Tuesday, April 3, 2012

11 - plenary

 

11 - plenary

19 March 2012

11:10

·         Watch the video

·         Can you explain why the brightness of the LED can be varied? 

Your explanation should consider:

o the length of the graphite

o the resistance of the graphite

o the current in the circuit

Answer

·         A short length of graphite gives a low resistance

·         A low resistance allows a large current to flow

·         A large current makes the LED bright

OR

·         A long length of graphite gives a high resistance

·         A high resistance allows a small current to flow

·         A small current makes the LED dim

1.32 and 1.34

 

 

1.32 and 1.34 Starter

16 March 2012

10:18

Tell the person next to you…

·         the names of the 8 planets in our solar system (in order!)

Answers

1.              Mercury (closest to the sun)

2.              Venus

3.              Earth

4.              Mars

5.              Jupiter

6.              Saturn

7.              Uranus

8.              Neptune (furthest from the sun)

 

How can you remember this?

·         "My Very Educated Mother Just Served Us Nothing"

·         "My Very Easy Method Just Speeds Up Naming (Planets)"

 

Image001

 

 

1.32 and 1.34 Starter 2 - Quick Planets quiz

12 May 2011

15:52

<<planets quiz.swf>>

 

 

1.32 and 1.34 Investigating the solar system - answers

16 March 2012

10:26

Moons

1.           How are moons different from planets?

Planets orbit the Sun; moons orbit planets

2.           The Earth has one moon.  Do all planets?

No.  Mercury and Venus have no moon, Mars has 2 and Venus and Saturn both have over 60 each!

3.           Do moons have gravitational fields?

Yes, any body that has mass generates a gravitational field.  The gravitational field strength on our Moon is

1.62N/kg, which is about 1/6 of the gravitational field strength on Earth.

 

Gravitational fields

4.           Which planet has the largest gravitational field?  What is it?

Jupiter = 26N/kg

5.           Which planet has the smallest gravitational field? What is it?

Mercury = 4N/kg (Pluto doesn't count!  See Q.11)

6.           What is the relationship between the mass of the planet and the gravitational field strength of the planet?

The larger the mass of a planet, the stronger the gravitational field strength

 

Period of orbit

7.           Which planet has the shortest period of orbit?  What is it?

Mercury = 3 x Earth month = 0.25 x Earth year

(if you lived on Mercury you would be over 60 years old!)

8.           Which planet has the longest period of orbit?  What is it?

Neptune = 1978 x Earth month = 164 x Earth year

(if you lived on Neptune you would be 0.1 years old!)

9.           What is the relationship between the period of orbit of a planet and its distance from the Sun?

The larger the distance from the Sun, the greater the period of orbit

10.     What is the relationship between the surface temperature of a planet and its distance from the Sun?

The larger the distance from the Sun, the lower the surface temperature

(the one exception to this rule is Venus which has an exceptionally high surface temperature of +465oC due to an atmosphere of 96% CO2 and clouds of H2SO4!)

 

Classification of astronomical bodies

11.     What 2 classifications are the planets grouped into?  What are the key features of each group?

4 Inner "rocky" planets

o    Rocky

o    Smaller diameters

o    Shorter periods

4 Outer "gas giant" planets

o    Gaseous

o    Larger diameters

o    Longer periods

o    Have rings (most noticeable for Saturn, but they all have them)

o  What are 2 key features of comets and 3 key features of their orbits?

                                             i.        Made from ice and dust

                                          ii.        Have a tail when they pass close to the Sun

                                             i.        Highly elliptical orbit - see blue trace. 

