Potential of a Dipole

A water molecule is electrically neutral — ten protons, ten electrons, net charge exactly zero. Yet stand a nanometre away from one and your test charge feels a landscape of hills and hollows tens of millivolts deep; multiply that by every molecule in a glass and you get a liquid that dissolves salt, bends near a charged comb, and heats in a microwave oven. Neutral is not the same as silent. What a neutral-but-lopsided object projects into the space around it is the subject of this module: the potential of an electric dipole. You already own both ingredients. From The Electric Dipole & Dipole Moment you have the object itself — charges +q+q and −q-q a small distance apart, packaged into the moment pp. From Potential of Point Charges & Charge Systems you have the superpower: potentials add as plain signed numbers. A dipole's potential is literally two terms of that scalar sum — one positive hill, one negative hollow, almost cancelling. The near-cancellation is the whole story: what survives falls off as 1/r21/r^2, one power faster than a single charge's 1/r1/r, and carries a cos⁡θ\cos\theta that makes the sign depend on which end of the dipole faces you. For CBSE and ISC this derivation is a standing 3-marker: "obtain the expression for the potential due to a short dipole." For JEE and NEET it is a favourite because one formula stores three answers — axial, equatorial, and general — plus a trap about zero potential that catches half of every cohort. Twenty minutes here banks all of it.

Key takeaways
  • A dipole's potential is the scalar sum of two point-charge terms: V=kq(1r+−1r−)V = kq\left(\frac{1}{r_+} - \frac{1}{r_-}\right) — no vectors, no components.
  • Far from a short dipole (r≫ar \gg a) this collapses to V=kpcos⁡θr2V = \dfrac{kp\cos\theta}{r^2}, with p=q(2a)p = q(2a) the dipole moment and θ\theta measured from the dipole axis.
  • On the axis: V=±kp/r2V = \pm kp/r^2 (positive toward the +q+q end). On the equatorial plane: V=0V = 0 exactly — the whole plane.
  • The 1/r21/r^2 falloff is one power faster than a point charge's 1/r1/r: neutrality kills the leading term, and the residue is the price of the separation between the charges.
  • Zero potential on the equatorial plane does not mean zero field there — the dipole field at that plane is kp/r3kp/r^3, pointing antiparallel to p⃗\vec{p}.
  • Key idea: a dipole's potential is a near-perfect cancellation — what survives is kpcos⁡θ/r2kp\cos\theta/r^2, signed by which end faces you and dying one power faster than a single charge.
The core insight

Because potentials superpose as signed numbers, a dipole's potential is two almost-cancelling point-charge terms whose far-field residue is V=kpcos⁡θ/r2V = kp\cos\theta/r^2 — positive ahead of the moment, negative behind, exactly zero on the equatorial plane, and falling as 1/r21/r^2 because the monopole term of a neutral object is gone.

Where this lives today

Every computational drug-discovery pipeline evaluates dipole potentials by the billion. A protein pocket and a candidate molecule are modelled as thousands of partial charges; the electrostatic potential each projects — monopole terms, dipole terms, the whole Legendre ladder — is computed on a grid, and docking software scores how well the candidate's hills nest into the pocket's hollows. The millivolt-scale, nanometre-range landscape you computed for one water molecule in the worked example is precisely the raw material: multiply it across a solvation shell and you have the electrostatics of biochemistry. The same physics runs the gadget in your kitchen. A microwave oven's 2.45 GHz field grabs water molecules by their dipole moments and twists them back and forth billions of times a second; the "thermal jostling" that fought the dipole in worked example 2 is exactly what the oven amplifies — friction between rocking dipoles becomes heat. Neutral molecules, non-zero pp: dinner.

The physical picture

Build the landscape by superposition. A lone +q+q raises a circular hill, +kq/r+kq/r. A lone −q-q digs a matching funnel, −kq/r-kq/r. Now slide them toward each other until they sit a small distance 2a2a apart: almost everywhere, the hill and the funnel nearly cancel, because almost everywhere you are nearly equidistant from the two charges. The surviving terrain is subtle — a low ridge on the side facing +q+q, a shallow trench on the side facing −q-q, and between them a perfectly flat line at sea level: the plane of points exactly equidistant from both charges, where the cancellation is total.

