I Gesuiti americani espulsi in Italia e Joaquín Camaño (1767-1814)

Joaquín Camaño fu un gesuita della Provincia del Paraguay, vissuto nell' esilio italiano la maggior parte della sua vita dal 1767 al 1820. Il suo lavoro e la sua fama possono essere considerati di minore importanza se paragonati a molti altri gesuiti esiliati per ordine di Carlo III alla fine del XVIII secolo in Emilia-Romagna. Attraverso la mia ricerca approfondisco il ruolo di J. Camaño quale personaggio minore che entra nella vita degli altri espulsi tramite un dinamico network relazionale di cui è stato uno dei principali artefici. Il mio obiettivo è stato quello di studiare l'impatto che ebbero gli esuli gesuiti americani, attraverso la vita di Joaquin Camaño, sul mondo intellettuale italiano, europeo ed americano dopo l'espulsione del 1767. Egli, con i suoi studi, si inserisce nella rinnovata e vivace retorica del “Mondo Nuovo” che in quegli anni assume un grande dinamismo. Nato nella modesta città di La Rioja, in Argentina, si erge come un brillante cartografo, etnografo e linguista nel contesto dell'Illustrazione europea grazie alla sua particolare vita da missionario. Dopo l'espulsione, Joaquin Camaño, insieme ad altri numerosi confratelli americani, arriverà a Faenza, nello Stato Pontificio, dedicandosi allo studio della cartografia, dell'etnografia e delle lingue americane. Le sue ricerche si collocano in un momento nevralgico per la storia del pensiero linguistico-antropologico, quando l'osservazione diretta e la riflessione teorica dei fenomeni si misuravano con la grande varietà umana ormai riscontrata nel mondo.

Deep ocean ventilation, carbon isotopes, marine sedimentation and the deglacial CO2 rise

The link between the atmospheric CO2 level and the ventilation state of the deep ocean is an important building block of the key hypotheses put forth to explain glacial-interglacial CO2 fluctuations. In this study, we systematically examine the sensitivity of atmospheric CO2 and its carbon isotope composition to changes in deep ocean ventilation, the ocean carbon pumps, and sediment formation in a global three-dimensional ocean-sediment carbon cycle model. Our results provide support for the hypothesis that a break up of Southern Ocean stratification and invigorated deep ocean ventilation were the dominant drivers for the early deglacial CO2 rise of ~35 ppm between the Last Glacial Maximum and 14.6 ka BP. Another rise of 10 ppm until the end of the Holocene is attributed to carbonate compensation responding to the early deglacial change in ocean circulation. Our reasoning is based on a multi-proxy analysis which indicates that an acceleration of deep ocean ventilation during the early deglaciation is not only consistent with recorded atmospheric CO2 but also with the reconstructed opal sedimentation peak in the Southern Ocean at around 16 ka BP, the record of atmospheric δ13CCO2, and the reconstructed changes in the Pacific CaCO3 saturation horizon.

Deep ocean ventilation, carbon isotopes, marine sedimentation and the deglacial CO2 rise

The link between the atmospheric CO2 level and the ventilation state of the deep ocean is an important building block of the key hypotheses put forth to explain glacial-interglacial CO2 fluctuations. In this study, we systematically examine the sensitivity of atmospheric CO2 and its carbon isotope composition to changes in deep ocean ventilation, the ocean carbon pumps, and sediment formation in a global 3-D ocean-sediment carbon cycle model. Our results provide support for the hypothesis that a break up of Southern Ocean stratification and invigorated deep ocean ventilation were the dominant drivers for the early deglacial CO2 rise of ~35 ppm between the Last Glacial Maximum and 14.6 ka BP. Another rise of 10 ppm until the end of the Holocene is attributed to carbonate compensation responding to the early deglacial change in ocean circulation. Our reasoning is based on a multi-proxy analysis which indicates that an acceleration of deep ocean ventilation during early deglaciation is not only consistent with recorded atmospheric CO2 but also with the reconstructed opal sedimentation peak in the Southern Ocean at around 16 ka BP, the record of atmospheric δ13CCO2, and the reconstructed changes in the Pacific CaCO3 saturation horizon.

