The Star That Hid Behind Its Own Ring ✛

Original: "Supernova 1987A was a "failed supernova" twenty thousand years before its jet-driven explosion"
· Noam Soker
arXiv:2608.24801v1 · 2026-08-25 · CC BY 4.0 · 1 min
Twenty thousand years before it exploded, a star wrapped itself in a gas ring and became nearly invisible to sideways observers.

The star that later exploded as supernova 1987A put on a gas ring twenty thousand years before the blast. Not one ring — three. The star's light, passing through the rings, scattered like a flashlight beam in fog. For an observer positioned exactly in the plane of the equatorial ring, the star nearly vanished: its brightness dropped to five percent. Today, such an event would be called a 'failed supernova'—a star that dimmed but didn't explode. But it was simply hiding behind its own ring.

The equatorial ring is expanding at 10.3 kilometers per second — thirty times slower than the ISS orbits. Over twenty thousand years, it has swelled to a radius a hundred times the distance from the Sun to Earth.

After a few thousand years, the ring became transparent, and the star returned to normal brightness. But astronomers searching for black holes born without a bang might mistake such a temporary dimming for a real collapse. The work shows that some 'failed supernovae' may simply be stars playing hide-and-seek. This matters for statistics: if we confuse one with the other, we miscount how often massive stars die without exploding.

The equatorial ring of Supernova 1987A is expanding at 10.3 km/s—30 times slower than the International Space Station's orbital speed. Over 20,000 years, it has inflated to a radius of about 1.5×$10^{18}$ cm, roughly 100 times the distance from the Sun to Earth.

\frac{L_e}{L_I} \approx 0.003 \left(\frac{\sin\alpha_e}{\sin 15^\circ}\right)^{5/2} \left(\frac{\tau_{T,z}}{\tau_{T,r}}\right)^{3/2} \left(\frac{M_{ring,e}}{0.1M_\odot}\right)^{-1/2} \left(\frac{v_e}{10\,\text{км/с}}\right) \left(\frac{t+\Delta t_e}{33\,\text{лет}}\right)^{1/2} \left(\frac{t}{30\,\text{лет}}\right)^{1/2}
Shows that the equatorial ring almost completely hides the star's light for an observer in its plane
j_e(1.5) = \omega(1.5) R^2(1.5) = 5\times10^{15} \left(\frac{\eta_s}{0.3}\right) \left(\frac{M_{core}}{8M_\odot}\right)^{1/2} \left(\frac{R_T}{3R_\odot}\right)^{-3/2} \left(\frac{R(1.5)}{0.1R_\odot}\right)^2 \,\text{см}^2/\text{с}
Estimate of the core rotation imparted by the companion's disruption; compared to the threshold for accretion disk formation
j_{dir} = v_{dir} r = \omega r^2 \sin\beta \simeq j_e(1.5) \sin\beta
Shows that late accretion from inclined directions can provide angular momentum with an axis tilted relative to the original rotation axis
Scientists
Subrahmanyan ChandrasekharEnrico FermiAugustin-Louis CauchyChristiaan HuygensEmmy NoetherIsaac Newton
Concepts
supernova 1987a progenitor m87 cassiopeia a ejecta supernova jets kilonova interstellar object ejection neutron star binary formation supernova interstellar object magnetorotational supernova helium flash