Feb. 18 – 24 (Conditions for Life, EM Spectrum, Nuclear Fusion)

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
  • Write today’s EQ

 

Conditions Necessary for Life

    • 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.

 

  • Discussion Teams 2 Selection

 

        • 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.

 

  • Discussion Team 3 Selection

 

      • Discuss: What processes necessary for life does energy create?

 

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

Energy Movement in a Star

 

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

Electromagnetic Spectrum

Slides #31 – 42

Lab:  Stars and Spectroscopy

  • 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)
  • 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.

 

No Comments »

Comments are closed.