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CONFIRMED EXOPLANET · Gas Giant

HATS-42 b

Orbits Host Star: HATS-42 · Distance: 2610.500 Light-Years (800.377 pc)
Planetary Radius
15.693 R⊕
Planetary Mass
597.520 M⊕
Surface Gravity
2.43 g / g⊕
Equilibrium Temp
1856K (+1583°C / +2881°F)
Orbital Period
2.292 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.07 / 1.00
Insolation Flux
1,637.21 S⊕

Astrophysical Synthesis & Habitability Characterization

HATS-42 b is a confirmed gas giant exoplanet orbiting the star HATS-42, located approximately 2610.5 light-years (800.38 parsecs) from the Solar System. First announced in 2018 by HATSouth using the Transit detection technique (producing an estimated primary transit depth of 0.945% across the stellar disk), this world measures 15.693 Earth radii (1.4 Jupiter radii) and has a measured mass of 597.52 Earth masses (1.88 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.85 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 2.43 g⊕ (23.83 m/s²), and an escape velocity of 69 km/s.

In its orbital architecture around HATS-42, HATS-42 b completes one full revolution every 2.292 Earth days at a semi-major axis of 0.03689 AU (an ultra-close orbit less than one-seventh of Mercury's 0.387 AU distance from the Sun, where strong stellar tidal forces typically induce synchronous rotation). Its mean orbital velocity is approximately 175.1 km/s (compared to Earth's 29.8 km/s). Its moderate orbital eccentricity of e = 0.229 carries the world between 0.0284 AU at periapsis and 0.0453 AU at apoapsis, driving measurable seasonal insolation cycles.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1856 K (+1583°C / +2881°F) and receiving 1,637.21 S⊕ (~2,228,237 W/m²), HATS-42 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star HATS-42 is classified as a stellar host with an effective photospheric temperature of 6,060 K, a radius of 1.48 R☉, a mass of 1.273 M☉, an estimated bolometric luminosity of 2.65 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.26 Gyr and a metallicity of [Fe/H] = 0.22 dex (metal-rich relative to the Sun). From Earth, HATS-42 shines at apparent V-band magnitude 13.682 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.07 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: HATSouth · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name HATS-42
Spectral Type Unclassified
Effective Temp (Teff) 6,060 K
Stellar Radius 1.4800 R☉
Stellar Mass 1.2730 M☉
Bolometric Luminosity 2.65 L☉
Metallicity [Fe/H] 0.220 dex
Stellar Age 3.260 Gyr
Apparent Magnitude V: 13.682 · G: 13.563
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.036890 AU
Orbital Period 2.292 days
Mean Orbital Velocity 175.1 km/s
Orbital Eccentricity (e) 0.22900
Orbital Inclination (i) 85.1000°
Mean Bulk Density 0.85 g/cm³ (69 km/s vesc)
Insolation Flux 1637.2058 S⊕ (~2,228,237 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 2610.500 LY (800.377 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 07h13m48.58s · DEC: -33d26m14.45s (J2000: 108.4524°, -33.43735°)
Target Field: HATS-42 (J2000 108.4524°, -33.43735°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
Aladin Lite v3 · Centre de Données astronomiques de Strasbourg (CDS)
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