STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // TOI-1516 b
← Return to All Worlds
CONFIRMED EXOPLANET · Gas Giant

TOI-1516 b

Orbits Host Star: TOI-1516 (Type F8 V) · Distance: 805.800 Light-Years (247.054 pc)
Planetary Radius
15.244 R⊕
Planetary Mass
1004.338 M⊕
Surface Gravity
4.32 g / g⊕
Equilibrium Temp
1839K (+1566°C / +2851°F)
Orbital Period
2.056 days
Discovery Year
2022 (Transit)
Earth Similarity (ESI)
0.07 / 1.00
Insolation Flux
1,899.83 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1516 b is a confirmed gas giant exoplanet orbiting the star TOI-1516, located approximately 805.8 light-years (247.05 parsecs) from the Solar System. First announced in 2022 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 1.5029% across the stellar disk), this world measures 15.244 Earth radii (1.36 Jupiter radii) and has a measured mass of 1004.338 Earth masses (3.16 Jupiter masses). Combining its mass and radius yields a mean bulk density of 1.56 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 4.32 g⊕ (42.36 m/s²), and an escape velocity of 90.8 km/s.

In its orbital architecture around TOI-1516, TOI-1516 b completes one full revolution every 2.056 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1839 K (+1566°C / +2851°F) and receiving 1,899.83 S⊕ (~2,585,669 W/m²), TOI-1516 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1516 is classified as a warm F-type star of spectral type F8 V with an effective photospheric temperature of 6,520 K, a radius of 1.14 R☉, a mass of 1.14 M☉, an estimated bolometric luminosity of 2.107 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.82 Gyr and a metallicity of [Fe/H] = -0.05 dex (near-solar heavy-element abundance). From Earth, TOI-1516 shines at apparent V-band magnitude 10.858 (faint and requiring research-grade or CCD telescopic photometry) in the Northern 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-1516
Spectral Type F8 V
Effective Temp (Teff) 6,520 K
Stellar Radius 1.1400 R☉
Stellar Mass 1.1400 M☉
Bolometric Luminosity 2.107 L☉
Metallicity [Fe/H] -0.050 dex
Stellar Age 4.820 Gyr
Apparent Magnitude V: 10.858 · G: 10.716
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 2.056 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 90.0000°
Mean Bulk Density 1.56 g/cm³ (90.8 km/s vesc)
Insolation Flux 1899.8300 S⊕ (~2,585,669 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 805.800 LY (247.054 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 22h40m20.31s · DEC: +69d30m13.43s (J2000: 340.08462°, 69.50373°)
Target Field: TOI-1516 (J2000 340.08462°, 69.50373°)
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 ↗