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Abell 222

Galaxy cluster in the constellation Cetus


Galaxy cluster in the constellation Cetus

FieldValue
nameAbell 222
imageAbell 222 imaged by Legacy Surveys.jpg
captionA portion of Abell 222 imaged by Legacy Surveys
epochJ2000
constellationCetus
ra
dec
brightest_memberLEDA 944643
richness3
bmtypeII-III
velocity_dispersion1,014 km/s
redshift0.2110
distance2.4 Gly
temperature3.77 ± 0.15 keV
mass
other_namesRXC J0137.4-1259

Abell 222 is a galaxy cluster in the constellation of Cetus. It holds thousands of galaxies together. It is located at a distance of 2.4 billion light-years from Earth.

Discovery of dark matter

Astronomers noticed an invisible string of matter was warping spacetime between Abell 222 and Abell 223. Upon further examination by using images from the Japanese Subaru telescope, astronomers discovered that this "invisible matter" is in fact dark matter. The astronomers used gravitational lensing to detect the dark matter filaments. The cluster is connected by a filament of dark matter to Abell 223 that is permeated by hot X-ray emitting gas. Further research shows that this filament only contains about 20 percent of normal matter, the rest is assumed to be dark matter. This is seen to be in good agreement with the cosmological standard model.{{cite news |archive-url = https://web.archive.org/web/20240601224509/https://www.nzz.ch/wissen/wissenschaft/eine-bruecke-aus-dunkler-materie-zwischen-zwei-galaxienhaufen-ld.664256 |archive-date = 2024-06-01 |access-date = 2012-09-24 |url-status = live

Baryonic matter evidence

Main article: Baryon

About 5% of the universe is estimated to be made up of baryonic or ordinary matter which contains protons and neutrons, also known as baryons, and electrons. Baryons and electrons are the foundation for atoms. Astronomers have not been able to locate the full 5% of baryonic matter within other galaxies, stars or gases. After observing gas that connects Abell 222 and Abell 223, scientists believe that a significant part of the missing baryonic matter is within the gas that bridges the two galaxy clusters. This was difficult to locate because the gas had a very low density, which made it hard to detect. This discovery was made possible because of Abell 222's location. It is within Earth's line of sight, so scientists were able to see a strong concentration of this extremely distant gas with the latest high-power infrared and X-ray telescopes, within a section of the sky.

References

References

  1. "ACO 222".
  2. "2MASX J01373406-1259288".
  3. (May 1989). "A catalog of rich clusters of galaxies". Astrophysical Journal Supplement Series.
  4. "NED results for object ABELL 0222". [[National Aeronautics and Space Administration]] / [[Infrared Processing and Analysis Center]].
  5. (2010). "The clusters Abell 222 and Abell 223: A multi-wavelength view". Astronomy and Astrophysics.
  6. Pete Spotts. (5 July 2012). "Cosmic scaffolding uncovered? Scientists find thread of dark matter.". [[Christian Science Publishing Society]].
  7. (2014-08-27). "Dark Matter Filaments Detected in Abell 222 And Abel 223 Supercluster".
  8. "ID: SEMHZOZXUFF: Galaxy clusters Abell 222 and Abell 223". esa.
  9. Dietrich, Jörg. "The Abell 222/223 Supercluster with dark matter Filament". University of Michigan/University Observatory Munich.
  10. (2014-08-27). "Do Abell 222 And Abell 223 Contain The Universe's 'Missing' Baryonic Matter?".
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