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CONFIRMED EXOPLANET · Sub-Neptune

K2-277 b

Orbits Host Star: K2-277 · Distance: 369.000 Light-Years (113.123 pc)
Planetary Radius
2.186 R⊕
Planetary Mass
7.400 M⊕
Surface Gravity
1.55 g / g⊕
Equilibrium Temp
1049K (+776°C / +1429°F)
Orbital Period
6.327 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.26 / 1.00
Insolation Flux
195.00 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-277 b is a confirmed sub-neptune exoplanet orbiting the star K2-277, located approximately 369 light-years (113.12 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0424% across the stellar disk), this world measures 2.186 Earth radii and has a measured mass of 7.4 Earth masses. Combining its mass and radius yields a mean bulk density of 3.91 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.55 g⊕ (15.2 m/s²), and an escape velocity of 20.6 km/s.

In its orbital architecture around K2-277, K2-277 b completes one full revolution every 6.327 Earth days at a semi-major axis of 0.0664 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 114.2 km/s (compared to Earth's 29.8 km/s). The planet follows a highly eccentric trajectory (e = 0.52, swinging from 0.0319 AU at periapsis out to 0.1009 AU at apoapsis), pointing to past dynamical scattering or secular gravitational perturbations.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1049 K (+776°C / +1429°F) and receiving 195.00 S⊕ (~265,395 W/m²), K2-277 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-277 is classified as a stellar host with an effective photospheric temperature of 5,680 K, a radius of 0.973 R☉, a mass of 0.974 M☉, an estimated bolometric luminosity of 0.884 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.9 Gyr and a metallicity of [Fe/H] = 0.078 dex (metal-rich relative to the Sun). From Earth, K2-277 shines at apparent V-band magnitude 10.364 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.26 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 K2-277
Spectral Type Unclassified
Effective Temp (Teff) 5,680 K
Stellar Radius 0.9730 R☉
Stellar Mass 0.9740 M☉
Bolometric Luminosity 0.884 L☉
Metallicity [Fe/H] 0.078 dex
Stellar Age 4.900 Gyr
Apparent Magnitude V: 10.364 · G: 10.121
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.066400 AU
Orbital Period 6.327 days
Mean Orbital Velocity 114.2 km/s
Orbital Eccentricity (e) 0.52000
Orbital Inclination (i) 86.8300°
Mean Bulk Density 3.91 g/cm³ (20.6 km/s vesc)
Insolation Flux 195.0000 S⊕ (~265,395 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 369.000 LY (113.123 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 13h28m03.89s · DEC: -15d56m16.71s (J2000: 202.01619°, -15.93797°)
Target Field: K2-277 (J2000 202.01619°, -15.93797°)
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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