Pillars in the Carina Nebula (HH901)

  • Released Wednesday, April 11, 2018

Herbig Haro 901 is an immense pillar of gas and dust inside the Carina Nebula, a huge star-forming region in our galaxy. The pillar is several light-years tall and contains a few massive young stars. They shoot out powerful jets that emerge from the cloud. In some cases, the jets create bow-shock patterns similar to the effects of a ship plowing through the ocean. In the visible-light (Hubble) view, very few stars can be seen because the gas and dust block starlight. But in the infrared (Hubble) view, stars become visible and numerous. The visible-light colors emerge from the glow of different gases: oxygen (blue), hydrogen/nitrogen (green), and sulfur (red). The Carina Nebula is approximately 7,500 light years from Earth.



Credits

Please give credit for this item to:

Video: NASA, ESA and G. Bacon (STScI) Image: NASA, ESA,and the Hubble 20th Anniversary Team (STScI)

Release date

This page was originally published on Wednesday, April 11, 2018.
This page was last updated on Friday, August 2, 2024 at 4:26 PM EDT.


Missions

This page is related to the following missions:

Datasets used

Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.