Discover · A route you could take
A body gives off light.
What does it lose?
A body at rest gives off two flashes of light. Its energy has gone down, and nothing you can see about it has changed. The shortest of the four papers asks what has, and answers with a number. You can reach it yourself in five moves and then check the number against the world.
A route you could take, not a transcript of Einstein’s private thoughts. Every step can be read without running anything.
The 1904 shelf, and the one thing that is not on it
Eight of the nine results below were available to a careful reader at the end of 1904. The ninth is the June 1905 transformation used at step 3, and it is marked as an import because it is one.
This list is a reconstruction aid assembled for learning, not a documentary history of what Einstein read.
Published 1847The total energy of an isolated system is conserved: it can change form but the books must balance.
Available by the end of 1904
The total energy of an isolated system is conserved: it can change form but the books must balance.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1847
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- Über die Erhaltung der Kraft Berlin: G. Reimer (1847)
Source verification pending library scan inspection.
Published 1867A body of mass m moving slowly at speed v carries energy of motion equal to one half m v squared.
Available by the end of 1904
A body of mass m moving slowly at speed v carries energy of motion equal to one half m v squared.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1867
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- Treatise on Natural Philosophy Oxford: Clarendon Press, §§ 212-213 (1867)
Source verification pending library scan inspection.
Published 1873Light falling on a surface presses on it, so a beam carries momentum as well as energy.
Available by the end of 1904
Light falling on a surface presses on it, so a beam carries momentum as well as energy.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1873
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- A Treatise on Electricity and Magnetism Oxford: Clarendon Press, § 792 (1873)
Source verification pending library scan inspection.
Published 1881J. J. Thomson finds that a charged sphere moving through the ether carries a magnetic field whose energy makes the sphere harder to accelerate: its charge adds to its inertia.
Available by the end of 1904
J. J. Thomson finds that a charged sphere moving through the ether carries a magnetic field whose energy makes the sphere harder to accelerate: its charge adds to its inertia.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1881
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- On the Electric and Magnetic Effects produced by the Motion of Electrified Bodies Phil. Mag. (5) 11, 229 (1881)
Source verification pending library scan inspection.
Published 1884Energy in the electromagnetic field flows, and the rate of flow through a surface can be written down.
Available by the end of 1904
Energy in the electromagnetic field flows, and the rate of flow through a surface can be written down.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1884
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- On the Transfer of Energy in the Electromagnetic Field Phil. Trans. R. Soc. 175, 343 (1884)
Source verification pending library scan inspection.
Published 1900To keep the centre of mass of a body and its field moving uniformly when the body emits radiation, Poincaré treats electromagnetic energy as a fictitious fluid whose mass is its energy divided by the square of the speed of light.
Available by the end of 1904
To keep the centre of mass of a body and its field moving uniformly when the body emits radiation, Poincaré treats electromagnetic energy as a fictitious fluid whose mass is its energy divided by the square of the speed of light.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1900
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- La théorie de Lorentz et le principe de réaction Arch. néerl. sci. exactes nat. (2) 5, 252 (1900)
Source verification pending library scan inspection.
Published 1901The pressure of light on a solid body was measured in the laboratory and agreed with the predicted magnitude.
Available by the end of 1904
The pressure of light on a solid body was measured in the laboratory and agreed with the predicted magnitude.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1901
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- Untersuchungen über die Druckkräfte des Lichtes Ann. Phys. (4) 6, 433 (1901)
Source verification pending library scan inspection.
Published 1904Hasenöhrl finds that the radiation enclosed in a moving cavity adds to the cavity's apparent mass, by an amount proportional to the radiation's energy divided by the square of the speed of light.
Available by the end of 1904
Hasenöhrl finds that the radiation enclosed in a moving cavity adds to the cavity's apparent mass, by an amount proportional to the radiation's energy divided by the square of the speed of light.
Historical context
Available in the published scientific literature or public proceedings prior to 1905.
Available by
Published 1904
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- Zur Theorie der Strahlung in bewegten Körpern Ann. Phys. (4) 15, 344 (1904)
Source verification pending library scan inspection.
Published 1905The energy a given bundle of light is measured to carry depends on the frame it is measured in, by a factor fixed by the frame's speed and the direction of the light.
Admitted 1905 import
The energy a given bundle of light is measured to carry depends on the frame it is measured in, by a factor fixed by the frame's speed and the direction of the light.
