HR 8799 d
Planet· orbits the Sun
HR 8799 d — a young, hot giant (~7-10 Jupiter masses) imaged at ~24 AU, orbiting in about a century. Like its siblings it shines by its own residual heat of formation; its size and mass are model estimates, so no density is quoted.
Open in 3D viewSee HR 8799 d in the live, interactive 3D map
Key facts
Mass
1.79 × 10²⁸ kg
9.44 M♃ (3,000 M⊕)
Year
101 Earth years
37,000 Earth days
Distance from HR 8799
24 AU
Science
Physical
- Mass
- 1.79 × 10²⁸ kg · 9.44 M♃ (3,000 M⊕)
- Radius
- Not measured
Orbital
- Semi-major axis
- 24 AU
- Eccentricity
- 0.1
- Inclination
- 0.00 °
- Orbital period
- 101.30 years
- Perihelion
- 21.6 AU
- Aphelion
- 26.4 AU
- Mean orbital velocity
- 7.06 km/s
Composition
- Bulk composition
- A young hydrogen/helium giant (~7–10 Jupiter masses) at ~24 AU, self-luminous at ~1,300 K. One of the three planets first photographed in 2008.
- 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 Vision mode; Realism shows a plain spectral colour.
Radiation & temperature
- Insolation
- 0.00986 S⊕ · 1/101 of the sunlight Earth receives
Discovery & history
- Method
- Directly imaged
- Name
- Designated 'd' under the IAU planet-lettering convention; no IAU proper name has been assigned.
One of the three planets directly imaged around HR 8799 in 2008 — a historic first.
Images
Directly imaged only as a point of light beside HR 8799 — see the system view for the real Keck time-lapse and Hubble images that show all four planets. No telescope has resolved this planet's disk or surface.