M62H b
Astrophysical Synthesis & Habitability Characterization
M62H b is a confirmed gas giant exoplanet orbiting the star M62H. First announced in 2024 by South African Radio Astronomy Observatory (SARAO) using the Pulsar Timing detection technique, this world has a minimum or true mass of 785.036 Earth masses (2.47 M♃), while its physical transit radius has not yet been geometrically observed.
In its orbital architecture around M62H, M62H b completes one full revolution every 0.133 Earth days.
ℹ️ Thermal & Atmospheric Regime: Current photometric and spectroscopic constraints for M62H b place it outside the conservative habitable zone definition pending further atmospheric characterization.
The host star M62H is classified as a stellar host with a mass of 1.4 M☉.
Discovery Facility: South African Radio Astronomy Observatory (SARAO) · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).
☀️ Host Star Telemetry
| Host Star Name | M62H |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | — |
| Stellar Radius | — |
| Stellar Mass | 1.4000 M☉ |
| Metallicity [Fe/H] | — |
| Stellar Age | — |
| Apparent Magnitude | — |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | — |
| Orbital Period | 0.133 days |
| Orbital Eccentricity (e) | Circular (0.00) |
| Orbital Inclination (i) | — |
| Insolation Flux | — |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | — |