Key parameters at a glance
- A radius of 6.20 Earth radii
- A mass of 31.78 Earth masses
- Surface gravity around 0.83 g
- An orbital period of 4.947 days
- Semi-major axis 0.0600 AU
- Distance from Earth 140.38 light-years
- Earth Similarity Index 0.417
- Travel time at Voyager 1 speed 2,475,552 years
Context from the literature
HD 49674 b, formally named Eburonia, is an extrasolar planet located approximately 134 light-years away in the constellation of Auriga, orbiting the star HD 49674. It was discovered orbiting the star in 2002. The planet is a gas giant and orbits extremely close to its star, which takes only 4.95 days to revolve.
Excerpted from Wikipedia · full article
HD 49674 b Planet Profile
Physical Specs
Classification
Planet Type
Neptune-like
Discovery
Size rank in cohort
Rank by radius
#262of 574
top 45.5%
This planet
6.20R⊕
Neptune-like median
6.39R⊕
Nearest-size peers
| Metric | Earth | HD 49674 b | Jupiter |
|---|---|---|---|
| Radius (R⊕) | 1.00 | 6.20 | 11.21 |
| Mass (M⊕) | 1.00 | 31.78 | 317.83 |
| Density (g/cm³) | 5.51 | 0.73 | 1.33 |
| Surface Gravity (g) | 1.00 | 0.83 | 2.53 |
| Insolation (S⊕) | 1.00 | — | 0.037 |
Alternative Mass Estimates
| Method | Value | Interpretation |
|---|---|---|
| Minimum mass (M sin i) | 31.783 M⊕ | Lower bound from radial-velocity fitting. |
Star Catalogue Identifiers
HD
HD 49674
HIP
HIP 32916
TIC
TIC 21267079
Gaia DR2
Gaia DR2 951427000863064192
Gaia DR3
Gaia DR3 951427000863064192
System
HD 49674
Percentile among Neptune-like cohort
Orbit & Habitability
Orbital Dynamics
Year Length
A year here lasts approximately 4.95 Earth days (1.4% of a terrestrial year) on a nearly circular orbit at a mean orbital distance of 0.0600 AU.
Extended Orbital Architecture
RV semi-amplitude (K)
12.000 m/s
Transit mid-time (BJD)
2,454,625.6140
Long. of periastron (ω)
17.00°
Angular separation (arcsec)
1.39000
Eq. Temperature
—
Insolation (S⊕)
—
Earth = 1.00
Earth Similarity (ESI)
0.417
0 = alien, 1 = Earth-identical
Discovery Paper
Primary reference
Butler et al. 2003Instrument
HIRES Spectrometer
Publication
2003-01
Observation locale
Ground
Discovery cohort
Planets confirmed in 2002 at W. M. Keck Observatory (7 shown).
Host System: HD 49674
Spectral Class
G-type yellow (Sun-like)
Effective Temperature
5,602 K — cooler than the Sun (5,778 K)
Estimated Age
3.62 Gyr — younger than the Sun (4.6 Gyr)
Stellar Radius
1.020 R☉
Stellar Mass
1.030 M☉
Metallicity [Fe/H]
0.32
Extended Stellar Properties
Surface gravity (log g)
4.440 dex
Stellar density
1.232 g/cm³
Systemic radial velocity
11.97 km/s
Rotational v·sin i
0.42 km/s
Activity index (log R'HK)
-4.800
Metallicity ratio
[Fe/H]
Multi-band Host Photometry — 11 bands
Astrometric Data
Parallax
23.205 mas
Total Proper Motion
127.575 mas/yr
PM Right Ascension
34.59 mas/yr
PM Declination
-122.80 mas/yr
Galactic Cartesian (pc)
x = -0.169 · y = 0.737 · z = 0.654
Equatorial (J2000)
RA 102.87735° · Dec 40.86723°
Galactic ℓ, b
175.339° · 17.371°
Ecliptic λ, β
100.197° · 17.883°
HTM-20 index
-814607088
Observation Record
Photometric series
1
RV measurements
2
Stellar spectra
1
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Kepler-696 b
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