Historical context
Imported from 1905. Section 8 of Zur Elektrodynamik bewegter Körper, received 30 June 1905, published 26 September 1905. The mass-energy paper was received 27 September 1905 and rests on it. Read that section of the paper
Available by
Published 1905
What the paper itself cites or asserts
- The mass-energy paper: Its opening paragraphs state this result, cite it to § 8 of the June paper with a footnote to Ann. d. Phys. 17, p. 891, and say that it will be used.
Where this site uses it
Primary evidence and sources
- Zur Elektrodynamik bewegter Körper, § 8 Ann. Phys. (4) 17, 891, at 912-914 (1905)
Source verification pending library scan inspection.
The dates on these cards come from standard bibliographies. No one here has checked them against the volumes, and the shelf marks each card as awaiting verification.
The nagging fact
A body that gives off light in one direction recoils. If it gives off equal pulses in opposite directions it does not recoil, and yet the two pulses carry different energies as a moving observer measures them.
The first honest question
If you already know how the energy of a light pulse changes between frames, what does the conservation of energy force you to say about the body that gave it off?
01 / Start with a body that does nothing
Where can the energy have gone?
Put a body at rest in front of you and let it give off light: two equal flashes, one to the left and one to the right, at the same moment. Because the flashes are equal and opposite, whatever push one gives the body the other takes away. The body does not recoil. It sits exactly where it sat, at rest, before and after.
Energy is conserved, so the energy carried off by the flashes came out of the body. But the body has not slowed down, because it was not moving, and it has not moved. Nothing you can see about it has changed. A quantity has left and no visible property has altered to account for it.
Why insist on two flashes rather than one?
One flash would push the body the other way, and then some of the bookkeeping would be about the recoil rather than about the body itself. The symmetric pair is a device for keeping the speed fixed so that only one unknown is left. It is a choice made to isolate a question, not a fact about how bodies emit light.
02 / Make a prediction
Is the body lighter, or is that a category error?
Before going on, commit to an answer. After the flashes have left, is the body’s mass the same as before, smaller, or is the question malformed because mass is not the sort of thing energy can be taken out of? There is a respectable case for each in 1904, and the argument below only decides between them under premises you will be able to see.
The case for “the question is malformed”
Mass in 1904 is the measure of how hard a body is to accelerate, fixed by the body and not by its history. Energy is a quantity of account that bodies exchange. On that reading, asking whether emitting light changes the mass is like asking whether paying a bill changes your height. There is a serious case for it, and nothing in the argument that follows refutes it directly. What the argument does is produce a number where that position predicts none.
03 / Describe the same event twice
Two accounts of one emission
Describe the same emission a second time, from a frame gliding steadily past at speed v. Nothing about the body changes; you have changed only where you are standing. Write down the body’s energy before and after in each account, four quantities in all.
You cannot evaluate any of the four, because each contains the body’s absolute energy content, which no one knows, in 1904 or now. That is why the second account earns its place: the quantity you cannot supply appears in both accounts, so a subtraction removes it.
The two accounts do not agree about the light, though. A given pair of flashes is measured to carry different total energy depending on the frame it is measured in, and by how much is fixed by the speed and the direction. That is the imported step. It comes from section 8 of the relativity paper, received in June of the same year, and it is the one thing in this route that a reader standing at the end of 1904 could not reach for. It is on the shelf below, marked as an import, with where it came from.
Why the import is declared rather than absorbed
A reconstruction that quietly used a 1905 result while claiming to start from 1904 would be telling you the argument is cheaper than it is. The September paper openly rests on the June one. Naming the debt is the difference between a route and a conjuring trick.
04 / Subtract
What survives when the unknowns cancel
Take the difference between the two accounts before the emission, take it again after, and subtract one from the other. Every absolute body energy disappears, because each appears once in each account. What is left on one side is a difference of differences, and on the other side the light energy multiplied by a factor that depends only on the speed.
The quantity that survives is the difference between what the moving observer and the resting observer say the body’s energy is, and how that difference changed when the light left. For a body whose speed never changed, that is its energy of motion, plus whatever fixed offset separates the two accounts.
The premise hiding in “whatever fixed offset”
Identifying the surviving quantity as a change in energy of motion requires that the offset is the same before and after. Nothing so far forces that. If the offset shifted when the light left, the subtraction still holds but it no longer isolates the energy of motion, and the route stops here with a constraint rather than a result. This is the premise worth arguing about, and the workbench below lets you remove it and see what survives.
