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CONFIRMED EXOPLANET · Gas Giant

HAT-P-47 b

Orbits Host Star: HAT-P-47 (Type F) · Distance: 920.100 Light-Years (282.096 pc)
Planetary Radius
14.717 R⊕
Planetary Mass
65.473 M⊕
Surface Gravity
0.3 g / g⊕
Equilibrium Temp
1605K (+1332°C / +2430°F)
Orbital Period
4.732 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.06 / 1.00
Insolation Flux
379.57 S⊕

Astrophysical Synthesis & Habitability Characterization

HAT-P-47 b is a confirmed gas giant exoplanet orbiting the star HAT-P-47, located approximately 920.1 light-years (282.1 parsecs) from the Solar System. First announced in 2026 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.7931% across the stellar disk), this world measures 14.717 Earth radii (1.31 Jupiter radii) and has a measured mass of 65.473 Earth masses (0.21 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.11 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.3 g⊕ (2.94 m/s²), and an escape velocity of 23.6 km/s.

In its orbital architecture around HAT-P-47, HAT-P-47 b completes one full revolution every 4.732 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1605 K (+1332°C / +2430°F) and receiving 379.57 S⊕ (~516,591 W/m²), HAT-P-47 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star HAT-P-47 is classified as a warm F-type star of spectral type F with an effective photospheric temperature of 6,703 K, a radius of 1.515 R☉, a mass of 1.387 M☉, an estimated bolometric luminosity of 4.157 L☉. Stellar evolution modeling indicates an estimated stellar age of 1.5 Gyr and a metallicity of [Fe/H] = -0.026 dex (near-solar heavy-element abundance). From Earth, HAT-P-47 shines at apparent V-band magnitude 10.609 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.06 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: Transiting Exoplanet Survey Satellite (TESS) · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name HAT-P-47
Spectral Type F
Effective Temp (Teff) 6,703 K
Stellar Radius 1.5150 R☉
Stellar Mass 1.3870 M☉
Bolometric Luminosity 4.157 L☉
Metallicity [Fe/H] -0.026 dex
Stellar Age 1.500 Gyr
Apparent Magnitude V: 10.609 · G: 10.547
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 4.732 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 84.5600°
Mean Bulk Density 0.11 g/cm³ (23.6 km/s vesc)
Insolation Flux 379.5670 S⊕ (~516,591 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 920.100 LY (282.096 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 02h33m13.94s · DEC: +30d21m37.63s (J2000: 38.30807°, 30.36045°)
Target Field: HAT-P-47 (J2000 38.30807°, 30.36045°)
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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