Beta Pictoris b

Beta Pictoris b

Planet· orbits Beta Pictoris

Beta Pictoris b — a giant planet of about 11 Jupiter masses orbiting at ~10 AU (a 24-year orbit), DIRECTLY IMAGED in 2008 sweeping through its star's debris disk. Young and hot from formation, it glows in the infrared — which is how it was photographed. Its size and mass are model estimates, so no density is quoted.

Open in 3D viewSee Beta Pictoris b in the live, interactive 3D map

Key facts

Mass
2.09 × 10²⁸ kg
11 M♃ (3,497 M⊕)
Year
23.8 Earth years
8,682 Earth days
Distance from Beta Pictoris
10.1 AU

Science

Physical

Mass
2.09 × 10²⁸ kg · 11 M♃ (3,497 M⊕)
Radius
Not measured
Directly imaged, never transited: the ~11 Jupiter mass and ~1.6 Jupiter-radii size are model estimates from its brightness and youth, so no density is quoted.

Orbital

Semi-major axis
10.1 AU
From the NASA Exoplanet Archive (direct imaging + orbit fit)
Eccentricity
0.105
From the NASA Exoplanet Archive (direct imaging + orbit fit)
Inclination
0.00 °
From the NASA Exoplanet Archive (direct imaging + orbit fit)
Orbital period
23.77 years
From the NASA Exoplanet Archive (direct imaging + orbit fit)
Perihelion
9.01 AU
Computed from the orbital elements
Aphelion
11.1 AU
Computed from the orbital elements
Mean orbital velocity
12.6 km/s
Computed from the orbital elements

Composition

Bulk composition
A young gas giant of about 11 Jupiter masses at ~10 AU, still hot from formation and glowing in the infrared — which is how it was photographed in 2008, embedded in its star's debris disk. Hydrogen/helium; true appearance unresolved.
Cloud appearance
Appearance based on NASA/JPL-Caltech's artist's concept. No spacecraft has imaged this world, so its real appearance is unknown — The banded clouds shown are a representation of its class, shown only in Visual mode; Realism shows a plain spectral colour.

Radiation & temperature

Insolation
0.0885 S⊕ · 9% of the sunlight Earth receives
Computed from Beta Pictoris's luminosity and the orbital distance (inverse-square; Earth's sunlight = 1).

Discovery & history

Method
Directly imaged
Name
Designated 'b' under the IAU planet-lettering convention; no IAU proper name.

Directly imaged in 2008 (VLT/ESO) — one of the first planets ever photographed, and the clearest case of a young giant caught inside a forming debris disk.

Images

Images from open archives · credit shown per image