Image002

o    Sometimes pass close to the Sun at very high speeds but spend most of their orbit in the outer reaches of the solar system moving at much lower speeds

                                        iii.        Periods can be from a few years to hundreds of thousands of years

           13.     How do the orbits of asteroids differ from the orbits of comets?

Asteroids are lumps of rock that mostly orbit the Sun in the "Asteroid Belt", between Mars and Jupiter, in approximately circular orbits

           14.     Which planet in the animation is no longer a planet? (it has been reclassified as a planetoid or dwarf planet)

Pluto was reclassified as a planetoid or dwarf in 2006 for reasons including its highly elliptical and tilted orbit

 

 

PhET animation - my solar system

31 January 2012

13:34

<<my-solar-system_en.jar>>

Website

http://phet.colorado.edu/en/simulation/my-solar-system

 

Embed code for your blog

<iframe src="http://phet.colorado.edu/sims/my-solar-system/my-solar-system_en.html" width="800" height="600"></iframe>

 

planets quiz.swf Download this file

1.33

 

 

1.33

15 March 2012

10:25

·         1.33 explain that gravitational force

·         causes moons to orbit planets

·         causes the planets to orbit the sun

·         causes artificial satellites to orbit the Earth

·         causes comets to orbit the sun

<<gravity-and-orbits_en.jar>>

http://phet.colorado.edu/en/simulation/gravity-and-orbits

 

1.              Turn on

Image001

2.              Experiment with the 4 different situations to see what orbits what and why

Image002

3.              Still not sure?  Try

Image003

 

 

PhET animation - gravity and orbits

31 January 2012

13:34

<<gravity-and-orbits_en.jar>>

Website

http://phet.colorado.edu/en/simulation/gravity-and-orbits

 

Embed code for your blog

<div style="position: relative; width: 300px; height: 226px;"><a href="http://phet.colorado.edu/sims/gravity-and-orbits/gravity-and-orbits_en.jnlp" style="text-decoration: none;"><img src="

Media_httpphetcolorad_xhjgv
" alt="Gravity and Orbits" style="border: none;" width="300" height="226"/><div style="position: absolute; width: 200px; height: 80px; left: 50px; top: 73px; background-color: #FFF; opacity: 0.6; filter: alpha(opacity = 60);"></div><table style="position: absolute; width: 200px; height: 80px; left: 50px; top: 73px;"><tr><td style="text-align: center; color: #000; font-size: 24px; font-family: Arial,sans-serif;">Click to Run</td></tr></table></a></div>

1.36

1.36

15 March 2012

10:27

·         1.36 understand that:

·         the universe is a large collection of billions of galaxies

·         a galaxy is a large collection of billions of stars

·         our solar system is in the Milky Way galaxy

Image001

Comparative sizes of planets and stars

Image002

 

Comparative sizes of galaxies

Image003

 

Powers of 10 - Cosmic Voyage

Image004

 

 

1.36 Space is big! Scale model of the solar system

12 May 2011

14:47

·         Type the length of your classroom into cell B5 to get the solar system scaled to fit!

·         Check out column U for information about the nearest star to our solar system!

<<scale model.xls>>

 

 

1.36 Plenary Answers

15 March 2012

10:30

1.  What is the solar system?

Everything that orbits our local star, the Sun

2.  What is the Milky Way?

The galaxy that contains our solar system

3.  What is a galaxy?

A huge collection of billions of stars

4.  How many galaxies are there in the Universe?

Billions

scale model.xls Download this file

1.35

 

 

1.35

15 March 2012

10:26

·         1.35 use the relationship between orbital speed, orbital radius and time period:

             orbital speed = 2×Π×orbital radius   

                                         time period                                               

                             v = 2×Π×r

                                        T

 

v = 2×Π×r

           T    

 

v = orbital speed (m/s or km/hr)

r = orbital radius (m or km)

T = orbital period (s or hr)

 

 

 

1.35 Plenary Answers

15 March 2012

10:30

Pearson Answers, p.56, Q3+4

 

Saturday, March 17, 2012

1.22 Plenary questions

Physics for You p.147

 

Image001

a)      Momentum = mv

Momentum = (2+6) x 8

Momentum = 64 kgm/s

b)      See exercise book

c)      KE is not conserved it is converted and wasted as other forms of energy.