Figure
The dipole's potential landscape — a ridge, a trench, and the flat V = 0 plane between
equatorial plane: V = 0 everywhere +q −q p V > 0 lobes ahead of p V < 0 lobes behind p P r θ equipotential lobes drawn at ±equal values; the flat green plane is the one zero-cost highway

Two features of this map decide every exam question. First, the sign compass: the potential is positive in the half-space the moment p⃗\vec{p} points into (the +q+q side), negative in the other half, zero on the boundary plane. The angle θ\theta between p⃗\vec{p} and your line of sight is all that decides the sign — through cos⁡θ\cos\theta, positive for θ<90°\theta < 90°, negative past it. Second, the falloff: double your distance from a point charge and VV drops to a quarter... no — to a half, since V∝1/rV \propto 1/r; but double your distance from a dipole and its potential drops to a quarter, V∝1/r2V \propto 1/r^2. The dipole's influence dies faster because from far away the two charges overlap and erase each other; only their failure to sit at the same point keeps VV alive at all. Keep the family portrait in view — it is a one-mark question in three disguises:

sourcepotential falls asfield falls aswhy
point charge QQ1/r1/r1/r21/r^2nothing cancels
short dipole1/r21/r^21/r31/r^3monopole cancelled; separation survives

The field column belongs to Field of a Dipole: Axial & Equatorial — we quote it here for the contrast and never re-derive it. Within each row, the field always falls one power faster than the potential: the field is the slope of the potential, and slopes of dying hills die faster, the rule you sharpened in Equipotentials & the Field–Potential Link.

Figure
Point charge vs dipole — the 1 over r hill and the 1 over r squared hill, matched at r = 1
distance r (units of the reference distance) V matched here, r = 1 point charge: V ∝ 1/r dipole: V ∝ 1/r² r = 3 double the distance: point charge keeps 1/2 dipole keeps only 1/4 the dipole's influence dies one power faster — neutrality erases the leading term

From two terms to one formula

Set up the standard geometry once, cleanly. Put the dipole at the origin with its axis along a line: −q-q at distance aa on one side, +q+q at distance aa on the other, total separation 2a2a, moment p=q(2a)p = q(2a) pointing from −q-q to +q+q. The observation point PP sits at distance rr from the centre, at angle θ\theta from the moment's direction. Call the distances from PP to the two charges r+r_+ and r−r_-. Because potential is a scalar — the doctrine of Potential of Point Charges & Charge Systems — the exact answer is one line:

V=kqr+−kqr−=kq r−−r+r+ r−(1)V = \frac{kq}{r_+} - \frac{kq}{r_-} = kq\,\frac{r_- - r_+}{r_+\,r_-} \qquad (1)

where: k=9.0×109 N m2/C2k = 9.0\times10^9\ \mathrm{N\,m^2/C^2}; r±r_\pm — the distances from PP to +q+q and −q-q. The second form, with the two fractions combined, is the one to remember: it shows that everything hangs on how different the two distances are (r−−r+r_- - r_+ upstairs) and how far away you are overall (r+r−r_+ r_- downstairs). If PP is equidistant from both charges, the numerator dies and V=0V = 0 — the equatorial plane, exactly, with no approximation. Far from a short dipole (r≫ar \gg a), two clean approximations turn equation (1) into the formula the boards want. The derivation card below earns them honestly; the results are r−−r+≈2acos⁡θr_- - r_+ \approx 2a\cos\theta (the path difference is the projection of the separation onto your line of sight) and r+r−≈r2r_+ r_- \approx r^2. Substituting both:

V=k pcos⁡θr2,p=q (2a)(2)V = \frac{k\,p\cos\theta}{r^2}, \qquad p = q\,(2a) \qquad (2)

where: pp — the dipole moment (C·m), direction −q→+q-q \to +q; θ\theta — the angle between p⃗\vec{p} and the line from the dipole's centre to PP; valid for r≫ar \gg a (the "short dipole" regime). Read the anatomy: the cos⁡θ\cos\theta is the sign compass, the r2r^2 is the accelerated falloff, and pp is the only thing about the dipole the far zone can still see — not qq and aa separately, only their product, exactly the lesson of The Electric Dipole & Dipole Moment. The two special directions every paper asks about drop straight out of equation (2):

