The University of Texas Rio Grande Valley is basking in the glow of another major advance in the science of detecting ancient cosmic cataclysms.
On Monday, coinciding with a formal announcement in Washington, UTRGV physics faculty, students and researchers gathered on the Brownsville campus for a news conference to discuss an Aug. 17 detection of gravitational waves created 130 million years ago by the collision of two rapidly spinning neutron stars. LIGO, the Laser Interferometer Gravitational Wave Observatory, made up of two separate facilities in Louisiana and Washington state, detected the waves, backed up by the Europe-based detector Virgo.
What’s different this time is that the wave detection was matched by visual confirmation of the primeval collision. Electromagnetic telescopes around the world and in space were able to detect the supernova burst of light given off by the colliding stars. Scientists are calling it the dawn of “multi-messenger astronomy.”
Gravitational waves, which Einstein theorized a century ago, were observed for the first time on Sept. 14, 2015. UTRGV’s Center for Gravitational Wave Astronomy, formed in 2003, is one of more than a 1,000 international members of the LIGO Scientific Collaboration. The first detection of gravitational waves — in that case caused by the collision of two black holes 1.3 billion years ago — was made possible by an algorithm developed by UTRGV physics faculty, working in collaboration with scientists at the University of Florida.
The CGWA also had a hand in the optical aspect of the Aug. 17 detection, via its Transient Optical Robotic Observatory of the South, a collaboration of scientists at UTRGV, Texas A&M and the National University of Cordoba (Argentina). The observatory, which is located in Argentina, serves as a “follow-up” instrument for LIGO and Virgo, searching for visual confirmation in deep space when gravitational waves are detected. TOROS was among the observatories that automatically sprung into action on Aug. 17.