf|archive-date=5 अक्तूबर 2011|url-status=dead}}</ref> thermal efficiency of reactor<ref>{{cite web|title=CANDU and Heavy Water Moderated Reactors|url=http://www.nucleartourist.com/type/candu.htm|accessdate=12 December 2011|quote=fuel burnup in a CANDU is only 6500 to 7500 MWd per metric ton uranium|archive-url=https://web.archive.org/web/20111116080800/http://www.nucleartourist.com/type/candu.htm|archive-date=16 नवंबर 2011|url-status=dead}}</ref><ref>Calculated:  7500e6 Watt-days/tonne * (0.020 tonnes per bundle) * 86400 seconds/day = 1.3e13 J of burnup energy. Electricity = burnup * ~29% efficiency = 3.8e12 J</ref>
<!--
|-
|3.7×10<sup>12</sup> J
| Average orbital kinetic energy of the [[Mir]] space station (124 tonnes{{Citation needed|date=December 2011}} at about 7680&nbsp;m/s{{Citation needed|date=December 2011}})<ref>Calculated: E = 1/2 m.v<sup>2</sup> = 1/2 * 124000 kg * (7680m/s)<sup>2</sup> = 3.66e12 J</ref>
-->
|-
|6.4×10<sup>12</sup> J || Energy contained in jet fuel in a [[Boeing 747]]-100B aircraft at max fuel capacity (183,380 liters<ref>{{cite web|title=747 Classics Technical Specs |url=http://www.boeing.com/commercial/747family/pf/pf_classics.html |publisher=Boeing |accessdate=12 December 2011 |quote=183,380 L |url-status=dead |archiveurl=https://web.archive.org/web/20071210173616/http://www.boeing.com/commercial/747family/pf/pf_classics.html |archivedate=10 December 2007 }}</ref> of [[Jet A-1]]<ref name=bp_jet_a1/>)<ref>Calculated: 183380 liters * 0.804&nbsp;kg/L * 43.15&nbsp;MJ/kg = 6.36e12 J</ref>
|}

==10<sup>13</sup> to 10<sup>18</sup> J==
{| class="wikitable"
|-
|rowspan=4|10<sup>13</sup>
|rowspan=4| &nbsp;
|1.1×10<sup>13</sup> J || Energy of the maximum fuel an [[Airbus A380]] can carry (320,000 liters<ref>{{cite web|title=A380-800 Dimensions & key data|url=http://www.airbus.com/aircraftfamilies/passengeraircraft/a380family/a380-800/specifications/|publisher=Airbus|accessdate=12 December 2011|quote=320,000 L|archive-url=https://web.archive.org/web/20120708071501/http://www.airbus.com/aircraftfamilies/passengeraircraft/a380family/a380-800/specifications/|archive-date=8 जुलाई 2012|url-status=live}}</ref> of [[Jet A-1]]<ref name=bp_jet_a1/>)<ref>Calculated: 320,000 l * 0.804 kg/L * 43.15 &nbsp;MJ/kg = 11.1e12 J</ref>
|-
|1.2×10<sup>13</sup> J || Orbital kinetic energy of the [[International Space Station]] (417 tonnes<ref>{{cite web |url=http://www.nasa.gov/mission_pages/station/structure/isstodate.html |title=International Space Station: The ISS to Date |publisher=NASA |accessdate=23 August 2011 |archive-url=https://web.archive.org/web/20150611163133/http://www.nasa.gov/mission_pages/station/structure/isstodate.html |archive-date=11 जून 2015 |url-status=live }}</ref> at 7.7&nbsp;km/s<ref>{{cite web|title=The wizards of orbits|url=http://www.esa.int/esaCP/ESA104MBAMC_FeatureWeek_0.html|publisher=European Space Agency|accessdate=10 December 2011|quote=The International Space Station, for example, flies at 7.7&nbsp;km/s in one of the lowest practicable orbits|archive-url=https://web.archive.org/web/20111203141638/http://www.esa.int/esaCP/ESA104MBAMC_FeatureWeek_0.html|archive-date=3 दिसंबर 2011|url-status=live}}</ref>)<ref>Calculated: E = 1/2 m.v<sup>2</sup> = 1/2 * 417000 kg * (7700m/s)<sup>2</sup> = 1.2e13 J</ref>
|-
|6.3×10<sup>13</sup> J || Yield of the [[Little Boy]] atomic bomb dropped on [[Hiroshima]] in [[World War II]] (15 kilotons)<ref>{{cite web|title=What was the yield of the Hiroshima bomb?|url=http://www.warbirdforum.com/hiroshim.htm|publisher=Warbird's Forum|quote=21 kt|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20170913004426/https://www.warbirdforum.com/hiroshim.htm|archive-date=13 सितंबर 2017|url-status=dead}}</ref><ref>Calculated:  15 kt = 15e9 grams of TNT-equivalent * 4.2e3 J/gram TNT-equivalent = 6.3e13 J</ref>
|-
|9×10<sup>13</sup> J || Theoretical total [[mass-energy]] of 1 gram of matter<ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=-3&num=1&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215101/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=-3&num=1&From=kg&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
