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CONFIRMED EXOPLANET · Terrestrial

Kepler-1607 b

Orbits Host Star: Kepler-1607 · Distance: 4194.700 Light-Years (1286.100 pc)
Planetary Radius
0.920 R⊕
Planetary Mass
0.721 M⊕
Surface Gravity
0.85 g / g⊕
Equilibrium Temp
913K (+640°C / +1184°F)
Orbital Period
13.647 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.35 / 1.00
Insolation Flux
449.63 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-1607 b is a confirmed terrestrial exoplanet orbiting the star Kepler-1607, located approximately 4194.7 light-years (1286.1 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0049% across the stellar disk), this world measures 0.92 Earth radii and has a measured mass of 0.721 Earth masses. Combining its mass and radius yields a mean bulk density of 5.11 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 0.85 g⊕ (8.34 m/s²), and an escape velocity of 9.9 km/s.

In its orbital architecture around Kepler-1607, Kepler-1607 b completes one full revolution every 13.647 Earth days at a semi-major axis of 0.11978 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 95.5 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 913 K (+640°C / +1184°F) and receiving 449.63 S⊕ (~611,949 W/m²), Kepler-1607 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1607 is classified as a stellar host with an effective photospheric temperature of 6,116 K, a radius of 1.21 R☉, a mass of 1.14 M☉, an estimated bolometric luminosity of 1.838 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.16 Gyr and a metallicity of [Fe/H] = 0.05 dex (near-solar heavy-element abundance). From Earth, Kepler-1607 shines at apparent V-band magnitude 13.969 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.35 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-1607
Spectral Type Unclassified
Effective Temp (Teff) 6,116 K
Stellar Radius 1.2100 R☉
Stellar Mass 1.1400 M☉
Bolometric Luminosity 1.838 L☉
Metallicity [Fe/H] 0.050 dex
Stellar Age 3.160 Gyr
Apparent Magnitude V: 13.969 · G: 13.875
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.119780 AU
Orbital Period 13.647 days
Mean Orbital Velocity 95.5 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 86.4700°
Mean Bulk Density 5.11 g/cm³ (9.9 km/s vesc)
Insolation Flux 449.6320 S⊕ (~611,949 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 4194.700 LY (1286.100 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h44m14.37s · DEC: +42d39m21.81s (J2000: 296.05987°, 42.65606°)
Target Field: Kepler-1607 (J2000 296.05987°, 42.65606°)
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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