The average life expectancy of citizens in 18 different Latin American countries was reported to bee 68.9 years with a standard deviation of 4.6 years. a) What is the critical value for 99% confidence? b) What is the 99% confidence interval of the true mean life expectancey?
The average life expectancy of citizens in 18 different Latin American countries was reported to bee 68.9 years with a standard deviation of 4.6 years. a) What is the critical value for 99% confidence? b) What is the 99% confidence interval of the true mean life expectancey?
MATLAB: An Introduction with Applications
6th Edition
ISBN:9781119256830
Author:Amos Gilat
Publisher:Amos Gilat
Chapter1: Starting With Matlab
Section: Chapter Questions
Problem 1P
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Transcribed Image Text:# Understanding Stars
## Stars: The Building Blocks of the Universe
Stars are massive, luminous spheres of plasma held together by gravity. They undergo nuclear fusion, converting hydrogen into helium and releasing a tremendous amount of energy in the form of light and heat.
### The Life Cycle of a Star:
1. **Nebula**:
- Stars are born in nebulae, which are vast clouds of gas and dust in space.
- Within these nebulae, regions of higher density collapse under their gravity, forming protostars.
2. **Main Sequence**:
- After reaching sufficient temperature and pressure, nuclear fusion begins, and the star enters the main sequence phase.
- In this stable period, stars spend most of their life converting hydrogen into helium.
3. **Red Giant / Supergiant**:
- As hydrogen depletes, the core contracts while the outer layers expand, cool, and redden.
4. **Fusion of Heavier Elements**:
- In massive stars, heavier elements are formed in successive fusion reactions.
- Elements up to iron may be produced in the core.
5. **End of Life Stages**:
- **Planetary Nebula / White Dwarf**: Medium-sized stars shed their outer layers, leaving behind a hot core that cools into a white dwarf.
- **Supernova / Neutron Star / Black Hole**: Massive stars may explode in a supernova, leaving behind either a dense neutron star or, if massive enough, a black hole.
### Stellar Classification
Stars are classified by their spectra and temperature:
- **O Type**: 30,000K or hotter, blue
- **B Type**: 10,000-30,000K, blue-white
- **A Type**: 7,500-10,000K, white
- **F Type**: 6,000-7,500K, yellow-white
- **G Type**: 5,200-6,000K, yellow (like the Sun)
- **K Type**: 3,700-5,200K, orange
- **M Type**: 2,400-3,700K, red
### Diagram Explanation
The diagram shows a star's life cycle:
- **Nebula**: Depicted as a cloud.
- **Protostar**: Shown forming within the nebula.
- **Main
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