HATS-42 b
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.
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) |