An international team of scientists has proved that Mercury, our solar system’s smallest planet, has geomagnetic storms similar to those on Earth.
From: University of Alaska Fairbanks
By Rod Boyce
March 29, 2022 -- The research by scientists in the
United States, Canada and China includes work by Hui Zhang, a space physics
professor at the University of Alaska Fairbanks Geophysical Institute.
Their finding, a first,
answers the question of whether other planets, including those outside our
solar system, can have geomagnetic storms regardless of the size of their
magnetosphere or whether they have an Earth-like ionosphere.
The research was
published in two papers in February. Zhang is among the co-authors of each
paper.
The first of those
papers proves the planet has a ring current, a doughnut-shaped field of charged
particles flowing laterally around the planet and excluding the poles. The
second proves the existence of geomagnetic storms triggered by the ring
current.
A geomagnetic
storm is a major disturbance in a planet’s magnetosphere caused by the
transfer of energy from the solar wind. Such storms in Earth’s magnetosphere
produce the aurora and can disrupt radio communications.
The geomagnetic storms
finding was published Feb. 18 in the journal Science China Technological
Sciences. QiuGang Zong of the Institute of Space Physics and Applied Technology
at Peking University and the Polar Research Institute of China is the author.
That paper built on a
finding published one day earlier that verified through data observation
earlier suggestions that Mercury has a ring current. Earth also has a ring
current.
The ring current paper,
published in Nature Communications, is authored by Jiutong Zhao, also of
the Institute of Space Physics and Applied Technology at Peking
University.
Seven of the 14
scientists involved worked on both papers.
“The processes are
quite similar to here on Earth,’ Zhang said of Mercury’s magnetic storms. “The
main differences are the size of the planet and Mercury has a weak magnetic
field and virtually no atmosphere.”
Confirmation about
geomagnetic storms on Mercury results from research made possible by a
fortuitous coincidence: a series of coronal mass ejections from the sun on
April 8-18, 2015, and the end of NASA’s Messenger space probe, which launched
in 2004 and crashed into the planet’s surface on April 30, 2015, at the
expected end of its mission.
A coronal mass
ejection, or CME, is an ejected cloud of the sun’s plasma — a gas made of
charged particles. That cloud includes the plasma’s embedded magnetic field.
The coronal mass
ejection of April 14 proved to be the key for scientists. It compressed
Mercury’s ring current on the sun-facing side and increased the current’s
energy.
New analysis of data
from Messenger, which had dropped closer to the planet, shows “the presence of
a ring current intensification that is essential for triggering magnetic
storms,” the second of the two papers reads.
“The sudden
intensification of a ring current causes the main phase of a magnetic storm,”
Zhang said.
But this doesn’t mean
Mercury has auroral displays like those on Earth.
On Earth, the storms
produce aurora displays when solar wind particles interact with the particles
of the atmosphere. On Mercury, however, solar wind particles don’t encounter an
atmosphere. Instead, they reach the surface unimpeded and may therefore be
visible only through X-ray and gamma ray examination.
The results of the two
papers show that magnetic storms are “potentially a common feature of
magnetized planets,” the second of the papers reads.
“The results obtained
from Messenger provide a further fascinating insight into Mercury’s place in
the evolution of the solar system following the discovery of its intrinsic
planetary magnetic field,” it concludes.
Other institutions
involved in the research include the University of Alberta, Edmonton;
University of Michigan and the Heliophysics Science Division at NASA’s Goddard
Space Flight Center.
https://uaf.edu/news/uaf-researcher-in-papers-that-prove-mercury-has-magnetic-storms.php
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