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SCIENCE · INVESTIGATE AND EXPLAIN

Calculate the small rest-mass difference

Use isotope-specific atomic masses to distinguish processed fuel from converted rest mass.

Learning outcome: Calculate total released energy with a consistent electron inventory.

Starting recap

Use neutral hydrogen and neutral helium together; most rest mass remains in helium.

All lessons are open directly. Your saved experiments remain when you leave and return.

Try

The mass difference is 0.02869687479 u, releasing about 26.73 MeV.

Open the experiment

Predict

Does doubling the reservoir double energy per completed chain?

Experiment

Compute the four-atom mass difference, then compare 10 and 20 percent reservoirs at fixed demand.

Trace fusion energy into a conditional fuel budget

Worked teaching model · synthetic values · Synthetic total mass 2.0×10³⁰ kg; the chosen accessible region has fixed hydrogen-1 mass fraction 0.70. Neutral-atom mass differences include electron bookkeeping. A restricted pp-I mean assigns 0.530 MeV per completion to escaping neutrinos. Remaining energy is assumed to support the specified average photon demand. Rates are required, not achieved; zero fuel supports zero duration. No actual stellar lifetime, reaction-rate, structure, mixing or evolution prediction is made.

Reset keeps your prediction, captures and practice history.

Build helium from hydrogen, then ask how much energy a specified fuel inventory could supply. The two controls change the hypothetical inventory and average photon demand; they do not change nuclear masses or calculate an actual stellar reaction rate.

pp-I worked mechanism · p = proton; n = neutron; e⁺ = positron; νe = neutrinoTwice: p + p → ²H (1p + 1n) + e⁺ + νeTwo weak conversions produce two neutrons and two escaping neutrinos.Twice: ²H + p → ³He (2p + 1n) + γγ denotes a gamma photon. Both intermediate helium-3 nuclei are used next.Once: ³He + ³He → ⁴He (2p + 2n) + p + pSix protons entered the preceding stages; two return. Net consumption: four.Also twice: e⁺ + e⁻ → photons. Surrounding electrons supply the e⁻.Cancel intermediates on paper. This chain is not one four-proton collision.Reaction count does not determine a rate; temperature and density are not modeled.

For the energy ledger, use four neutral hydrogen-1 atoms and one neutral helium-4 atom. This is consistent rest-mass bookkeeping for the net process, not neutral atoms inside the hot core. Four initial electrons account for two in the final atom and two annihilating with positrons. Do not add annihilation rest energy again. Plasma ionization and tiny neutrino rest-mass corrections are omitted.

Rest masses · common scale 0–4.1 u4 neutral H-11 neutral He-40 u4.1 uDifference 0.02869687 u ≈ 0.712% of initial fuel rest mass.Released energy · separate scale 0–27 MeV0 MeV27 MeVDeposited: 26.201 MeV; neutrinos: 0.530 MeV mean.Total: 26.731 MeV. Mass-energy is conserved.

The gold energy segment is the stipulated mean carried away by two pp neutrinos, not a fixed energy for each event or a universal average over all fusion branches. Deposited energy can thermalize before escaping as photons. Nearly all initial fuel rest mass remains in helium.

Hypothetical available inventory and required demand rates
QuantitySelected demandSame inventory, 1 nominal solar luminosity
Accessible region kg2.00000e+292.00000e+29
Hydrogen inventory kg1.40000e+291.40000e+29
Possible net completions2.09138e+552.09138e+55
Helium product rest mass kg1.39003e+291.39003e+29
Total released budget J8.95692e+438.95692e+43
Neutrino budget J1.77591e+421.77591e+42
Deposited budget J8.77933e+438.77933e+43
Prescribed photon demand W3.82800e+263.82800e+26
Required completions per second9.11894e+379.11894e+37
Required hydrogen processing kg/s6.10434e+116.10434e+11
Required rest-mass conversion kg/s4.34538e+94.34538e+9
Implied neutrino power at required rate W7.74338e+247.74338e+24
Conditional support duration Gyr7.267517.26751
Compare independent reservoirs · NOT a stellar time historyConditional support duration (Gyr) · solid/circle selected; dashed/square reference030609012015005101520Available core region (% of synthetic total mass)Hydrogen fraction fixed at 0.70. Long budget ≠ a physically predicted stellar lifetime.

Selected support budget: 7.26751 Gyr; same inventory at the reference demand: 7.26751 Gyr. The two curves coincide because their demands are equal. Each curve compares separate inventories; it does not show a core expanding over time.

Connect fuel, mass difference and power

Let q be the selected region percentage divided by 100. Available hydrogen mass is Mfuel = 0.70 × q × 2.0 × 10³⁰ kg. Count possible net completions as N = Mfuel / (4mH u), with mH = 1.00782503223 and u = 1.66053906892 × 10⁻²⁷ kg. The selected isotope mass differs from a natural-isotope average.

Mass defect per completion is Δm = (4mH − mHe)u, with mHe = 4.00260325413. Released energy is Qtotal = Δm c²; c = 299792458 m/s. Subtract the stipulated mean neutrino energy once: Qdeposit = Qtotal − Qν. One MeV = 1.602176634 × 10⁻¹³ J. Total deposited budget is N Qdeposit.

