Orders of magnitude (power)
This page lists examples of the power in watts produced by various sources of energy. They are grouped by orders of magnitude from small to large.
Below 1 W
| Factor | SI prefix | Value | Value (decibel-milliwatts) | Item |
| 10−50 | 5.4 × 10−50 | −463 dBm | astro: Hawking radiation power of the ultramassive black hole TON 618. | |
| 10−27 | ronto- | 1.64 | −238 dBm | phys: approximate power of gravitational radiation emitted by a 1000 kg satellite in geosynchronous orbit around the Earth. |
| 10−24 | yocto- | 1 | −210 dBm | |
| 10−21 | 1 | −180 dBm | biomed: approximate lowest recorded power consumption of a deep-subsurface marine microbe | |
| 10−20 | 1 | −170 dBm | tech: approximate power of Galileo space probe's radio signal as received on earth by a 70-meter DSN antenna. | |
| 10−18 | atto- | 1 | −150 dBm | phys: approximate power scale at which operation of nanoelectromechanical systems are overwhelmed by thermal fluctuations. |
| 10−16 | 1 | −130 dBm | tech: the GPS signal strength measured at the surface of the Earth. | |
| 10−16 | 2 | −127 dBm | biomed: approximate theoretical minimum luminosity detectable by the human eye under perfect conditions | |
| 10−15 | femto- | 2.5 | −116 dBm | tech: minimum discernible signal at the antenna terminal of a good FM radio receiver |
| 10−14 | 1 | −110 dBm | tech: approximate lower limit of power reception on digital spread-spectrum cell phones | |
| 10−12 | pico- | 1 | −90 dBm | biomed: average power consumption of a human cell |
| 10−11 | 1.84 | −77 dBm | phys: power lost in the form of synchrotron radiation by a proton revolving in the Large Hadron Collider at 7000 GeV | |
| 10−11 | 2.9 | −72 dBm | astro: power per square meter received from Proxima Centauri, the closest star known | |
| 10−10 | 1 | −68 dBm | astro: estimated total Hawking radiation power of all black holes in the observable universe. | |
| 10−10 | 1.5 | −68 dBm | biomed: power entering a human eye from a 100-watt lamp 1 km away | |
| 10−9 | nano- | 2–15 | −57 dBm to −48 dBm | tech: power consumption of 8-bit PIC microcontroller chips when in "sleep" mode |
| 10−6 | micro- | 1 | −30 dBm | tech: approximate consumption of a quartz or mechanical wristwatch |
| 10−6 | micro- | 3 | −25 dBm | astro: cosmic microwave background radiation per square meter |
| 10−5 | 5 | −13 dBm | biomed: sound power incident on a human eardrum at the threshold intensity for pain. | |
| 10−3 | milli- | 1.55 | −4.7 dBm | astro: power per square meter received from the Sun by Sedna at its aphelion |
| 10−3 | milli- | 5 | 7 dBm | tech: laser in a CD-ROM drive |
| 10−3 | milli- | 5–10 | 7 dBm to 10 dBm | tech: laser in a DVD player |
| 10−2 | centi- | 7 | 18 dBm | tech: antenna power in a typical consumer wireless router |
| 10−1 | deci- | 1.2 | 21 dBm | astro: total proton decay power of Earth, assuming the half life of protons to take on the value 1035 years. |
| 10−1 | deci- | 5 | 27 dBm | tech: maximum allowed carrier output power of an FRS radio |
1 to 102 W
| Factor | SI prefix | Value | Item |
| 100 | W | 1 | tech: cellphone camera light |
| 100 | W | 1.508 | astro: power per square metre received from the Sun at Neptune's aphelion |
| 100 | W | 2 | tech: maximum allowed carrier power output of a MURS radio |
| 100 | W | 4 | tech: the power consumption of an incandescent night light |
| 100 | W | 4 | tech: maximum allowed carrier power output of a 10-meter CB radio |
| 100 | W | 7 | tech: the power consumption of a typical Light-emitting diode light bulb |
| 100 | W | 8 | tech: human-powered equipment using a hand crank. |
| 101 | deca- | 1.4 × 101 | tech: the power consumption of a typical household compact fluorescent light bulb |
| 101 | deca- | 2–4 × 101 | biomed: approximate power consumption of the human brain |
| 101 | deca- | 3–4 × 101 | tech: the power consumption of a typical household fluorescent tube light |
| 101 | deca- | 6 × 101 | tech: the power consumption of a typical household incandescent light bulb |
| 102 | hecto- | 1 × 102 | biomed: approximate basal metabolic rate of an adult human body |
| 102 | hecto- | 1.2 × 102 | tech: electric power output of solar panel in full sunlight, at sea level |
| 102 | hecto- | 1.3 × 102 | tech: peak power consumption of a Pentium 4 CPU |
| 102 | hecto- | 2 × 102 | tech: stationary bicycle average power output |
