STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // TOI-907.01
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CONFIRMED EXOPLANET · Gas Giant

TOI-907.01

Orbits Host Star: TOI-907 · Distance: 1019.300 Light-Years (312.529 pc)
Planetary Radius
9.616 R⊕
Planetary Mass
67.000 M⊕
Surface Gravity
0.72 g / g⊕
Equilibrium Temp
1847K (+1574°C / +2865°F)
Orbital Period
4.585 days
Discovery Year
2024 (Transit)
Earth Similarity (ESI)
0.07 / 1.00
Insolation Flux
1,729.67 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-907.01 is a confirmed gas giant exoplanet orbiting the star TOI-907, located approximately 1019.3 light-years (312.53 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 0.1832% across the stellar disk), this world measures 9.616 Earth radii (0.86 Jupiter radii) and has a measured mass of 67 Earth masses (0.21 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.42 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.72 g⊕ (7.06 m/s²), and an escape velocity of 29.5 km/s.

In its orbital architecture around TOI-907, TOI-907.01 completes one full revolution every 4.585 Earth days at a semi-major axis of 0.055225 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 131 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1847 K (+1574°C / +2865°F) and receiving 1,729.67 S⊕ (~2,354,083 W/m²), TOI-907.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-907 is classified as a stellar host with an effective photospheric temperature of 6,272 K, a radius of 2.0598 R☉, a mass of 1.0694 M☉, an estimated bolometric luminosity of 5.891 L☉. From Earth, TOI-907 shines at apparent V-band magnitude 10.394 (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: Transiting Exoplanet Survey Satellite (TESS) · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name TOI-907
Spectral Type Unclassified
Effective Temp (Teff) 6,272 K
Stellar Radius 2.0598 R☉
Stellar Mass 1.0694 M☉
Bolometric Luminosity 5.891 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.394 · G: 10.327
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.055225 AU
Orbital Period 4.585 days
Mean Orbital Velocity 131 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 0.42 g/cm³ (29.5 km/s vesc)
Insolation Flux 1729.6714 S⊕ (~2,354,083 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1019.300 LY (312.529 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 17h28m44.02s · DEC: -62d50m25.38s (J2000: 262.18341°, -62.84038°)
Target Field: TOI-907 (J2000 262.18341°, -62.84038°)
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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