luteceslettuce:

but too much is falling in mine (x)

763 notes

confusedtree:

TRIBBLES OF THE PLANET IOTA GEMINORUM IV DREADED MORTAL ENEMIES OF THE GREAT KLINGON EMPIRE

confusedtree:

TRIBBLES OF THE PLANET IOTA GEMINORUM IV
DREADED MORTAL ENEMIES OF THE GREAT KLINGON EMPIRE

(Source: ninjaterra)

8,106 notes

pittarifit:

Portfolio 1001056
Photographed by Marcy Anarchy 2010
ttp://www.dlmarket.jp/manufacturer.php/manufacturers_id/2715

pittarifit:

Portfolio 1001056

Photographed by Marcy Anarchy 2010

ttp://www.dlmarket.jp/manufacturer.php/manufacturers_id/2715

3 notes

akibaranger:

theluckythirteenth:

Akibaranger Season 2 Wishlist: (expect changes as the series goes on!)

  • Swimsuit episode Coming soon based on this image
  • Character Swapping (Bodyswap)
  • Idol  Luna Iwashimizu
  • New team members
  • Gattai Robo
  • Battle Damage (refer to Go-Busters)
  • Kyoto setting episode
  • Power-Up Mode Super AkibaRed waifu armor

Luna is a “new team member” too.

14 notes

thegreenguitar:

RATTATA TA RATTATA TA TA HEY

thegreenguitar:

RATTATA TA RATTATA TA TA HEY

272 notes

pizza-omelette:

Sadly this is a true story …. yeah shut up

pizza-omelette:

Sadly this is a true story …. yeah shut up

38 notes

fuckyeahfluiddynamics:

During a solar flare, magnetic field lines on the sun are often visible due to the flow of plasma—charged particles—along the lines. According to theory, these magnetic lines should remain intact, but they are sometimes observed breaking and reconnecting with other lines. An interdisciplinary team of researchers suggests that turbulence may be the missing link. In their magnetohydrodynamic simulation, they found that the presence of chaotic turbulent motions made the magnetic line motion entirely unpredictable, whereas laminar flows behaved according to conventional flux-freezing theory. (Photo credit: NASA SDO; Research credit: G. Eyink et al.; via SpaceRef; submitted by jshoer)

fuckyeahfluiddynamics:

During a solar flare, magnetic field lines on the sun are often visible due to the flow of plasma—charged particles—along the lines. According to theory, these magnetic lines should remain intact, but they are sometimes observed breaking and reconnecting with other lines. An interdisciplinary team of researchers suggests that turbulence may be the missing link. In their magnetohydrodynamic simulation, they found that the presence of chaotic turbulent motions made the magnetic line motion entirely unpredictable, whereas laminar flows behaved according to conventional flux-freezing theory. (Photo credit: NASA SDO; Research credit: G. Eyink et al.; via SpaceRef; submitted by jshoer)

3,084 notes

the-science-llama:

Galaxy Coast
— Bill Shupp // Flickr

Taken near Bixby Bridge north of Big Sur, CA, this is a 12 shot vertical panorama taken around 4 am this past Monday, when the Milky Way was pretty high in the sky. The glow near the horizon is a lighthouse just around the bend.

All shots are 20 seconds, except the bottom one, which is 3 minutes

4,548 notes