SPACE PIXEL

Space Codex / Exoplanet reference

Published exoplanet measurements

LP 791-18 d

LP 791-18 d orbits LP 791-18 once every 2.75485 days. The system is about 86.4076 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 2.75485 days, or 0.00754237 Earth years. Its reported semimajor axis is 0.01992 AU. That orbital scale is 0.0514598 times Mercury's semimajor axis. The listed eccentricity is 0.0011. Using those central values, the model's nearest and farthest star–planet distances are about 0.0198981 and 0.0199419 AU. These are derived comparisons, without propagated errors. 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 1.032 (+0.044 / −0.043) Earth radii. Radius describes size; it does not specify the mass or the atmospheric composition. The mass parameter is 0.91 (+0.19 / −0.19) Earth masses. Its archive provenance is Mass. The source lists a bulk-density parameter of 4.56 (+1.12 / −1.12) 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 LP 791-18. The selected row gives spectral type M(6.1 +/- 0.7) V. Its reported effective temperature is 2960 K. Its reported radius is 0.182 solar radii. Its reported mass is 0.139 solar masses. 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 LP 791-18

The fetched archive contains 3 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 LP 791-18
PlanetPeriod (days)Radius (Earth)Mass parameter (Earth)Mass definition
LP 791-18 b0.947998 (+2.1e-06 / −2.1e-06)1.212 (+0.059 / −0.058)Not reported in this solutionNot specified
LP 791-18 d2.75485 (+0.00013 / −0.00013)1.032 (+0.044 / −0.043)0.91 (+0.19 / −0.19)Mass
LP 791-18 c4.98991 (+1.2e-06 / −1.4e-06)2.488 (+0.096 / −0.096)7.16 (+0.65 / −0.65)Mass

Earth comparison

Units and scale comparisons
QuantityReported value or conversionComparison
Orbital period2.75485 days0.00754237 Earth years
System distance26.4927 parsecs86.4076 light-years
Orbital scale0.01992 (+0.00024 / −0.00024)AU; Earth = 1
Radius1.032 (+0.044 / −0.043)Earth radii; Earth = 1
Mass parameter0.91 (+0.19 / −0.19)Earth masses; check mass definition

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 LP 791-18 d
ParameterValue and reported uncertaintyUnit or definition
Orbital period2.75485 (+0.00013 / −0.00013)days
Semimajor axis0.01992 (+0.00024 / −0.00024)AU
Radius1.032 (+0.044 / −0.043)Earth radii
Mass parameter0.91 (+0.19 / −0.19)Earth masses
Orbital eccentricity0.0011 (+0.001 / −0.0008)dimensionless
Orbital inclination89.34 (+0.41 / −0.41)degrees
Equilibrium temperatureNot reported in this solutionK; model estimate
Incident fluxNot reported in this solutionEarth flux
Bulk density4.56 (+1.12 / −1.12)g/cm³
Host effective temperature2960 (+55 / −55)K
Host radius0.182 (+0.007 / −0.007)solar radii
Host mass0.139 (+0.005 / −0.005)solar masses
Host metallicity-0.09 (+0.19 / −0.19)dex; archive abundance definition
Host ageLower limit: 0.5billion years
Host luminosity-2.63827 (+0.00188 / −0.00189)log10 solar luminosity
Host surface gravity5.115 (+0.094 / −0.094)log10 cm/s²
Host rotation periodNot reported in this solutiondays
System distance26.4927 (+0.064 / −0.0638)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 referenceGreklek-McKeon et al. 2025
Discovery methodTransit
Discovery year2023
Discovery facilitySpitzer Space Telescope
Mass provenanceMass
Host stars in system1
Archive system planet count3
Planetary solution publication date2025-08
Row update date2026-02-26
Archive release date2026-02-26

Source: NASA Exoplanet Archive overview for LP 791-18 d, 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.