Divide that energy budget by prescribed average photon luminosity Lγ to obtain a duration in seconds. Divide by 31557600 and one billion to express Gyr. A required completion rate Lγ/Qdeposit is distinct from the amount of fuel. At 10% region and one nominal solar luminosity, 1.40 × 10²⁹ kg of hydrogen supplies about 8.77933 × 10⁴³ J deposited energy, a conditional 7.26751 Gyr budget.

This assumes all deposited energy supports the average photon demand, with no net storage change, mechanical loss or alternate source. Actual stellar temperature, density, mixing, luminosity history and other branches are absent. No present age, remaining lifetime or feasible reaction rate follows from this ratio.

Sources: isotope-specific masses from NIST hydrogen and helium; CODATA conversion constants; Berkeley pp-chain explanation; Fukugita and Peebles on neutrino energy; IAU nominal luminosity. Values use central reference constants without uncertainty propagation; displayed precision is not a new measurement.

Available hydrogen 1.4000e+29 kg; deposited budget 8.7793e+43 J; conditional support duration 7.2675 Gyr.

The prescribed photon demand would require 9.1189e+37 pp-I completions/s and 6.1043e+11 kg/s of hydrogen processing. These are demand-derived required rates, not actual output. The energy/power ratio is not a stellar lifetime prediction.

Captures preserve hypothetical fuel-region and photon-demand choices. Replaying calculates conditional energy budgets and required rates, not measured fusion output or actual stellar lifetimes.

Understand

Find the small difference before multiplying

Put four hydrogen atoms on one side of a paper balance and one helium atom on the other. The helium contains almost all the initial rest mass, but the totals are slightly different. The difference supplies released energy through E = Δmc². Here E is energy in joules, Δm is the reduction of rest mass in kilograms, and c is light speed in meters per second.

This is conservation of total mass-energy, not matter vanishing without an energy destination. It also does not mean that every kilogram of processed hydrogen becomes a kilogram’s worth of radiation. Most becomes helium rest mass. Your task is to distinguish the fuel processed from the much smaller rest mass converted.

Use isotope-specific neutral masses

The fixed reference uses NIST hydrogen-1 mass 1.00782503223 u and NIST helium-4 mass 4.00260325413 u. The symbol u is an atomic mass unit. These are selected isotope masses, not chemical atomic weights averaged over an isotope mixture.

Calculate four times the hydrogen mass: 4.03130012892 u. Subtract the helium mass to obtain 0.02869687479 u. Keep several digits during subtraction because the small difference is sensitive to premature rounding. Report the final energy with reasonable precision, rather than treating every calculator digit as experimental accuracy.

Both masses describe neutral atoms. Four initial electrons are accounted for by two final helium electrons and two electrons involved in annihilating the produced positrons. Do not add annihilation rest energy again. A calculation using neutral hydrogen and a bare helium nucleus would use incompatible electron inventories.

Convert units and interpret the result

The NIST CODATA constants table supplies u approximately 1.66053906892 × 10⁻²⁷ kg and c = 299792458 m/s. Multiplying the mass difference by u gives about 4.76523 × 10⁻²⁹ kg. Multiplying that by c² gives about 4.28277 × 10⁻¹² J per completed chain.

Nuclear energies are often written in megaelectronvolts: one MeV is one million electronvolts, and one electronvolt equals 1.602176634 × 10⁻¹⁹ J. The released total is therefore approximately 26.73 MeV. This total includes energy subsequently carried away by neutrinos; it is not all available for photon luminosity.

Now divide the mass difference by the initial four-atom mass. The fraction is approximately 0.0071185. Multiply by 100 to obtain about 0.712 percent. The denominator is initial fuel rest mass, not released energy. Write that denominator beside your percentage so you cannot confuse it with the fraction of released energy deposited in the star.

Compare a reaction with a reservoir

At 10 percent available core region, the hypothetical hydrogen inventory is 1.40 × 10²⁹ kg. Increase the region to 20 percent while keeping photon demand fixed. Predict unchanged per-chain mass defect and doubled total available energy. Use paired notebook captures and compare both rows of the ledger.

The tabulated masses and atomic mass constant have source uncertainties; this calculation uses their central values without uncertainty propagation. It omits plasma ionization corrections and tiny neutrino rest-mass corrections. Printed decimal places do not establish a confidence interval. The neutral-atom convention already includes atomic binding-energy contributions in those tabulated masses.

A useful cross-check is initial fuel mass equals final helium mass plus total released energy divided by c². Use total released energy here, including the neutrino channel. Substituting only deposited energy would leave part of the mass-energy accounting unexplained.

Transfer: two inconsistent corrections

A student uses the correct neutral atomic masses, calculates Δmc², and then adds two electron-rest-mass energies as an annihilation bonus. Another student instead replaces helium’s atomic mass with a bare alpha-particle mass while leaving hydrogen unchanged. Explain why neither is the same consistent calculation.

Check the fusion-mass transfer

The first calculation double-counts electron bookkeeping already included in the neutral-atom difference. The second changes the final electron inventory without changing the initial convention. Use the supplied neutral hydrogen-1 and helium-4 masses together; their difference gives approximately 26.73 MeV total. A fully nuclear convention could be constructed, but all electrons and positrons would have to be handled consistently.

Apply

After using the correct neutral atomic masses, should you add a separate positron-annihilation rest-energy bonus?

Public practice checks a specific claim. It does not establish independent mastery.

Distinguish per-chain energy, total energy and the initial-mass denominator.

Continue

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