|rowspan=2|10<sup>14</sup>
|rowspan=2| &nbsp;
| 3.75×10<sup>14</sup> J || Total energy released by the [[Chelyabinsk meteor]].<ref name="chelyabinsk">{{cite web|title=JPL - Fireballs and bolides|url=https://cneos.jpl.nasa.gov/fireballs/|website=Jet Propulsion Laboratory|publisher=NASA|accessdate=13 April 2017|archive-url=https://web.archive.org/web/20170314153125/https://cneos.jpl.nasa.gov/fireballs/|archive-date=14 मार्च 2017|url-status=dead}}</ref>
|-
| 6×10<sup>14</sup> J || Energy released by an average [[hurricane]] in 1 second<ref name="noaa">{{cite web|title=How much energy does a hurricane release?|url=http://www.aoml.noaa.gov/hrd/tcfaq/D7.html|work=FAQ : HURRICANES, TYPHOONS, AND TROPICAL CYCLONES|publisher=NOAA|accessdate=12 November 2011|archive-url=https://web.archive.org/web/20171102212903/http://www.aoml.noaa.gov/hrd/tcfaq/D7.html|archive-date=2 नवंबर 2017|url-status=live}}</ref>
|-
|rowspan=3| 10<sup>15</sup>
|rowspan=3| [[Peta-]] (PJ) {{anchor|1015}}
|> 10<sup>15</sup> J || Energy released by a severe [[thunderstorm]]<ref>{{cite web|title=The Gathering Storms|url=http://www.cosmosmagazine.com/node/3302/full|publisher=COSMOS|accessdate=10 December 2011|archive-url=https://web.archive.org/web/20120404113209/http://www.cosmosmagazine.com/node/3302/full|archive-date=4 अप्रैल 2012|url-status=dead}}</ref>
|-
|1×10<sup>15</sup> J || Yearly [[electricity]] consumption in [[Greenland]] as of 2008<ref name="CIA_electricity_consumption">{{cite web|title=Country Comparison :: Electricity – consumption |url=https://www.cia.gov/library/publications/the-world-factbook/rankorder/2042rank.html |work=The World Factbook |publisher=CIA |accessdate=11 December 2011 |url-status=dead |archiveurl=https://web.archive.org/web/20120128032332/https://www.cia.gov/library/publications/the-world-factbook/rankorder/2042rank.html |archivedate=28 January 2012 |df= }}</ref><ref>Calculated:  288.6e6 kWh * 3.60e6 J/kWh = 1.04e15 J</ref>
|-
|4.2×10<sup>15</sup> J || Energy released by explosion of 1 [[TNT equivalent|megaton of TNT]]<ref name=NIST_SI_units/><ref>Calculated:  4.2e9 J/ton of TNT-equivalent * 1e6 tons/megaton = 4.2e15 J/megaton of TNT-equivalent</ref>
|-
|rowspan=3| 10<sup>16</sup>
|rowspan=3| &nbsp;
| 1×10<sup>16</sup> J || Estimated impact energy released in forming [[Meteor Crater]]{{Citation needed|date=November 2011}}
|-
| 1.1×10<sup>16</sup> J || Yearly [[electricity consumption]] in [[Mongolia]] as of 2010<ref name="CIA_electricity_consumption"/><ref>Calculated:  3.02e9 kWh * 3.60e6 J/kWh = 1.09e16 J</ref>
|-
| 9×10<sup>16</sup> J || [[Mass-energy]] in 1 kilogram of [[antimatter]] (or matter)<ref>Calculated:  E = mc^2 = 1 kg * (2.998e8 m/s)^2 = 8.99e16 J</ref>
|-
|rowspan=6| 10<sup>17</sup>
|rowspan=6| &nbsp;
|1×10<sup>17</sup> J || Energy released on the Earth's surface by the magnitude 9.1–9.3 [[2004 Indian Ocean earthquake and tsunami|2004 Indian Ocean earthquake]]<ref>{{cite web|url=http://neic.usgs.gov/neis/eq_depot/2004/eq_041226/neic_slav_e.html |title=USGS Energy and Broadband Solution |publisher=National Earthquake Information Center, US Geological Survey |accessdate=9 December 2011 |url-status=dead |archiveurl=https://web.archive.org/web/20100404013939/http://neic.usgs.gov/neis/eq_depot/2004/eq_041226/neic_slav_e.html |archivedate=4 April 2010 |df= }}</ref>
|-
|1.7×10<sup>17</sup> J || Total energy from the [[Sun]] that strikes the face of the [[Earth]] each second<ref name="sun1">The Earth has a [[cross section (geometry)|cross section]] of 1.274×10<sup>14</sup> [[square meter]]s and the [[solar constant]] is 1361 [[watt]]s per square meter.</ref>
|-
|2.1×10<sup>17</sup> J || Yield of the [[Tsar Bomba]], the largest [[nuclear weapon]] ever tested (50 megatons)<ref>{{cite web|title=The Soviet Weapons Program – The Tsar Bomba|url=http://www.nuclearweaponarchive.org/Russia/TsarBomba.html|publisher=The Nuclear Weapon Archive|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20180618223830/http://www.nuclearweaponarchive.org/Russia/TsarBomba.html|archive-date=18 जून 2018|url-status=live}}</ref><ref>Calculated:  50e6 tons TNT-equivalent * 4.2e9 J/ton TNT-equivalent = 2.1e17 J</ref>
