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CONFIRMED EXOPLANET · Sub-Neptune

TOI-697 b

Orbits Host Star: TOI-697 · Distance: 305.800 Light-Years (93.771 pc)
Planetary Radius
2.359 R⊕
Planetary Mass
6.160 M⊕
Surface Gravity
1.11 g / g⊕
Equilibrium Temp
840K (+567°C / +1053°F)
Orbital Period
8.608 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.31 / 1.00
Insolation Flux
117.55 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-697 b is a confirmed sub-neptune exoplanet orbiting the star TOI-697, located approximately 305.8 light-years (93.77 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 0.0499% across the stellar disk), this world measures 2.359 Earth radii and has a measured mass of 6.16 Earth masses. Combining its mass and radius yields a mean bulk density of 2.59 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.11 g⊕ (10.89 m/s²), and an escape velocity of 18.1 km/s.

In its orbital architecture around TOI-697, TOI-697 b completes one full revolution every 8.608 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 840 K (+567°C / +1053°F) and receiving 117.55 S⊕ (~159,985 W/m²), TOI-697 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-697 is classified as a stellar host with an effective photospheric temperature of 5,682 K, a radius of 0.9681 R☉, a mass of 0.97 M☉, an estimated bolometric luminosity of 0.876 L☉. From Earth, TOI-697 shines at apparent V-band magnitude 10.004 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.31 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-697
Spectral Type Unclassified
Effective Temp (Teff) 5,682 K
Stellar Radius 0.9681 R☉
Stellar Mass 0.9700 M☉
Bolometric Luminosity 0.876 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.004 · G: 9.827
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 8.608 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.5417°
Mean Bulk Density 2.59 g/cm³ (18.1 km/s vesc)
Insolation Flux 117.5495 S⊕ (~159,985 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 305.800 LY (93.771 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 04h38m49.01s · DEC: -36d40m52.77s (J2000: 69.70422°, -36.68133°)
Target Field: TOI-697 (J2000 69.70422°, -36.68133°)
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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