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#mikako icons
pfpanimes · 3 months
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⌕ gokinjo monogatari - mikako.
like or reblog if you save/use.
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lowkey-aro-ace · 1 year
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Weirdcore Purple Mikako Icon
Free to use! No Credit Needed!
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lazitos · 11 months
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Strawberry Cream Soda Pop (~。~@)♪♪♪⭐️🍫
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barbie19219 · 1 year
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Gokinjo monogatari (1995)
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kaijugifs · 9 days
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godblessya · 7 months
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— You know all those foreign CDs she has? That’s the kind of music that he likes.
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serexvu · 2 months
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mikako kouda from gokinjo monogatari
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bryqe · 24 days
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gokinjo monogatari 4 mangas, ai yazawa ❤︎︎
they’ll be re-edited in spain so finally i’ll have them all i’m soooooooooooooooo happy! wrappppp! ✩
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parakindo707 · 1 year
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empty-skies-edits · 1 year
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spacecore mikako kurokawa icons! requested by nobody, suggested by @i-cant-stop-fandoming-help
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fanganedit-beach · 2 years
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Pride month dra girls icons!
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notmonaca · 2 years
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lmao [posts my sim version of a character from a fairly obscure piece of media]
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ninjagirlstar5 · 2 months
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Mikako Kurokawa, Ultimate Exorcist redesign go brrrr!
Okay, to be fair, this isn't much different to her OG outfit, but I wanted to change it up while still keeping the most iconic parts of her outfit like the giant bead necklace around her neck and ponytail and her long coat. The most obvious differences are the collar I added, the change of her skirt and socks, her hair looking even messier and unkempt, and I removed her cross necklace and instead put it on her collar and necktie as a symbol instead. Sorry, but that necklace just felt SO out of place amongst everything else, even with the context that she's the Ultimate Exorcist. Especially when she's already wearing an eye catching necklace with the giant beads, so the cross necklace either becomes so unnoticeable or just jarring when you DO notice it. But I didn't want to get rid of it entirely since it's a part of her design and she's an exorcist, so I just turned it into a symbol on her tie instead and made it a part of her collar. I also changed her color palette a little bit, that way the colors aren't so bleeding. Seriously, LINUJ really liked to use brightly saturated colors back then, huh?
Anyways, Mikako deserved the world. She did not deserve what she got!!
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googledetective · 4 months
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what I would get the DRA cast for Christmas :)
Utsuro - cocaine
Akane Taira - I think I’d get her a huge fucking teddy bear that you’d get like someone on Valentine’s Day
Tsurugi Kinjo - mental help
Rei Mekaru - I’d get her a list of every other fictional character name Rei and their statistics so she can see every Rei she is better than
Teruya Otori - okay so there’s this one dude on Peppa Pig who deadass had everything in his van, so I would get him that van
Kiyoka Maki - Fortnite
Mitsuhiro Higa - a self help guide on how to talk to women
Kizuna Tomori - a dictionary of every slur so she has nice nicknames to give people :)
Ayame Hatano - I’m just thinking like idk I think she would like a pair of sneakers but I would want to buy her like every fucking sneaker to ever exist bc she deserves it
Kanata Inori - operation board game (it’s that tabletop surgery game)
Kakeru Yamaguchi - i have no idea why but I think it would be hysterical if I got him shit like Nike Tech and Yeezy Foam runners and turned him into a basic boy 💀
Kinji Uehara - the Bible in every single language & that book of iconic quotes but they add the word ‘fuck’ to every quote
Haruhiko Kobashikawa - playboy magazine
Satsuki Iranami - the same exact clown suit she has already except it’s in every color combination possible
Yamato Kisaragi - those Discovery science projects for kids
Mikako Kurokawa - I’d somehow make MCR5 happen like rn
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Webb reveals new structures within iconic supernova
NASA's James Webb Space Telescope has begun the study of one of the most renowned supernovae, SN 1987A (Supernova 1987A). Located 168,000 light-years away in the Large Magellanic Cloud, SN 1987A has been a target of intense observations at wavelengths ranging from gamma rays to radio for nearly 40 years, since its discovery in February of 1987. New observations by Webb's NIRCam (Near-Infrared Camera) provide a crucial clue to our understanding of how a supernova develops over time to shape its remnant.
