Maunakea Observatories Response to Coronavirus Pandemic

maunakea_logomaunakea_logomaunakea_logomaunakea_logo
  • MKO@Home
  • About
  • Community
  • Stewardship
  • Science
  • Culture
  • Our News
  • Careers
  • Contact

Observing Clusters of Galaxies Collide

  • Home
  • News Placeholder
  • General
  • Observing Clusters of Galaxies Collide
Galaxies in the Infant Universe were Surprisingly Mature
November 2, 2020
Two Maunakea Telescopes Confirm First Brown Dwarf Discovered by Radio Observations
November 18, 2020
November 17, 2020
Categories
  • General
Tags
  • Subaru Telescope

Composite image showing HSC J023336-053022 (XLSSC 105), a pair of colliding galaxy clusters located 4 billion light-years away in the constellation Cetus. The background image was taken by the Subaru Telescope. Overlaid colors show the distributions of dark matter (blue), hot gas observed in X-rays (green), and high-pressure gas observed by radio (red). This cluster contains two concentrations of galaxies, which overlap with the distribution of the dark matter. (Credit: GBT/NSF/NAOJ/HSC-SSP/ESA/XMM-Newton/XXL survey consortium)

Using a trio of world-leading observatories, including the Subaru Telescope on Maunakea, astronomers have observed clusters of galaxies colliding in the distant Universe. The Subaru telescope can observe the visible light from stars, but these galaxies also have other important components, including dark matter and hot gas, which can’t be seen with visible light. So the astronomers combined visible, radio, and X-ray light to create a complete picture of the collision. In doing so, they discovered that the large amounts of energy released during this collision heats the gas to 400 million degrees centigrade (720 million degrees Fahrenheit), which is nearly 30 times hotter than the core of our Sun. These types of observations are important for understanding the evolution of our Universe.

Read more, in the Subaru Telescope  press release.

Share
6
xzhang
xzhang

Related posts

Artist view of the very young eruptive red dwarf AU Mic (left) and its newly discovered close-in planet (right) with the debris disc from which the planet was born in the background. Image credits: NASA-JPL/Caltech

February 10, 2021

CFHT Stares at a Young Rebel: the AU Mic Planetary System


Read more

An artist’s impression of quasar J0313-1806 showing the supermassive black hole and the extremely high velocity wind. The quasar, seen just 670 million years after the Big Bang, is 1000 times more luminous than the Milky Way, and is powered by the earliest known supermassive black hole, which weighs in at more than 1.6 billion times the mass of the Sun. Credit: NOIRLab/NSF/AURA/J. da Silva

February 10, 2021

The Earliest Supermassive Black Hole and Quasar in the Universe


Read more
Animation of the asteroid 1998 KY26

The asteroid 1998 KY26 (the point of light located at where the two lines would cross) captured by Hyper Suprime-Cam mounted on the Subaru Telescope. The blurring of the background stars is due to the motion of the telescope tracking the asteroid. Five shots, each with a 2-minute exposure time, taken during 2:04–2:16 on December 10, 2020 (Hawaiʻi Standard Time) were stacked to create this image. The field of view is 30 x 15 arcseconds. (Credit: NAOJ)

January 12, 2021

Subaru Telescope Charts a Course to a Close-passing Asteroid


Read more

Comments are closed.

Search Our Blog

Recent Posts

  • CFHT Stares at a Young Rebel: the AU Mic Planetary System
    February 10, 2021
  • The Earliest Supermassive Black Hole and Quasar in the Universe
    February 10, 2021
  • Animation of the asteroid 1998 KY26
    Subaru Telescope Charts a Course to a Close-passing Asteroid
    January 12, 2021
  • New Instrument on Maunakea Telescope Nets its First Discovery
    December 18, 2020
  • Blast from the Past!
    December 8, 2020
© 2020 Maunakea Observatories. All Rights Reserved. See Photo Credits