Pelvis Polus Australis–Aitken est depressio lata et profunda in superficie illius faciei lunaris quae a Tellure non videtur.
Depressio ovoides a polo, extremitate australi, usque ad craterem minorem Aitken, extremitate boreali, extendit. Relictum esse censetur crateris illisionis lunae et omnis systematis solaris maximi, aevo praenectario annos plures quam 3 900 000 000 a.p. facti. Vestigia gravia meteoritae vel asteroidis, cuius lapsu crater factus est, sub pelvi etiam hodie latent.
Natura huius pelvis a D. E. Wilhelms et collegas iam intellecta est. Forma et profunditas praecipue in operibus Pauli Spudis patefactae sunt explorationis gratia speculatri spatialis Clementine Speculatrum Sinense Chang'e 4 die 3 Ianuarii 2019 ad craterem Von Kármán in hac regione ad specimina mineralium adprehenda advenit.
Vicimedia Communia plura habent quae ad pelvem Polus Australis–Aitken spectant. |
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