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Published bySabrina Small Modified over 8 years ago
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What we will do What we will learn Do Now: Find the strength of the Sun’s grav field for the Earth’s location Sun’s Mass (2E30kg), radius of orbit is 150 million km. How does this compare to g on Earth? How to apply our skills to the higher level thinking. HRT and early HW marking so we can go to interval on time tomorrow How to make great use of time. If behaviour is poor, we will start the next unit on radian measure How to make great use of time 13Px 02 Poutū-Te-Rangi 2016
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HW item Skills practiced Mex: Pages 45 - 47 Due Wed 24 Feb, end of pd 2 Impulse and the change of momentum Mex: Pages 48 & 49 Due Fri 26 Feb, end of pd 4 Circular motion (NCEA2 revised) Mex: Pages 50 - 53 Due Thurs 3 March, end of pd 4 Circular motion extended Conical pendula Mex: Page 54 Due Thurs 3 March, end of pd 4 Gravitation Mex: Page 55 and 56 Due Thurs 3 March, end of pd 4 Satellites Mex: Page 57 - 59 Due Thurs 3 March, end of pd 4 Concepts and calculations for gravitational force fields
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No. of marks What for 1Having sketches & FULL working for all 1Neat presentation and down-page format 1Answer underlined and units given 1Self marked and all correct – eventually 1In on time and signed for (“This is my own work”…….) Total A mark out of five that will contribute to the “homework” grade in the reports
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