Astronomers observe the first radiation belt seen outside of our solar
system
High-resolution imaging of radio emissions from an ultracool dwarf show a double-lobed structure like the radiation belts of Jupiter

Date:
May 15, 2023
Source:
University of California - Santa Cruz
Summary:
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. The images
of persistent, intense radio emissions from an ultracool dwarf
reveal the presence of a cloud of high-energy electrons trapped
in the object's powerful magnetic field, forming a double-lobed
structure analogous to radio images of Jupiter's radiation belts.


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==========================================================================
FULL STORY ========================================================================== 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. The images of persistent,
intense radio emissions from an ultracool dwarf reveal the presence of a
cloud of high-energy electrons trapped in the object's powerful magnetic
field, forming a double- lobed structure analogous to radio images of
Jupiter's radiation belts.

"We are actually imaging the magnetosphere of our target by observing the radio-emitting plasma -- its radiation belt -- in the magnetosphere. That
has never been done before for something the size of a gas giant planet
outside of our solar system," said Melodie Kao, a postdoctoral fellow at
UC Santa Cruz and first author of a paper on the new findings published
May 15in Nature.

Strong magnetic fields form a "magnetic bubble" around a planet called a magnetosphere, which can trap and accelerate particles to near 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 planets,
have radiation belts consisting of these high-energy charged particles
trapped by the planet's magnetic field.

Earth's radiation belts, known as the Van Allen belts, are large
donut-shaped zones of high-energy particles captured from solar winds
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 that Kao and
her team have imaged would be 10 million times brighter than Jupiter's.

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 capable of differentiating
between the location of an object's aurora and its radiation belts
outside our solar system.

The ultracool dwarf imaged in this study straddles the boundary between
low- mass stars and massive brown dwarfs. "While the formation of stars
and planets can be different, the physics inside of them can be very
similar in that mushy part of the mass continuum connecting low-mass
stars to brown dwarfs and gas giant planets," Kao explained.

Characterizing the strength and shape of the magnetic fields of this class
of objects is largely uncharted terrain, she said. Using their theoretical understanding of these systems and numerical models, planetary scientists
can predict the strength and shape of a planet's magnetic field, but
they haven't had a good way to easily test those predictions.

"Auroras can be used to measure the strength of the magnetic field,
but not the shape. We designed this experiment to showcase 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're thinking about
the habitability of exoplanets, the role of their magnetic fields in maintaining a stable environment is something to consider in addition
to things like the atmosphere and climate," Kao said.

To generate a magnetic field, a planet's interior must be hot enough to
have electrically conducting fluids, which in the case of Earth is the
molten iron in its core. In Jupiter, the conducting fluid is hydrogen
under so much pressure it becomes metallic. Metallic hydrogen probably
also generates magnetic fields in brown dwarfs, Kao said, while in the interiors of stars the conducting fluid is ionized hydrogen.

The ultracool dwarf known as LSR J1835+3259 was the only object Kao
felt confident would yield the high-quality data needed to resolve its radiation belts.

"Now that we've established that this particular kind of steady-state,
low- level radio emission traces radiation belts in the large-scale
magnetic fields of these objects, when we see that kind of emission from
brown dwarfs -- and eventually from gas giant exoplanets -- we can more confidently say they probably have a big magnetic field, even if our
telescope isn't big enough to see the shape of it," Kao said, adding that
she is looking forward to when the Next Generation Very Large Array,
currently being planned by the National Radio Astronomy Observatory
(NRAO), can image many more extrasolar radiation belts.

"This is a critical first step in finding many more such objects and
honing our skills to search for smaller and smaller magnetospheres,
eventually enabling us to study those of potentially habitable, Earth-size planets," said coauthor Evgenya Shkolnik at Arizona State University,
who has been studying the magnetic fields and habitability of planets
for many years.

The team used the High Sensitivity Array, consisting of 39 radio dishes coordinated by the NRAO in the United States and the Effelsberg radio
telescope operated by the Max Planck Institute for Radio Astronomy
in Germany.

"By combining radio dishes from across the world, we can make incredibly
high- resolution images to see things no one has ever seen before. Our
image is comparable to reading the top row of an eye chart in California
while standing in Washington, D.C.," said coauthor Jackie Villadsen at
Bucknell University.

Kao emphasized that this discovery was a true team effort, relying heavily
on the observational expertise of co-first author Amy Mioduszewski
at NRAO in planning the study and analyzing the data, as well as the multiwavelength stellar flare expertise of Villadsen and Shkolnik. This
work was supported by NASA and the Heising-Simons Foundation.

* RELATED_TOPICS
o Space_&_Time
# Solar_Flare # Sun # Extrasolar_Planets # Stars #
Jupiter # Solar_System # Cosmic_Rays # Eris_(Xena)
* RELATED_TERMS
o Radio_telescope o Solar_flare o Ionosphere o
Van_Allen_radiation_belt o Solar_system o Geomagnetic_reversal
o Spitzer_space_telescope o Green_Bank_Telescope

========================================================================== Story Source: Materials provided by
University_of_California_-_Santa_Cruz. Original written by Tim
Stephens. Note: Content may be edited for style and length.


========================================================================== Journal Reference:
1. Melodie M. Kao, Amy J. Mioduszewski, Jackie Villadsen, Evgenya L.

Shkolnik. Resolved imaging confirms a radiation belt around an
ultracool dwarf. Nature, 2023; DOI: 10.1038/s41586-023-06138-w ==========================================================================

Link to news story: https://www.sciencedaily.com/releases/2023/05/230515131947.htm

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