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CONFIRMED EXOPLANET · Sub-Neptune

K2-71 b

Orbits Host Star: K2-71 · Distance: 499.600 Light-Years (153.192 pc)
Planetary Radius
2.150 R⊕
Planetary Mass
5.270 M⊕
Surface Gravity
1.14 g / g⊕
Equilibrium Temp
533K (+260°C / +500°F)
Orbital Period
6.985 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.50 / 1.00
Insolation Flux
13.40 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-71 b is a confirmed sub-neptune exoplanet orbiting the star K2-71, located approximately 499.6 light-years (153.19 parsecs) from the Solar System. First announced in 2016 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.2141% across the stellar disk), this world measures 2.15 Earth radii and has a measured mass of 5.27 Earth masses. Combining its mass and radius yields a mean bulk density of 2.92 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.14 g⊕ (11.18 m/s²), and an escape velocity of 17.5 km/s.

In its orbital architecture around K2-71, K2-71 b completes one full revolution every 6.985 Earth days at a semi-major axis of 0.0559 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 87.1 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 533 K (+260°C / +500°F) and receiving 13.40 S⊕ (~18,237 W/m²), K2-71 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-71 is classified as a stellar host with an effective photospheric temperature of 4,006 K, a radius of 0.426 R☉, a mass of 0.477 M☉, an estimated bolometric luminosity of 0.042 L☉. From Earth, K2-71 shines at apparent V-band magnitude 16.14 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.50 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 K2-71
Spectral Type Unclassified
Effective Temp (Teff) 4,006 K
Stellar Radius 0.4260 R☉
Stellar Mass 0.4770 M☉
Bolometric Luminosity 0.042 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 16.140 · G: 15.189
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.055900 AU
Orbital Period 6.985 days
Mean Orbital Velocity 87.1 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.92 g/cm³ (17.5 km/s vesc)
Insolation Flux 13.4000 S⊕ (~18,237 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 499.600 LY (153.192 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 22h46m53.97s · DEC: -09d52m53.80s (J2000: 341.72487°, -9.88161°)
Target Field: K2-71 (J2000 341.72487°, -9.88161°)
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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