Gas giant · GU Psc

GU Psc b

ExoplanetsDiscovered 2014

Scientific overview

GU Psc b is a gas giant orbiting GU Psc, about 155 light-years from Earth. It was discovered in 2014 using the direct imaging.

Host star

Spectral type

M3

Temperature

4,032 K

Mass

0.325 M☉

Discovery and detection

Detection method

Discovery year

2014

Gemini Observatory

Knowledge connections

OrbitsGU Psc
Discovered by methodDirect Imaging
Discovered atGemini Observatory
Catalogued inNASA Exoplanet Archive

Quick facts

Class: Gas giant
Host star: GU Psc
Discovery method: Direct Imaging
Discovery year: 2014
Semi-major axis: 2000 AU
Radius: 14.18 R⊕
Mass: 3591.3 M⊕
Density: 6.94 g/cm³ · derived
Equilibrium temp.: 1050 K
Distance: 155 ly

Density is derived from the archive mass and radius via ρ = M / (4⁄3·π·r³); all other values are catalogued measurements.

Derived values

Computed from source-backed inputs via standard formulae — not observations. Every input and constant is traced below.

Bulk density6.94 g/cm³derived
Formula & inputs
Formula: ρ = M / (4⁄3·π·r³) (v1.0.0, impl v1.0.0)
Inputs:
- massEarth = 3591.3 M⊕ · NASA
- radiusEarth = 14.18 R⊕ · NASA
Assumptions: M⊕ = 5.972e+24 kg, R⊕ = 6371000 m (IAU 2015 B3 nominal); Assumes a uniform sphere.
Limitations: Withheld above 30 g/cm³ (inconsistent mass/radius inputs).; Archive mass/radius carry no propagated uncertainty here.
Uncertainty: not propagated (inputs carry no catalogued uncertainty)
Computed as of 2026-06-29.

Quality & authority

Partial

Unreviewed

Description: Complete
Source coverage: Partial
Relationship coverage: Complete
Review coverage: None
Citation coverage: None
Image coverage: Not applicable

Data from the NASA Exoplanet Archive. See source quality.