Science & Technology

Hubble Spots an Astronomical Intruder in a Distant Galaxy

This Hubble Space Telescope image includes a host of astronomical objects. Strewn across the image are background galaxies ranging from stately spirals to fuzzy ellipticals. Also present are bright foreground stars much closer to Earth, surrounded by diffraction spikes. In the center of the frame, the faint outline of the tiny galaxy UGC 7983 can be seen as a blurry cloud of light. But hidden within this image lies an unexpected cosmic intruder. Credit: ESA/Hubble & NASA, R. Tully

A host of astronomical objects throng this image from the Hubble Space Telescope. Background galaxies ranging from stately spirals to fuzzy ellipticals are strewn across the image, and bright foreground stars much closer to home are also present, surrounded by diffraction spikes. In the center of the image, the vague shape of the small galaxy UGC 7983 appears as a hazy cloud of light. UGC 7983 is around 30 million light-years from Earth in the constellation Virgo, and is a dwarf irregular galaxy — a type thought to be similar to the very earliest galaxies in the Universe.

This image also conceals an astronomical interloper. A minor asteroid, only a handful of kilometers across, can be seen streaking across the upper left-hand side of this image. The trail of the asteroid is visible as four streaks of light separated by small gaps. These streaks of light represent the four separate exposures that were combined to create this image, the small gaps between each observation being necessary to change the filters inside NASA/ESA Hubble’s Advanced Camera for Surveys (ACS).

Capturing an asteroid was a fortunate side effect of a larger effort to observe every known galaxy close to the Milky Way. When this project was first proposed, roughly 75% of all the Milky Way’s near galactic neighbors had been imaged by Hubble. A group of astronomers proposed using the gaps between longer Hubble observations to capture images of the remaining 25%. The project was an elegantly efficient way to fill out some gaps not only in Hubble’s observing schedule, but also in our knowledge of nearby galaxies.

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