Von KI (Opus 5.5) aus der englischen Karte übersetzt. Zahlen, Namen und Quellen sind unverändert.

Stern mit 4 bekannten Planeten

Kepler-26

In Ouranos öffnen

Kepler-26, ein M0 V-Stern, hat 4 bestätigte Planeten.

Gemessen

Entfernung: etwa 1,094 Lichtjahre
Spektraltyp des Sterns: M0 V
Bestätigte Planeten: 4

Entfernung von der Sonne

Über 1,090 Lichtjahre. Zum Durchqueren:

Licht1,090 Jahre
Geschwindigkeit von Voyager 119.4 Millionen Jahre
Fahrt mit 100 km/h11.8 Milliarden Jahre

Voyager 1 mit der Geschwindigkeit, mit der sie sich im Jahr bis 2026-10-25 nach außen bewegte (JPL Horizons). Fahrt: ohne Pause, ohne je nachzutanken.

Fakten

Kepler-26 e hat eine Gleichgewichtstemperatur zwischen −50 und +50 °C.

Wie er entdeckt wurde

Erster Planet, entdeckt 2011 durch Transit (NASA Exoplanet Archive).

Seine Planeten

Kepler-26 c — 2.7 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 17 days; about 110 °C, hotter than boiling water; found in 2011 by transit.
Kepler-26 e — 2.4 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 47 days; about 3 °C, between freezing and boiling; found in 2014 by transit.
Kepler-26 b — 2.8 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 12 days; about 160 °C, hotter than boiling water; found in 2011 by transit.
Kepler-26 d — 1.1 times Earth's width, about Earth-sized — probably rocky; its year lasts 4 days; about 380 °C, hotter than boiling water; found in 2014 by transit.

The NASA Exoplanet Archive's page

Woher das stammt

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.

Jeder Katalog, den Ouranos verwendet, wird auf der Seite mit den Quellenangaben genannt.

Seine Planeten

Kepler-26 c — 2.7 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 17 days; about 110 °C, hotter than boiling water; found in 2011 by transit.

Kepler-26 e — 2.4 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 47 days; about 3 °C, between freezing and boiling; found in 2014 by transit.

Kepler-26 b — 2.8 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 12 days; about 160 °C, hotter than boiling water; found in 2011 by transit.

Kepler-26 d — 1.1 times Earth's width, about Earth-sized — probably rocky; its year lasts 4 days; about 380 °C, hotter than boiling water; found in 2014 by transit.

Woher das stammt

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.