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CONFIRMED EXOPLANET · Super-Earth

K2-61 b

Orbits Host Star: K2-61 · Distance: 1323.300 Light-Years (405.732 pc)
Planetary Radius
1.920 R⊕
Planetary Mass
4.350 M⊕
Surface Gravity
1.18 g / g⊕
Equilibrium Temp
1325K (+1052°C / +1926°F)
Orbital Period
2.573 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.20 / 1.00
Insolation Flux
730.00 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-61 b is a confirmed super-earth exoplanet orbiting the star K2-61, located approximately 1323.3 light-years (405.73 parsecs) from the Solar System. First announced in 2016 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0313% across the stellar disk), this world measures 1.92 Earth radii and has a measured mass of 4.35 Earth masses. Combining its mass and radius yields a mean bulk density of 3.39 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.18 g⊕ (11.57 m/s²), and an escape velocity of 16.8 km/s.

In its orbital architecture around K2-61, K2-61 b completes one full revolution every 2.573 Earth days at a semi-major axis of 0.0392 AU (an ultra-close orbit less than one-seventh of Mercury's 0.387 AU distance from the Sun, where strong stellar tidal forces typically induce synchronous rotation). Its mean orbital velocity is approximately 165.7 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1325 K (+1052°C / +1926°F) and receiving 730.00 S⊕ (~993,530 W/m²), K2-61 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-61 is classified as a stellar host with an effective photospheric temperature of 5,748 K, a radius of 0.995 R☉, a mass of 0.97 M☉, an estimated bolometric luminosity of 0.97 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.03 dex (near-solar heavy-element abundance). From Earth, K2-61 shines at apparent V-band magnitude 13.173 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.20 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 K2-61
Spectral Type Unclassified
Effective Temp (Teff) 5,748 K
Stellar Radius 0.9950 R☉
Stellar Mass 0.9700 M☉
Bolometric Luminosity 0.97 L☉
Metallicity [Fe/H] 0.030 dex
Stellar Age —
Apparent Magnitude V: 13.173 · G: 12.858
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.039200 AU
Orbital Period 2.573 days
Mean Orbital Velocity 165.7 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 85.9963°
Mean Bulk Density 3.39 g/cm³ (16.8 km/s vesc)
Insolation Flux 730.0000 S⊕ (~993,530 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1323.300 LY (405.732 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 22h38m41.96s · DEC: -13d33m36.16s (J2000: 339.67484°, -13.56004°)
Target Field: K2-61 (J2000 339.67484°, -13.56004°)
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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