Orders of magnitude (density)
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Skylab measured several orders of magnitude of the Sun's density (top scale: 10−18 to 10−6 g⋅cm−3, equivalent to 10−15 to 10−3 kg⋅m−3) at different temperatures and heights above its surface.
| Factor | Multiple | Value | Item |
|---|---|---|---|
| 10−27 | 1 yg/m3 | 1 × 10−27 kg/m3 | Very approximate density of the universe |
| 10−26 | |||
| 10−25 | |||
| 10−24 | 1 zg/m3 | ||
| 10−23 | |||
| 10−22 | 100 zg/m3 | 1 × 10−22 kg/m3 | Probable lowest observed density of space in galactic spiral arm (1 hydrogen atom every 16 cubic centimeters) |
| 10−21 | 1 ag/m3 | ||
| 10−20 | |||
| 10−19 | |||
| 10−18 | 1 fg/m3 | 1 × 10−18 kg/m3 | Observed density of space in core of galaxy (600 hydrogen atoms in every cubic centimetre) |
| Best vacuum from a laboratory (1 pPa)[1] | |||
| 10−17 | |||
| 10−16 | |||
| 10−15 | 1 pg/m3 | ||
| 10−14 | 2.0 × 10−14 kg/m3 | (2.0 × 10−17 g/cm3) density of Sun's corona[2] | |
| 10−13 | 1.0 × 10−13 kg/m3 | (1.0 × 10−16 g/cm3) density at top of solar transition region[2] | |
| 10−12 | 1 ng/m3 | ||
| 10−11 | 1.0 × 10−11 kg/m3 | (1.0 × 10−14 g/cm3) density at bottom of solar transition region[2] | |
| 10−10 | |||
| 10−9 | 1 μg/m3 | ||
| 10−8 | |||
| 10−7 | |||
| 10−6 | 1 mg/m3 | ||
| 10−5 | 1.34 × 10−5 kg/m3 | Earth atmosphere at 82 kilometre altitude; star Mu Cephei's approximate mean density |
|
| 10−4 | 0.1 g/m3 | 1.09 × 10−4 kg/m3 | Earth atmosphere at 68 kilometre altitude; |
| 2.0 × 10−4 kg/m3 | (2.0 × 10−7 g⋅cm−3) Density of Solar photosphere–chromosphere boundary[2] | ||
| 4.0 × 10−4 kg/m3 | (4.0 × 10−7 g⋅cm−3) Density of Solar photosphere's lower boundary[2] | ||
| 10−3 | 1 g/m3 | 1 × 10−3 kg/m3 | Vacuum from a mechanical vacuum pump; density of Sun just below its photosphere[2] |
| 10−2 | 10 g/m3 | 1.8 × 10−2 kg/m3 | Earth atmosphere at 30 kilometre altitude[3] |
| 9 × 10−2 kg/m3 | Hydrogen gas, the least dense substance at STP | ||
| 10−1 | 100 g/m3 | 1.6 × 10−1 kg/m3 | Earth atmosphere at 16 kilometre altitude[3] |
| Factor | Multiple | Value | Item |
|---|---|---|---|
| 100 | 1 kg/m3 | 0.9 kg/m3 = 0.0009 g/cm3 | Ultralight metallic microlattice.[4] |
| 1.48 kg/m3 = 0.00148 g/cm3 | Earth atmosphere at sea level | ||
| 3 kg/m3 = 0.003 g/cm3 | Typical[citation needed] density of aerogel | ||
| 101 | |||
| 102 | 534 kg/m3 = 0.534 g/cm3 | Lithium at near room temperature | |
| 103 | 1 Mg/m3 1 t/m3 |
1000 kg/m3 = 1 g/cm3 | Liquid water at 4 °C |
| 1010 kg/m3 = 1.01 g/cm3 | Average human body | ||
| 1400 kg/m3 = 1.4 g/cm3 | Average density of Sun | ||
| 104 | 10000 kg/m3 | 10490 kg/m3 = 10.49 g/cm3 | Silver (Ag) |
| 11340 kg/m3 = 11.34 g/cm3 | Lead (Pb) | ||
| 13534 kg/m3 = 13.534 g/cm3 | Mercury (Hg) | ||
| 19100 kg/m3 = 19.1 g/cm3 | Uranium (U) | ||
| 19250 kg/m3 = 19.25 g/cm3 | Tungsten (W) | ||
| 19300 kg/m3 = 19.3 g/cm3 | Gold (Au) | ||
| 21450 kg/m3 = 21.45 g/cm3 | Platinum (Pt) | ||
| 22560 kg/m3 = 22.56 g/cm3[5] | Iridium (Ir) | ||
| 22590 kg/m3 = 22.59 g/cm3[5] | Osmium (Os), the densest known substance at STP | ||
| 105 | 150,000 kg/m3 = 150 g/cm3 | Core of the Sun | |
| 106 | 1 Gg/m3 | ||
| 107 | |||
| 108 | |||
| 109 | 1 Tg/m3 | White dwarf | |
| 1010 | |||
| 1011 | |||
| 1012 | 1 Pg/m3 | ||
| 1013 | 2 × 1013 kg/m3 | Universe at end of electroweak epoch (approximately) | |
| 1014 | |||
| 1015 | 1 Eg/m3 | ||
| 1016 | |||
| 1017 | 2 × 1017 kg/m3 | Atomic nuclei and neutron stars | |
| 1018 | 1 Zg/m3 | ||
| 1019 | |||
| 1020 | |||
| 1021 | 1 Yg/m3 | ||
| 1022 | |||
| 1023 | 1023 kg/m3 | Density of a hypothetical preon star | |
| ... | ... | ... | ... |
| 1096 | 5.1 × 1096 kg/m3 | Planck density | |
| ∞ | ∞ kg/m3 | Density of a black hole at singularity |
[edit] Notes
- ^ http://dx.doi.org/10.1016/0042-207X(93)90084-N
- ^ a b c d e f "SP-402 A New Sun: The Solar Results From Skylab". http://history.nasa.gov/SP-402/p2.htm.
- ^ a b "AtmosModeler Simulator - Version 1.2a". NASA. http://www.grc.nasa.gov/WWW/K-12/airplane/atmosi.html. Retrieved 22 January 2012.
- ^ "Ultralight Metallic Microlattices". http://www.sciencemag.org/content/334/6058/962.
- ^ a b Arblaster, J. W. (1989). "Densities of osmium and iridium: recalculations based upon a review of the latest crystallographic data" (PDF). Platinum Metals Review 33 (1): 15. http://www.platinummetalsreview.com/pdf/pmr-v33-i1-014-016.pdf. "at 20°C"
[edit] External links
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