aikkkkk:

このボールペンの書きやすさが神の領域

Track Title: WHATEVER LOLA WANTS

Artist: Sarah Vaughan

Album: single - WHATEVER LOLA WANTS

retromusicdaily-1950s:

WHATEVER LOLA WANTS

Sarah Vaughan

Peak date & (Position) = 5/28/1955 (#6)

RG Year Rank #63 (3,065 pts.) / Billboard Rank #51

http://rgmusiclists.proboards.com/

sweet-land-of-libertea:

Quick SCC22 otsukare from Menu ｡oO(冬眠モード):

artist note:

( [－]ω[－])。゜　|ω言)　｡oO(Right now I’ve…. gotta do it…!!)

source: pixiv

just finished watching “Grave of the Fireflies”

havent cried this much over a movie ever

patrickandmarcus:

Women’s complaints: We don’t make enough money, we’re hypersexualized, polticians vote over control of our bodies, we’re blamed for our own assaults

Men’s complaints: They keep saying they hate us

jen-suis:

Reblogging my own translation but I love this poem.polish poetry ftw

richotte:

i have this issue where when i buy something new, i immediately draw my oc flavor of the month making use of it

truxtondogyuun:

Wow I can’t believe Kaiba Corporation just bought Tumblr

thewoodlanders:

This is, without doubt, the creepiest photo ever taken. It shows the Apollo astronauts hand casts, used to produce the gloves worn on the missions.

spaceplasma:

Black-body radiation

When astronomers refer to the temperature of a star, they are talking about the temperature of the gases in the photosphere, and they express those temperatures on the Kelvin temperature scale.  On this scale, zero degrees Kelvin (written 0 K) is absolute zero (2273.2°C or 2459.7°F), the temperature at which an object contains no thermal energy that can be extracted. Water freezes at 273 K and boils at 373 K (at sea-level atmospheric pressure). The Kelvin temperature scale is useful in astronomy because it is based on absolute zero and consequently is related directly to the motion of the particles in an object.

Now you can understand why a hot object glows, or to put it another way, why a hot object emits photons, bundles of electromagnetic energy. The hotter an object is, the more motion there is among its particles. The agitated particles, including electrons, collide with each other, and when electrons accelerate—change their motion—part of the energy is carried away as electromagnetic radiation. The radiation emitted by a heated object is called black-body radiation, a name translated from a German term that refers to the way a perfectly opaque object would behave. A perfectly opaque object would be both a perfectly efficient absorber and a perfectly efficient emitter of radiation. At room temperature, such a perfect absorber and emitter would look black, but at higher temperatures it would glow at wavelengths visible to a human eye. That explains why in astronomy and physics contexts you will see the term black-body referring to objects that glow brightly.

Black-body radiation is quite common. In fact, it is responsible for the light emitted by an incandescent light bulb. Electricity flowing through the filament of the bulb heats it to high temperature, and it glows. You can also recognize the light emitted by hot lava as black-body radiation. Many objects in the sky, including the sun and other stars, primarily emit black-body radiation because they are mostly opaque.

Credit: Michael A. Seeds, Dana E. Backman

Gif credit: caucasianmale

kapooyah:

these zazzle shirts fit them ok

onixx-the-witch:

「一人は皆の為に

Artist: 中gut身 

and while tumblr obsesses about things i will never understand or attmept to, i will go play my mmporg