|-
|4.2×10<sup>17</sup> J || Yearly [[electricity consumption]] of [[Norway]] as of 2008<ref name="CIA_electricity_consumption"/><ref>Calculated:  115.6e9 kWh * 3.60e6 J/kWh = 4.16e17 J</ref>
|-
|4.5×10<sup>17</sup> J || Approximate energy needed to accelerate one ton to one-tenth of the speed of light<!-- energy = 0.5*mass*speed<sup>2</sup> = 0.5 * 1000 * (c/10)^2 -->
|-
|8×10<sup>17</sup> J || Estimated energy released by the eruption of the [[1883 eruption of Krakatoa|Indonesian volcano, Krakatoa, in 1883]]<ref>{{cite book|last=Alexander|first=R. McNeill|title=Dynamics of Dinosaurs and Other Extinct Giants|year=1989|publisher=Columbia University Press|isbn=0-231-06667-8|url=https://books.google.com/books?id=0q_1xk3SVKEC|page=144|quote=the explosion of the island volcano Krakatoa in 1883, had about 200 megatonnes energy.|access-date=14 अगस्त 2017|archive-url=https://web.archive.org/web/20161203195922/https://books.google.com/books?id=0q_1xk3SVKEC|archive-date=3 दिसंबर 2016|url-status=live}}</ref><ref>Calculated:  200e6 tons of TNT equivalent * 4.2e9 J/ton of TNT equivalent = 8.4e17 J</ref>
|-
|rowspan=1| 10<sup>18</sup>{{Anchor|1018}}
|rowspan=1| [[Exa-]] (EJ)
|1.4×10<sup>18</sup> J || Yearly [[electricity consumption]] of [[South Korea]] as of 2009<ref name="CIA_electricity_consumption"/><ref>Calculated:  402e9 kWh * 3.60e6 J/kWh = 1.45e17 J</ref>
|}

==10<sup>19</sup> to 10<sup>24</sup> J==
{| class="wikitable"
|-
|rowspan=5| 10<sup>19</sup>
|rowspan=5| &nbsp;
|1.4×10<sup>19</sup> J || Yearly [[electricity consumption]] in the [[United States|U.S.]] as of 2009<ref name="CIA_electricity_consumption"/><ref>Calculated:  3.741e12 kWh * 3.600e6 J/kWh = 1.347e19 J</ref>
|-
|1.4×10<sup>19</sup>J || Yearly [[electricity production]] in the [[United States|U.S.]] as of 2009<ref name=CIA_us>{{cite web|title=United States|url=https://www.cia.gov/library/publications/the-world-factbook/geos/us.html|work=The World Factbook|publisher=USA|accessdate=11 December 2011|archive-url=https://web.archive.org/web/20080109013304/https://www.cia.gov/library/publications/the-world-factbook/geos/us.html|archive-date=9 जनवरी 2008|url-status=live}}</ref><ref>Calculated:  3.953e12 kWh * 3.600e6 J/kWh = 1.423e19 J</ref>
|-
|5×10<sup>19</sup> J || Energy released in 1-day by an average [[hurricane]] in producing rain (400 times greater than the wind energy)<ref name="noaa"/>
|-
|6.4×10<sup>19</sup> J || Yearly [[electricity consumption]] of the world {{As of|2008|lc=on}}<ref name=CIA_world>{{cite web|title=World|url=https://www.cia.gov/library/publications/the-world-factbook/geos/xx.html|work=The World Factbook|publisher=CIA|accessdate=11 December 2011|archive-url=https://web.archive.org/web/20180315230249/https://www.cia.gov/library/publications/the-world-factbook/geos/xx.html|archive-date=15 मार्च 2018|url-status=live}}</ref><ref>Calculated:  17.8e12 kWh * 3.60e6 J/kWh = 6.41e19 J</ref>
|-
|6.8×10<sup>19</sup> J || Yearly electricity generation of the world {{As of|2008|lc=on}}<ref name=CIA_world/><ref>Calculated:  18.95e12 kWh * 3.60e6 J/kWh = 6.82e19 J</ref>
<!--
|-
|6.7×10<sup>19</sup> J || Total energy released by the magnitude 8.8 [[2010 Chile earthquake]]{{Citation needed|date=November 2011}}
-->
|-
|rowspan=2| 10<sup>20</sup>
|rowspan=2| &nbsp;
|5x10<sup>20</sup> J || [[World energy resources and consumption|Total world annual energy consumption]] in 2010<ref name=BP_Statistical_Review_2011>{{cite web|title=Statistical Review of World Energy 2011 |url=http://www.bp.com/assets/bp_internet/globalbp/globalbp_uk_english/reports_and_publications/statistical_energy_review_2011/STAGING/local_assets/pdf/statistical_review_of_world_energy_full_report_2011.pdf |publisher=BP |accessdate=9 December 2011 |url-status=dead |archiveurl=https://web.archive.org/web/20110902033116/http://www.bp.com/assets/bp_internet/globalbp/globalbp_uk_english/reports_and_publications/statistical_energy_review_2011/STAGING/local_assets/pdf/statistical_review_of_world_energy_full_report_2011.pdf |archivedate= 2 September 2011 |df= }}</ref><ref>Calculated:  12002.4e6 tonnes of oil equivalent * 42e9 J/tonne of oil equivalent = 5.0e20 J</ref>
