Robertdowneyjr #flashback to The #Women of @marvelstudios #mcu lunch I Had The Pleasure Of Hosting… #girlpower #epic #bts (📸 @jimmy_rich) #TeamStark #thankyou

Hard to argue science with conspiracy theorists

higher further faster gayer

Station 19 - 4x02

only time and chromatography can hahahaha

The lab ran out of balloons that we often use to keep reactions under nitrogen atmosphere and a colleague had a a desperate attempt to use a nitrile glove instead of a balloon. 

I think that anyone is able to decide whether or not it has been successful…

MARIA HILL WILL BE IN FAR FROM HOME

MARIA HILL WILL BE IN FAR FROM HOME

This is not a simulation

New stills from Spider-Man: Far From Home (2019)

I like when an article thumbnail features a pic of a woman conductor, as it is the closest I will get to living in a world where newspapers write feel-good human-interest stories about a local witch who is proud to show off her new spell.

I can't wait any longer FOR GOD'S SAKE NAUGHTY DOG

“Life” is just a word for all the trivial stuff that happens while you’re waiting for The Last of Us 2

imagine entering the gym for your daily workout and finding brie on the floor like this

DUDE

Brie Larson

2020 March 25

Star Forming Region S106 Image Credit: NASA, ESA, Hubble Legacy Archive; Processing & Copyright: Utkarsh Mishra

Explanation: Massive star IRS 4 is beginning to spread its wings. Born only about 100,000 years ago, material streaming out from this newborn star has formed the nebula dubbed Sharpless 2-106 Nebula (S106), featured here. A large disk of dust and gas orbiting Infrared Source 4 (IRS 4), visible in brown near the image center, gives the nebula an hourglass or butterfly shape. S106 gas near IRS 4 acts as an emission nebula as it emits light after being ionized, while dust far from IRS 4 reflects light from the central star and so acts as a reflection nebula. Detailed inspection of a relevant infrared image of S106 reveal hundreds of low-mass brown dwarf stars lurking in the nebula’s gas. S106 spans about 2 light-years and lies about 2000 light-years away toward the constellation of the Swan (Cygnus).

∞ Source: apod.nasa.gov/apod/ap200325.html