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Inquiry Learning Spaces (ILSs) are personalized learning resources for students, including a lab, apps, and any other type of multimedia material. ILSs follow an inquiry cycle. Inquiry cycles can differ but the basic Go-Lab cycle consists of the phases Orientation, Conceptualisation, Investigation, Conclusion, and Discussion. The aim of an ILS is to provide students with an opportunity to conduct scientific experiments, being guided through the inquiry process and supported at each step.

This page presents ILSs created by teachers or the Go-Lab and/or Next-Lab team (and often in co-creation), on a large set of domains and in many languages. You can create ILSs starting from an online lab, but also copy and adapt an existing ILS with the help of the Go-Lab authoring platform. Visit the Support page where you will find demo-videos, tips & tricks, and user manuals, that explain how to work with the Go-Lab authoring platform and how to publish your own ILS once it is finished.

If you are looking for Inquiry Learning Spaces especially suitable for the curricula of Benin, Kenya or Nigeria, please visit our Collections page.

Astronomy
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Irish language version of Northern Lights

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Cet ILS permet de comprendre les lois de la gravitation universelle et de pouvoir les énoncer. Comment nos pieds restent toujours en contact avec le sol, pourquoi y'a la révolution et la rotation de la terre autour du soleil.

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Ανιχνεύσιμα βαρυτικά κύματα, μπορούν να δημιουργηθούν από πολύ μεγάλης μάζας σώματα όπως οι μελανές οπές και οι αστέρες νετρονίων τα οποία περιστρέφονται το ένα γύρω από το άλλο.

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Las ondas gravitacionales detectables pueden ser creadas por objetos compactos masivos (como agujeros negros o estrellas de neutrones) que orbitan entre sí. ¿Cómo podemos modelar esto con materiales cotidianos?

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Como utilizamos o espaço para nos observarmos? O que é que as medições do clima e da meteorologia nos dizem sobre a Terra e o nosso ambiente?

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ILS intended for elementary preservice science teachers. Study of the phases of the moon from different locations and the moon's face towards Earth.

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Una aurora es la emisión de luz causada por la colisión de partículas cargadas altamente energéticas procedentes del plasma emitido por el sol (viento solar) con los gases de la parte de la atmósfera terrestre llamada Termosfera.

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¿Cómo utilizamos el espacio para mirarnos a nosotros mismos? ¿Qué nos dicen las mediciones climáticas y meteorológicas sobre la Tierra y nuestro entorno? Los estudiantes explorarán los datos de irradiación solar utilizando datos de satélite.

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Detectable Gravitational Waves can be created by massive compact objects (like black holes or neutron stars) that orbit each other. How can we model this with everyday materials? How can we use Tracker to carry out digital video analysis of our model to study the circular motion?

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Το Σέλας είναι η εκπομπή φωτός που προκαλείται από την αλληλεπίδραση φορτισμένων σωματιδίων από τον Ήλιο με τα αέρια των ανώτερων στρωμάτων της ατμόσφαιρας.