(Press-News.org)
A new study by researchers including those at the University of Tokyo revealed that atmospheric gravity waves play a crucial role in driving latitudinal air currents on Mars, particularly at high altitudes. The findings, based on long-term atmospheric data, offer a fresh perspective on the behaviors of Mars' middle atmosphere, highlighting fundamental differences from Earth’s. The study applied methods developed to explore Earth’s atmosphere to quantitatively estimate the influence of gravity waves on Mars’ planetary circulation.
Despite it being a very cold planet, Mars is quite a hot topic these days. With human visitation seemingly on the horizon, it will pay to know more about the conditions there so all involved can plan and prepare accordingly. Something that has become possible to explore in detail in recent years is a range of Martian atmospheric phenomena. Naturally, a lot of the methods used for this originate from the study of our own atmosphere, and thanks to this, we can see how things on Mars differ greatly and what the implications of this might be.
"On Earth, large-scale atmospheric waves caused by the planet’s rotation, known as Rossby waves, are the primary influence on the way air circulates in the stratosphere, or the lower part of the middle atmosphere. But our study shows that on Mars, gravity waves (GWs) have a dominant effect at the mid and high latitudes of the middle atmosphere," said Professor Kaoru Sato from the Department of Earth and Planetary Science. “Rossby waves are large-scale atmospheric waves, or resolved waves, whereas GWs are unresolved waves, meaning they are too fine to be directly measured or modeled and must be estimated by more indirect means.”
Not to be confused with gravitational waves from massive stellar bodies, GWs are an atmospheric phenomenon when a packet of air rises and falls due to variations in buoyancy. That oscillating motion is what gives rise to GWs. Due to the small-scale nature of them and the limitations of observational data, researchers have previously found it challenging to quantify their significance in the Martian atmosphere. So Sato and her team turned to the Ensemble Mars Atmosphere Reanalysis System (EMARS) dataset, produced by a range of space-based observations over many years, to analyze seasonal variations up there.
“We found something interesting, that GWs facilitate the rapid vertical transfer of angular momentum, significantly influencing the meridional, or north-south, in the middle atmosphere circulations on Mars,” said graduate student Anzu Asumi. “It’s interesting because it more closely resembles the behavior seen in Earth’s mesosphere rather than in our stratosphere. This suggests existing Martian atmospheric circulation models may need to be refined to better incorporate these wave effects, potentially improving future climate and weather simulations.”
The research also underscores the importance of planetary comparisons in atmospheric science. Mars’ similarity to Earth in terms of rotational speed and axial tilt makes it an ideal test case for studying planetary weather systems. At the same time, its distinct characteristics, such as a thin carbon dioxide-rich atmosphere and pronounced seasonal variations, offer insights into alien atmospheres. By analyzing these differences, researchers can improve their understanding of fundamental atmospheric dynamics, which may ultimately contribute to better climate models for Earth too.
“Looking ahead, we plan to investigate the impact of Martian dust storms on atmospheric circulation. So far, our analysis has focused on years without major dust storms,” said Sato. “However, these storms dramatically alter atmospheric conditions, and we suspect they may intensify the role of GWs in circulation. Our research lays the groundwork for forecasting Martian weather, which will be essential for ensuring the success of future Mars missions."
Future studies will examine how these storms lead to significant shifts in global atmospheric patterns. With these advancements, the prospect of accurately predicting atmospheric conditions on Mars moves one step closer to reality. Will you tune into the Martian weather report one day?
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Journal article:
Anzu Asumi, Kaoru Sato, Masashi Kohma, and Yoshi-Yuki Hayashi, “Climatology of the Residual Mean Circulation of the Martian Atmosphere and Contributions of Resolved and Unresolved Waves Based on a Reanalysis Dataset”, Journal of Geophysical Research: Planets, DOI: 10.1029/2023JE008137
https://doi.org/10.1029/2023JE008137
Funding: This research was supported by the Japan Society for the Promotion of Science (Grant 22H00169).
Useful links:
Department of Earth and Planetary Science - https://www.eps.s.u-tokyo.ac.jp/en/
Graduate School of Science - https://www.s.u-tokyo.ac.jp/en/index.html
Research contact:
Ms. Anzu Asumi
Department of Earth and Planetary Science, The University of Tokyo,
7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
asumi@eps.s.u-tokyo.ac.jp
Press contact:
Mr. Rohan Mehra
Public Relations Group, The University of Tokyo,
7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-8656, Japan
press-releases.adm@gs.mail.u-tokyo.ac.jp
About The University of Tokyo:
The University of Tokyo is Japan's leading university and one of the world's top research universities. The vast research output of some 6,000 researchers is published in the world's top journals across the arts and sciences. Our vibrant student body of around 15,000 undergraduate and 15,000 graduate students includes over 4,000 international students. Find out more at www.u-tokyo.ac.jp/en/ or follow us on X (formerly Twitter) at @UTokyo_News_en.
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