Modelling the Dynamics of a Hypothetical Planet X by way of Gravitational N-body Simulator

التفاصيل البيبلوغرافية
العنوان: Modelling the Dynamics of a Hypothetical Planet X by way of Gravitational N-body Simulator
المؤلفون: Cowley, Michael J., Hughes, Stephen W.
المصدر: Cowley, M., & Hughes, S. 2017, Eur J Phys, 38 (IOP Publishing), 025602
سنة النشر: 2017
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Instrumentation and Methods for Astrophysics
الوصف: This paper describes a novel activity to model the dynamics of a Jupiter-mass, trans-Neptunian planet of a highly eccentric orbit. Despite a history rooted in modern astronomy, "Planet X", a hypothesised hidden planet lurking in our outer Solar System, has often been touted by conspiracy theorists as the cause of past mass extinction events on Earth, as well as other modern-day doomsday scenarios. Frequently dismissed as pseudoscience by astronomers, these stories continue to draw the attention of the public by provoking mass media coverage. Targeted at junior undergraduate levels, this activity allows students to debunk some of the myths surrounding Planet X by using simulation software to demonstrate that such a large-mass planet with extreme eccentricity would be unable to enter our Solar System unnoticed, let alone maintain a stable orbit.
Comment: 11 pages, 4 figures, published in Eur. J. Phys
نوع الوثيقة: Working Paper
DOI: 10.1088/1361-6404/aa5448
URL الوصول: http://arxiv.org/abs/1701.07711
رقم الانضمام: edsarx.1701.07711
قاعدة البيانات: arXiv
الوصف
DOI:10.1088/1361-6404/aa5448