Orders of magnitude (time)
In the context of time, an order of magnitude is a description of the quantity of a time in respect to comparison between differing magnitudes. In common usage, the scale is usually the base10 or base−10 exponent being applied to an amount, making the order of magnitude 10 times greater or smaller.[1] As the differences are measured in factors of 10, a logarithmic scale is applied. In terms of time, the relationship between the smallest limit of time, the Planck time, and the next order of magnitude larger is 10.
Low order of magnitude - measures by the unit second (s)
Unit (s) | Multiple | Symbol | Definition | Comparative examples & common units | |
---|---|---|---|---|---|
10−44 | 1 Planck time | tP | The time required to travel one Planck length at the speed of light (c) | ys = 10−20 s: One 10−44Planck time tP = ≈ ×10−44 s 5.4[2] is the briefest physically meaningful span of time. It is the unit of time in the natural units system known as Planck units. | |
10−24 | 1 yoctosecond | ys[3] | Yoctosecond, (yocto- + second), is one septillionth of a second | 0.3 ys: mean life of the W and Z bosons.[4][5][lower-alpha 1] 0.5 ys: time for top quark decay, according to the Standard Model. 2 ys: time taken for a quark to emit a gluon. 23 ys: half-life of 7H. | |
10−21 | 1 zeptosecond | zs | Zeptosecond, (zepto- + second), is one sextillionth of one second | 7 zs: half-life of helium-9's outer neutron in the second nuclear halo. 17 zs: approximate period of electromagnetic radiation at the boundary between gamma rays and X-rays. 300 zs: approximate typical cycle time of X-rays, on the boundary between hard and soft X-rays. 500 zs: current resolution of tools used to measure speed of chemical bonding[6] 850 zs:The time it takes the electron to change its quantum state from the very constricted, bound state around the atom to a free state,[7] which is currently the quickest time ever observed. | |
10−18 | 1 attosecond | as | One quintillionth of one second | 12 attoseconds: best timing control of laser pulses.[8] | |
10−15 | 1 femtosecond | fs | One quadrillionth of one second | 1 fs: Cycle time for 300 nanometre light; ultraviolet light; light travels 0.3 micrometres (µm). 140 fs: Electrons have localized onto individual bromine atoms 6Å apart after laser dissociation of Br2.[9] | |
10−12 | 1 picosecond | ps | One trillionth of one second | 1 ps: half-life of a bottom quark; light travels 0.3 millimeters (mm) 1 ps: lifetime of a transition state 4 ps: Time to execute one machine cycle by an IBM Silicon-Germanium transistor | |
10−9 | 1 nanosecond | ns | One billionth of one second | 1 ns: Time to execute one machine cycle by a 1 GHz microprocessor 1 ns: Light travels 30 centimetres (12 in) | |
10−6 | 1 microsecond | µs | One millionth of one second | 1 µs: Time to execute one machine cycle by an Intel 80186 microprocessor 4–16 µs: Time to execute one machine cycle by a 1960s minicomputer | |
10−3 | 1 millisecond | ms | One thousandth of one second | 1 ms: time for a neuron in human brain to fire one impulse and return to rest[10] 4–8 ms: typical seek time for a computer hard disk | |
10−2 | 1
centisecond |
cs | One hundredth of one second | 18–300 ms (=0.02–0.3 s): Human reflex response to visual stimuli
20 ms: cycle time for European 50 Hz AC electricity | |
10−1 | 1
decisecond |
ds | One tenth of a second | 100–400 ms (=0.1–0.4 s): Blink of an eye[11] 150 ms: recommended maximum time delay for telephone service 185 ms: the duration of a full rotation of the main rotor on Bell 205, 212 and 412 helicopters (normal rotor speed is 324 RPM) | |
100 | 1 second | s | The duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the caesium 133 atom. | 1 s: 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the cesium-133 atom.[12]
6 s: time it takes for a human to breathe | |
101 | 1 decasecond | das | Ten seconds | 19.54 s: Half-life of Carbon-10
40 s: Time until cyanide starts acting 60 s: 1 minute | |
102 | 1 hectosecond | hs | One hundred seconds | 494 s: Time it takes for light to reach the sun
600 s: Half-life of Neutronium | |
103 | 1 kilosecond (16.7 minutes) |
ks | One thousand seconds | 3.6 ks: 3600 s or 1 hour 86.4 ks: 86 400 s or 1 day 604.8 ks: 1 week |
103 s, 104 s, 105 s |
106 | 1 megasecond (11.6 days) |
Ms | One million seconds |
2.6 Ms: approximately 1 month | |
109 | 1 gigasecond (32 years) |
Gs | One billion seconds |
2.1 Gs: average human life expectancy at birth (2011 estimate)[13] | |
1012 | 1 terasecond (32,000 years) |
Ts | One trillion seconds |
6 Ts: Time since the appearance of Homo sapiens (approximately) | |
1015 | 1 petasecond (32,000,000 years) |
Ps | One quadrillion seconds | 2.1 Ps: (66 million years) Time elapsed since the Cretaceous–Paleogene extinction event, during which all non-avian dinosaurs became extinct.[16] 7.1–7.9 Ps: 1 galactic year (225-250 million years)[17] | |
1018 | 1 exasecond (32,000,000,000 years) |
Es | One quintillion seconds | 312 Es: Estimated lifespan of a 0.1 solar mass red dwarf star. | |
1021 | 1 zettasecond (32,000,000,000,000 years) |
Zs | One sextillion seconds | 3 Zs: Estimated duration of Stelliferous Era. | |
1024 | 1 yottasecond (32,000,000,000,000,000 years) |
Ys | One septillion seconds | 1.6416 Ys: Estimated half-life of the meta-stable 209 83Bi radioactive isotope. 6.616×1050 Ys: Time required for a 1 solar mass black hole to evaporate completely due to Hawking radiation, if nothing more falls in. |
See also
- Heat death of the Universe
- Second law of thermodynamics
- Big Rip
- Big Crunch
- Big Bounce
- Big Bang
- Cyclic model
- Dyson's eternal intelligence
- Final anthropic principle
- Ultimate fate of the Universe
- Timeline of the Big Bang
- Timeline of the far future
- Graphical timeline of the Big Bang
- Graphical timeline from Big Bang to Heat Death. This timeline uses the loglog scale for comparison with the graphical timeline included in this article.
