News Release Archive:

News Release 454 of 1051

August 17, 2006 02:00 PM (EDT)

News Release Number: STScI-2006-37

Hubble Sees Faintest Stars in a Globular Cluster


Image: Tale of Two Stellar Populations in Globular Cluster NGC 6397

Tale of Two Stellar Populations in Globular Cluster NGC 6397

Screen-use options: These files are created for viewing on your monitor

Print-use download options: These files are designed to fit on letter-size paper


This graph schematically plots two populations of stars Hubble has seen in a neighboring star cluster. The graph, a simplified version of the original data, plots stellar brightness (vertical axis) against stellar color-temperature. The normal main sequence stars in the cluster are plotted on the right curve. The cooler a star is, the redder it appears, and it diminishes in brightness. Hubble has identified the very coolest and faintest normal stars in the cluster.

The curve on the left plots the white dwarf population of burned-out sunlike stars. It follows a normal "cooling slope" until the white dwarf begins to look bluer and hook toward the left. The dwarfs aren't getting hotter. Chemical changes in their atmospheres make them look cooler. This predicted "white dwarf hook" has never been seen before.

Image Type: Illustration

Credit: NASA, ESA and A. Feild (STScI)


All images from this news release:

To access available information and downloadable versions of images in this news release, click on any of the images below: