26. She/her. I can be super pedantic, so I apologize if I come off as rude. Variety content here, but usually feel good stuff. WillowWispFlame everywhere. pfp by hunbloom
My name is Willow! I'm an avid pokemon fan, my favorites being Absol and Leafeon. I read a lot of fanfiction and enjoy fanart - I often reblog cool art and memes. This is my main blog, so I post things from all fandoms here, though I try to keep it ~feeling good~ here. I make models with Blockbench for Minecraft projects. Maybe you've seen some of my work.
Pokemon is always big for me, but I’m also interested in Astronomy, Danmei, Minecraft Youtube, Dragons, Avatar the Last Airbender, Flight Rising, the Magnus Archives, Dungeons and Dragons, Fullmetal Alchemist: Brotherhood, Mystic Messenger, Stardew Valley, My Hero Academia, and more! These things sort of pop up randomly here as I reblog art or meta I like. Feel free to chat with me about any of them.
There is a blog impersonating me. I am NOT willowwispflame1
Under Shen Qingqiu’s hand, the punishing line of Luo Binghe's spine softened into something newly delicate, and Shen Qingqiu felt another twinge of helpless affection for this hardworking disciple of his, so trusting, facing the greatest of the three Realms’ horrors for a chance to come back home.
being a kid and hearing adults say stuff like "woah 2011 was 4 years ago haha" didn't really convey the fucking horror of a youtube video crossing my recommended labelled "9 years ago" and it's from 2017. that's not true. 9 years ago is 2010 or something. don't lie.
US American Science is Under Attack. Again. But You Can Help!
Hey, remember how last year, we all came together to protest on behalf of science against potential cuts to government funding? Well, we're back in the ring this year.
Meteorologists and climate scientists are back streaming for 50 hours to save America's forecasts on youtube with free talks by specialists, as the Trump administration takes aim at funding science and dismantles critical weather and climate labs:
From June 1st to June 3rd 2026, join meteorologists and climate scientists from across the US for a 50-hour livestream! We will share our sc
This substack article does a good job of summarizing the proposed changes to rules for federal financial assistance to researchers, which don't just affect climate and weather scientists, but impact all fields funded by the federal government:
Russell Vought is going to destroy American Science
Among the usual suspects of anti-trans, anti-DEI moves, the proposed changes aim to make political appointees be in charge of grant awards, dismantling the peer review system of using scientific merit to approve grant proposals. This is the push to try and make Trump's bogus executive order to align US American science with his own priorities legitimate, without congressional approval. This cannot be allowed to happen.
What can you do? Yes, of course call your representatives about it, but these proposed changes are also up for public comment.
The public comment period closes approximately July 13, 2026. Comments must be submitted to regulations.gov, Docket OMB-2026-0034.
You can view other public comments for inspiration if need be.
never lose hope. somewhere, a middle-aged, gender ambiguous person with an advanced degree in an esoteric field and a fiber arts hobby could be crashing out and pinning all their remaining mental health on getting obsessed with your otp. any day now, the most elegantly written 100k fanfic you have ever read is going to hit ao3. it could happen. it has happened.
This illustration shows the relative scale of the Nancy Grace Roman Space Telescope and a Tyrannosaurus rex. Roman is over 42 feet (12.7 meters) long — about the length of a T. rex — and over 14 feet (4.4 meters) wide when fully deployed. Roman also weighs around 18,000 pounds, or 8,000 kilograms (dry mass), which is the approximate mass of a T. rex as well.
Did you know NASA’s Nancy Grace Roman Space Telescope is both roughly as long and as massive as a Tyrannosaurus rex? This observatory, which will move to the launch site at NASA’s Kennedy Space Center in Florida very soon, is over 42 feet (12.7 meters) long and weighs around 18,000 pounds (8,000 kilograms), not including the fuel. Let’s explore some of the components that bring Roman to T. rex proportions.
Artist's concepts of NASA's Nancy Grace Roman Space Telescope (left) and NASA's Hubble Space Telescope (right), highlighting the 7.9-foot (2.4-meter) primary mirrors that sit in the heart of each observatory.
At the observatory’s heart sits a mirror that’s 7.9 feet (2.4 meters) across and 410 pounds (186 kilograms), or about the length and weight of a protoceratops! Roman’s primary mirror is the same size as the Hubble Space Telescope’s main mirror, but less than one-fourth the weight thanks to major improvements in technology.
