STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // Kepler-1276 b
← Return to All Worlds
CONFIRMED EXOPLANET · Terrestrial

Kepler-1276 b

Orbits Host Star: Kepler-1276 · Distance: 1756.300 Light-Years (538.481 pc)
Planetary Radius
1.190 R⊕
Planetary Mass
1.810 M⊕
Surface Gravity
1.28 g / g⊕
Equilibrium Temp
886K (+613°C / +1135°F)
Orbital Period
12.572 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.36 / 1.00
Insolation Flux
139.77 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-1276 b is a confirmed terrestrial exoplanet orbiting the star Kepler-1276, located approximately 1756.3 light-years (538.48 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0081% across the stellar disk), this world measures 1.19 Earth radii and has a measured mass of 1.81 Earth masses. Combining its mass and radius yields a mean bulk density of 5.92 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.28 g⊕ (12.55 m/s²), and an escape velocity of 13.8 km/s.

In its orbital architecture around Kepler-1276, Kepler-1276 b completes one full revolution every 12.572 Earth days at a semi-major axis of 0.10863 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 94 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 886 K (+613°C / +1135°F) and receiving 139.77 S⊕ (~190,227 W/m²), Kepler-1276 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1276 is classified as a stellar host with an effective photospheric temperature of 6,188 K, a radius of 1.21 R☉, a mass of 1.14 M☉, an estimated bolometric luminosity of 1.926 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.09 Gyr and a metallicity of [Fe/H] = -0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-1276 shines at apparent V-band magnitude 12.992 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.36 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-1276
Spectral Type Unclassified
Effective Temp (Teff) 6,188 K
Stellar Radius 1.2100 R☉
Stellar Mass 1.1400 M☉
Bolometric Luminosity 1.926 L☉
Metallicity [Fe/H] -0.020 dex
Stellar Age 3.090 Gyr
Apparent Magnitude V: 12.992 · G: 12.849
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.108630 AU
Orbital Period 12.572 days
Mean Orbital Velocity 94 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 89.2700°
Mean Bulk Density 5.92 g/cm³ (13.8 km/s vesc)
Insolation Flux 139.7700 S⊕ (~190,227 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1756.300 LY (538.481 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h11m25.68s · DEC: +40d32m49.89s (J2000: 287.85702°, 40.54719°)
Target Field: Kepler-1276 (J2000 287.85702°, 40.54719°)
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 ↗
NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