|-
|8×10<sup>20</sup> J || Estimated global [[uranium]] resources for generating electricity 2005<ref name=iaea>{{cite web|url=http://www.iaea.org/NewsCenter/News/2006/uranium_resources.html|publisher=iaea.org|title=Global Uranium Resources to Meet Projected Demand &#124; International Atomic Energy Agency|accessdate=26 December 2016|archive-url=https://web.archive.org/web/20140805201113/http://www.iaea.org/newscenter/news/2006/uranium_resources.html|archive-date=5 अगस्त 2014|url-status=live}}</ref><ref>{{Cite web |url=http://www.eia.doe.gov/pub/international/iealf/table63.xls |title=U.S. Energy Information Administration,  International Energy Generation |access-date=14 अगस्त 2017 |archive-url=https://web.archive.org/web/20000817093423/http://www.eia.doe.gov/pub/international/iealf/table63.xls |archive-date=17 अगस्त 2000 |url-status=live }}</ref><ref name="doe">{{cite web|url=http://www.eia.doe.gov/oiaf/ieo/electricity.html|publisher=eia.doe.gov|title=U.S. EIA International Energy Outlook 2007.|accessdate=26 December 2016|archive-url=https://web.archive.org/web/20110523001859/http://www.eia.doe.gov/oiaf/ieo/electricity.html|archive-date=23 मई 2011|url-status=live}}</ref><ref>Final 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:  6.25×10<sup>19</sup>×0.159×85&nbsp;= 8.01×10<sup>20</sup>.</ref>
|-
|rowspan=2| 10<sup>21</sup>
|rowspan=2| [[Zetta-]] (ZJ) {{anchor|1021}}
|6.9×10<sup>21</sup> J || Estimated energy contained in the world's [[natural gas]] [[Mineral resource classification#Mineral reserves|reserves]] as of 2010<ref name=BP_Statistical_Review_2011 /><ref>Calculated:  "6608.9 trillion cubic feet" => 6608.9e3 billion cubic feet * 0.025 million tonnes of oil equivalent/billion cubic feet * 1e6 tonnes of oil equivalent/million tonnes of oil equivalent * 42e9 J/tonne of oil equivalent = 6.9e21 J</ref>
|-
|7.9×10<sup>21</sup> J || Estimated energy contained in the world's [[petroleum]] reserves as of 2010<ref name=BP_Statistical_Review_2011 /><ref>Calculated: "188.8 thousand million tonnes" => 188.8e9 tonnes of oil * 42e9 J/tonne of oil = 7.9e21 J</ref>
|-
|rowspan=5| 10<sup>22</sup>
|rowspan=5| &nbsp;
|1.5×10<sup>22</sup>J || Total energy from the Sun that strikes the face of the Earth each day<ref name="sun1"/><ref>Calculated:  1.27e14 m^2 * 1370 W/m^2 * 86400 s/day = 1.5e22 J</ref>
|-
|2.4×10<sup>22</sup> J || Estimated energy contained in the world's [[coal]] reserves as of 2010<ref name=BP_Statistical_Review_2011 /><ref>Calculated:  860938 million tonnes of coal => 860938e6 tonnes of coal * (1/1.5 tonne of oil equivalent / tonne of coal) * 42e9 J/tonne of oil equivalent = 2.4e22 J</ref>
|-
|2.9×10<sup>22</sup> J || Identified global [[uranium-238]] resources using [[Fast-neutron reactor|fast reactor]] technology<ref name=iaea/>
|-
|3.9×10<sup>22</sup> J || Estimated energy contained in the world's [[fossil fuel]] reserves as of 2010<ref name=BP_Statistical_Review_2011 /><ref>Calculated:  natural gas + petroleum + coal = 6.9e21 J + 7.9e21 J + 2.4e22 J = 3.9e22 J</ref>
|-
|4×10<sup>22</sup> J || Estimated total energy released by the magnitude 9.1–9.3 [[2004 Indian Ocean earthquake and tsunami|2004 Indian Ocean earthquake]]<ref>{{cite web|url=http://neic.usgs.gov/neis/eq_depot/2004/eq_041226/neic_slav_hrv.html |title=USGS, Harvard Moment Tensor Solution |publisher=[[National Earthquake Information Center]] |date=26 December 2004 |accessdate=9 December 2011 |url-status=dead |archiveurl=https://web.archive.org/web/20100117084041/http://neic.usgs.gov/neis/eq_depot/2004/eq_041226/neic_slav_hrv.html |archivedate=17 January 2010 |df= }}</ref>
|-
|rowspan=3| 10<sup>23</sup>
|rowspan=3| &nbsp;
|-
|2.2×10<sup>23</sup> J || Total global [[uranium-238]] resources using fast reactor technology<ref name=iaea/>
|-
