A University of Toronto astronomer’s research suggests the solar system is surrounded by a magnetic tunnel that can be seen in radio waves.
Jennifer West, a research associate at the Dunlap Institute for Astronomy & Astrophysics, is making a scientific case that two bright structures seen on opposite sides of the sky – previously considered to be separate – are actually connected and are made of rope-like filaments. The connection forms what looks like a tunnel around our solar system.
The data results of West’s research have been published in the Astrophysical Journal.
“If we were to look up in the sky,” says West, “we would see this tunnel-like structure in just about every direction we looked – that is, if we had eyes that could see radio light.”
Called “the North Polar Spur” and “the Fan Region,” astronomers have known about these two structures for decades, West says. But most scientific explanations have focused on them individually. West and her colleagues, by contrast, believe they are the first astronomers to connect them as a unit.
Left: A curving tunnel, with lines formed by the tunnel lights and road lane markers, forms a similar geometry to the proposed model of the North Polar Spur and Fan Region. Credit: photo by Pixabay/ illustration by Jennifer West. Right: The sky as it would appear in radio polarized waves. Credit: image by Dominion Radio Astrophysical Observatory/Villa Elisa telescope/ESA/Planck Collaboration/Stellarium/Jennifer West
Made up of charged particles and a magnetic field, the structures are shaped like long ropes, and are located about 350 light-years away from us – and are about 1,000 light-years long.
“That’s the equivalent distance of traveling between Toronto and Vancouver two trillion times,” West says.
West has been thinking about these features on and off for 15 years – ever since she first saw a map of the radio sky. More recently, she built a computer model that calculated what the radio sky would look like from Earth as she varied the shape and location of the long ropes. The model allowed West to “build” the structure around us, and showed her what the sky would look like through our telescopes. It was this new perspective that helped her to match the model to the data.
Illustrated map of Milky Way Galaxy shown with the position and size of proposed filaments. Inset shows a more detailed view of the Local environments, and the position of Local Bubble and various nearby dust clouds. Credit: Image by NASA/JPL-Caltech/R. Hurt/SSC/Caltech with annotations by Jennifer West
“A few years ago, one of our co-authors, Tom Landecker, told me about a paper from 1965 – from the early days of radio astronomy,” West says. “Based on the crude data available at this time, the authors [Mathewson and Milne], speculated that these polarized radio signals could arise from our view of the Local Arm of the galaxy, from inside it.
“That paper inspired me to develop this idea and tie my model to the vastly better data that our telescopes give us today.”
West uses the Earth’s map as an example. The North pole is on the top and the equator is through the middle – unless you re-draw the map from a different perspective. The same is true for the map of our galaxy. “Most astronomers look at a map with the North pole of the galaxy up and the galactic center in the middle,” West explains. “An important part that inspired this idea was to remake that map with a different point in the middle.”