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

Stern mit 5 bekannten Planeten

HD 158259

In Ouranos öffnen

HD 158259, ein G0-Stern, hat 5 bestätigte Planeten.

Gemessen

Entfernung: etwa 88.2 Lichtjahre
Spektraltyp des Sterns: G0
Bestätigte Planeten: 5

Entfernung von der Sonne

Über 88.2 Lichtjahre. Zum Durchqueren:

Licht88.2 Jahre
Geschwindigkeit von Voyager 11.57 Millionen Jahre
Fahrt mit 100 km/h952 Millionen 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.

Wie er entdeckt wurde

Erster Planet, entdeckt 2020 durch Radialgeschwindigkeit (NASA Exoplanet Archive).

Seine Planeten

HD 158259 d — 2.2 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 5 days; found in 2020 by radial velocity.
HD 158259 b — 1.3 times Earth's width, about Earth-sized — probably rocky; its year lasts 2 days; about 1,200 °C, hot enough to melt rock; found in 2020 by radial velocity.
HD 158259 c — 2.2 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 3 days; found in 2020 by radial velocity.
HD 158259 e — 2.3 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 8 days; found in 2020 by radial velocity.
HD 158259 f — 2.4 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 12 days; found in 2020 by radial velocity.

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

HD 158259 d — 2.2 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 5 days; found in 2020 by radial velocity.

HD 158259 b — 1.3 times Earth's width, about Earth-sized — probably rocky; its year lasts 2 days; about 1,200 °C, hot enough to melt rock; found in 2020 by radial velocity.

HD 158259 c — 2.2 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 3 days; found in 2020 by radial velocity.

HD 158259 e — 2.3 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 8 days; found in 2020 by radial velocity.

HD 158259 f — 2.4 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 12 days; found in 2020 by radial velocity.

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.