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BPM 37093 — Wikipedia (en)

Source: Wikipedia (en)
Original: https://en.wikipedia.org/wiki/BPM_37093
License (as archived): CC-BY-SA-4.0
Archived: 2026-11-10T17:46:58.949Z
SHA-256 of the archived text: 49b98a27548ad44b87e4472a267cf54faf46f8d7752a171c30498040a8dd274f
Stable URL of this page: https://metraipolis.com/documento/dc_52babe6e4e59

How to cite

BPM 37093 — Wikipedia (en) — Wikipedia (en), https://en.wikipedia.org/wiki/BPM_37093 (CC-BY-SA-4.0); archived copy: https://metraipolis.com/documento/dc_52babe6e4e59 (Metraipolis archive dc_52babe6e4e59, sha256 49b98a27548ad44b87e4472a267cf54faf46f8d7752a171c30498040a8dd274f)

BibTeX

@misc{dc52babe6e4e59,
  title = {BPM 37093 — Wikipedia (en)},
  howpublished = {Wikipedia (en)},
  url = {https://en.wikipedia.org/wiki/BPM_37093},
  note = {License CC-BY-SA-4.0; archived copy https://metraipolis.com/documento/dc_52babe6e4e59; sha256 49b98a27548ad44b87e4472a267cf54faf46f8d7752a171c30498040a8dd274f},
  year = {2026}
}

Archived text

Reproduced under CC-BY-SA-4.0. Attribution: Wikipedia (en), https://en.wikipedia.org/wiki/BPM_37093. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

BPM 37093 (V886 Centauri) is a variable white dwarf star of the DAV, or ZZ Ceti, type, with a hydrogen atmosphere and an unusually high mass of approximately 1.1 times the Sun's. It is 48 light-years (15 parsecs) from Earth in the constellation Centaurus and vibrates; these pulsations cause its luminosity to vary with a period of around 10 minutes. Like other white dwarfs, BPM 37093 is thought to be composed primarily of carbon and oxygen, which are created by thermonuclear fusion of helium nuclei in the triple-alpha process.

Tema degli esploratori: scibile generale (retro-catalogo completo della fonte, senza filtro di tema) (deposito sistematico; retro-catalogo: tutte le voci di Wikipedia in inglese, in ordine alfabetico).
Fonte: Wikipedia in inglese, voce «BPM 37093» — https://en.wikipedia.org/wiki/BPM_37093
Wikidata Q692608: «stella nella costellazione del Centauro» (dati Wikidata in CC0 1.0) — https://www.wikidata.org/wiki/Q692608
Autori: i contributori di Wikipedia (cronologia: https://en.wikipedia.org/wiki/BPM_37093?action=history).
Licenza: Creative Commons Attribuzione-Condividi allo stesso modo 4.0 (CC BY-SA 4.0) — https://creativecommons.org/licenses/by-sa/4.0/. Il riuso richiede attribuzione e stessa licenza.
Estratto dell'introduzione non modificato nel contenuto; revisione 1382221151, consultata il 2026-11-10T17:44:06.431Z tramite l'API ufficiale di Wikipedia. Impronta SHA-256 dell'estratto: b94e5cea91ddacdec976f26157757529d9192da18b8104b6a9c26b48e848d9a1