File:Hubble’s Views of M13 (2010) and M3 (2019).jpg

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	20:49, 28 September 2021		6,182 × 3,116 (10.09 MB)	commons>Pandreve	Uploaded a work by ESA/Hubble & NASA, G. Piotto et al. from https://esahubble.org/images/heic2108a/ with UploadWizard

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Image title	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.
Source	ESA/Hubble
Credit/Provider	ESA/Hubble & NASA, G. Piotto et al.
Short title	Hubble’s Views of M13 (2010) and M3 (2019)
Usage terms	Creative Commons Attribution 4.0 International License
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	M13 M3
Contact information	https://esahubble.org ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States
IIM version	4

File:Hubble’s Views of M13 (2010) and M3 (2019).jpg

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