# Stellar types

### Placed mass-sequence evaluations · taxonomic join modelled · doctrine unedited

**Date:** 2026-10-24
**Status:** **RECORD** · public page `/cosmology/stellar-types` · **[M packaging]** under §0bn1143
**Parent:** measey.com `documents/a_geom_stellar_types_micro_macro_bridge_grok_placement_record.md`

> **The printed clocks, the Hale product, the retention rectangle, the iron-peak maximum of the inserted \(\kappa_C\), the nuclear saturation density, the Euclidean neutron-star ball, and the electron-scale length \(\ell_0\) are direct evaluations. The two-coordinate taxonomy stays modelled. Doctrine v1.1.13 stays unedited. No ledger row. No token.**

At \(\rho_c=1.67\times 10^6\,\mathrm{kg\,m^{-3}}\) and \(\mu_e=1.17647\) the cold Fermi pressure is \(1.776\times 10^{17}\,\mathrm{Pa}\). With \(\mu=1/1.62\) that pressure matches \(7.96\times 10^6\,\mathrm{K}\). The mass-lifetime prints are \(3.16\times 10^{12}\,\mathrm{yr}\) at \(0.10\,M_\odot\) and \(1.38\times 10^{11}\,\mathrm{yr}\) at \(0.35\,M_\odot\). The inductive floor at \(2000\,\mathrm{H}\) and \(10^{12}\,\mathrm{A}\) is \(1.00\times 10^{27}\,\mathrm{J}\). The unrounded drift inverse is \(8.799\times 10^9\).

\(Z^{1/3}\) on \([0.013,\,0.020]\) prints \([0.235,\,0.271]\). \(\pi\sqrt{L_m C_{\mathrm{DL}}}=11.00366\,\mathrm{yr}\) and the Hale period prints \(22.01\,\mathrm{yr}\). Shedding of the file specific-angular-momentum ratio is \(99.999518\%\). Triple-\(\alpha\) prints \(7.275\,\mathrm{MeV}\) and \(5.85\times 10^{13}\,\mathrm{J\,kg^{-1}}\). The \(\mu_e=2\) Chandrasekhar root is \(1.456\,M_\odot\).

\(\nabla_{\mathrm{ad}}=0.4\) for \(\gamma=5/3\). At \(R=2.087\times 10^9\,\mathrm{m}\) and \(\sigma=10^6\,\mathrm{S\,m^{-1}}\) the fossil-loop decay time is \(1.75732\times 10^{10}\,\mathrm{yr}\). Retention across the conductivity window prints from \(81.3\%\) to \(99.997\%\), and stays above \(90\%\) for \(M\ge 2\,M_\odot\).

The inserted \(\kappa_C=0.530\,\mathrm{MeV}\) has its maximum at \(A^*=59.864\). \(\rho_{\mathrm{nuc}}c^2\) prints \(0.15146\,\mathrm{GeV\,fm^{-3}}\) and the mint ratio prints \(13.205\). A \(1.4\,M_\odot\) Euclidean ball of radius \(12\,\mathrm{km}\) has mean density \(3.85\times 10^{17}\,\mathrm{kg\,m^{-3}}\). At period \(0.0335\,\mathrm{s}\) and auxiliary \(10^8\,\mathrm{T}\) the unipolar voltage is \(1.35042\times 10^{18}\,\mathrm{V}\). \(\ell_0=3.29875\times 10^{-14}\,\mathrm{m}\). \(GM/c^2\) at \(2.5\,M_\odot\) is \(3.69\times 10^3\,\mathrm{m}\).

Fence F4 stays intact. \(\mathbf{B}\) stays auxiliary. Finding GW2 stays [M]. Baseline \(H_0=68.973\) stays [P].