Modeling with Embodiment for Inquiry-Based Science Education
Abstract
1. Theoretical Framework
2. Methodology
2.1. Inquiry-Based Modeling with Embodiment (IBME): An Approach to Teach Science Phenomena
- (A)
- Problematization and first ingredientsThis step corresponds to the first phase of inquiry-based learning, as it involves first observations or clues that are going to serve students in building their model. It is important here not to give students hints about the model itself but the ingredients that they have to use to fit their proposals.
- (B)
- Model buildingThis is one of the most important parts of the modeling process, which is the selection of properties that we want to include/exclude compared to the real phenomenon. With the construction of the model and its subsequent representation, the students begin the investigation phase of IBL, characterized here by the search, representation, and improvement of the model through successive iterations.
- (a)
- What properties do we want to represent? What objects, interactions, or variables do we want to represent? These are called included variables.
- (b)
- What objects, interactions, or variables are we going to exclude because they are not relevant? This is a model-building decision: an appropriate model choice that better fits the goal of my study (how far or close I want to be from the real phenomenon). These are called excluded variables by choice.
- (c)
- What objects, interactions, or variables are we going to exclude because they cannot be represented by my modeling tool? There will be variables that are impossible to be present in the model due to the limitations of the modeling tool. These are called excluded variables due to model limitations.
- (C)
- Model representationAlthough the entire class, which works in teams under this framework, developed their model (step B), we typically conduct a collective analysis of the representation. In this way, only one team will present their representation (role play, embodiment) to the rest. The acting team must remain silent and should not inform the other teams about the roles they are playing or the details of the dynamics being represented: they should only perform. The other teams, while thinking about their own models, should begin making notes on step D as they observe the representation.As we mentioned at the beginning, this is an iterative process, so it is possible that the analysis step (D) leads to another representation, performed by the same team or by a different one.
- (D)
- Model testingIn the conclusion phase of the inquiry process, students must, after testing the model, verify its scope. To test whether the proposed model is “the good” model or still needs iteration, here are some questions that must be addressed:
- (a)
- Identify elements of the model and their functions: included variables.
- (b)
- Discuss the properties of the phenomenon that have been excluded: excluded variables by choice or by model limitations.
- (c)
- Reliability of the model: Does it match the observations? Is it consistent with other established models/knowledge? Our model should not contradict other models/knowledge that have already been proven.
- (E)
- Model scopeWhat predictions does it provide? What are the limitations of our model? What is the related phenomenology?These steps are formulated to be solved by the students, under the guidance of the teacher.
2.2. The Evaluation of the IBME Research Methodology
2.2.1. The Design and the Sample
2.2.2. The Teaching Sequences Based on IBME Methodology
2.2.3. Instruments for Evaluating the Effectiveness of the Didactic Sequence
- (1)
- Descriptive evaluation.The session descriptions are presented in the Section 3. The variables used to summarize the progress of the induced modeling process are below. This could be reviewed through the recordings of the sessions.
- Achievement of the final model: Did the modeling refinement process enable students to propose the best model, in line with the learning objectives?
- Complexity of the model: How many model iterations were needed to reach the final model? It is worth noting that a higher or lower number of iterations does not necessarily indicate higher or lower effectiveness of the modeling process, as long as these iterations contribute to discussing ideas intertwined with the phenomenon. However, it does indicate the complexity of the model and the understanding of the phenomenon.
- Related submodels and misconceptions or difficulties: In most cases, the iterations occur because either the “excluded/included variables” need to be adjusted, or because a particular iteration includes a misconception that needs to be discussed. This is why we also account for the submodels that emerge and provide a summary of the difficulties that students have had to overcome.
- (2)
- Quantitative evaluation through a questionnaire.Both the experimental group (n = 86) and the control group (n = 68) of students answered an 8-question questionnaire on some basic concepts related to teaching sequences (see Appendix A). For validation, expert judgment and a pilot test were conducted on a group not included in the control and experimental groups. The data obtained by the four researchers were then discussed until a final consensus was reached, allowing the design of the current questionnaire. The Cronbach’s Alpha test was applied, yielding a value of 0.723 for the pilot group, which was also higher than 0.7 for the experimental and control groups, indicating a medium-high reliability. The questionnaire was completed by all students one month after the last teaching intervention, without prior warning, to assess real learning.Questions 1 to 3 refer to some of the concepts related to the modeling experiences of the Solar System (see Appendix A):
- Lunar phases and eclipses.
