File:Hubble Probes Storm Systems on Jupiter (49887088206).jpg
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[edit]DescriptionHubble Probes Storm Systems on Jupiter (49887088206).jpg |
Thanks to collaborative observations by the NASA/ESA Hubble Space Telescope, the Gemini Observatory, and the Juno spacecraft, scientists have probed deeper into the atmosphere of the planet Jupiter. This collection of observations have facilitated the monitoring of Jupiter's weather and to estimate the amount of water in the atmosphere, providing insight into how Jupiter operates today as well as how it and the other planets in our solar system formed more than four-and-a-half billion years ago. This illustration of lightning, convective towers (thunderheads), deep water clouds, and clearings in Jupiter's atmosphere is based on data collected by these observatories. The Hubble Space Telescope has detected sunlight that is reflected off clouds in Jupiter's atmosphere. Different wavelengths penetrate to different depths in the clouds, giving researchers the ability to determine the relative heights of cloud tops. Credit: NASA, ESA, M.H. Wong (UC Berkeley), and A. James and M.W. Carruthers (STScI) |
Date | |
Source | Hubble Probes Storm Systems on Jupiter |
Author | Hubble ESA |
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This image was originally posted to Flickr by Hubble Space Telescope / ESA at https://flickr.com/photos/51268976@N08/49887088206. It was reviewed on 7 December 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
7 December 2020
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current | 12:43, 7 December 2020 | 1,280 × 812 (146 KB) | Eyes Roger (talk | contribs) | Transferred from Flickr via #flickr2commons |
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Author | Space Telescope Science Institute Office of Public Outreach |
Source | ESA/Hubble |
Credit/Provider | NASA, ESA, M.H. Wong (UC Berkeley), and A. James and M.W. Carruthers (STScI) |
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Usage terms |
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Date and time of data generation | 16:35, 12 May 2020 |
JPEG file comment | This illustration of lightning, convective towers (thunderheads), deep water clouds, and clearings in Jupiter's atmosphere is based on data collected by the Juno spacecraft, the Hubble Space Telescope, and the Gemini Observatory. Juno detects radio signals generated by lightning discharges. Because radio waves can pass through all of Jupiter's cloud layers, Juno is able to detect lightning in deep clouds as well as lightning on the day side of the planet. Hubble detects sunlight that has reflected off clouds in Jupiter's atmosphere. Different wavelengths penetrate to different depths in the clouds, giving researchers the ability to determine the relative heights of cloud tops. Gemini maps the thickness of cool clouds that block thermal infrared light from warmer atmospheric layers below the clouds. Thick clouds appear dark in the infrared maps, while clearings appear bright. The combination of observations can be used to map the cloud structure in three dimensions and infer details of atmospheric circulation. Thick, towering clouds form where moist air rises (upwelling and active convection). Clearings form where drier air sinks (downwelling). The clouds shown rise five times higher than similar convective towers in Earth's relatively shallow atmosphere. The region illustrated covers a horizontal span one-third greater than that of the continental United States. |
Software used | Adobe Photoshop 21.0 (Macintosh) |
File change date and time | 11:43, 29 April 2020 |
Date and time of digitizing | 07:41, 29 April 2020 |
Date metadata was last modified | 19:17, 4 May 2020 |
Unique ID of original document | uuid:65E6390686CF11DBA6E2D887CEACB407 |
Keywords | Jupiter |
Contact information | outreach@stsci.edu
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
IIM version | 4 |