|5×10<sup>23</sup> J || Approximate energy released in the formation of the [[Chicxulub Crater]] in the [[Yucatán Peninsula]]<ref>{{cite journal|url=http://www.geosc.psu.edu/people/faculty/personalpages/tbralower/Braloweretal1998.pdf |date=April 1998 |title=The Cretaceous–Tertiary boundary cocktail: Chicxulub impact triggers margin collapse and extensive sediment gravity flows |first=Timothy J. |last=Bralower |author2=Charles K. Paull |author3=R. Mark Leckie |journal=[[Geology (journal)|Geology]] |volume=26 |issue=4 |pages=331–334 |accessdate=6 June 2013 |format=PDF |quote="The kinetic energy derived by the impact is estimated at ~5 × 10^30 ergs" |doi=10.1130/0091-7613(1998)026<0331:tctbcc>2.3.co;2 |bibcode=1998Geo....26..331B |url-status=dead |archiveurl=https://web.archive.org/web/20071128093102/http://www.geosc.psu.edu/people/faculty/personalpages/tbralower/Braloweretal1998.pdf |archivedate=28 November 2007 |df= }}</ref>
|-
| 10<sup>24</sup> || [[Yotta-]] (YJ) || 5.5×10<sup>24</sup> J || Total energy from the [[Sun]] that strikes the face of the [[Earth]] each year<ref name="sun1"/><ref>Calculated:  1.27e14 m^2 * 1370 W/m^2 * 86400 s/day = 5.5e24 J</ref>
|}

==> 10<sup>25</sup>  J==
{| class="wikitable"
|-
| 10<sup>25</sup> || &nbsp; || 6×10<sup>25</sup> J || Energy released by a typical [[solar flare]]
|-
| rowspan=2 | 10<sup>26</sup>
| rowspan=2 | &nbsp;
| 1.3×10<sup>26</sup> J || Conservative estimate of the energy released by the impact that created the [[Caloris basin]] on [[Mercury (planet)|Mercury]]{{Citation needed|date=November 2011}}
|-
| 3.8×10<sup>26</sup> J || Total energy output of the [[Sun]] each second<ref name=sun2>{{cite web|title=Ask Us:  Sun:  Amount of Energy the Earth Gets from the Sun|url=http://helios.gsfc.nasa.gov/qa_sun.html#sunenergymass|work=Cosmicopia|publisher=NASA|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20111106095009/http://helios.gsfc.nasa.gov/qa_sun.html#sunenergymass|archive-date=6 नवंबर 2011|url-status=dead}}</ref>
|-
| 10<sup>27</sup> || &nbsp; || &nbsp; || &nbsp;
|-
| 10<sup>28</sup> || &nbsp; || 3.8×10<sup>28</sup> J || Kinetic energy of the [[Moon]] in its [[Orbit of the Moon|orbit]] around the Earth (counting only its velocity relative to the Earth)<ref>{{cite web | url= http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html | title= Moon Fact Sheet | publisher= NASA | accessdate= 16 December 2011 | archive-url= https://web.archive.org/web/20100323165650/http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html | archive-date= 23 मार्च 2010 | url-status= live }}</ref><ref>Calculated:  KE = 1/2 * m * v^2.  v = 1.023e3 m/s.  m = 7.349e22 kg.  KE = 1/2 * (7.349e22 kg) * (1.023e3 m/s)^2 = 3.845e28 J.</ref>
|-
| 10<sup>29</sup> || &nbsp; || 2.1×10<sup>29</sup> J || [[Rotational energy]] of the [[Earth]]<ref>{{cite web|title=Moment of Inertia—Earth|url=http://scienceworld.wolfram.com/physics/MomentofInertiaEarth.html|work=Eric Weisstein's World of Physics|accessdate=5 November 2011|archive-url=https://web.archive.org/web/20190203090309/http://scienceworld.wolfram.com/physics/MomentofInertiaEarth.html|archive-date=3 फ़रवरी 2019|url-status=live}}</ref><ref>{{cite web|last=Allain|first=Rhett|title=Rotational energy of the Earth as an energy source|url=http://scienceblogs.com/dotphysics/2009/06/rotational-energy-of-the-earth-as-an-energy-source.php|work=.dotphysics|publisher=Science Blogs|accessdate=5 November 2011|quote=the Earth takes 23.9345 hours to rotate|archive-url=https://web.archive.org/web/20111117014824/http://scienceblogs.com/dotphysics/2009/06/rotational-energy-of-the-earth-as-an-energy-source.php|archive-date=17 नवंबर 2011|url-status=live}}</ref><ref>Calculated:  E_rotational = 1/2 * I * w^2 = 1/2 * (8.0e37 kg m^2) * (2*pi/(23.9345 hour period * 3600 seconds/hour))^2 = 2.1e29 J</ref>
|-
| 10<sup>30</sup> || &nbsp; || 1.8×10<sup>30</sup> J || [[Gravitational binding energy]] of [[Mercury (planet)|Mercury]]
|-
| 10<sup>31</sup> || &nbsp; || 3.3×10<sup>31</sup> J || Total energy output of the [[Sun]] each day<ref name="sun2"/><ref>Calculated:  3.8e26 J/s * 86400 s/day = 3.3e31 J</ref>
|-
