Machine generated contents note: Part I: Sources for Mesopotamian Cosmic Geography -- 1. The Levels of the Universe: KAR 307 30-38 and AO 8196 iv 20-223 -- 2. "The Babylonian Map of the World"20 -- 3. The Flights of Etana and the Eagle into the Heavens43 -- 4. The Sargon Geography67 -- 5. Gilgamesh and the Distant Reaches of the Earth's Surface 96 -- 6. Cosmic Geography in Accounts of Creation 107 -- 7. The Geography of the Sky: The "Astrolabes', (...) Mul-Apin, and Related Texts150 -- 8. BagM. Beih. 2 no. 98 and the Compass Points193 -- 9. "Seven Heavens and Seven Earths"208 -- Part II: The Regions of the Universe -- Names for Heaven223 -- 11. The Geography of the Heavens243 -- 12. Names for Earth268 -- 13. The Geography of Earth318 -- Appendixes363 -- Indexes369 -- Subject Index369 -- Ancient Texts and Modern Editions382 -- Sumerian and Akkadian Terms391 -- Stars3 9 7 -- Plates399. (shrink)

Abstract.The present paper is an attempt to describe the observational practices behind a large and homogeneous body of Babylonian observation reports involving planets and certain bright stars near the ecliptic (“Normal Stars”). The reports in question are the only precise positional observations of planets in the Babylonian texts, and while we do not know their original purpose, they may have had a part in the development of predictive models for planetary phenomena in the second half of the first millennium B.C. (...) The paper is organized according to the following topics: (I) Sections 1–3 review the format of the observations and the texts in which they are found; (II) Sections 4–6 discuss the composition of the Normal Star list; (III) Sections 7–8 concern the orientation of the reported celestial directions from star to planet; (IV) Sect. 9 concerns the relationship between the reported distances and the actual angular distances between planet and star; and (V) Sect. 10 discusses the reports of planetary stations, which are the most common reports giving precise locations of planets when they are not near their closest approach to stars, and draws some brief general conclusions about the utility of the Babylonian observations for estimating planetary longitudes and calibrating models in antiquity. (shrink)