05 / Read the coefficient
A number where a category error predicted none
Let the second observer glide past slowly and the speed factor simplifies. The paper prints the result on its last page, in the notation it was set in, where L is the energy given off and V is the speed of light:
Now put that beside the energy of motion you already had on the shelf, one half of the mass times the speed squared. The two expressions have the same shape, and in the place where a mass belongs stands the energy given off divided by the square of the speed of light. The body behaves, for every purpose that mass is measured by, as though it lost that much of it.
Why the slow-speed limit and not the exact factor
At a finite speed you get a coefficient that depends on the speed, which is a proxy and not an identification: you would be reading a mass off a quantity that still remembers how fast you happened to be gliding. The identification is made in the limit as the speed goes to zero, which is where the comparison with one half m v squared is exact. Running the instrument at zero speed instead gives zero on both sides and settles nothing, which is a different thing from taking the limit.
First write the result as the paper prints it, in its own letters.
A body gives off an energy L as light. By how much does its mass fall? Write it using L and V, the paper’s letters for the energy given off and the speed of light.
Answers are compared for L from 1 to 1 × 1010 and V from 2.99 × 108 to 3 × 108.
Show a worked explanation
The paper's last page reads the coefficient off the comparison with the energy of motion: the mass falls by L/V², the energy given off divided by the square of the speed of light, which is written c today. With L in joules and V in metres per second, L/V² comes out in kilograms. L/V is not a mass but a momentum, and L·V² is not a mass either; the square of the speed goes underneath.
Now put a number to it. The coefficient is small in the units of everyday things, and working one case shows how small.
A sealed box holds a lamp and the battery that powers it. For a year, about 3.156 × 10⁷ seconds, it gives off 100 watts as light and heat. By how much has the box’s mass fallen? Give it in kilograms or grams.
Show a worked explanation
The energy given off is the power times the time: 100 W × 3.156 × 10⁷ s = 3.156 × 10⁹ J. The paper’s result says the mass falls by that energy divided by the square of the speed of light. With the speed of light as the SI defines it, 299 792 458 m/s, its square is about 8.988 × 10¹⁶ m²/s², so the mass falls by 3.156 × 10⁹ / 8.988 × 10¹⁶, about 3.51 × 10⁻⁸ kg: some 35 micrograms. For comparison, the paper’s closing paragraph suggests that the theory might be tested on bodies whose energy content varies a great deal, such as radium salts.
The year is given to four figures, so an answer within 1 percent is the same answer.
Two accounts of the same bookkeeping: does a fictitious fluid carried by the light save the centre of mass, or did the body's own inertia change?
The branches vary which theoretical principle is taken as a starting postulate.
Give the radiation a fictitious fluid
Historical proponent: Henri Poincaré, 1900
Keep the centre of mass moving uniformly by treating the radiation's energy as a fluid that carries mass: its energy divided by the square of the speed of light. The question is the field's bookkeeping, not the emitting body's inertia.
Wherever the question is how the centre of mass of a body and its radiation moves. Within that scope it gives the same numbers as the paper's route.
Deductive steps (3)
- Let a body give off a pulse of radiation. It recoils, and unless the travelling radiation is counted as carrying mass, the centre of mass of the body and the radiation together moves.
- Give the radiation a mass equal to its energy divided by the square of the speed of light, and the centre of mass moves uniformly again.
- Now ask what the body lost. The fluid accounts for the radiation. It does not say what happened to the body, and that is the question this route answers.
Within its scope the fluid gives the same numbers, and nothing on the 1904 shelf refutes it. It says something different: it gives mass to the light and leaves the body's inertia alone, where the paper's route says the body's inertia changed.
Observable class scope: The centre-of-mass bookkeeping of emission and absorption treated in Poincaré's 1900 paper.
Energy has inertia
The energy the body gave off was part of its inertia, so its mass fell by that energy divided by the square of the speed of light.
Under the two-ledger argument's premises: the light-energy transformation, energy conservation in both frames, and an offset between the ledgers that the emission does not change.
Deductive steps (2)
- Read the slow-speed result as a statement about the body: its energy of motion changed as though its mass had fallen by L/V².
- Generalise, as the paper does in one sentence, from light to any energy leaving the body: the mass of a body is a measure of its energy content.
This is the paper's conclusion. Its last step, from light to any form of energy, is a stated inference and not a further derivation.
