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To help compare different orders of magnitude, the following lists describe various levels between 10−67 and 1052 kg. The least massive thing listed here is a , and the most massive thing is the observable universe. Typically, an object having greater mass will also have greater weight (see mass versus weight), especially if the objects are subject to the same gravitational field strength.


Units of mass

The table at right is based on the (kg), the base unit of mass in the International System of Units (SI). The kilogram is the only standard unit to include an ( kilo-) as part of its name. The (10−3 kg) is an SI derived unit of mass. However, the names of all SI mass units are based on gram, rather than on kilogram; thus 103 kg is a megagram (106 g), not a * kilokilogram.

The (t) is an SI-compatible unit of mass equal to a megagram ( Mg), or 103 kg. The unit is in common use for masses above about 103 kg and is often used with SI prefixes. For example, a gigagram ( Gg) or 109 g is 103 tonnes, commonly called a kilotonne.


Other units
Other units of mass are also in use. Historical units include the stone, the pound, the carat, and the grain.

For subatomic particles, physicists use the mass-equivalent of an (eV). At the atomic level, chemists use the mass of one-twelfth of a carbon-12 atom (the dalton). Astronomers use the ().


The least massive things: below 10−24 kg
Unlike other physical quantities, mass–energy does not have an a priori expected minimal quantity, or an observed basic quantum as in the case of electric charge. Planck's law allows for the existence of with arbitrarily low energies. Consequently, there can only ever be an experimental upper bound on the mass of a supposedly massless particle; in the case of the photon, this confirmed upper bound is of the order of = .

!Factor () !Value !Item

10−671.07 kg, upper bound (6 eV/ c2)
10−404.2 kgMass equivalent of the energy of a at the peak of the spectrum of the cosmic microwave background radiation (0.235 meV/ c2)
10−361.8 kg1 eV/ c2, the mass equivalent of one
3.6 kg, upper limit on mass (2 eV/ c2) "The most sensitive analysis on the neutrino mass ... is compatible with a neutrino mass of zero. Considering its uncertainties this value corresponds to an upper limit on the electron neutrino mass of m<2.2 eV/c2 (95% Confidence Level)" The Mainz Neutrino Mass Experiment
10−33
quectogram (qg)
10−319.11 kg (511 keV/ c2), the lightest elementary particle with a measured nonzero
10−30
rontogram (rg)
3.0–5.5 kg (as a current quark) (1.7–3.1 MeV/ c2)
10−281.9 kg (106 MeV/ c2)
10−27
yoctogram (yg)
1.661 kgDalton (Da), a.k.a. unified atomic mass unit (u)
1.673 kg (938.3 MeV/ c2)
1.674 kg atom, the lightest atom
1.675 kg (939.6 MeV/ c2)
10−261.2 kg atom (6.941 Da)
3.0 kg (18.015 Da)
8.0 kg atom (47.867 Da)
10−251.1 kg atom (63.546 Da)
1.6 kgZ boson (91.2 GeV/ c2)
2.2 kg (125 GeV/ c2)
3.1 kg (173 GeV/ c2), the heaviest known elementary particle
3.2 kg molecule (194 Da)
3.5 kg-208 atom
4.9 kg-294 atom, the heaviest known


10−24 to 10−18 kg
10−24
zeptogram (zg)
1.2 kgBuckyball molecule (720 Da)
10−231.4 kg, a small ubiquitous protein (8.6 kDa)
5.5 kgA typical (median size of roughly 300 ≈ 33 kDa)
10−221.1 kg molecule in blood (64.5 kDa)
10−21
attogram (ag)
1.65 kgDouble-stranded molecule consisting of 1,578 (995 kDa)From attograms to Daltons: Cornell NEMS device detects the mass of a single DNA molecule [2]. Retrieved 2010-10-14
4.3 kgProkaryotic (2.6 MDa)
7.1 kgEukaryotic (4.3 MDa)
7.6 kgBrome mosaic virus, a small (4.6 MDa)
10−203 kg in rats (16.1 ± 3.8 MDa)
6.8 kgTobacco mosaic virus (41 MDa)
10−191.1 kgNuclear pore complex in yeast (66 MDa)
2.5 kgHuman (150 MDa)


