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35 Comae Berenices — Wikipedia (en)

Source: Wikipedia (en)
Original: https://en.wikipedia.org/wiki/35_Comae_Berenices
License (as archived): CC-BY-SA-4.0
Archived: 2026-11-06T13:37:16.521Z
SHA-256 of the archived text: 6215321b7cc2b53558c2f8e18c71f8c33721bb6d148748ec4410b927e328385e
Stable URL of this page: https://metraipolis.com/documento/dc_83bb6484a751

How to cite

35 Comae Berenices — Wikipedia (en) — Wikipedia (en), https://en.wikipedia.org/wiki/35_Comae_Berenices (CC-BY-SA-4.0); archived copy: https://metraipolis.com/documento/dc_83bb6484a751 (Metraipolis archive dc_83bb6484a751, sha256 6215321b7cc2b53558c2f8e18c71f8c33721bb6d148748ec4410b927e328385e)

BibTeX

@misc{dc83bb6484a751,
  title = {35 Comae Berenices — Wikipedia (en)},
  howpublished = {Wikipedia (en)},
  url = {https://en.wikipedia.org/wiki/35_Comae_Berenices},
  note = {License CC-BY-SA-4.0; archived copy https://metraipolis.com/documento/dc_83bb6484a751; sha256 6215321b7cc2b53558c2f8e18c71f8c33721bb6d148748ec4410b927e328385e},
  year = {2026}
}

Archived text

Reproduced under CC-BY-SA-4.0. Attribution: Wikipedia (en), https://en.wikipedia.org/wiki/35_Comae_Berenices. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

35 Comae Berenices is a multiple star system in the northern constellation of Coma Berenices, located about 6° from the north galactic pole. It is faintly visible to the naked eye with an apparent visual magnitude of 4.93. Based upon parallax measurements, it is located around 280 light years from the Sun. The system is moving closer to the Earth with a heliocentric radial velocity of −6 km/s. This was found to be a wide binary by Struve in 1828, but it has completed less than half an orbit since then and the orbital elements remain poorly constrained. It has an orbital period of 539±95 years and an eccentricity of 0.2±0.1. The pair have been resolved into stellar classifications of an evolved G-type giant primary of class G5 III and an F-type secondary, most likely main sequence with a class of F1 V. The primary component is a spectroscopic binary with a period of 7.9624 ± 0.0117 years and an eccentricity of 0.63. A fourth component, 35 Com C, is located 29″ from the primary and may have a physical association.

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 «35 Comae Berenices» — https://en.wikipedia.org/wiki/35_Comae_Berenices
Wikidata Q4635544: «stella multipla nella costellazione della Chioma di Berenice» (dati Wikidata in CC0 1.0) — https://www.wikidata.org/wiki/Q4635544
Autori: i contributori di Wikipedia (cronologia: https://en.wikipedia.org/wiki/35_Comae_Berenices?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 1356270256, consultata il 2026-11-06T13:33:40.929Z tramite l'API ufficiale di Wikipedia. Impronta SHA-256 dell'estratto: 5f2b7715bdd902f09df8a71347612addf35d8c4602e73fdcf5a6eb7e7b0a3312