Monday, March 26, 2012

1.36

·         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

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Comparative sizes of galaxies

Image003

 

Powers of 10 - Cosmic Voyage

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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

MABA's complete IGCSE Physics formulae list

IGCSE Physics Formulae.doc Download this file

1.35

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

 

1.32 and 1.34

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>>

1.33

·         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;">Gravity and Orbits

Click to Run
</div>

Sunday, March 18, 2012

1.24

Can you explain this in terms of the Principle of Conservation of Momentum?

 

 

1.24

Tuesday, July 06, 2010

3:04 PM

·         1.24 demonstrate an understanding of Newton’s third law

Image001

<<N3 pairs.swf>>

<<Newton's 1,2,3 summary.swf>>

Newton's 1,2,3 summary.swf Download this file

N3 pairs.swf Download this file

N3 guy jumps off boat.swf Download this file

1.21

1.21 use the ideas of momentum to explain safety features

Image001

Example

Explain how motorcycle and bicycle helmets can protect their users during a collision

 

Answer

·         Helmet or bare head, the change in momentum of your head during a collision is equal

·         With a helmet, this change in momentum takes place over a longer time

·         This means that the force needed to change the momentum of your head is less

or use the equation

·         Impulse = Δp = F x t where Δp = constant

·         cushioning in helmet => increases t

·         and therefore decreases F

 

 

1.21 Plenary answers

13 March 2012

15:20

Physics for You p.147 Q2c

2c. Why is the front of a car designed to collapse in a serious collision? (3 marks)

 

·         There is a force when you crash that decelerates the car (decreases your momentum)

·         If the front of the car collapses (this is the crumple zone), this force acts for a longer time than if the front of the car were rigid

·         This means that the force needed to change the car's momentum is less and there's less risk of injury to the driver

or use the equation

·         Impulse = Δp = F x t where Δp = constant

·         crumple zone increases t

·         and therefore decreases F

1.23 Plenary answers

Image001

1.20 to 1.24 Plenary answers

Physics for You p.147 Q6

Image001

6.

Consider initial momentum

 

Man   

p = m x v

p = 80 x 0

p = 0kgm/s

 

Bullet  

p = m x v

p = 0.02 x 400

p = 8kgm/s     

 

total initial momentum = 8+0 = 8kgm/s   

 

Principle of Conservation of Momentum tells us:

total initial momentum = total final momentum

                               Σpi = Σpf

 

so total final momentum = 8kgm/s

 

Consider final momentum

 

Σpf = pbullet + pman

8 = 0 + pman

pman = 8kgm/s

 

Man

p = m x v

8 = 80 x v

v = 0.1m/s

 

·         Considerably less dramatic than Hollywood!

Momentum and Impulse Plenary (Gapfill) - PFY.ppt Download this file

Sunday, February 26, 2012

7.13

·         7.13 describe the uses of radioactivity in medical and non-medical tracers, in radiotherapy and in the radioactive dating of archaeological specimens and rocks

<<Uses of radioactivity.pptm>>

Medical Tracers

Radioactive Dating

<<DJFPh106carb2.swf>>

<<DJFPh108dating5.swf>>

Uses of radioactivity.pptm Download this file

DJFPh108dating5.swf Download this file

DJFPh106carb2.swf Download this file

7.10 to 7.12 answers

1.              What happens to the amount of ‘mother’ nuclei as time passes?

Decrease

2.              What sort of radioisotope will decay the fastest - one with a long half life or one with a short half life?

One with a short half life

3.              Does half life tell us exactly when a particular nucleus in a radioisotope will decay?

No.  It is a random process - we can not know exactly when a particular nucleus will decay

4.              What are the two definitions of half life?

a.                  The time taken for the activity of a sample to halve

b.                  The time taken for the number of radioactive atoms in a sample to halve

5.              What does the activity of a source mean?

The number of decays per second

6.              What is the unit of activity?

Becquerel (Bq)

7.              What will happen to the number of ‘mother’ nuclei after two half lives?

1    è    ½     è    ¼  

     1xhalf life       2xhalf life 

The number of mother nuclei will be ¼ of the original number

8.              What will happen to the activity of a source after two half lives?

1    è    ½     è    ¼  

     1xhalf life       2xhalf life 

The activity will be ¼ of the original activity

 

 

7.10 to 7.12 calculation answers

12 January 2012

10:24

1.              A radioisotope has a half life of 12 years. What fraction of the radioisotope will be left after 60 years?

Fraction remaining:

1    è    ½     è    ¼    è   1/8    è   1/16    è   1/32

1xhalf life       2xhalf life          3xhalf life        4xhalf life          5xhalf life

      12 years        24 years            36 years          48 years            60 years

 

2.              If the activity of a sample falls to 1/64th of its original level after 2 hours, what is the half life of the sample?

 

è  ½  è  ¼  è  1/8  è  1/16  è  1/32  è  1/64

      1xhalf life    2xhalf life     3xhalf life      4xhalf life         5xhalf life         6xhalf life

Decay takes 2 hours (= 120 minutes)

This is 6 half lives

So 1 half life = 120 minutes / 6 half lives = 20 minutes

 

3.              The background radiation in a laboratory is 7 Bq. The count rate from a radioisotope is measured and it has a reading of 119 Bq. If the half life of the radioisotope is 10 minutes, what will be the reading 20 minutes later?

 

Initial count rate at detector = 119 Bq

But Background rate = 7 Bq

So activity of radioisotope = 119 – 7 = 112 Bq

 

è  ½  è  ¼

      1xhalf life    2xhalf life

    10mins   +  10mins = 20mins

112Bq  è  56Bq  è  28Bq = activity of radioisotope after 20 mins

 

But this doesn’t include the background rate!

Detector reading = 28Bq + 7Bq = 35Bq

 

4.              Potassium decays into argon.  The half life of potassium is 1.3 billion years.  A sample of rock from Mars is found to contain three argon atoms for every atom of potassium.  How old is the rock?

 

Proportion of K:       1  è  ½  è  ¼

Proportion of Ar:      0  è  ½  è  3/4   

                                                   1xhalf life    2xhalf life

So after 2 half lives there will be 3 times as many Ar atoms as K atoms

Age of rocks = 2 x half life = 2 x 1.3x109 = 2.6 billion years

 

7.4 to 7.12 Plenary questions

radioactivitty plenary multichoice questions.pptm Download this file

7.14

starter

01 February 2012

13:08

Tell the person next to you…

·         What is the most dangerous type of radiation outside the body?  Why?

·         What is the most dangerous type of radiation inside the body?  Why?

·         Gamma radiation is the most dangerous type of radiation outside the body because it is extremely penetrating.  (Alpha radiation is not dangerous because it is stopped by skin)

·         Alpha radiation is the most dangerous type of radiation inside the body because it is highly ionising due to its high charge (+2) and high mass (RAM=4).  (Gamma radiation is only very weakly ionising)

 

 

7.14

12 January 2012

10:24

·         7.14 describe the dangers of ionising radiations, including:

·         radiation can cause mutations in living organisms

·         radiation can damage cells and tissue

·         the problems arising in the disposal of radioactive waste

<<Dangers of radioactivity.pptm>>

Chernobyl Disaster

Hiroshima and Nagasaki - the first nuclear bombs

After the Hiroshima bomb

Dangers of radioactivity.pptm Download this file

alpha, beta, gamma - effect on human body.pptx Download this file