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AY 80:Space-age Solar System

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Presentation on theme: "AY 80:Space-age Solar System"— Presentation transcript:

1 AY 80:Space-age Solar System
Instructor: Doug Lin ISB 337, Tel: , Lectures: T/Th 8-9:45am Thimann 1 Office hours: Tue/Thur 2-3:15 pm, ISB 337 general info: TA: Laura Langlang-Shula ISB 111, Tel: , Office hours: Mon/Wed 3-4 pm, ISB 111 Sections: Wed/Fri 2-3pm, ISB 165 Text books: Into the final frontier, by Bernard McNamara Life in the Universe, by J. Bennett, S. Shostak, B. Jakosky Exams (Participation in both exams is necessary to pass): Midterm: Feb 8, 8-9:15am, in class Final: Mar 15, 12-3pm, in class Homeworks: Hand out on Thursdays & return a week later Homework 20%, Midterm 35%, Final 45%

2 Philosophy Main topics
Understanding the process of scientific methodology. To learn some astronomy with regard to the roots of life, planets, & stars. To satisfy the general education and math requirements. Main topics Life in the Universe Our physical environment Nature of life Evolution of the Earth Space flights beyond the Earth Scientitic unmanned missions Life in the solar system Search for other worlds

3 Lecture 1: an overview Life in the Universe
Are we alone?

4 Once habitable environment
Condition which harbors life Liquid water! Ocean below the ice surface on Europa Salt deposit on Marsian rocks: dried up lake.

5 Probability of life 1: worlds beyond imagination
100 billion stars

6 Vast range of distance scales
1 light year = speed of light x 1 yr = 9,460,000,000,000 km

7 Life cycle of stars From gas to stars to gas
Red giants Planetary nebula Young stars Main sequence Interstellar medium supernoave

8 Nucleo synthesis powers the Sun
The pp chain

9 Chemical abundance Triple a reaction CNO cycle Solar abundance

10 Heavy elements in massive stars
supernovae Stellar winds Radioactive isotope production

11 Large structure of the universe cosmic expansion
Big bang & age of the universe: 12 Gyr

12 Chemical abundance in stars heavy element contamination

13 Star and planet formation
Condensation of dust and formation of planets

14 Probability of life 2: Necessary conditions
Chemical elements Sources of energy from stellar luminosity Organic molecules in the interstellar medium Life emerged on earth within 1 Gyr Life survived major disasters Life can be transported elsewhere

15 Quest: to search for the origin and proliferation of life in the Universe


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