| 10<sup>32</sup> || &nbsp; || 2×10<sup>32</sup> J || [[Gravitational binding energy]] of the Earth<ref>{{cite web|title=Earth's Gravitational Binding Energy|url=http://typnet.net/Essays/EarthBind.htm|accessdate=19 March 2012|quote=Variable Density Method: the Earth's gravitational binding energy is −1.711×10^32 J|archive-url=https://web.archive.org/web/20120317085735/http://typnet.net/Essays/EarthBind.htm|archive-date=17 मार्च 2012|url-status=dead}}</ref>
|-
| 10<sup>33</sup> || &nbsp; || 2.7×10<sup>33</sup> J || [[Earth|Earth's]] kinetic energy in its orbit<ref name="uwgb">{{cite web|url=http://www.uwgb.edu/DutchS/pseudosc/flipaxis.htm|publisher=uwgb.edu|title=DutchS/pseudosc/flipaxis|accessdate=26 December 2016|archive-url=https://web.archive.org/web/20170822172540/http://www.uwgb.edu/dutchs/pseudosc/flipaxis.htm|archive-date=22 अगस्त 2017|url-status=dead}}</ref>
|-
| 10<sup>34</sup> || &nbsp; || 1.2×10<sup>34</sup> J || Total energy output of the [[Sun]] each year<ref name="sun2"/><ref>Calculated:  3.8e26 J/s * 86400 s/day * 365.25 days/year = 1.2e34 J</ref>
|-
| 10<sup>39</sup> || &nbsp; || 6.6×10<sup>39</sup> J || Theoretical total [[mass-energy]] of the [[Moon]]
|-
|rowspan=2 | 10<sup>41</sup>
|rowspan=2 | &nbsp;
| 5.4×10<sup>41</sup> J || Theoretical total [[mass-energy]] of the [[Earth]]<ref>{{cite web | url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Earth&Display=Facts | title=Earth: Facts & Figures | work=Solar System Exploration | publisher=NASA | accessdate=29 September 2011 | archive-url=https://web.archive.org/web/20150419035450/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Earth&Display=Facts | archive-date=19 अप्रैल 2015 | url-status=live }}</ref><ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=24&num=6.0&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215023/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=24&num=6.0&From=kg&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
| 6.87×10<sup>41</sup> J || Gravitational binding energy of the [[Sun]]<ref name="U"><math>U = \frac{(3/5)GM^2}{r}</math><br/>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)<br>Lang, K. R. 1980, ''Astrophysical Formulae'' (Berlin: Springer Verlag), p. 272</ref>
|-
|rowspan=1|10<sup>43</sup>
|rowspan=1| &nbsp;
| 5×10<sup>43</sup> J
| Total energy of all gamma rays in a typical [[gamma-ray burst]]<ref>{{Cite journal | last1 = Frail | first1 = D. A. | last2 = Kulkarni | first2 = S. R. | last3 = Sari | first3 = R. | last4 = Djorgovski | first4 = S. G. | last5 = Bloom | first5 = J. S. | last6 = Galama | first6 = T. J. | last7 = Reichart | first7 = D. E. | last8 = Berger | first8 = E. | last9 = Harrison | first9 = F. A. | last10 = Price | first10 = P. A. | last11 = Yost | first11 = S. A. | last12 = Diercks | first12 = A. | last13 = Goodrich | first13 = R. W. | last14 = Chaffee | first14 = F. | title = Beaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir | doi = 10.1086/338119 | journal = The Astrophysical Journal | volume = 562 | pages = L55 | year = 2001 | pmid =  | pmc = | url = http://arxiv.org/PS_cache/astro-ph/pdf/0102/0102282v1.pdf| format = PDF|arxiv = astro-ph/0102282 |bibcode = 2001ApJ...562L..55F }} "the gamma-ray energy release, corrected for geometry, is narrowly clustered around 5 * 10^50 erg"</ref><ref>Calculated:  5e50 erg * 1e-7 J/erg = 5e43 J</ref>
|-
|rowspan=2|10<sup>44</sup>
|rowspan=2| &nbsp;
| 1–2×10<sup>44</sup> J || Estimated energy released in a [[supernova]],<ref>{{cite journal | author=Khokhlov, A.; Mueller, E.; Hoeflich, P. | title=Light curves of Type IA supernova models with different explosion mechanisms | journal=[[Astronomy and Astrophysics]] | year=1993 | volume=270 | issue=1–2 | pages=223–248 | bibcode=1993A&A...270..223K | last2=Mueller | last3=Hoeflich }}</ref> sometimes referred to as a ''[[foe (unit)|foe]]''
|-
| {{Val|1.2|e=44|u=J}} || Approximate lifetime energy output of the [[Sun]].<!-- Computation from [[Foe (unit)]] -->
|-
|rowspan=2|10<sup>45</sup>
|rowspan=2| &nbsp;
| {{Val|1.1|0.2|e=45|u=J}} || Brightest observed [[hypernova]] [[ASASSN-15lh]]<ref>{{cite journal
 |last1=Dong|first1=S.|last2=Shappee|first2=B. J.|last3=Prieto|first3=J. L.|last4=Jha|first4=S. W.
