Lunar Eclipse

Last night’s eclipse was spectacular. The reddening moon hung below Regulus (the brightest star in Leo) and next to Saturn.
It was the twenty-sixth eclipse of Saros Cycle 133, which began with the lunar eclipse of May 13th, 1557, and will end with the eclipse of June 29th, 2918. Each Saros Cycle comprises eclipses with very similar geometries and approximate periodicity of 18 years, 11 days and 8 hours. There are currently forty-one different active lunar Saros Cycles.
Babylonian astronomy had become quite sophisticated by the time of the reign of Nabonassar (747-733 BCE), and the Saros Cycle was well understood by Babylonian astronomer-priests by the sixth century BCE. Lacking knowledge of the true geometry of the solar system (or so we presume), the Babylonians kept records of the observable circumstances of lunar and solar eclipses beginning perhaps as far back as the eighteenth century BCE and eventually gleaned their hidden patterns of recurrence. Ancient Babylon is present day Iraq.
This picture is a composite of three bracketed shots, layered together in Photoshop. I took it with a Nikon D80. It was attached by a t-connector to a TeleVue Pronto telescope - effectively a 480mm (equivalent to 720mm on a 35mm camera), f6.8 telephoto lens.
