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Hubble sees a glowing jet from a young star

Date:
February 24, 2013
Source:
NASA
Summary:
The Hubble Space Telescope has captured a new image showing an object known as HH 151, a bright jet of glowing material trailed by an intricate, orange-hued plume of gas and dust.

HH 151.
Credit: ESA/Hubble & NASA

The Hubble Space Telescope has captured a new image showing an object known as HH 151, a bright jet of glowing material trailed by an intricate, orange-hued plume of gas and dust.

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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.


Story Source:

The above story is based on materials provided by NASA. Note: Materials may be edited for content and length.


Cite This Page:

NASA. "Hubble sees a glowing jet from a young star." ScienceDaily. ScienceDaily, 24 February 2013. <www.sciencedaily.com/releases/2013/02/130224082136.htm>.
NASA. (2013, February 24). Hubble sees a glowing jet from a young star. ScienceDaily. Retrieved January 31, 2015 from www.sciencedaily.com/releases/2013/02/130224082136.htm
NASA. "Hubble sees a glowing jet from a young star." ScienceDaily. www.sciencedaily.com/releases/2013/02/130224082136.htm (accessed January 31, 2015).

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