equation

Nernst equation

The Nernst equation calculates the equilibrium potential for an ion across a membrane based on its concentration gradient.
3 related articles · 3 formulas · 1 who worked here

Description

German physical chemist Walther Nernst derived his equation in 1888 while studying galvanic cells. He realized that the electrical voltage at the metal-solution interface arises from the competition between two forces: chemical (the tendency of ions to dissolve) and electrical (the attraction of ions to the charged metal). Later, the equation was adapted for biological membranes. In living cells, the membrane is pierced by ion channels—protein pores that selectively allow certain ions to pass. The Nernst equation calculates the equilibrium potential for each ion: E = (RT/zF) * ln([ion outside]/[ion inside]). Here, R is the gas constant, T is absolute temperature, z is the ion charge, and F is Faraday's constant. At body temperature (37°C), the factor RT/F is approximately 26.7 mV. If the potassium concentration inside a cell is 30 times higher than outside, the potassium equilibrium potential is 26.7 * ln(1/30) ≈ -90 mV. This means the electrical force holding positive potassium ions inside the cell balances their tendency to leak out along the concentration gradient.

History

Walther Nernst, a student of Ludwig Boltzmann, formulated the equation in 1888 as part of his dissertation on electrochemistry. He studied potentials at the interface between metals and their salt solutions and established the logarithmic dependence of potential on ion concentration. In 1920, Nernst received the Nobel Prize in Chemistry for his work on thermochemistry. In the 1940s, Alan Hodgkin and Bernard Katz applied the Nernst equation to biological membranes, showing that the resting potential of the squid axon is close to the potassium equilibrium potential. This became the foundation for the Hodgkin-Huxley model describing nerve impulse generation.

How it works

In electrochemistry, the Nernst equation is used to calculate the EMF of galvanic cells and determine the pH of solutions. In biology, it is used to find equilibrium potentials for K⁺, Na⁺, Cl⁻, and Ca²⁺, which is essential for understanding cell excitability. Limitations: the equation is valid for dilute solutions (concentrations less than 0.1 M) and in the absence of side reactions at the electrodes. In concentrated solutions, activities replace concentrations with correction factors. For biological membranes, it must be considered that the actual membrane potential rarely matches the Nernst potential for a single ion due to permeability to multiple ions.

In practice

Calculating voltage across membranes of living cells, essential for understanding nerve and muscle function. In chemistry, determining ion concentrations in solutions using electrodes.

Fun fact

The Nernst equation explains why bananas and potatoes can be used as batteries: different ion concentrations in the flesh and at the electrodes create voltage. School experiments with potato clocks work precisely on this principle.

Concept graph →

Formulas

$$M(<r) = -\frac{r^2}{G}\frac{dP}{dr}$$
Mass enclosed within radius r derived from pressure gradient under hydrostatic equilibrium.
What is in the formula
M(<r)variablemass enclosed within radius r — mass kilogram
rvariableradial distance from the center — radius metre
Pvariablepressure — pressure pascal
Gconstantconstant of proportionality in Newton's law of universal gravitation — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared
dP/droperatorderivative of pressure with respect to radius — radial derivative
m_{\rmhse}(<r)=-\frac{r^2}{g}\frac{dp}{dr}\frac{1}{n_g} · 2607.20721v1
$$f''' + f f'' + \beta (1 - (f')^2) = 0$$
Describes boundary layer flow with pressure gradient.
What is in the formula
fvariablesimilarity solution function — stream function
\betavariablepressure gradient parameter — pressure gradient parameter
'operatorderivative with respect to similarity variable — derivative
y'''+yy''=0 · 2607.00237
$$\frac{dP_r}{dr} = -\frac{G(\epsilon + P_r)(m + 4\pi r^3 P_r/c^2)}{c^2 r^2 (1 - 2Gm/(c^2 r))} + \frac{2(P_t - P_r)}{r}$$
Describes hydrostatic equilibrium in general relativity with anisotropic pressure.
What is in the formula
P_rvariableRadial pressure — pressure pascal
rvariableRadial coordinate — radius metre
εvariableEnergy density — energy density joule per cubic metre
mvariableMass enclosed within radius r — mass kilogram
P_tvariableTangential pressure — pressure pascal
GconstantFundamental constant governing gravitational strength — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared
cconstantUniversal speed limit for massless particles — speed of light = 299792458 metre per second
d/droperatorDifferentiates a function with respect to r — ordinary derivative
\frac{dp_r}{dr}=-\frac{g(ε+p_r)(m+4πr^3p_r/c^2)}{c^2r^2(1-2gm/(c^2r))}+\frac{2(p_t-p_r)}{r} · 2607.25055v1

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