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CONFIRMED EXOPLANET · Super-Earth

Kepler-1986 b

Orbits Host Star: Kepler-1986 · Distance: 2974.800 Light-Years (912.085 pc)
Planetary Radius
1.890 R⊕
Planetary Mass
4.230 M⊕
Surface Gravity
1.18 g / g⊕
Equilibrium Temp
579K (+306°C / +583°F)
Orbital Period
19.549 days
Discovery Year
2023 (Transit)
Earth Similarity (ESI)
0.48 / 1.00
Insolation Flux
26.62 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-1986 b is a confirmed super-earth exoplanet orbiting the star Kepler-1986, located approximately 2974.8 light-years (912.09 parsecs) from the Solar System. First announced in 2023 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.056% across the stellar disk), this world measures 1.89 Earth radii and has a measured mass of 4.23 Earth masses. Combining its mass and radius yields a mean bulk density of 3.45 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.18 g⊕ (11.57 m/s²), and an escape velocity of 16.7 km/s.

In its orbital architecture around Kepler-1986, Kepler-1986 b completes one full revolution every 19.549 Earth days at a semi-major axis of 0.1307 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 72.7 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 579 K (+306°C / +583°F) and receiving 26.62 S⊕ (~36,230 W/m²), Kepler-1986 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1986 is classified as a stellar host with an effective photospheric temperature of 5,549 K, a radius of 0.732 R☉, a mass of 0.776 M☉, an estimated bolometric luminosity of 0.456 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.54 dex (metal-poor relative to the Sun). From Earth, Kepler-1986 shines at apparent V-band magnitude 15.661 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.48 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-1986
Spectral Type Unclassified
Effective Temp (Teff) 5,549 K
Stellar Radius 0.7320 R☉
Stellar Mass 0.7760 M☉
Bolometric Luminosity 0.456 L☉
Metallicity [Fe/H] -0.540 dex
Stellar Age —
Apparent Magnitude V: 15.661 · G: 15.718
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.130700 AU
Orbital Period 19.549 days
Mean Orbital Velocity 72.7 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 89.0500°
Mean Bulk Density 3.45 g/cm³ (16.7 km/s vesc)
Insolation Flux 26.6200 S⊕ (~36,230 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 2974.800 LY (912.085 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h31m49.99s · DEC: +42d51m17.61s (J2000: 292.95827°, 42.85489°)
Target Field: Kepler-1986 (J2000 292.95827°, 42.85489°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
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