Parallel edition

On the Electrodynamics of Moving Bodies

By A. Einstein · Annalen der Physik (4) 17, 891–921 (1905).

Deutsch

[p. 891]
Zur Elektrodynamik bewegter Körper;

English

On the Electrodynamics of Moving Bodies

Deutsch

[p. 891]
von A. Einstein.

English

by A. Einstein

Deutsch

[p. 892]I. Kinematischer Teil.

English

I. Kinematical Part.

Deutsch

English

II. Electrodynamical Part.

Deutsch

[p. 910]§ 7. Theorie des Doppelerschen Prinzips und der Aberration.

English

§ 7. Theory of Doppler’s Principle and of Aberration.

Deutsch

[p. 910]Im Systeme KK befinde sich sehr ferne vom Koordinatenursprung eine Quelle elektrodynamischer Wellen, welche in einem den Koordinatenursprung enthaltenden Raumteil mit genügender Annäherung durch die Gleichungen dargestellt sei:X=X0sin⁡Φ,L=L0sin⁡Φ,Y=Y0sin⁡Φ,M=M0sin⁡Φ,Φ=ω(t−ax+by+czV).Z=Z0sin⁡Φ,N=N0sin⁡Φ,\begin{aligned} X &= X_0 \sin \Phi , &\quad L &= L_0 \sin \Phi , \\ Y &= Y_0 \sin \Phi , &\quad M &= M_0 \sin \Phi , &\quad \Phi &= \omega \left( t - \frac{a x + b y + c z}{V} \right) . \\ Z &= Z_0 \sin \Phi , &\quad N &= N_0 \sin \Phi , \end{aligned}Electric field, stationary systemElectric field amplitude (stationary system)Wave phaseMagnetic field, stationary systemMagnetic field amplitude (stationary system)Electric field, stationary systemElectric field amplitude (stationary system)Magnetic field, stationary systemMagnetic field amplitude (stationary system)Wave angular frequency (stationary system)Time in the stationary systemDirection cosine (stationary system)Position in the stationary systemDirection cosine (stationary system)Position in the stationary systemDirection cosine (stationary system)Position in the stationary systemSpeed of lightElectric field, stationary systemElectric field amplitude (stationary system)Magnetic field, stationary systemMagnetic field amplitude (stationary system)Explain this equation Hierbei sind (X0,Y0,Z0)(X_0, Y_0, Z_0) und (L0,M0,N0)(L_0, M_0, N_0) die Vektoren, welche die Amplitude des Wellenzuges bestimmen, aa, bb, cc die Richtungskosinus der Wellennormalen.

English

In the system KK, very far from the coordinate origin, let there be a source of electrodynamic waves which, in a part of space containing the coordinate origin, may be represented to a sufficient approximation by the equations: X=X0sin⁡Φ,L=L0sin⁡Φ,Y=Y0sin⁡Φ,M=M0sin⁡Φ,Φ=ω(t−ax+by+czV).Z=Z0sin⁡Φ,N=N0sin⁡Φ,\begin{aligned} X &= X_0 \sin \Phi , &\quad L &= L_0 \sin \Phi , \\ Y &= Y_0 \sin \Phi , &\quad M &= M_0 \sin \Phi , &\quad \Phi &= \omega \left( t - \frac{a x + b y + c z}{V} \right) . \\ Z &= Z_0 \sin \Phi , &\quad N &= N_0 \sin \Phi , \end{aligned}Electric field, stationary systemElectric field amplitude (stationary system)Wave phaseMagnetic field, stationary systemMagnetic field amplitude (stationary system)Electric field, stationary systemElectric field amplitude (stationary system)Magnetic field, stationary systemMagnetic field amplitude (stationary system)Wave angular frequency (stationary system)Time in the stationary systemDirection cosine (stationary system)Position in the stationary systemDirection cosine (stationary system)Position in the stationary systemDirection cosine (stationary system)Position in the stationary systemSpeed of lightElectric field, stationary systemElectric field amplitude (stationary system)Magnetic field, stationary systemMagnetic field amplitude (stationary system)Explain this equation Here (X0,Y0,Z0)(X_0, Y_0, Z_0) and (L0,M0,N0)(L_0, M_0, N_0) are the vectors that determine the amplitude of the wave train, and aa, bb, cc the direction cosines of the wave normal.