Vaxial=±kpr2(θ=0° or 180°),Vequatorial=0(θ=90°)(3)V_{\text{axial}} = \pm\frac{kp}{r^2} \qquad (\theta = 0° \text{ or } 180°), \qquad\qquad V_{\text{equatorial}} = 0 \qquad (\theta = 90°) \qquad (3)

where: the ++ sign holds on the +q+q side (θ=0\theta = 0, cos⁡θ=+1\cos\theta = +1), the −- sign on the −q-q side (θ=180°\theta = 180°, cos⁡θ=−1\cos\theta = -1). Every intermediate direction interpolates through cos⁡θ\cos\theta — at 60°60° from the axis you get exactly half the axial value, a favourite quick-check in MCQs.

Derivation AThe dipole potential from two point charges

The goal is equation (2), V=kpcos⁡θ/r2V = kp\cos\theta/r^2, built from the exact two-term sum (1) using only algebra and one honest geometric approximation — this is the CBSE/ISC 3-mark derivation in full dress. The strategy: express the path difference r−−r+r_- - r_+ and the product r+r−r_+ r_- in the far-field regime r≫ar \gg a by projecting the charge separation onto the line of sight, then substitute both into (1) and watch the dipole moment assemble itself. The step to watch is the projection: it is where cos⁡θ\cos\theta — and therefore all the sign physics — enters.

Step 1. Write the exact scalar sum. With PP at distance r+r_+ from +q+q and r−r_- from −q-q:

V=kqr+−kqr−=kq r−−r+r+ r−V = \frac{kq}{r_+} - \frac{kq}{r_-} = kq\,\frac{r_- - r_+}{r_+\,r_-}

Why we may simply subtract: potential is a scalar — the two contributions add as signed numbers with no angles or components, the whole advantage of the potential route over the field route.

Step 2. Find the path difference by projection. Drop a perpendicular from each charge onto the line joining the centre to PP. For r≫ar \gg a, the lines from the two charges to PP are effectively parallel, and each charge's distance to PP differs from rr only by the projection of its offset onto that line: r+≈r−acos⁡θr_+ \approx r - a\cos\theta and r−≈r+acos⁡θr_- \approx r + a\cos\theta. Subtracting:

r−−r+≈2acos⁡θr_- - r_+ \approx 2a\cos\theta

Why the projection appears: only the component of the separation along your line of sight changes the distances; the transverse component moves the charges sideways, which at long range changes distances only at second order in a/r — invisible at this accuracy.

Step 3. Approximate the product. Both distances differ from rr by at most aa, so

r+ r−≈(r−acos⁡θ)(r+acos⁡θ)=r2−a2cos⁡2θ≈r2r_+\,r_- \approx (r - a\cos\theta)(r + a\cos\theta) = r^2 - a^2\cos^2\theta \approx r^2

Why we may drop the second term: it is smaller than r2r^2 by the factor (a/r)2(a/r)^2 — at r=10ar = 10a that is a 1% correction to the denominator, beneath the accuracy of the whole approximation scheme.

Step 4. Substitute both into Step 1 and name the moment:

V≈kq 2acos⁡θr2=k (q⋅2a)cos⁡θr2=k pcos⁡θr2V \approx kq\,\frac{2a\cos\theta}{r^2} = \frac{k\,(q\cdot 2a)\cos\theta}{r^2} = \frac{k\,p\cos\theta}{r^2}

The combination q(2a)q(2a) appeared on its own — the far zone genuinely cannot see qq and 2a2a separately, only their product pp. Verified numerically: for q=1.0q = 1.0 nC, 2a=2.02a = 2.0 cm, at r=0.10r = 0.10 m on the axis, the exact sum (1) gives kq(10.09−10.11)=18.2kq\left(\frac{1}{0.09} - \frac{1}{0.11}\right) = 18.2 V while formula (2) gives kp/r2=18.0kp/r^2 = 18.0 V — a 1% difference at r=10ar = 10a, closing rapidly at larger rr; at r=5ar = 5a the error is 4%. Matches the NCERT §2.4 result and the far-field limit of the UG treatment.