 |last5=Stanek|first5=K. Z.|last6=Holoien|first6=T. W.- S.|last7=Kochanek|first7=C. S.|last8=Thompson|first8=T. A.
 |last9=Morrell|first9=N.|last10=Thompson|first10=I. B.|last11=Basu|first11=U.|last12=Beacom|first12=J. F.
 |last13=Bersier|first13=D.|last14=Brimacombe|first14=J.|last15=Brown|first15=J. S.
 |last16=Bufano|first16=F.|last17=Chen|first17=P.|last18=Conseil|first18=E.|last19=Danilet|first19=A. B. 
 |last20=Falco|first20=E.|last21=Grupe|first21=D.|last22=Kiyota|first22=S.|last23=Masi|first23=G.
 |last24=Nicholls|first24=B.|last25=Olivares E.|first25=F.|last26=Pignata|first26=G.|last27=Pojmanski|first27=G.
 |last28=Simonian|first28=G. V.|last29=Szczygiel|first29=D. M.|last30=Wozniak|first30=P. R.
 |display-authors=10
 |title=ASASSN-15lh: A highly super-luminous supernova
 |journal=[[Science (journal)|Science]]
 |date=15 January 2016
 |volume=351 |issue=6270 |pages=257–260
 |doi=10.1126/science.aac9613
 |arxiv=1507.03010|bibcode = 2016Sci...351..257D |pmid=26816375}}</ref>
|-
| few times×10<sup>45</sup> J || Beaming-corrected 'True' total [[energy]] (Energy in gamma rays+relativistic kinetic energy) of hyper-energetic [[Gamma Ray Burst]]<ref>url= http://arxiv.org/abs/1003.3885 {{Webarchive|url=https://web.archive.org/web/20180505070214/https://arxiv.org/abs/1003.3885 |date=5 मई 2018 }}</ref><ref>url= http://arxiv.org/abs/1004.2900 {{Webarchive|url=https://web.archive.org/web/20180505070459/https://arxiv.org/abs/1004.2900 |date=5 मई 2018 }}</ref><ref>url= http://arxiv.org/abs/0905.0690 {{Webarchive|url=https://web.archive.org/web/20180505070304/https://arxiv.org/abs/0905.0690 |date=5 मई 2018 }}</ref><ref>url= http://tsvi.phys.huji.ac.il/presentations/Frail_AstroExtreme.pdf {{Webarchive|url=https://web.archive.org/web/20140801172839/http://tsvi.phys.huji.ac.il/presentations/Frail_AstroExtreme.pdf |date=1 अगस्त 2014 }}</ref><ref>url= http://fermi.gsfc.nasa.gov/science/mtgs/grb2010/tue/Dale_Frail.ppt {{Webarchive|url=https://web.archive.org/web/20161223063425/http://fermi.gsfc.nasa.gov/science/mtgs/grb2010/tue/Dale_Frail.ppt |date=23 दिसंबर 2016 }}</ref>
|-
| 10<sup>46</sup> || &nbsp; || 1×10<sup>46</sup> J || Estimated energy released in a [[hypernova]]<ref>{{cite web|title=A Hypernova: The Super-charged Supernova and its link to Gamma-Ray Bursts|url=http://imagine.gsfc.nasa.gov/docs/science/know_l1/why_hyper.html|work=Imagine the Universe!|publisher=NASA|accessdate=9 December 2011|quote=With a power about 100 times that of the already astonishingly powerful "typical" supernova|archive-url=https://web.archive.org/web/20111019233153/http://imagine.gsfc.nasa.gov/docs/science/know_l1/why_hyper.html|archive-date=19 अक्तूबर 2011|url-status=live}}</ref>
|-
|rowspan=3 | 10<sup>47</sup>
|rowspan=3 | &nbsp;
|1.8×10<sup>47</sup> J || Theoretical total [[mass-energy]] of the [[Sun]]<ref>{{cite web |url= http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html |title= Sun Fact Sheet |publisher= NASA |accessdate= 15 October 2011 |archive-url= https://web.archive.org/web/20100715200549/http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html |archive-date= 15 जुलाई 2010 |url-status= live }}</ref><ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=30&num=2.0&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215025/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=30&num=2.0&From=kg&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
|5.4×10<sup>47</sup> J || [[Mass-energy]] emitted as [[gravitational waves]] during the merger of two [[black holes]], originally about 30 Solar masses each, as observed by [[LIGO]]<ref>{{Cite journal | last1 = Abbott | first1 = B. | last2 = Abbott | first2 = R. | display-authors=1 | title = Observation of Gravitational Waves from a Binary Black Hole Merger | journal = Physical Review Letters | doi = 10.1103/PhysRevLett.116.061102 | volume = 116 | issue = 6 | year = 2016|arxiv = 1602.03837 |bibcode = 2016PhRvL.116f1102A | pmid=26918975 | pages=061102}}</ref>
|-
