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Stella con 4 pianeti noti

HD 3167

Apri in Ouranos

HD 3167, una stella K0 V, ha 4 pianeti confermati.

Misurato

Distanza: circa 154 anni luce
Tipo spettrale della stella: K0 V
Pianeti confermati: 4

Distanza dal Sole

Informazioni 154 anni luce. Per attraversarlo:

Luce154 anni
Velocità della Voyager 12.74 milioni di anni
In movimento a 100 km/h1.66 miliardi di anni

Voyager 1 alla velocità con cui si è allontanata nell'anno fino al 2026-10-25 (JPL Horizons). In auto: senza sosta, senza mai fare rifornimento.

Come è stato scoperto

Primo pianeta scoperto nel 2016 con il transito e la velocità radiale (NASA Exoplanet Archive).

I suoi pianeti

HD 3167 b — 1.6 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 23 hours; about 1,500 °C, hot enough to melt rock; found in 2016 by transit.
HD 3167 c — 3 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 30 days; about 290 °C, hotter than boiling water; found in 2016 by transit.
HD 3167 d — 2.6 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 8 days; about 590 °C, hotter than boiling water; found in 2017 by radial velocity.
HD 3167 e — 4 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 92 days; about 120 °C, hotter than boiling water; found in 2022 by radial velocity.

The NASA Exoplanet Archive's page

Da dove proviene

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.

Ogni catalogo utilizzato da Ouranos è citato nella pagina dei crediti.

I suoi pianeti

HD 3167 b — 1.6 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 23 hours; about 1,500 °C, hot enough to melt rock; found in 2016 by transit.

HD 3167 c — 3 times Earth's width, a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 30 days; about 290 °C, hotter than boiling water; found in 2016 by transit.

HD 3167 d — 2.6 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 8 days; about 590 °C, hotter than boiling water; found in 2017 by radial velocity.

HD 3167 e — 4 times Earth's width (estimated from its mass, not measured), a 'sub-Neptune' — bigger than Earth, smaller than Neptune; its year lasts 92 days; about 120 °C, hotter than boiling water; found in 2022 by radial velocity.

Da dove proviene

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.