Space Industry and Business News  
SOLAR SCIENCE
Jupiter's Atmosphere Heats up under Solar Wind
by Staff Writers for NASA News
Greenbelt MD (SPX) Apr 09, 2019

Sensitive to Jupiter's stratospheric temperatures, these infrared images were recorded by the Cooled Mid-Infrared Camera and Spectrograph (COMICS) at the Subaru Telescope on the summit of Mauna Kea, Hawaii. Areas of the atmosphere that are more yellow and red indicate the hotter regions. Aurora produce enhanced and variable heating at Jupiter's poles. The heating occurs when the magnetosphere and the solar wind interact and deposit energy into Jupiter's atmosphere. Images were captured less than a day apart, from Jan. 11-12, 2017, and illustrate how quickly the atmosphere varied in response to the solar wind.

New Earth-based telescope observations show that auroras at Jupiter's poles are heating the planet's atmosphere to a greater depth than previously thought - and that it is a rapid response to the solar wind.

"The solar wind impact at Jupiter is an extreme example of space weather," said James Sinclair of NASA's Jet Propulsion Laboratory in Pasadena, California, who led new research published April 8 in Nature Astronomy. "We're seeing the solar wind having an effect deeper than is normally seen."

Auroras at Earth's poles (known as the aurora borealis at the North Pole and aurora australis at the South Pole) occur when the energetic particles blown out from the Sun (the solar wind) interact with and heat up the gases in the upper atmosphere. The same thing happens at Jupiter, but the new observations show the heating goes two or three times deeper down into its atmosphere than on Earth, into the lower level of Jupiter's upper atmosphere, or stratosphere.

Understanding how the Sun's constant outpouring of solar wind interacts with planetary environments is key to better understanding the very nature of how planets and their atmospheres evolve.

"What is startling about the results is that we were able to associate for the first time the variations in solar wind and the response in the stratosphere - and that the response to these variations is so quick for such a large area," said JPL's Glenn Orton, co-author and part of the observing team.

Within a day of the solar wind hitting Jupiter, the chemistry in its atmosphere changed and its temperature rose, the team found. An infrared image captured during their observing campaign in January, February and May of 2017 clearly shows hot spots near the poles, where Jupiter's auroras are. The scientists based their findings on observations by the Subaru Telescope, atop the summit of Mauna Kea in Hawaii, which is operated by the National Astronomical Observatory of Japan.

The telescope's Cooled Mid-Infrared Camera and Spectograph (COMICS) recorded thermal images - which capture areas of higher or lower temperatures - of Jupiter's stratosphere.

"Such heating and chemical reactions may tell us something about other planets with harsh environments, and even early Earth," said Yasumasa Kasaba of Tohoku University, who also worked on the observing team.


Related Links
Subaru Telescope
Solar Science News at SpaceDaily


Thanks for being here;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Contributor
$5 Billed Once


credit card or paypal
SpaceDaily Monthly Supporter
$5 Billed Monthly


paypal only


SOLAR SCIENCE
And the Blobs Just Keep on Coming
Greenbelt MD (SPX) Apr 05, 2019
When Simone Di Matteo first saw the patterns in his data, it seemed too good to be true. "It's too perfect!" Di Matteo, a space physics Ph.D. student at the University of L'Aquila in Italy, recalled thinking. "It can't be real." And it wasn't, he'd soon find out. Di Matteo was looking for long trains of massive blobs - like a lava lamp's otherworldly bubbles, but anywhere from 50 to 500 times the size of Earth - in the solar wind. The solar wind, whose origins aren't yet fully understood, is the s ... read more

Comment using your Disqus, Facebook, Google or Twitter login.



Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle

SOLAR SCIENCE
Maxar and NASA complete Design Review for Restore-L On-Orbit Servicing Spacecraft Bus

ESA oversees teaching of Europe's next top solderers

Russia's new ISS modules will be shielded with fabrics used in body armour

Arralis announces 10W GaN-SiC MMIC high power amplifier for K-Band comms

SOLAR SCIENCE
US Army selects Hughes for cooperative effort to upgrades NextGen Friendly Forces System

United Launch Alliance launches WGS-10 satellite for USAF

United Launch Alliance set to launch WGS-10 for US Air Force

Raytheon awarded $406M for Army aircraft radio system

SOLAR SCIENCE
SOLAR SCIENCE
Record-Breaking Satellite Advances NASA's Exploration of High-Altitude GPS

China, Arab states eye closer cooperation on satellite navigation to build "Space Silk Road"

Second GPS III satellite arrives at Cape Canaveral ahead of July launch

GPS 3 space vehicle 02 "Magellan" arrives in Florida; prepares for July launch

SOLAR SCIENCE
Britain to deploy F-35Bs for first time, sending them to Cyprus air basel

Sierra Nevada awarded $42.7M to train Afghan Air Force on A-29 Super Tucano

In hidden mountain air base, Albania stores MiGs for sale

Naval teams narrow factors in physiological episodes on jets

SOLAR SCIENCE
Ferromagnetic nanoparticle systems show promise for ultrahigh-speed spintronics

DARPA Announces Second Annual ERI Summit

Ushering in ultrafast cluster electronics

A new hope of quantum computers for factorizations of RSA with a thousand-fold excess

SOLAR SCIENCE
DLR and the UStuttgart test transmission of EO data using laser communications

Sun, moon and sea as part of a 'seismic probe'

Natural climate processes overshadow recent human-induced Walker circulation trends

Declassified U2 spy plane images reveal bygone Middle Eastern archaeological features

SOLAR SCIENCE
Children in South Asia hardest hit by air pollution, says study

Asia's pollution exodus: Firms struggle to woo top talent

Residents split on future of Romania's trash heap 'time-bomb'

Air pollution hotspots in Europe









The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.