49 posts
š¤ Before And After I Manifested Pale Skin š¤
Hello everyone š„°š„°š¦š¦ Here is my skin before I started to manifest pale skin, it was already a light color but I wanted that white as paper vampire look
And this is my skin today ššš¤š¤
Itās so white I look like a vampire in person and I really love mannequins so I wanted to look like one! Iām so happy :,) š¤š¤š¤ All I did was listen to pale skin subliminals once a day for 3 weeks and every time I thought about my skin I told myself āmy skin is so white it makes paper jealousā āmy skin is so white I look like a mannequinā and I continued to think this way even when I saw zero changes in reality š¤š¤š¤ And three weeks later I look like this !! ššš¤š¤ Here is video evidence and if anyone wants the subliminals I listened to just let me know š„°š„°š¤š¤
Before āļøš¦āļø After āļøš©øāļø
Please, please read.
3 years ago I wrote a very personal prose piece titled The Morning After I Killed Myself, about a young woman who commits suicide and looks back on the impact it has on her family and friends and ends up regretting her decision. I posted it on my writing blog 3 years ago and it went viral, shared over 300,000 times on my blog and almost a million times on Imgur/Reddit.Ā
So many people have told me itās saved their lives.
But I almost wish I hadnāt written it. Because, despite all the good it managed to do, itās been plagiarized over a hundred times, probably several hundred. Iāve seen dozens of cases of it being stolen and retitled with someone elseās name as the author, cases of it being published in someone elseās book under their name, cases of it being used as song lyrics by a band who claims they wrote it, cases of it being posted nearly ten times on the same website alone and because the website is so enormous they didnāt catch each instance of plagiarismā¦
Once a girl based her senior art thesis off of my pieceā¦only she accidentally based it off of a plagiarized version of my piece and had no idea. She called me, a complete stranger, in tears, begging me to forgive her for something that was not her fault at all, but the fault of the person who plagiarized me. She had to redo portions of the thesis she worked so hard on.
Iāve had cases of it being submitted to writing contests under other peoplesā names and them winning awards for it. One girl submitted it to the Scholastic Art and Writing Awards and won a gold key for it, coincidentally the same contest I submitted some of my work to in high school and won awards for. What was her excuse? She said she read the piece awhile ago, liked it so much that she saved it to her computer, and when the time came to submit to the contest, she āforgot she hadnāt written itā and sent it in under her name.
I had a case of a stranger who posted it on their blog under their name and when I asked them, politely, to provide me with credit and remove their name, they claimed theyād āwritten the piece 10 years ago in their private journal and that I was the one who plagiarized them.ā
Iāve had cases of people messaging my writing blog and accusing me of plagiarismā¦of my own piece, because they saw plagiarized versions of it going viral and had no idea I was the original author.
And finally, a few weeks ago, a girl submitted it to a contest under her name and won $100 for it. Now sheās apparently denying plagiarism.
This piece of mine was intended to help people. Itās a very very personal piece and always will be. Iām glad itās helped so many people. But something that is so personal and painful for me has been twisted and manipulated and stolen and published for profit and taken away from me so many times Iāve lost count. I donāt care about money. But when I saw this girl win $100 for a piece about suicide that I wrote, that is the last straw.
Please, for the love of god, donāt steal from artists and writers. Donāt steal something and claim you wrote it. Write and create your own work. If you see a piece of art or writing floating around with no source or a mis-attributed source, tell the original author. Spread the word. Donāt share artworks without sources on them.Ā
You might think that itās not a big deal, that it doesnāt matter, that it only happened once.
But it happens all the time. All the time. This is exhausting and artists deserve credit. They deserve respect.
Iāve considered deleting the writing blog Iāve had for 5 years because of how often this piece is plagiarized.
Donāt let it get to that point, where someone considers getting rid of something they love because itās hardly theirs anymore.
Thanks for reading.
I would embrace them.
