SPACE PIXEL

Space Codex / Exoplanet reference

Published exoplanet measurements

TOI-2018 b

TOI-2018 b orbits TOI-2018 once every 7.43558 days. The system is about 91.3094 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 7.43558 days, or 0.0203575 Earth years. The listed eccentricity is 0. A zero may be a circular assumption fixed in the fit; consult the paper before treating it as an exact observed shape. 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 2.268 (+0.069 / −0.069) Earth radii. Radius describes size; it does not specify the mass or the atmospheric composition. The mass parameter is 9.2 (+2.1 / −2.1) Earth masses. Its archive provenance is Mass.

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

The host star and received light

The host is cataloged as TOI-2018. The selected row gives spectral type K V. Its reported effective temperature is 4174 K. Its reported radius is 0.62 solar radii. Its reported mass is 0.57 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 TOI-2018

The fetched archive contains 1 selected default planet record for this host. This is the retrieved record set, and additional or revised discoveries may appear in later research.

Planet records for TOI-2018
PlanetPeriod (days)Radius (Earth)Mass parameter (Earth)Mass definition
TOI-2018 b7.43558 (+2.2e-05 / −2.2e-05)2.268 (+0.069 / −0.069)9.2 (+2.1 / −2.1)Mass

Earth comparison

Units and scale comparisons
QuantityReported value or conversionComparison
Orbital period7.43558 days0.0203575 Earth years
System distance27.9956 parsecs91.3094 light-years
Radius2.268 (+0.069 / −0.069)Earth radii; Earth = 1
Mass parameter9.2 (+2.1 / −2.1)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 TOI-2018 b
ParameterValue and reported uncertaintyUnit or definition
Orbital period7.43558 (+2.2e-05 / −2.2e-05)days
Semimajor axisNot reported in this solutionAU
Radius2.268 (+0.069 / −0.069)Earth radii
Mass parameter9.2 (+2.1 / −2.1)Earth masses
Orbital eccentricity0dimensionless
Orbital inclination88.52 (+0.22 / −0.22)degrees
Equilibrium temperatureNot reported in this solutionK; model estimate
Incident fluxNot reported in this solutionEarth flux
Bulk densityNot reported in this solutiong/cm³
Host effective temperature4174 (+34 / −42)K
Host radius0.62 (+0.01 / −0.01)solar radii
Host mass0.57 (+0.02 / −0.02)solar masses
Host metallicity-0.58 (+0.18 / −0.18)dex; archive abundance definition
Host ageNot reported in this solutionbillion years
Host luminosity-1 (+0.04139 / −0.04576)log10 solar luminosity
Host surface gravity4.62 (+0.02 / −0.03)log10 cm/s²
Host rotation period23.5days
System distance27.9956 (+0.0214 / −0.0213)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 referenceDai et al. 2023
Discovery methodTransit
Discovery year2023
Discovery facilityTransiting Exoplanet Survey Satellite (TESS)
Mass provenanceMass
Host stars in system1
Archive system planet count1
Planetary solution publication date2023-08
Row update date2023-06-27
Archive release date2023-06-27

Source: NASA Exoplanet Archive overview for TOI-2018 b, 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.