lighting bending

3

Reference: Luke Skywalker

Model: Sara Jean Underwood

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Exquisite.

I drew my favorite fashion model, Symmetra.~ *throws sparkles* I wish she would get more legendary skins. OTL

You Who... [M] (ft. Jeongguk)

Drabble Game Prompt 96. “Here, let me.” with badboy/jock!jeongguk

→ badboy football jk (warning: overstimulation, cumplay, fluff, and fuckingjeonjungkook)
→ 1.4k words prequel part 01 | 02

A/N: i have no idea where this came from, my hand sort of slipped, jfc what have i done 

UPDATE: added the highly-requested prequel as a thank you for 1k+ notes :) make sure to check out Give and Take! It’s a similar AU to this one! 


“There you go, yes, you can do it babe,” Jeongguk encourages, as you bite down on your lip.  

He grins up at you as you move your hips slowly against his, finding the way you squeeze your eyes shut tightly the cutest thing ever. 

“J-jeongguk I-I can’t–” you stutter, arms clutching at his bare shoulders as your movements stutter and begin to slow down. But you whimper instead at the loss of friction between your legs and begin to cry tears of frustration as you don’t know whether to continue grinding against him and chase after another orgasm or to stop completely. 

He just laughs huskily from beneath you, and wipes a tear from your cheek and presses a quick peck to your chin as you make up your mind and your movements continue. His head dips down to press open-mouthed kisses against your collarbone, painting the skin there in blossoms of red and pink. “Shh,” he grates against your neck, a gentle hand coming up to stroke down your spine and settling on the curve of your hip to firmly help guide you up and down his cock. “you got this.” 

He’s in awe as he watches you desperately move against him, your soft breasts and nipples brushing up against his hard chest and melting him on the spot. It’s been years since he’s met you and only a few months since the both of you finally started having sex, but he’s secretly delighted at how sensitive you are and how desperate you are to pleasure the both of you. He wants to spread you out and fuck you with his fingers and tongue and make you cum over and over until you’re screaming hoarsely or tie you down onto the bed and tease you for hours until you’re begging for him, but he smiles as he relishes in actually convincing you to top him for once. 

Cause this time he’s being a little selfish and pushing the boundaries on how far he can take you because he’s currently coaxing your through your third orgasm and is harder than he’s ever been in his life as he watches you in tears because you’re desperate to reach the peak once again. 

You muffle your cries in in his neck and thread your fingers in his hair as you feel the wave approaching again. “Jeongguk, ‘m gonna come,” you murmur breathlessly, making his dick clench at how fucking submissive you sound to him right now. He whispers sooth encouragements into your ear and moves his hips up to meet yours just right and grazes the spot inside of you that has you cringing and sighing into his neck as he grunts when you clamp down on him and bite gently into his shoulder to muffle your cries. 

The orgasm is stronger than the last two he brought you to with his fingers and his mouth, respectively, as the feeling of his skin beneath your fingertips and the sheer rawness of his length brushing your walls makes you clamp down on his girth harder than you’ve ever come before. You cry out and clench your teeth and you’re going through your third intense wave of your orgasm when suddenly he flips the both of you over and pins your hips to his bed and begins to pound into you desperately.

His voice is strained and his hairline slick with sweat as he props himself up above you and glares determinedly into your face thats scrunched up in pleasure, moving his hips against you until he reaches his own peak. You feel his dick twitch once before he’s letting out a loud groan and a strangled cry of your name before his chest pulses for a moment and then he slumps down onto you. 

The both of you are spent and you’re still crying from the overwhelming feeling of being coaxed through three orgasms, with the third being the most intense you’ve ever felt in your life, and your chest heaves from the effort it took. Jeongguk is no better, as he pulls out of you with a groan and kneels between your legs. 

Taking advantage of your slumped and exhausted state, he pushes up a thigh and leans down a bit to see how his cum leaks out of your slit and grasps his cock that hasn’t softened yet with a groan. He gently holds the base of his sensitive member and collects the cum that’s already oozed out onto your thigh with his tip before pushing it back into you. 

You let out a strangled cry, a hand coming up to your mouth so you can muffle your cries, and another desperately clutching onto the wrist holding onto your thigh. He pauses, glancing up at your expression and waiting for you to push him away, but a slight movement of your wrist draws your thigh higher up and his hips a bit closer to you. Grinning, he grasps his softening cock once again and drags his tip from your upper thigh back into your slit, massaging his own cum into your center. 

