NASA

Hubble Examines a Possible Relic

This NASA Hubble Space Telescope image captures the dwarf irregular galaxy UGC 4879 or VV124. As this image illustrates, Hubble’s high resolution can detect individual stars, even in the densest parts of the galaxy. This allows astronomers to better determine the galaxy’s distance, and the composition and age of its stars. UGC 4879 is an […]

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Aug 20, 2024 - 20:00

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Hubble Examines a Possible Relic

An oblong smudge of stars stretches diagonally across the image from upper-left to lower-right. It holds stars in blue, orange, yellow, and white. The highest concentration of stars is near the image center and toward the lower-right. This region also holds bright, light-blue clumps of stars. Star densities taper off in all directions as you move away from the core. A number of bright, distant galaxies dot the scene, with a few shining through UGC 4879.

NASA, ESA, K. Chiboucas (NOIRLab – Gemini North (HI), and M. Monelli (Instituto de Astrofisica de Canarias); Image Processing: Gladys Kober (NASA/Catholic University of America)

This NASA Hubble Space Telescope image captures the dwarf irregular galaxy UGC 4879 or VV124. As this image illustrates, Hubble’s high resolution can detect individual stars, even in the densest parts of the galaxy. This allows astronomers to better determine the galaxy’s distance, and the composition and age of its stars.

UGC 4879 is an isolated dwarf galaxy, lying just beyond our own Local Group of galaxies some four million light-years away. Because of its isolation, astronomers are studying UGC 4879 to determine if it is a relatively undisturbed, old galaxy. Theories suggest that the lowest mass dwarf galaxies may have been the first galaxies to form. If UGC 4879 is a relic of the early universe, it could provide clues to the hierarchical structure and evolution of galaxies, galaxy clusters, and even the universe itself.

The image combines data from two Hubble observing programs, both focused on learning more about dwarf galaxies: how they form and evolve.