Mini-Neptune · HD 147379

HD 147379 b

ExoplanetsDiscovered 2017

Scientific overview

HD 147379 b is a mini-neptune orbiting HD 147379, completing an orbit every 87 days, about 35 light-years from Earth. It was discovered in 2017 using the radial velocity method.

Host star

HD 147379

Spectral type

M0.0 V

Temperature

4,090 K

Mass

0.58 M☉

Discovery and detection

Detection method

Radial Velocity Method

Discovery year

2017

Knowledge connections

OrbitsHD 147379
Discovered by methodRadial Velocity Method
Catalogued inNASA Exoplanet Archive

Quick facts

Class: Mini-Neptune
Host star: HD 147379
Discovery method: Radial Velocity Method
Discovery year: 2017
Orbital period: 86.58 d
Semi-major axis: 0.3193 AU
Eccentricity: 0.063
Radius: 4.94 R⊕
Mass: 21.6 M⊕
Density: 0.99 g/cm³ · derived
Equilibrium temp.: 277 K
Insolation: 0.78 S⊕
Distance: 35 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 density0.99 g/cm³derived
Formula & inputs
Formula: ρ = M / (4⁄3·π·r³) (v1.0.0, impl v1.0.0)
Inputs:
- massEarth = 21.6 M⊕ · NASA
- radiusEarth = 4.94 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.