1 / 44

Exam Grades

Exam Grades. Due to the rush to get exams back, I did not record credit for those who wrote out their own answers. If you did write out your own answer to a question, please bring me your exam so I can update your score. Announcements.

rmeisel
Download Presentation

Exam Grades

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Exam Grades Due to the rush to get exams back, I did not record credit for those who wrote out their own answers. If you did write out your own answer to a question, please bring me your exam so I can update your score.

  2. Announcements • Note: the exam questions were mostly taken from the quiz and assignments. It is therefore important to understand the questions, not just memorize the correct answer, since they will be asked differently. • Assignments will have TWO parts: (1) an application or practice of what you have learned, (2) questions about the reading for the next lecture. • Planet Assignment 3, due Wednesday Feb 25, • Part 1: Astronomy Place tutorial “Formation of the Solar System” • Part 2: Angel Planet Assignment 3

  3. Confusions & Questions? • Solar Nebula Theory - collapse & heating • What triggers the collapse • How does it collapse • What heats it up • Asteroids - why are they between Mars & Jupiter • Dating rocks, radioactive decay • Doppler Effect

  4. What is a Planet? An object that has a mass between that of Pluto and the nuclear reaction threshold of 13 MJ   and that forms in orbit around a star that generates energy by nuclear reactions.

  5. The Solar System

  6. Solar System Properties • Patterns of Motion • All planets orbit the Sun in the same direction (as Sun spins), in nearly the same plane, & in nearly circular orbit • Two types of planets • Terrestrial: small, rocky, inner • Jovian: large, liquid H, He & ices, outer • Astroids & Comets • Comets dirty ice, Astroids rocks & iron • Ubiquitous impact craters • All old solid surfaces • Exceptions • Uranus rotates sideways, Venus rotates backwards

  7. Patterns of Motion

  8. Two Types of Planets Terrestrial: small rocky, iron inner Jovian: large H, He, ices outer

  9. Asteroid & Comets Dirty ice Rocks & iron

  10. Ubiquitous Craters Mars Moon Callisto

  11. Solar System - How did it Form?What produced the organized motions? • Planets formed as part of the formation of the Sun. • Begin with region of higher density composed of H & He + traces of heavier elements in the space between the stars (called “interstellar cloud”) • Gravity makes the “cloud” collapse • Triggered possibly by explosion of a nearby star

  12. Collapse of Interstellar Cloud Angular Momentum Is conserved. As “cloud” collapses it spins faster.

  13. Why are orbits in nearly same plane? Collapses more along poles than in equator. Forms a disk.

  14. Why are orbits nearly circular?

  15. Solar System - How did it Form?Why are there two types of planets? • Planets formed as part of the formation of the Sun. • As “cloud” collapses gets hotter (falling converts gravitational potential energy to kinetic energy). Inner regions hotter than outer (fell farther). • Rocks & iron solid at high temperatures • Ices solid only at low temperatures

  16. Solidification Temperatures

  17. Condensation Regions

  18. Terrestrial & Jovian Planets • Close to Sun - rocks and iron are solidMake rocky terrestrial planets • Far from Sun - Ices (water, carbon dioxide, methane, ammonia) are solidMake larger proto-planets withGravity large enough to attract H & He gasMake Jovian planets

  19. Terrestrial & Jovian Planets

  20. Gravity captures H & He gas

  21. Humans (& Earth) are made of the flotsam and jetsam of the universe

  22. Solar System - How did it Form?What are Comets & Asteroids? Leftover planetesimals.

  23. Asteroids • Left over rocky & iron planetesimals from formation of planets

  24. Comets • Left over icy planetesimals from formation of the Jovian planets

  25. Solar System - How did it Form? Why ubiquitous impact craters? Remains of accretion of planetesimals.

  26. Accretion of Planetesimals

  27. Review of nebular theory

  28. When did the Solar System Form? Measurements of decaying elements in meteorites indicate age of solar system: 4.6 billion years

  29. Thought Question Suppose you bought a carton of special eggs -- each day half of the eggs in the carton hatch. You open the carton and find 9 chicks and 3 eggs. How long ago was it packed? A. Yesterday B. Two days ago C. Three days ago D. Last week

  30. Example: Half of all potassium-40 nuclei decay into argon-40 every 1.25 billion years

  31. What about Moons?

  32. Moons of Jovian Planets form in miniature disks

  33. Earth’s moon was probably created when a big planetesimal tore a chunk out of the newly forming Earth.

  34. Collisionsimulation

  35. Other Evidence?Other Planetary Systems • Activity • 1. Predict what you expect to be found about the properties of other planetary systems • 2. We will then see what was actually found, and you will compare that with your predictions You will not be graded on the accuracy of your predictions, but on their relevance & completeness.

  36. How are Extrasolar Planets Detected? By the Wobble they produce in their parent star. Detection limit: > 0.3 MJupiter

  37. Doppler Effect Analogy Suppose photons are busses on Grand River Ave. Busses come once every 10 min on average If you are walking East towards Okemos, will the busses heading west from Okemos pass you every 10 min, or less or more? If you are walking West towards Lansing, will the busses heading west from Okemos pass you every 10 min, or less or more?

  38. What has been found? • 120 Planets around Main Sequence (solar like stars) • In 105 planetary systems • 15 multiple planet systems

  39. What has been found - Masses

  40. What has been found - Eccentricity Solar System Eccentricities < 0.1 Except Mercury & Pluto

  41. What has been found - Composition

  42. What we expected What we found Nearly circular orbits Jovian planets far from star Highly eccentric orbits Jovian planets close to star

  43. Implications for Life • Eccentric Jovian planets will eject small terrestrial planets from the system. • Migrating Jovian planets will eject small terrestrial planets as they pass. • Young stars with more heavy elements are more likely to form planets than older stars with less heavy elements.

  44. Questions? • How are circular orbits produced? Are they typical or atypical? • How are hot, close Jovian planets produced? Do they form as outer planets and migrate inward? What makes them migrate?

More Related