10−18 to 10−12 kg
10−18
femtogram (fg)
1 kg virusCalculated : volume = 4/3 × π × (126e−9 m / 2)3 = 1.05e−21 m3. Assume density = 1 g/cm3 => mass = 1.05e−21 m3 × 1e3 kg/m3 = 1.05e−18 kg
4.7 kg sequence of length 4.6 Mbp, the weight of the genome
10−17~1 kg virus, a large virus
1.1 kgMass equivalent of 1
10−163 kg cyanobacteria, the smallest (and possibly most plentiful) photosynthetic organism on Earth
10−15
picogram (pg)
1 kg bacterium (wet weight)
6 kg in a typical human cell (approximate)
10−142.2 kgHuman cellM. R. Curry, J. D. Millar, S. M. Tamuli & P. F. Watson, "," Biology of Reproduction, 55, 6 (1996‑12‑01): 1325–32.
6 kg cell (quite variable)
10−131.5 kgDunaliella salina, a (dry weight)


10−12 to 10−6 kg
10−12
 (ng)
1 kgAverage human cell (1 nanogram)
2–3 kg human cell
8 kgGrain of "the total pollen grain mass of approximately 7.85 ng"
10−11  
10−102.5 kgGrain of "The dry weight of individual pollen grains has been estimated at 250 ng"
3.5 kgVery fine grain of (0.063 mm diameter, 350 nanograms)
10−9
 (μg)
3.6 kgHuman Mass calculated from volume assuming density of 1 g/mL
2.4 kgUS RDA for vitamin B12 for adults
10−8 Speculated approximate lower limit of the mass of a primordial black hole
US RDA for for adults
~2 kgUncertainty in the mass of the International Prototype of the Kilogram (IPK) (±~20μg)Report to the CGPM, 14th meeting of the Consultative Committee for Units (CCU), April 2001, 2. (ii); General Conference on Weights and Measures, 22nd Meeting, October 2003, which stated "The kilogram is in need of a new definition because the mass of the prototype is known to vary by several parts in 108 over periods of time of the order of a month ..." ( 3.2MB ZIP file, here).
2.2 kg, can be expressed as the mass of a 2 Planck Length radius black hole
~7 kgOne eyelash hair (approximate)
10−71.5 kgUS RDA for for adults
2–3 kgFruit fly (dry weight)


10−6 to 1 kg
10−6
 (mg)
2.5 kg, common smaller species (about 2.5 milligrams), grain of salt or sand, medicines are typically expressed in milligrams
10−5
 (cg)
1.1 kgSmall granule of quartz (2 mm diameter, 11 milligrams)Quartz has a density of 2.65. Mass = Volume × Density = (4/3 × π × (1e−3 m)3) × (2.65 × 1e3 kg/m3) = 1.1e−5 kg.
2 kgAdult ( Musca domestica, 21.4 milligrams)
10−4
 (dg)
0.27–2.0 kgRange of amounts of in one cup of (27–200 milligrams)
1.5 kgA frame of 35mm motion picture film (157 milligrams)
2 kgMetric carat (200 milligrams)
10−3
 (g)
1 kgOne of water (1 gram)
1 kgUS dollar bill (1 gram)
~1 kgTwo (approximately 1 gram)
~8 kgCoins of one (7.5 grams), one U.S. dollar (8.1 grams) and one Canadian (7 grams pre-2012, 6.27 grams 2012-)
10−2
decagram (dag)
1.2 kgMass of one mole (6.02214 atoms) of carbon-12 (12 grams)
1.37 kgAmount of defined as one in the U.S. (13.7 grams)
2–4 kgAdult mouse ( , 20–40 grams)
2.8 kg () (28.3495 grams)
4.7 kgMass equivalent of the energy that is 1 megaton of Calculated: 1e6 tons of TNT-equivalent × 4.184e9 J/ton of TNT-equivalent × 1.1e−17 kg of mass-equivalent/J = 4.7e−2 kg of mass-equivalent
10−1
hectogram   (hg)
0.1-0.2 kgAn (100–200 grams)
0.142-0.149 kgA baseball used in the major league.Christina Lee, "Mass of a Baseball", The Physics Factbook, 1999. Retrieved 2018-07-04
0.454 kgPound () (453.6 grams)


