CIERA Associate Director and Northwestern LIGO group member Shane Larson describes how different the 2017 Neutron Star Merger (GW170817) signal is from previous signals.
LIGO-Virgo / Northwestern
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.
LIGO-Virgo / Northwestern
CIERA Director and Northwestern LIGO group lead Vicky Kalogera talks about how basic science is discovered and used in society.
LIGO-Virgo / Northwestern
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!
CIERA / Northwestern
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
CIERA / Northwestern
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
CIERA / Northwestern
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.
LIGO-Virgo / Northwestern
Supported Browsers: Windows: Google Chrome Mac: Google Chrome or Safari
Visualization: LIGO -Virgo / Frank Elavsky, Aaron Geller / Northwestern
This video illustrates the collision of two neutron stars (GW170817).
LIGO-Virgo / Northwestern
This interactive allows you to investigate possible past lives of the two neutron stars that merged in an event called GW170817 in the galaxy NGC 4993. The pair of stars—a neutron star and a normal star—orbit quietly, until the normal star undergoes a supernova, spawning a second neutron star and “kicking” the system into an elliptical orbit.
LIGO-Virgo / Aaron Geller / Northwestern
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.
LIGO-Virgo / Northwestern
What is a neutron star? What is it like when two neutron stars collide? Northwestern University astronomers describe the GW170817 merger of these massive objects in our Universe.
LIGO-Virgo / Northwestern
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 audience question & answer period from this event.
CIERA / Northwestern
A neutron star compared with the skyline of Chicago. Neutron stars are about 12 miles in diameter and are extremely dense.
Nick Gertonson / Daniel Schwen / Northwestern / LIGO-Virgo
How many merger binary black holes are there? There are lots of uncertainties in our understanding of stellar evolution. This plot shows one prediction from the COMPAS population synthesis code for the number of gravitational-wave detections: there would be about 500 detections per year of observing time once our detectors reach design sensitivity! In Barrett, Gaebel,
Barrett, Gaebel, Neijssel, Vigna-Gómez, Stevenson, Berry, Farr, & Mandel (2018)
This image shows the most probable source galaxies for a simulated gravitational-wave signal from a binary neutron star system. Accurately identifying the source of gravitational waves is extremely important for directing follow-up observations with telescopes, and for measuring the expansion of the Universe. In Del Pozzo, Berry, Ghosh, Haines, Singer & Vecchio (2018; http://adsabs.harvard.edu/abs/2018MNRAS.479..601D) we applied
Del Pozzo, Berry, Ghosh, Haines, Singer & Vecchio (2018)
APERTURE: A Precise Extremely large Reflective Telescope Using Reconfigurable Elements. This is the deployment concept which was produced during the NIAC Phase I feasibility study. APERTURE is a UV-Visible telescope with a 16-m diameter primary mirror. The primary is a flexible membrane coated with magnetic smart material. The shape of the reflector can be corrected
Mel Ulmer / CIERA Northwestern
