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#this one has the same amount of rays as solar
snowe-zolynn-rogers · 5 months
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If this is really my boy, I’m gonna be insufferable and I already know it.
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sallyastral · 9 months
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Since you asked for headcanons:
I honestly believe that both Pavitr and Miles are extremely smart in their own ways.
Pavitr reinvented "gaslight, gatekeep, girlboss" and can even manipulate people like Miguel into underestimating him.
Miles is a really good strategist and his power control/experience is terrifying.
But when they are together?
Then they are to busy giving the other hearteyes. Every braincell is concentrated on the pretty boyfriend.
Hello there! Thank you so much for all the prompts you gave me, it's not annoying at all, really!/srs
I'll try to post both this one and the angst one tonight, and it'll take a bit more for the shifter AU because I never wrote one, so I'll need to think it through!
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As we know, being Spider-Man requires a fair amount of intelligence and strategy, and these two seem to posses both at insane levels
If you went around the Spider Society and asked about Pavitr, they'd surely describe him as that solar and optimist ray of sunshine who thinks nothing can go wrong and couldn't hurt a fly
Even though this is partially true, Pavitr actually gaslit a fair amount of the Spider Society to think of him that way
Miguel and Jessica too fell into his trap, the only ones to know the truth are Hobie, Gwen and of course Miles
In reality, he's definitely able to beat the shit out of someone with ease and with little remorse
He just thinks it's easier to do so if everyone around underestimates him, because he's free to do whatever he wants as no one will really pay attention to what he's doing
And just in case he gets in a fight with them, they'll surely go easy on him thinking Pavitr has little to no experience
But those six months of being Spider-Man were enough to teach him strategies
Miles instead prefers it the other way round
Even though he's still training, his control over his venom is terrifying to some members of the Spider Society because it's a pretty unusual power
And bro can turn invisible, creepy
So that's why after that small fight with Miguel they think twice before getting in a conflict with him
But this is only when they're alone
Because when they're together...
They're yes an unstoppable team, but It's like all that intelligence they had disappears in the void, every single braincell focused only on their boyfriend and his beauty
Miguel and Jessica learned the hard way it's best not to set them up on missions together, because all they'll do is getting distracted because of each other and end up doing something totally different
And if they really need them to be on the same mission, they can't be left completely alone, so that's why they always send at least two or more spider people with them
Missions with these two are frustrating, to say the least
They always have to keep them separated if they want the job to be successful
Otherwise, you can say bye bye to the mission
"Miles, can't you just focus-" "Sorry my boyfriend looked so hot spinning that web and I couldn't look away, sorry-"
And don't get me started on conversations and meetings
Everyone could be talking about the most important thing, on which the whole multiverse's life could depend on, and you'd still catch them looking into each other's eyes or having their own private conversation
It's like everything else disappears
No thoughts, just pretty boyfriend
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radiant-reid · 1 year
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I posted 2,107 times in 2022
That's 1,747 more posts than 2021!
2,047 posts created (97%)
60 posts reblogged (3%)
I tagged 2,060 of my posts in 2022
Only 2% of my posts had no tags
#spencer reid - 965 posts
#rr answers - 701 posts
#criminal minds - 590 posts
#spencer reid x reader - 350 posts
#spencer reid x you - 291 posts
#spencer reid x y/n - 287 posts
#spencer reid fandom - 277 posts
#spencer reid blurb - 156 posts
#spencer reid fanfiction - 129 posts
#spencer reid headcanon - 127 posts
My Top Posts in 2022:
#5
I NEED a blurb where reader is just shocked how good Spencer is in bed and after he's done literally beating her back in he's all like "so there's this new film I think we should go see" and reader is still in shock and is like speechless Cate. I need this.
this would be such a spencer thing
Spencer flops down on the bed next to you, running a hand through his hair to get it situated properly again.
You lay next to him, trying to regulate your breathing and get your heart rate under control before you have to go to the hospital. A sex injury is not something you want to explain to the team.
"So I was thinking we should start the new season of Doctor Who because even though it's not all out yet, we'll miss some nights on cases." Spencer starts, and it takes you hitting his chest for him to stop.
"That's what you're thinking about?" You ask, out of breath as you pant.
He looks at you strangely, frowning. "Are you okay? You sound kind of out of breath."
