Art

[rarararar]

I just want to say, your art is gorgeous!!! I hope you can get plenty of financial help!

Thank you so much!!!! :’)!!!!! In this trying time, I appreciate kind words from kind turtles!

[stylebythemodels]

[omgthatdress]

Jacket

1928

Kerry Taylor Auctions

[stylebythemodels]

[modelsoffthecatwalk]

[stimful-gifts]

View this post on Instagram

[geniusoflove]

this is the most dramatic video I’ve ever seen

[huskyvagina-deactivated20210528]

I’m gagging…

[wiiiine]

I thought the caption was an exaggeration but it’s not

[fashionsfromhistory]

Boots

Jerry Edouard

c.1975

The MET

[monsieur-j]

Christopher Kane S/S 2018 Runway Details

[lefuckinsoleil]

A dress revealing your butt or boobs is nothing compared to a dress revealing THE INNER VOID™.

[hoopyfrood]

@thingstaakowouldwear

[glitter-skank]

[lescretia]

@thingstaakowouldwear

[stylebythemodels]

[monsieur-j]

On-Off S/S 2018 Runway Details

[stylebythemodels]

[vetyr]

Witch of changing skies

[rarararar]

[wonders-of-the-cosmos]

The material around SN 1987A (artist’s impression)

This artist’s impression of the material around a recently exploded star, known as Supernova 1987A (or SN 1987A), is based on observations which have for the first time revealed a three dimensional view of the distribution of the expelled material. The observations were made by astronomers using ESO’s Very Large Telescope. The original blast was not only powerful, according to the new results. It was also more concentrated in one particular direction. This is a strong indication that the supernova must have been very turbulent, supporting the most recent computer models. This video shows the different elements present in SN 1987A: two outer rings, one inner ring and the deformed, innermost expelled material.

Just how a supernova explodes is not very well understood, but the way the star exploded is imprinted on this inner material. The astronomers could deduce that this material was not ejected symmetrically in all directions, but rather seems to have had a preferred direction. Besides, this direction is different to what was expected from the position of the rings.

Credit: ESO/L. Calçada

[wonders-of-the-cosmos]

NGC 6888: The Crescent Nebula

NGC 6888, also known as the Crescent Nebula, is a cosmic bubble about 25 light-years across, blown by winds from its central, bright, massive star. This sharp telescopic portrait uses narrow band image data that isolates light from hydrogen and oxygen atoms in the wind-blown nebula. The oxygen atoms produce the blue-green hue that seems to enshroud the detailed folds and filaments. Visible within the nebula, NGC 6888’s central star is classified as a Wolf-Rayet star (WR 136). The star is shedding its outer envelope in a strong stellar wind, ejecting the equivalent of the Sun’s mass every 10,000 years. The nebula’s complex structures are likely the result of this strong wind interacting with material ejected in an earlier phase. Burning fuel at a prodigious rate and near the end of its stellar life this star should ultimately go out with a bang in a spectacular supernova explosion. Found in the nebula rich constellation Cygnus, NGC 6888 is about 5,000 light-years away.

Image Credit: Michael Miller & Jimmy Walker

[xohighglo]

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