Deutsch

[pp. 910–911]Wir fragen nach der Beschaffenheit dieser Wellen, wenn dieselben von einem in dem bewegten System kk ruhenden Beobachter untersucht werden. — Durch Anwendung der in § 6 gefundenen Transformationsgleichungen für die elektrischen und magnetischen Kräfte und der in § 3 gefundenen Transformationsgleichungen für die Koordinaten und die Zeit erhalten wir unmittelbar:X′=X0sin⁡Φ′,L′=L0sin⁡Φ′,Y′=β(Y0−vVN0)sin⁡Φ′,M′=β(M0+vVZ0)sin⁡Φ′,Z′=β(Z0+vVM0)sin⁡Φ′,N′=β(N0−vVY0)sin⁡Φ′,Φ′=ω′(τ−a′ξ+b′η+c′ζV),\begin{aligned} X' &= X_0 \sin \Phi' , &\qquad L' &= L_0 \sin \Phi' , \\ Y' &= \beta \left( Y_0 - \frac{v}{V} N_0 \right) \sin \Phi' , &\qquad M' &= \beta \left( M_0 + \frac{v}{V} Z_0 \right) \sin \Phi' , \\ Z' &= \beta \left( Z_0 + \frac{v}{V} M_0 \right) \sin \Phi' , &\qquad N' &= \beta \left( N_0 - \frac{v}{V} Y_0 \right) \sin \Phi' , \\ \Phi' &= \omega' \left( \tau - \frac{a' \xi + b' \eta + c' \zeta}{V} \right) , \end{aligned}Electric field, moving systemElectric field amplitude (stationary system)Wave phaseMagnetic field, moving systemMagnetic field amplitude (stationary system)Electric field, moving systemLorentz factorElectric field amplitude (stationary system)Speed of the moving systemSpeed of lightMagnetic field amplitude (stationary system)Magnetic field, moving systemMagnetic field amplitude (stationary system)Electric field amplitude (stationary system)Electric field, moving systemMagnetic field, moving systemWave angular frequency (moving system)Time in the moving systemDirection cosine (moving system)Position in the moving systemDirection cosine (moving system)Position in the moving systemDirection cosine (moving system)Position in the moving systemExplain this equation wobeiω′=ωβ(1−avV),\omega' = \omega \beta \left( 1 - a \frac{v}{V} \right) ,Wave angular frequency (moving system)Wave angular frequency (stationary system)Lorentz factorDirection cosine (stationary system)Speed of the moving systemSpeed of lightExplain this equationa′=a−vV1−avV,a' = \frac{a - \frac{v}{V}}{1 - a \frac{v}{V}} ,Direction cosine (moving system)Direction cosine (stationary system)Speed of the moving systemSpeed of lightExplain this equationb′=bβ(1−avV),b' = \frac{b}{\beta \left( 1 - a \frac{v}{V} \right)} ,Direction cosine (moving system)Direction cosine (stationary system)Lorentz factorDirection cosine (stationary system)Speed of the moving systemSpeed of lightExplain this equationc′=cβ(1−avV)c' = \frac{c}{\beta \left( 1 - a \frac{v}{V} \right)}Direction cosine (moving system)Direction cosine (stationary system)Lorentz factorDirection cosine (stationary system)Speed of the moving systemSpeed of lightExplain this equation gesetzt ist.

