Archivo de imágenes de Hubble

Vistas del Hubble de M13 (2010) y M3 (2019)

To investigate the physics underpinning white dwarf evolution, astronomers compared cooling white dwarfs in two massive collections of stars: the globular clusters M13 and M3. These two clusters share many physical properties such as age and metallicity, but the populations of st...

Fecha
Jan 1, 2021
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2021-050-01feh155dmewsw3ez4m23c9vyx
Por

To investigate the physics underpinning white dwarf evolution, astronomers compared cooling white dwarfs in two massive collections of stars: the globular clusters M13 and M3. 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 M13 and M3 together a perfect natural laboratory in which to test how different populations of white dwarfs cool.

Credits

Science

ESA, NASA, Giampaolo Piotto

Detalles de la imagen

About The Object
Object NameM13 and M3
Object DescriptionGlobular star clusters
DistanceM13 and M3 are respectively 25,000 and 34,000 lightyears away.

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Fuente

La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.

Ver en NASA.gov

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