- Apparent retrograde motion of the planets.
- Discussion of the geocentric and heliocentric models.
Questions 4 to 7 deal with some of the concepts related to the experiences of modeling the states of matter:- Properties of states.
- Changes of state.
3. Results
3.1. Descriptive Evaluation
3.1.1. Proposal for the Earth–Sun–Moon System
Lunar Phases and Eclipses
Apparent Retrograde Motion of the Planets (A.9)
Discussion Between the Geocentric and the Heliocentric Model: Parallax (A.10)
Summary of the Descriptive Results for Macroscopic Phenomena
3.1.2. Proposal for the States of Matter
Properties of the States of Matter
Changes of State
Summary of the Descriptive Results for Microscopic Phenomena
3.2. Results of the Quantitative Evaluation Through Questionnaires
“Because there is only an eclipse when they are on the same line, as the line (orbit) is inclined, it is not at the same level, and there is no eclipse.”“Because the orbit is inclined, i.e., it is not at the same level.”“Because they are not totally aligned, and for an eclipse to exist, they have to be aligned.”
“Because the Moon is in front of the Sun so that the side of the Moon facing the Earth is not illuminated by the Sun’s rays. Therefore, it is not illuminated from the Earth.”“The Moon is located between the Earth and the Sun so that its illuminated hemisphere cannot be seen from our planet.”
“From Earth, we can see Mars going forwards and backwards because each planet rotates at different speeds, and so at each moment, we can see Mars in a more forward or backward position.”
“Due to the great distance between the Earth and the stars, no movement of the stars can be seen.”
“Bonds allow it (liquid) to change shape, but the volume remains the same.”
“The bonds between the particles are so strong that they do not separate, therefore, the solid always maintains its shape and volume.”
“Because the particles are very close together and move very little.”
“Because the bonds that join the particles of gases are so weak that they allow them to both change position and increase the distance between them and therefore occupy all the space available to them.”
“…as the temperature rises, they would have to move more in their place, then changing places and finally around the whole class.”
“They can only stand upright, although they can climb on a chair.”“You don’t know the exact amount of temperature that rises or falls, so you don’t know the dimension to which the pupils have to expand.”“…people don’t go as fast as particles...”“It is difficult to represent the links.”
3.3. Results for the Additional Question for Students in the Experimental Group
“There were times when I did not understand with the theoretical explanation, but with the moon cycle, I found it very useful.”“More visual, easier to learn.”“It helps a lot to understand, in spite of the limitations it may have to represent specific aspects.”“It has been quite useful when it comes to remembering both astronomy and chemistry questions.”
4. Discussion
5. Conclusions
Author Contributions
Funding
Institutional Review Board Statement
Informed Consent Statement
Data Availability Statement
Conflicts of Interest
Abbreviations
IBME | Inquiry-based modeling with embodiment |
Appendix A
I have been informed of the characteristics of the Research Project. I have been able to express any questions that have arisen in this regard. I consider that I have understood this information. I am informed of the possibility of withdrawing from the study at any time. Under these conditions, I agree to participate in this study. Name and surname: Age: Baccalaureate option you studied: 1.a. It depicts in a schematic drawing the phases of the Moon (as if you were an observer outside the Earth). In the drawing the Moon, the Earth and the Sun must appear. Indicate with an arrow what is the direction of movement of the Moon.