Limiting cases

caseresultmeaning
θ=0°\theta = 0° (axis, +q+q side)V=+kp/r2V = +kp/r^2maximum positive — facing the ridge
θ=180°\theta = 180° (axis, −q-q side)V=−kp/r2V = -kp/r^2maximum negative — facing the trench
θ=90°\theta = 90° (equatorial plane)V=0V = 0 exactlytotal cancellation; true even without the far-field approximation
θ=60°\theta = 60°V=12×V = \tfrac12 \times axial valuecos⁡60°=12\cos 60° = \tfrac12 — the MCQ interpolation check
r≫ar \gg aformula (2) accurate1% at r=10ar = 10a, 4% at r=5ar = 5a
r∼ar \sim a (close in)formula (2) fails; use the exact sum (1)near zone belongs to the two charges separately
a→0a \to 0 at fixed qqV→0V \to 0charges coincide and erase each other — no lopsidedness, no potential

Worked examples

Board level — axial, angled and equatorial in one sweep (CBSE/ISC pattern)

Two charges ±1.0 nC\pm 1.0\ \mathrm{nC} are separated by 2.0 cm2.0\ \mathrm{cm}. Find the electric potential (a) at a point 10 cm10\ \mathrm{cm} from the centre on the axis, on the +q+q side; (b) at 10 cm10\ \mathrm{cm} from the centre at 60°60° from the axis; (c) on the equatorial plane. Take k=9.0×109 N m2/C2k = 9.0\times10^9\ \mathrm{N\,m^2/C^2}.

Step 1. Assemble the moment first — it is the only dipole property the formula needs: p=q(2a)=(1.0×10−9)(2.0×10−2)=2.0×10−11 C mp = q(2a) = (1.0\times10^{-9})(2.0\times10^{-2}) = 2.0\times10^{-11}\ \mathrm{C\,m}.

Step 2. Check the regime: r=0.10r = 0.10 m against a=0.010a = 0.010 m gives r=10ar = 10a — comfortably "short dipole", so equation (2) applies (with ~1% honesty, worth one line in an answer).

Step 3. Axial, +q+q side (θ=0\theta = 0): V=kpr2=(9.0×109)(2.0×10−11)(0.10)2=0.180.010=+18 VV = \dfrac{kp}{r^2} = \dfrac{(9.0\times10^9)(2.0\times10^{-11})}{(0.10)^2} = \dfrac{0.18}{0.010} = \boxed{+18\ \mathrm{V}}.

Step 4. At 60°60°: multiply by cos⁡60°=0.5\cos 60° = 0.5: V=18×0.5=+9.0 VV = 18 \times 0.5 = \boxed{+9.0\ \mathrm{V}}. No new computation — the axial answer is the amplitude, cos⁡θ\cos\theta is the dial.

Step 5. Equatorial (θ=90°\theta = 90°): cos⁡90°=0\cos 90° = 0, so V=0V = \boxed{0} — and state the reason for the mark: every equatorial point is equidistant from +q+q and −q-q, so the two scalar contributions cancel exactly.

Competitive level — a water molecule versus thermal chaos (JEE-Main/NEET pattern)

A water molecule has dipole moment p=6.2×10−30 C mp = 6.2\times10^{-30}\ \mathrm{C\,m}. (a) Find the potential it produces at r=1.0 nmr = 1.0\ \mathrm{nm} from its centre, at θ=60°\theta = 60° from its axis. (b) Find the potential energy of an electron placed at that point, and compare its magnitude with the thermal energy scale kBTk_BT at 300 K300\ \mathrm{K} (kB=1.38×10−23 J/Kk_B = 1.38\times10^{-23}\ \mathrm{J/K}). Use k=8.99×109 N m2/C2k = 8.99\times10^9\ \mathrm{N\,m^2/C^2}, e=1.6×10−19 Ce = 1.6\times10^{-19}\ \mathrm{C}.

