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CONFIRMED EXOPLANET · Sub-Neptune

K2-380 b

Orbits Host Star: K2-380 · Distance: 813.100 Light-Years (249.303 pc)
Planetary Radius
2.729 R⊕
Planetary Mass
7.890 M⊕
Surface Gravity
1.06 g / g⊕
Equilibrium Temp
—
Orbital Period
9.401 days
Discovery Year
2022 (Transit)
Earth Similarity (ESI)
0.67 / 1.00

Astrophysical Synthesis & Habitability Characterization

K2-380 b is a confirmed sub-neptune exoplanet orbiting the star K2-380, located approximately 813.1 light-years (249.3 parsecs) from the Solar System. First announced in 2022 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0359% across the stellar disk), this world measures 2.729 Earth radii and has a measured mass of 7.89 Earth masses. Combining its mass and radius yields a mean bulk density of 2.14 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.06 g⊕ (10.4 m/s²), and an escape velocity of 19 km/s.

In its orbital architecture around K2-380, K2-380 b completes one full revolution every 9.401 Earth days.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 2.729 R⊕, K2-380 b exceeds the empirical ~1.8–2.2 R⊕ Fulton radius valley threshold, indicating a substantial hydrogen-helium or supercritical volatile envelope without a conventional solid terrestrial surface.

The host star K2-380 is classified as a stellar host with an effective photospheric temperature of 5,911 K, a radius of 1.32 R☉, a mass of 0.993 M☉, an estimated bolometric luminosity of 1.908 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.049 dex (near-solar heavy-element abundance). From Earth, K2-380 shines at apparent V-band magnitude 11.688 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.67 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: K2 · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name K2-380
Spectral Type Unclassified
Effective Temp (Teff) 5,911 K
Stellar Radius 1.3200 R☉
Stellar Mass 0.9930 M☉
Bolometric Luminosity 1.908 L☉
Metallicity [Fe/H] -0.049 dex
Stellar Age —
Apparent Magnitude V: 11.688 · G: 11.442
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 9.401 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.14 g/cm³ (19 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 813.100 LY (249.303 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 18h53m44.31s · DEC: -26d32m19.43s (J2000: 283.43464°, -26.53873°)
Target Field: K2-380 (J2000 283.43464°, -26.53873°)
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)
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NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
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