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CONFIRMED EXOPLANET · Gas Giant

BD-14 3065 b

Orbits Host Star: BD-14 3065 A · Distance: 1922.400 Light-Years (589.423 pc)
Planetary Radius
21.590 R⊕
Planetary Mass
3932.000 M⊕
Surface Gravity
8.44 g / g⊕
Equilibrium Temp
2001K (+1728°C / +3142°F)
Orbital Period
4.289 days
Discovery Year
2024 (Transit)
Earth Similarity (ESI)
0.06 / 1.00
Insolation Flux
646.76 S⊕

Astrophysical Synthesis & Habitability Characterization

BD-14 3065 b is a confirmed gas giant exoplanet orbiting the star BD-14 3065 A, located approximately 1922.4 light-years (589.42 parsecs) from the Solar System. First announced in 2024 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.7094% across the stellar disk), this world measures 21.59 Earth radii (1.93 Jupiter radii) and has a measured mass of 3932 Earth masses (12.37 Jupiter masses). Combining its mass and radius yields a mean bulk density of 2.15 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 8.44 g⊕ (82.77 m/s²), and an escape velocity of 151 km/s.

In its orbital architecture around BD-14 3065 A, BD-14 3065 b completes one full revolution every 4.289 Earth days at a semi-major axis of 0.0656 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 166.4 km/s (compared to Earth's 29.8 km/s). Its moderate orbital eccentricity of e = 0.066 carries the world between 0.0613 AU at periapsis and 0.0699 AU at apoapsis, driving measurable seasonal insolation cycles.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 2001 K (+1728°C / +3142°F) and receiving 646.76 S⊕ (~880,242 W/m²), BD-14 3065 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star BD-14 3065 A is classified as a stellar host with an effective photospheric temperature of 6,935 K, a radius of 2.35 R☉, a mass of 1.41 M☉, an estimated bolometric luminosity of 11.461 L☉. Stellar evolution modeling indicates an estimated stellar age of 2.24 Gyr and a metallicity of [Fe/H] = -0.34 dex (metal-poor relative to the Sun). From Earth, BD-14 3065 A shines at apparent V-band magnitude 11.1 (faint and requiring research-grade or CCD telescopic photometry) in the Southern 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 BD-14 3065 A
Spectral Type Unclassified
Effective Temp (Teff) 6,935 K
Stellar Radius 2.3500 R☉
Stellar Mass 1.4100 M☉
Bolometric Luminosity 11.461 L☉
Metallicity [Fe/H] -0.340 dex
Stellar Age 2.240 Gyr
Apparent Magnitude V: 11.100 · G: 10.910
System Architecture 3 Stars, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.065600 AU
Orbital Period 4.289 days
Mean Orbital Velocity 166.4 km/s
Orbital Eccentricity (e) 0.06600
Orbital Inclination (i) 80.7800°
Mean Bulk Density 2.15 g/cm³ (151 km/s vesc)
Insolation Flux 646.7610 S⊕ (~880,242 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1922.400 LY (589.423 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 10h14m40.72s · DEC: -15d38m34.21s (J2000: 153.66967°, -15.64284°)
Target Field: BD-14 3065 A (J2000 153.66967°, -15.64284°)
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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