Step 1. Potential from equation (2): V=kpcos⁡θr2=(8.99×109)(6.2×10−30)(0.5)(1.0×10−9)2V = \dfrac{kp\cos\theta}{r^2} = \dfrac{(8.99\times10^9)(6.2\times10^{-30})(0.5)}{(1.0\times10^{-9})^2}.

Step 2. Numerator: 8.99×109×6.2×10−30×0.5=2.79×10−208.99\times10^9 \times 6.2\times10^{-30} \times 0.5 = 2.79\times10^{-20}. Denominator: 1.0×10−181.0\times10^{-18}. So V=2.79×10−2 V≈28 mVV = 2.79\times10^{-2}\ \mathrm{V} \approx \boxed{28\ \mathrm{mV}} — millivolt terrain, a nanometre out.

Step 3. Potential energy of the electron there — the U=qVU = qV bridge from Electric Potential & Potential Difference: ∣U∣=eV=(1.6×10−19)(2.79×10−2)=4.5×10−21 J|U| = eV = (1.6\times10^{-19})(2.79\times10^{-2}) = \boxed{4.5\times10^{-21}\ \mathrm{J}}. (Sign: the electron is negative, so at this positive-VV point its energy is −4.5×10−21-4.5\times10^{-21} J — it is attracted toward the positive lobe.)

Step 4. Thermal comparison: kBT=(1.38×10−23)(300)=4.1×10−21 Jk_BT = (1.38\times10^{-23})(300) = 4.1\times10^{-21}\ \mathrm{J}. The ratio is 4.5/4.1≈1.14.5/4.1 \approx 1.1 — the dipole's electrical grip at a nanometre is only just as strong as ambient thermal jostling. That single comparison is why water's dipoles do not lock rigidly to every passing ion at room temperature, and why polar interactions in liquids are constantly made and broken — the microscopic backdrop for Dielectrics & Polarisation, where thermal randomisation fights the field for control of the molecules. Timing note: 3 minutes. The mark-getters are the clean powers of ten in Step 2 (practise 109×10−30/10−1810^9 \times 10^{-30}/10^{-18}-type collections until they take five seconds) and remembering that (b) is one multiplication by ee — not a new formula. If the paper asks "at what angle is V half the axial value", answer 60°60° from cos⁡θ=12\cos\theta = \tfrac12 without touching the calculator.

Exam traps

Mixing the dipole's VV and EE formulas. V∝1/r2V \propto 1/r^2; the field magnitudes go as 1/r31/r^3 (axial 2kp/r32kp/r^3, equatorial kp/r3kp/r^3 — from Field of a Dipole). Writing kpcos⁡θ/r3kp\cos\theta/r^3 for the potential, or kp/r2kp/r^2 for a field, is the most common single error. Anchor: potential is always one power slower than field.

Measuring rr from a charge instead of the centre. In the board example above, taking rr from the +q+q charge (0.09 m... or worse, 0.10 m to +q+q and 0.12 m to −q-q) gives 15 V instead of 18 V — a wrong answer that looks plausible. The formula's rr starts at the dipole's midpoint. Always.

Forgetting the sign of the axial potential. +kp/r2+kp/r^2 only on the +q+q side; the −q-q side is −kp/r2-kp/r^2. Read the question's geometry before writing the sign, and remember p⃗\vec{p} points from −q-q to +q+q — the direction convention itself is a one-mark question.

θ measured from the wrong line. θ\theta is the angle from the axis (the direction of p⃗\vec{p}), not from the equatorial plane. A point "30° above the equatorial plane" sits at θ=60°\theta = 60° — translate before substituting.

Using the far-field formula too close. Equation (2) needs r≫ar \gg a: at r=5ar = 5a it is already 4% off, and JEE-Advanced setters exploit this by asking for the exact two-term sum (1) at moderate range. If rr and aa are within a factor of ~5, compute both distances and use (1).

