So amazing! Canβt wait for the next scene ππ»ππ»ππ»ππ»ππππ
βAnd will he not come again? And will he not come again? No, no, he is dead: Go to thy death-bed: He never will come again. His beard was as white as snow, All flaxen was his poll: He is gone, he is gone.β See Act 1, Scene 1 in full here on my website.
Join me on Wednesday for Act 1, Scene 2.
If I haven't mentioned it recently, I β€οΈyou!
Keep reading
π π‘π€¬π π‘π€¬
hereβs the trailer:
And if thereβs no showings in your area? Tweet at your local theater! Or call them or comment on their Facebook or Instagram page.
Itβs especially important that you post about the movie, even if you canβt buy a ticket or get your local theater to screen it. Lionsgate, the distributor, threw it under the bus by giving it barely any marketing, putting it the same weekend as Endgame, and only releasing in limited theaters.
Hi Tony stans/RdJ lovers,
So.
We have a new number.
βI love you 3,247β
As said by RDJ
while receiving his MTV movie awards for βBEST HEROβ for being 'TONY STARKβ
I was thinking may be ,
βI love you 3,247β
= I love you 3000, 24/7
I LOVE THIS MOVIE SO MUCH!!!!ππ»ππ»ππ
Costume series β White Christmas (requested by anonymous)
This little guy came into my job a few days previous and at first, I thought it was just a child's toy (from the way the boy held it), but soon as I started to look at it more intently, it turned my direction and winked at me π He was so gracious as to pose for me π
25 October 1415: Saint Crispin's Day/ Battle of Agincourt
You may have seen the famous blue marble or pale blue dot images showing Earth from 18,000 and 3.7 billion miles away, respectively. But closer to home β some 300 miles above Earthβs surface β you might encounter an unfamiliar sight: vibrant swaths of red and green or purple and yellow light emanating from the upper atmosphere.
This light is airglow.
Airglow is created when atoms and molecules in the upper atmosphere, excited by sunlight, emit light to shed excess energy. Or, it can happen when atoms and molecules that have been ionized by sunlight collide with and capture a free electron. In both cases, these atmospheric particles emit light in order to relax again. The process is similar to how auroras are created, but while auroras are driven by high-energy solar wind, airglow is energized by day-to-day solar radiation.
Since sunlight is constant, airglow constantly shines throughout Earthβs atmosphere, and the result is a tenuous bubble of light that closely encases our planet. Its light is too dim to see easily except in orbit or on the ground with clear, dark skies and a sensitive camera β itβs one-tenth as bright as the light given off by all the stars in the night sky. Β
Airglow highlights a key part of our atmosphere: the ionosphere. Stretching from roughly 50 to 400 miles above Earthβs surface, the ionosphere is an electrified layer of the upper atmosphere generated by extreme ultraviolet radiation from the Sun. It reacts to both terrestrial weather below and solar energy streaming in from above, forming a complex space weather system. Turbulence in this ever-changing sea of charged particles can manifest as disruptions that interfere with Earth-orbiting satellites or communication and navigation signals.
Understanding the ionosphereβs extreme variability is tricky because it requires untangling interactions between the different factors at play β interactions of which we donβt have a clear picture. Thatβs where airglow comes in. Each atmospheric gas has its own favored airglow color, hangs out at a different height and creates airglow by a different process, so we can use airglow to study different layers of the atmosphere.
Airglow carries information on the upper atmosphereβs temperature, density, and composition, but it also helps us trace how particles move through the region itself. Vast, high-altitude winds sweep through the ionosphere, pushing its contents around the globe β and airglowβs subtle dance follows their lead, highlighting global patterns.
Two NASA missions take advantage of precisely this effect to study the upper atmosphere: ICON β short for Ionospheric Connection Explorer β and GOLD β Global-scale Observations of the Limb and Disk.
ICON focuses on how charged and neutral gases in the upper atmosphere behave and interact, while GOLD observes what drives change β the Sun, Earthβs magnetic field or the lower atmosphere β in the region.
By imaging airglow, the two missions will enable scientists to tease out how space and Earthβs weather intersect, dictating the regionβs complex behavior.
Keep up with the latest in NASAβs airglow and upper atmosphere research on Twitter and Facebook or at nasa.gov/sunearth.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
Iβm getting closer to a half-century and I want to do him
Lol, youβre 25 years old and Sebastian Stan will be 36 soon.. heβs literally 11 years older than you yet you want to fuck him?
this canβt be a legitimate question
I β€οΈ him so hard