Turbulence in a Star Forming Region

The nebula’s sparkling centerpiece is a giant, young star cluster named NGC 2070, only 2 million years old. Its stellar inhabitants number roughly 500,000. The cluster is a hotbed for young, massive stars. The cluster’s dense core, known as R136, is packed with some of the heftiest stars found in the nearby universe.

The cluster’s core is home to more than 10,000 stars. Several of them may be over 100 times more massive than our Sun. These hefty stars are destined to pop off, like a string of firecrackers, as supernovas in a few million years. Only two or three of the hottest stars in R136 are providing 50 percent of the radiation in the cluster.

30 Doradus is the brightest, nearby star-forming region and home to the most massive stars in our cosmic neighborhood of about 25 galaxies. The nebula is close enough to Earth that Hubble can resolve individual stars, giving astronomers important information about the stars’ birth and evolution. 30 Doradus resides 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way.

Credit: NASA, ESA

A Mosaic of the Tarantula Nebula

"The Tarantula Nebula (also known as 30 Doradus, or NGC 2070) is an H II region in the Large Magellanic Cloud (LMC). It was originally thought to be a star, but in 1751 Nicolas Louis de Lacaille recognized its nebular nature.

The Tarantula Nebula has an apparent magnitude of 8. Considering its distance of about 49 kpc (160,000 light-years), this is an extremely luminous non-stellar object. Its luminosity is so great that if it were as close to Earth as the Orion Nebula, the Tarantula Nebula would cast shadows. In fact, it is the most active starburst region known in the Local Group of galaxies. It is also one of the largest such region in the Local Group with an estimated diameter of 200 pc. The nebula resides on the leading edge of the LMC, where ram pressure stripping, and the compression of the interstellar medium likely resulting from this, is at a maximum. At its core lies the compact star cluster R136 (approximate diameter 35 light years) that produces most of the energy that makes the nebula visible. The estimated mass of the cluster is 450,000 solar masses, suggesting it will likely become a globular cluster in the future.”

Credit: Mazlin from starshadows.com/Wikipedia

8: Sexual orientation? Straight

19: What am I listening to right now? The silence of my room at 2:45am

35: Favorite holiday. Canada Day. I’m not Canadian but like… It’s nice to see people be happy and celebrate where they come from.

49: Am I excited for anything? FIELD SHOW PRACTICE IN 12 HOURS AND 48 MINUTES!!!!!!!!!

53: What if the last person I kissed was kissing someone else right in front of me? I’ve never romantically kissed someone but if I did and this happened I’d be a little upset.

57: What do I think about most? I never stop thinking about how one day my best friend won’t be alive and I just pray it isn’t anytime soon.

64: Do I believe in magic? I don’t believe in magic in the sense of pulling rabbits out of a hat but I do believe there’s this type of magic that flows in everyone that allows us all to find happiness some how.

81: My top 5 blogs on tumblr? I love all the blogs I follow and that follow me. The ones I check daily however are: lukesintodrummers, 5sos-official, mpregashton, whereshiphappens, and psychedelichemmo

149: What my greatest achievements are. My greatest achievement was being voted to be the Princess of Big Island for mayday at my school. It was the one day where I can honestly I was happy the entire time.

The Tarantula Nebula

Located inside the Large Magellanic Cloud (LMC) – one of our closest galaxies – in what some describe as a frightening sight, the Tarantula nebula is worth looking at in detail. Also known as 30 Doradus or NGC 2070, the nebula owes its name to the arrangement of its bright patches that somewhat resemble the legs of a tarantula. Taking the name of one of the biggest spiders on Earth is very fitting in view of the gigantic proportions of this celestial nebula — it measures nearly 1,000 light years across ! Its proximity, the favourable inclination of the LMC, and the absence of intervening dust make this nebula one of the best laboratories to better understand the formation of massive stars. This spectacular nebula is energised by an exceptionally high concentration of massive stars, often referred to as super star clusters. This image is based on data acquired with the 1.5 m Danish telescope at the ESO La Silla Observatory in Chile, through three filters (B: 80 s, V: 60 s, R: 50 s).

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Credit: ESO

NGC2070 by cosmicphotos on Flickr.

Via Flickr:
Discovered by Nicolas Louis de Lacaille in 1751, the Tarantula nebula (aka NGC 2070) is a bright HII region located in the southern constellation of Dorado. The spider shaped structure is fuelled by the brightest and most prolific star-forming region in our galactic neighbourhood, known as 30 Doradus. 30 Doradus is home to several million young stars, among which live the most massive stars ever seen. The nebula resides 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way.

Image is a HaOIII+RGB composite.

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