Complete world information

LHS 1140 b

Its measurable mass, radius and 2026 atmospheric detection make it one of the strongest nearby targets for habitability research, without proving surface life or oceans.

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Scientific status

No exoplanet is confirmed habitable or inhabited. Habitable-zone position only means that liquid surface water could be possible under the right atmospheric conditions. Rate the Earth percentages are editorial comparison scores, not scientific probabilities.

Rate the Earth habitability percentages are editorial comparison scores, not scientific proof of habitability or life.
NASA-style scientific artist conceptCold ocean super-Earth concept
Rate the Earth habitability comparison66%
Potential candidate — not confirmed habitable
Probability of other life40%
Candidate for simple life
Distance modelApprox. 48.9 light-years

The listed value is the approximate present distance from Earth. Interstellar destinations move, but the difference is negligible compared with the enormous journey time at current spacecraft speeds.

One-way light time48.9 years

Minimum delay for information travelling at light speed.

Round-trip communication97.8 years

Approximate send-and-reply delay before processing time.

Real mission comparisonBeyond current mission capability

No spacecraft has travelled to this system

Host systemLHS 1140Open the complete star-system information page →

Life potential

Could other life exist on LHS 1140 b?

LHS 1140 b is treated as a potentially habitable candidate, so this site assigns it a moderate editorial probability for simple non-human life.

Editorial probability of other life40%
Candidate for simple life

Why this score?

  • Rate the Earth habitability comparison score: 66%.
  • Atmosphere clue: Detected escaping helium; deeper composition under study.
  • Host-star context: M-type red dwarf.
  • The catalog flags this world as a potentially habitable candidate.

This probability is an editorial astrobiology estimate based on public characteristics, not a formal scientific measurement.

Complete data sheet

Everything listed for LHS 1140 b

Measured values, estimates, discovery information and the main uncertainties are shown together below.

WorldLHS 1140 b
ClassificationDense super-Earth
Host systemLHS 1140
Host starM-type red dwarf
Distance from EarthApprox. 48.9 light-years
RadiusAbout 1.73 × Earth
MassAbout 5.6 × Earth
GravityHigher than Earth
AtmosphereDetected escaping helium; deeper composition under study
TemperatureModel-dependent
Orbital period24.7 days
Discovery year2017
Discovery methodTransit and radial velocity
Habitability statusPotential candidate — not confirmed habitable
Candidate classificationPotentially habitable candidate — not confirmed habitable
Image statusNo resolved surface image; displayed visual is a labelled artist concept
DistanceAbout 48.9 light-years
RadiusAbout 1.73 × Earth
MassAbout 5.6 × Earth
Orbital periodAbout 24.7 days

Travel calculation

How long would the journey take?

Straight-line arithmetic is compared with real mission history. Actual trajectories depend on orbital mechanics, acceleration, braking, launch windows and gravity assists.

At light speed48.9 years299,792 km/s

A physical reference only. A spacecraft with mass cannot reach light speed.

At 10% of light speed489 years29,979 km/s — hypothetical

No operational spacecraft can sustain this interstellar cruise speed.

At 1% of light speed4,890 years2,998 km/s — hypothetical

Still far beyond current spacecraft propulsion.

At Parker Solar Probe peak76,265 yearsAbout 692,000 km/h

Parker reaches this speed only very close to the Sun; it is not an interstellar cruise speed.

At New Horizons launch speed901,590 yearsAbout 58,536 km/h

A comparison using a real high-energy launch from Earth.

At Voyager 1 speed862,344 yearsAbout 61,200 km/h

A practical comparison with a spacecraft already moving into interstellar space.

Research guide

What we know, and what we do not know

What is directly known

The planet itself is not resolved as a detailed globe. Its existence and properties are inferred mainly through transit and radial velocity, together with measurements of the host star.

What remains unknown

Surface geography, oceans, continents, clouds and living organisms have not been directly observed. Atmosphere and composition may also remain uncertain.

What is known

Transit spectroscopy detected time-variable escaping helium in 2024 observations, providing evidence that LHS 1140 b retained an atmosphere; its lower atmospheric composition remains under study.

Habitability limits

An atmosphere is not the same as habitability. Surface pressure, ocean state, clouds, chemistry and day-night climate remain uncertain.

Why it stands out

It is one of the best nearby super-Earths for future atmospheric characterization.

Primary catalog source: Science — 2026 atmosphere study