New research published in Nature has revealed the solution to Jupiter’s ‘energy crisis’, which has puzzled astronomers for decades.
From: University of Leicester
August
4, 2021 -- Space scientists at the University of Leicester worked with
colleagues from the Japanese Space Agency (JAXA), Boston University, NASA’s
Goddard Space Flight Center and the National Institute of Information and
Communications Technology (NICT) to reveal the mechanism behind Jupiter’s
atmospheric heating.
Now, using data from the Keck Observatory
in Hawai’i, astronomers have created the most-detailed yet global map of the
gas giant’s upper atmosphere, confirming for the first time that Jupiter’s
powerful aurorae are responsible for delivering planet-wide heating.
Dr James O’Donoghue is a researcher at
JAXA and completed his PhD at Leicester, and is lead author for the research
paper.
He said: “We first began trying to
create a global heat map of Jupiter’s uppermost atmosphere at the University of
Leicester. The signal was not bright enough to reveal anything outside of
Jupiter’s polar regions at the time, but with the lessons learned from that
work we managed to secure time on one of the largest, most competitive
telescopes on Earth some years later.
“Using the Keck telescope we produced
temperature maps of extraordinary detail. We found that temperatures start very
high within the aurora, as expected from previous work, but now we could
observe that Jupiter’s aurora, despite taking up less than 10% of the area of
the planet, appear to be heating the whole thing.
“This research started in Leicester and
carried on at Boston University and NASA before ending at JAXA in Japan.
Collaborators from each continent working together made this study successful,
combined with data from NASA’s Juno spacecraft in orbit around Jupiter and
JAXA’s Hisaki spacecraft, an observatory in space.”
Dr Tom Stallard and Dr Henrik Melin are
both part of the School of Physics and Astronomy at the University of
Leicester. Dr Stallard added: “There has been a very long-standing puzzle in
the thin atmosphere at the top of every Giant Planet within our solar system.
“With every Jupiter space mission, along
with ground-based observations, over the past 50 years, we have consistently
measured the equatorial temperatures as being much too hot.
“This ‘energy crisis’ has been a long
standing issue – do the models fail to properly model how heat flows from the
aurora, or is there some other unknown heat source near the equator?
“This paper describes how we have mapped
this region in unprecedented detail and have shown that, at Jupiter, the
equatorial heating is directly associated with auroral heating.”
Aurorae occur when charged particles are
caught in a planet’s magnetic field. These spiral along the field lines towards
the planet’s magnetic poles, striking atoms and molecules in the atmosphere to
release light and energy.
On Earth, this leads to the
characteristic light show that forms the Aurora Borealis and Australis. At
Jupiter, the material spewing from its volcanic moon, Io, leads to the most
powerful aurora in the Solar System and enormous heating in the polar regions
of the planet.
Although the Jovian aurorae have long
been a prime candidate for heating the planet’s atmosphere, observations have
previously been unable to confirm or deny this until now.
Previous maps of the upper atmospheric
temperature were formed using images consisting of only several pixels. This is
not enough resolution to see how the temperature might be changed across the
planet, providing few clues as to the origin of the extra heat.
Researchers created five maps of the
atmospheric temperature at different spatial resolutions, with the highest
resolution map showing an average temperature measurement for squares two
degrees longitude ‘high’ by two degrees latitude ‘wide’.
The team scoured more than 10,000
individual data points, only mapping points with an uncertainty of less than
five per cent.
Models of the atmospheres of gas giants
suggest that they work like a giant refrigerator, with heat energy drawn from
the equator towards the pole, and deposited in the lower atmosphere in these
pole regions.
These new findings suggest that
fast-changing aurorae may drive waves of energy against this poleward flow,
allowing heat to reach the equator.
Observations also showed a region of
localised heating in the sub-auroral region that could be interpreted as a
limited wave of heat propagating equatorward, which could be interpreted as
evidence of the process driving heat transfer.
Planetary research at the University of
Leicester spans the breadth of Jovian system, from the planet’s magnetosphere
and atmosphere, out to its diverse collection of satellites.
Leicester researchers are members of the
Juno mission made up of a global team astronomers observing the giant planet,
and are leading
Jupiter observations from the forthcoming James Webb Space Telescope.
Leicester also plays a leading role in science and instrumentation on the
European Space Agency (ESA)’s Jupiter Icy Moons Explorer (JUICE), due for
launch in 2022.
‘Global upper-atmospheric heating on
Jupiter by the polar aurorae’ is available in Nature.
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