File:Hubble’s Views of M13 (2010) and M3 (2019).jpg
![File:Hubble’s Views of M13 (2010) and M3 (2019).jpg](https://upload.wikimedia.org/wikipedia/commons/thumb/4/4b/Hubble%E2%80%99s_Views_of_M13_%282010%29_and_M3_%282019%29.jpg/800px-Hubble%E2%80%99s_Views_of_M13_%282010%29_and_M3_%282019%29.jpg?20210928204934)
Original file (6,182 × 3,116 pixels, file size: 10.09 MB, MIME type: image/jpeg)
Captions
Captions
Summary
[edit]DescriptionHubble’s Views of M13 (2010) and M3 (2019).jpg |
English: To investigate the physics underpinning white dwarf evolution, astronomers compared cooling white dwarfs in two massive collections of stars: the globular clusters M3 and M13. These two clusters share many physical properties such as age and metallicity but the populations of stars which will eventually give rise to white dwarfs are different. This makes M3 and M13 together a perfect natural laboratory in which to test how different populations of white dwarfs cool. |
Date | |
Source | https://esahubble.org/images/heic2108a/ |
Author | ESA/Hubble & NASA, G. Piotto et al. |
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:
|
![]() |
![w:en:Creative Commons](https://upload.wikimedia.org/wikipedia/commons/thumb/7/79/CC_some_rights_reserved.svg/90px-CC_some_rights_reserved.svg.png)
![attribution](https://upload.wikimedia.org/wikipedia/commons/thumb/1/11/Cc-by_new_white.svg/24px-Cc-by_new_white.svg.png)
- 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 | 20:49, 28 September 2021 | ![]() | 6,182 × 3,116 (10.09 MB) | Pandreve (talk | contribs) | Uploaded a work by ESA/Hubble & NASA, G. Piotto et al. from https://esahubble.org/images/heic2108a/ with UploadWizard |
You cannot overwrite this file.
File usage on Commons
There are no pages that use this file.
File usage on other wikis
The following other wikis use this file:
- Usage on en.wikipedia.org
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.
Image title |
|
---|---|
Source | ESA/Hubble |
Credit/Provider | ESA/Hubble & NASA, G. Piotto et al. |
Short title |
|
Usage terms |
|
Date and time of data generation | 17:00, 6 September 2021 |
JPEG file comment | To investigate the physics underpinning white dwarf evolution, astronomers compared cooling white dwarfs in two massive collections of stars: the globular clusters M3 and M13. These two clusters share many physical properties such as age and metallicity but the populations of stars which will eventually give rise to white dwarfs are different. This makes M3 and M13 together a perfect natural laboratory in which to test how different populations of white dwarfs cool. |
Software used | Adobe Photoshop 22.4 (Windows) |
File change date and time | 19:07, 21 August 2021 |
Date and time of digitizing | 21:04, 21 August 2021 |
Date metadata was last modified | 21:07, 21 August 2021 |
Unique ID of original document | xmp.did:be09bcff-d104-2b42-ab66-ba7135cbb411 |
Keywords |
|
Contact information |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIM version | 4 |