© Eut.d

© Eut.d
© Eut.d

© eut.d

More Posts from Chewydrageee and Others

4 years ago

objection your honor if you don’t let me go to the bathroom right now we’re going to have a new piece of evidence in this court room

5 years ago
Ethereal
Ethereal
Ethereal
Ethereal

Ethereal

5 years ago

8216

OK new game. Use this website to see how common your first name is, and then put that number in the tags. 

5 years ago
♡
♡
♡

5 years ago
Something To Brighten Your Day.
Something To Brighten Your Day.
Something To Brighten Your Day.
Something To Brighten Your Day.
Something To Brighten Your Day.
Something To Brighten Your Day.
Something To Brighten Your Day.
Something To Brighten Your Day.
Something To Brighten Your Day.
Something To Brighten Your Day.

Something to brighten your day.

Please stay strong.

If you enjoy my art, please reblog and follow. I’ll keep doing my best.

5 years ago
Purple And Orange Really Look Beautiful Together I Haven’t Realized Till Now

Purple and orange really look beautiful together I haven’t realized till now


Tags
5 years ago

SHES BEAUTIFUL

Sparkling At The Centre Of This Beautiful NASA/ESA Hubble Space Telescope Image Is A Wolf–Rayet Star known

Sparkling at the centre of this beautiful NASA/ESA Hubble Space Telescope image is a Wolf–Rayet star known as WR 31a, located about 30 000 light-years away in the constellation of Carina (The Keel). The distinctive blue bubble appearing to encircle WR 31a, and its uncatalogued stellar sidekick, is a Wolf–Rayet nebula — an interstellar cloud of dust, hydrogen, helium and other gases. Created when speedy stellar winds interact with the outer layers of hydrogen ejected by Wolf–Rayet stars, these nebulae are frequently ring-shaped or spherical. The bubble — estimated to have formed around 20 000 years ago — is expanding at a rate of around 220 000 kilometres per hour!

Unfortunately, the lifecycle of a Wolf–Rayet star is only a few hundred thousand years — the blink of an eye in cosmic terms. Despite beginning life with a mass at least 20 times that of the Sun, Wolf–Rayet stars typically lose half their mass in less than 100 000 years. And WR 31a is no exception to this case. It will, therefore, eventually end its life as a spectacular supernova, and the stellar material expelled from its explosion will later nourish a new generation of stars and planets.

Credit: ESA/Hubble & NASA Acknowledgement: Judy Schmidt7l

#wolfrayetstar #estrela #star #space #espaço #astronomy #astronomia https://www.instagram.com/p/B2C1GtpJ1LC/?igshid=wys9sipew632

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chewydrageee - gwen 💌
gwen 💌

(^з^)-☆

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