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

Estrella con 2 planetas conocidos

KOI-55

KOI-55, una estrella B, tiene 2 planetas confirmados.

Medido

Acerca de 4,010 años luz. Para cruzarlo:

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.

Primer planeta descubierto en 2011, por modulación orbital del brillo (NASA Exoplanet Archive).

KOI-55 c — 0.9 times Earth's width, about Earth-sized — probably rocky; its year lasts 8 hours; about 6,600 °C, hot enough to melt rock; found in 2011 by orbital brightness modulation.
KOI-55 b — 0.8 times Earth's width, smaller than the Earth; its year lasts 6 hours; about 7,500 °C, hot enough to melt rock; found in 2011 by orbital brightness modulation.

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.

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

Estrella con 2 planetas conocidos

KOI-55, una estrella B, tiene 2 planetas confirmados.

Acerca de 4,010 años luz. Para cruzarlo:

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.

Primer planeta descubierto en 2011, por modulación orbital del brillo (NASA Exoplanet Archive).

KOI-55 c — 0.9 times Earth's width, about Earth-sized — probably rocky; its year lasts 8 hours; about 6,600 °C, hot enough to melt rock; found in 2011 by orbital brightness modulation.
KOI-55 b — 0.8 times Earth's width, smaller than the Earth; its year lasts 6 hours; about 7,500 °C, hot enough to melt rock; found in 2011 by orbital brightness modulation.

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.