"V = 0 means no work ever". Bringing a charge from infinity to an equatorial point costs zero net work — true, and a favourite assertion-reason item. But moving it from an equatorial point to an axial point costs q ΔV≠0q\,\Delta V \ne 0. Zero is a value of the landscape at some places, not a promise about all journeys.

Constants. k=9.0×109 N m2/C2k = 9.0\times10^9\ \mathrm{N\,m^2/C^2} is accepted by CBSE/ISC/NEET; carry 8.99×1098.99\times10^9 in JEE-Advanced when options sit close. Dipole moments of molecules are often quoted in debye: 1 D=3.34×10−30 C m1\ \mathrm{D} = 3.34\times10^{-30}\ \mathrm{C\,m} — water's 6.2×10−30 C m6.2\times10^{-30}\ \mathrm{C\,m} is 1.85 D; convert to SI before any formula.

Origins · 1 minAdrien-Marie Legendre and how this was discovered
AL
Adrien-Marie Legendre
1752–1833 · Paris

The cos⁡θ\cos\theta in the dipole formula has a surname, and it is Legendre's. In 1782 he attacked the problem of the gravitational pull of a spheroid — a planet-shaped lump — and found that the potential of any compact body, seen from outside, could be expanded in powers of 1/r1/r, each power carrying its own characteristic function of the viewing angle. Those angle functions are the Legendre polynomials, and the first of them, P1(cos⁡θ)=cos⁡θP_1(\cos\theta) = \cos\theta, is precisely the angular fingerprint of a dipole. In that expansion, your formula kpcos⁡θ/r2kp\cos\theta/r^2 is the second rung of an infinite ladder — monopole, dipole, quadrupole, … — that physicists still climb today, from planetary gravity to molecular chemistry to the pattern of the cosmic microwave background. Legendre, meanwhile, spent his life in Paris quietly building tools — his textbook on geometry trained a century of students — and feuding with no one except, famously, over credit with Gauss.

History
1782
— Legendre expands the potential of a spheroid; the polynomials Pl(cos⁡θ)P_l(\cos\theta) — and the dipole's cos⁡θ\cos\theta — are born.
1812
— Poisson applies potential theory to electrostatics: charged bodies get the same mathematics as planets.
1828
— Green's essay names the "potential function" and gives electricity its landscape language.
1912
— Debye explains the dielectric behaviour of liquids via permanent molecular dipole moments — molecules are little pp vectors.
1936
— Debye's Nobel Prize; the unit of molecular dipole moment is named the debye in his honour.

Going further

Texts. NCERT Physics Part 1, Ch. 2 §2.4 — the board-canonical derivation this module dresses in full · HC Verma, Concepts of Physics 2, Ch. 29 · Halliday, Resnick & Walker Ch. 24. For the multipole ladder the cos⁡θ\cos\theta came from — and the dipole field in coordinate-free form — see Electric Dipole Moment (UG deep dive).

Provenance. Standard results per NCERT §2.4 and HRW Ch. 24. A verifier should recompute: p=(1.0×10−9)(0.020)=2.0×10−11p = (1.0\times10^{-9})(0.020) = 2.0\times10^{-11} C·m; axial V=kp/r2=18.0V = kp/r^2 = 18.0 V at r=0.10r = 0.10 m vs exact kq(1/0.09−1/0.11)=18.2kq(1/0.09 - 1/0.11) = 18.2 V (1.0% low); V(60°)=9.0V(60°) = 9.0 V; water molecule V=(8.99×109)(6.2×10−30)(0.5)/10−18=27.9V = (8.99\times10^9)(6.2\times10^{-30})(0.5)/10^{-18} = 27.9 mV; ∣U∣=eV=4.5×10−21|U| = eV = 4.5\times10^{-21} J vs kBT(300 K)=4.1×10−21k_BT(300\,\mathrm{K}) = 4.1\times10^{-21} J, ratio 1.08; far-field error 4% at r=5ar = 5a.

Prerequisites. The Electric Dipole & Dipole Moment · Potential of Point Charges & Charge Systems. Leads to. Dielectrics & Polarisation · Electric Dipole Moment (UG deep dive).

