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Jurin's law

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(Redirected fromCapillary rise)
Analysis of capillary action
Capillary rise or fall in a tube.

Jurin's law, orcapillary rise, is the simplest analysis ofcapillary action—the induced motion of liquids in small channels[1]—and states that the maximum height of a liquid in a capillary tube isinversely proportional to the tube'sdiameter. Capillary action is one of the most common fluid mechanical effects explored in the field ofmicrofluidics. Jurin's law is named afterJames Jurin, who discovered it between 1718 and 1719.[2] His quantitative law suggests that the maximum height of liquid in a capillary tube is inversely proportional to the tube's diameter. The difference in height between the surroundings of the tube and the inside, as well as the shape of themeniscus, are caused bycapillary action. The mathematical expression of this law can be derived directly fromhydrostatic principles and theYoung–Laplace equation. Jurin's law allows the measurement of thesurface tension of a liquid and can be used to derive thecapillary length.[3]

Formulation

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The law is expressed as[citation needed]

h=2γcosθρgr0{\displaystyle \qquad h={\frac {2\gamma \cos \theta }{\rho gr_{0}}}},

where

It is only valid if the tube is cylindrical and has a radius (r0) smaller than thecapillary length (λc2=γ/(ρg){\displaystyle \lambda _{\rm {c}}^{2}=\gamma /(\rho g)}). In terms of the capillary length, the law can be written as

λc2=hr02cosθ{\displaystyle \lambda _{\rm {c}}^{2}={\frac {hr_{0}}{2\cos \theta }}}.

Examples

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Water height in a capillary tube plotted against diameter.
Main article:Capillary action

For a water-filled glass tube in air atstandard conditions for temperature and pressure,γ = 0.0728 N/m at 20 °C,ρ = 1000 kg/m3, andg = 9.81 m/s2. Because waterspreads on clean glass, the effective equilibrium contact angle is approximately zero.[4] For these values, the height of the water column is

h1.48×105r0 m.{\displaystyle h\approx {{1.48\times 10^{-5}} \over r_{0}}\ {\mbox{m}}.}

Thus for a 2 m (6.6 ft) radius glass tube in lab conditions given above, the water would rise an unnoticeable 0.007 mm (0.00028 in). However, for a 2 cm (0.79 in) radius tube, the water would rise 0.7 mm (0.028 in), and for a 0.2 mm (0.0079 in) radius tube, the water would rise 70 mm (2.8 in).

Capillary action is used by many plants to bring up water from the soil. For tall trees (larger than ~10 m (32 ft)), other processes likeosmotic pressure andnegative pressures are also important.[5]


History

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During the 15th century,Leonardo da Vinci was one of the first to propose thatmountain streams could result from the rise of water through small capillary cracks.[3][6]

It is later, in the 17th century, that the theories about the origin of capillary action begin to appear.Jacques Rohault erroneously supposed that the rise of the liquid in a capillary could be due to the suppression of air inside and the creation of a vacuum. The astronomerGeminiano Montanari was one of the first to compare the capillary action to the circulation ofsap in plants. Additionally, the experiments ofGiovanni Alfonso Borelli determined in 1670 that the height of the rise was inversely proportional to the radius of the tube.

Francis Hauksbee, in 1713, refuted the theory of Rohault through a series of experiments on capillary action, a phenomenon that was observable in air as well as in vacuum. Hauksbee also demonstrated that the liquid rise appeared on different geometries (not only circular cross sections), and on different liquids and tube materials, and showed that there was no dependence on the thickness of the tube walls.Isaac Newton reported the experiments of Hauskbee in his workOpticks but without attribution.[3][6]

It was the English physiologistJames Jurin, who finally in 1718[2] confirmed the experiments of Borelli and the law was named in his honour.[3][6]

Derivation

[edit]
Scheme showing the relevant variables to the problem for a positive height.

The heighth{\displaystyle h} of the liquid column in the tube is constrained by thehydrostatic pressure and by thesurface tension. The following derivation is for a liquid that rises in the tube; for the opposite case when the liquid is below the reference level, the derivation is analogous but pressure differences may change sign.[1]

Laplace pressure

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Above the interface between the liquid and the surface, the pressure is equal to the atmospheric pressurepatm{\displaystyle p_{\rm {atm}}}. At the meniscus interface, due to the surface tension, there is a pressure difference ofΔp=patmpint{\displaystyle \Delta p=p_{\rm {atm}}-p_{\rm {int}}}, wherepint{\displaystyle p_{\rm {int}}} is the pressure on the convex side; andΔp{\displaystyle \Delta p} is known asLaplace pressure. If the tube has a circular section of radiusr0{\displaystyle r_{0}}, and the meniscus has a spherical shape, the radius of curvature isr=r0/cosθ{\displaystyle r=r_{0}/\cos \theta }, whereθ{\displaystyle \theta } is thecontact angle. The Laplace pressure is then calculated according to theYoung-Laplace equation:Δp=2γr,{\displaystyle \Delta p={\frac {2\gamma }{r}},}whereγ{\displaystyle \gamma } is the surface tension.

Hydrostatic pressure

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Outside and far from the tube, the liquid reaches a ground level in contact with the atmosphere. Liquids incommunicating vessels have the same pressures at the same heights, so a pointw{\displaystyle {\rm {w}}}, inside the tube, at the same liquid level as outside, would have the same pressurepw=patm{\displaystyle p_{\rm {w}}=p_{\rm {atm}}}. Yet the pressure at this point follows avertical pressure variation as

pw=pint+ρgh,{\displaystyle p_{\rm {w}}=p_{\rm {int}}+\rho gh,}

whereg{\displaystyle g} is thegravitational acceleration andρ{\displaystyle \rho } the density of the liquid. This equation means that the pressure at pointw{\displaystyle {\rm {w}}} is the pressure at the interface plus the pressure due to the weight of the liquid column of heighth{\displaystyle h}. In this way, we can calculate the pressure at the convex interfacepint=pwρgh=patmρgh.{\displaystyle p_{\rm {int}}=p_{\rm {w}}-\rho gh=p_{\rm {atm}}-\rho gh.}

Result at equilibrium

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The hydrostatic analysis shows thatΔp=ρgh{\displaystyle \Delta p=\rho gh}, combining this with the Laplace pressure calculation we have:ρgh=2γcosθr0,{\displaystyle \rho gh={\frac {2\gamma \cos \theta }{r_{0}}},}solving forh{\displaystyle h} returns Jurin's law.

References

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  1. ^abRapp, E., Bastian (13 December 2016).Microfluidics : modeling, mechanics and mathematics. Kidlington, Oxford, United Kingdom.ISBN 9781455731510.OCLC 966685733.{{cite book}}: CS1 maint: location missing publisher (link) CS1 maint: multiple names: authors list (link)
  2. ^abSee:
  3. ^abcdQuéré, David; Brochard-Wyart, Françoise; Gennes, Pierre-Gilles de (2004), "Capillarity and Gravity",Capillarity and Wetting Phenomena, Springer, New York, NY, pp. 33–67,doi:10.1007/978-0-387-21656-0_2,ISBN 9781441918338
  4. ^"Capillary Tubes - an overview | ScienceDirect Topics".www.sciencedirect.com. Retrieved2021-10-29.
  5. ^Karen Wright (March 2003)."The Physics of Negative Pressure".Discover.Archived from the original on 8 January 2015. Retrieved31 January 2015.
  6. ^abcBush, John W. M. (3 June 2013)."18.357 Interfacial Phenomena Fall 2010"(PDF).MIT OpenCourseware. Retrieved19 December 2018.
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