File:Detailed images of the surface of the star R Doradus (eso2412a).jpg
Size of this preview: 800 × 322 pixels. Other resolutions: 320 × 129 pixels | 640 × 258 pixels | 1,024 × 412 pixels | 1,280 × 515 pixels | 3,378 × 1,360 pixels.
Original file (3,378 × 1,360 pixels, file size: 285 KB, MIME type: image/jpeg)
| This is a file from the Wikimedia Commons. The description on its description page there is shown below.
|
Summary
| DescriptionDetailed images of the surface of the star R Doradus (eso2412a).jpg |
English: Astronomers have captured a sequence of images of a star other than the Sun in enough detail to track the motion of bubbling gas on its surface. The images of the star, R Doradus, were obtained with the Atacama Large Millimeter/submillimeter Array (ALMA), a telescope co-owned by ESO, in July and August 2023. This panel shows three of these real images, taken with ALMA on 18 July, 27 July and 2 August 2023. The giant bubbles — 75 times the size of the Sun — seen on the star’s surface are the result of convection motions inside the star. The size of the Earth’s orbit is shown for scale. |
||
| Date | 11 September 2024 (upload date) | ||
| Source |
|
||
| Author | ALMA (ESO/NAOJ/NRAO)/W. Vlemmings et al. | ||
| Other versions |
|
Licensing
This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. | |
This file is licensed under the Creative Commons Attribution 4.0 International license.
| |
Captions
Astronomers have captured a sequence of images of a star other than the Sun in enough detail to track the motion of bubbling gas on its surface.
Items portrayed in this file
depicts
image/jpeg
1,360 pixel
3,378 pixel
292,292 byte
6e350c46491b7b02e55a902caf281ae541425ef1
11 September 2024
3urfopxihk9v2k73lwn6x2tnmcap5fi8gkww0akwcn6z946hmc
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Dimensions | User | Comment | |
|---|---|---|---|---|
| current | 23:15, 11 September 2024 | 3,378 × 1,360 (285 KB) | OptimusPrimeBot | #Spacemedia - Upload of https://cdn.eso.org/images/large/eso2412a.jpg via Commons:Spacemedia |
File usage
The following page uses this file:
Metadata
This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
If the file has been modified from its original state, some details may not fully reflect the modified file.
| Image title |
|
|---|---|
| Date and time of data generation | 17:00, 11 September 2024 |
| Software used | Adobe Photoshop 25.11 (Windows) |
| File change date and time | 14:11, 14 August 2024 |
| Date and time of digitizing | 08:47, 28 September 2023 |
| Date metadata was last modified | 16:11, 14 August 2024 |
| Credit/Provider | ALMA (ESO/NAOJ/NRAO)/W. Vlemmings et al. |
| Source | European Southern Observatory |
| Unique ID of original document | xmp.did:ab88397e-b7e6-fc48-9732-d82c82cf8076 |
| Short title |
|
| Keywords | R Doradus |
| Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
| Usage terms |
|
| IIM version | 4 |
| JPEG file comment | Astronomers have captured a sequence of images of a star other than the Sun in enough detail to track the motion of bubbling gas on its surface. The images of the star, R Doradus, were obtained with the Atacama Large Millimeter/submillimeter Array (ALMA), a telescope co-owned by ESO, in July and August 2023. This panel shows three of these real images, taken with ALMA on 18 July, 27 July and 2 August 2023. The giant bubbles — 75 times the size of the Sun — seen on the star’s surface are the result of convection motions inside the star. The size of the Earth’s orbit is shown for scale. |
