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The Scorpion's Tail - Douglas Preston & Lincoln Child - Discount Books

The Scorpion's Tail

From #1 bestselling authors Preston & Child comes a thrilling novel following archaeologist Nora Kelly and FBI Agent Corrie Swanson as they work together to solve a twisted crime that reaches far beyond any of their worst fears.
Following the acclaimed debut of Old Bones, this second "happily anticipated" new thriller in Preston & Child's series features Nora Kelly, archaeologist at the Santa Fe Archeological Institute, and rookie FBI Agent Corrie Swanson, as they team up to solve a mystery that quickly escalates into nightmare (Booklist).

A mummified corpse, over half a century old, is found in the cellar of an abandoned building in a remote New Mexico ghost town. Corrie is assigned what seems to her a throwaway case: to ID the body and determine cause of death. She brings archaeologist Nora Kelly to excavate the body and lend her expertise to the investigation, and together they uncover something unexpected and shocking: the deceased apparently died in agony, in a fetal position, skin coming off in sheets, with a rictus of horror frozen on his face.

Hidden on the corpse lies a 16th century Spanish gold cross of immense value.

When they at last identify the body -- and the bizarre cause of death -- Corrie and Nora open a door into a terrifying, secret world of ancient treasure and modern obsession: a world centered on arguably the most defining, frightening, and transformative moment in American history.


The Scorpion's Tail - Douglas Preston & Lincoln Child Summary

Messier 7 or M7, also designated NGC 6475 and sometimes known as the Ptolemy Cluster, is an open cluster of stars in the constellation of Scorpius. The cluster is easily detectable with the naked eye, close to the "stinger" of Scorpius. With a declination of −34.8°, it is the southernmost Messier object. M7 has been known since antiquity; it was first recorded by the 2nd-century Greek-Roman astronomer Ptolemy, who described it as a nebula in 130 AD. Italian astronomer Giovanni Batista Hodierna observed it before 1654 and counted 30 stars in it. In 1764, French astronomer Charles Messier catalogued the cluster as the seventh member in his list of comet-like objects. English astronomer John Herschel described it as "coarsely scattered clusters of stars".Telescopic observations of the cluster reveal about 80 stars within a field of view of 1.3° across. At the cluster's estimated distance of 980 light years this corresponds to an actual diameter of 25 light years. The tidal radius of the cluster is 40.1 ly (12.3 pc) and it has a combined mass of about 735 times the mass of the Sun. The age of the cluster is around 200 million years while the brightest member star is of magnitude 5.6. In terms of composition, the cluster contains a similar abundance of elements other than hydrogen and helium as the Sun.On August 29, 2006, Messier 7 was used for first light image of the Long Range Reconnaissance Imager (LORRI) telescope on the Pluto-bound New Horizons spacecraft...


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