When he’s completely limp and cringing himself from the overstimulation of pushing himself back into your pussy, he drops your thigh and climbs back up, whispering sweet things into your ear. 

“Baby, you were so good,” he coos, smoothing back your hair and wiping leftover tears. “You deserved that, you were so hot. Here, let me,” he gets a warm towel from the restroom and wipes down your thighs and core before dressing you in his t-shirt (a sight which he’ll never admit he absolutely loves) and pulling on a pair of boxers before climbing into bed with you and pulling you into his chest.

“I loved it.” 

You hiccup, breath short from the sensitivity but also from your tears. “You did?” 

And he thinks its the damned cutest thing ever, how even if you were an innocent girl he’d never thought he’d date, you suddenly turned into a sex starved shyer version of yourself because of him, and then returned back to the sweet blushing one he’d fallen in love with even after hours of rough sex and the dirtiest things. It absolutely fucking thrills him and makes his dick so hard whenever he brings you to too many orgasms, when you reach the point where you dont know whether to stop or continue, or to cry or kiss him. He’s had his fair share of flings and sexcapades, but he knows that the only girl who’s ever made him so whipped, the only girl who’s gotten Jeon Jeongguk wrapped around her tiny little finger, is you. 

You who he began to tease and flirt with as a joke, but ended up falling so damn hard for you after just a partner project where you ended up sympathizing with him and treating him like a real fucking human being, and not the football athlete that everyone worshipped and expected so much out of. You who always looked at him, past his body and face and extracurriculars, and into his soul and really truly understood who he was at the core. You who drunkenly kissed him one night underneath the stars and you who’s cheeks went furiously red when he kissed you again in front of the entire school. You who weren’t afraid of telling him when he was being too cocky or just a dick, and made sure to keep him in check, to the point that his teammates were commenting on what a kind softie he was becoming. 

And finally, you who he found himself hopelessly irrevocably in love with. 

And he looks down at you, with your bare face that’s not really anything special. Eyes, nose, and lips that are average, hair that’s common, and a body that others will say they’ve seen better. But its the way you look at him with your eyes that makes him love you. The way you press your nose against his neck when you cuddle with him and the way you shyly move your soft lips against him when you kiss him goodbye. It’s the way your hair feels like absolute silk underneath his fingers when he runs his hands through them when you’re asleep, and the way your entire body literally lights up and bends at his will and his only

Those are the things, amongst many, that made the high and mighty bad boy Jeon Jeongguk fall in love with you. 

So he cups your face and smiles as he pecks against your lips, peppering your face with them until you giggle and shriek against his attack. Laughing, he draws you close. 

“I did, because I fucking love you.”


Prequel: 01 & 02 [fin], Give and Take[M]

anonymous asked:

Hey! Just wondering, how did a solar eclipse prove the theory of relativity?

According to the theory of relativity space is not static. The movements of objects can change the structure of space.

In Einstein’s view, space is combined with another dimension - time - which creates universewide “fabric” called space-time. Object travel through this fabric, which can be warped, bent and twisted by the masses and motions of objects within space-time.

One prediction of general relativity was that light should not travel in a perfectly straight line. When traveling through space-time and approaching the gravitational field of a mass object, the light must bend-but not too much.

Then the English astronomer Sir Frank Watson Dyson proposed that the total solar eclipse of 1919 could prove, because the Sun would cross the bright Hyades star cluster. Star light would have to cross the gravitational field of the sun on the way to Earth, but would be visible due to the darkness of the eclipse. This would allow precise measurements of the positions displaced by the gravity of the stars in the sky.

Because of this, teams of researchers strategically positioned themselves in two locations that would initially provide the best conditions for observing the eclipse. One group stayed in Ilha do Príncipe, in São Tomé and Príncipe, and other researchers settled in Sobral, Ceará (Brazil).

Eddington, who led the experiment, first measured the “true” positions of the stars during January and February of 1919. In May, he went to remote Prince Island (in the Gulf of Guinea, on the west coast of Africa) to measure Positions of the stars during the eclipse, seen through the gravitational lens of the sun.

The total eclipse lasted about 6 minutes and 51 seconds, during those few minutes the astronomers captured several photos of the total eclipse. When Eddington returned to England, his data from Príncipe confirmed Einstein’s predictions. Eddington announced his discoveries on November 6, 1919.

