Past exam of the short options paper of the physics Prelims of the University of Oxford / 2021 / S02 / 1

The astronomical magnitude convention is $m_1-m_2=-2.5{\log }_{10}(F_1/F_2)$, with both fluxes measured through the same photometric passband. A five-unit magnitude difference therefore corresponds toThe brighter endpoint has one hundred times the visual flux of the fainter endpoint. Absolute fluxes require a magnitude zero point, which is not given.

TODO: numerical endpoints require the unreadable source diagram. Let ${\ell }_{V,\max }$ and ${\ell }_{V,\min }$ be the maximum and minimum main sequence visual luminosities, in units of the Sun's visual luminosity. At a distance $d$, the inverse-square law and the magnitude difference relation giveThus, using $m_{V,\odot }=-26.77$,At the naked-eye detection threshold $m_V=6$, the greatest distances for the intrinsically brightest and faintest main sequence stars would respectively beThe historical $m_V=1$ endpoint is a brightness reference, not the visibility threshold: if that endpoint were intended instead, the corresponding coefficient would be $1.736$ rather than $17.36$.

The source Hertzsprung-Russell diagram has lost the stellar loci and luminosity scale except for a surviving top tick; neither endpoint can be read reliably. If its scale was bolometric luminosity rather than visual luminosity, bolometric corrections would also be needed, especially for very hot and very cool stars. Equating the two luminosity ratios would then be an explicitly approximate assumption. These missing data are not replaced by invented endpoint values. Interstellar extinction is neglected in the displayed distance relation.

For spherical hydrostatic equilibrium, the stellar structure equations includeEliminate $\rho$ to obtain $dP/dm=-Gm/(4\pi r^4)$. Since $r(m)<R_{\odot }$ through the interior, integration givesWith negligible surface pressure, this provesThis is a conservative lower bound; concentrating mass near the centre increases the required pressure.

For the temperature inference assume predominantly ideal gas support, a nearly fully ionized hydrogen–helium mixture with mean molecular weight $\mu \simeq 0.61$, and the hottest region at the centre. A rigorous scale estimate follows from the stellar virial theorem, rather than substituting the mean mass density for the unknown central mass density. With negligible surface pressure,The ideal gas law gives $\int PdV=k_B\int Tdm/(\mu m_p)$. The mass-weighted mean temperature consequently obeysThis establishes several million kelvin under the stated physical assumptions. The central pressure inequality alone does not give a central temperature bound without an equation of state and information about mass density or an integrated argument.

TODO: the plotted location of Procyon B is missing from the damaged source diagram. The Stefan–Boltzmann law would determine the stellar radius from its effective temperature and bolometric luminosity:A visual luminosity alone must first be converted with the appropriate bolometric correction. Procyon B is a white dwarf, so its small stellar radius and hot surface place it below the main sequence, rather than among giant stars or supergiants. This classification does not supply the missing numerical coordinates. A source-based numerical stellar radius cannot be claimed from the surviving image.^[ref]