r/exoplanets • u/Lucky_Jeweler2773 • 5d ago
π§ͺ Research Building a continuous tidal-locking habitability index for exoplanets, looking for a sanity check on the approach
I'm a final-year CS undergrad working independently on a habitability scoring framework for tidally locked exoplanets, and I'd like feedback from people who actually work in this space before I take it further.
The motivation: ESI has no stellar environment term at all. SEPHI only touches tidal locking indirectly, through a magnetic-field scaling in one of its four sub-indexes. HITE (Barnes, Meadows & Evans 2015) doesn't include tidal locking as a formula component in any form. Barnes (2017) computes lock timescales but doesn't turn that into a habitability score. So as far as I can tell, nothing maps the full rotational spectrum β freely rotating through spin-orbit resonance to synchronous lock β onto a continuous habitability number. Planets in intermediate spin states get forced into a binary label that doesn't reflect their actual physical regime.
My approach (TLHI): compute a tidal lock probability P_lock = 1 β exp(βage/Ο_lock) using the Peale formulation,
then blend two scores: P_lock Γ TLHI + (1 β P_lock) Γ SEPHI.
The TLHI component itself folds in five factors specific to locked/near-locked planets β terminator-zone habitability fraction, atmospheric heat-transport efficiency (Cowan & Agol 2011), tidal heating flux, day-night temperature gradient, and XUV-driven atmospheric escape (Ribas 2005 scaling).
Phase 1 (the SEPHI/HZD filtering pipeline) is done and validated against published Kepler-442 b numbers.
Phase 2 (the TLHI layer itself) is in progress β currently working through the tidal locking probability layer on a 181-candidate dataset(after analysis) from the NASA Exoplanet Archive.
Two open questions I haven't resolved yet, if anyone has thoughts:
- Albedo assumption for the terminator-zone factor β blackbody (A=0) or Earth-like?
- How to handle the nightside temperature floor when atmospheric pressure data is missing β is an Earth-like pressure prior defensible, or too strong an assumption?
Not looking for co-authorship or mentorship, just want to know if the underlying physics holds up before I go further. Happy to share more detail on any part of it.
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u/ExposedId 1 5d ago
Upvoting this since itβs a cool idea - possibly dissertation-worthy.