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Xenarchus and the reception of aristotle’s physics in antiquity
Xenarchus’ criticism of the thesis that the heavens are made of a special simple body, unique to them, was preserved and passed on to late antiquity by Alexander of Aphrodisias. Alexander is ultimately responsible for its integration into the ancient commentary tradition. The role that Xenarchus plays in this tradition can be usefully contrasted with the one played by Eudemus of Rhodes. Eudemus was not only a direct pupil of Aristotle; with the exception of Theophrastus, he was also the most prominent Peripatetic philosopher of his time. What we know about his Physics suggests that Eudemus followed the sequence of topic discussed in Aristotle's Physics very closely – so closely that it is tempting to consider him an interpreter (exegetês) of Aristotle's Physics. Because of what is perceived as loyalty to Aristotle, his views are often cited by Simplicius in his commentary on Aristotle's Physics. There, Eudemus is regarded as an exegetical aid in the exposition of Aristotle's text. By contrast, Xenarchus is treated as an adversary whose objections are to be answered in order to reaffirm the transcendence of the heavens. It is telling that his affiliation to the Peripatos is not recorded by Simplicius. This silence is symptomatic of the role that Xenarchus ended up playing in the commentary tradition. Seen through the lens of a pro-Aristotelian exegesis that ultimately goes back to Alexander of Aphrodisias, Xenarchus played the outsider within the Peripatetic tradition. This role does not do full justice to Xenarchus – or so I have argued.
A study of the reasons which may have led a Peripatetic philosopher like Xenarchus to criticize Aristotle's celestial physics helps us to better appreciate how unusual Aristotle's conception of the natural world was in antiquity. Several aspects of this conception were strongly resisted. But nothing generated more controversy than Aristotle's views on the material composition of the heavens. The mixed reception of these views indicates that his conception of the celestial world was truly exceptional, if not even anomalous. When we say that for Aristotle the natural world consisted of a celestial and a sublunary part, we do not do full justice to his position. In antiquity it was common to think of the celestial world as a somehow special region of the world. Stability and incorruptibility were often given as its differentiating features. In fact, the position recommended by Aristotle was much stronger than a generic commitment to the incorruptibility and stability of the celestial world. Aristotle was committed to the existence of material discontinuity between the celestial and the sublunary regions of this world. The so-called fifth substance or fifth body is not just different from earth, water, air, or fire. At least for Aristotle, this substance cannot be reduced to any of them. The expressions “fifth body” and “fifth substance,” which Aristotle never uses in his writings on natural philosophy, are themselves an indication of how many, if not most, people felt about Aristotle's celestial simple body in antiquity. They felt that this was an additional body, or an additional substance, alongside earth, water, air, and fire whose theoretical necessity was at best very dubious.
Xenarchus of Seleucia is best known for his vigorous criticism of Aristotle's thesis that the celestial bodies are made of a special simple body, unique to them: the fifth substance, also known as the fifth body, fifth element, quinta essentia, or aither. However, his activity was not confined to the study of physics, let alone celestial physics. Although the surviving evidence is slim, and at times frustratingly so, there is no doubt that Xenarchus was concerned with issues of ethics and psychology as well as of physics. In this book I consider all areas of his activity in order to offer as complete a picture of Xenarchus as our sources permit.
For two reasons, particular emphasis is placed on Xenarchus’ criticism of Aristotle's doctrine of the fifth substance. The first reason is that the sophistication and ingenuity involved in this criticism presuppose a close textual study of Aristotle's works. This study led Xenarchus to a brilliant revision of the conceptual apparatus developed in Aristotle's writings on natural philosophy. Xenarchus elaborated a creative interpretation of Aristotle's theory of natural motion which made the celestial simple body expendable. There is conceptual discontinuity between this creative interpretation and what we know about the Hellenistic theories of motion. Xenarchus developed his theory of natural motion as a direct response to Aristotle's theory of motion. His critical engagement with Aristotle strongly suggests that his activity is best understood in the context of the return to Aristotle which took place in the first century bce. While some of his views are rooted in the philosophical debates of the late Hellenistic period, his activity as a whole presupposes the distance from Aristotle that confronted post-Hellenistic philosophers. In Xenarchus’ case, this distance prompted direct attention to Aristotle's text.
From Strabo we learn that Xenarchus was originally from Seleucia on the Calycadnus in Cilicia Tracheia, but that he spent most of his life away from home, teaching philosophy first in Alexandria, then in Athens, and finally in Rome [T1]. Strabo adds that he himself attended Xenarchus’ lectures. Finally, he names two people that must have been very important in Xenarchus’ life: Arius and the emperor Augustus. Arius is Arius of Alexandria, a philosopher who may have been the same person as the doxographer Arius Didymus and the Stoic philosopher listed on the index locupletior to Diogenes Laertius’ Lives. Arius was not only a friend, a teacher, and a confidant of Augustus; he was also a senior political advisor and a very influential member of Augustus’ most inner circle. Strabo seems to suggest that the friendship with Arius played a significant role in Xenarchus’ career. More directly, it is possible that Xenarchus owed his friendship with Augustus to Arius. On the basis of this biographical information, we can date Xenarchus’ activity to the second half of the first century bce.