English

We ask about the nature of these waves when they are examined by an observer at rest in the moving system kk. — By applying the transformation equations for the electric and magnetic forces found in § 6, and the transformation equations for the coordinates and the time found in § 3, we obtain directly: X′=X0sin⁡Φ′,L′=L0sin⁡Φ′,Y′=β(Y0−vVN0)sin⁡Φ′,M′=β(M0+vVZ0)sin⁡Φ′,Z′=β(Z0+vVM0)sin⁡Φ′,N′=β(N0−vVY0)sin⁡Φ′,Φ′=ω′(τ−a′ξ+b′η+c′ζV),\begin{aligned} X' &= X_0 \sin \Phi' , &\qquad L' &= L_0 \sin \Phi' , \\ Y' &= \beta \left( Y_0 - \frac{v}{V} N_0 \right) \sin \Phi' , &\qquad M' &= \beta \left( M_0 + \frac{v}{V} Z_0 \right) \sin \Phi' , \\ Z' &= \beta \left( Z_0 + \frac{v}{V} M_0 \right) \sin \Phi' , &\qquad N' &= \beta \left( N_0 - \frac{v}{V} Y_0 \right) \sin \Phi' , \\ \Phi' &= \omega' \left( \tau - \frac{a' \xi + b' \eta + c' \zeta}{V} \right) , \end{aligned}Electric field, moving systemElectric field amplitude (stationary system)Wave phaseMagnetic field, moving systemMagnetic field amplitude (stationary system)Electric field, moving systemLorentz factorElectric field amplitude (stationary system)Speed of the moving systemSpeed of lightMagnetic field amplitude (stationary system)Magnetic field, moving systemMagnetic field amplitude (stationary system)Electric field amplitude (stationary system)Electric field, moving systemMagnetic field, moving systemWave angular frequency (moving system)Time in the moving systemDirection cosine (moving system)Position in the moving systemDirection cosine (moving system)Position in the moving systemDirection cosine (moving system)Position in the moving systemExplain this equation where ω′=ωβ(1−avV),\omega' = \omega \beta \left( 1 - a \frac{v}{V} \right) ,Wave angular frequency (moving system)Wave angular frequency (stationary system)Lorentz factorDirection cosine (stationary system)Speed of the moving systemSpeed of lightExplain this equation a′=a−vV1−avV,a' = \frac{a - \frac{v}{V}}{1 - a \frac{v}{V}} ,Direction cosine (moving system)Direction cosine (stationary system)Speed of the moving systemSpeed of lightExplain this equation b′=bβ(1−avV),b' = \frac{b}{\beta \left( 1 - a \frac{v}{V} \right)} ,Direction cosine (moving system)Direction cosine (stationary system)Lorentz factorDirection cosine (stationary system)Speed of the moving systemSpeed of lightExplain this equation c′=cβ(1−avV)c' = \frac{c}{\beta \left( 1 - a \frac{v}{V} \right)}Direction cosine (moving system)Direction cosine (stationary system)Lorentz factorDirection cosine (stationary system)Speed of the moving systemSpeed of lightExplain this equation have been set.

Deutsch

[pp. 911–912]Aus der Gleichung für ω′\omega' folgt: Ist ein Beobachter relativ zu einer unendlich fernen Lichtquelle von der Frequenz ν\nu mit der Geschwindigkeit vv derart bewegt, daß die Verbindungslinie „Lichtquelle–Beobachter“ mit der auf ein relativ zur Lichtquelle ruhendes Koordinatensystem bezogenen Geschwindigkeit des Beobachters den Winkel φ\varphi bildet, so ist die von dem Beobachter wahrgenommene Frequenz ν′\nu' des Lichtes durch die Gleichung gegeben:ν′=ν1−cos⁡φvV1−(vV)2.\nu' = \nu \frac{1 - \cos \varphi \frac{v}{V}}{\sqrt{1 - \left( \frac{v}{V} \right)^2}} .Frequency, moving systemFrequency, stationary systemAngle to the motion, stationary systemSpeed of the moving systemSpeed of lightExplain this equation Dies ist das Doppelersche Prinzip für beliebige Geschwindigkeiten. Für φ=0\varphi = 0 nimmt die Gleichung die übersichtliche Form an:ν′=ν1−vV1+vV.\nu' = \nu \sqrt{\frac{1 - \frac{v}{V}}{1 + \frac{v}{V}}} .Frequency, moving systemFrequency, stationary systemSpeed of the moving systemSpeed of lightExplain this equation Man sieht, daß — im Gegensatz zu der üblichen Auffassung — für v=−∞v = -\infty, ν=∞\nu = \infty ist.

English

From the equation for ω′\omega' it follows: If an observer moves with the velocity vv relative to an infinitely distant light source of frequency ν\nu in such a way that the line joining “light source–observer” makes the angle φ\varphi with the velocity of the observer, referred to a coordinate system at rest relative to the light source, then the frequency ν′\nu' of the light perceived by the observer is given by the equation: ν′=ν1−cos⁡φvV1−(vV)2.\nu' = \nu \frac{1 - \cos \varphi \frac{v}{V}}{\sqrt{1 - \left( \frac{v}{V} \right)^2}} .Frequency, moving systemFrequency, stationary systemAngle to the motion, stationary systemSpeed of the moving systemSpeed of lightExplain this equation This is Doppler’s principle for arbitrary velocities. For φ=0\varphi = 0 the equation takes the perspicuous form: ν′=ν1−vV1+vV.\nu' = \nu \sqrt{\frac{1 - \frac{v}{V}}{1 + \frac{v}{V}}} .Frequency, moving systemFrequency, stationary systemSpeed of the moving systemSpeed of lightExplain this equation One sees that — contrary to the usual view — for v=−∞v = -\infty, ν=∞\nu = \infty.

