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CONFIRMED EXOPLANET · Sub-Neptune

Kepler-513 b

Orbits Host Star: Kepler-513 · Distance: 1527.300 Light-Years (468.258 pc)
Planetary Radius
2.200 R⊕
Planetary Mass
5.480 M⊕
Surface Gravity
1.13 g / g⊕
Equilibrium Temp
623K (+350°C / +662°F)
Orbital Period
28.862 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.43 / 1.00
Insolation Flux
36.53 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-513 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-513, located approximately 1527.3 light-years (468.26 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0362% across the stellar disk), this world measures 2.2 Earth radii and has a measured mass of 5.48 Earth masses. Combining its mass and radius yields a mean bulk density of 2.84 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.13 g⊕ (11.08 m/s²), and an escape velocity of 17.7 km/s.

In its orbital architecture around Kepler-513, Kepler-513 b completes one full revolution every 28.862 Earth days at a semi-major axis of 0.1779 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 67.1 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 623 K (+350°C / +662°F) and receiving 36.53 S⊕ (~49,713 W/m²), Kepler-513 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-513 is classified as a stellar host with an effective photospheric temperature of 5,849 K, a radius of 1.06 R☉, a mass of 1.02 M☉, an estimated bolometric luminosity of 1.18 L☉. Stellar evolution modeling indicates an estimated stellar age of 5.5 Gyr and a metallicity of [Fe/H] = -0.01 dex (near-solar heavy-element abundance). From Earth, Kepler-513 shines at apparent V-band magnitude 13.019 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.43 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-513
Spectral Type Unclassified
Effective Temp (Teff) 5,849 K
Stellar Radius 1.0600 R☉
Stellar Mass 1.0200 M☉
Bolometric Luminosity 1.18 L☉
Metallicity [Fe/H] -0.010 dex
Stellar Age 5.500 Gyr
Apparent Magnitude V: 13.019 · G: 12.882
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.177900 AU
Orbital Period 28.862 days
Mean Orbital Velocity 67.1 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 88.3500°
Mean Bulk Density 2.84 g/cm³ (17.7 km/s vesc)
Insolation Flux 36.5270 S⊕ (~49,713 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1527.300 LY (468.258 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h00m09.99s · DEC: +50d04m31.41s (J2000: 285.04162°, 50.07539°)
Target Field: Kepler-513 (J2000 285.04162°, 50.07539°)
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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