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Use the supplied atomic masses consistently. Their mass defect per four hydrogen atoms is $4(1.0078)-4.0026=0.0286$ atomic mass units. The conversion efficiency isThe atomic-mass bookkeeping includes the associated positron-annihilation energy; an exact photon-heating budget also subtracts energy carried away by neutrinos. With the stated ten-percent fuel fraction and constant present solar luminosity, the main sequence lifetime estimate isThe much longer timescale explains why stellar nuclear fusion can power the Sun throughout its long main-sequence history.

The radiation registered in the stated solar luminosity includes two Positron annihilations but excludes the two escaping neutrinos. Thus the visible energy per completed helium-producing chain isThe signs in this energy ledger matter: adding the neutrino energy would overestimate the energy available to sustain the measured radiation. Using $1\mathrm{MeV}=1.602176634\times 10^{-13}$ J, the chain rate and hydrogen-consumption rate areWith a year taken as $365.25$ days, the stated elapsed time is $1.4516496\times 10^{17}$ s. Consequently,At the same fixed luminosity, the remaining time would beOnly about $5.93\%$ of the stipulated initial reservoir has been consumed under these assumptions. This is a calculation for an entirely accessible hydrogen reservoir with constant luminosity. It is not a prediction of the Sun's remaining main-sequence lifetime: only part of the hydrogen participates in core burning, and stellar structure and luminosity evolve.

The solar mass, written $M_{\odot }$, is a mass unit based on the Sun, approximately $1.99\times 10^{30}\mathrm{kg}$. Expressing stellar masses in this unit makes comparisons immediate: a $2M_{\odot }$ star has roughly twice the Sun's mass. It does not follow that it has twice the solar luminosity, because the mass-luminosity relation is nonlinear.

Orbital observations constrain the gravitational parameter $GM$ more directly than mass in kilograms. The nominal solar mass parameter supplies an exact conventional conversion for such comparisons; converting it to kilograms additionally requires the measured gravitational constant. A nominal constant is therefore distinct from claiming that the physical Sun's changing mass is known exactly.^[ref]

The Sun is the star at the centre of the Solar system and a nearby example of a main-sequence star. Its effective temperature is approximately $5772\mathrm{K}$, its stellar radius about $6.96\times 10^8\mathrm{m}$, and its luminosity about $3.83\times 10^{26}\mathrm{W}$. These describe different aspects of the same object: radiating area and effective temperature combine through the Stefan–Boltzmann law to give solar luminosity.^[ref]

Core hydrogen burning supplies the long-term energy budget. Energy reaches the photosphere through radiative transfer and convection, while solar neutrino detection samples the nuclear processes more directly. Resolved solar granulation and starspots reveal that the visible disc is structured and time-dependent. Comparing these accessible phenomena with unresolved stars helps calibrate wider stellar astrophysics.