Discover the best method of teaching science and download free teaching resources


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Discover the best method of teaching science and download free teaching resources------

Food! Community Research Guide
Food! is a freely available community research guide that uses the United Nations Sustainable Development Goals (SDGs) as a framework to focus on sustainable actions that are defined and implemented by students (download it here).
Mosquito! Community Research Guide
This module effectively promotes excellence within science education while fostering pioneering approaches to empower and unite educators around the world. Mosquito! addresses the problem of diseases transmitted by mosquitoes from an educational point of view (download it here). 
Other teaching resources and guides
You can download more teaching resources and guides here.

Science education ideas
The IAP publication “Working with Big Ideas of Science Education” (available for free here) includes this list of ideas that all students should have had opportunity to learn by the end of compulsory education:
All matter in the Universe is made of very small particles
Atoms are the building blocks of all matter, living and non-living. The behaviour and arrangement of the atoms explains the properties of different materials. In chemical reactions atoms are rearranged to form new substances. Each atom has a nucleus containing neutrons and protons, surrounded by electrons. The opposite electric charges of protons and electrons attract each other, keeping atoms together and accounting for the formation of some compounds.
Objects can affect other objects at a distance
All objects have an effect on other objects without being in contact with them. In some cases the effect travels out from the source to the receiver in the form of radiation (e.g. visible light). In other cases action at a distance is explained in terms of the existence of a field of influence between objects, such as a magnetic, electric or gravitational field. Gravity is a universal force of attraction between all objects however large or small, keeping the planets in orbit round the Sun and causing terrestrial objects to fall towards the centre of the Earth.

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