How far does the claim reach: to the energy of a charged body's field, or to energy of every kind?
The branches vary which theoretical principle is taken as a starting postulate.
Only the field's energy has inertia
Historical proponent: J. J. Thomson, 1881
A charged body's field adds to its inertia, so inertia belongs to the energy of the electromagnetic field. The light in this argument is field energy, so its leaving lowers the inertia, and nothing follows about energy of other kinds.
For charged bodies and their fields, where the added inertia can be calculated. How much it adds depends on the model of the charge.
Deductive steps (3)
- Start from Thomson's result: a moving charged sphere carries a magnetic field whose energy makes it harder to accelerate.
- Read the paper's argument the same way. The energy that leaves is light, which is field energy, so the lost inertia can be booked to the field.
- Ask what would tell this apart from the paper's claim: a body whose energy of another kind changes by enough to weigh.
On the evidence of 1904 this branch is neither refuted nor confirmed. It is a narrower claim than the paper's, and the measurement that bears on it came twenty-seven years later.
Why 1904 evidence is insufficient: The 1904 shelf carries no measurement of a body whose non-electromagnetic energy changes by enough to weigh, so it cannot separate a claim about field energy from a claim about energy as such.
Later resolving measurement: Cockcroft and Walton's lithium disintegration(1932)
Energy of every kind has inertia
The inertia of a body depends on its energy content, whatever form that energy takes.
Wherever the paper's premises hold. Its last step, from light to energy of any form, is the one sentence in the paper that goes beyond the calculation.
Deductive steps (2)
- Find where the argument used the fact that the energy left as light: only in the rule for how the light's energy changes between frames. What it concluded is about the body's energy of motion.
- Conclude, as the paper does, that the mass of a body is a measure of its energy content.
This is the paper's statement, and it is a stated inference: the paper calls it evident that nothing depends on the energy leaving as radiation.
06 / Check it against the world
Where the paper says to look
What the result says depends on what you weigh. In the ledger below one joule of light leaves a body: draw the boundary around the body alone, around the light, or around both, and read the mass that goes with it. Its cards put the same rule to radium, the Sun, coal, a candle and a year of a light bulb.
System boundary energy ledger
The boundary ledger, for the check
Static worked example
CurrentThese numbers match the current settings.
Model note
- Primary outputs energyChange, massChange, radiationEnergyChange, radiationMassChange, systemEnergyChange, systemMassChange: Host calculation (massEnergy.boundaryLedger). Owner massEnergy.boundaryLedger.
- Primary output invariantMass: Host calculation (massEnergy.fourMomentum). Owner massEnergy.fourMomentum.
- Accepted input revision 1.
- Snapshot version 1.
- Not modeled: gravitational weighing; wall stresses, or external work beyond declared inputs; nuclear and chemical mechanisms beyond cited energies; heat losses not declared; neutrino and solar-wind mass loss; the practical measurability of tiny mass changes; the 1905 argument's premises (inherited, not re-derived); non-inertial or accelerated frames.
Predict before the numbers
A sealed box holds a battery-powered lamp and a mirror. When the lamp lights up inside, does the box's total mass change?
The result appears when you choose, say you have one in mind, or skip.
Experiment settings seven cited energy sources, notation
Worked example: Radium-226 alpha decay, with the boundary around the body alone: the radiation escapes, and the energy figure is 4.871 MeV.
Where the boundary is drawn
Inside the boundary: the body alone. The radiation escapes.
Energy and mass inside the boundary
- Inside the boundary
- The body alone
- Energy change ΔE
- −1 J
- Mass change Δm
- −1.1127 × 10−17 kg
- Case study
- Radium-226 alpha decay
- Mass change
- 0.0052292 u/decay (5.229 mg/mol)
Case study facts: Radium-226 alpha decay
Citation: NuDat 3.0 / Evaluated Nuclear Structure Data File (ENSDF), Brookhaven National Laboratory (226Ra Q-alpha = 4.871 MeV).
- 1. System before:
- Radium-226 nucleus at rest
- 2. System after:
- Radon-222 nucleus and alpha particle after heat emission
- 3. Matter crosses boundary:
- No (Closed system: The radon-222 nucleus and the alpha particle both stay inside the boundary.)
- 4. Radiation disposition:
- escapes (The decay energy leaves as heat.)
