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Patreon: https://www.patreon.com/mattbatwings.
Discord: https://discord.gg/V5KFaF63mV
My socials: https://linktr.ee/mattbatwings.
My texture pack: https://modrinth.com/resourcepack/mattpack.
World Download: (JAVA 1.21) https://www.planetminecraft.com/project/3d-maze-explorer/

Oscar’s 3D Maze Program: https://youtu.be/2hdc0Fn302w.
Thanks again to @captainluma7991 for working with me on this!

Want to get more involved in the logical redstone community?
Learn Logical Redstone! https://youtube.com/playlist?list=PL5LiOvrbVo8keeEWRZVaHfprU4zQTCsV4
Open Redstone Engineers (ORE): https://openredstone.org/

0:00 Intro.
0:32 Oscar91
1:48 Generalization.
2:59 Display.
4:53 Maze to Tilemap Conversion.
6:12 Maze Exploration.
7:51 Wireframe Display.
8:27 Random Generation.

Music (in order):

That hurdle has now been cleared. A newly analyzed radio image reveals twin lobes stretching roughly 66,000 light-years on each side of a quasar called J1601+3102.

Because the radio waves began their trip across space more than 12.1 billion years ago, the observation shows the quasar as it was when the universe had completed only about nine percent of its history.

This particular quasar, J1601+3102, belongs to a youthful universe – it flared into view when the cosmos was less than 1.2 billion years old.

Somewhere in our galaxy are engines capable of driving atomic fragments to velocities that come within a whisker of lightspeed.

The explosive deaths of stars seems like a natural place to search for sources of these highly energetic cosmic bullets, yet when it comes to the most powerful particles, researchers have had their doubts.

Numerical simulations by a small international team of physicists may yet save the supernova theory of cosmic ray emissions at the highest of energies, suggesting there is a brief period where a collapsing star could still become the Universe’s most extreme accelerator.

A study published in Astronomy & Astrophysics has identified four previously unknown primordial open cluster (OC) groups in the Milky Way.

Open clusters, loose assemblies of stars born from the same giant molecular cloud (GMC), are typically considered to form in isolation. However, the newly discovered OC groups consist of multiple member clusters originating from the same GMC, formed through sequential processes.

Notably, two of these groups, labeled G1 and G2, appear to have formed via a hierarchical mechanism triggered by multiple supernova (SN) explosions.