Straight Friend Groups Be Like: *blonde Girl* *chad* *the Funny One* *kyle* *brunette Girl* *frat Boy*

straight friend groups be like: *blonde girl* *chad* *the funny one* *kyle* *brunette girl* *frat boy*

gay friend groups be like: *catboy* *suicidal mentor figure* *a walking nervous breakdown* *murderous trans guy* *sadistic traumatized doctor* *killed 35 people* *autistic detective* *kenji*

More Posts from Selenesparis and Others

4 years ago

They say the loveliest angels make the cruelest demons, and my darling

They Say The Loveliest Angels Make The Cruelest Demons, And My Darling
They Say The Loveliest Angels Make The Cruelest Demons, And My Darling

You were so beautiful

Before they dragged you into hell.

3 months ago
Happy Valumtimes!

Happy Valumtimes!

7 months ago

Part of why you are lovable is because you're nonbinary.

Your perspectives, particular style, the way you carry yourself, and more are what draw people to you.

Being nonbinary touches on everything you do, and it's a quality to be proud of.

10 months ago

Retrogression by Dazai Osamu is the #1 New Release in Japanese Literature!

Retrogression By Dazai Osamu Is The #1 New Release In Japanese Literature!

"This book aims to piece together the fractured and disorderly lifestyle of one of history's greatest romantics and pairs it with a particular moment in his life; losing the Akutagawa Prize. The ensuing drama that unfolded through private letters, newspaper articles, diaries, obituaries, and fiction created a scandal that disturbed the early Showa literati with its coarse and indecent honesty. Dazai's fiction, fiction about Dazai, speculation and reality intertwined to create an explosive event that not only changed the desired trajectory of his life but also raised issues of discrimination within prominent literary circles and the treatment of mental illness in 1930s Japan." - From the Introduction by translator A. L. Raye

Retrogression also includes annotations and background information on every story, letter, diary, and eulogy, adding history and insights that are difficult to find available in other English translations so far.

You can find more information and free translations on Yobanashi Café. Retrogression is available for purchase in either paperback or eBook format on Amazon.

7 months ago

the idealized version of my tomorrow self will fix this

9 months ago
Voices Of The Past By Ly Ber
Voices Of The Past By Ly Ber
Voices Of The Past By Ly Ber

Voices of the Past by Ly Ber

4 years ago

Black holes

A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light—can escape from inside it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which no escape is possible is called the event horizon. Although the event horizon has an enormous effect on the fate and circumstances of an object crossing it, no locally detectable features appear to be observed. In many ways a black hole acts like an ideal black body, as it reflects no light.  

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The idea of a body so massive that even light could not escape was briefly proposed by astronomical pioneer and English clergyman John Michell in a letter published in November 1784. Michell’s simplistic calculations assumed that such a body might have the same density as the Sun, and concluded that such a body would form when a star’s diameter exceeds the Sun’s by a factor of 500, and the surface escape velocity exceeds the usual speed of light.

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At the center of a black hole, as described by general relativity, lies a gravitational singularity, a region where the spacetime curvature becomes infinite. For a non-rotating black hole, this region takes the shape of a single point and for a rotating black hole, it is smeared out to form a ring singularity that lies in the plane of rotation. In both cases, the singular region has zero volume. It can also be shown that the singular region contains all the mass of the black hole solution. The singular region can thus be thought of as having infinite density. 

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How Do Black Holes Form?

Scientists think the smallest black holes formed when the universe began.

Stellar black holes are made when the center of a very big star falls in upon itself, or collapses. When this happens, it causes a supernova. A supernova is an exploding star that blasts part of the star into space.

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Scientists think supermassive black holes were made at the same time as the galaxy they are in.

Supermassive black holes, which can have a mass equivalent to billions of suns, likely exist in the centers of most galaxies, including our own galaxy, the Milky Way. We don’t know exactly how supermassive black holes form, but it’s likely that they’re a byproduct of galaxy formation. Because of their location in the centers of galaxies, close to many tightly packed stars and gas clouds, supermassive black holes continue to grow on a steady diet of matter.

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If Black Holes Are “Black,” How Do Scientists Know They Are There?

A black hole can not be seen because strong gravity pulls all of the light into the middle of the black hole. But scientists can see how the strong gravity affects the stars and gas around the black hole. 

Scientists can study stars to find out if they are flying around, or orbiting, a black hole.

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When a black hole and a star are close together, high-energy light is made. This kind of light can not be seen with human eyes. Scientists use satellites and telescopes in space to see the high-energy light.

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On 11 February 2016, the LIGO collaboration announced the first observation of gravitational waves; because these waves were generated from a black hole merger it was the first ever direct detection of a binary black hole merger. On 15 June 2016, a second detection of a gravitational wave event from colliding black holes was announced. 

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Simulation of gravitational lensing by a black hole, which distorts the image of a galaxy in the background 

Animated simulation of gravitational lensing caused by a black hole going past a background galaxy. A secondary image of the galaxy can be seen within the black hole Einstein ring on the opposite direction of that of the galaxy. The secondary image grows (remaining within the Einstein ring) as the primary image approaches the black hole. The surface brightness of the two images remains constant, but their angular size varies, hence producing an amplification of the galaxy luminosity as seen from a distant observer. The maximum amplification occurs when the background galaxy (or in the present case a bright part of it) is exactly behind the black hole.

Could a Black Hole Destroy Earth?

Black holes do not go around in space eating stars, moons and planets. Earth will not fall into a black hole because no black hole is close enough to the solar system for Earth to do that.

image

Even if a black hole the same mass as the sun were to take the place of the sun, Earth still would not fall in. The black hole would have the same gravity as the sun. Earth and the other planets would orbit the black hole as they orbit the sun now.

The sun will never turn into a black hole. The sun is not a big enough star to make a black hole.

More posts about black holes

Source 1, 2 & 3

2 years ago

love the word "methinks". like lol. yeah. me sure is thinksing.

7 months ago
Dragon Boat Festival By Lei Min
Dragon Boat Festival By Lei Min
Dragon Boat Festival By Lei Min
Dragon Boat Festival By Lei Min
Dragon Boat Festival By Lei Min
Dragon Boat Festival By Lei Min
Dragon Boat Festival By Lei Min
Dragon Boat Festival By Lei Min

Dragon Boat Festival by lei min

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selenesparis - selene's paris
selene's paris

/ walking on glass /

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