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CONFIRMED EXOPLANET · Super-Earth

Kepler-753 b

Orbits Host Star: Kepler-753 · Distance: 896.200 Light-Years (274.767 pc)
Planetary Radius
1.910 R⊕
Planetary Mass
4.310 M⊕
Surface Gravity
1.18 g / g⊕
Equilibrium Temp
641K (+368°C / +694°F)
Orbital Period
5.748 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.44 / 1.00
Insolation Flux
41.67 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-753 b is a confirmed super-earth exoplanet orbiting the star Kepler-753, located approximately 896.2 light-years (274.77 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0726% across the stellar disk), this world measures 1.91 Earth radii and has a measured mass of 4.31 Earth masses. Combining its mass and radius yields a mean bulk density of 3.41 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 16.8 km/s.

In its orbital architecture around Kepler-753, Kepler-753 b completes one full revolution every 5.748 Earth days at a semi-major axis of 0.054 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 102.2 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 641 K (+368°C / +694°F) and receiving 41.67 S⊕ (~56,718 W/m²), Kepler-753 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-753 is classified as a stellar host with an effective photospheric temperature of 4,346 K, a radius of 0.65 R☉, a mass of 0.68 M☉, an estimated bolometric luminosity of 0.135 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.63 Gyr and a metallicity of [Fe/H] = -0.03 dex (near-solar heavy-element abundance). From Earth, Kepler-753 shines at apparent V-band magnitude 14.891 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.44 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-753
Spectral Type Unclassified
Effective Temp (Teff) 4,346 K
Stellar Radius 0.6500 R☉
Stellar Mass 0.6800 M☉
Bolometric Luminosity 0.135 L☉
Metallicity [Fe/H] -0.030 dex
Stellar Age 3.630 Gyr
Apparent Magnitude V: 14.891 · G: 14.475
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.054000 AU
Orbital Period 5.748 days
Mean Orbital Velocity 102.2 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 88.3300°
Mean Bulk Density 3.41 g/cm³ (16.8 km/s vesc)
Insolation Flux 41.6740 S⊕ (~56,718 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 896.200 LY (274.767 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h27m36.78s · DEC: +37d54m08.52s (J2000: 291.90324°, 37.90237°)
Target Field: Kepler-753 (J2000 291.90324°, 37.90237°)
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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