HH 212
![]() Image of HH 212 using NIRCAM | |
Object type | Herbig-Haro |
---|---|
Other designations | MHO 499, HH 212 |
Observation data (Epoch J2000) | |
Constellation | Orion |
5 43 50.64 | |
Declination | -1° 3' 11.46" |
Distance | 1,400 ly |
Estimated age | 7000 yr |
Notable features | Symmetrical jets |
HH 212 is a Herbig–Haro object (HH) located roughly 1,400 light years from Earth in the constellation of Orion[1], not far from the Horsehead nebula. The protostar, which is embedded deep into the center of HH 212 is very young, only being a few thousand years old (probably around ~7000 years old). It is emitting prominent jets which show remarkable symmetry. The high speeds of these jets also create bowshocks.[2][3]
Jets
The protostar (IRAS 05413–0104) is emitting large bipolar jets traveling at speeds of 170 kilometers per second. These jets show a remarkably symmetric appearance. There appear to be several symmetrical knots appearing on either side of the jet at relatively stable intervals, (roughly 0.01 parsecs) suggesting that it varies regularly over a short timescale of just 30 years.[2][4] The fast speeds of the jet rams into the interstellar medium creating two main bowshocks. They are located north and south of the jets symmetrically.
References
- ^ "Herbig-Haro 212 (VLT)". Webb. Retrieved 2025-08-07.
- ^ a b information@eso.org. "Outbursts from a newborn star". www.eso.org. Retrieved 2025-08-07.
- ^ Reipurth, Bo; Davis, C. J.; Bally, John; Raga, A. C.; Bowler, B. P.; Geballe, T. R.; Aspin, Colin; Chiang, Hsin-Fang (2019-08-12). "The Giant Herbig–Haro Flow HH 212 and Associated Star Formation". The Astronomical Journal. 158 (3): 107. arXiv:1911.05877. Bibcode:2019AJ....158..107R. doi:10.3847/1538-3881/ab2d25. ISSN 1538-3881.
- ^ Zinnecker, H.; McCaughrean, M. J.; Rayner, J. (1996). HH 212: The Most Beautiful Protostellar Jet Known to Date. Lecture Notes in Physics. Vol. 465. pp. 236–245. Bibcode:1996LNP...465..236Z. doi:10.1007/BFb0102641. ISBN 978-3-540-61389-3. ISSN 0075-8450.
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