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Explanation: Some features of HH-34 are understood -- some are not. At the core of Herbig-Haro 34 lies a seemingly typical young star. This star, though, somehow ejects energetic "bullets" of high-energy particles, appearing as red streaks toward the lower right of the this image. Astronomers speculate that a burst of these particles might rebound when gas from a disk surrounding the star momentarily collapses onto the star. Visible near the end of each light-year long jet is a glowing cap. HH-34 lies about 1500 light-years away in the Orion Nebula star-forming region. The cause of the large arc of gas on the upper left known as the waterfall remains unexplained.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: Orion - jet - arcs - star formation
Publications with words: Orion - jet - arcs - star formation
See also:
- APOD: 2025 April 9 Á HH 49: Interstellar Jet from Webb
- APOD: 2025 March 26 Á Star Formation in the Pacman Nebula
- A December Winter Night
- APOD: 2024 October 22 Á M16: Pillars of Star Creation
- APOD: 2024 October 1 Á Porphyrion: The Longest Known Black Hole Jets
- Star Factory Messier 17
- APOD: 2024 August 19 Á IC 5146: The Cocoon Nebula