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LIGO – Virgo discovery marks first cosmic event observed in both gravitational waves and light. Announcement made at the National Press Club, Washington, DC. Panel with representatives from various telescopes, begins at 51:21 (Please note that Marica Branchesi’s institutional affiliation is incorrectly indicated in the video. The correct affiliation for Dr. Branchesi is Gran Sasso

This simulation shows a binary-binary encounter involving four black holes, which can occur at the cores of dense stellar systems such as gloublar clusters. Such encounters can lead to long-lived “resonating” interactions, through which many temporary binary systems are created. By incorporating a more accurate description of Einstein’s gravity in the equations of motion, the formation

Astronomers using ALMA studied a cataclysmic stellar explosion known as a gamma-ray burst, or GRB, and found its enduring “afterglow.” The rebound, or reverse shock, triggered by the GRB’s powerful jets slamming into surrounding debris, lasted thousands of times longer than expected. These observations provide fresh insights into the physics of GRBs, one of the

CIERA Associate Director and Northwestern LIGO group member Shane Larson says that inspiration and collaboration, two huge parts of scientific discoveries, can help us solve society’s problems.

An international research collaboration, including four Northwestern University astronomers, is the first to detect the spectacular collision of two neutron stars in a nearby galaxy using both gravitational waves and light.

CIERA Director and Northwestern LIGO group lead Vicky Kalogera talks about the different types of waves astronomers have used throughout history to study the Universe. Now, we are in the age of “multi-messenger” astronomy. This means that different types of waves from the same cosmic event can be studied.

CIERA Director Vicky Kalogera and Associate Director Shane Larson talk about the history of gamma ray bursts, and the theory that short gamma ray bursts are caused by collisions of neutron starts. Now, that puzzle is solved!

Northwestern University astronomers talk about gravitational waves — what they are, how to understand them, and why they are important to studying the Universe.

CIERA Associate Director and Northwestern LIGO group member Shane Larson describes how different the 2017 Neutron Star Merger (GW170817) signal is from previous signals.

CIERA Associate Director and Northwestern LIGO group member Shane Larson describes how the masses of objects in our Universe is very important to astronomers’ understanding of events like GW170817.

CIERA Director and Northwestern LIGO group lead Vicky Kalogera talks about how basic science is discovered and used in society.

Following the October 16, 2017 announcement of the first-ever observation of a binary neutron star inspiral and merger, Northwestern’s astronomy research center, CIERA, held a discussion with the Northwestern scientists behind the discovery. View the lecture by Shane Larson to understand the science behind this amazing astronomical event!

Following the October 16, 2017 announcement of the first-ever observation of a binary neutron star inspiral and merger, Northwestern’s astronomy research center, CIERA, held a discussion with the Northwestern scientists behind the discovery. View the recording of this event in full, and join Professors Vicky Kalogera, Shane Larson, Raffaella Margutti and Wen-fai Fong as they

Following the October 16, 2017 announcement of the first-ever observation of a binary neutron star inspiral and merger, Northwestern’s astronomy research center, CIERA, held a discussion with the Northwestern scientists behind the discovery. View the panel discussion with Professors Vicky Kalogera, Raffaella Margutti, and Wen-fai Fong. Panel moderated by Adler Planetarium President & CEO, Michelle

After the spectacular collision of two neutron stars, which produced gravitational waves that were detected here on Earth, astronomers at Northwestern University describe how telescopes around the world looked for light.