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CONFIRMED EXOPLANET · Sub-Neptune

Kepler-281 b

Orbits Host Star: Kepler-281 · Distance: 5692.900 Light-Years (1745.450 pc)
Planetary Radius
2.820 R⊕
Planetary Mass
324.000 M⊕
Surface Gravity
40.74 g / g⊕
Equilibrium Temp
694K (+421°C / +790°F)
Orbital Period
14.646 days
Discovery Year
2014 (Transit)
Earth Similarity (ESI)
0.18 / 1.00
Insolation Flux
118.25 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-281 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-281, located approximately 5692.9 light-years (1745.45 parsecs) from the Solar System. First announced in 2014 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0827% across the stellar disk), this world measures 2.82 Earth radii and has a measured mass of 324 Earth masses (1.02 Jupiter masses). Combining its mass and radius yields a mean bulk density of 79.66 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 40.74 g⊕ (399.52 m/s²), and an escape velocity of 119.9 km/s.

In its orbital architecture around Kepler-281, Kepler-281 b completes one full revolution every 14.646 Earth days at a semi-major axis of 0.117 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 86.9 km/s (compared to Earth's 29.8 km/s). The orbit is modeled as circular (e = 0.00), maintaining a constant stellar distance throughout its year.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 694 K (+421°C / +790°F) and receiving 118.25 S⊕ (~160,933 W/m²), Kepler-281 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-281 is classified as a stellar host with an effective photospheric temperature of 5,723 K, a radius of 0.899 R☉, a mass of 0.95 M☉, an estimated bolometric luminosity of 0.778 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.6 Gyr and a metallicity of [Fe/H] = 0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-281 shines at apparent V-band magnitude 15.931 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-281 system is a multi-planet architecture hosting 3 confirmed worlds, with Kepler-281 b sharing its stellar neighborhood alongside Kepler-281 c, Kepler-281 d.

Earth Similarity Index (ESI): 0.18 Earth Baseline = 1.00
0.00 Dissimilar 0.50 Mars Scale 0.70 Analog Regime 1.00 Earth

Methodology: Computed using the Schulze-Makuch et al. (2011) weighted metric comparing physical interior (radius, estimated density) and surface thermal regime (escape velocity, equilibrium temperature).

Discovery Facility: Kepler · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name Kepler-281
Spectral Type Unclassified
Effective Temp (Teff) 5,723 K
Stellar Radius 0.8990 R☉
Stellar Mass 0.9500 M☉
Bolometric Luminosity 0.778 L☉
Metallicity [Fe/H] 0.020 dex
Stellar Age 0.600 Gyr
Apparent Magnitude V: 15.931 · G: 15.754
System Architecture 1 Star, 3 Planets

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.117000 AU
Orbital Period 14.646 days
Mean Orbital Velocity 86.9 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 88.0900°
Mean Bulk Density 79.66 g/cm³ (119.9 km/s vesc)
Insolation Flux 118.2460 S⊕ (~160,933 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 5692.900 LY (1745.450 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h36m25.96s · DEC: +44d46m14.35s (J2000: 294.10815°, 44.77065°)
Target Field: Kepler-281 (J2000 294.10815°, 44.77065°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
Aladin Lite v3 · Centre de Données astronomiques de Strasbourg (CDS)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗

Other Worlds in the Kepler-281 System (2)

NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
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