The Subtle Unstructured Beauty of Galaxy ESO 245-5 in Phoenix | Hubble

The Subtle Unstructured Beauty of Galaxy ESO 245-5 in Phoenix | Hubble

This image shows a densely packed field of stars, laid on top of a background of dust, gas, and light from more distant celestial objects. The stars take up so much of the field of view in this image that it is a little tricky to discern that you are in fact looking at most of a galaxy, known as ESO 245-5. This galaxy is a relatively close neighbor of the Milky Way, lying at the fairly modest distance of 15 million light-years from Earth in the constellation Phoenix. 

Another reason that it is perhaps a little tricky to spot that ESO 245-5 is a galaxy is its apparent lack of structure. Hubble images of spiral galaxies are interesting to look at in part because of their seemingly extraordinarily ordered arms of stars, gas and dust. ESO 245-5, in contrast, is classified as an IB(s)m type galaxy under the system of galaxy classification known as the De Vaucouleurs system. The IB(s)m designation specifically means that the galaxy is irregular (I), barred (B), has a slight spiral structure ((s)), and is of the Magellanic type (m).

Irregular in this context is quite intuitive. The galaxy does not appear to have a regular, ordered structure. In fact, essentially the entire view here is covered by the stars of this galaxy. The second term means that the galaxy has a barred shape at its center. This is the dense stretch of stars that crosses through the center of this image. The third term says that there are hints of a spiral structure, but nothing clear or definitive (hence the ‘s’ is bracketed). Finally, the last term indicates ESO 245-5’s similarity to the Magellanic Clouds—two dwarf galaxies that are close neighbors of the Milky Way. 

Image Description: An irregular galaxy: a cloud of tiny, point-like stars on a dark background. The cloud is densest along a broad, curved band across the center of the image, colored a faint blue with glowing purplish patches, and the stars grow more dense out to the edges but don’t fully vanish. A few distant background galaxies appear among the stars as glowing spots.

Credit: ESA/Hubble & NASA, M. Messa

Release Date: Feb. 5, 2024

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