Read this craigslist ad for a 1999 toyota corolla.
i wonder if its like this bc itās showing you how no curves would look
Fuck Rick & Morty.
but the thing is, who tf calls macaroni and cheese āmacā?
Is macaroni and cheese āmacā because its short for macaroni⦠or because āmacā is an acronym for macaroni and cheese
Shoutout to the male rape victims that suffer in silence out of fear of embarrassment or feeling publicly emasculated. Your pain is valid. Your trauma is valid. Your trust issues are valid. Your emotions are valid. They do not emasculate you. You are still strong. You are always going to be strong. And your story matters.
This is the Goose of Outrageous Self Assuredness.Ā Take from her example, her ludicrous and excellent poise in the face of bullying, and be confident in your place, your course, your equal validity.
track art for new song āFor Fā by LLLL, featuring Meishi Smile and Calendula
Collaboration with Brenden Savi @savicorp
Released on Zoom Lens
listen to the track hereĀ !
instagram: @abi_laurel
made this recently and ended up not using it! if anyone wants it for track/album art iāll sell it for $35 (originally a $200 value) ;)Ā
message if interested, paypal only
donāt delete caption
chinatown winter 2016
Is there anything more beautiful than women supporting women?
body: you are dying of The Heat
me: [removes blanket]
body: never have you been So Frozen
Can y'all please report this tumblr blog to the fbi: https://youngmomma371.tumblr.com/
She posts and reblogs pictures of girls in sexual poses and basically admitted to sexually abusing her daughters
@comrade-lecter @the-map-community-is-dangerous @block-report-program @report-a-predator @anti-pedo-patrol
ā wander around barefoot, especially in the grass (please be cautious though!)
ā sip some tea and admire little details about your surroundings ā i promise you thereās always something to enjoy even when it doesnāt seem like it
ā take a shower and sing out loud until all your bad thoughts flutter away
ā blow dandelion seeds
ā Ā go for a long walk and collect things that fascinate you along the way, whether it be an old coin, feathers, flowers or lost trinkets. start a collection.
ā sit in your natural state, learn to love your naked body with no make-up, nail polish, and your hair down.
ā smile at yourself in the mirror
ā play some instrumental or classical music (suggestion: yayo instrumental by lana del rey, itās magical)
ā sprinkle a little glitter in your hair, in a bath, or in dull areas of your room
ā doodle things a fairy would see in their day to day lives, berries, flowers, leaves, creatures, butterflies, etc
ā spend time with an animal friend, have a conversation with them
ā wear your favourite dress casually, donāt be afraid to leave the house in it
ā wear flowers in your hair around the house
ā coat your lips in honey
ā buy plenty of fresh fruit (especially berries) and enjoy
ā³ i hope this inspires you to take care of yourself. requests on habits & tips (or more) are greatly appreciated!
Iāve been staring at this for five minutes wondering why the fuck im still on this site
Sink Hole.
| #GIF | #DAILY | #C4D |
photo: abi laurel
model: nicole ruggiero
makeup: dollfilleĀ
instagram: @abi_laurel
side blog: @turnt-shoujoā
Bastet
Interiors of various Luminaria, inflatable temporary structures by Architects of Air (1990-present)
Blue supergiant stars are hot luminous stars, referred to scientifically as OB supergiants. They have luminosity class I and spectral class B9 or earlier.
Blue supergiants (BSGs) are found towards the top left of the HertzsprungāRussell diagram to the right of the main sequence. They are larger than the Sun but smaller than a red supergiant, with surface temperatures of 10,000ā50,000 K and luminosities from about 10,000 to a million times the Sun.
Supergiants are evolved high-mass stars, larger and more luminous than main-sequence stars. O class and early B class stars with initial masses around 10-100 Mā evolve away from the main sequence in just a few million years as their hydrogen is consumed and heavy elements start to appear near the surface of the star. These stars usually become blue supergiants, although it is possible that some of them evolve directly to WolfāRayet stars.Ā
Expansion into the supergiant stage occurs when hydrogen in the core of the star is depleted and hydrogen shell burning starts, but it may also be caused as heavy elements are dredged up to the surface by convection and mass loss due to radiation pressure increase.