This image reveals a central structure like a keyhole. This center is packed with clumpy gas and dust ejected by the supernova explosion. The dust is so dense that even near-infrared light that Webb detects can't penetrate it, shaping the dark "hole" in the keyhole.
A bright, equatorial ring surrounds the inner keyhole, forming a band around the waist that connects two faint arms of hourglass-shaped outer rings. The equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots, which appeared as the supernova's shock wave hit the ring. Now spots are found even exterior to the ring, with diffuse emission surrounding it. These are the locations of supernova shocks hitting more exterior material.
While these structures have been observed to varying degrees by NASA's Hubble and Spitzer Space Telescopes and Chandra X-ray Observatory, the unparalleled sensitivity and spatial resolution of Webb revealed a new feature in this supernova remnant—small crescent-like structures.
These crescents are thought to be a part of the outer layers of gas shot out from the supernova explosion. Their brightness may be an indication of limb brightening, an optical phenomenon that results from viewing the expanding material in three dimensions. In other words, our viewing angle makes it appear that there is more material in these two crescents than there actually may be.
The high resolution of these images is also noteworthy. Before Webb, the now-retired Spitzer telescope observed this supernova in infrared throughout its entire lifespan, yielding key data about how its emissions evolved over time. However, it was never able to observe the supernova with such clarity and detail.
Despite the decades of study since the supernova's initial discovery, there are several mysteries that remain, particularly surrounding the neutron star that should have been formed in the aftermath of the supernova explosion. Like Spitzer, Webb will continue to observe the supernova over time.
Its NIRSpec (Near-Infrared Spectrograph) and MIRI (Mid-Infrared Instrument) instruments will offer astronomers the ability to capture new, high-fidelity infrared data over time and gain new insights into the newly identified crescent structures. Further, Webb will continue to collaborate with Hubble, Chandra, and other observatories to provide new insights into the past and future of this legendary supernova.
TOP IMAGE....Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A). At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W). Credit: Science: NASA, ESA, CSA, Mikako Matsuura (Cardiff University), Richard Arendt (NASA-GSFC, UMBC), Claes Fransson (Stockholm University), Josefin Larsson (KTH), Image Processing: Alyssa Pagan (STScI)
LOWER IMAGE....Webb’s NIRCam (Near-Infrared Camera) captured this detailed image of SN 1987A (Supernova 1987A), which has been annotated to highlight key structures. At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. In this image blue represents light at 1.5 microns (F150W), cyan 1.64 and 2.0 microns (F164N, F200W), yellow 3.23 microns (F323N), orange 4.05 microns (F405N), and red 4.44 microns (F444W). Credit: Science: NASA, ESA, CSA, Mikako Matsuura (Cardiff University), Richard Arendt (NASA-GSFC, UMBC), Claes Fransson (Stockholm University), Josefin Larsson (KTH), Image Processing: Alyssa Pagan (STScI)
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yomiurinikei · 1 year
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my favorite details from the new art
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1)tsurugis hat?? the floppiness of it the shape the fucking. puff. 😭🥺
2)logically speaking i know yamato just has like. a shirt collar or something. but it’s rlly funny to imagine his neck is just… half as thick as his arm. stick figure proportions
3)mikakos ear muffs <333
4)also the fuzz on her shoes? the collar of her jacket? she’s cute. fashion icon. ignore the entire rest of her jacket-
5) linuj did good with this background im proud of him
6) the singular visible button on yamatos jacket…..
7) actually no let’s keep going. yamato what are u wearing under that jacket what’s the white layer underneath that can be seen? why don’t your clothes fit you my son…
8) let’s keep going with clothes. what is tsurugi wearing he’s going to freeze……
9) ALSO this is interesting in terms of like… for the theory that tsurugi has some sort of inherited illness he got from juu, it’s cool to see his complexion/general coloring as a teen in linujs updated style? like, bc his coloring choices and the like changed, it’s interesting to have a more accurate drawing of him as a teen! it’s a lot less saturated than his look in dra, and more similar to how he is in sdra2.
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