1.c. Why don’t you see the new moon? 2. How can we explain, with the heliocentric model, that from the point of view of the Earth we see that a planet like Mars goes back and forth in its journey through the sky? 3. When Copernicus defended the heliocentric model, astronomers objected that how could it be, if the Earth moved, that we see the stars retain their relative position. That is, if the Earth moves, wouldn’t we have to see the distance between two stars in the same constellation vary for a matter of perspective, in the same way that we see that the distance between two buildings changes as we pass by in a running car? Explains Copernicus’ reasoning for answering this question. 4. How can you explain at the corpuscular (microscopic) level that the liquid changes shape, but not volume when changing the container? 5. How can you explain at the corpuscular (microscopic) level that the solid does not change shape or volume when changing the container? 6. How can you explain at the corpuscular (microscopic) level the property of gases to occupy the entire volume where they are located? 7. Imagine that a group of students have to represent the changes in state from solid to liquid and from liquid to gas, as the temperature rises. Each of them would represent a molecule of the material that, all together, they represent, while the material changes state.
(Experimental group only) 8. Value the embodiment experience:
|
Appendix B
Rating Scale | Item |
(1) Accurately represents the Sun–Earth–Moon astronomical system, the relative positions of the three bodies in each phase, and indicates the Moon’s direction of rotation. | 1a |
(0.5) Same as above but without indicating the direction of rotation or with an error in one of the phases. | |
(0) The astronomical system is nonsensical or not represented (e.g., shows the phases as seen from Earth or something similar). | |
(1) Correctly mentions the effect of alignment in the difference between lunar phase and eclipse. Not just describes what an eclipse is, but explains why the lunar phase being compared is not an eclipse. | 1b |
(0.5) Only describes what an eclipse is but does not explain why it does not occur every month in the corresponding lunar phase. Does not compare both phenomena. Also applies if only alignment is mentioned. | |
(0) Other cases or incorrect mention of the above effect. | |
(1) Complete and correct explanation using the relative positions of the Earth–Sun–Moon system. | 1c |
(0.5) Semi-complete explanation: Only indicates the position but does not explain. | |
(0) Incorrect explanation (wrong Earth–Sun–Moon positions or refers to what would be seen “during the day,” which is not possible, etc.). | |
(1) Complete and correct explanation of the retrograde motion phenomenon: refers to both the different orbital speeds and the different orbit sizes. | 2 |
(0.5) Semi-complete explanation: Partially explains the phenomenon or explains it superficially. Mentions only speed or only orbit size. | |
(0) Incorrect explanation. | |
(1) Correct answer: The distance to the stars is too great in comparison to the size of Earth’s orbit (Note: must say “in comparison”). | 3 |
(0.5) Only says that we are very far away or refers to only one of the two effects. | |
(0) Incorrect answer. | |
(1) Complete explanation: Particles in a liquid feel forces that hold them together, but not as strongly as in a solid. This allows them to leave their “positions” but not stray “too far” from each other. Refers to both bonding and particle positions. | 4 |
(0.5) Semi-complete explanation: More or less the above, but with little rigor or inappropriate language. Forgets bonding and only talks about positions or vice versa. | |
(0) Incorrect explanation: Any other. | |
(1) Complete explanation: The forces between particles are so strong that the lattice remains intact. This prevents them from leaving their positions or changing the distance between them. Mentions both positions and bonding. | 5 |
(0.5) Semi-complete explanation: Same as above but less rigorous and incomplete. | |
(0) Incorrect explanation: Any other. Shows the alternative idea that assigns macroscopic properties to microscopic particles. | |
(1) Complete explanation: The forces between the particles are very weak, and the particles leave their positions and are not constrained by the presence of others (they can change the distance between them—almost free particles). | 6 |
(0.5) Semi-complete explanation: Same as above but with less rigor and detail. | |
(0) Incorrect explanation: Any other. Shows the alternative idea that assigns macroscopic properties to microscopic particles. | |
(1) Has a clear understanding of the content and the proposed model is free of errors. Proposes the model elements and their dynamics correctly. Mentions particles, the variables of position and force between particles, and correctly describes the gradation. | 7a |