- 5. Reference frame:
- Rest frame of parent nucleus
- 6. Energy figure:
- 4.871 MeV (energy released per decay)
Show the reference code & kernel bindings
Reference evaluator: src/physics/reference/massEnergy.ts
// evaluateBoundaryLedger
const bodyDeltaM = -emittedEnergy / (c * c);
const sysDeltaM = disposition === "retained" ? inputEnergy / (c * c) : 0;
// evaluateFourMomentum
const mSquared = (totalEnergy / c)^2 - p^2;
const invariantMass = Math.sqrt(Math.max(0, mSquared));Energy that leaves a body takes mass with it. Draw the boundary around the body alone and it gets lighter; draw it around the body and the light it gave off, and nothing is lost.
The mass–energy paper concludes that a body giving off energy L loses mass L/V², that it does not matter that the energy leaves as radiation, and that, if the theory is right, radiation carries inertia from the body that emits it to the body that absorbs it. The instrument keeps the accounting honest by making you choose where the boundary goes. With 1 J emitted and the boundary around the body alone, the body's energy falls by 1 J and its mass by 1.11 × 10−17 kg. Around the radiation alone, 1 J arrives, and the lab gives it no rest mass in the 1905 account, saying so rather than inventing one. Around the body and its light together, an isolated system, nothing changes. In the four-momentum lens, a modern addition, two opposite pulses of total energy 1 J have an invariant mass of 1.11 × 10−17 kg, which is where the body's lost mass went. The energy-source cards apply ΔE/c² to cited modern transfers: a radium-226 alpha decay of 4.871 MeV changes mass by 8.68 × 10−30 kg; the Sun's 3.828 × 1026 W takes away 4.26 × 109 kg each second; a kilogram of coal burned at 30 MJ, 3.34 × 10−10 kg; a candle for an hour, 3.20 × 10−12 kg; a 100 W bulb for a year, 3.51 × 10−8 kg. In the 1906 photon-in-a-box mode (credit: Poincaré 1900), a pulse crossing a floating box shows that the centre of mass stays put only if the light is given the mass E/c².
The rule is Δm = ΔE/c², with c² = (2.998 × 108)² = 8.988 × 1016 m²/s², so 1 J corresponds to 1/(8.988 × 1016) = 1.11 × 10−17 kg. The sign follows the boundary. A body that emits 1 J has 1 J less inside its boundary, so its mass falls by 1.11 × 10−17 kg. Move the boundary around the body and its light, and the energy inside does not change, so neither does the mass: the joule left the body but not the system. Now the cards. The radium decay releases 4.871 × 106 × 1.602 × 10−19 = 7.80 × 10−13 J, which divided by c² is 8.68 × 10−30 kg, about 2 parts in 100 000 of the radium atom's mass. The Sun radiates 3.828 × 1026 J each second, and dividing by c² gives 4.26 × 109 kg, some four million tonnes a second. The bulb uses 100 W × 31 557 600 s = 3.156 × 109 J in a year, which is 3.51 × 10−8 kg, about 35 micrograms. Now the 1906 box argument. A box of mass 1 kg and length 1 m floats free. A pulse of 1 J leaves one end carrying momentum E/c = 1/(2.998 × 108) = 3.34 × 10−9 kg·m/s, so the box recoils the other way at 3.34 × 10−9 m/s. The pulse takes l/c = 3.34 × 10−9 s to cross, and in that time the box moves back 3.34 × 10−9 × 3.34 × 10−9 = 1.11 × 10−17 m, which is El/(Mc²). When the pulse is absorbed at the far end, the box stops. Nothing outside acted on the box, so the centre of mass of the whole system cannot have moved. The box's backward step is balanced only if the pulse carried a mass m across the length l with ml = M × 1.11 × 10−17 m, so m = 1.11 × 10−17 kg = E/c². Switch that assignment off and the lab shows the centre of mass moving by 1.11 × 10−17 m, which an isolated system cannot do.
The 1905 conclusions are conditional. The paper says it is not excluded that bodies whose energy content varies greatly, radium salts for instance, could test the theory, and that if the theory corresponds to the facts, radiation carries inertia between the emitting and absorbing bodies. It gives no rest mass to free radiation; the invariant mass of a system of light belongs to the later four-momentum language. The box is Einstein's 1906 argument (credit: Poincaré 1900): his paper credits Poincaré's remark of 1900 that electromagnetic energy behaves like a fluid with inertia. The energy-source values are modern and cited on each card; none was measured in 1905, and the mass changes of chemical and everyday transfers are far too small to weigh.
