{"id":38485,"date":"2023-10-20T10:31:05","date_gmt":"2023-10-20T09:31:05","guid":{"rendered":"https:\/\/www.innovationnewsnetwork.com\/?p=38485"},"modified":"2023-10-20T10:31:05","modified_gmt":"2023-10-20T09:31:05","slug":"never-before-seen-feature-jupiters-atmosphere-discovered-webb","status":"publish","type":"post","link":"https:\/\/www.innovationnewsnetwork.com\/never-before-seen-feature-jupiters-atmosphere-discovered-webb\/38485\/","title":{"rendered":"Never-before-seen feature of Jupiter\u2019s atmosphere discovered by Webb"},"content":{"rendered":"

NASA\u2019s James Webb Space Telescope has uncovered a new feature in Jupiter\u2019s atmosphere \u2013 a narrow jet stream near the planet’s equator.<\/h2>\n

The newly discovered jet stream in Jupiter\u2019s atmosphere spans more than 3,000 miles wide and has winds travelling at around 320 miles per hour.<\/p>\n

The jet provides an insight into how the layers of Jupiter\u2019s atmosphere interact with each other, and how Webb is capable of tracking those features.<\/p>\n

\u201cThis is something that totally surprised us,\u201d said Ricardo Hueso of the University of the Basque Country, lead author on the paper describing the findings.<\/p>\n

\u201cWhat we have always seen as blurred hazes in Jupiter\u2019s atmosphere now appear as crisp features that we can track along with the planet\u2019s fast rotation.\u201d<\/p>\n

The results of the study, \u2018An intense narrow equatorial jet in Jupiter\u2019s lower stratosphere observed by JWST<\/a>,\u2019 is published in the journal Nature Astronomy. <\/em><\/p>\n

Webb data versus data from other ground-based telescopes<\/h3>\n

The researchers analysed data from Webb\u2019s Near Infrared Camera captured in July 2022.<\/p>\n

The Early Release Science programme was designed to take images of Jupiter ten hours apart in four different filters. These filters are uniquely able to detect changes in small features at different altitudes of Jupiter\u2019s atmosphere.<\/p>\n

Imke de Pater from the University of California, co-lead author of the study, said: \u201cEven though various ground-based telescopes, spacecraft like NASA\u2019s Juno and Cassini, and NASA\u2019s Hubble Space Telescope have observed the Jovian system\u2019s changing weather patterns, Webb has already provided new findings on Jupiter\u2019s rings, satellites, and its atmosphere.\u201d<\/p>\n

Although Jupiter differs significantly from Earth both planets have layered atmospheres. Infrared, visible, radio, and ultraviolet light wavelengths detected by the other telescopes identify the deeper layers of the planet\u2019s atmosphere.<\/p>\n

In comparison, Webb looks farther into the near-infrared to the higher-altitude layers of the atmosphere. These layers are around 15 to 30 miles above Jupiter\u2019s cloud tops.<\/p>\n

In near infrared imaging, high-altitude hazes appear blurry, but with Webb, finer details are resolved within the bright hazy band.<\/p>\n

Comparing the new feature of Jupiter’s atmosphere with previous data<\/h3>\n

The jet stream travels at around 320 miles per hour, twice the sustained winds of a Category 5 hurricane on Earth. It is located approximately 25 miles above the clouds in Jupiter\u2019s lower stratosphere.<\/p>\n

The team compared the winds observed by Webb at high altitudes to the winds observed by the Hubble<\/a> at deeper layers. They found that they could measure how fast the winds change with altitude and generate wind shears.<\/p>\n

Although Webb\u2019s resolution allowed for the detection of small cloud features used to track the jet in Jupiter\u2019s atmosphere, the Hubble observations taken one day after these discoveries helped to determine the base state of Jupiter\u2019s equatorial atmosphere. The complementary observations revealed the development of convective storms in Jupiter\u2019s equator not connected to the jet.<\/p>\n

\"\"
\u00a9 NASA, ESA, CSA, STScI, Ricardo Hueso (UPV), Imke de Pater (UC Berkeley), Thierry Fouchet (Observatory of Paris), Leigh Fletcher (University of Leicester), Michael H. Wong (UC Berkeley)<\/figcaption><\/figure>\n

\u201cWe knew the different wavelengths of Webb and Hubble would reveal the three-dimensional structure of storm clouds, but we were also able to use the timing of the data to see how rapidly storms develop,\u201d said team member Michael Wong of the University of California, who led the associated Hubble observations.<\/p>\n

Observing the jet stream over time<\/h3>\n

Now, the team will complete additional observations of Jupiter with Webb to find out if the jet\u2019s speed and altitude change over time.<\/p>\n

\u201cJupiter has a complicated but repeatable pattern of winds and temperatures in its equatorial stratosphere, high above the winds in the clouds and hazes measured at these wavelengths,\u201d explained team member Leigh Fletcher of the University of Leicester.<\/p>\n

\u201cIf the strength of this new jet is connected to this oscillating stratospheric pattern, we might expect the jet to vary considerably over the next two to four years \u2013 it\u2019ll be really exciting to test this theory in the years to come.\u201d<\/p>\n","protected":false},"excerpt":{"rendered":"

Webb has uncovered a new feature in Jupiter\u2019s atmosphere \u2013 a narrow jet stream near the planet’s equator. Read more here.<\/p>\n","protected":false},"author":18,"featured_media":38488,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"footnotes":""},"categories":[771],"tags":[3477],"acf":[],"yoast_head":"\nNever-before-seen feature of Jupiter\u2019s atmosphere discovered by Webb<\/title>\n<meta name=\"description\" content=\"Webb has uncovered a new feature in Jupiter\u2019s atmosphere \u2013 a narrow jet stream near the planet's equator. 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