Experience Tumblr Like Never Before
My childhood crush. Both him and Aurora.
Okay, so he’s got a girly face, and he wears tights and some high boots. Sure.
But check out that noble steed. That’s one ready-to-kick-ass-and-take-names steed.
While other princesses just run away and leave nothing, Philip gets AN INVITE TO HER HOUSE. He gets a song, a dance, and a first date.
He comes home, just to tell his dad he’s not going to marry the princess because he’s in love.
No. Other. Reason. He rides in and is just like, “I met the girl I’m going to marry. Now I’ve got a birthday party to be at. Bye Dad.”
Now how much do you think his dad weighs? That short fat little man? Probably pretty heavy.Not a problem for Prince Philip.
And then he gets jumped by goblins, both hands tied behind his back
But that’s not enough to stop Prince Philip.Oh no.
He breaks his hands free and starts chucking goblins.
Look at that face. That face. The “BITCH JUST YOU WAIT” face. He may be tied down by a dozen goblins but he’s not gonna take no shit from this witch.
In fact, he’s so strong, she ends up keeping him chained to the wall, but he still fights back.
Now when he finally does get free–
He’s ready to go into battle UNARMED. He don’t need no shield or sword, he’s going to go punch Maleficent’s face in with his fist. If Flora didn’t stop him, he probably would have, too.
Backed up against a cliff edge, nowhere to go. Fighting off goblins. But there’s so many and just one Philip.
NBD I’LL JUST JUMP AND SLIDE DOWN THE ROCK PILE IN MY SKIN-TIGHT TIGHTS.
Gate closing?
who gives a fuck? certainly not prince philip.
Lighting hitting rocks around me?
NBD BRO
Giant forest of thorns?
Bitch, get out of my way. I’ve got a princess to save.
Giant dragon of hell?
CHARGE HEAD ON.
Fire? Dragon? Burning dry twigs? No. Fucking. Problem.
Just smack that bitch on the nose.
Sheer cliff face? Fire burning behind me? Back to a wall?
Calm down guys, I got this.
I’LL JUST FUCKING SCALE IT ONE-HANDED.
And fight the bloody beast from 500 feet high, with literally nothing to save me if I fall.
Lose the shield off the cliff?
JUST STAND THERE AND SMILE ‘CAUSE I’VE GOT A FUCKING MAGIC SWORD THAT’S GOING THROUGH YOUR HEART BITCH.
Just chuck it. Straight through.
Then jump out of the way…
And survive. That’s what happens to bitches who mess with the woman I love.
Get the horse.
Get the girl.
EXPLAIN NOTHING.
that’s how he EARNED his happily ever after.
Srsly. The most bad. ass. prince. disney ever wrote.
randomly looking outside and seeing aurora wasn’t on my to-do list this year
Some Fan Art For A Fellow Pal. Hope You Like It Aurora~
Aurora belongs to @aurora-starlight-silly
(Decided to do something a little different :3 I know it isn’t CGI but I thought this might be fun to post too!)
Visions are seldom all they seem.
Lmao Aurora’s eyes roll SO hard in that second gif after Merida *gently* makes sure she’s paying attention
Well, I’m really not supposed to speak to strangers, but we’ve met before.
What I mean is that you're like someone from another world. You have a romantic aura.
Eileen Chang, Love in a Fallen City (1943)
Northern lights
Morning of the 12th in Fairbanks AK
Дни 11 и 12 для Крисса Красса и Авроры/Days 11 and 12 for Kriss Krass and Aurora
My local version of Aurora (Sleeping Beauty)
Exterior - Farmhouse Exterior Large country white two-story mixed siding home design idea with a black roof and shingles on top
Okay so I am definitly lost in a world full of nonsense XD
Oooups, I dit it again X'3 I wanted to draw more than just a panel but too tired for it X'3
Also, I tried a new way to "shade" even though it looks terrible X3 Would I have had more time, skills and motivation, I'd probably draw the whole movie since I love it so so much X3 The Azran returns again XD
I was rewatching The Cat Returns from Ghibli and I just thought of something X3 had to draw about it of course XD
So here are two drawings I did. I like the first one better than the second one but hey, friends told me it was good enough to be posted so X3
Let's call this The Azran returns XD
New drawing X3
I did a redraw of a famous scene from the Disney movie "Atlantis" But with Aurora from Azran Legacy X3 also I changed her clothes and damn it was hard to draw her as if she was some kind of cristal girl XD
This winter, our scientists and engineers traveled to the world's northernmost civilian town to launch rockets equipped with cutting-edge scientific instruments.
This is the beginning of a 14-month-long campaign to study a particular region of Earth's magnetic field — which means launching near the poles. What's it like to launch a science rocket in these extreme conditions?
Our planet is protected by a natural magnetic field that deflects most of the particles that flow out from the Sun — the solar wind — away from our atmosphere. But near the north and south poles, two oddities in Earth's magnetic field funnel these solar particles directly into our atmosphere. These regions are the polar cusps, and it turns out they're the ideal spot for studying how our atmosphere interacts with space.
