Simulasi Dampak Ledakan Supernova terhadap Planet Terdekat

Authors

  • Margareth Jacoba Da Gomes Universitas Negeri Medan
  • Cesilia Uli Sondang Sitanggang Jurusan Fisika, Program Studi Pendidikan Fisika, FMIPA, Universitas Negeri Medan,
  • Septi Maria Gultom Jurusan Fisika, Program Studi Pendidikan Fisika, FMIPA, Universitas Negeri Medan,
  • Howard Situmorang Jurusan Fisika, Program Studi Pendidikan Fisika, FMIPA, Universitas Negeri Medan,
  • Dewi Wulandari Jurusan Fisika, Program Studi Pendidikan Fisika, FMIPA, Universitas Negeri Medan,
  • Yuni Warty Jurusan Fisika, Program Studi Pendidikan Fisika, FMIPA, Universitas Negeri Medan,

DOI:

https://doi.org/10.29303/goescienceed.v6i4.1202

Keywords:

Astrophysics, Cosmic Energi, Visual Simulation, Supernova Explosion

Abstract

This study aims to analyze the comparison of kinetic energy generated by five planets in the solar system and to visually simulate the supernova explosion process as a part of exploring cosmic energy dynamics. A quantitative computational method was employed using Python programming within the Visual Studio Code environment to calculate the kinetic energy of each planet based on its mass and orbital velocity. The data were presented on a logarithmic scale graph to clearly illustrate the wide range of energy magnitudes. The simulation results show that Jupiter generates the highest energy, approximately 3,39 × 1038 Joules, while Mercury yields the lowest, around 6,83× 1030 Joules. In addition to numerical analysis, this research includes a visual simulation of a supernova explosion to depict the dramatic transition of a massive star collapsing and releasing a tremendous amount of energy. The video illustrates the sequential phases of the explosion, including core collapse, shock wave formation, and the outward dispersal of stellar material represented by intense light bursts and dynamic color shifts. This visualization reinforces the understanding of the extreme energy scales involved in supernova events and their impact on the surrounding cosmic environment, including the possible formation of neutron stars or black holes. This study demonstrates how computational modeling and visual simulations can complement each other in explaining complex astrophysical phenomena and serve as an educational tool to enhance understanding of cosmic energy and stellar evolution.

References

Bhardwaj, A., Sam, L., Buchroithner, M. F., & Grau Galofre, A. (2022). Editorial: Advances in Mars research and exploration. Frontiers in Astronomy and Space Sciences, 9(8), 1–2. https://doi.org/10.3389/fspas.2022.971104

Dastidar, R., Pignata, G., Dukiya, N., Misra, K., Hiramatsu, D., Silva-Farfán, J., Howell, D. A., Bostroem, K. A., Singh, M., Gangopadhyay, A., Kumar, A., & McCully, C. (2024). SN 2019nyk: A rapidly declining Type II supernova with early interaction signatures. Astronomy and Astrophysics, 685(A44), 1–18. https://doi.org/10.1051/0004-6361/202348642

Dessart, L., Yoon, S. C., Aguilera-Dena, D. R., & Langer, N. (2020). Supernovae Ib and Ic from the explosion of helium stars. Astronomy and Astrophysics, 642(A106), 1–16. https://doi.org/10.1051/0004-6361/202038763

Hanusch, A., Liseykina, T. V., & Malkov, M. (2019). Acceleration of cosmic rays in supernova shocks: Elemental selectivity of the injection mechanism. The Astrophysical Journal, 872(1), 108. https://doi.org/10.3847/1538-4357/aafdae

Kamijima, S. F., & Ohira, Y. (2024). Cosmic-ray acceleration in core-collapse supernova remnants with the wind termination shock. Physical Review D, 110(4), 1–16. https://doi.org/10.1103/physrevd.110.043046

Liu, Z. W., Röpke, F. K., & Han, Z. (2023). Type Ia supernova explosions in binary systems: A review. Research in Astronomy and Astrophysics, 23(8). https://doi.org/10.1088/1674-4527/acd89e

Nittler, L. R., Chabot, N. L., Grove, T. L., & Peplowski, P. N. (2018). The chemical composition of Mercury. In Mercury: The view after Messenger (Vol. 2, pp. 30–51). Cambridge University Press. https://doi.org/10.1017/9781316650684.003

O’Rourke, J. G., Wilson, C. F., Borrelli, M. E., Byrne, P. K., Dumoulin, C., Ghail, R., Gülcher, A. J. P., Jacobson, S. A., Korablev, O., Spohn, T., Way, M. J., Weller, M., & Westall, F. (2023). Venus, the planet: Introduction to the evolution of Earth’s sister planet. Space Science Reviews, 219(1), 1–61. https://doi.org/10.1007/s11214-023-00956-0

Pieri, D. C., & Dziewonski, A. M. (2014). Earth as a planet: Surface and interior (3rd ed.). Elsevier.

Rodríguez, Ó. (2022). Luminosity distribution of Type II supernova progenitors. Monthly Notices of the Royal Astronomical Society, 515(1), 897–913. https://doi.org/10.1093/mnras/stac1831

Sadiq, S. (2024). Life cycle of high mass star. American Scientific Research Journal for Engineering, Technology, and Sciences, 97(1), 11–29.

Solomon, S. C., & Byrne, P. K. (2019). The exploration of Mercury by spacecraft. Elements, 15(1), 15–20. https://doi.org/10.2138/gselements.15.1.15

Svensmark, H. (2023). A persistent influence of supernovae on biodiversity over the Phanerozoic. Ecology and Evolution, 13(3), 1–9. https://doi.org/10.1002/ece3.9898

Tsuna, D., Kashiyama, K., & Shigeyama, T. (2019). Type IIn supernova light curves powered by forward and reverse shocks. The Astrophysical Journal, 884(1), 87. https://doi.org/10.3847/1538-4357/ab40ba

Yamanaka, M., Fujii, M., & Nagayama, T. (2023). Bright Type II supernova 2023ixf in M101: A quick analysis of the early-stage spectra and near-infrared light curves. Publications of the Astronomical Society of Japan, 75(5), L27–L31. https://doi.org/10.1093/pasj/psad051

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Published

2025-11-04

How to Cite

Gomes, M. J. D., Sitanggang, C. U. S., Gultom, S. M., Situmorang, H., Wulandari, D., & Warty, Y. (2025). Simulasi Dampak Ledakan Supernova terhadap Planet Terdekat. Jurnal Pendidikan, Sains, Geologi, Dan Geofisika (GeoScienceEd Journal), 6(4), 1844–1851. https://doi.org/10.29303/goescienceed.v6i4.1202

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