Deutsch

[p. 912]Nennt man φ′\varphi' den Winkel zwischen Wellennormale (Strahlrichtung) im bewegten System und der Verbindungslinie „Lichtquelle–Beobachter“, so nimmt die Gleichung für a′a' die Form an:cos⁡φ′=cos⁡φ−vV1−vVcos⁡φ.\cos \varphi' = \frac{\cos \varphi - \frac{v}{V}}{1 - \frac{v}{V} \cos \varphi} .Angle to the motion, moving systemAngle to the motion, stationary systemSpeed of the moving systemSpeed of lightExplain this equation Diese Gleichung drückt das Aberrationsgesetz in seiner allgemeinsten Form aus. Ist φ=π/2\varphi = \pi/2, so nimmt die Gleichung die einfache Gestalt an:cos⁡φ′=−vV.\cos \varphi' = - \frac{v}{V} .Angle to the motion, moving systemSpeed of the moving systemSpeed of lightExplain this equation

English

If we call φ′\varphi' the angle between the wave normal (direction of the ray) in the moving system and the line joining “light source–observer”, the equation for a′a' takes the form: cos⁡φ′=cos⁡φ−vV1−vVcos⁡φ.\cos \varphi' = \frac{\cos \varphi - \frac{v}{V}}{1 - \frac{v}{V} \cos \varphi} .Angle to the motion, moving systemAngle to the motion, stationary systemSpeed of the moving systemSpeed of lightExplain this equation This equation expresses the law of aberration in its most general form. If φ=π/2\varphi = \pi/2, the equation takes the simple form: cos⁡φ′=−vV.\cos \varphi' = - \frac{v}{V} .Angle to the motion, moving systemSpeed of the moving systemSpeed of lightExplain this equation

Deutsch

[p. 912]Wir haben nun noch die Amplitude der Wellen, wie dieselbe im bewegten System erscheint, zu suchen. Nennt man AA bez. A′A' die Amplitude der elektrischen oder magnetischen Kraft im ruhenden bez. im bewegten System gemessen, so erhält man:A′2=A2(1−vVcos⁡φ)21−(vV)2,A'^2 = A^2 \frac{\left( 1 - \frac{v}{V} \cos \varphi \right)^2}{1 - \left( \frac{v}{V} \right)^2} ,Light amplitude (moving system)Light amplitude (stationary system)Speed of the moving systemSpeed of lightAngle to the motion, stationary systemExplain this equation welche Gleichung für φ=0\varphi = 0 in die einfachere übergeht:A′2=A21−vV1+vV.A'^2 = A^2 \frac{1 - \frac{v}{V}}{1 + \frac{v}{V}} .Light amplitude (moving system)Light amplitude (stationary system)Speed of the moving systemSpeed of lightExplain this equation

English

We still have to find the amplitude of the waves as it appears in the moving system. If AA or A′A' denotes the amplitude of the electric or magnetic force measured in the stationary or the moving system respectively, we obtain: A′2=A2(1−vVcos⁡φ)21−(vV)2,A'^2 = A^2 \frac{\left( 1 - \frac{v}{V} \cos \varphi \right)^2}{1 - \left( \frac{v}{V} \right)^2} ,Light amplitude (moving system)Light amplitude (stationary system)Speed of the moving systemSpeed of lightAngle to the motion, stationary systemExplain this equation an equation which for φ=0\varphi = 0 passes over into the simpler one: A′2=A21−vV1+vV.A'^2 = A^2 \frac{1 - \frac{v}{V}}{1 + \frac{v}{V}} .Light amplitude (moving system)Light amplitude (stationary system)Speed of the moving systemSpeed of lightExplain this equation

Deutsch

[p. 912]Es folgt aus den entwickelten Gleichungen, daß für einen Beobachter, der sich mit der Geschwindigkeit VV einer Lichtquelle näherte, diese Lichtquelle unendlich intensiv erscheinen müßte.

English

It follows from the equations developed that, for an observer approaching a light source with the velocity VV, this light source would have to appear infinitely intense.

Deutsch

[p. 921]
Zum Schlusse bemerke ich, daß mir beim Arbeiten an dem hier behandelten Probleme mein Freund und Kollege M. Besso treu zur Seite stand und daß ich demselben manche wertvolle Anregung verdanke.

English

In conclusion I remark that in working on the problem treated here my friend and colleague M. Besso stood loyally by my side, and that I owe him several valuable suggestions.

Deutsch

[p. 921]
Bern, Juni 1905.

English

Bern, June 1905.

Deutsch

[p. 921]
(Eingegangen 30. Juni 1905.)

English

(Received 30 June 1905.)