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136 Tauri — Wikipedia (en)

Source: Wikipedia (en)
Original: https://en.wikipedia.org/wiki/136_Tauri
License (as archived): CC-BY-SA-4.0
Archived: 2026-10-07T22:42:12.403Z
SHA-256 of the archived text: 4760b80a45ecdf9b67efa8a5f8c1066a16642132c41fc71a11903865cd99b65e
Stable URL of this page: https://metraipolis.com/documento/dc_bb4e683aa2af

How to cite

136 Tauri — Wikipedia (en) — Wikipedia (en), https://en.wikipedia.org/wiki/136_Tauri (CC-BY-SA-4.0); archived copy: https://metraipolis.com/documento/dc_bb4e683aa2af (Metraipolis archive dc_bb4e683aa2af, sha256 4760b80a45ecdf9b67efa8a5f8c1066a16642132c41fc71a11903865cd99b65e)

BibTeX

@misc{dcbb4e683aa2af,
  title = {136 Tauri — Wikipedia (en)},
  howpublished = {Wikipedia (en)},
  url = {https://en.wikipedia.org/wiki/136_Tauri},
  note = {License CC-BY-SA-4.0; archived copy https://metraipolis.com/documento/dc_bb4e683aa2af; sha256 4760b80a45ecdf9b67efa8a5f8c1066a16642132c41fc71a11903865cd99b65e},
  year = {2026}
}

Archived text

Reproduced under CC-BY-SA-4.0. Attribution: Wikipedia (en), https://en.wikipedia.org/wiki/136_Tauri. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

136 Tauri is a white-hued binary star system in the zodiac constellation of Taurus. It has a combined apparent visual magnitude of 4.56, which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 7.71±0.22 mas as seen from Earth's orbit, it is located approximately 420 light years from the Sun. The system is moving nearer with a heliocentric radial velocity of −17.2 km/s, and is expected to make its closest approach in 6.5 million years at a distance of 150 ly (45 pc). This is a close, double-lined spectroscopic binary with an orbital period of 5.96 days and an eccentricity of 0.00. Tidal effects between the pair may have circularized their orbit and slowed their rotation rates – the primary has a projected rotational velocity of 10 km/s. They have a combined stellar classification of A0 V, and both are most likely A-type main-sequence stars of the same class.

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 «136 Tauri» — https://en.wikipedia.org/wiki/136_Tauri
Wikidata Q14555256 (dati Wikidata in CC0 1.0) — https://www.wikidata.org/wiki/Q14555256
Autori: i contributori di Wikipedia (cronologia: https://en.wikipedia.org/wiki/136_Tauri?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 1374810356, consultata il 2026-10-07T22:18:19.235Z tramite l'API ufficiale di Wikipedia. Impronta SHA-256 dell'estratto: 4148a790c065b3af4aa9490cbf2c499247ae7e3585c915d3a3e32fdf5247863d