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Evidence for dark matter in the inner Milky Way

Date:
February 9, 2015
Source:
Stockholm University
Summary:
A new study is providing evidence for the presence of dark matter in the innermost part of the Milky Way, including in our own cosmic neighborhood and the Earth's location. The study demonstrates that large amounts of dark matter exist around us, and also between us and the Galactic center. The result constitutes a fundamental step forward in the quest for the nature of dark matter.
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A new study is providing evidence for the presence of dark matter in the innermost part of the Milky Way, including in our own cosmic neighbourhood and the Earth’s location. The study demonstrates that large amounts of dark matter exist around us, and also between us and the Galactic centre. The result constitutes a fundamental step forward in the quest for the nature of dark matter.

The existence of dark matter in the outer parts of the Milky Way is well established. But historically it has proven very difficult to establish the presence of dark matter in the innermost regions, where the Solar System is located. This is due to the difficulty of measuring the rotation of gas and stars with the needed precision from our own position in the Milky Way.

“In our new study, we obtained for the first time a direct observational proof of the presence of dark matter in the innermost part of the Milky Way. We have created the most complete compilation so far of published measurements of the motion of gas and stars in the Milky Way, and compared the measured rotation speed with that expected under the assumption that only luminous matter exists in the Galaxy. The observed rotation cannot be explained unless large amounts of dark matter exist around us, and between us and the Galactic centre”, says Miguel Pato at the Department of Physics, Stockholm University.

Dark matter is about five times more abundant than the matter that we are familiar with, made of atoms. Its existence in galaxies was robustly established in the 1970s with a variety of techniques, including the measurement of the rotation speed of gas and stars, which provides a way to effectively “weigh” the host galaxy and determine its total mass.

 “Our method will allow for upcoming astronomical observations to measure the distribution of dark matter in our Galaxy with unprecedented precision. This will permit to refine our understanding of the structure and evolution of our Galaxy, and it will trigger more robust predictions for the many experiments worldwide that search for dark matter particles. The study therefore constitutes a fundamental step forward in the quest for the nature of dark matter”, says Miguel Pato.


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Materials provided by Stockholm University. Note: Content may be edited for style and length.


Journal Reference:

  1. Miguel Pato, Fabio Iocco, Gianfranco Bertone. Evidence for dark matter in the inner MilkyWay. Nature, 2015 DOI: 10.1038/nphys3237

Cite This Page:

Stockholm University. "Evidence for dark matter in the inner Milky Way." ScienceDaily. ScienceDaily, 9 February 2015. <www.sciencedaily.com/releases/2015/02/150209113046.htm>.
Stockholm University. (2015, February 9). Evidence for dark matter in the inner Milky Way. ScienceDaily. Retrieved March 18, 2024 from www.sciencedaily.com/releases/2015/02/150209113046.htm
Stockholm University. "Evidence for dark matter in the inner Milky Way." ScienceDaily. www.sciencedaily.com/releases/2015/02/150209113046.htm (accessed March 18, 2024).

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