#astronomy #stars #WolfRayetStar #WR124 #JWST

An image captured by the James Webb Space Telescope shows the star WR 124 and the surrounding nebula in never-before-seen detail. This is a case where a star is nearing the end of its life, which could culminate in a supernova.

https://english.tachyonbeam.com/2023/03/21/the-star-wr-124-is-a-rare-type-of-candidate-to-die-in-a-supernova/

The star WR 124 is a rare type of candidate to die in a supernova

An image captured by the James Webb Space Telescope shows the star WR 124 and the surrounding nebula in never-before-seen detail. This is a case where a star...

Since JWST dropped a picture of WR 124 recently, I think it's time to repost my little painting of WR 124 as seen by Hubble
I'll need to paint the JWST version! ☺️

#Astrodon #WR124 #JWST #Art #Mastoart #SpaceArt #SciArt #Astronomy #AcrylicPainting #Acrylics #Hubble #WolfRayetStar

This study from 2012, using 24 µm data from Spitzer, revealed that the ionized gas of nebula M1-67 ejected by WR 124 is condensed in knots aligned in a preferred axis along the NE-SW direction, with “holes” along the perpendicular direction.

The sketch below illustrates the (proposed) structure as an inner region with bipolar or elliptical shape along the direction NE−SW surrounded by an external spherical bubble.

https://www.aanda.org/articles/aa/pdf/2013/06/aa20773-12.pdf
#JWST #WR124 #WolfRayet
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When #WR124 does go #supernova will it be visible to the naked eye? #astrophysics #astronomy
Wolf–Rayet stars are massive luminous hot stars that have lost their outer hydrogen and are fusing helium and heavier elements in the core.
WR 124:
Distance: 15,000 ly
Location: Milky Way Galaxy, in the constellation Sagittarius.
Discovered by : Paul W. Merrill in 1938.
Mass: 30x solar mass ☉; has shed 10☉ worth of material so far.
Nebula size: 6 ly
Temp: 44,700 K
Elements: 15% hydrogen, rest is mainly helium.
Age: just 8.6 Myr
https://en.wikipedia.org/wiki/WR_124
https://arxiv.org/pdf/1602.03422.pdf
#JWST #WR124
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WR 124 - Wikipedia

This image of the Wolf-Rayet star WR 124 and Nebula M1-67 was released by the JWST team today at #SXSW. The image was taken using the NIRCam and MIRI instruments in June 2022.
The 2nd image was taken by Hubble in 1998 and re-processed in 2015 by @spacegeck.
The massive young hot star is expelling star-stuff at ~200 km/s into the surrounding nebula.
It will explode as a type Ib or Ic supernova in a few 100,000 years.
https://esawebb.org/news/weic2307/
https://esahubble.org/images/potw1533a/
#JWST #WR124 #WolfRayet
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Webb captures rarely seen prelude to a supernova

A Wolf-Rayet star is a rare prelude to the famous final act of a massive star: the supernova. As one of its first observations in 2022, the NASA/ESA/CSA James Webb Space Telescope captured the Wolf-Rayet star WR 124 in unprecedented detail. A distinctive halo of gas and dust frames the star and glows in the infrared light detected by Webb, displaying knotty structure and a history of episodic ejections. Despite being the scene of an impending stellar ‘death’, astronomers also look to Wolf-Rayet stars for insight into new beginnings. Cosmic dust is forming in the turbulent nebulas surrounding these stars, dust that is composed of the heavy-element building blocks of the modern Universe, including life on Earth.

www.esawebb.org