Supports National Curriculum, Key Stages 1D, 3F, 5E
Suitable for years 4,5 and 6. The first sections might be suitable for year 3.
The time for whole session is about 1 hour 30mins. This can be varied by taking shorter paths through the material e.g. by omitting the section on eclipses for younger children or by omitting the sections on shadows for older children. Choices will depend on the particular needs of the school.
Outline of content
Aims to
Points to note:
Please read the notes about risks and agree the assessment with the teacher before the session! (Link to safety notes at end of this file)
Cross References
- The slides in the PowerPoint presentation are referenced in the table.
Vocabulary: The presentation uses expressions included in the KS1&2 strategies http://www.standards.dfes.gov.uk/schemes2/science/?view=get
Misconceptions – ie - points that are often misunderstood
The session should be held in a room that is not brightly lit. Curtains or slat blinds could be shut but the activities have been planned so that blackout is NOT required as this is difficult to achieve in most primary schools and also might cause behaviour problems.
|
Activities |
Discussion |
Aims/facts |
1 |
Slide 2 |
The first few slides allows them to discuss their ideas of fast speeds and to try grasp some understanding of the distances between the Earth, Moon and Sun. Explain that these are thought experiments or mental space journeys. |
To establish that the Sun is very much further away from Earth than the Moon and both distances are very large compared to distances on Earth. |
2 |
Slide 3 |
They might point out that the petrol would run out or the driver would need food but explain that it is a thought experiment that overcomes problems. |
The Moon is a very, very long way away from the Earth compared with distances between cities. |
3 |
Slide 4 |
They enjoy discussing the problems with travelling for such a long time. This emphasises the huge distance. |
The Sun is very, very much further away from Earth than the Moon. |
4 |
Slide 5 + 6 |
Take the opportunity to point out that the Sun is a powerful source of light and heat. |
Light moves very, very quickly through space. |
5 |
Slide 7 – Point a bright torch across the room and shake chalk dust from a duster in the beam of light so that they can see that light travels in straight lines. |
Discuss what happens when something gets in the way of the light. |
Light travels in straight lines |
6 |
Slide 8 - Shadows |
(This may be covered quickly if it has already been studied.) |
Light cannot bend round a barrier. |
7 |
Game with sheet |
Stand to one side during the demonstration with the sheet so that you can see the class and keep control during this fun activity. Discuss the changes in the shadow as positions change. |
Shadows are similar in shape to the objects forming them. |
8 |
Slide 10 |
Discuss the fact that the part of the Earth with the Sun shining on it is in ‘daylight’ while at the opposite side of the Earth it is night. |
During daytime the Sun light reaches half the globe. During one day the Earth rotates once on its axis. A day = 24 hours |
9 |
Ask for a volunteer who should stand at the front looking towards the class. Point a bright torch onto the child as ask him/her to turn round slowly. Point out that you and the torch are acting as the Sun and the volunteer is the Earth. Ask whether the Earth just rotates or whether it also moves. Encourage the child to move around you – eventually rotating slowly to simulate the movement of the Earth round the Sun. |
Ask how long it takes for the Earth to move round the Sun once – 1 year. |
The Earth takes 365 days to orbit (rotate around) the Sun. The Earth rotates 365 times during the time it takes to orbit the Sun once. |
10 |
Slide 14 |
Discuss whether the Sun shines in at same place in the classroom during the day. |
The Sun appears to move across the sky in a regular way every day. |
11 |
Slide 15 |
Discuss sundials – often seen on or by old buildings. |
Shadows caused by the Sun can be used to tell the time. |
12 |
Slide 16 |
Slide 17 |
|
13 |
The seasons |
Ask whether they notice any difference in the path of the sun across the sky during winter and summer. They may comment that shadows caused by the Sun generally are longer during winter. |
In winter the weather is colder than in summer. |
14 |
Slide 19 The slide also shows that days are longer in summer than winter. |
In discussion point out that the Sun rises at a point further east and sets at appoint further west in summer than in winter (some websites incorrectly show the sunrise at the same point on the horizon for summer and winter). |
The Sun rises in the East and sets in the West. |
15 |
Slide 20 |
Ask what makes it colder in winter than in summer. They may answer that the Earth is further from the Sun in winter. It is true that the orbit of the Sun is slightly elliptical but the Earth can be closest to the Sun in January. |
|
16 |
Demonstration |
Repeat the demonstration and discuss the effect Also the Sun is above the horizon for a shorter time than in Summer so the total heat reaching the region is less than in Summer. The light travels slightly further through the atmosphere in winter so more heat is absorbed. Explain that the seasons are caused because the axis of the Earth is tipped by 23 degrees. |
Extra to KS2: |
17 |
Game |
Emphasise that the effect is for heat as well as light and discuss the effects if first one stands in front of a radiant heater and then stands to one side. |
|
18 |
Slide 21, 22 |
In demonstration 1 the ball does not rotate, which is incorrect. |
The Moon is not a source of light. The Moon reflects light from the Sun to the Earth. The Moon takes approximately 28 days to orbit the Earth. The changing appearance of the Moon over 28 days provides evidence for a 28-day cycle. |
19 |
Slide 23 |
Slide 24 - They should answer |
Reinforce ideas. |
20 |
Slide 25 |
It is best to demonstrate this first at the front and discuss the distances before allowing the groups to try the game. Explain that this helps to understand why the Moon and the Sun appear the same size. Refer back to the distances discussed at the start of the session. |