The paper ends with a number and a suggestion. A change of energy L changes the mass by L/9·10²⁰, with the energy in erg and the mass in grams, and bodies whose energy content changes a great deal, radium salts for instance, might test it. The ledger below lets one joule of light leave a body. Move its boundary and read the mass that goes with it.
What Einstein printed on the paper's last page
the mass changes by L/9·10²⁰, with the energy in erg and the mass in grams
From the boundary ledger above, as it now stands
With the boundary drawn around the body alone:
- Change of energy inside the boundary
- −1 J, or −1 × 10⁷ erg
- Change of mass inside the boundary
- −1.11 × 10⁻¹⁷ kg, or −1.11 × 10⁻¹⁴ g
An ideal model computed here, with today’s speed of light, for the one joule the ledger lets leave. Divide the energy in erg by 9·1020 and set it beside the mass in grams. Move the boundary or choose a setup in the ledger, and these numbers follow.
Later evidence, not on the 1904 shelf
Published, 1932-07Cockcroft and Walton break lithium nuclei apart with fast protons, producing pairs of alpha particles, and compare the energy the alpha particles carry with the loss of mass computed from the atomic masses. The two agree within the uncertainty of the masses then known.
Later confirmation
Cockcroft and Walton break lithium nuclei apart with fast protons, producing pairs of alpha particles, and compare the energy the alpha particles carry with the loss of mass computed from the atomic masses. The two agree within the uncertainty of the masses then known.
Historical context
Later empirical or theoretical confirmation developed after 1905.
Available by
Published, 1932-07
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- Experiments with high velocity positive ions. II. The disintegration of elements by high velocity protons Proc. R. Soc. A 137, 229 (1932)
Source verification pending library scan inspection.
Published 1933Bainbridge measures the masses of the nuclei in the lithium disintegration with a mass spectrograph, and sets the mass that disappears beside the energy the alpha particles carry away.
Later confirmation
Bainbridge measures the masses of the nuclei in the lithium disintegration with a mass spectrograph, and sets the mass that disappears beside the energy the alpha particles carry away.
Historical context
Later empirical or theoretical confirmation developed after 1905.
Available by
Published 1933
What the paper itself cites or asserts
Not yet recorded for this card.
Where this site uses it
Primary evidence and sources
- The Equivalence of Mass and Energy Phys. Rev. 44, 123 (1933)
Source verification pending library scan inspection.
The paper says only that a test is not ruled out for bodies whose energy content changes a great deal, and names radium salts. The cards above are later tests of another kind: in 1932 Cockcroft and Walton set the energy released when lithium nuclei break apart beside the mass lost, and in 1933 Bainbridge weighed those nuclei with a mass spectrograph. They test the result, and they were on no one’s shelf when the paper was written.
07 / Try it yourself
Four pieces of the argument to work by hand
First the step that makes the direction of the light irrelevant. Any correct form is accepted: the checker compares your expression with the answer at sample values of L, v and V, not by matching text.
In the moving frame one pulse carries (L/2)(1 − (v/V)cos φ)/√(1 − (v/V)²) and the other (L/2)(1 + (v/V)cos φ)/√(1 − (v/V)²). Add them. Write the total using only L, v and V.
Answers are compared for L from 1 to 1 × 1010, v from 0 to 2.8 × 108 and V from 2.99 × 108 to 3 × 108.
Show a worked explanation
Both pulses share the factor (L/2)/√(1 − (v/V)²). Inside the brackets −(v/V)cos φ and +(v/V)cos φ cancel, and 1 + 1 leaves 2, so the total is L/√(1 − (v/V)²) whatever the angle φ. One pulse gains what the other loses to the angle, and only the speed remains. At v = 0.6V the square root is 0.8, so the pair carries 1.25 L, against the L the body gave off in its own frame.
Next the 1906 route, the side door below. The number is small enough that the sign is the only thing you could see.
Einstein’s argument of 1906: a closed box of mass 1 kg and length 1 m, floating free, sends a pulse of 1 J of light from one end to the other. The light carries momentum, so the box recoils until the light arrives. How far has the box moved? Give its displacement along the direction the light travels, negative if it moves back.