(0.5) Has a clear understanding of the content, but the proposed model has errors or is poorly detailed. | |
(0) Does not have a clear understanding of the content, and the proposed model is very limited. | |
(1) Identifies the limitations of the model (not to be confused with errors!), that is, what things it does not explain because they are not relevant. | 7b |
(0.5) Points out space as one of the limitations. Note if any mention of scale is made. | |
(0) Does not respond appropriately. |
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Inquiry Problem | Step | Learning Objectives | Activity |
---|---|---|---|
Lunar phases: Identification and analysis. | A | Identify the phases of the Moon and the role of the Sun, Earth, and Moon in the phenomenon. Separate the lunar phases into similar phases: quarters, full, and new. | A.1 Give a brief description of the movement of the Moon around the Earth and the phases of the Moon (previous modeling data). A.2 Which way does the Earth rotate? |
Representation of the full moon and new lunar phases using a model. | B, C | Identify the Sun, Earth, and Moon as elements of the model and the translation of the Moon around the Earth as a mechanism of the phenomenon. Analyze the similarities and differences between the “full and new” and “quarter” phases. | A.3 Represent the movement of the Moon around the Earth. What face of the Moon do we see? How many times has the Earth turned around itself when the Moon has made one complete revolution? A.4 Represent the phases of the full and new moon using the heliocentric model. |
Discussion of the role of misalignment between the Sun, Earth, and Moon in these phases. Refinement of the model with the inclination of the lunar orbit. | D, E | Discuss and analyze why solar and lunar eclipses do not occur every “month”. | A.5 Why do eclipses not occur every month at the full and new moon phases? |
Representation of the first and last quarters and discussion of the direction of rotation of the Moon around the Earth. | B, C | Find the relative position of the Sun, Earth, and Moon in the phases of waxing and waning quarters, as well as analyze the succession of the four lunar phases. | A.6 Represent the lunar phases of the waxing and waning quarters and discuss the direction of rotation of the Moon around the Earth. |
Discussion about the times of day when you can see the different phases. | D, E | Highlight the diurnal visibility of the Moon and analyze the relative position of the three bodies in this situation. Analyze and compare the “fourth” phase with the new moon phase. | A.7 Discuss the times of day when the different phases can actually be seen. |
Discussion of how the shape of the same phase of the Moon changes depending on latitude. | D, E | Highlight the link between astronomical knowledge and the usual geolocation. Extrapolate the knowledge acquired to situations different from the usual ones. Formulation and contrast of general hypotheses. | A.8 Could the model used in the previous activities be used for learning in schools in Australia? Analyze what the phases of the Moon would look like in the southern hemisphere. |
Extension of phenomenology: retrogradation, parallax, and Kepler’s laws. | E (A, B, C, D) | Identify the size of the solar system as one of the limitations to the representation of the model. Expand the phenomenology associated with the elements and dynamics of the solar system. | A.9 One of the main difficulties of the geocentric model was the explanation of the retrogradation of Mars by epicycles and deferents, which the heliocentric theory elegantly solved. Represent the retrograde motion of Mars using the heliocentric model. A.10 Fixed stars were used as an argument against the Copernican heliocentric theory. If the Earth moves, as Copernicus said, should we see how the position of a star on the background (the celestial sphere) varies as a matter of perspective? Represent the situation in the classroom. |
Inquiry Problem | Step | Learning Objectives | Activity |
---|---|---|---|
Macroscopic and microscopic structure of matter. Kinetic theory. | A | Enunciate the macroscopic differences between solids, liquids, and gases and propose their microscopic structure based on atomic-molecular theory and the links between particles. | A.1 Mention the macroscopic differences between solids, liquids, and gases (previous modeling data). |
Microscopic structure of matter: kinetic theory. | B | Develop the model to be represented considering people as the particles that make up matter and propose the chemical bonds between them. | A.2 According to the macroscopic properties of solids, propose a microscopic representation for this state. A.3 According to the macroscopic properties of liquids, propose a microscopic representation for this state. A.4 According to the macroscopic properties of gases, propose a microscopic representation for this state. |