You scoff shallowly. "You literally just rearranged my guts, and you're asking me why I'm breathless?"
Spencer blushes at the dirty euphemism like he hadn't just made you cum so hard you cried. "Sorry." He apologizes.
"I'm not complaining." You assure him, shaking your head. "It was amazing. You just clearly have a lot more stamina than me."
"Better tell Morgan that next time he's telling me I'm unfit." He jokes.
"Oh yeah." You agree sarcastically. "I'll tell our colleague all about our sex life."
Spencer grimaces. "On second thought, maybe not. I think I'll keep how good I can fuck you as our little secret."
2,738 notes - Posted October 24, 2022
#4
Secret Life
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Summary: The team accidentally stumbles upon Spencer, a mystery woman, a mystery girl, and a decade-long secret
hii!! I've had this idea for some time in my head and you write spender Reid so good I just had to send it here. :) What if Spencer has been dating someone in secret for a long time, they even have a kid, but they decided to only tell their parents about it to protect his parter and kid from his job and one day they visit him at work and the entire team is confused because since when does Spencer have a wife and kid?
A/n: thank you so much !! and thank you for this request, i'm a sucker for hidden relationships
Pairing: Spencer Reid x Fem!Reader (Fluff)
Content Warning: nothing ?
Word Count: 1.8k
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"Coat, sweetie, you need your coat." Y/n directed the young girl away from sitting on the couch and towards the coat rack in the entryway.
"Momma, don't wanna." She replied, pouting as she dragged her feet across the wooden steps towards to front door.
It was difficult for Y/n not to laugh, especially when she'd seen her father do the exact same expression. Mostly when she tried to get him to stop working or go to sleep. Both of them were stubborn, although most people wouldn't be able to pick it on first meeting them.
"What did daddy tell you?" Y/n asked, handing her the light pink woolen coat to put on before putting her own on.
"That it's cold because the northern hemisphere is tilted slightly away from the sun, and the rays come in at an angle that lowers the amount of solar radiation reaching the surface." She repeated verbatim even if she didn't totally understand the scientific definition. Even when she was two, Spencer suspected she had an audiographic memory. "And I have to wear a coat." She recited, annoyed about it.
When she looked back up at her mom, Y/n was looking in the mirror, criticizing her face. Silently, of course, to avoid giving her daughter a complex. "What did daddy tell you?" She questioned, giving her a taste of her own medicine.
"That we are the most beautiful girls in the world," Y/n spoke, unable to stop the grin her face broke out into. She looked down at the little girl. "Don't you forget that either."
"So, can we go?" She asked, crossing her arms over her chest in the same way Spencer did when he was being sassy. It was something Y/n loved about both of them, although she refrained from telling them.
Y/n shrugged her light pink coat over her shoulders, bracing herself for the chilliness that was DC in late January. "Okay then." She replied, quickly looking at the little girl to ensure she was dressed in enough warm clothing. A thermal shirt, sweatpants, a kids Caltech sweatshirt, and her coat were enough.
After a car ride without much traffic, brewing anticipation, and some helpful commentary provided by Spencer's mini-me, they were at the FBI. Y/n roughly knew where to go, but the receptionist checked her ID and directed them to the sixth floor.
Both of them were excited on the elevator ride, exchanging wide grins as the mission to surprise Spencer came closer. A quick glance around confirmed Y/n's hypothesis that the floor was deserted aside from her husband. The first step in their plan-previous decided in the car- started as soon as the elevator doors opened.
It relied on Y/n and the hope that she could walk through the glass doors and behind Spencer without being heard as she carried their daughter. Probably because he was in such deep thought, it worked.
Silently, Poppy wrapped her hands around his eyes, making him jump in surprise, no doubt scared about who was behind him. He relaxed when he realized the fingers were 5-year-old size.
"Guess who, daddy?" She asked, trying to disguise her voice by deepening it, which sent both her parents into a fit of giggles. Spencer was quick to shut the case file on his desk that, thankfully, didn't contain any pictures. His mind was instantly off the brutal double homicide and on his family.
"Well." Spencer pretended to consider it. "There's only tw-one, there's only one person in the world that calls me that. So, I'm going to guess that it's Miss Poppy Rae Reid." He decided to use her full name to make the guess official.