If the dipole is neutral overall, why is there any potential at all?

Because the two charges are not at the same place, and potential cares about distance. From any point not on the equatorial plane you are slightly closer to one charge than the other, so its kq/rkq/r term slightly outweighs the other's −kq/r-kq/r — near-cancellation, not cancellation. The survivor is proportional to the path difference 2acos⁡θ2a\cos\theta, which is why everything scales with the separation: shrink 2a2a to zero and the potential genuinely dies everywhere. Neutrality kills the 1/r1/r term a net charge would have; the 1/r21/r^2 residue is the electrical signature of shape — of charge that is balanced but not coincident.

Why does the potential fall as 1/r² when each individual charge falls as 1/r?

Write the combined form of the sum: V=kq(r−−r+)/(r+r−)V = kq(r_- - r_+)/(r_+ r_-). The numerator, the path difference, saturates at the fixed value 2acos⁡θ2a\cos\theta — it does not grow as you retreat. The denominator grows as r2r^2. So the whole expression inherits one factor of 1/r1/r from each distance in the product: the 1/r1/r of a lone charge, times an extra 1/r1/r because the two charges' contributions overlap more and more perfectly with distance. Each rung of the multipole ladder repeats the trick — a quadrupole (two back-to-back dipoles) cancels the dipole term too and falls as 1/r31/r^3.

Is V = 0 on the equatorial plane exact, or only a far-field approximation?

Exact — and it is the only feature of the dipole potential that is. Any point of the perpendicular-bisector plane is precisely equidistant from +q+q and −q-q by the plane's definition, so the two contributions +kq/r+kq/r and −kq/r-kq/r cancel identically, with no expansion, no assumption about r≫ar \gg a. Everything else in the module — the cos⁡θ\cos\theta, the 1/r21/r^2 — carries the far-field caveat. This is worth flagging in derivation answers: state "exact by symmetry" for the equatorial zero and "for r≫ar \gg a" for the rest, and the marks-scheme boxes tick themselves.

How short is a "short" dipole — when am I allowed to use kp cosθ/r²?

The formula's error is of order (a/r)2(a/r)^2 in the denominator plus the neglected transverse projection — in practice: about 1% at r=10ar = 10a, about 4% at r=5ar = 5a, and unusable by r≈2ar \approx 2a. Board questions are built in the safe zone (r≥5ar \ge 5a) and expect the formula. JEE-Advanced occasionally sets r=2ar = 2a or asks explicitly for the exact potential — the tell is a nice pair of distances like 0.09 m and 0.11 m hiding in the geometry. When in doubt, compute r+r_+ and r−r_- and use the exact two-term sum; it is never wrong, just slower.

Does the sign of V flip if I look at the dipole from behind?

Yes — and that is the physics, not a bookkeeping accident. The formula's cos⁡θ\cos\theta is positive when your line of sight makes an acute angle with p⃗\vec{p} (you are facing the +q+q end) and negative past 90° (the −q-q end faces you). Walk in a circle around a dipole at fixed distance and the potential you sample runs +kp/r2→0→−kp/r2→0→+kp/r2+kp/r^2 \to 0 \to -kp/r^2 \to 0 \to +kp/r^2 — a smooth cosine wave in your walking angle. A voltmeter carried on that walk would read the wave directly. The two zero crossings are your two intersections with the equatorial plane.

Where does this show up beyond textbook dipoles — why do chemists care about p?

Because pp is the leading electrical descriptor of any neutral molecule. Water (1.85 D), HCl (1.08 D), ammonia (1.47 D) — these numbers, measured largely by the methods Debye pioneered, predict boiling points, solubility ("like dissolves like" is dipole language), infrared absorption and microwave heating. In proteins, the backbone's repeating dipoles stack into helix "macro-dipoles" that steer binding. And the same cos⁡θ/r2\cos\theta/r^2 term, in gravity's version of the ladder, is how satellites feel Earth's equatorial bulge. One formula, three sciences — which is exactly what Legendre's expansion promised.

Before this

Where this leads