Macroscopic properties of solids, liquids, and gases from the microscopic representation. | C, D | Understand the behavior of the particles that form matter according to the kinetic-molecular theory, the bonds that are established between them. | A.5. Represent a transition from solid to liquid and then to gas as the temperature increases. |
Phase of matter changes. | E (B, C, D) | Understand the role of bonds between particles as a determinant of the phase of matter. | |
Temperature as a measure of particle velocity. | E (B, C, D) | Understand the state of motion of the particles that make up matter. Understand temperature as a measure of the average kinetic energy of particles. Understand the meaning of absolute zero temperature. |
Model | Achievement of the Final Model | Iterations | Related Submodel |
---|---|---|---|
Lunar phases and eclipses | Completed through the modeling process. Found difficulties: distances between celestial bodies. Relative rotational periods. | 2 | Rotation and translation of the Earth and the Moon and their periods, determining the relevance of the models regarding the phenomenon (selection of variables) |
2 | Difficulty in distinguishing between the movements of rotation and translation to show the same face of the Moon | ||
3 | Discussions about the alignment between celestial bodies to describe lunar phases and solar and lunar eclipses | ||
1 | Correlation between the times of day when phases are “seen” and the north–south hemisphere difference | ||
Apparent retrograde motion of the planets | Completed through the modeling process. | 1 | Differentiating the relevance of the rotation and translation of the planets regarding the phenomenon under study |
1 | Discussion about the speed and scale of the model | ||
1 | Determining the point of view on a planet and verbally describing the trajectories of other planets | ||
Parallax | Completed through the modeling process. Found difficulties: distance between Earth and stars and Earth orbit eccentricity. | 3 | Problem setting and relative scales to accurately represent distances |
1 | Translation movement of a planet relative to fixed stars and approximation of parallax according to the planet’s point of view |
Model | Achievement of the Final Model | Iterations | Related Submodel |
---|---|---|---|
The solid state | Completed through the modeling process. Found difficulties: Representing vibrations. | 2 | Particle arrangement (molecules or atoms) and identification of properties with the representation (distance between them, bonds…) |
2 | Identification of macroscopic properties (solid behavior according to temperature or container change, compression) with microscopic behavior | ||
The liquid state | Completed through the modeling process. | 1 | Particle arrangement (molecules or atoms) and identification of properties with the representation (distance between them, bonds…) |
1 | Bonding in liquids | ||
2 | Identification of macroscopic properties (solid behavior according to temperature or container change, compression) with microscopic behavior | ||
The gaseous state | Completed through the modeling process. Found difficulties: Simulating the full particle movement using the classroom completely. | 1 | Particle arrangement (molecules or atoms) and identification of properties with the representation (distance between them, bonds…) |
1 | Bonding in gases and pressure | ||
1 | Identification of macroscopic properties (solid behavior according to temperature or container change, compression) with microscopic behavior | ||
Changes of state according to temperature | Completed through the modeling process. Found difficulties: How to model bond changes in the state change moment. | 2 | Combination of all the previous elements, nuances on intermediate states |
Cohen’s d | Effect Size | |
---|---|---|
1.a. Moon phases | 0.43 | Middle |
1.b. Lunar eclipse | 0.36 | Small |
1.c. New Moon | 0.54 | Middle |
2. Retrograde motion | 0.65 | Middle |
3. Parallax | 1.26 | Large |
4. Liquid | 0.46 | Middle |
5. Solid | 0.48 | Middle |
6. Gas | 0.65 | Middle |
7. Phase transition (model) | 1.10 | Large |
8. Phase transition (limitation) | 0.99 | Large |
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Solbes, J.; Palomar, R.; Petit, M.F.; Tuzón, P. Modeling with Embodiment for Inquiry-Based Science Education. Educ. Sci. 2025, 15, 796. https://doi.org/10.3390/educsci15070796
Solbes J, Palomar R, Petit MF, Tuzón P. Modeling with Embodiment for Inquiry-Based Science Education. Education Sciences. 2025; 15(7):796. https://doi.org/10.3390/educsci15070796
Chicago/Turabian StyleSolbes, Jordi, Rafael Palomar, M. Francisca Petit, and Paula Tuzón. 2025. "Modeling with Embodiment for Inquiry-Based Science Education" Education Sciences 15, no. 7: 796. https://doi.org/10.3390/educsci15070796
APA StyleSolbes, J., Palomar, R., Petit, M. F., & Tuzón, P. (2025). Modeling with Embodiment for Inquiry-Based Science Education. Education Sciences, 15(7), 796. https://doi.org/10.3390/educsci15070796