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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1243 b

Orbits Host Star: TOI-1243 (Type M2.0 V) · Distance: 140.900 Light-Years (43.187 pc)
Planetary Radius
2.330 R⊕
Planetary Mass
7.700 M⊕
Surface Gravity
1.42 g / g⊕
Equilibrium Temp
450K (+177°C / +351°F)
Orbital Period
4.659 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.58 / 1.00
Insolation Flux
17.27 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1243 b is a confirmed sub-neptune exoplanet orbiting the star TOI-1243, located approximately 140.9 light-years (43.19 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 0.1747% across the stellar disk), this world measures 2.33 Earth radii and has a measured mass of 7.7 Earth masses. Combining its mass and radius yields a mean bulk density of 3.36 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.42 g⊕ (13.93 m/s²), and an escape velocity of 20.3 km/s.

In its orbital architecture around TOI-1243, TOI-1243 b completes one full revolution every 4.659 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 450 K (+177°C / +351°F) and receiving 17.27 S⊕ (~23,500 W/m²), TOI-1243 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1243 is classified as a low-mass red dwarf of spectral type M2.0 V with an effective photospheric temperature of 3,515 K, a radius of 0.511 R☉, a mass of 0.515 M☉, an estimated bolometric luminosity of 0.036 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.2 dex (metal-poor relative to the Sun). From Earth, TOI-1243 shines at apparent V-band magnitude 13.427 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.58 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-1243
Spectral Type M2.0 V
Effective Temp (Teff) 3,515 K
Stellar Radius 0.5110 R☉
Stellar Mass 0.5150 M☉
Bolometric Luminosity 0.036 L☉
Metallicity [Fe/H] -0.200 dex
Stellar Age —
Apparent Magnitude V: 13.427 · G: 12.359
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 4.659 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.2400°
Mean Bulk Density 3.36 g/cm³ (20.3 km/s vesc)
Insolation Flux 17.2664 S⊕ (~23,500 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 140.900 LY (43.187 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 09h02m55.83s · DEC: +71d38m11.10s (J2000: 135.73264°, 71.63642°)
Target Field: TOI-1243 (J2000 135.73264°, 71.63642°)
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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