ROSS 128 SYSTEM / PLANETARY DOSSIER

Ross 128 b

A short orbit around a faint star, with a surface still beyond our view.

Artist’s impression of Ross 128 b; appearance and diameter are unconfirmed
Terrestrial-mass exoplanet

A nearby world with an unanswered climate.

Environment ↗

02
ATMOSPHERE

Not measured

DIAMETER
Not measured
POSSIBILITY FOR LIFE
Unknown · potentially temperate
WITHOUT PROTECTION
Not established as survivable

Mass comparison ↗

04
MINIMUM MASS1.35 × Earth

± 0.2 Earth masses

Measured m sin i · true mass may be larger.
ROSS 128 B

Instrument detail

Artist’s impression of Ross 128 b

Artist’s impression · appearance and diameter are unconfirmed.

Close to a much fainter sun.

Ross 128 b circles its star in just under ten Earth days. Its orbit lies far closer to the star than Earth does to Sol, but a red dwarf supplies much less light. Distance alone is therefore a poor guide to climate. The discovery drew attention because a compact orbit could still produce an interesting range of possible heating conditions.

A tug with an important qualifier.

The planet was found through the small motion it induces in its star. Radial velocities measure movement toward and away from us, leaving the orbital tilt uncertain. That is why the graph says minimum mass. A radius would supply another essential clue to density and composition; an Earth-like mass alone cannot tell us whether the imagined rocks resemble anything on the real world.

An energy balance is not a weather report.

Equilibrium temperature estimates depend on how much starlight a world reflects and simplify how it releases heat. An atmosphere can change the surface conditions substantially. A number near Earth’s temperature scale would therefore not prove a temperate landscape, let alone breathable air. Our black sky and hard shadows illustrate one airless scenario, while the profile keeps the actual climate unknown.

No silhouette across the star.

The discovery study used K2 photometry to rule out transits. Without a planetary silhouette crossing the stellar disk, that route to measuring its radius is unavailable. The close-up scenes here remain reconstructions, not photographs of a known surface.

Size, mass and atmosphere

DIAMETER / EARTH

Not measured.

The radius has not been measured; the illustration does not establish its size.

SIZE UNKNOWN
MINIMUM MASS / EARTH
  • Ross 128 b · minimum1.35 ± 0.20 M⊕
  • Earth · reference mass1.00 M⊕

Shared scale: 0–2 Earth masses. The planetary measurement is m sin i, a minimum mass with measurement uncertainty. Unknown orbital inclination allows a larger true mass. Bonfils et al., discovery study, Table 3, first model column. This is a minimum mass, not a measured radius or density.

ATMOSPHERE / COMPOSITION

Not measured

We cannot assign atmospheric percentages or surface pressure. An atmosphere has not been established here; that is different from proving the planet is airless.

Habitability

NATURAL CONDITIONSUnknown · potentially temperate

Its stellar heating makes it interesting for climate studies, but its position relative to the habitable-zone boundary depends on models. An atmosphere, surface water and life have not been established.

HUMANS / WITHOUT PROTECTIONNot established as survivable

Breathable air, safe pressure and tolerable temperatures are not known. A survival time would be speculation.

SURFACE TEMPERATURE
Unknown · no measured climate
SURFACE PRESSURE
Unknown
LIQUID WATER
Not established
SURFACE GRAVITY
Unknown · radius required

A year around Ross 128

9.86 Earth days

Semimajor axis: 0.0493 AU. One astronomical unit is approximately the mean Earth–Sun distance.

The overview is a schematic: sizes, orbital shape and the planet’s position are illustrative. It does not show a measured eccentricity, the orbit’s orientation or a live position.

Ross 128 b circles its star in just under ten Earth days. Its orbit lies far closer to the star than Earth does to Sol, but a red dwarf supplies much less light. Distance alone is therefore a poor guide to climate. The discovery drew attention because a compact orbit could still produce an interesting range of possible heating conditions.

Bonfils et al. · HARPS discovery study · orbital measurements ↗
A hypothetical dry, airless rocky surface with pale gray terraces and a low basin rim. The terrain, mineral colors and absence of air are artistic assumptions, not observations of Ross 128 b.

Above a possible basin

A hypothetical dry, airless rocky surface with pale gray terraces and a low basin rim. The terrain, mineral colors and absence of air are artistic assumptions, not observations of Ross 128 b.

An imagined ground-level view across fractured rock and regolith. No landing site has been mapped here. The scene continues an airless rocky possibility without establishing the planet’s actual geology or atmosphere.

Beside the broken outcrop

An imagined ground-level view across fractured rock and regolith. No landing site has been mapped here. The scene continues an airless rocky possibility without establishing the planet’s actual geology or atmosphere.

A large fractured rocky slab and smaller angular fragments under subdued warm starlight, crisp shadows. An artistic reconstruction of Ross 128 b; local detail, lighting and viewpoint are imagined. The depicted environment is a possibility, not an observed surface or weather map.

Rock textures under distant light

A large fractured rocky slab and smaller angular fragments under subdued warm starlight, crisp shadows. An artistic reconstruction of Ross 128 b; local detail, lighting and viewpoint are imagined. The depicted environment is a possibility, not an observed surface or weather map.

Planet and landscape images are hypothetical artistic interpretations.