I’m sure my Japanese is full of mistakes ;; でも、 試し続けます! ^^
Reading French: Well shit this might as well be english I can read this quickly and with 100% understanding wow
Listening to French: *blank expression staring light years past the person as my facial features slowly petrify*
Stationery addict 🤷🏻♀️ all stocked up and ready to start specialising in graphics next week ✏️
Hey! I have to do a quick presentation (like 2 minutes, tops) about literally any topic for a nuclear science class. I was thinking something along the lines of radiation in space but I'm clueless. Any suggestions?
You could talk about nuclear fusion in the core of stars, and how stars don’t create elements heavier than iron because instead of creating energy through fusion it requires energy.
All elements heavier than iron are formed during supernovae. After a star dies, the energy can be transferred into creating heavier elements! Thank a dead star for your existence
https://www.instagram.com/ctrl.st/
13017 || last week’s spread 💫
honestly?? this pic was just an excuse to show my milk bottle shaped flask i got from sm town in seoul,, it has #luckyone stamped on it and i lov it bc im exo trash anyway if y’all are interested in purchasing the two lovely notebooks shown in the pic, use my code “LUSTRE10″ on messybunny or “studylustre” on kawaiipenshop for 10% off!! they both have free international shipping woOoOo ✨
ig: studylustre
Good afternoon! This is the notes I’m trying to finish today. I just realized that I kept using pink in my recent post. It’s not even my favorite color lol (it’s green if any or you is wondering😂💚). Have a lovely day guys! 🌸✨
Studygram: @natastudies
“Gravitational ejection is about 100 times more likely than a random merger, meaning our star and the remaining bound planets will probably be ejected into the abyss of now-empty space after around 10^19 years. But even at that, with Earth orbiting our stellar remnant and with nothing else around, things won’t last forever. Every orbit — even gravitational orbits in General Relativity — will very, very slowly decay over time. It might take an exceptionally long time, some 10^150 years, but eventually, the Earth (and all the planets, after enough time) will have their orbits decay, and will spiral into the central mass of our Solar System.”
Worried about the environment of Earth today? Here’s a sobering fact: we already know how it’s all going to end. Not just when the next ice age will come or the next supervolcano will blow, but on cosmic scales stretching billions of years into the future and beyond. From the death of life on Earth to the end of the Sun, we can predict some major catastrophes our Solar System will face. But even after the Sun has died, the Earth and what’s left of our parent star will likely stick around for more. The matter expelled by our Sun will ignite new stars, which will die as well. White dwarfs will cool off into black dwarfs, and the Universe will go dark. And yet, thanks to gravitational effects, more interactions, on long enough timescales, will still remain.
Come get the long-term story of the future of our Solar System and see how it all will, in the ultra-distant future, come to an end.
11917 || hello everyone !! this is my bullet journal spread for this week so far ~ ٩(๑❛ᴗ❛๑)۶ ♡
inspired by milkteastudies :D
recent bujo spread ft. fortunes from a shrine and snaps from my trip to the tate ✨ ig: studylustre