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White Dwarfs in Globular Cluster M4

White Dwarfs in Globular Cluster M4

This graph shows the relationship between the temperature and brightness of a sampling of stars in the globular cluster M4. The line of dots at upper right represents main-sequence stars, those whose cores are fusing hydrogen. Normal stars like our Sun fall in the middle of this line.

The white dwarfs are not part of the main-sequence stars because they have used up their hydrogen fuel. These dying stars are fainter and yet hotter than their main-sequence relatives. NASA's Hubble Space Telescope hunted for the faintest and coolest of the white dwarfs [bottom of white dwarf population.]

  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    M4, NGC 6121
  • Release Date
    April 24, 2002
  • Science Release
    Hubble Uncovers Oldest “Clocks” in Space to Read Age of Universe

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Last Updated
Mar 14, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov