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Coloquios IAFE 2025 | Miércoles 25 de junio Dr. Xianming Han (*) Department of Physics and Astronomy, Butler University, Indianapolis, EEUU Resumen: Most stars are actually in pairs or triplets. Observing binary stars helps develop stellar evolution theories. If their orbital plane of a binary star system is more or less parallel to the line of sight, one star will block the other as they orbit around each other. This is known as eclipsing binary. In this talk, we will discuss observations of eclipsing binary star systems and what information we can extract from their lightcurves. We will also discuss observations of Jovian satellites and asteroids using our SARA (Southeastern Association for Research in Astronomy) and Holcomb telescopes. (*) Acerca del Dr. Xianming Han: Education: 1978-1982, Department of Physics, University of Science and Technology of China, undergraduate student. 1982: BS in Physics 1982-1983, Anhui Institute of Optics and Fine Mechanics, graduate student. 1983-1989, Department of Physics, University of Colorado, Boulder, Colorado, USA, graduate student. 1986: MS in Physics 1989: Ph.D in Physics Work experience: 1989-1991: Department of Physics, University of Idaho, Moscow, Idaho, USA, visiting assistant professor. 1991-present: assistant professor, associate professor, and professor, Department of Physics and Astronomy, Butler University, Indianapolis, Indiana, USA. Astronomer affiliated with the Southeastern Association for Research in Astronomy (SARA). From 2008 to 2017, served as the department chair. Hobbies: Travel, photography, and languages