1 kg to 105 kg
1 kg
 (kg)
1 kgOne (0.001 m3) of water
1–3 kgSmallest breed of dog (Chihuahua)
1–3 kgTypical computer, 2010
1–3 kgAdult domestic
2.5–4 kgNewborn human
4.0 kgWomen's
4–5 kg
7.26 kgMen's
1019–27 kgMedium-sized
10–30 kgA computer or set
50 kgLarge dog breed ()
70 kg
102130–180 kgMature , female (130 kg) and male (180 kg)
(1996). 9782831700458, IUCN/SSC Cat Specialist Group.
200–250 kg
240–450 kgGrand Calculated: 540 lbs × 0.4536 kg/lb = 240 kg. 990 lb × 0.4536 kg/lb = 450 kg.
400–900 kg
500–500,000 kgA teaspoon (5 ml) of material (0.5–500 tonnes)Using the quoted density of 1e5 to 1e8 kg/m3 for white dwarf material, 1 teaspoon = 5mL = 5e−3 m3 has a calculated mass of: Low end: 5e−3 m3 × 1e5 kg/m3 = 5e2 kg High end: 5e−3 m3 × 1e8 kg/m3 = 5e5 kg
635 kgHeaviest human in recorded history (Jon Brower Minnoch)
907.2 kg1 (2000 pounds - U.S.)
103
 (Mg)
1000 kg1 (U.S. spelling: metric ton)
1000 kg1 of water
1016.05 kg (British) / 1 (2240 pounds - U.S.)
1300–1600 kgTypical passenger
2700–6000 kgAdult
(1994). 9780856610882, T & A D Poyser.
1041.1 kgHubble Space Telescope (11 tonnes)
1.2 kgLargest on record (12 tonnes)
1.4 kg (bell) (14 tonnes)
2.7 kg computer, 1946 (30 tonnes)
4 kgMaximum gross mass (truck + load combined) of a semi-trailer truck in the (40–44 tonnes)
5–6 kg; (50–60 tonnes)
6.0 kgLargest single-piece , Hoba West Meteorite (60 tonnes)
7.3 kgLargest dinosaur, (73 tonnes)
1051.74-1.83 kgOperational empty weight of a Boeing 747-300
1.8 kgLargest animal ever, a (180 tonnes)
4.2 kgInternational Space Station (417 tonnes)
6 kgWorld's heaviest aircraft: Antonov An-225 (maximum take-off mass: 600 tonnes, payload: 250 tonnes)


106 to 1011 kg
106
 (Gg)
1 kgTrunk of the giant sequoia tree named General Sherman, largest living tree by trunk volume (1121 tonnes)
2.0 kgLaunch mass of the (2041 tonnes)
6 kgLargest , the named Pando (largest living organism) (6000 tonnes)
7.8 kgVirginia-class nuclear submarine (submerged weight)
1071 kgAnnual production of
5.2 kg when fully loaded (52,000 tonnes)
9.97 kgHeaviest train ever: Australia's BHP Iron Ore, 2001 record (99,700 tonnes)
1086.6 kgLargest ship and largest mobile man-made object, , when fully loaded (660,000 tonnes)
7 kgHeaviest (non-pyramid) building, Palace of the Parliament in Bucharest, Romania
109
 (Tg)
4.3 kgAmount of matter converted into energy by the each second
6 kgGreat Pyramid of Giza
(2025). 9781404260597, Rosen Publishing Group.
1010
6 kgAmount of in the Three Gorges Dam, the world's largest concrete structure
1011~1 kgThe mass of a primordial black hole with an evaporation time equal to the age of the universe
2 kgAmount of water stored in London storage reservoirs (0.2 km3)
6 kgTotal mass of the world's human population
5 kgTotal biomass of , one of the most plentiful animal species on the planet in terms of
(1997). 9789251040126, Food and Agriculture Organization. .


