Suzaku Finds Common Chemical Composition at Largest Cosmic Scales

  • Released Monday, October 26, 2015

Suzaku mapped iron, magnesium, silicon and sulfur in four directions all across the Virgo Galaxy Cluster for the first time. The northern arm of the survey (top) extends 5 million light-years from M87 (center), the massive galaxy at the cluster's heart. Ratios of these elements are constant throughout the cluster, which means they were mixed well early in cosmic history. The dashed circle shows what astronomers call the virial radius, the boundary where gas clouds are just entering the cluster. Some prominent members of the cluster are labeled as well. The background image is part of the all-sky X-ray survey acquired by the German ROSAT satellite. The blue box at center indicates the area shown in the visible light image.    Credit: A. Simionescu (JAXA) and Hans Boehringer (MPE)

Suzaku mapped iron, magnesium, silicon and sulfur in four directions all across the Virgo Galaxy Cluster for the first time. The northern arm of the survey (top) extends 5 million light-years from M87 (center), the massive galaxy at the cluster's heart. Ratios of these elements are constant throughout the cluster, which means they were mixed well early in cosmic history. The dashed circle shows what astronomers call the virial radius, the boundary where gas clouds are just entering the cluster. Some prominent members of the cluster are labeled as well. The background image is part of the all-sky X-ray survey acquired by the German ROSAT satellite. The blue box at center indicates the area shown in the visible light image.

Credit: A. Simionescu (JAXA) and Hans Boehringer (MPE)

A new survey of hot, X-ray-emitting gas in the Virgo Galaxy Cluster shows that the elements needed to make stars, planets and people were evenly distributed across millions of light-years early in cosmic history, more than 10 billion years ago.

The Virgo Cluster, located about 54 million light-years away, is the nearest galaxy cluster and the second brightest in X-rays. The cluster is home to more than 2,000 galaxies, and the space between them is filled with a diffuse gas so hot it glows in X-rays.

Using Japan's Suzaku X-ray satellite, a team led by Aurora Simionescu, an astrophysicist at the Japan Aerospace Exploration Agency (JAXA) in Sagamihara, acquired observations of the cluster along four arms extending up to 5 million light-years from its center.

Heavier chemical elements from carbon on up are produced and distributed into interstellar space by stars that explode as supernovae at the ends of their lifetimes. This chemical dispersal continues at progressively larger scales through other mechanisms.

Different classes of supernovae produce different chemical compositions. Surveying the distribution of these elements over a vast volume of space, such as a galaxy cluster, helps astronomers reconstruct how, when, and where they were produced. Once the chemical elements made by supernovae are scattered and mixed into interstellar space, they become incorporated into later generations of stars. The overall composition of a large volume of space depends on the mix of supernova types contributing to it.

The survey mapped iron, magnesium, silicon and sulfur all the way across a galaxy cluster for the first time. The elemental ratios are constant throughout the entire volume of the cluster and roughly consistent with the composition of the sun and most of the stars in our own galaxy.

The study shows that the same ratio of supernova types to be responsible for the solar system's makeup was at work throughout the universe. This likely happened when the universe was between 2 and 4 billion years old, a period when stars were being formed at the fastest rate in cosmic history.

This visible light view shows the central part of the Virgo Cluster. The brightest object is the giant elliptical galaxy M87 (left of center). The image spans approximately 1.2 degrees, or about 2.4 times the apparent diameter of a full moon. Credit: NOAO/AURA/NSF

This visible light view shows the central part of the Virgo Cluster. The brightest object is the giant elliptical galaxy M87 (left of center). The image spans approximately 1.2 degrees, or about 2.4 times the apparent diameter of a full moon.

Credit: NOAO/AURA/NSF

Unlabeled image. Suzaku mapped iron, magnesium, silicon and sulfur in four directions all across the Virgo Galaxy Cluster for the first time. The northern arm of the survey (top) extends 5 million light-years from M87 (center), the massive galaxy at the cluster's heart. Ratios of these elements are constant throughout the cluster, which means they were mixed well early in cosmic history. Some prominent members of the cluster are labeled as well. The background image is part of the all-sky X-ray survey acquired by the German ROSAT satellite. Credit: A. Simionescu (JAXA) and Hans Boehringer (MPE)

Unlabeled image. Suzaku mapped iron, magnesium, silicon and sulfur in four directions all across the Virgo Galaxy Cluster for the first time. The northern arm of the survey (top) extends 5 million light-years from M87 (center), the massive galaxy at the cluster's heart. Ratios of these elements are constant throughout the cluster, which means they were mixed well early in cosmic history. Some prominent members of the cluster are labeled as well. The background image is part of the all-sky X-ray survey acquired by the German ROSAT satellite.

Credit: A. Simionescu (JAXA) and Hans Boehringer (MPE)



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This page was originally published on Monday, October 26, 2015.
This page was last updated on Wednesday, May 3, 2023 at 1:49 PM EDT.


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