Hot Jupiter · HD 49674

HD 49674 b

ExoplanetsDiscovered 2002

Scientific overview

HD 49674 b is a hot jupiter orbiting HD 49674, completing an orbit every 5 days, about 140 light-years from Earth. It was discovered in 2002 using the radial velocity method.

Host star

Nervia

Spectral type

G5 V

Temperature

5,602 K

Mass

1.03 M☉

Discovery and detection

Detection method

Radial Velocity Method

Discovery year

2002

Discovered at

W. M. Keck Observatory

Knowledge connections

OrbitsNervia
Discovered by methodRadial Velocity Method
Discovered atW. M. Keck Observatory
Catalogued inNASA Exoplanet Archive

Quick facts

Class: Hot Jupiter
Host star: Nervia
Discovery method: Radial Velocity Method
Discovery year: 2002
Orbital period: 4.9474 d
Semi-major axis: 0.06 AU
Eccentricity: 0.09
Radius: 6.2 R⊕
Mass: 31.78 M⊕
Density: 0.74 g/cm³ · derived
Equilibrium temp.: 1114 K
Insolation: 264.29 S⊕
Distance: 140 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 density0.74 g/cm³derived
Formula & inputs
Formula: ρ = M / (4⁄3·π·r³) (v1.0.0, impl v1.0.0)
Inputs:
- massEarth = 31.78 M⊕ · NASA
- radiusEarth = 6.2 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.