White Dwarf Stars in Open Cluster NGC 6791

White Dwarf Stars in Open Cluster NGC 6791

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Fast Facts
News release ID: STScI-2008-25
Release Date: Jul 10, 2008
Image Use: Copyright
About this image

In studying the dimmest burned-out stars in globular star cluster NGC 6791, NASA's Hubble Space Telescope has uncovered a paradox: three different populations of stars exist in an object where all the stars should have formed at the same time out of an interstellar cloud of gas and dust.

[Left] – This is a ground-based telescopic view of NGC 6791, located 13,300 light-years away in the constellation Lyra. The green inset box shows the view with Hubble's Advanced Camera for Surveys.

[Top right] – The full Hubble Advanced Camera for Surveys field is full of stars estimated to be 8 billion years old. Two background galaxies can be seen at upper left.

[Bottom right] – A blow up of view of a small region of the Advanced Camera for Surveys field reveals very faint white dwarfs. The blue circles identify hotter dwarfs that are 4 billion years old. The red circles identify cooler dwarfs that are 6 billion years old.

Annotated Observations, Open Clusters, Star Clusters


NASA, ESA, Digitized Sky Survey, and L. Bedin (STScI)