Astronomers have described the first radiation belt observed outside our solar system, using a coordinated array of 39 radio dishes from Hawaii to Germany to obtain high-resolution images. Images of continuous, intense radio emissions from a supercooled dwarf reveal a cloud of high-energy electrons trapped in the object’s strong magnetic field, forming a double-lobe structure similar to radio images of Jupiter’s radiation belts.
“We’re actually imaging our target’s magnetosphere by observing radio-emitting plasma — it’s radiation Belt – in the magnetosphere. This has never happened before for something the size of a gas giant outside our solar system, said Melody Cao, a postdoctoral fellow at the University of California, Santa Cruz and first author of a paper on the new findings published May 15. nature.
form strong magnetic fieldsmagnetic bubble“About a planet called the magnetosphere, which can trap particles and accelerate them close to the speed of light. All the planets in our solar system that have such magnetic fields, including Earth, as well as Jupiter and the other Giant planetsOwns radiation belts It consists of these charged, high-energy particles that are trapped by the planet’s magnetic field.
Earth’s radiation belts, known as the Van Allen belts, are large donut-shaped regions of high-energy particles captured from the solar wind by the magnetic field. Most of the particles in Jupiter’s belts are from volcanoes on its moon Io. If you could put them side by side, the radiation belt imaged by Kao and her team would be 10 million times brighter than Jupiter’s belt.
Particles deflected by the magnetic field toward the poles generate auroras (“northern lights”) when they interact with the atmosphere, and Kao’s team also obtained the first image able to distinguish between the location of an object’s aurora and radiation belts outside of our own. Solar System.
The supercooled dwarf imaged in this study straddles the boundary between them Low mass stars and huge brown dwarfs. “While the composition of stars and planets can be different, the physics inside them can be very similar in that mushy part of the collective chain that connects low-mass stars to brown dwarfs and gas giant planets,” Kao explained.
Characterizing the strength and shape of magnetic fields for this class of objects, she said, is largely uncharted terrain. Using their theoretical understanding of these systems and numerical models, planetary scientists could predict the strength and shape of a planet’s magnetic field, but they had no good way to easily test these predictions.
“Aurora borealis can be used to measure magnetic field strength, but not shape. We designed this experiment to demonstrate a method for assessing the shapes of magnetic fields on brown dwarfs and, eventually, exoplanets,” Kao said.
The strength and shape of the magnetic field can be an important factor in determining a planet’s habitability. “When we think about the habitability of exoplanets, the role of magnetic fields in maintaining a stable environment is something to consider in addition to things like the atmosphere and climate,” Cao said.
To generate a magnetic field, the interior of the planet must be hot enough to have electrically conductive fluids, which in Earth’s case is the molten iron in its core. On Jupiter, the conducting liquid is hydrogen under so much pressure that it becomes metallic. Metallic hydrogen may also generate magnetic fields in brown dwarfs, Kao said, while in the interiors of stars the conductive fluid is ionized hydrogen.
Known as LSR J1835+3259, the supercold dwarf was the only object that Kao felt confident would yield the high-quality data needed to resolve its radiation belts.
“Now that we have established that this particular type of steady-state, low-level radio emission traces the radiation belts into the large-scale magnetic fields of these objects, when we see this type of emission from brown dwarfs – and eventually from gas giant exoplanets – we can say with more confidence that That they have a big planet magnetic fieldEven if our telescope is not big enough to see what it looks like,” Kao said, adding that she is looking forward to the time when the next generation of the Very Large Array, currently being planned by the National Astronomical Observatory (NRAO), can image many extrasolar radiation belts.
“This is a critical first step in finding many more of these objects and honing our skills to search for smaller and smaller magnetospheres, eventually enabling us to study those potentially habitable, Earth-sized planets,” said co-author Evgenya Shkolnik of Arizona. University that has been studying magnetic fields and habitability of planets for many years.
The team used the 39-component High Sensitivity Array radio dishes Coordinated by NRAO in the US and the Effelsberg radio telescope operated by the Max Planck Institute for Radio Astronomy in Germany.
“By bringing together radio dishes from all over the world, we can create incredible high-definition pictures To see things no one has seen before. Our image is comparable to reading the top row of an eye chart in California while standing in Washington, D.C.”
The discovery was a true team effort, Kao emphasized, drawing heavily on the observational expertise of co-first author Amy Miodoshevsky at NRAO in study planning and data analysis, as well as on the multi-wavelength stellar flare expertise of Veladsen and Shkolnik.
Melody Cow, Resolved imaging of an exoplanet radiation belt around a supercooled dwarf, nature (2023). doi: 10.1038/s41586-023-06138-w. www.nature.com/articles/s41586-023-06138-w
University of California – Santa Cruz
the quote: astronomers observe first radiation belt seen outside our solar system (2023, May 15) Retrieved May 15, 2023 from https://phys.org/news/2023-05-astronomers-belt-solar.html
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