BEBOP-4 AB b
Astrophysical Synthesis & Habitability Characterization
BEBOP-4 AB b is a confirmed gas giant exoplanet orbiting the star BEBOP-4 A, located approximately 764.2 light-years (234.29 parsecs) from the Solar System. First announced in 2025 by Haute-Provence Observatory using the Radial Velocity detection technique (measuring periodic Doppler reflex motion in the host star's spectrum), this world has a minimum or true mass of 8358.887 Earth masses (26.3 M♃), while its physical transit radius has not yet been geometrically observed.
In its orbital architecture around BEBOP-4 A, BEBOP-4 AB b completes one full revolution every 1823.5 Earth days (4.99Julian years) at a semi-major axis of 3.634 AU (corresponding to the middle-system regime between Mars at 1.52 AU and Jupiter at 5.20 AU). Its mean orbital velocity is approximately 21.7 km/s (compared to Earth's 29.8 km/s). The planet follows a highly eccentric trajectory (e = 0.428, swinging from 2.0786 AU at periapsis out to 5.1894 AU at apoapsis), pointing to past dynamical scattering or secular gravitational perturbations.
✓ Classified as a Temperate Habitable Zone Candidate.
With an estimated equilibrium temperature of 239 K (-34°C / -29°F) and an incident stellar irradiance of 0.55 S⊕ (~745 W/m²), BEBOP-4 AB b orbits within the empirical circumstellar habitable zone where a rocky surface under sufficient atmospheric pressure can maintain liquid surface water.
The host star BEBOP-4 A is classified as a solar-type yellow star of spectral type G3 V with an effective photospheric temperature of 5,701 K, a radius of 2.7565 R☉, a mass of 1.507 M☉, an estimated bolometric luminosity of 7.201 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.262 dex (metal-rich relative to the Sun). From Earth, BEBOP-4 A shines at apparent V-band magnitude 9.646 (accessible to binoculars and small amateur telescopes) in the Northern celestial hemisphere.
Discovery Facility: Haute-Provence Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).
☀️ Host Star Telemetry
| Host Star Name | BEBOP-4 A |
| Spectral Type | G3 V |
| Effective Temp (Teff) | 5,701 K |
| Stellar Radius | 2.7565 R☉ |
| Stellar Mass | 1.5070 M☉ |
| Bolometric Luminosity | 7.201 L☉ |
| Metallicity [Fe/H] | 0.262 dex |
| Stellar Age | — |
| Apparent Magnitude | V: 9.646 · G: 9.433 |
| System Architecture | 2 Stars, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 3.634000 AU |
| Orbital Period | 1823.5 days |
| Mean Orbital Velocity | 21.7 km/s |
| Orbital Eccentricity (e) | 0.42800 |
| Orbital Inclination (i) | — |
| Insolation Flux | 0.5477 S⊕ (~745 W/m²) |
| Habitable Zone Status | ★ Temperate Zone |
| Celestial Distance | 764.200 LY (234.294 pc) |