In Iceland’s Relationship with Norway c.870 – c.1100: Memory, History and Identity, Ann-Marie Long reassesses the development of Icelandic society from the earliest settlements to the twelfth century. Through a series of thematic studies, the book discusses the place of Norway in Icelandic cultural memory and how Icelandic authors envisioned and reconstructed their past. It examines in particular how these authors instrumentalized Norway to explain the changing parameters of Icelandic autonomy. Over time this strategy evolved to meet the needs of thirteenth-century Icelandic politics as well as the demands posed by the transition from autonomous island to Norwegian dependency.

Literary Nonfiction. California Interest. Women's Studies. Film. Memoir. THE BIG LOVE is a Hollywood nightmare. It tells the story of Errol Flynn--a fading, alcoholic movie star--and the underage dancer-actress Beverly Aadland. The narrator? Beverly Aadland's fame-worshiping mother Mrs. Florence Aadland, who spurs the relationship on. There is nothing subtle or sympathetic about this memoir: It is outrageous, grotesque, surreal, notorious--an intimate look at Hollywood exploitation and decay. On the one hand, THE BIG LOVE depicts the deterioration of Errol Flynn, an actor who is quickly losing relevance after years of playing irresistible swashbucklers in films such as Captain Blood (1935) and The Adventures of Robin Hood (1938). He is riddled with medical problems, drinking himself to death. On the other hand, there is Mrs. Florence Aadland, also an alcoholic, an uncultured stage mother psychotically pushing her daughter Beverly forward even at the cost of her own marriage. A bizarre, seedy time capsule of the 1950s, THE BIG LOVE is the long-lost literary sister of Barbara Payton's I AM NOT ASHAMED. And, after languishing out of print for years, it is ready to shock brand new audiences with its absurd humor, villainous characters, and sickly dissipation.

As to the first, the last discoveries of Saturn to be tricorporeall, and of the mutations of Figure in Venus, like to those that are seen in the Moon, together with the Consequents depending thereupon, have not so much occasioned the demur, as the investigation of the times of the Conversions of each of the Four Medicean Planets about Jupiter, which I lighted upon in April the year past, 1611, at my being in Rome; where, in the end, I assertained my selfe, that the first and neerest to Jupiter, moved about 8 gr. & 29 m. of its Sphere in an houre, makeing its whole revolution in one naturall day, and 18 hours, and almost an halfe. The second moves in its Orbe 14 gr. 13 min. or very neer, in an hour, and its compleat conversion is consummate in 3 dayes, 13 hours, and one third, or thereabouts. The third passeth in an hour, 2 gr. 6 min. little more or less of its Circle, and measures it all in 7 dayes, 4 hours, or very neer. The fourth, and more remote than the rest, goes in one houre, 0 gr 54 min. and almost an halfe of its Sphere, and finisheth it all in 16 dayes, and very neer 18 hours. But because the excessive velocity of their returns or restitutions, requires a most scrupulous precisenesse to calculate their places, in times past and future, especially if the time be for many Moneths or Years; I am therefore forced, with other Observations, and more exact than the former, and in times more remote from one another, to correct the Tables of such Motions, and limit them even to the shortest moment: for such exactnesse my first Observations suffice not; not only in regard of the short intervals of Time, but because I had not as then found out a way to measure the distances between the said Planets by any Instrument: I Observed such Intervals with simple relation to the Diameter of the Body of Jupiter; taken, as we have said, by the eye, the which, though they admit not errors of above a Minute, yet they suffice not for the determination of the exact greatness of the Spheres of those Stars. But now that I have hit upon a way of taking such measures without failing, scarce in a very few Seconds, I will continue the observation to the very occultation of JUPITER, which shall serve to bring us to the perfect knowledge of the Motions, and Magnitudes of the Orbes of the said Planets, together also with some other consequences thence arising. I adde to these things the observation of some obscure Spots, which are discovered in the Solar Body, which changing, position in that, propounds to our consideration a great argument either that the Sun revolves in it selfe, or that perhaps other Starrs, in like manner as Venus and Mercury, revolve about it, invisible in other times, by reason of their small digressions, lesse than that of Mercury, and only visible when they interpose between the Sun and our eye, or else hint the truth of both this and that; the certainty of which things ought not to be contemned, nor omitted.

Drawing from recent archaeological and linguistic evidence, as well as more traditional literary and narrative sources, the author distinguishes between the initial phase of migrations in the ninth and tenth centuries, and the secondary period of settlement up to c. 1100 AD. He emphasizes, too, the differences in nature and intensity of the Viking impact on the societies that were slowly developing into the historic kingdoms of England and Scotland, and the more complex political structures of Wales and Ireland. Throughout the book, the effects of the Scandinavian invasions on Britain are set within the wider European context.