Show a worked explanation
The pulse carries momentum E/c, so the box recoils at E/(Mc) = 1/(1 × 2.998 × 10⁸), about 3.34 × 10⁻⁹ m/s. It moves for as long as the light takes to cross, ℓ/c, also about 3.34 × 10⁻⁹ s. The displacement is the product, Eℓ/(Mc²) = 1.11 × 10⁻¹⁷ m, backwards, so −1.11 × 10⁻¹⁷ m along the light. A closed box’s centre of mass cannot move on its own, so the light must have carried a mass E/c² from one end to the other. The argument credits Poincaré’s fluid of 1900, and it treats the box as rigid, its recoil as slow and the crossing time as ℓ/c.
The inputs are round numbers and the speed of light is exact, so an answer within 1 percent is the same answer.
Then the step that decides where the mass is read: at a finite speed the quotient is not yet the mass.
At 0.6 of the speed of light, γ = 1.25, so a body that gives off L = 1 J of light loses exactly 0.25 J of energy of motion. Read a mass off that drop as you would off one half of mass times speed squared: take twice the drop and divide by v². What do you get, in kilograms?
Show a worked explanation
Twice the drop is 0.5 J, and v² = (0.6 × 2.998 × 10⁸ m/s)² = 3.236 × 10¹⁶ m²/s², so the quotient is 0.5 / (3.236 × 10¹⁶), about 1.545 × 10⁻¹⁷ kg. That is 1.389 times L/c², which is 1.113 × 10⁻¹⁷ kg. The quotient still depends on the speed you chose: as the speed goes to zero it comes down to L/c², and only there does one half of mass times speed squared describe the energy of motion. The paper reads the mass off that limit, not off this quotient at any finite speed.
0.6 and 0.25 are exact and the speed of light is exact, so an answer within half a percent is the same answer.
Last, the choice the whole argument rests on, in your own words.
Why does the argument have the body give off two equal pulses in opposite directions, rather than one?
What you write stays in this box. Nothing on the page reads it, marks it or sends it anywhere, and it is gone when you leave.
Compare with a worked explanation
Only a person can judge an explanation, and here that person is you. Read yours against each of these in turn:
- With two equal pulses in opposite directions the body does not recoil, so its speed is the same before and after.
- With the speed unchanged, a change in its energy of motion can only come from a change in its mass.
- Seen from the moving frame the two pulses carry different energies, but their total does not depend on the direction they leave in.
- The symmetry is a choice made to isolate one unknown, not a claim about how bodies give off light.
One pulse would push the body the other way, and afterwards some of the change in its energy of motion would be a change of speed. Two equal pulses in opposite directions push equally both ways, so the body stays at rest in its own frame and keeps the same speed in the moving one. Then the only thing left that can account for the drop in its energy of motion is its mass. The moving observer measures one pulse with more energy than the other, but the sum does not depend on the direction of emission, so the argument need not say which way the light went.
Predict, change one thing, then explain
Predict first. A body gives off one joule of light. Does its mass fall by about a gram, about a microgram, or by far less than either?
Open the boundary ledger with one joule emitted and the boundary around the body alone, and read the change in mass. Then move the boundary around the body and its light together, and read it again.
Explain both readings. Say what you divide the energy by and why the first answer is so small, and why the second is zero.
Where this enters the paper
The paper is three pages and its title is a question rather than a claim. It sets out the two accounts, performs the subtraction, takes the slow-speed limit, and states the conclusion in a single sentence. Its German text is on this site, not yet reviewed; the English translation is not written yet.
The two accounts: the paper writes the body's energy before and after the emission in two frames, and uses the June paper's rule for the energy of the light in each.
Taking the accounts from each other removes the body's unknown energy and leaves its energy of motion, with the premise about the offset stated.
The paper's last page takes the slow-speed limit, sets it beside one half m v squared, and states the conclusion in a sentence.
Multiple routes, one arrival point
All doors arrive at the same result: the mass falls by L/V²
The paper's argument: two accounts of one emission
Write the body's energy in two frames, take one account from the other, and read the slow-speed limit.
Arrives at: the mass falls by L/V²
The 1906 box, for programmers
Einstein's argument of 1906, crediting Poincaré's fluid of 1900: a pulse crosses a floating box, and the centre of mass stays put only if the light carries the mass E/c². It comes after the paper, and says so.
Arrives at: the mass falls by L/V²
Two accounting sheets and one subtraction
No algebra: keep one sheet for an observer at rest and one for an observer gliding past, and take one from the other.
Arrives at: the mass falls by L/V²