Traducido por IA (Opus 5.5) a partir de la ficha en inglés. Los números, nombres y fuentes no se han modificado.

Estrella con 6 planetas conocidos

Kepler-80

Abrir en Ouranos

Kepler-80, una estrella K5, tiene 6 planetas confirmados.

Medido

Distancia: unos 1,205 años luz
Tipo espectral de la estrella: K5
Planetas confirmados: 6

Distancia al Sol

Acerca de 1,210 años luz. Para cruzarlo:

Luz1,210 años
Velocidad de la Voyager 121.4 millones de años
Conduciendo a 100 km/h13 mil millones de años

La Voyager 1 a la velocidad con la que se alejó durante el año hasta 2026-10-25 (JPL Horizons). Conduciendo: sin parar, sin repostar nunca.

Cómo se descubrió

Primer planeta descubierto en 2012, por tránsito (NASA Exoplanet Archive).

Sus planetas

Kepler-80 c — 2.7 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 10 days; about 220 °C, hotter than boiling water; found in 2012 by transit.
Kepler-80 d — 1.5 times Earth's width, about Earth-sized — probably rocky; its year lasts 3 days; about 450 °C, hotter than boiling water; found in 2014 by transit.
Kepler-80 b — 2.7 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 7 days; about 270 °C, hotter than boiling water; found in 2012 by transit.
Kepler-80 e — 1.6 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 5 days; about 360 °C, hotter than boiling water; found in 2014 by transit.
Kepler-80 f — 1.2 times Earth's width, about Earth-sized — probably rocky; its year lasts 24 hours; about 780 °C, hotter than boiling water; found in 2016 by transit.
Kepler-80 g — 1.1 times Earth's width, about Earth-sized — probably rocky; its year lasts 15 days; about 150 °C, hotter than boiling water; found in 2017 by transit.

The NASA Exoplanet Archive's page

De dónde proceden estos datos

NASA Exoplanet Archive, Planetary Systems Composite Parameters (fetched 2026-11-02). Composite values: where a planet's size or mass was not measured, the archive estimates it from the other.
This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with NASA under the Exoplanet Exploration Program.

Todos los catálogos que usa Ouranos se citan en la página de créditos.

Sus planetas

Kepler-80 c — 2.7 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 10 days; about 220 °C, hotter than boiling water; found in 2012 by transit.

Kepler-80 d — 1.5 times Earth's width, about Earth-sized — probably rocky; its year lasts 3 days; about 450 °C, hotter than boiling water; found in 2014 by transit.

Kepler-80 b — 2.7 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 7 days; about 270 °C, hotter than boiling water; found in 2012 by transit.

Kepler-80 e — 1.6 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 5 days; about 360 °C, hotter than boiling water; found in 2014 by transit.

Kepler-80 f — 1.2 times Earth's width, about Earth-sized — probably rocky; its year lasts 24 hours; about 780 °C, hotter than boiling water; found in 2016 by transit.

Kepler-80 g — 1.1 times Earth's width, about Earth-sized — probably rocky; its year lasts 15 days; about 150 °C, hotter than boiling water; found in 2017 by transit.

De dónde proceden estos datos

NASA Exoplanet Archive, Planetary Systems Composite Parameters (fetched 2026-11-02). Composite values: where a planet's size or mass was not measured, the archive estimates it from the other.

This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with NASA under the Exoplanet Exploration Program.