- Graphical timeline of the universe. This timeline uses the more intuitive linear time, for comparison with this article.
- Graphical timeline of the Stelliferous Era
- The Last Question, a short story by Isaac Asimov which considers the inevitable outcome of heat death in the universe and how it may be reversed.
- Orders of magnitude (frequency)
- Annum
- Geologic timescale
- Logarithmic timeline
- Natural history
- Physical unit
- Planck units
- Second
- SI unit
- Temporal resolution
- Timeline of evolution
- Timeline of the Big Bang
- Terasecond and longer
Footnotes
- Notes
- ↑ PDG reports the resonance width (Γ). Here the conversion τ = ħ⁄Γ is given instead.
- References
- ↑ Brians, Paus. "Orders of Magnitude" (8/4/2013)
- ↑ "CODATA Value: Planck time". The NIST Reference on Constants, Units, and Uncertainty. NIST. Retrieved October 1, 2011.
- ↑ The American Heritage Dictionary of the English Language: Fourth Edition. 2000. Available at: http://www.bartleby.com/61/21/Y0022100.html. Accessed December 19, 2007. note: abbr. ys or ysec
- ↑ C. Amsler et al. (2009): Particle listings – W boson
- ↑ C. Amsler et al. (2009): Particle listings – Z boson
- ↑ esciencenews (2010)
- ↑ http://www.sciencealert.com/scientists-measure-the-smallest-fragment-of-time-ever-witness-an-electron-escaping-an-atom
- ↑ "12 attoseconds is the world record for shortest controllable time".
- ↑ Li, Wen; et al. (November 23, 2010). "Visualizing electron rearrangement in space and timeduring the transition from a molecule to atoms". PNAS. 107 (47): 20219–20222. PMC 2996685 . PMID 21059945. doi:10.1073/pnas.1014723107. Retrieved 12 July 2015.
- ↑ http://www.noteaccess.com/APPROACHES/ArtEd/ChildDev/1cNeurons.htm
- ↑ Eric H. Chudler. "Brain Facts and Figures: Sensory Apparatus: Vision". Retrieved October 10, 2011.
- ↑ http://tycho.usno.navy.mil/leapsec.html
- ↑ CIA - The World Factbook -- Rank Order - Life expectancy at birth
- ↑ Ribas, I.; et al. (2005). "First Determination of the Distance and Fundamental Properties of an Eclipsing Binary in the Andromeda Galaxy". Astrophysical Journal Letters. 635 (1): L37–L40. Bibcode:2005ApJ...635L..37R. arXiv:astro-ph/0511045 . doi:10.1086/499161.
- ↑ Patterson N, Richter DJ, Gnerre S, Lander ES, Reich D (June 2006). "Genetic evidence for complex speciation of humans and chimpanzees". Nature. 441 (7097): 1103–8. PMID 16710306. doi:10.1038/nature04789.
- ↑ Renne, Paul R.; Deino, Alan L.; Hilgen, Frederik J.; Kuiper, Klaudia F.; Mark, Darren F.; Mitchell, William S.; Morgan, Leah E.; Mundil, Roland; Smit, Jan (7 February 2013). "Time Scales of Critical Events Around the Cretaceous-Paleogene Boundary". Science. 339 (6120): 684–687. Bibcode:2013Sci...339..684R. PMID 23393261. doi:10.1126/science.1230492.
- ↑ Leong, Stacy (2002). "Period of the Sun's Orbit around the Galaxy (Cosmic Year)". The Physics Factbook.
- ↑ "Age of the Earth". U.S. Geological Survey. 1997. Retrieved January 10, 2006.
- ↑ Dalrymple, G. Brent (2001). "The age of the Earth in the twentieth century: a problem (mostly) solved". Special Publications, Geological Society of London. 190 (1): 205–221. Bibcode:2001GSLSP.190..205D. doi:10.1144/GSL.SP.2001.190.01.14.
- ↑ Manhesa, Gérard; Allègrea, Claude J.; Dupréa, Bernard & Hamelin, Bruno (1980). "Lead isotope study of basic-ultrabasic layered complexes: Speculations about the age of the earth and primitive mantle characteristics". Earth and Planetary Science Letters. 47 (3): 370–382. Bibcode:1980E&PSL..47..370M. doi:10.1016/0012-821X(80)90024-2.
- ↑ Bouvier, Audrey and Meenakshi Wadhwa, "The age of the solar system redefined by the oldest Pb-Pb age of a meteoritic inclusion". Nature Geoscience, Nature Publishing Group, a division of Macmillan Publishers Limited. Published online August 22, 2010, retrieved August 26, 2010, doi:10.1038/NGEO941.
- ↑ Bonanno, A.; Schlattl, H.; Paternò, L. (2008). "The age of the Sun and the relativistic corrections in the EOS". Astronomy and Astrophysics. 390 (3): 1115–1118. Bibcode:2002A&A...390.1115B. arXiv:astro-ph/0204331 . doi:10.1051/0004-6361:20020749.
External links
- Exploring Time from Planck time to the lifespan of the universe