Wright Center for Science EducationTufts University                                                         Chandra workshop 2003 Logo

vertical line
• Schedule

Chandra and the X-Ray Universe

Black hole stormThe Chandra X-ray Observatory, part of NASA's Structure and Evolution of the Universe Forum, is the most sophisticated X-ray observatory launched by NASA. Chandra is designed to observe X-rays from high-energy regions of the universe, such as the remnants of supernovae explosions, colliding galaxies, black holes, pulsars, quasars, and X-ray binary stars. The spectacular results from the Chandra observational data are changing and reshaping our theories about the evolution of stars and galaxies. Each exciting new image shows glimpses of such exotic phenomena as surprising black hole activity in old galaxies, rivers of gravity that define the cosmic landscape, unexpected x-ray activity in proto-stars and failed stars, puzzling distributions of elements in supernovae remnants, and the even the tantalizing possibility of an entirely new form of matter - the strange quark star. The technology onboard the Chandra Observatory allows scientists to view, study, and examine the invisible x-ray universe from a 64-hour orbit that reaches one third of the distance to the moon. This unprecedented accomplishment has allowed Chandra to see the universe as it formed, watch doomed matter falling into a black hole get a new lease on life, and discover connections between supernovae and gamma-ray bursts.

The Chandra X-ray Observatory is changing our knowledge of the evolution of the universe, and producing educational materials to integrate this knowledge into the classroom. This workshop is dedicated to presenting the Chandra mission and the Chandra educational materials. These materials, aligned to National Science Standards and Benchmarks, will allow the participants to integrate the latest results from the Chandra X-ray Observatory into existing curricular, and use the image analysis software that will allow their students to research and investigate x-ray phenomena. Participants will increase their knowledge of high-energy astronomy, and learn to use the software imaging analysis tools to investigate x-ray phenomena, and learn how to access all resources available to incorporate x-ray astronomy into the classroom.