Archaeology: Cultural Affiliation "Unknown cultural affiliations and loss of identity at high elevations ” These are words used to propose the hypothesis that archaeological sites tend to lose their identity as altitude extremes are reached. This idea is based on the notion that prehistoric people tended not to take trade wares to temporary settings and/or isolated areas (Source: Prehistoric Ne w Mexico: Background for Surrey, by D. E. Stuart andR. P Gauthier. University of New Mexico Press). As elevation zones of prehistoric people (in what is now the state of New Mexico) increased, there seemed to be a loss of artifact identification. Consider the following information:
Elevation Zone | Number of Artifacts | Number Unidentified |
7000-7500 ft | 112 | 69 |
5000-5500 ft | 140 | 26 |
Let
(a) Find a 99% confidence interval for
(b) Interpretation Explain the meaning of the confidence interval in part (at in the context of this problem Does the confidence interval contain all positive numbers? all negative numbers? both positive and negative numbers? What does this tell you (at the 99% confidence level) about the population proportion of unidentified artifacts at high elevations (7000- 7500 ft) compared with the population proportion of unidentified artifacts at lower elevations (5000-5500 ft) ? How does this relate to the stated hypothesis?
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Chapter 10 Solutions
Understanding Basic Statistics
- Running Speed A man is running around a circular track that is 200 m in circumference. An observer uses a stopwatch to record the runner’s time at the each of each lap, obtaining the data in the following table. (a) What was the man’s average speed (rate) between 68 s and 152 s? (b) What was the man’s average speed between 263 s and 412 s? (c) Calculate the man’s speed for cadi lap, Is he slowing down, speeding up, or neither?arrow_forwardMass-Luminosity Relation Roughly 90 of all stars are main-sequence stars. Exceptions include supergiants, giants, and dwarfs. For main-sequence stars including the sun, there is an important relationship called the mass-luminosity relation between the relative luminosity L and the mass M in terms of solar masses. Relative masses and luminosities of several main-sequence stars are reported in the accompanying table. Star Solar mass M Luminosity L Spica 7.3 1050 Vega 3.1 55 Altair 1 1.1 The Sun 1 1 61 Cygni A 0.17 0.002 a Find a power model for the data in this table. Round the power and the coefficient to one decimal place. The function you find is known to astronomers as the mass-luminosity relation. b Kruger 60 is a main sequence star that is about 0.11 solar mass. Use functional notation to express the relative luminosity of Kruger 60, and then calculate that value. c Wolf 359 has a relative luminosity of about 0.0001. How massive is Wolf 359? d If one star is 3 times as massive as another, how do their luminosities compare?arrow_forward
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