Kepler-1544 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1544 b is a confirmed super-earth exoplanet orbiting the star Kepler-1544, located approximately 1092.9 light-years (335.09 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0486% across the stellar disk), this world measures 1.78 Earth radii and has a measured mass of 3.82 Earth masses. Combining its mass and radius yields a mean bulk density of 3.73 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.21 g⊕ (11.87 m/s²), and an escape velocity of 16.4 km/s.
In its orbital architecture around Kepler-1544, Kepler-1544 b completes one full revolution every 168.811 Earth days at a semi-major axis of 0.54465 AU (situated at an orbital separation between Mercury's 0.39 AU and Venus's 0.72 AU). Its mean orbital velocity is approximately 35.1 km/s (compared to Earth's 29.8 km/s). The orbit is modeled as circular (e = 0.00), maintaining a constant stellar distance throughout its year.
✓ Classified as a Temperate Habitable Zone Candidate.
With an estimated equilibrium temperature of 269 K (-4°C / +25°F) and an incident stellar irradiance of 0.83 S⊕ (~1,134 W/m²), Kepler-1544 b orbits within the empirical circumstellar habitable zone where a rocky surface under sufficient atmospheric pressure can maintain liquid surface water.
The host star Kepler-1544 is classified as a stellar host with an effective photospheric temperature of 4,886 K, a radius of 0.74 R☉, a mass of 0.81 M☉, an estimated bolometric luminosity of 0.28 L☉. Stellar evolution modeling indicates an estimated stellar age of 2.34 Gyr and a metallicity of [Fe/H] = 0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-1544 shines at apparent V-band magnitude 14.287 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.
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: Kepler · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).
☀️ Host Star Telemetry
| Host Star Name | Kepler-1544 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 4,886 K |
| Stellar Radius | 0.7400 R☉ |
| Stellar Mass | 0.8100 M☉ |
| Bolometric Luminosity | 0.28 L☉ |
| Metallicity [Fe/H] | 0.020 dex |
| Stellar Age | 2.340 Gyr |
| Apparent Magnitude | V: 14.287 · G: 14.039 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.544650 AU |
| Orbital Period | 168.811 days |
| Mean Orbital Velocity | 35.1 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.7970° |
| Mean Bulk Density | 3.73 g/cm³ (16.4 km/s vesc) |
| Insolation Flux | 0.8330 S⊕ (~1,134 W/m²) |
| Habitable Zone Status | ★ Temperate Zone |
| Celestial Distance | 1092.900 LY (335.090 pc) |