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Orbital motions of astronomical bodies and their centre of mass from different reference frames: A conceptual step between the geocentric and heliocentric models

Title
Orbital motions of astronomical bodies and their centre of mass from different reference frames: A conceptual step between the geocentric and heliocentric models
Type
Article in International Scientific Journal
Year
2016
Authors
Guerra, AGC
(Author)
Other
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Carvalho, PS
(Author)
FCUP
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Journal
Title: Physics EducationImported from Authenticus Search for Journal Publications
Vol. 51
Final page: 055012
ISSN: 0031-9120
Indexing
Scientific classification
CORDIS: Social sciences > Educational sciences > Education > Science education
FOS: Social sciences > Educational sciences
Other information
Authenticus ID: P-00K-TZN
Abstract (EN): The motion of astronomical bodies and the centre of mass of the system is not always well perceived by students. One of the struggles is the conceptual change of reference frame, which is the same that held back the acceptance of the Heliocentric model over the Geocentric one. To address the question, the notion of centre of mass, motion equations (and their numerical solution for a system of multiple bodies), and change of frame of reference is introduced. The discussion is done based on conceptual and real world examples, using the solar system. Consequently, through the use of simple 'do it yourself' methods and basic equations, students can debate complex motions, and have a wider and potentially effective understanding of physics. © 2016 IOP Publishing Ltd.
Language: English
Type (Professor's evaluation): Scientific
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