I Wanted To Lock In Before The New Year, So I Finally Got Through The Final Part Of My Circuits Lecture!!!

☕ 27.01.2025 // I completed my to do list and had a latte with a friend (Yes, we both took a latte ahah) 🩷

📖 X

🎧 The adults are talking - The Strokes

06/05/25 day 28/30

(4 hrs 26 mins on YPT)

Well the time doesn't actually matter because I studied for two and a half hours at most and after that I got busy with something else and forgot about the timer eeh- (human error -forgive me) Anyways I did maths (inverse trigonometry) and made notes for physics (electric charges).

my car

m42 (great nebula in orion) | 28 sec | 1/12/25

(it may be 00:06...) || ༻`` 25 Jan 25 — Saturday

.. > 12dopmas challenge, Day 2

I made notes for one of my last year's math units (im repeating the exam) and I started making notes for this year's work

/

/

Did 2 pistol squats on each leg (seems very little but they're actually very difficult! or are for me anyway)

I finished a digital drawing I started a while back. I think it's just alright, no strong feelings about it but im glad I got it done

I forgot about the questions again but I will catch up on them!

130 days clean

Day 0

Floor time ✅️ // 🍊

6/feb/2025, thursday

wasted most my time after school

subsequently had a lil mental breakdown & then pulled myself out of spiraling in a lowk mature way

washed my hair

prepared for psychology practical/viva

💤 3-4 hrs - maybe this is the reason my mental health has been a bit shit. looking forward to sleeping properly & FINISHING MY PORTIONS BEFOREHAND SO THAT I DON'T HAVE TO STAY UP LATE STRESSING

random physics comp i probably bombed 😭

classical mechanics is so fundamental but also kind of plain

Dolphin Head Nebula taken by Ben Brown on February 23 2024

The Dolphin Head Nebula, Sh 2-308, is an emission nebula caused by the Wolf-Rayet star EZ Canis Majoris. WR stars have completed fusion of hydrogen and are now fusing heavier elements such as helium and carbon. They have unique emission spectrums for this reason, with no hydrogen emission lines.

The temperature of WR stars is much higher than typical stars, reaching 20,000 K to 210,000 K. WR stars are some of the most luminous stars due to their high temperatures, but most of their output is in the ultraviolet spectrum, meaning we can't see it with the naked eye.

This UV radiation ionizes the gas around it, leading to the emission nebula you can see in the photograph.

lazed tf out of sunday

writing emails at midnight to 850 recipients will never go wrong, right?