This image shows an object known as HH 151, a bright jet of glowing material
trailed by an intricate, orange-hued plume of gas and dust. It is located some
460 light-years away in the constellation of Taurus (The Bull), near to the
young, tumultuous star HL Tau.
In the first few hundred thousand years of
life, new stars like HL Tau pull in material that falls towards them from the
surrounding space. This material forms a hot disc that swirls around the
coalescing body, launching narrow streams of material from its poles. These jets
are shot out at speeds of several hundred kilometers (or miles) per second and
collide violently with nearby clumps of dust and gas, creating wispy, billowing
structures known as Herbig-Haro objects — like HH 151 seen in the
image.
Such objects are very common in star-forming regions. They are
short-lived, and their motion and evolution can actually be seen over very short
timescales, on the order of years. They quickly race away from the newly-forming
star that emitted them, colliding with new clumps of material and glowing
brightly before fading away.
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