The scientists of the Grand Challenge Initiative — Cusp are using sounding rockets to do their research. Sounding rockets are suborbital rockets that launch to a few hundred miles in altitude, spending a few minutes in space before falling back to Earth. That means sounding rockets can carry sensitive instruments above our atmosphere to study the Sun, other stars and even distant galaxies.
They also fly directly through some of the most interesting regions of Earth's atmosphere, and that's what scientists are taking advantage of for their Grand Challenge experiments.
One of the ideal rocket ranges for cusp science is in Ny-Ålesund, Svalbard, off the coast of Norway and within the Arctic circle. Because of its far northward position, each morning Svalbard passes directly under Earth's magnetic cusp.
But launching in this extreme, remote environment puts another set of challenges on the mission teams. These launches need to happen during the winter, when Svalbard experiences 24/7 darkness because of Earth's axial tilt. The launch teams can go months without seeing the Sun.
Like for all rocket launches, the science teams have to wait for the right weather conditions to launch. Because they're studying upper atmospheric processes, some of these teams also have to wait for other science conditions, like active auroras. Auroras are created when charged particles collide with Earth’s atmosphere — often triggered by solar storms or changes in the solar wind — and they're related to many of the upper-atmospheric processes that scientists want to study near the magnetic cusp.
But even before launch, the extreme conditions make launching rockets a tricky business — it's so cold that the rockets must be encased in styrofoam before launch to protect them from the low temperatures and potential precipitation.
When all is finally ready, an alarm sounds throughout the town of Ny-Ålesund to alert residents to the impending launch. And then it's up, up and away! This photo shows the launch of the twin VISIONS-2 sounding rockets on Dec. 7, 2018 from Ny-Ålesund.
These rockets are designed to break up during flight — so after launch comes clean-up. The launch teams track where debris lands so that they can retrieve the pieces later.
The next launch of the Grand Challenge Initiative is AZURE, launching from Andøya Space Center in Norway in March 2019.
For even more about what it's like to launch science rockets in extreme conditions, check out one scientist's notes from the field: https://go.nasa.gov/2QzyjR4
For updates on the Grand Challenge Initiative and other sounding rocket flights, visit nasa.gov/soundingrockets or follow along with NASA Wallops and NASA heliophysics on Twitter and Facebook.
@NASA_Wallops | NASA’s Wallops Flight Facility | @NASASun | NASA Sun Science
In Hollywood blockbusters, explosions and eruptions are often among the stars of the show. In space, explosions, eruptions and twinkling of actual stars are a focus for scientists who hope to better understand their births, lives, deaths and how they interact with their surroundings. Spend some of your Fourth of July taking a look at these celestial phenomenon:
Credit: NASA/Chandra X-ray Observatory
This object became a sensation in the astronomical community when a team of researchers pointed at it with our Chandra X-ray Observatory telescope in 1901, noting that it suddenly appeared as one of the brightest stars in the sky for a few days, before gradually fading away in brightness. Today, astronomers cite it as an example of a “classical nova,” an outburst produced by a thermonuclear explosion on the surface of a white dwarf star, the dense remnant of a Sun-like star.
Credit: NASA/Hubble Space Telescope
The brilliant tapestry of young stars flaring to life resemble a glittering fireworks display. The sparkling centerpiece is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground located 20,000 light-years away from Earth in the constellation Carina.
Credit: NASA/THEMIS/Sebastian Saarloos
Sometimes during solar magnetic events, solar explosions hurl clouds of magnetized particles into space. Traveling more than a million miles per hour, these coronal mass ejections, or CMEs, made up of hot material called plasma take up to three days to reach Earth. Spacecraft and satellites in the path of CMEs can experience glitches as these plasma clouds pass by. In near-Earth space, magnetic reconnection incites explosions of energy driving charged solar particles to collide with atoms in Earth’s upper atmosphere. We see these collisions near Earth’s polar regions as the aurora. Three spacecraft from our Time History of Events and Macroscale Interactions during Substorms (THEMIS) mission, observed these outbursts known as substorms.
Credit: NASA/Hubble Space Telescope//ESA/STScI
Every galaxy has a black hole at its center. Usually they are quiet, without gas accretions, like the one in our Milky Way. But if a star creeps too close to the black hole, the gravitational tides can rip away the star’s gaseous matter. Like water spinning around a drain, the gas swirls into a disk around the black hole at such speeds that it heats to millions of degrees. As an inner ring of gas spins into the black hole, gas particles shoot outward from the black hole’s polar regions. Like bullets shot from a rifle, they zoom through the jets at velocities close to the speed of light. Astronomers using our Hubble Space Telescope observed correlations between supermassive black holes and an event similar to tidal disruption, pictured above in the Centaurus A galaxy.
