KIC 10001893 b
KIC 10001893 b orbits the star KIC 10001893, 5,456.4 light-years from Earth. It completes an orbit in 0.22 Earth days.
Get to know this world ↓Size-based classification; composition may be uncertain.
Time to complete one orbit.
Its light travels for roughly 5,456 years to reach us.
Orbital Brightness Modulation
Overview
KIC 10001893 b is one of the confirmed worlds in the NASA Exoplanet Archive. Recorded as discovered in 2014. The credited discovery facility is Kepler. Its Orbital Brightness Modulation evidence gives us a way to study a planet that is usually too faint to see directly.
Its radius is not currently available in this catalogue, so we leave its size class unassigned.
The planet
A reliable mass is not available in this record.
Mass and radius constrain possible interiors; multiple compositions can fit a given set of measurements.
Orbit & year
A year here lasts 0.22 Earth days.
Host star
Planetary system
3 confirmed planets are stored for this star.
KIC 10001893 b · 0.22-day orbit
KIC 10001893 c · 0.325-day orbit
KIC 10001893 d · 0.812-day orbit
Discovery
Reported discovery year: 2014. Method: Orbital Brightness Modulation. Facility: Kepler.
First stored in this atlas: 04/10/2026. This is an ingestion date, not a confirmation date.
How these methods work ↗Potential habitability
The data here does not establish habitability, liquid water, or life. An appropriate atmosphere and many other conditions would be needed.
Understand the habitable zone ↗What do we actually know?
The underlying light, motion or timing signal. Usually not a photograph of the planet.
Parameters derived from observations, with instrument and model uncertainty.
Our light-year conversion and browsing class are calculated from archive values.
Equilibrium temperature is an energy-balance estimate, not surface weather.
Possible composition depends on models and may not be unique.
Surface conditions and the presence of life are not established here.
Measured signals are interpreted through models. The archive’s composite table combines published values and may include calculated estimates. Values do not necessarily form one self-consistent solution.
Radius and mass can be estimated or inferred, orbital period comes from recurring observations, and size classification is calculated by this site. Atmospheric and surface conditions remain unknown unless established by specific observations.
Consult the archive for individual parameter references and uncertainty intervals before scientific use.
Scientific data
| Orbital period | 0.2197 Earth days |
|---|---|
| Host star temperature | 27,500 K |
| Host star mass | 0.47 Solar masses |
| Host star radius | 0.18 Solar radii |
| Distance | 1,672.94 parsecs |
| Discovery year | 2,014 |
| Discovery method | Orbital Brightness Modulation |
| Discovery facility | Kepler |
| Discovery publication | 2014-10 |
Uncertainties and parameter provenance
Archive uncertainty ranges and published references, where available. A missing uncertainty does not imply an exact value.
| Parameter | Uncertainty / source |
|---|---|
| Orbital period | Upper uncertainty unavailable / Lower uncertainty unavailableSilvotti et al. 2014 |
Sources
NASA Exoplanet Archive · Planetary Systems Composite Parameters (PSCompPars).
Open the scientific archive record ↗Last changed in this atlas: 04/10/2026, 11:39:41. Read our methodology.