SPACE PIXEL

Space Codex / Exoplanet reference

Published exoplanet measurements

LHS 1140 c

LHS 1140 c orbits LHS 1140 once every 3.77794 days. The system is about 48.8781 light-years from Earth.

Archive retrieved November 1, 2026 (America/New_York). The selected paper and archive update dates appear below.

The recorded orbit

The selected archive solution gives an orbital period of 3.77794 days, or 0.0103434 Earth years. Its reported semimajor axis is 0.027 AU. That orbital scale is 0.0697498 times Mercury's semimajor axis. The listed eccentricity is 0.05. The period measures a year on this planet. It does not establish the length of its rotation or the duration of daylight.

Read how orbital period, size, and eccentricity fit together.

Size and mass

The radius parameter is 1.272 (+0.026 / −0.026) Earth radii. Radius describes size; it does not specify the mass or the atmospheric composition. The mass parameter is 1.91 (+0.06 / −0.06) Earth masses. Its archive provenance is Mass. The source lists a bulk-density parameter of 5.1 (+0.4 / −0.4) g/cm³. Different interior mixtures can overlap in density; the value does not identify a unique surface.

Compare rocky planets, sub-Neptunes, and giant planets.

The host star and received light

The host is cataloged as LHS 1140. The selected row gives spectral type M4.5 V. Its reported effective temperature is 3096 K. Its reported radius is 0.2159 solar radii. Its reported mass is 0.1844 solar masses. The planet's incident-flux parameter is 5.3 (+0.4 / −0.4) times Earth's received stellar flux. The equilibrium-temperature entry is 422 (+7 / −7) K. This is a model quantity, not a measured surface temperature. The available stellar and orbital entries do not establish a breathable atmosphere, surface water, or life.

What a habitable-zone claim does and does not mean · How a star changes over time.

Other planets around LHS 1140

The fetched archive contains 2 selected default planet records for this host. This is the retrieved record set, and additional or revised discoveries may appear in later research.

Planet records for LHS 1140
PlanetPeriod (days)Radius (Earth)Mass parameter (Earth)Mass definition
LHS 1140 c3.77794 (+2e-06 / −2e-06)1.272 (+0.026 / −0.026)1.91 (+0.06 / −0.06)Mass
LHS 1140 b24.7372 (+2e-05 / −2e-05)1.73 (+0.025 / −0.025)5.6 (+0.19 / −0.19)Mass

Earth comparison

Units and scale comparisons
QuantityReported value or conversionComparison
Orbital period3.77794 days0.0103434 Earth years
System distance14.9861 parsecs48.8781 light-years
Orbital scale0.027 (+0.0005 / −0.0005)AU; Earth = 1
Radius1.272 (+0.026 / −0.026)Earth radii; Earth = 1
Mass parameter1.91 (+0.06 / −0.06)Earth masses; check mass definition
Received stellar flux5.3 (+0.4 / −0.4)Earth flux; Earth = 1

Conversions use rounded central values. They are navigation aids for the data, not additional observations. Uncertainties for the original parameters remain in the next table.

Measurement table

Selected published solution for LHS 1140 c
ParameterValue and reported uncertaintyUnit or definition
Orbital period3.77794 (+2e-06 / −2e-06)days
Semimajor axis0.027 (+0.0005 / −0.0005)AU
Radius1.272 (+0.026 / −0.026)Earth radii
Mass parameter1.91 (+0.06 / −0.06)Earth masses
Orbital eccentricityUpper limit: 0.05dimensionless
Orbital inclination89.8 (+0.14 / −0.19)degrees
Equilibrium temperature422 (+7 / −7)K; model estimate
Incident flux5.3 (+0.4 / −0.4)Earth flux
Bulk density5.1 (+0.4 / −0.4)g/cm³
Host effective temperature3096 (+48 / −48)K
Host radius0.2159 (+0.003 / −0.003)solar radii
Host mass0.1844 (+0.0045 / −0.0045)solar masses
Host metallicity-0.15 (+0.09 / −0.09)dex; archive abundance definition
Host ageLower limit: 5billion years
Host luminosity-2.42022 (+0.033 / −0.03572)log10 solar luminosity
Host surface gravity5.041 (+0.016 / −0.016)log10 cm/s²
Host rotation period131days
System distance14.9861 (+0.0153 / −0.0152)parsecs

Parentheses show the reported upper and lower uncertainties when both are supplied. Bounds are explicitly labeled. A missing entry means unavailable in this solution, not zero. The confidence convention belongs to the source paper.

Research record and limitations

Discovery and provenance
RecordValue
Planetary referenceCadieux et al. 2024
Discovery methodTransit
Discovery year2018
Discovery facilityMultiple Observatories
Mass provenanceMass
Host stars in system1
Archive system planet count2
Planetary solution publication date2024-01
Row update date2024-03-04
Archive release date2024-03-04

Source: NASA Exoplanet Archive overview for LHS 1140 c, Planetary Systems table, default solution. The collection excludes entries flagged controversial at retrieval. A selected default is a published reference choice, not a claim that every parameter is the latest estimate in all literature.

This profile documents measurements and their scope. It is separate from the 3D planet catalog and does not create a sponsorship placement or a new explorer destination.