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https://spacescoop.org/en/scoops/2125/this-one-winged-cosmic-butterfly-holds-a-baby-star/
Link to the original article & photo: https://noirlab.edu/public/news/noirlab2129/
The nebula has its beautiful wing-like shape because its central star emits infrared and visible light that escapes the tunnel inside the cloud and scatters off its walls.
There’s a bright red smear on the right, close to the center.
It’s one of what astronomers call the Herbig-Haro, or HH objects, bright areas of nebulosity commonly found near newborn stars like we have here.
They form when fast-moving gas thrown out by stars smashes into slower-moving gas that’s part of the ISM, the interstellar medium of gas and dust.
We've added a new way to donate to 365 Days of Astronomy to support editing, hosting, and production costs.
Just visit: https://www.patreon.com/365DaysOfAstronomy and donate as much as you can!
Share the podcast with your friends and send the Patreon link to them too!
Every bit helps! Thank you!
------------------------------------
Do go visit http://www.redbubble.com/people/CosmoQuestX/shop for cool Astronomy Cast and CosmoQuest t-shirts, coffee mugs and other awesomeness!
http://cosmoquest.org/Donate This show is made possible through your donations.
Thank you! (Haven't donated? It's not too late! Just click!)
------------------------------------
The 365 Days of Astronomy Podcast is produced by the Planetary Science Institute. http://www.psi.edu
Visit us on the web at 365DaysOfAstronomy.org or email us at [email protected].
4.4
329329 ratings
https://spacescoop.org/en/scoops/2125/this-one-winged-cosmic-butterfly-holds-a-baby-star/
Link to the original article & photo: https://noirlab.edu/public/news/noirlab2129/
The nebula has its beautiful wing-like shape because its central star emits infrared and visible light that escapes the tunnel inside the cloud and scatters off its walls.
There’s a bright red smear on the right, close to the center.
It’s one of what astronomers call the Herbig-Haro, or HH objects, bright areas of nebulosity commonly found near newborn stars like we have here.
They form when fast-moving gas thrown out by stars smashes into slower-moving gas that’s part of the ISM, the interstellar medium of gas and dust.
We've added a new way to donate to 365 Days of Astronomy to support editing, hosting, and production costs.
Just visit: https://www.patreon.com/365DaysOfAstronomy and donate as much as you can!
Share the podcast with your friends and send the Patreon link to them too!
Every bit helps! Thank you!
------------------------------------
Do go visit http://www.redbubble.com/people/CosmoQuestX/shop for cool Astronomy Cast and CosmoQuest t-shirts, coffee mugs and other awesomeness!
http://cosmoquest.org/Donate This show is made possible through your donations.
Thank you! (Haven't donated? It's not too late! Just click!)
------------------------------------
The 365 Days of Astronomy Podcast is produced by the Planetary Science Institute. http://www.psi.edu
Visit us on the web at 365DaysOfAstronomy.org or email us at [email protected].
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