Drama plays out in deep space as a small fish swims from the jaws of a larger creature.
Herbig-Haro 32 formed when the young central stars ejected jets of material out into space. Most of the dust in this NASA Hubble Space Telescope image has been cleared away but some gas is attracted to the central stars by gravity. This material slowly spirals into the star. Most of the material will accrete onto the star adding to the mass. The rest of the material is ejected at the poles of the star to form two jets, one pointing over the top of the star and another pointing down. These jets plow into quiet surrounding nebula at high speed causing the gas to glow. This glow is called a Herbig-Haro object. Astronomers George Herbig and Guillermo Haro studied and described these objects in the 1950s.
Explore the image and find the two greenish jets. Imagine the top jet is tilted slightly toward Earth. It is brighter and larger. The small jet at the bottom is located on the far side of the central star. Gas and dust between the jet and Earth block the light and make it slightly redder and dimmer.
HH 32 is located about 1,000 light-years from Earth toward the constellation of Aquila, the Eagle. Aquila is a bright summer constellation in the northern hemisphere. The constellation is ancient, being one of the 48 constellations described by Ptolemy in the 2nd century.
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