Why it matters
Menrva shows that crater scarcity is also scientific information: Titan's surface can hide and rework impact traces.
Measurements and uncertainty
Extended record: core parameters have an editorial baseline, while age, depth, and preservation still require primary-source review.
Profil scientifique
Titan requires radar and infrared reading: crater morphology here is tied to atmosphere, precipitation, and organic materials.
Galerie de reconstruction
Davantage de lectures visuelles du cratère
Si l'image vérifiée ne suffit pas, la fiche reçoit une reconstruction scientifique : non pas de la fantaisie à la place du fait, mais une hypothèse visuelle séparée des sources.
Visual reconstruction
Reverse reconstruction → Chronological inversion → Bidirectional analysis → The present as an archive of the future
Chaque fiche doit avoir un aperçu visuel : image existante, source traitée esthétiquement ou reconstruction scientifique.
Historique de recherche
The name was adopted by the IAU in 2006; the feature is known from Cassini data and official nomenclature.
Sources
- Last reviewed
- 2026-05-08
- Source baseline
- Gazetteer of Planetary Nomenclature; NASA Image and Video Library
- Uncertainty note
- Extended record: core parameters have an editorial baseline, while age, depth, and preservation still require primary-source review.
Education mode
Faits
- Official diameter: about 392 km.
- Titan has a dense atmosphere, making craters rare.
- Menrva connects craters with the theme of active surfaces.
