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

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Maelezo
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.
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Chanzo https://esahubble.org/images/heic2108a/
Mwandishi ESA/Hubble & NASA, G. Piotto et al.

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This file is licensed under the Creative Commons Attribution 4.0 International license.
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sasa hivi20:49, 28 Septemba 2021Picha ndogo ya toleo la 20:49, 28 Septemba 20216,182 × 3,116 (10.09 MB)PandreveUploaded a work by ESA/Hubble & NASA, G. Piotto et al. from https://esahubble.org/images/heic2108a/ with UploadWizard

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