Development and Classroom Trial of Suzaku X-ray Data Materials for Measuring the Age of the Universe
Teaching Methods and Tools
IAU OAE Conference 2026
Tuesday Nov. 17, 2026
UTC: 8 p.m. - 9:30 p.m. America/New_York: 3 p.m.- 4:30 p.m.
Wednesday Nov. 18, 2026
UTC: 2 p.m. - 3:30 p.m. America/New_York: 9 a.m.- 10:30 a.m.
Thursday Nov. 19, 2026
UTC: 9:30 a.m. - 11 a.m. America/New_York: 4:30 a.m.- 6 a.m.
Friday Nov. 20, 2026
UTC: 1 p.m. - 2:30 p.m. America/New_York: 8 a.m.- 9:30 a.m.
Hideki Uchiyama
(Shizuoka University)
Coauthors: Shimano Masahiro (Rikkyo Niiza High School) , Ueda Kento (Shizuoka University) , Takeo Mochizuki (Shizuoka University)
We developed educational materials using Suzaku X-ray satellite data to verify the Hubble–Lemaître law and determine the Hubble time (the approximate age of the universe). Suzaku data are easily analyzed via UDON2, a web-based tool by ISAS/JAXA C-SODA. We selected 14 galaxy clusters and galaxies with distances known via non-redshift methods that exhibit strong highly ionized iron lines. Measuring central line energy from X-ray spectra using UDON2, we calculated recession velocity via the Doppler formula, yielding a Hubble time of ~13 billion years. These materials enable high school students to learn the Doppler effect, electromagnetic waves, photons, and atomic spectra. We report their practical application in a physics class focused on "The Beginning of the Universe."
Biography:
Hideki Uchiyama is an X-ray astronomer who graduated from Kyoto University with a B.S. in 2005, an M.S. in 2007, and a Ph.D. in 2010. He participated in the Suzaku (ASTRO-E2) and Hitomi (ASTRO-H) missions and is currently working on the XRISM mission. His main research interest is the Milky Way Galaxy, especially the high-energy activity in its central region. He teaches at the Faculty of Education, Shizuoka University, and has recently been involved in science education using (small) satellites.
