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CONFIRMED EXOPLANET · Terrestrial

Kepler-1598 b

Orbits Host Star: Kepler-1598 · Distance: 2021.700 Light-Years (619.862 pc)
Planetary Radius
0.950 R⊕
Planetary Mass
0.809 M⊕
Surface Gravity
0.9 g / g⊕
Equilibrium Temp
1236K (+963°C / +1765°F)
Orbital Period
4.342 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.25 / 1.00
Insolation Flux
308.46 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-1598 b is a confirmed terrestrial exoplanet orbiting the star Kepler-1598, located approximately 2021.7 light-years (619.86 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0064% across the stellar disk), this world measures 0.95 Earth radii and has a measured mass of 0.809 Earth masses. Combining its mass and radius yields a mean bulk density of 5.2 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 0.9 g⊕ (8.83 m/s²), and an escape velocity of 10.3 km/s.

In its orbital architecture around Kepler-1598, Kepler-1598 b completes one full revolution every 4.342 Earth days at a semi-major axis of 0.05207 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 130.5 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 1236 K (+963°C / +1765°F) and receiving 308.46 S⊕ (~419,814 W/m²), Kepler-1598 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1598 is classified as a stellar host with an effective photospheric temperature of 5,940 K, a radius of 1.09 R☉, a mass of 1.07 M☉, an estimated bolometric luminosity of 1.327 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.8 Gyr and a metallicity of [Fe/H] = 0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-1598 shines at apparent V-band magnitude 13.929 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.25 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-1598
Spectral Type Unclassified
Effective Temp (Teff) 5,940 K
Stellar Radius 1.0900 R☉
Stellar Mass 1.0700 M☉
Bolometric Luminosity 1.327 L☉
Metallicity [Fe/H] 0.040 dex
Stellar Age 3.800 Gyr
Apparent Magnitude V: 13.929 · G: 13.814
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.052070 AU
Orbital Period 4.342 days
Mean Orbital Velocity 130.5 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 89.4700°
Mean Bulk Density 5.2 g/cm³ (10.3 km/s vesc)
Insolation Flux 308.4600 S⊕ (~419,814 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 2021.700 LY (619.862 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h13m52.59s · DEC: +46d47m01.13s (J2000: 288.46911°, 46.78365°)
Target Field: Kepler-1598 (J2000 288.46911°, 46.78365°)
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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