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Northwestern’s ‘Micro-X’ rocket to image supernova remnant (b roll)

Video

Northwestern’s ‘Micro-X’ rocket to image supernova remnant (b roll)

On Aug. 21, 2022, a NASA-funded Northwestern University team of astrophysicists launched its “Micro-X” rocket from White Sands Missile Range in southern New Mexico. The rocket spent 15 minutes in space — just enough time to snap a quick image of supernova remnant Cassiopeia A, a star in the Cassiopeia constellation that exploded approximately 11,000

Northwestern University

Northwestern’s ‘Micro-X’ rocket to image supernova remnant

Video

Northwestern’s ‘Micro-X’ rocket to image supernova remnant

On Aug. 21, 2022, a NASA-funded Northwestern University team of astrophysicists will launched its “Micro-X” rocket from White Sands Missile Range in southern New Mexico. The rocket spent 15 minutes in space — just enough time to snap a quick image of supernova remnant Cassiopeia A, a star in the Cassiopeia constellation that exploded approximately

Northwestern University

Micro-X rocket

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Micro-X rocket

On Aug. 21, the NASA-funded team launched its “Micro-X” rocket from White Sands Missile Range in southern New Mexico. The rocket spent 15 minutes in space — just enough time to snap a quick image of supernova remnant Cassiopeia A, a star in the Cassiopeia constellation that exploded approximately 11,000 light-years away from Earth. Then,

Northwestern University

Black Hole Accretion Disk

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Black Hole Accretion Disk

The massive black hole in M33 X-7 is hidden in the X-ray bright center of the pancake-like accretion disk of matter. The black-hole’s hot (blue) and massive star companion is losing mass in a wind that gets pulled and captured by the black hole. Learn more. 

NU Viz and CIERA: Matthew McCrory, Francesca Valsecchi, and Vicky Kalogera

GRB181123B

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GRB181123B

The afterglow of GRB181123B, captured by the Gemini North telescope. Learn more: Short gamma ray burst leaves most-distant optical afterglow ever detected

International Gemini Observatory/NOIRLab/NSF/AURA/K. Paterson & W. Fong (Northwestern University).

Black Hole Accretion Disc

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Black Hole Accretion Disc

A detailed simulation of a black hole’s accretion disc created by a global team of computational astrophysicists – including CIERA’s Prof. Sasha Tchekhovskoy – solved a decades-old mystery. The accretion disc is matter that orbits and then falls into a black hole. Researchers discovered how the disc aligns with the hole’s equator, details vital to

AT2018cow

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AT2018cow

An image of AT2018cow and its host galaxy obtained on August 17, 2018 using W. M. Keck Observatory’s instrument, the DEep Imaging and Multi-Object Spectrograph (DEIMOS). Learn more: Birth of a Black Hole or Neutron Star Captured for First Time

R. MARGUTTI/W. M. KECK OBSERVATORY

CIERA’s 10th Annual Public Lecture, “The NU Astronomy of Stars, Black Holes, and Cosmic Explosions”

Event

CIERA’s 10th Annual Public Lecture, “The NU Astronomy of Stars, Black Holes, and Cosmic Explosions”

CIERA’s 10th annual public lecture was presented October 11, 2018 by director Vicky Kalogera. Kalogera’s talk–a glimpse into the years of fascinating work conducted by CIERA–highlighted key discoveries and what they mean for the future of astronomy. Kalogera discussed the lives of stars, how their influence on the Cosmos has changed in the recent decade,

CIERA / Northwestern

  • Event,
  • Interdisciplinary

How Do You Detect a Black Hole? LIGO and the Measurement of Gravitational Waves

Interview / Event

How Do You Detect a Black Hole? LIGO and the Measurement of Gravitational Waves

Black holes may hold the key to understanding the most fundamental truths of the universe, but how do you see something that’s, well, black? Astronomers think they have the answer. Thanks to a global array of radio telescopes that turn the Earth into a giant receiver, we may soon have the first picture of the

World Science Festival

How many merger binary black holes are there?

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How many merger binary black holes are there?

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)

Revealing the Lives of Stars Through the Cataclysmic Collisions of Black Holes

Event

Revealing the Lives of Stars Through the Cataclysmic Collisions of Black Holes

Northwestern Physics and Astronomy student Mike Zevin presents a talk as part of the Northwestern Ready Set Go (RSG) program. The goals of the program are to increase awareness for the urgent need for excellent research communicators and to coach graduate and post doctoral researchers to improve their own presentation skills. The program focuses on three important

Northwestern's RSG Program

Listening for Colliding Black Holes

Interview

Listening for Colliding Black Holes

Northwestern Physics and Astronomy student Michael Katz presents a talk as part of the Northwestern Ready Set Go (RSG) program. The goals of the program are to increase awareness for the urgent need for excellent research communicators and to coach graduate and post doctoral researchers to improve their own presentation skills. The program focuses on three important

Northwestern's RSG Program