 

Image002

1.22

 

1.22

Tuesday, July 06, 2010

3:04 PM

·        1.22 use the conservation of momentum to calculate the mass, velocity or momentum of objects

Momentum conserved in collisions

 

 

<<AirTrack simulation.swf>>

 

and 1.20 animation

 

Momentum conserved in explosions

 

 

<<newtons_cradle[1].swf>>

 

<<N3L - Every action has a Gun fire.mpeg>>

 

Example - Pearson, p.41

Image001

 

Consider final momentum

 

Truck, plasticine and pellet

p = m x v

p = (0.1+0.002) x 0.8

p = 0.0816kgm/s

 

total final momentum = pf = 0.0816kgm/s   

 

Principle of Conservation of Momentum tells us:

total initial momentum = total final momentum

                               Σpi = Σpf

 

so total initial momentum = pi = 0.0816kgm/s

 

 

Consider initial momentum

 

Truck and plasticine   

p = m x v

p = 0.1 x 0

p = 0kgm/s 

 

Pellet   

p = m x v

0.0816 = 0.002 x v

v = 40.8m/s

 

 

1.22 animation

14 March 2012

15:49

newtons_cradle[1].swf Download this file

AirTrack simulation.swf Download this file

Investigating Momentum

Starter - Spot the mistakes!

13 March 2012

16:35

·        http://sites.google.com/site/winfailphysics/all-videos/roadrunner-human-cannonball

·        http://sites.google.com/site/winfailphysics/all-videos/roadrunner-spring-punch

·        You know that these situations are wrong, but why are they wrong?!

 

 

 

Guided discovery - Investigating Momentum

14 March 2012

07:20

When we collide two gliders on the

air track, what happens?

 

Situation 1: Elastic collision with a stationary glider

Initial

Initial speed of LH glider = ul = 1m/s

Initial speed of RH glider = ur = 0m/s

Image001

 

Final

Final speed of LH glider = vl = 0m/s

Final speed of RH glider = vr = 1m/s

Image002

 

We can represent this graphically as

 

Initial

Image003

Final

Image004

 

Conclusion

·        It appears that the speed is "transferred" to the RH glider

 

 

Situation 2: Inelastic collision with a stationary glider

Initial

Initial speed of LH glider = ul = 1m/s

Initial speed of RH glider = ur = 0m/s

Image005

 

Final

Final speed of LH glider = vl = 0.5m/s

Final speed of RH glider = vr = 0.5m/s

Image006

 

We can represent this graphically as

 

Initial

Image003

Final

Image007

 

Conclusion

·        Speed is conserved in the collision

·        Total Initial speed = Total Final speed

 

 

Situation 3: Head on collision

Initial

Initial speed of LH glider = ul = 1m/s

Initial speed of RH glider = ur = -1m/s

Image008

 

Final

Final speed of LH glider = vl = 0m/s

Final speed of RH glider = vr = 0m/s

Image009

 

We can represent this graphically as

 

Initial

Image010

Final

Image011

 

Conclusion

·        Velocity is conserved in the collision

·        Total Initial velocity = Total Final velocity

 

 

Situation 4: Head on collision with different masses

Initial

Initial speed of LH glider = ul = 1m/s

Initial speed of RH glider = ur = -1m/s

Image012

 

Final

Final speed of LH glider = vl = 0m/s

Final speed of RH glider = vr = 0m/s

Image013

 

Problem!

Our previous conclusion that

o   Velocity is conserved in the collision

doesn't hold for this situation!

 

Why do they move off to the left?

Because the RH glider has twice the mass

 

What could I change about the LH glider to make both gliders stop after the collision?

o   Double the mass (obvious)

o   Double the initial velocity

 

We can represent this graphically as

 

Initial

Image014

Final

Image015

 

So something is conserved in the collision, but what is it?

 

What does the area of the rectangles represent?!

 

Time to label our axes!

Image016

Final Conclusion

·        The area of the rectangles are mass x velocity

·        Momentum = mass x velocity

·        So momentum is conserved in collisions