1012 to 1017 kg
1012
petagram (Pg)
0.8–2.1 kgGlobal biomass of
4 kgGlobal annual human food production
4 kgWorld crude production in 2009 (3,843 Mt)
5.5 kgA teaspoon (5 ml) of material (5000 million tonnes)The average density of material in a neutron star of radius 10 km is . Therefore, 5 ml of such material is , or 5 500 000 000 t. This is about 15 times the total mass of the human world population. Alternatively, 5 ml from a neutron star of radius 20 km radius (average density ) has a mass of about 400 Mt, or about the mass of all humans.
10131 kgMass of comet 67P/Churyumov–Gerasimenko
4 kgGlobal annual human carbon dioxide emission
10141.05 kgGlobal net primary production – the total mass of carbon fixed in organic compounds by photosynthesis each year on Earth
7.2 kgTotal carbon stored in Earth's atmosphere
1015
exagram (Eg)
2.0 kgTotal carbon stored in the terrestrial
3.5 kgTotal carbon stored in deposits worldwide
10161 kg951 Gaspra, the first asteroid ever to be closely approached by a spacecraft (rough estimate)
2.9–3.7 kgThe
4 kg
10221.3 kg
2.1 kgTriton, largest moon of Neptune
7.3 kgEarth's
10231.3 kgTitan, largest moon of Saturn
1.5 kgGanymede, largest moon of Jupiter
3.3 kgMercury
6.4 kg


1024 to 1029 kg
1024
ronnagram (Rg)
4.9 kg
6.0 kg
10253 kg
8.7 kg
10261.0 kg
5.7 kg
1027
quettagram (Qg)
1.9 kg
10282–14 kg (approximate)
10293 kgBarnard's Star, a nearby


1030 to 1035 kg
10302 kgThe (one or = 1.989 kg)
2.8 kgChandrasekhar limit ()p. 55, How A Supernova Explodes, Hans A. Bethe and Gerald Brown, pp. 51–62 in Formation And Evolution of Black Holes in the Galaxy: Selected Papers with Commentary, Hans Albrecht Bethe, Gerald Edward Brown, and Chang-Hwan Lee, River Edge, NJ: World Scientific: 2003. .
10314 kg, a red star ()Kaler, Jim. "Betelgeuse" (2008). Stars. University of Illinois. Retrieved on 2009-02-08.
10324–7 kgR136a1, the most massive of known stars (230 to 345 )
6–8 kgHyades star cluster (300 to 400 ) The Astrophysics Spectator: Open Star Clusters. Retrieved 2008-09-15
10331.6 kg star cluster ()
1034
1035~1035 kgTypical in the (overall range: 3 to 4 )
2 kgLow end of mass range for giant (1 to 1 )
7.3 kg of a giant at 100  and density 30 atoms per cubic centimeter;
possible example: Orion molecular cloud complex


1036 to 1041 kg
10361.79 kgThe entire .
2.4 kgThe of stars, including the Sun ()
7–8 kgThe supermassive black hole at the center of the Milky Way, associated with the radio source Sagittarius A* ()
8 kg, the largest globular cluster in the Milky Way, containing approximately 10 million stars.
1037  
1038  
1039  
1040  
10411.98 kg, the largest supermassive black hole, weighing 100 billion ()
4 kgVisible mass of the Milky Way galaxy


The most massive things: 1042 kg and greater
10421.2 kgMilky Way galaxy ()
2–3 kg of galaxies, including the Milky Way ()
10435.37 kg Https://arxiv.org/pdf/2208.08843.pdf< /ref>
1044  
10451–2 kgLocal or Virgo Supercluster of galaxies, including the Local Group ()
1046  
10472 kgLaniakea Supercluster of galaxies, which encompasses the Virgo supercluster
10482 kgPisces–Cetus Supercluster Complex, a that includes the Laniakea Supercluster.
10494 kgHercules–Corona Borealis Great Wall, the largest structure in the known universe
1050  
1051  
10524.4506 kgMass of the observable universe as estimated by

1.4 kgMass of the observable universe as estimated by the U.S. National Solar Observatory


See also
  • Lists of astronomical objects


Notes

External links

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