Detrital Zircon Evidence for Mixing of Mazatzal Province Age Detritus With Yavapai Age (ca. 1700-1740 Ma) and Older Detritus in the ca. 1650 Ma Mazatzal Province of Central New Mexico, USA

Preliminary detrital zircon age distributions from Mazatzal crustal province quartzite and schist exposed in the Manzano Mountains and Pedernal Hills of central New Mexico are consistent with a mixture of detritus from Mazatzal age (ca. 1650 Ma), Yavapai age (ca. 1720 Ma.), and older sources. A quartzite sample from the Blue Springs Formation in the Manzano Mountains yielding 67 concordant grain analyses shows two dominant age peaks of 1737 Ma and 1791 Ma with a minimum peak age of 1652 Ma. Quartzite and micaceous quartzite samples from near Pedernal Peak give unimodal peak ages of ca. 1695 Ma and 1738 Ma with minimum detrital zircon ages of ca. 1625 Ma and 1680 Ma, respectively. A schist sample from the southern exposures of the Pedernal Hills area gives a unimodal peak age of 1680 Ma with a minimum age of ca. 1635 Ma. Minor amounts of older detritus (>1800 Ma) possibly reflect Trans-Hudson, Wyoming, Mojave Province, and older Archean sources and aid in locating potential source terrains for these detrital zircon. The Blue Springs Formation metarhyolite from near the top of the Proterozoic section in the Manzano Mountains yields 71 concordant grains that show a preliminary U-Pb zircon crystallization age of 1621 ¿ 5 Ma, which provides a minimum age constraint for deposition in the Manzano Mountains. Normalized probability plots from this study are similar to previously reported age distributions in the Burro and San Andres Mountains in southern New Mexico and suggest that Yavapai Province age detritus was deposited and intermingled with Mazatzal Province age detritus across much of the Mazatzal crustal province in New Mexico. This data shows that the tectonic evolution of southwestern Laurentia is associated with multiple orogenic events. Regional metamorphism and deformation in the area must postdate the Mazatzal Orogeny and ca. 1610 Ma ¿ 1620 Ma rhyolite crystallization and is attributed to the Mesoproterozoic ca. 1400 ¿ 1480 Ma Picuris Orogeny.

Sulle tracce del primo Neoclassicismo. Il viaggio del principe ereditario Friedrich Christian di Sassonia in Italia (1738-1740)

Vom 13. Mai 1738 bis zum 7. September 1740 befindet sich der sächsische Kurprinz Friedrich Christian (1722-1764) auf seiner Italienreise. Sein eigenhändig geschriebenes Reisejournal, sowie die Berichte seines Tutors geben einen tiefen Einblick über das aktuelle Kunstgeschehen in Rom. Friedrich Christian wird durch die Fürsorge der Kardinäle Alessandro und Annibale Albani mit der intellektuellen Elite und mit den namhaftesten in Rom wirkenden Künstlern sowie mit der Kunst Raphaels und der bolognesisch-römischen Barock-Klassizisten bekannt beziehungsweise vertraut gemacht. In der römischen Akademie der Arkadier und in der Académie de France kommt er mit dem Ideal der Simplizität und der 'Nachahmung' der Antike in Berührung. Auf seinem Rückweg von Rom nach Venedig ist hierfür der Aufenthalt bei Scipione Maffei in Verona bezeichnend. In Venedig schließlich kann im besonderen Friedrich Christians Kenntnis von der Inventarisation des dortigen 'Statuario Pubblico', der ehemaligen Antikensammlung in der Antisala der Bibliothek von San Marco verzeichnet werden. Friedrich Christian kehrte mit diesen neuen Eindrücken nach Dresden zurück, wo Anton Raphael Mengs seine Karriere als Künstler begann und ein paar Jahre später sich Johann Joachim Winckelmann aufhielt. Unter der Obhut des Kardinals Alessandro Albani sollten Mengs und Winckelmann dann in Rom die malerische und theoretische Grundlage für den Klassizismus schaffen.