Key parameters at a glance
- A radius of 1.11 Earth radii
- A mass of 1.40 Earth masses
- Surface gravity around 1.14 g
- An orbital period of 9.866 days
- Semi-major axis 0.0496 AU
- Equilibrium temperature 301 K (28 °C)
- Distance from Earth 11.01 light-years
- Earth Similarity Index 0.949
- Travel time at Voyager 1 speed 194,095 years
- Almost certainly tidally locked to its host star given the close orbit
Context from the literature
Ross 128 b is a confirmed Earth-sized exoplanet, likely rocky, that is orbiting near the inner edge of the habitable zone of the red dwarf star Ross 128, at a distance of 11.007 light-years from Earth in the constellation of Virgo. The exoplanet was found using a decade's worth of radial velocity data using the European Southern Observatory's HARPS spectrograph at the La Silla Observatory in Chile. Ross 128 b is the nearest exoplanet around a quiet red dwarf, and is considered one of the best candidates for habitability. The planet is only 35% more massive than Earth, receives only 38% more starlight, and is expected to be a temperature suitable for liquid water to exist on the surface, if it has an atmosphere.
Excerpted from Wikipedia · full article
Ross 128 b Planet Profile
Physical Specs
Classification
Planet Type
Rocky Terrestrial
Discovery
Size rank in cohort
Rank by radius
#209of 570
top 36.5%
This planet
1.11R⊕
Rocky Terrestrial median
1.01R⊕
Nearest-size peers
| Metric | Earth | Ross 128 b | Jupiter |
|---|---|---|---|
| Radius (R⊕) | 1.00 | 1.11 | 11.21 |
| Mass (M⊕) | 1.00 | 1.40 | 317.83 |
| Density (g/cm³) | 5.51 | 5.63 | 1.33 |
| Surface Gravity (g) | 1.00 | 1.14 | 2.53 |
| Insolation (S⊕) | 1.00 | 1.38 | 0.037 |
Alternative Mass Estimates
| Method | Value | Interpretation |
|---|---|---|
| Minimum mass (M sin i) | 1.400 M⊕ | Lower bound from radial-velocity fitting. |
Star Catalogue Identifiers
HIP
HIP 57548
TIC
TIC 325275315
Gaia DR2
Gaia DR2 3796072592206250624
Gaia DR3
Gaia DR3 3796072592206250624
System
Ross 128
Percentile among Rocky Terrestrial cohort
Orbit & Habitability
Orbital Dynamics
Year Length
A year here lasts approximately 9.87 Earth days (2.7% of a terrestrial year) on a mildly elliptical path at a mean orbital distance of 0.0496 AU.
Eq. Temperature
301K
(28 °C)
Insolation (S⊕)
1.38
Earth = 1.00
Earth Similarity (ESI)
0.949
0 = alien, 1 = Earth-identical
Within the conservative habitable zone — liquid water is physically possible with adequate atmospheric pressure. Close-orbiting tidally-locked around a cool host.
Discovery Paper
Primary reference
Bonfils et al. 2018Instrument
HARPS Spectrograph
Publication
2018-05
Observation locale
Ground
Discovery cohort
Planets confirmed in 2017 at La Silla Observatory (12 shown).
Host System: Ross 128
Spectral Class
M-type red dwarf
Effective Temperature
3,192 K — cooler than the Sun (5,778 K)
Estimated Age
5.00 Gyr — older than the Sun (4.6 Gyr)
Stellar Radius
0.197 R☉
Stellar Mass
0.168 M☉
Metallicity [Fe/H]
-0.02
Extended Stellar Properties
Surface gravity (log g)
5.047 dex
Stellar density
27.334 g/cm³
Systemic radial velocity
-30.90 km/s
Rotation period
123.00 days
Metallicity ratio
[M/H]
Multi-band Host Photometry — 9 bands
Astrometric Data
Parallax
296.307 mas
Total Proper Motion
1,365.937 mas/yr
PM Right Ascension
607.68 mas/yr
PM Declination
-1,223.32 mas/yr
Galactic Cartesian (pc)
x = -0.998 · y = 0.053 · z = 0.014
Equatorial (J2000)
RA 176.93760° · Dec 0.79929°
Galactic ℓ, b
270.157° · 59.556°
Ecliptic λ, β
176.868° · -0.484°
HTM-20 index
-1767574165
Observation Record
Photometric series
1
Stellar spectra
3
Archive notes
1
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