Technicians installed Roman’s primary instrument, the Wide Field Instrument (pictured at left), in the fall of 2025.
The mission’s 300-megapixel infrared camera, called the Wide Field Instrument, is over 8 feet (about 2.5 meters) tall, which is about the length of a triceratops skull. It will give Roman the same angular resolution as Hubble while capturing an area of sky at least 100 times larger. The mission will gather data up to 1,000 times faster than Hubble.
Its sweeping cosmic surveys will help scientists discover new information about planets beyond our solar system, untangle mysteries like dark energy, and map how both normal matter and dark matter are structured and distributed throughout the universe. Casting such a wide, deep “net” into space will give astronomers plenty of cosmic bycatch as well; Roman’s crisp, panoramic views will offer practically limitless opportunities for astronomers to do all kinds of exciting science.
The Coronagraph Instrument was installed on Roman’s instrument carrier in October 2024.
Roman’s Coronagraph Instrument is about as wide (5.5 feet, or 1.7 meters) as a velociraptor is long. The Coronagraph is designed to demonstrate new technologies for directly imaging planets around other stars. It will block the glare from a star and make it possible for scientists to see the faint reflected light from planets in orbit around them.
The Coronagraph aims to photograph worlds and dusty disks around nearby stars in visible light to help us see giant worlds that are older, colder, and in closer orbits than the hot, young super-Jupiters direct imaging has mainly revealed so far.
This photo shows Roman’s 18 detectors, which are the heart of the mission’s 300-megapixel camera.
Roman’s “eyes,” 18 saltine cracker-sized detectors in its primary instrument, are each about as tall as an allosaurus tooth. They each have about 16.8 million tiny pixels for a total of 300 million, which means Roman’s images will be super hi-res. Each detector is made of millions of mercury-cadmium-telluride photodiodes (sensors that convert light into an electrical current), one for each pixel.
Principal technician Billy Keim installs a cover plate over Roman’s detectors.
The detectors are secured to a silicon electronics board that will help process the light signals using indium, a soft metal that has roughly the same consistency as chewing gum. Together, these ultra-sensitive detectors can capture vast areas of sky in a single shot while still revealing incredibly fine detail, allowing Roman to map the cosmos faster and more precisely than ever before.
Roman’s electrical wiring was installed on the spacecraft flight structure in the summer of 2023.
There are 1,000 pounds, or 450 kilograms, (the weight of a pachycephalosaurus) of electrical cabling, made up of about 32,000 wires and 900 connectors, laced throughout the observatory. If the wires were laid out end-to-end they would span 45 miles — nearly enough to trace the entire perimeter fence in the imagined Jurassic Park! Functioning as the Roman’s “nervous system,” the cabling enables different parts of the observatory to communicate with one another, provides power, and helps the central computer monitor the observatory’s function.
The Roman observatory was fully integrated on Nov. 25, 2025, at NASA’s Goddard Space Flight Center in Greenbelt, Md.
Roman’s six solar panels each measure about 7 by 10 feet (2 by 3 meters), collectively giving Roman a “wingspan” similar to a pteranodon’s! Together, they will provide a total of 4 kilowatts of power, which is about the same rate that a modest rooftop solar panel system produces during the daytime.
Over the course of two days in June 2025, eight technicians installed Roman’s solar panels onto the outer portion of the observatory.
The panels are covered in a total of 3,902 solar cells that will convert sunlight directly into electricity much like plants convert sunlight to chemical energy. When tiny bits of light, called photons, strike the cells, some of their energy transfers to electrons within the material. This jolt excites the electrons, which start moving more or jump to higher energy levels. In a solar cell, excited electrons create electricity by breaking free and moving through a circuit, sort of like water flowing through a pipe. The panels are designed to channel that energy to power the observatory.
Roman’s high-gain antenna will provide the primary communication link between the spacecraft and the ground.
The radio dish that will send data across a million miles of intervening space back to Earth spans 5.6 feet (1.7 meters) in diameter. That’s about the size of the largest known dinosaur footprints, yet it weighs only 24 pounds (10.9 kilograms). Its large size will help Roman send radio signals across a million miles of intervening space to Earth. The dual-band antenna will use one frequency band to receive commands and send back information about the spacecraft’s health and location. It will use another frequency band to transmit a deluge of data at up to 500 megabits per second.
We’re only a few months out from launch, and so close to a completely new understanding of the universe and our place within it. Follow along with Roman’s road to launch at nasa.gov/roman, and virtually tour the Roman observatory here.
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