| 102 | hecto- | 2.76 × 102 | astro: fusion power output of 1 cubic meter of volume of the Sun's core. |
| 102 | hecto- | 2.9 × 102 | units: approximately 1000 BTU/hour |
| 102 | hecto- | 3 × 102 | tech: PC GPU Nvidia GeForce RTX 4080 peak power consumption |
| 102 | hecto- | 4 × 102 | tech: legal limit of power output of an amateur radio station in the United Kingdom |
| 102 | hecto- | 5 × 102 | biomed: power output of a person working hard physically |
| 102 | hecto- | units: 1 horsepower | |
| 102 | hecto- | 7.5 × 102 | astro: approximately the amount of sunlight falling on a square metre of the Earth's surface at noon on a clear day in March for northern temperate latitudes |
| 102 | hecto- | 9.09 × 102 | biomed: peak output power of a healthy human during a 30-second cycle sprint at 30.1 degree Celsius. |
103 to 108 W
The productive capacity of electrical generators operated by utility companies is often measured in MW. Few things can sustain the transfer or consumption of energy on this scale; some of these events or entities include: lightning strikes, naval craft, engineering hardware, and some scientific research equipment.For reference, about 10,000 100-watt lightbulbs or 5,000 computer systems would be needed to draw 1 MW. Also, 1 MW is approximately 1360 horsepower. Modern high-power diesel-electric locomotives typically have a peak power of 3–5 MW, while a typical modern nuclear power plant produces on the order of 500–2000 MW peak output.
109 to 1014 W
1015 to 1026 W
Over 1027 W
| 1030 | quetta- | 1.99 × 1030 W | astro: peak luminosity of the Sun in its thermally-pulsing, late AGB phase |
| 1030 | quetta- | 4.1 × 1030 W | astro: approximate luminosity of Canopus |
| 1031 | 2.53 × 1031 W | astro: approximate luminosity of the Beta Centauri triple star system | |
| 1031 | 3.3 × 1031 W | astro: approximate luminosity of Betelgeuse, a highly evolved red supergiant | |
| 1032 | 1.23 × 1032 W | astro: approximate luminosity of Deneb | |
| 1033 | 1.26 × 1033 W | astro: approximate luminosity of the Pistol Star, an LBV which emits in 10 seconds the Sun's annual energy output | |
| 1033 | 1.79 × 1033 W | astro: approximate luminosity of R136a1, a massive Wolf-Rayet star and the most luminous single star known | |
| 1033 | 2.1 × 1033 W | astro: approximate luminosity of the Eta Carinae system, a highly elliptical binary of two supergiant blue stars orbiting each other | |
| 1034 | 4 × 1034 W | tech: approximate power used by a type III civilization in the Kardashev scale. | |
| 1036 | 5.7 × 1036 W | astro: approximate luminosity of the Milky Way galaxy | |
| 1037 | 2 × 1037 W | astro: approximate luminosity of the Local Group, the volume enclosed by our gravitational cosmic horizon | |
| 1037 | 4 × 1037 W | astro: approximate internal luminosity of the Sun for a few seconds as it undergoes a helium flash. | |
| 1038 | 2.2 × 1038 W | astro: approximate luminosity of the extremely luminous supernova ASASSN-15lh | |
| 1039 | 1 × 1039 W | astro: average luminosity of a quasar | |
| 1039 | 1.57 × 1039 W | astro: approximate luminosity of 3C273, the brightest quasar seen from Earth | |
| 1040 | 5 × 1040 W | astro: approximate peak luminosity of the energetic fast blue optical transient CSS161010 | |
| 1041 | 1 × 1041 W | astro: approximate luminosity of the most luminous quasars in our universe, e.g., APM 08279+5255 and HS 1946+7658. | |
| 1042 | 1.7 × 1042 W | astro: approximate luminosity of the Laniakea Supercluster | |
| 1042 | 3 × 1042 W | astro: approximate luminosity of an average gamma-ray burst | |
| 1043 | 2.2 × 1043 W | astro: average stellar luminosity in one cubic gigalight-year of space | |
| 1045 | |||
| 1046 | 1 × 1046 W | astro: record for maximum beaming-corrected intrinsic luminosity ever achieved by a gamma-ray burst | |
| 1047 | 7.519 × 1047 W | phys: Hawking radiation luminosity of a Planck mass black hole | |
| 1048 | 9.5 × 1048 W | astro: luminosity of the entire Observable universe ≈ 24.6 billion trillion solar luminosity. | |
| 1049 | 3.6 × 1049 W | astro: peak gravitational wave radiative power of GW150914, the merger event of two distant stellar-mass black holes. It is attributed to the first observation of gravitational waves. | |
| 1052 | 3.63 × 1052 W | phys: the unit of power as expressed under the Planck units, at which the definition of power under modern conceptualizations of physics breaks down. Equivalent to one Planck mass-energy per Planck time. |