HD 34445, ein G0-V-Stern, hat 6 bestätigte Planeten.
Gemessen
Entfernung
etwa 150 Lichtjahre
Spektraltyp des Sterns
G0 V
Bestätigte Planeten
6
Entfernung von der Sonne
Über 150 Lichtjahre. Zum Durchqueren:
Licht150 Jahre
Geschwindigkeit von Voyager 12.67 Millionen Jahre
Fahrt mit 100 km/h1.62 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
HD 34445 f und HD 34445 b haben eine Gleichgewichtstemperatur zwischen −50 und +50 °C.
Wie er entdeckt wurde
Erster Planet, entdeckt 2009 durch Radialgeschwindigkeit (NASA Exoplanet Archive).
Seine Planeten
HD 34445 d — 6.1 times Earth's width (estimated from its mass, not measured), Neptune-sized; its year lasts 120 days; about 200 °C, hotter than boiling water; found in 2017 by radial velocity.
HD 34445 c — 8.4 times Earth's width (estimated from its mass, not measured), Neptune-sized; its year lasts 210 days; about 120 °C, hotter than boiling water; found in 2017 by radial velocity.
HD 34445 g — 14 times Earth's width (estimated from its mass, not measured), a giant, Jupiter-sized or more; its year lasts about 16 Earth years; about −140 °C, below freezing; found in 2017 by radial velocity.
HD 34445 e — 4.3 times Earth's width (estimated from its mass, not measured), Neptune-sized; its year lasts 49 days; about 370 °C, hotter than boiling water; found in 2017 by radial velocity.
HD 34445 f — 6.9 times Earth's width (estimated from its mass, not measured), Neptune-sized; its year lasts 680 days; about −7 °C, below freezing; found in 2017 by radial velocity.
HD 34445 b — 14 times Earth's width (estimated from its mass, not measured), a giant, Jupiter-sized or more; its year lasts about 3 Earth years; about −42 °C, below freezing; found in 2009 by radial velocity.
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.