3°Image: Negative of the 1919 solar eclipse taken from the report of Sir Arthur Eddington on the expedition to verify Einstein’s prediction of the bending of light around the sun.

Hubble Sees A Smiling Lens: In the center of this image, taken with the NASA/ESA Hubble Space Telescope, is the galaxy cluster SDSS J1038+4849 and it seems to be smiling.

You can make out its two orange eyes and white button nose. In the case of this happy face, the two eyes are very bright galaxies and the misleading smile lines are actually arcs caused by an effect known as strong gravitational lensing.

Galaxy clusters are the most massive structures in the Universe and exert such a powerful gravitational pull that they warp the spacetime around them and act as cosmic lenses which can magnify, distort and bend the light behind them. This phenomenon, crucial to many of Hubbles discoveries, can be explained by Einsteins theory of general relativity.

In this special case of gravitational lensing, a ring known as an Einstein Ring is produced from this bending of light, a consequence of the exact and symmetrical alignment of the source, lens and observer and resulting in the ring-like structure we see here.

Hubble has provided astronomers with the tools to probe these massive galaxies and model their lensing effects, allowing us to peer further into the early Universe than ever before. This object was studied by Hubbles Wide Field and Planetary Camera 2 as part of a survey of strong lenses.

A version of this image was entered into the Hubbles Hidden Treasures image processing competition by contestant Judy Schmidt.

Image Credit: NASA/ESA
Caption: ESA

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Astronomy and Astrophysics: Facts

Here is a list of some curiosities of astronomy and astrophysics. From our solar system to interstellar space.

Pluto: Pluto  is a dwarf planet in the Kuiper belt, a ring of bodies beyond Neptune. It was the first Kuiper belt object to be discovered. Like other Kuiper belt objects, Pluto is primarily made of ice and rock and is relatively small—about one-sixth the mass of the Moon and one-third its volume. It has a moderately eccentric and inclined orbit during which it ranges from 30 to 49 astronomical units or AU (4.4–7.4 billion km) from the Sun. 

Great Red Spot: The Great Red Spot is a persistent zone of high pressure, producing an anticyclonic storm on the planet Jupiter, 22° south of the equator. It has been continuously observed for 187 years, since 1830. Earlier observations from 1665 to 1713 are believed to have been the same storm; if this is correct, it has existed for more than 350 years.

Moons of Jupiter: There are 69 known moons of Jupiter. This gives Jupiter the largest number of moons with reasonably stable orbits of any planet in the Solar System. 

Uranus: Axial tilt: The Uranian axis of rotation is approximately parallel with the plane of the Solar System, with an axial tilt of 97.77° (as defined by prograde rotation). This gives it seasonal changes completely unlike those of the other planets. Near the solstice, one pole faces the Sun continuously and the other faces away. Only 

VFTS 102: VFTS 102 is a star located in the Tarantula nebula, a star forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way.

The peculiarity of this star is its projected equatorial velocity of ~600 km/s (about 2.000.000 km/h), making it the fastest rotating massive star known. The resulting centrifugal force tends to flatten the star; material can be lost in the loosely bound equatorial regions, allowing for the formation of a disk. The spectroscopic observations seem to confirm this, and the star is classified as Oe, possibly due to emission from such an equatorial disk of gas.

Black Holes: Monsters in Space: This artist’s concept illustrates a supermassive black hole with millions to billions times the mass of our sun. Supermassive black holes are enormously dense objects buried at the hearts of galaxies. (Smaller black holes also exist throughout galaxies.) In this illustration, the supermassive black hole at the center is surrounded by matter flowing onto the black hole in what is termed an accretion disk. This disk forms as the dust and gas in the galaxy falls onto the hole, attracted by its gravity. 

Saturn’s hexagon: Saturn’s hexagon is a persisting hexagonal cloud pattern around the north pole of Saturn, located at about 78°N. The sides of the hexagon are about 13,800 km (8,600 mi) long, which is more than the diameter of Earth (about 12,700 km (7,900 mi)). 

Gravitational lens: A gravitational lens is a distribution of matter (such as a cluster of galaxies) between a distant light source and an observer, that is capable of bending the light from the source as the light travels towards the observer. This effect is known as gravitational lensing, and the amount of bending is one of the predictions of Albert Einstein’s general theory of relativity.

