STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // BEBOP-4 AB b
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CONFIRMED EXOPLANET · Gas Giant ★ TEMPERATE HABITABLE ZONE

BEBOP-4 AB b

Orbits Host Star: BEBOP-4 A (Type G3 V) · Distance: 764.200 Light-Years (234.294 pc)
Planetary Radius
—
Planetary Mass
8358.887 M⊕
Surface Gravity
—
Equilibrium Temp
239K (-34°C / -29°F)
Orbital Period
1823.5 days
Discovery Year
2025 (Radial Velocity)
Insolation Flux
0.55 S⊕

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)

🔭 Deep Space Viewport // Host Star Field

RA: 12h50m18.54s · DEC: +26d09m34.33s (J2000: 192.57727°, 26.15954°)
Target Field: BEBOP-4 A (J2000 192.57727°, 26.15954°)
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)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗
NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