Feb. 18 – 24 (Conditions for Life, EM Spectrum, Nuclear Fusion)
Feb 19th 2020
Tuesday, Feb. 18
Unit Essential Question: Are there planets outside our solar system that could support life? How can we locate them and determine their habitability?
Daily Essential Question: What are the conditions necessary for life?
Routine – Answer Yesterday’s EQ in the “Summary” section of the notes
- Review “Conditions for Life” (Liquid Medium, Raw Materials, Energy) (8 min)
- Liquid Medium
- Water
- Raw Materials
- Oxygen, Carbon, Hydrogen, Nitrogen
- Energy
- The Sun, a star, produces the vast majority
- Liquid Medium
- Write today’s EQ
Conditions Necessary for Life
- Focus Note Format in SNB
- “Conditions that Support Life: https://learn.genetics.utah.edu/content/astrobiology/conditions/ (20 min)
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- Student’s take notes in SNB
- Slide 8 – Oxygen, Carbon, Nitrogen and Hydrogen make up 97% of body
- Slide 9 – Elements come from stars; present throughout the universe; life needs a continuous supply
- Slide 10 – Life on Earth based on Carbon, can build many stable molecules; trapped in rock is not useful, but it cycles out of rock and into living things.
- Slide 11 – Look for life elsewhere, look for chemical reactions carried out by living things.
- Student’s take notes in SNB
- Discussion Teams 2 Selection
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- Discuss: Why is carbon the key element in life?
- Slide 12 – Energy from the Sun is important for chemical reactions; used by planets to build larger molecules; animals use energy from break down molecules to fuel the building of new ones they need.
- Slide 13 – Look for system of free flowing energy; energy from Sun and Earth’s core provide energy to system on Earth
- Slide 14 – Energy from Sun heats planet and gravity create wind and ocean currents and tides, which circulate material. ADD – circulation of materials is very important
- Slide 15 – Energy from core results in movement of plates
- Slide 16 – Subduction zone plate material melts in asthenosphere, chem. react. ADD – these are examples of large scale circulation of raw materials, if this does not happen, life won’t exist or ceases to exist (Mars is an example)
- Slide 17 – Speculation of other energy sources
- Slide 18 – To search for life elsewhere, look for similar conditions on other planets
- Slide 19 – Life on other planets may look different than we know it.
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- Discussion Team 3 Selection
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- Discuss: What processes necessary for life does energy create?
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HW: Reading in Discovery Ed. on Conditions for Life and Habitable Zone (Concept 2.2), Explore section 4, scroll down to “Earth: A Unique Planet in the Solar System”; Answer the Concept 2.2 Companion Questions (Published link for website Concept 2.2 Companion Questions). Due Wednesday (Video: Alien Planets Revealed, good to watch to answer #8-11)
Wednesday, Feb. 19
Unit Essential Question: Are there planets outside our solar system that could support life? How can we locate them and determine their habitability?
Daily Essential Question: What kind of spectrum does the Sun produce?
HW Due and Review
Intro to Electromagnetic Spectrum and Wavelength
- Slides #1-9, Quick overview of slides #35 -42
- Observations of the Sun’s absorption spectrum
HW: Quiz on Wednesday (Conditions for Life). Use Astronomy Study Guide Questions 1 – 2 on Google Classroom.
Read and watch the listed videos on Disc. Ed., Concept 1.2. Answer the Concept 1.2 Companion Questions Due on Friday.
Thursday, Feb. 20
Unit Essential Question: Are there planets outside our solar system that could support life? How can we locate them and determine their habitability?
Daily Essential Question: What happens during nuclear fusion?
Quiz 1 – Conditions for Life
Intro to Nuclear Fusion and Electromagnetic Spectrum
- Slides #10-30
- Discussion Teams
HW: Read and watch selected videos on Discovery Ed. Concept 3.1, Stars. Answer the Companion Questions 3.1 – Due Friday
Friday, Feb. 21
Unit Essential Question: Are there planets outside our solar system that could support life? How can we locate them and determine their habitability?
Daily Essential Question: What
HW Due and Review – Nuclear Fusion
Slides #31 – 42
- Label lab title: Stars and Spectroscopy
- Add to table of contents
- Instructions in Google Classroom (27A Stars and Spectroscopy)
- Identify the Task and the Driving Question
- How can we determine the amount of energy produced by a star?
- Add to Science Notebook top of right page (page 13)
- How can we determine the amount of energy produced by a star?
- Tool Talk
- Get spectrometers and CPO Investigations books (page 178)
- Read “Using a Spectrometer”.
HW: Quiz on Nuclear Fusion and Energy Movement (Day 48). Use Astronomy Study Guide Questions 3 – 9 on Google Classroom.
HW: Read and watch the listed videos on Disc. Ed., Concept 1.2. Answer the Concept 1.2 Companion Questions. (Published version Concept 1.2 Companion Questions) Due on Wednesday.
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