Quasar: A quasar is an active galactic nucleus of very high luminosity. A quasar consists of a supermassive black hole surrounded by an orbiting accretion disk of gas. As gas in the accretion disk falls toward the black hole, energy is released in the form of electromagnetic radiation. Quasars emit energy across the electromagnetic spectrum and can be observed at radio, infrared, visible, ultraviolet, and X-ray wavelengths. 

Stretching SpaceTime: According to general relativity, the sun’s mass makes an imprint on the fabric of spacetime that keeps the planets in orbit. A neutron star leaves a greater mark. But a black hole is so dense that it creates a pit deep enough to prevent light from escaping.

Source: Wikipedia, NASA & ESO 

Image credit: NASA, JPL, New Horizons, Keck Observatory, Hubble, Chandra, Kevin Gill, James Provost  

9

Katara

I will never, *ever* turn my back on people who need me…

A Hitchhiker’s Ride to Space

This month, we are set to launch the latest weather satellite from the National Oceanic and Atmospheric Administration (NOAA). The Joint Polar Satellite System-1, or JPSS-1, satellite will provide essential data for timely and accurate weather forecasts and for tracking environmental events such as forest fires and droughts.

Image Credit: Ball Aerospace

JPSS-1 is the primary satellite launching, but four tiny satellites will also be hitchhiking a ride into Earth orbit. These shoebox-sized satellites (part of our CubeSat Launch Initiative) were developed in partnership with university students and used for education, research and development. Here are 4 reasons why MiRaTA, one of the hitchhikers, is particularly interesting…

Miniaturized Weather Satellite Technology

The Microwave Radiometer Technology Acceleration (MiRaTA) CubeSat is set to orbit the Earth to prove that a small satellite can advance the technology necessary to reduce the cost and size of future weather satellites. At less than 10 pounds, these nanosatellites are faster and more cost-effective to build and launch since they have been constructed by Principal Investigator Kerri Cahoy’s students at MIT Lincoln Laboratory (with lots of help). There’s even a chance it could be put into operation with forecasters.

The Antenna? It’s a Measuring Tape

That long skinny piece coming out of the bottom right side under MiRaTA’s solar panel? That’s a measuring tape. It’s doubling as a communications antenna. MiRaTA will measure temperature, water vapor and cloud ice in Earth’s atmosphere. These measurements are used to track major storms, including hurricanes, as well as everyday weather. If this test flight is successful, the new, smaller technology will likely be incorporated into future weather satellites – part of our national infrastructure.

Tiny Package Packing a Punch

MiRaTA will also test a new technique using radio signals received from GPS satellites in a higher orbit. They will be used to measure the temperature of the same volume of atmosphere that the radiometer is viewing. The GPS satellite measurement can then be used for calibrating the radiometer. “In physics class, you learn that a pencil submerged in water looks like it’s broken in half because light bends differently in the water than in the air,” Principal Investigator Kerri Cahoy said. “Radio waves are like light in that they refract when they go through changing densities of air, and we can use the magnitude of the refraction to calculate the temperature of the surrounding atmosphere with near-perfect accuracy and use this to calibrate a radiometer.” 

What’s Next?

In the best-case scenario, three weeks after launch MiRaTA will be fully operational, and within three months the team will have obtained enough data to study if this technology concept is working. The big goal for the mission—declaring the technology demonstration a success—would be confirmed a bit farther down the road, at least half a year away, following the data analysis. If MiRaTA’s technology validation is successful, Cahoy said she envisions an eventual constellation of these CubeSats orbiting the entire Earth, taking snapshots of the atmosphere and weather every 15 minutes—frequent enough to track storms, from blizzards to hurricanes, in real time.

Learn more about MiRaTA

Watch the launch!

The mission is scheduled to launch this month (no sooner than Nov. 14), with JPSS-1 atop a United Launch Alliance (ULA) Delta II rocket lifting off from Space Launch Complex 2 at Vandenberg Air Force Base in California. You’ll be able to watch on NASA TV or at nasa.gov/live.

Watch the launch live HERE on Nov. 14, liftoff is scheduled for Tuesday, 4:47 a.m.! 

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

you ever just think about how satya was probably told she’s the best and a genius her whole life to the point where probably all it would take is one mistake to shatter the little glass dome of perfectionism she’s under and she’ll be left cut, with bits of glass in her hair, picking up the pieces of everything she thought she knew, and they’ll never go back properly? the world’s a little different now, the world’s cold, and harsh, and she’s exposed, and she can’t really do anything, because when you’ve been told you’re the best, anything less than that is the same as failure.

you ever just think about that? cause I do, a lot