File:Hubble’s two new views of Jupiter (January 2024) (heic2404a).jpg
From Wikimedia Commons, the free media repository
Jump to navigation
Jump to search
Size of this preview: 800 × 400 pixels. Other resolutions: 320 × 160 pixels | 640 × 320 pixels | 1,024 × 511 pixels | 1,280 × 639 pixels | 2,625 × 1,311 pixels.
Original file (2,625 × 1,311 pixels, file size: 465 KB, MIME type: image/jpeg)
File information
Structured data
Captions
Summary
[edit]DescriptionHubble’s two new views of Jupiter (January 2024) (heic2404a).jpg |
English: The giant planet Jupiter, in all its banded glory, is revisited by the NASA/ESA Hubble Space Telescope in these latest images, taken on 5–6 January 2024, that capture both sides of the planet. Hubble monitors Jupiter and the other outer Solar System planets every year under the Outer Planet Atmospheres Legacy programme (OPAL). This is because these large worlds are shrouded in clouds and hazes stirred up by violent winds, leading to a kaleidoscope of ever-changing weather patterns.[left image] - Big enough to swallow Earth, the classic Great Red Spot stands out prominently in Jupiter's atmosphere. To its lower right, at a more southerly latitude, is a feature sometimes dubbed Red Spot Jr. This anticyclone was the result of storms merging in 1998 and 2000, and it first appeared red in 2006 before returning to a pale beige in subsequent years. This year it is somewhat redder again. The source of the red coloration is unknown but may involve a range of chemical compounds: sulphur, phosphorus or organic material. Staying in their lanes, but moving in opposite directions, Red Spot Jr. passes the Great Red Spot about every two years. Another small red anticyclone appears in the far north.[right image] - Storm activity also appears in the opposite hemisphere. A pair of storms: a deep red cyclone and a reddish anticyclone, appear to be next to each other at right of centre. They look so red that at first glance, it looks like Jupiter skinned a knee. These storms are rotating in opposite directions, indicating an alternating pattern of high- and low-pressure systems. For the cyclone, there’s an upwelling on the edges with clouds descending in the middle causing a clearing in the atmospheric haze.The storms are expected to bounce past each other because their opposing clockwise and counterclockwise rotations make them repel each other. Toward the left edge of the image is the innermost Galilean moon, Io — the most volcanically active body in the Solar System, despite its small size (only slightly larger than Earth's moon). Hubble resolves volcanic outflow deposits on the surface. Hubble's sensitivity to blue and violet wavelengths clearly reveals interesting surface features.[Image description: A side-by-side image showing both faces of Jupiter on the black background of space. The left image is labelled January 5, 2024. Jupiter is banded with stripes of brownish orange, light grey, soft yellow, and shades of cream, punctuated with many large storms and small white clouds. The Great Red Spot is the most prominent feature in the left bottom third of this view. The right image is labelled January 6, 2024. This opposite side of Jupiter is also banded with stripes of brownish orange, light grey, soft yellow, and shades of cream. At upper right of centre, a pair of storms appear next to each other: a deep-red, triangle-shaped cyclone and a reddish anticyclone. Toward the far-left edge of this view is Jupiter’s tiny orange-coloured moon Io.] |
Date | 14 March 2024 (upload date) |
Source | Hubble’s two new views of Jupiter (January 2024) |
Author | NASA, ESA, J. DePasquale (STScI), A. Simon (NASA-GSFC) |
Other versions |
|
Licensing
[edit]ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
Conditions:
Notes:
|
This file is licensed under the Creative Commons Attribution 4.0 International license.
Attribution: ESA/Hubble
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 09:01, 17 March 2024 | 2,625 × 1,311 (465 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://cdn.esahubble.org/archives/images/large/heic2404a.jpg via Commons:Spacemedia |
You cannot overwrite this file.
File usage on Commons
The following page uses this file:
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Author | Space Telescope Science Institute Office of Public Outreach |
---|---|
Credit/Provider | NASA, ESA, J. DePasquale (STScI), A. Simon (NASA-GSFC) |
Source | ESA/Hubble |
Image title |
|
Short title |
|
Usage terms |
|
Date and time of data generation | 15:00, 14 March 2024 |
JPEG file comment | he monster planet Jupiter in all its banded glory is revisited by NASA‘s Hubble Space Telescope in this latest image taken on January 6, 2024. Hubble monitors Jupiter and the other outer planets every year under the Outer Planet Atmospheres Legacy program (OPAL). This is because these large worlds are shrouded in clouds and hazes stirred up by violent winds causing a kaleidoscope of ever-changing weather patterns. [Image left] Big enough to swallow Earth, the classic Great Red Spot (GRS) stands out prominently in Jupiter’s atmosphere. Below and to the right and at a more southerly latitude is a feature sometimes dubbed Red Spot Jr. This anticyclone was the result of storms merging in 1998 and 2000, and it first appeared red in 2006 before returning to a pale beige in subsequent years. This year it is somewhat redder again. The source of the red coloration is unknown but may involve a range of chemical compounds: sulfur, phosphorus or organic material. Staying in their lanes, but moving in opposite directions, Red Spot Jr. passes the GRS about every two years. Another small red anticyclone appears in the far north. [image right] Storm activity also appears in the opposite hemisphere. A pair of storms, a deep red cyclone and a reddish anticyclone, appear right of center; they look so red that at first glance, it looks like Jupiter skinned a knee. These storms are rotating in opposite directions, indicating an alternating pattern of high- and low-pressure systems. For the cyclone, there’s an upwelling on the edges with clouds descending in the middle causing a clearing in the atmospheric haze. The storms are expected to bounce past each other because their opposing clockwise and counterclockwise rotation makes them repel each other. “The many large storms and small white clouds are a hallmark of a lot of activity going on in Jupiter’s atmosphere right now,” said OPAL project lead Amy Simon of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Toward the left edge of the photo is the innermost Galilean moon, Io, the most volcanically active body in the solar system despite its small size (only slightly larger than Earth’s moon). Hubble resolves volcanic outflow deposits on the surface. Hubble’s sensitivity to blue and violet wavelengths clearly reveals interesting surface features. In 1979 NASA’s Voyager 1 spacecraft discovered Io’s pizza-like appearance and volcanism, to the surprise of planetary scientists because it is such a small moon. Hubble is picking up where Voyager left off by keeping an eye on restless Io year by year. |
Software used | Adobe Photoshop 24.7 (Macintosh) |
File change date and time | 10:18, 14 February 2024 |
Date and time of digitizing | 06:11, 13 February 2024 |
Date metadata was last modified | 10:08, 14 February 2024 |
Unique ID of original document | xmp.did:b4d262d2-633c-44d4-8d08-0fbb12f92cda |
Keywords | Jupiter |
Contact information | outreach@stsci.edu
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIM version | 4 |