Blue supergiants are newly evolved from the main sequence, have extremely high luminosities, high mass loss rates, and are generally unstable. Many of them become luminous blue variables (LBVs) with episodes of extreme mass loss. Lower mass blue supergiants continue to expand until they become red supergiants. In the process they obviously must spend some time as yellow supergiants or yellow hypergiants, but this expansion occurs in just a few thousand years and so these stars are rare. Higher mass red supergiants blow away their outer atmospheres and evolve back to blue supergiants, and possibly onwards to WolfāRayet stars.Ā Depending on the exact mass and composition of a red supergiant, it can execute a number of blue loops before either exploding as a type II supernova or finally dumping enough of its outer layers to become a blue supergiant again, less luminous than the first time but more unstable.Ā If such a star can pass through the yellow evolutionary void it is expected that it becomes one of the lower luminosity LBVs.
The most massive blue supergiants are too luminous to retain an extensive atmosphere and they never expand into a red supergiant. The dividing line is approximately 40 Mā, although the coolest and largest red supergiants develop from stars with initial masses of 15-25 Mā. It isnāt clear whether more massive blue supergiants can lose enough mass to evolve safely into a comfortable old age as a Wolf Rayet star and finally a white dwarf, or they reach the Wolf Rayet stage and explode as supernovae, or they explode as supernovaeĀ while blue supergiants.
Because of their extreme masses they have relatively short lifespans and are mainly observed in young cosmic structures such as open clusters, the arms of spiral galaxies, and in irregular galaxies. They are rarely observed in spiral galaxy cores, elliptical galaxies, or globular clusters, most of which are believed to be composed of older stars, although the core of the Milky Way has recently been found to be home to several massive open clusters and associated young hot stars.
The best known example is Rigel, the brightest star in the constellation of Orion. Its mass is about 20 times that of the Sun, and its luminosity is around 117,000 times greater. Despite their rarity and their short lives they are heavily represented among the stars visible to the naked eye; their immense brightness is more than enough to compensate for their scarcity.
Blue supergiants have fast stellar winds and the most luminous, called hypergiants, have spectra dominated by emission lines that indicate strong continuum driven mass loss. Blue supergiants show varying quantities of heavy elements in their spectra, depending on their age and the efficiency with which the products of nucleosynthesis in the core are convected up to the surface. Quickly rotating supergiants can be highly mixed and show high proportions of helium and even heavier elements while still burning hydrogen at the core, and these stars show spectra very similar to a Wolf Rayet star.
While the stellar wind from a red supergiant is dense and slow, the wind from a blue supergiant is fast but sparse. When a red supergiant becomes a blue supergiant, the faster wind it produces impacts the already emitted slow wind and causes the outflowing material to condense into a thin shell. In some cases several concentric faint shells can be seen from successive episodes of mass loss, either previous blue loops from the red supergiant stage, or eruptions such as LBV outbursts.
Astronomers suggest that blue supergiant stars may be the most likely sources of ultra-long GRBs. These stars hold about 20 times the sunās mass and may reach sizes 1,000 times larger than the sun, making them nearly wide enough to span Jupiterās orbit.
Source
Rigel
Fourth image:Ā Hubble Space Telescope image of nebula M1-67 around WolfāRayet star WR 124. (source).
Fifth image:Ā Rigel and the IC 2118 nebula which it illuminates. (source).Ā Ā
Sixth image: Spectrum of a B2 star. (souce).
Seventh image: Star cluster NGC 3572 and its surroundings. (source).
Eighth image: Orion constellation (The star Rigel is at the top right of the image. by: Joseph Brimacombe)
images of star comparisons. (nasa).