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CONFIRMED EXOPLANET · Super-Earth

PSR B1257+12 c

Orbits Host Star: PSR B1257+12 · Distance: 1956.900 Light-Years (600.000 pc)
Planetary Radius
1.910 R⊕
Planetary Mass
4.300 M⊕
Surface Gravity
1.18 g / g⊕
Equilibrium Temp
—
Orbital Period
66.542 days
Discovery Year
1992 (Pulsar Timing)
Earth Similarity (ESI)
0.80 / 1.00 Moderate

Astrophysical Synthesis & Habitability Characterization

PSR B1257+12 c is a confirmed super-earth exoplanet orbiting the star PSR B1257+12, located approximately 1956.9 light-years (600 parsecs) from the Solar System. First announced in 1992 by Arecibo Observatory using the Pulsar Timing detection technique, this world measures 1.91 Earth radii and has a measured mass of 4.3 Earth masses. Combining its mass and radius yields a mean bulk density of 3.4 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 PSR B1257+12, PSR B1257+12 c completes one full revolution every 66.542 Earth days at a semi-major axis of 0.36 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 58.9 km/s (compared to Earth's 29.8 km/s). With a near-circular eccentricity of e = 0.0186 (ranging from 0.3533 AU at periapsis to 0.3667 AU at apoapsis), the planet experiences minimal orbital distance variation.

ℹ️ Thermal & Atmospheric Regime: Current photometric and spectroscopic constraints for PSR B1257+12 c place it outside the conservative habitable zone definition pending further atmospheric characterization.

The host star PSR B1257+12 is classified as a stellar host with a mass of 1.4 M☉. Stellar evolution modeling indicates an estimated stellar age of 3 Gyr. The PSR B1257+12 system is a multi-planet architecture hosting 3 confirmed worlds, with PSR B1257+12 c sharing its stellar neighborhood alongside PSR B1257+12 b, PSR B1257+12 d.

Earth Similarity Index (ESI): 0.80 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: Arecibo Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name PSR B1257+12
Spectral Type Unclassified
Effective Temp (Teff) —
Stellar Radius —
Stellar Mass 1.4000 M☉
Metallicity [Fe/H] —
Stellar Age 3.000 Gyr
Apparent Magnitude —
System Architecture 1 Star, 3 Planets

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.360000 AU
Orbital Period 66.542 days
Mean Orbital Velocity 58.9 km/s
Orbital Eccentricity (e) 0.01860
Orbital Inclination (i) 53.0000°
Mean Bulk Density 3.4 g/cm³ (16.8 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1956.900 LY (600.000 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 13h00m03.58s · DEC: +12d40m56.5s (J2000: 195.0149°, 12.68235°)
Target Field: PSR B1257+12 (J2000 195.0149°, 12.68235°)
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)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗

Other Worlds in the PSR B1257+12 System (2)

NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