The sun and the Moon look the same size because they are different distances from the Earth. |
21 |
Slide 26 Slide 29 |
During discussion slide 28 will help. Explain that sometimes the Sun Moon and Earth are not quite in line. Then there is a partial eclipse. These are much more common. If possible tell them when the next partial eclipse can be seen in the UK. The last total eclipse visible from the UK was seen in southern England on 11th August 1999. An animation of an eclipse on 29th March 2006 that was visible as a partial eclipse from the UK can be seen at http://www.eclipse.org.uk/eclipse/0212006/ The next eclipse of the Sun visible from the UK will be on 1st August 2008 and will be seen as a partial eclipse from the UK. |
Extra to KS2: |
22 |
Slide 30 |
Explain that this is different from the situation for a new moon because then the moon is between the earth and the Sun. |
Extra to KS2: |
23 |
Take the opportunity to revise using slide 31. |
|
|
24 |
Slide 32 |
The picture shows the space shuttle leaving the international space station. Encourage a discussion about the benefits- and whether they would like to be astronauts- point out that many astronauts have studied physics (most have studied science). |
|
25 |
Slide 34 |
Link back to the time worked out to reach the Sun and Moon at 70 mph and explain that space probes travel much faster than that. |
|
26 |
Slide 36 |
Keep asking questions. |
There is a lot more for scientists to find out. |
Safety Notes
Warn children NEVER to look directly at the Sun. It can cause permanent damage to their eyes. Blindness can result.
Tell them that it can burn their eyes because it is so bright.
See 'Be Safe' section 13 - available form the ASE
http://www.ase.org.uk/htm/book_store/detail.php?SIID=67
Apparatus
Please read the safety notes.
Activity 5 – light travels in straight lines – quick demonstration
Activity 7 – Game with sheet
Activity 8 - Day and night
Activity 12 - solar pyramid website
http://www.solarpyramid.co.uk/
Activity 16 - Seasons:
Slide 20 - consider beams of light (and heat) from the Sun, reaching the surface of the Earth. During the winter a beam, of a fixed cross-section, reaching the surface of the Earth will be spread over a greater area than a similar beam reaching the Earth in the summer. An umbrella is held first with its surface tipped towards the beam of light from the torch and then tipped away. The torch should be the same distance from the umbrella throughout the experiment because it is not emitting a parallel beam of light.
The demonstration could also be used to show that in summer, when the sun is high in the sky, the heat and light is concentrated on the surface - a small bright circle is seen in the demonstration. Then in winter when the Sun is low in the sky, a larger dimmer oval is seen because the heat and light are less concentrated, (less spread out).
Understanding statements such as ‘the energy received per unit cross sectional area of the surface of the Earth’ is difficult for all children. This demonstration and slides 19 and 20 explain why it is colder in winter than in summer. Also the Sun is above the horizon for a shorter time than in summer so the total heat reaching the region is less than in summer. The light travels slightly further through the atmosphere in winter so more heat is absorbed.
Activity 17 – Game to explain seasons
For each group of about 4 children:
Activity 18 – Demonstration 1 of phases of the Moon
Cover the ball so that it is half white and half black
Activity 18 – Demonstration 2 of phases of the Moon
(if a white ball is not available then paint a ball or cover it with white plastic.)
Use a maker pen to draw a large face on one side of the white ball.
Make a sliding cover:
Use the adhesive tape to stick the black plastic round the edge of the clear plastic circle.
Shape the plastic over the ball and draw the black plastic loosely to keep the cover on the ball. Cut a hole to allow your hand to hold the ball.
Activity 20 – Game to explain that apparent size varies with distance
For each group of about 4 children:
Activity 21 – to explain eclipse of Sun
Activity 25 - Pluto probe
http://space.newscientist.com/article.ns?id=dn8587&feedId=online-news_rss20
http://www.washingtonpost.com/wp-dyn/content/article/2005/12/18/AR2005121800976_2.html
Source: https://www.iop.org/activity/outreach/resources/pips/topics/sunlight_space/file_43050.doc
Web site to visit: https://www.iop.org
Author of the text: indicated on the source document of the above text
If you are the author of the text above and you not agree to share your knowledge for teaching, research, scholarship (for fair use as indicated in the United States copyrigh low) please send us an e-mail and we will remove your text quickly. Fair use is a limitation and exception to the exclusive right granted by copyright law to the author of a creative work. In United States copyright law, fair use is a doctrine that permits limited use of copyrighted material without acquiring permission from the rights holders. Examples of fair use include commentary, search engines, criticism, news reporting, research, teaching, library archiving and scholarship. It provides for the legal, unlicensed citation or incorporation of copyrighted material in another author's work under a four-factor balancing test. (source: http://en.wikipedia.org/wiki/Fair_use)
The information of medicine and health contained in the site are of a general nature and purpose which is purely informative and for this reason may not replace in any case, the council of a doctor or a qualified entity legally to the profession.
The texts are the property of their respective authors and we thank them for giving us the opportunity to share for free to students, teachers and users of the Web their texts will used only for illustrative educational and scientific purposes only.
All the information in our site are given for nonprofit educational purposes