CWRU Astronomy is a community of active researchers and educators, with research strengths in the fields of galaxy formation and evolution, stellar chemical abundances, and telescope instrumentation and design.
We offer graduate and undergraduate degree programs, and host a series of public talks for the general public. Come inside and learn more about our on-going research, our faculty, staff, and students, and all the new things happening in CWRU Astronomy.
You can also read the latest edition of our annual CWRU Astronomy newsletter.
Date posted: December 8th, 2016
This fall marks the full public release of CWRU Astronomy’s Burrell Schmidt Deep Virgo Survey. Over the course of seven observing seasons from 2004 through 2011, CWRU astronomer Chris Mihos and collaborators used the Burrell Schmidt telescope to conduct deep wide-field imaging of the nearby Virgo Cluster of galaxies. …Read more.
Date posted: November 1st, 2016
Every year CWRU Astronomy holds a Halloween pumpkin carving event for faculty, staff, and students. This year added an extra treat — a campus-wide power outage in the middle of the carving! …Read more.
Date posted: September 22nd, 2016
A new radial acceleration relation found among spiral and irregular galaxies challenges current understanding – and possibly existence – of dark matter.
In the late 1970s, astronomers Vera Rubin and Albert Bosma independently found that spiral galaxies rotate at a nearly constant speed: the velocity of stars and gas inside a galaxy does not decrease with radius, as one would expect from Newton’s laws and the distribution of visible matter, but remains approximately constant. …Read more.
Date posted: September 8th, 2016
With the new fall semester kicking off, we’ve just published the latest CWRU Astronomy newsletter. It features a Hubble Space Telescope study of the nearby spiral galaxy M101 by Chris Mihos and collaborators, a variety of new research databases created by CWRU astronomers, a feature of our historic 9.5″ Warner and Swasey refractor, and more. …Read more.