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56 Aquilae — Wikipedia (en)

Source: Wikipedia (en)
Original: https://en.wikipedia.org/wiki/56_Aquilae
License (as archived): CC-BY-SA-4.0
Archived: 2026-11-06T18:09:08.525Z
SHA-256 of the archived text: 4ed57ac2fe32153a195d8068d599121ba9556dd3f3ab5b22184bdd68afab56ed
Stable URL of this page: https://metraipolis.com/documento/dc_79da8a204af7

How to cite

56 Aquilae — Wikipedia (en) — Wikipedia (en), https://en.wikipedia.org/wiki/56_Aquilae (CC-BY-SA-4.0); archived copy: https://metraipolis.com/documento/dc_79da8a204af7 (Metraipolis archive dc_79da8a204af7, sha256 4ed57ac2fe32153a195d8068d599121ba9556dd3f3ab5b22184bdd68afab56ed)

BibTeX

@misc{dc79da8a204af7,
  title = {56 Aquilae — Wikipedia (en)},
  howpublished = {Wikipedia (en)},
  url = {https://en.wikipedia.org/wiki/56_Aquilae},
  note = {License CC-BY-SA-4.0; archived copy https://metraipolis.com/documento/dc_79da8a204af7; sha256 4ed57ac2fe32153a195d8068d599121ba9556dd3f3ab5b22184bdd68afab56ed},
  year = {2026}
}

Archived text

Reproduced under CC-BY-SA-4.0. Attribution: Wikipedia (en), https://en.wikipedia.org/wiki/56_Aquilae. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

56 Aquilae is a single star in the equatorial constellation of Aquila. 56 Aquilae is its Flamsteed designation. Its apparent visual magnitude is 5.79, meaning it is barely visible to the naked eye as a dim, orange-hued point of light, under ideal viewing conditions. The star is located at a distance of around 593 light-years away from the Sun, based on parallax. It is moving closer to the Earth with a heliocentric radial velocity of −50 km/s, and is predicted to come as near as 222 light-years in around 3.3 million years. This is an aging giant star with a stellar classification of K5 III, having exhausted the supply of hydrogen at its core and expanded to 43 times the Sun's radius. It is radiating 896 times the luminosity of the Sun from its photosphere at an effective temperature of 3,885 K. 56 Aquilae is a double star, but it does not appear to be a binary star system. It is one of the double stars profiled in Admiral William Henry Smyth's 1864 work, Sidereal Chromatics.

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 «56 Aquilae» — https://en.wikipedia.org/wiki/56_Aquilae
Wikidata Q2401002: «stella nella costellazione dell'Aquila» (dati Wikidata in CC0 1.0) — https://www.wikidata.org/wiki/Q2401002
Autori: i contributori di Wikipedia (cronologia: https://en.wikipedia.org/wiki/56_Aquilae?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 1377044877, consultata il 2026-11-06T18:05:39.598Z tramite l'API ufficiale di Wikipedia. Impronta SHA-256 dell'estratto: 1c36dd9ada3f55d648bcb3ae92e228aae91619a6d2e244755c8579016a411857