Heavier and Louder Than a Heavy and Loud Thing @jacksmetalmachine - Tumblr Blog

Maybe I just feel so creatively drained lately is because everything is comprised of superhero movies and overproduced music for fuck’s sake. I need some new and real fucking inspiration if I want to move forward as an overall-creative person.

outofcontextdnd

“I throw my kebab at the vampire.” “It dies.” “What?” “Garlic.”

Check out the new, kickass music video and song from Pure Riff Her V!!! MARIGOLD - PERIPHERY |||: SELECT DIFFICULTY

#Periphery #Marigold #Select Difficulty #Metal #Prog Metal #Progressive Metal #Prog #Djent #Thall

thecommonchick

californiapunk-deactivated20180

Visit Original Link

Slayer - Raining Blood

jacksmetalmachine

Sometimes, you just gotta jam to muthafuckin’ SLAYERRRRR

outvade

New view of the Pillars of Creation via NASA/ESA

outvade

back-to-the-stars-again

Pismis 24 and NGC 6357.

Credit: NASA, ESA and J Maiz Apellaniz

theclassylion-deactivated202102

distant-traveller

Inside the Flame nebula

The Flame Nebula stands out in this optical image of the dusty, crowded star forming regions toward Orion’s belt, a mere 1,400 light-years away. X-ray data from the Chandra Observatory and infrared images from the Spitzer Space Telescope can take you inside the glowing gas and obscuring dust clouds though. The image will reveal many stars of the recently formed, embedded cluster NGC 2024, ranging in age from 200,000 years to 1.5 million years young. The X-ray/infrared composite image overlay spans about 15 light-years across the Flame’s center. The X-ray/infrared data also indicate that the youngest stars are concentrated near the middle of the cluster. That’s the opposite of the simplest models of star formation for the stellar nursery. They predict star formation to begin first in the denser center and progressively move outward toward the edges leaving the older stars, not the younger ones, in the center of the Flame Nebula.

Image credit: Optical: DSS; Infrared: NASA/JPL-Caltech; X-ray: NASA/CXC/PSU/ K.Getman, E.Feigelson, M.Kuhn & the MYStIX team