SN 1987A: neutrinos from a collapsing core reach Earth
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Three underground detectors - Kamiokande-II in Japan, IMB in Ohio and Baksan in the Soviet Union - recorded a coincident burst of neutrino interactions lasting about a dozen seconds, totalling roughly two dozen events. The optical supernova was found in the Large Magellanic Cloud, about 50 kiloparsecs away, the following night. It remains the only occasion on which the collapse of a stellar core has been observed by any means other than the light it eventually produced, and the neutrino timing and energies matched core-collapse predictions closely enough to confirm the mechanism. The progenitor, catalogued as Sanduleak -69 202, was a blue supergiant rather than the red supergiant theory expected - a genuine surprise that forced revisions to massive-star evolution models. Event counts are quoted inconsistently in the literature, with Kamiokande-II's given as both 11 and 12.
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Timeline
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Connections · 5
- Supernovaevidence_for
- Supernovainstance_of
- Neutron starconcerns
- Kamioka Observatory, Mozumi mineconcerns
- Initial stellar massconcerns
Assembled narrative · 1
Assembled from 45 blocks · 1 evidence · 37 related
- Story
- Three underground detectors - Kamiokande-II in Japan, IMB in Ohio and Baksan in the Soviet Union - recorded a coincident burst of neutrino interactions lasting about a dozen seconds, totalling roughly two dozen events. The optical supernova was found in the Large Magellanic Cloud, about 50 kiloparsecs away, the following night. It remains the only occasion on which the collapse of a stellar core has been observed by any means other than the light it eventually produced, and the neutrino timing and energies matched core-collapse predictions closely enough to confirm the mechanism. The progenitor, catalogued as Sanduleak -69 202, was a blue supergiant rather than the red supergiant theory expected - a genuine surprise that forced revisions to massive-star evolution models. Event counts are quoted inconsistently in the literature, with Kamiokande-II's given as both 11 and 12.
- Knowledge
- Initial stellar mass
- Supernova
- Neutron star
- Kamioka Observatory, Mozumi mine
- SN 1987A: neutrinos from a collapsing core reach Earth
- Connections
- Kamioka Observatory, Mozumi mine
- Supernova
- Supernova
- Neutron star
- Kamioka Observatory, Mozumi mine
- Initial stellar mass
- Initial stellar mass
- The iron peak in nuclear binding energy
- Giant molecular cloud
- Neutron star
- Stellar-mass black hole
- A guest star appears in Taurus and is recorded in East Asia
- Baade and Zwicky propose supernovae and neutron stars
- A pulsar is found inside the Crab Nebula
- SN 1987A: neutrinos from a collapsing core reach Earth
- SN 1987A: neutrinos from a collapsing core reach Earth
- JWST finds the compact object in SN 1987A
- Degeneracy pressure
- Supernova
- Baade and Zwicky propose supernovae and neutron stars
- A regularly pulsing radio source is identified
- A pulsar is found inside the Crab Nebula
- SN 1987A: neutrinos from a collapsing core reach Earth
- A neutron-star merger is detected in gravitational waves and light
- A radius is measured for the heaviest known neutron star
- JWST finds the compact object in SN 1987A
- SN 1987A: neutrinos from a collapsing core reach Earth
- SN 1987A: neutrinos from a collapsing core reach Earth
- Hydrogen fusion: the proton-proton chain and the CNO cycle
- Main sequence (core hydrogen burning)
- Supernova
- Protostar
- The first stars form from metal-free gas
- SN 1987A: neutrinos from a collapsing core reach Earth
- Evidence
- Records a coincident neutrino burst at approximately 07:35 UT on 23 February 1987 across three detectors, totalling roughly two dozen events. Volume and page numbers are deliberately not asserted because they were not confirmed. Reported event counts differ between accounts: Kamiokande-II is quoted as both 11 and 12 events, with 8 for IMB and 5 for Baksan.
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