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A team of researchers from the University of Zaragoza, King's College London and the Institute of Astronomy in the UK, led by Ciaran O'Hare, found a collection of stars that were all moving in the same direction. They called this the S1 stream, and these stars are believed to be the remnants of a dwarf galaxy that was swallowed by the Milky Way, billions of years ago.

The S1 stream is a set of 30,000 stars, and it was identified last year by ESA’s Gaia satellite in an ongoing billion-star survey. In fact, about 30 such streams have been found in our galaxy, each the remnant of a previous collision. These streams are the debris of a small galaxy that crashed into the Milky Way.

Tracing the Dark Matter “Hurricane”

In their paper published in the journal, Physical Review D, the group described their findings and why these observations may offer help in understanding the dark matter better.

The matter that presented in the S1 stream was particularly interesting, and also, it is currently “blowing” past us at about 500 km/s, according to the study’s authors. Scientists believe that this may generate remarkable effects on the dark matter that exists near us, giving us a much better chance for its detection.

As per a statement from APS Physics, “Current detectors looking for weakly interacting massive particles (WIMPs) – one widely discussed form of dark matter – probably won’t see any effect from S1, but future WIMP detectors might.”

Weakly-Interacting Massive Particles (WIMPs), Gravitationally-Interacting Massive Particles (GIMPs) and axions (hypothetical elementary particles posited by physicists) could be the place from where dark matter comes.

It might be probable to detect axions from the stream, which are ultralight particles that we cannot see, 500 million times lighter than an electron and could compose dark matter. They could also be converted to visible photons in the presence of a very strong magnetic field.

It is believed that all galaxies are formed inside a large aura of dark matter, which we cannot see and does not interact with the external environment of normal matter.

The researchers of this study said that about 10 million solar masses of dark matter came from the original dwarf galaxy and was traveling along the S1 stream.

A simulation of collision of a smaller galaxy with that of the Milky Way. (Source: Koppelman, V. et al, Kapteyn Astronomical Institute, University of Groningen, The Netherlands)

Project leader, O'Hare mentioned, “What we want to do is add the stream as part of our kind of the main prediction for the types of signal that should show up in a dark matter experiment. As the S1 stream ‘hits the Solar System slap in the face,' its counter-rotating structure will dramatically increase the amount of dark matter appearing to come from the same patch of sky as the standard dark matter wind. Indeed, it should produce a tell-tale ‘ring’-like structure around this wind, something that directional dark matter detectors… could easily detect in future.”

This dark matter "hurricane" may be moving at high speeds, which might provide experts with the opportunity to observe dark matter for the first time, at such a close distance.

The chances are better for axion detectors as the energy spectrum from axionic dark matter typically exhibits a broad strike with an additional narrow peak if the S1 hurricane is truly buffeting our shores.

“There are things known and there are things unknown, and in between are the doors of perception.” - Aldous Huxley

Top Image: Astronomers and scientists observe a dark matter “hurricane” that is passing very close to the Earth. (Image Source: Smithsonian Institution/Flickr)


1. Marc Ward, 2018. Earth Is Passing Through A Dark Matter "Hurricane" Right Now [Online] Available at:

2. Michael Schirber, 2018. Synopsis: Dark Matter Blowing Like a Hurricane

[Online] Available at:

3. Jackson Ryan, 2018.

4. Chelsea Gohd, 2018. A ‘dark matter hurricane’ is storming past Earth [Online] Available at:

5. Bob Yirka, 2018. Dark matter 'hurricane' offers chance to detect axions [Online] Available at:

Nikos Dimitris Fakotakis's picture

Nikos Dimitris Fakotakis

Fakotakis Nikos Dimitris received his BSc-MEng in Computer and Information Engineering from the Polytechnic School of Patras, Greece, in 2015. He is currently a PhD student in the Wireless Communication Laboratory of the same department. His research interests are in the field of Artificial Intelligence and Human Computer Interaction. In parallel with his studies he has been working as computer and network engineer, database administrator, and software developer (Java, python, etc.).Read More

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