I tend to treat everyone online like an adult. If you don't want to read lewd jokes, dark/edgy humor, or discussions about potentially triggering topics, you shouldn't follow me or interact. If you'd like me to tag a trigger of yours, just send me an ask or a DM and I'll try my best. If you don't want people reblogging your stuff with a walltext of strong opinions, you should definitely block me. I'm chill towards and accepting of all queer and neurodivergent people. Autistic, ADHD, nonbinary, and trans people are especially welcome.
Topics I like:
any kind of science
memes/shitposts (the more obscure and abstract, the better)
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Under Virginia law, a month had to elapse before the death sentence could be carried out. Governor Wise resisted pressures to move up the execution date because, he said, he wanted everyone to see that Brown's rights had been thoroughly respected.
Brown made it clear repeatedly in his letters and conversations that these were the happiest days of his life. He would be publicly murdered, as he put it, but he was an old man and, he said, near death anyway. Brown was politically shrewd and realized his execution would strike a massive blow against Slave Power, a greater blow than he had made so far or had prospects of making otherwise. His death now had a purpose. In the meantime, the death sentence allowed him to publicize his anti-slavery views through the reporters constantly present in Charles Town, and through his voluminous correspondence.
Before his conviction, reporters were not allowed access to Brown, as the judge and Andrew Hunter feared that his statements, if quickly published, would exacerbate tensions, especially among the enslaved. This was much to Brown's frustration, as he stated that he wanted to make a full statement of his motives and intentions through the press.[54]: 212 Once he had been convicted, the restriction was lifted, and, glad for the publicity, he talked with reporters and anyone else who wanted to see him, except pro-slavery clergy.[46]
Brown received more letters than he ever had in his life. He wrote replies constantly, hundreds of eloquent letters, often published in newspapers,[133]: 43 and expressed regret that he could not answer every one of the hundreds more he received. His words exuded spirituality and conviction. Letters picked up by the Northern press won him more supporters in the North while infuriating many white people in the South.
Just a couple of the quotes about him that I like:
“His zeal in the cause of freedom was infinitely superior to mine. Mine was as the taper light, his was as the burning sun. Mine was bounded by time. His stretched away to the silent shores of eternity. I could speak for the slave. John Brown could fight for the slave. I could live for the slave. John Brown could die for the slave.”
-Frederick Douglass
"That new saint, than whom nothing purer or more brave was ever led by into conflict and death, — the new saint awaiting his martyrdom, and who, if he shall suffer, will make the gallows glorious like the cross."
[Image Description: initial tweet by Haymarket Books, at HaymarketBooks. It is dated May 9, Twenty twenty-three. It says "Abolitionist John Brown was born May 9, Eighteen hundred." Beneath the tweet is a grayscale portrait of John Brown, an elderly white man with a long, bushy beard. In reply, Edward Ongweso Jr, @ BigBlackJacobin, tweets "Happy birthday to this crazy ass white boy. One day we are gonna go back in time and give him power armor." End I.D.]
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You'll have a single mother of three who's fleeing a DV relationship. She has no recent work history because her ex kept her barefoot and pregnant. She's struggling with depression+PTSD while trying to find work in a horrific job market.
Now I have to be the one to tell her "Dept of Social Services insists every child over the age of 5 have their own bedroom, so you'll have to get a 4 bedroom, which will likely cost $5000/mo. You will get a housing voucher that covers 50% of the cost, so $2500/mo. You will need to make $90k/yr to comfortably afford this"
You and her both know a full-time minimum wage job comes out to $32k/yr in your area and most of that is going to go towards child care so she can work a job that will never pay enough to cover her living expenses. Even if she worked two full-time jobs, she'd still be ~$30k/yr short of the required income.
She can do everything right, she can work her ass off, she can get benefits, and it still won't make a difference. Her abusive ex is going to get the kids in the divorce simply because he has a steady income and home.
You see, in that moment, the woman start to consider going back to a guy who'll probably kill her and/or the kids someday and there's really fuck all you can do. Like " uhh I can help you apply for SNAP, you'll probably get $200/mo. Sorry for all the systemic issues"
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.
Make sure to follow us on Tumblr for your regular dose of space!
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