Consiglio Nazionale delle Ricerche

Tipo di prodottoArticolo in rivista
TitoloGeological evolution of the Sinus Iridum basin
Anno di pubblicazione2020
Formato-
Autore/iHu T.; Kang Z.; Massironi M.; Hiesinger H.; van der Bogert C.H.; Gamba P.; Brunetti M.T.; Melis M.T.
Affiliazioni autoriChina University of Geosciences in Beijing, Xueyuan Road 29, Haidian District, Beijing, 100083, Chinese University of Geosciences in Beijing, China University of Geosciences, Xueyuan Road, Beijing, 100083 China, , China; Department of Geosciences, University of Padua, Via Gradenigo 6, Padova, 35131, University of Padua, Via G. Gradenigo 6, 35131 Padova, Italy, , Italy; Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Str. 10, Münster, 48149, Institut fur Planetologie, Westfalische Wilhelms-Universitat Munster, Wilhelm-Klemm-Str. 10, 48149 Munster, Germany, , Germany; Department of Electrical, Computer and Biomedical Engineering, University of Pavia, Pavia, 27100, Department of Electrical, Computer and Biomedical Engineering, University of Pavia, 27100 Pavia, Italy, , Italy; Research Institute for Geo-Hydrological Protection Italian National Research Council, Via Madonna Alta 126, Perugia, 06128, CNR IRPI, Via Madonna Alta 126, 06128 Perugia, Italy, , Italy; Department of Chemical and Geological Sciences, University of Cagliari, via Trentino 51, Cagliari, 09127, Department of Chemical and Geological Sciences, University of Cagliari, Via Trentino 51-09127 Cagliari, , Italy
Autori CNR e affiliazioni
  • MARIA TERESA BRUNETTI
Lingua/e
  • inglese
AbstractAs a semi-enclosed crater basin on the northwest rim of Imbrium basin, Sinus Iridum is a key site to investigate the geological characteristics at the intersection of two basins. For this reason, we focused on model age determination in Sinus Iridum basin using Chang'E-2 high-resolution images coupled with compositional maps from the Clementine data sets, as well as with digital elevation models (DEMs) from the Lunar Orbiter Laser Altimeter (LOLA) onboard the Lunar Reconnaissance Orbiter (LRO). With these datasets we identified different geologic units onto which we performed model age determinations based on crater counting. This systematic analysis of the Sinus Iridum basin shows that the age of the oldest exposed basaltic unit is 3.37 Ga (Imbrian age), while the youngest, a mare basalt unit that enters the basin from Imbrium basin, is 1.24 Ga (late Eratosthenian). In general, the ages of the geologic units inside the Sinus Iridum basin gradually decrease from the northeast to the southwest, with the only exception of the young units being located in the north-eastern area. We conclude that the crater size-frequency distributions (CSFD) reflect a multi-layer sequence, suggesting multiple resurfacing events inside Sinus Iridum. The model age determinations identify several infilling events of basalts ranging from 3.37 Ga to 1.24 Ga, which are all derived mare basalt flows from the Imbrium basin.
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RivistaPlanetary and space science
Attiva dal 1959
Editore: Pergamon Press. - New York
Paese di pubblicazione: Regno Unito
Lingua: inglese
ISSN: 0032-0633
Titolo chiave: Planetary and space science
Titolo proprio: Planetary and space science.
Titolo abbreviato: Planet. space sci.
Numero volume della rivista194
Fascicolo della rivista-
DOI10.1016/j.pss.2020.105134
Verificato da refereeSì: Internazionale
Stato della pubblicazionePublished version
Indicizzazione (in banche dati controllate)
  • Scopus (Codice:2-s2.0-85095859200)
Parole chiaveSinus iridum, Age determination, Crater counting, Geological analysis
Link (URL, URI)http://www.scopus.com/record/display.url?eid=2-s2.0-85095859200&origin=inward
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Strutture CNR
  • IRPI — Istituto di ricerca per la protezione idrogeologica
Moduli/Attività/Sottoprogetti CNR-
Progetti Europei-
Allegati
Geological evolution of the Sinus Iridum basin (documento privato )
Tipo documento: application/pdf