Credit: NASA/Hubble Space Telescope/ESA
Supernovae can occur one of two ways. The first occurs when a white dwarf—the remains of a dead star—passes so close to a living star that its matter leaks into the white dwarf. This causes a catastrophic explosion. However most people understand supernovae as the death of a massive star. When the star runs out of fuel toward the end of its life, the gravity at its heart sucks the surrounding mass into its center. At the turn of the 19th century, the binary star system Eta Carinae was faint and undistinguished. Our Hubble Telescope captured this image of Eta Carinae, binary star system. The larger of the two stars in the Eta Carinae system is a huge and unstable star that is nearing the end of its life, and the event that the 19th century astronomers observed was a stellar near-death experience. Scientists call these outbursts supernova impostor events, because they appear similar to supernovae but stop just short of destroying their star.
Credit: NASA/GSFC/SDO
Extremely energetic objects permeate the universe. But close to home, the Sun produces its own dazzling lightshow, producing the largest explosions in our solar system and driving powerful solar storms.. When solar activity contorts and realigns the Sun’s magnetic fields, vast amounts of energy can be driven into space. This phenomenon can create a sudden flash of light—a solar flare.The above picture features a filament eruption on the Sun, accompanied by solar flares captured by our Solar Dynamics Observatory.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
On Jan. 25, we’re going for GOLD!
We’re launching an instrument called Global-scale Observations of the Limb and Disk, GOLD for short. It’s a new mission that will study a complicated — and not yet fully understood — region of near-Earth space, called the ionosphere.
Space is not completely empty: It’s teeming with fast-moving energized particles and electric and magnetic fields that guide their motion. At the boundary between Earth’s atmosphere and space, these particles and fields — the ionosphere — co-exist with the upper reaches of the neutral atmosphere.
That makes this a complicated place. Big events in the lower atmosphere, like hurricanes or tsunamis, can create waves that travel all the way up to that interface to space, changing the wind patterns and causing disruptions.
It’s also affected by space weather. The Sun is a dynamic star, and it releases spurts of energized particles and blasts of solar material carrying electric and magnetic fields that travel out through the solar system. Depending on their direction, these bursts have the potential to disrupt space near Earth.
This combination of factors makes it hard to predict changes in the ionosphere — and that can have a big impact. Communications signals, like radio waves and signals that make our GPS systems work, travel through this region, and sudden changes can distort them or even cut them off completely.
Low-Earth orbiting satellites — including the International Space Station — also fly through the ionosphere, so understanding how it fluctuates is important for protecting these satellites and astronauts.
GOLD is a spectrograph, an instrument that breaks light down into its component wavelengths, measuring their intensities. Breaking light up like this helps scientists see the behavior of individual chemical elements — for instance, separating the amount of oxygen versus nitrogen. GOLD sees in far ultraviolet light, a type of light that’s invisible to our eyes.
GOLD is a hosted payload. The instrument is hitching a ride aboard SES-14, a commercial communications satellite built by Airbus for SES Government Solutions, which owns and operates the satellite.
Also launching this year is the Ionospheric Connection Explorer, or ICON, which will also study the ionosphere and neutral upper atmosphere. But while GOLD will fly in geostationary orbit some 22,000 miles above the Western Hemisphere, ICON will fly just 350 miles above Earth, able to gather close up images of this region.
Together, these missions give us an unprecedented look at the ionosphere and upper atmosphere, helping us understand the very nature of how our planet interacts with space.
To learn more about this region of space and the GOLD mission, visit: nasa.gov/gold.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
Freaky fast and really awesome! NASA astronaut Jack Fischer posted this GIF to his social media Tuesday saying, “I was checking the view out the back window & decided to take a pic so you can see proof of our ludicrous speed! #SpaceIsAwesome”.
In case you didn’t know, the International Space Station travels 17,500 miles per hour as it orbits 250 miles above the Earth.
Currently, three humans are living and working there, conducting important science and research. The orbiting laboratory is home to more than 250 experiments, including some that are helping us determine the effects of microgravity on the human body. Research on the station will not only help us send humans deeper into space than ever before, including to Mars, but also benefits life here on Earth.
Follow NASA astronaut Jack Fischer on Instagram and Twitter.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
Aboard the International Space Station, astronaut Thomas Pesquet of the European Space Agency snapped this photo and wrote, 'The view at night recently has been simply magnificent: few clouds, intense #aurora. I can't look away from the windows.'
The dancing lights of the aurora provide stunning views, but also capture the imagination of scientists who study incoming energy and particles from the sun. Aurora are one effect of such energetic particles, which can speed out from the sun both in a steady stream called the solar wind and due to giant eruptions known as coronal mass ejections or CMEs. Credit: NASA/ESA
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Is there a pot of gold at the end of a green aurora? Not sure, but these dancing green lights provide a spectacular view fitting for the St. Patrick’s Day holiday.
This stunning aurora was captured by NASA astronaut Jeff Williams during his 2016 mission on the International Space Station.
Even though auroras are best seen at night, they are actually caused by the sun. The sun sends us more than just heat a light…it sends lots of other energy and small particles toward Earth. The protective magnetic field around Earth shields us from most of the energy and particles. Sometimes, the particles interact with gases in our atmosphere resulting in beautiful displays of light in the sky. Oxygen gives off green and red light, while nitrogen glows blue and purple.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com