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CONFIRMED EXOPLANET · Gas Giant

Kepler-719 b

Orbits Host Star: Kepler-719 · Distance: 8145.800 Light-Years (2497.510 pc)
Planetary Radius
8.520 R⊕
Planetary Mass
54.500 M⊕
Surface Gravity
0.75 g / g⊕
Equilibrium Temp
998K (+725°C / +1337°F)
Orbital Period
5.007 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.15 / 1.00
Insolation Flux
234.28 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-719 b is a confirmed gas giant exoplanet orbiting the star Kepler-719, located approximately 8145.8 light-years (2497.51 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.6353% across the stellar disk), this world measures 8.52 Earth radii (0.76 Jupiter radii) and has a measured mass of 54.5 Earth masses (0.17 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.49 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.75 g⊕ (7.35 m/s²), and an escape velocity of 28.3 km/s.

In its orbital architecture around Kepler-719, Kepler-719 b completes one full revolution every 5.007 Earth days at a semi-major axis of 0.0556 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 120.8 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 998 K (+725°C / +1337°F) and receiving 234.28 S⊕ (~318,855 W/m²), Kepler-719 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-719 is classified as a stellar host with an effective photospheric temperature of 5,777 K, a radius of 0.98 R☉, a mass of 0.99 M☉, an estimated bolometric luminosity of 0.96 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.98 Gyr and a metallicity of [Fe/H] = -0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-719 shines at apparent V-band magnitude 16.128 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.15 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-719
Spectral Type Unclassified
Effective Temp (Teff) 5,777 K
Stellar Radius 0.9800 R☉
Stellar Mass 0.9900 M☉
Bolometric Luminosity 0.96 L☉
Metallicity [Fe/H] -0.020 dex
Stellar Age 3.980 Gyr
Apparent Magnitude V: 16.128 · G: 15.904
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.055600 AU
Orbital Period 5.007 days
Mean Orbital Velocity 120.8 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 87.8700°
Mean Bulk Density 0.49 g/cm³ (28.3 km/s vesc)
Insolation Flux 234.2800 S⊕ (~318,855 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 8145.800 LY (2497.510 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h42m08.66s · DEC: +43d53m03.88s (J2000: 295.53606°, 43.88441°)
Target Field: Kepler-719 (J2000 295.53606°, 43.88441°)
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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