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CONFIRMED EXOPLANET · Gas Giant

TOI-1036 b

Orbits Host Star: TOI-1036 · Distance: 600.200 Light-Years (184.015 pc)
Planetary Radius
6.285 R⊕
Planetary Mass
32.500 M⊕
Surface Gravity
0.82 g / g⊕
Equilibrium Temp
1294K (+1021°C / +1870°F)
Orbital Period
3.78 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.13 / 1.00
Insolation Flux
466.53 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1036 b is a confirmed gas giant exoplanet orbiting the star TOI-1036, located approximately 600.2 light-years (184.02 parsecs) from the Solar System. First announced in 2026 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.2403% across the stellar disk), this world measures 6.285 Earth radii (0.56 Jupiter radii) and has a measured mass of 32.5 Earth masses (0.1 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.72 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.82 g⊕ (8.04 m/s²), and an escape velocity of 25.4 km/s.

In its orbital architecture around TOI-1036, TOI-1036 b completes one full revolution every 3.78 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1294 K (+1021°C / +1870°F) and receiving 466.53 S⊕ (~634,945 W/m²), TOI-1036 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1036 is classified as a stellar host with an effective photospheric temperature of 5,665 K, a radius of 1.1755 R☉, a mass of 1.03 M☉, an estimated bolometric luminosity of 1.277 L☉. From Earth, TOI-1036 shines at apparent V-band magnitude 10.973 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.13 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-1036
Spectral Type Unclassified
Effective Temp (Teff) 5,665 K
Stellar Radius 1.1755 R☉
Stellar Mass 1.0300 M☉
Bolometric Luminosity 1.277 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.973 · G: 10.737
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 3.78 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.1760°
Mean Bulk Density 0.72 g/cm³ (25.4 km/s vesc)
Insolation Flux 466.5280 S⊕ (~634,945 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 600.200 LY (184.015 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 10h31m28.11s · DEC: -42d14m25.61s (J2000: 157.86711°, -42.24045°)
Target Field: TOI-1036 (J2000 157.86711°, -42.24045°)
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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