Elsewhere Strabo tells us that he (Strabo) studied Aristotelian philosophy with Boethus, the Peripatetic philosopher native to Sidon. This piece of information has been combined with what Strabo says about Xenarchus to suggest that Boethus and Strabo were fellow students in Rome, and Xenarchus was their teacher. But the information in our possession does not justify this conclusion. In all probability, Strabo is saying that he was a student of Boethus, not that they were fellow students. Moreover, there is no evidence linking Boethus to Xenarchus, except what Alexander of Aphrodisias says in his Mantissa [T16]. There, Alexander names Boethus and Xenarchus as champions of the attempt to elaborate an Aristotelian doctrine of the first appropriate thing (prôton oikeion) out of what Aristotle says on love (philia). But this doctrinal agreement does not suffice to establish that Boethus studied with Xenarchus, or that Boethus and Xenarchus were personally close in any other way.
Aristotle's writings had a limited circulation in the Hellenistic period. Strange as it may seem to us today, the most common attitude toward Aristotle at the time was not opposition or resistance to his ideas, but rather indifference. The situation changed in the first century bce. The so-called return to Aristotle is one of the most conspicuous features of the century. This return marked a new beginning in the Peripatetic tradition, which is clearly divided into a Hellenistic and a post-Hellenistic period. The post-Hellenistic period begins with the return to Aristotle in the first century bce and ends with Alexander of Aphrodisias in the late second and early third centuries ce.
The division of the Peripatetic tradition into two phases is not a modern invention but was already recognized in antiquity. The ancient explanation for this curious phenomenon was that the loss of Aristotle's books deprived the Hellenistic Peripatos of its most important theoretical tools. Without these books, the Peripatos could not keep up with the other schools. When they became available in the first century bce, the school of Aristotle could flourish again. It has been pointed out that this explanation is based on the anachronistic assumption that serious philosophizing requires direct attention to a written text. While this is a common assumption in the post-Hellenistic return to Aristotle, it has no parallel in the Hellenistic era. Although anachronistic, it points to a central feature of the post-Hellenistic return to Aristotle: it took the form of a vigorous engagement with Aristotle's writings. At least in the Peripatetic tradition, this was a strikingly new development.
Malcolm Walker tells the story of the UK's national meteorological service from its formation in 1854 with a staff of four to its present position as a scientific and technological institution of national and international importance with a staff of nearly two thousand. The Met Office has long been at the forefront of research into atmospheric science and technology and is second to none in providing weather services to the general public and a wide range of customers around the world. The history of the Met Office is therefore largely a history of the development of international weather prediction research in general. In the modern era it is also at the forefront of the modelling of climate change. This volume will be of great interest to meteorologists, atmospheric scientists and historians of science, as well as amateur meteorologists and anyone interested generally in weather prediction.
This paper throws light on the development of experimental zoology in Britain by focusing on the establishment of the British Journal of Experimental Biology (BJEB) and the Society for Experimental Biology (SEB) in 1923. The key actors in this story were Lancelot T. Hogben, Julian S. Huxley and Francis A.E. Crew, who started exploring the possibility of establishing an experimentally oriented zoological journal in 1922. In order to support the BJEB and further the cause of the experimental approach, Hogben, Crew, Huxley and their colleagues decided to found a society, which led to the formation of the SEB. From its inception the journal was plagued with difficulties that led to the merger of the BJEB and the Biological Proceedings of the Cambridge Philosophical Society in the autumn of 1925. Also discussed are the views that the leading proponents of experimental zoology in Britain in the 1920s expressed towards morphology and how their views further complicate the already much modified ‘revolt from morphology’ thesis.
During its centennial celebrations in 2008, the Museum of Vertebrate Zoology (MVZ) at the University of California, Berkeley paid homage to its founding director, Joseph Grinnell. Recognized as a leading scientific institution, the MVZ managed to grow throughout the twentieth century, a period often characterized by the decline of natural history. To understand how and why research flourished at the MVZ, this paper looks closely at Grinnell's undergraduate course, the Natural History of the Vertebrates (NHV). Taught by MVZ affiliates since 1914, the NHV offers an important window on Grinnell's approach and legacy. This paper argues that the NHV contributed to the MVZ's long-term success by acting as, first, a gateway to natural history; second, a vector for the MVZ's research programme; and third, a shared faculty responsibility. Grinnell's significance in the history of science is understated, in part because his writing style de-emphasized the importance of his theoretical contributions, including his development of the niche concept, his emphasis on population thinking and geographic isolation in studies of evolution, and his effort to integrate speciation questions and genetics. Studying the NHV highlights these contributions because Grinnell freely communicated his ideas to his students. An analysis of Grinnell's course material shows that his theoretical and methodological approach pre-dated the evolutionary synthesis and inspired natural-history research throughout the past century.