Why it matters
Mead sets the scale for the Venus section and asks the interface to explain radar imagery.
Measurements and uncertainty
Extended record: core parameters have an editorial baseline, while age, depth, and preservation still require primary-source review.
Profil scientifique
The structure shows ring morphology, radar-bright ejecta, and the relationship between impact forms and Venusian terrain.
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
Its detailed image is primarily associated with Magellan radar mapping.
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
- Venus has few very small craters because of its dense atmosphere.
- Mead is named after anthropologist Margaret Mead.