|8.8×10<sup>47</sup> J || [[GRB 080916C]] - the most powerful Gamma-Ray Burst (GRB) ever recorded - total 'apparent'/isotropic (not corrected for beaming) energy output estimated at 8.8 × 10<sup>47</sup> joules (8.8 × 10<sup>54</sup> erg), or 4.9 times the sun’s mass turned to energy.<ref>{{cite web|url= http://www.astronomynow.com/090220fermisrecordbreakinggrb.html|title= Fermi’s record breaking gamma-ray burst|access-date= 14 अगस्त 2017|archive-url= https://web.archive.org/web/20171021094409/http://www.astronomynow.com/090220fermisrecordbreakinggrb.html|archive-date= 21 अक्तूबर 2017|url-status= dead}}</ref>
|-
| 10<sup>53</sup> || &nbsp; || 6x10<sup>53</sup> J || Total mechanical [[energy]] or [[enthalpy]] in the powerful [[Active galactic nucleus|AGN]] outburst in the RBS 797<ref>url= http://arxiv.org/abs/1103.0630 {{Webarchive|url=https://web.archive.org/web/20180617043512/https://arxiv.org/abs/1103.0630 |date=17 जून 2018 }}</ref>
|-
| 10<sup>54</sup> || &nbsp; || 3x10<sup>54</sup> J || Total mechanical [[energy]] or [[enthalpy]] in the powerful AGN outburst in the Hercules A (3C 348)<ref>url= http://iopscience.iop.org/1538-4357/625/1/L9/fulltext/19121.text.html</ref>
|-
| 10<sup>55</sup> || &nbsp; || 10<sup>55</sup> J || Total mechanical [[energy]] or [[enthalpy]] in the powerful AGN outburst in the [[MS 0735.6+7421]]
|-
| 10<sup>58</sup> || &nbsp; || 4×10<sup>58</sup> J || Visible [[mass-energy]] in our [[galaxy]], the [[Milky Way]]<ref>{{cite web |url=http://physics.uoregon.edu/~jimbrau/astr123/Notes/Chapter23.html#mass |title=The Milky Way Galaxy |author=[[James E. Brau|Jim Brau]] |accessdate=4 November 2011 |archive-url=https://web.archive.org/web/20130618201430/http://physics.uoregon.edu/~jimbrau/astr123/notes/chapter23.html#mass |archive-date=18 जून 2013 |url-status=live }}</ref><ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=41&num=4&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215020/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=41&num=4&From=kg&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
| 10<sup>59</sup> || &nbsp; || 1×10<sup>59</sup> J || Total [[mass-energy]] of our [[galaxy]], the [[Milky Way]], including [[dark matter]] and [[dark energy]]<ref name=Karachentsev2006>{{cite journal | last1 = Karachentsev | first1 = I. D. | last2 = Kashibadze | first2 = O. G. | year = 2006 | title = Masses of the local group and of the M81 group estimated from distortions in the local velocity field | url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006Ap.....49....3K | journal = Astrophysics | volume = 49 | issue = 1| pages = 3–18 | doi = 10.1007/s10511-006-0002-6 | bibcode=2006Ap.....49....3K}}</ref><ref>{{cite web|title=Conversion from kg to J|url=http://physics.nist.gov/cgi-bin/cuu/Convert?exp=42&num=1.2&From=kg&To=j&Action=Convert+value+and+show+factor|publisher=NIST|accessdate=4 November 2011|archive-url=https://web.archive.org/web/20140202215028/http://physics.nist.gov/cgi-bin/cuu/Convert?exp=42&num=1.2&From=kg&To=j&Action=Convert+value+and+show+factor|archive-date=2 फ़रवरी 2014|url-status=dead}}</ref>
|-
| 10<sup>62</sup> || &nbsp; || 1–2×10<sup>62</sup> J || Total [[mass-energy]] of the [[Virgo Supercluster]] including [[dark matter]], the [[Supercluster]] which contains the [[Milky Way]]<ref name="ein07">{{cite journal
| author  = Einasto, M.
| title   = The richest superclusters. I. Morphology
| journal = Astronomy and Astrophysics
| date    = December 2007
| volume  = 476
| issue   = 2
| pages   = 697–711
| bibcode     = 2007A&A...476..697E
| doi     = 10.1051/0004-6361:20078037
| display-authors  = 1
| last2  = Saar
| first2  = E.
| last3  = Liivamägi
| first3  = L. J.
| last4  = Einasto
| first4  = J.
| last5  = Tago
| first5  = E.
| last6  = Martínez
| first6  = V. J.
| last7  = Starck
| first7  = J.-L.
| last8  = Müller
| first8  = V.
| last9  = Heinämäki
| first9  = P.
|arxiv = 0706.1122 }}</ref>
|-
| 10<sup>69</sup> || &nbsp; || 4×10<sup>69</sup> J || Estimated total [[mass-energy]] of the [[observable universe]]<ref name="nasa">{{cite web|url=http://imagine.gsfc.nasa.gov/docs/ask_astro/answers/980211b.html |publisher=web.archive.org |title=Big Bang Energy |accessdate=26 December 2016 |deadurl=bot: unknown |archiveurl=https://web.archive.org/web/20140819120709/http://imagine.gsfc.nasa.gov/docs/ask_astro/answers/980211b.html |archivedate=19 August 2014 |df= }}</ref>
|-
|}


==इन्हें भी देखें==
*[[ऊर्जा]]

==टिप्पणी==
{{Reflist|30em}}


{{परिमाण की कोटि}}

[[श्रेणी:ऊर्जा]]