The worship and organization of the Christian church must be defined by the Hellenistic world in which it took root and emerged victorious over Roman Imperial paganism. The struggle of the early church to maintain a testimony and doctrine that would be faithful to the Rule of Faith--which was established by the authority of certain Apostles who had the biggest impact in setting up the missional churches of the first century--and would conform to Jesus Christ's earthly ministry. Eusebia (piety) marks the Hellenistic understanding of all worship based on the relationships that are changed as a result of an encounter with a supreme being. This opens the door to explore all the aspects of Church History as a product of corporate worship. Five cities emerge in the apologetic and concilar church ages (150-850 CE) that have the greatest impact on the world of Christianity for all time. Those churches are called the Patristic churches because their bishops became the power holders of all the churches (for good or for bad). This book provides insight into the contribution of the five patriarchal cities (Jerusalem, Antioch, Alexandria, Rome, and Constantinople) to the worship, polity, doctrine, and traditions of the church. The account begins with the exegetical back-drop of the Hebrew and Greek words for worship and the impact of these in the milieu of a Jewish church and a gentile church. The study of the patriarchal leadership in the apostolic, apologetic, and concilar ages of the church marks a clear direction of the church to the beginnings of the medieval era. It clearly delineates the differences in the East and West and the struggles within the Empire to gain unity through preeminence of polity. A unique approach was taken to combine the historical events and activities of the leaders of each of the churches with motive and intent toward good or bad. It was written from a Protestant and Orthodox perspective, which adds insight to set up the spiritual and theological reasons for the Reformation that begun under Wycliffe, Huss, and later Luther.
Arriving in Seattle on the eve of World War II, Japanese-born Mitsuko falls for Tom, a widowed pastor, and becomes surrogate mother to his fair-haired American toddler, Bill. But the bombing of Pearl Harbor strains the newly formed family as U.S. government mandates and Tom’s growing discomfort with all things Japanese force Mitsuko and young Bill to leave Seattle and Tom behind for the Minidoka Internment Camp, unsure if they will ever return. Two decades later, memories of Minidoka and long-lost Mitsuko haunt Bill, sparking an arduous journey that leads him from Seattle’s International District to newly reconstructed Japan to find his Japanese mother and learn the truth about their shared past. Jay Rubin is one of the foremost English-language translators of Japanese literature. He is best known for his numerous translations of works by Haruki Murakami, Japan’s leading contemporary novelist, and the study Haruki Murakami and the Music of Words. Most recently, he has translated the first two books of Murakami’s bestselling novel, 1Q84. In addition, Rubin’s Making Sense of Japanese remains one the widely used guides to Japanese language studies. Jay Rubin received his PhD in Japanese literature from the University of Chicago and taught at Harvard University and the University of Washington. He lives near Seattle with his wife.
ASTRONOMY: FROM THE EARTH TO THE UNIVERSE describes the current state of astronomy, both the fundamentals of astronomical knowledge that have been built up over decades and the exciting advances that are now taking place. The writing style is friendly and carefully detailed. It serves as a valuable reference for both beginners and astronomy enthusiasts. This book is organized as a number of stories. Individual chapters often tell what used to be known, how space and other modern observations have transformed our understanding, and then what is scheduled for the future. This is done with each planet. Consequently, an instructor can easily add photos (available as slides, overheads, CD-ROMs, and on the World Wide Web) and movies and keep a student's interest for a whole lecture on each planet, if desired. Students learn about astronomy through concrete examples, rather than merely being given overarching concepts without enough underpinning.
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