With a cheer from the correctly identified girl, she scrambled to get out of Y/n's arms. She wrapped her arms around Spencer's neck and her legs around his waist so she could tightly hug him. Spencer held her small figure just as tight, resting their noses together when she untucked her head from his neck. Watching them, Y/n's heart was filled with love as she suddenly wanted another baby.
Spencer placed a kiss on the little girl's forehead, having to push back brown curls that paralleled his own. "What are you doing here?" He asked, glancing up at Y/n.
Poppy bet her to an answer. "Mommy said that if I finished the last four chapters of Geronimo Stilton, then we could come here to get you and get hot chocolate on the way home."
"I did underestimate how quickly we'd get through it." Y/n mentioned.
Spencer laughed loudly, looking at his daughter, whose expression grew increasingly guilty for a reason Y/n didn't know. "You were tricked, lovely." He answered before she had to ask, smiling at her. "We finished it last night, didn't we?" He asked, looking back to Poppy with a pointed look. She dramatically pouted, resting her head on his chest so she could look up at both of them with innocent eyes.
"We should have called you mischief." Y/n joked, reaching down to tickle her.
She squirmed on Spencer while she giggled. "M-make her s-stop." She pleaded to her dad between laughter, getting Y/n to stop.
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2,767 notes - Posted February 4, 2022
#3
What's in a name?
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Summary: Spencer accidentally gets misidentified by a little kid whose mom means the world to him
reader has that weird super friendship/seems like a relationship type thing with spencer. Reader is like a social worker member of a BAU who adopts a baby/toddler from a bad case that everyone adores and it randomly starts calling spencer daddy because the baby sees him so often
Pairing: Spencer Reid x Fem!Reader (Fluff)
Content Warning: little bit of usual cm case details |
Word Count: 2.2k
Masterlist Navigation
The first time Y/n met her future son, she legitimately cried. The little boy was so vulnerable, with the only thing he'd had to call a mother taken from him by the serial killer the BAU were hunting down.
Lots of the kids she came into contact with were troubled, but sweet, six-month-old Beckham needed someone. He didn't have a dad listed on his birth certificate, and his mom was a runaway with no family.
As part of her job on cases involving children, she often had to give them over to the foster care workers, and she knew how bad the system usually was.
Y/n was fully committed to going to Hotch to plead with him before they had to leave. Leaving Beckham with Spencer, she found Hotch in the boardroom they were occupying.
"Hotch, I need to talk with you." She announced, parading as much confidence as she had as she shut the door.
His face showed a bit of concern as he looked up from his paperwork at her. "What's wrong?"
"It's Beckham. I want to take him back to DC with me, adopt him and raise him." She spat out quickly but firmly.
"L/n." He replied in a flat tone.
It sounded too much like a warning for her to not interrupt and try to persuade him. "He doesn't have any family, and I've spent enough time with him this week to know he's sweet. I know raising a baby is a lot of work, but I have time, money, and love, and I just can't watch him go into foster care when I know that I can give him a better life." She persisted, not taking a breath until she finished her sentence.
"Y/n." Hotch stopped her when he used her first name. "I think it's a great idea."
"Oh." Y/n realized, letting her frown change to a smile when she realized what he'd just said. "So I can adopt him?"
He nodded slightly. "I know a good lawyer who can help you, too. I'll give you her number."
~
Her very best friend in the world, and the easiest option for godfather, Spencer, helped her right from the start.
"Is this a crazy thing to do?" She asked as they sat on the floor the first night, putting together the expensive, oval-shaped, white wooden crib that she'd brought. Beckham was in the car seat carrier she'd had to buy when they were still in North Carolina, before they drove back to DC.
Spencer glanced at her for a moment like he was trying to figure out the correct answer, but then he looked at the baby and how Y/n looked at him when she rocked the car seat carrier.
The answer was simple after he admired her for a second. "No."
"Good, because I trust your judgment." She almost absentmindedly told him, but Spencer knew he'd be thinking about it for the rest of the week. "Even if I am kind of scared about this." She confessed.
"You're going to be an amazing mother, Y/n." He assured her with a smile, one that made her heart flutter just a little bit.
Trying to hide the blush on her cheeks, she laughed. "I trust your judgment even more now." She joked, earning a chuckle from him.
Not only was Spencer her (now second) favorite person, he also had a degree in Engineering which should have made him skilled at building furniture. However, she found that wasn't true when it was 11 o'clock before the crib was built.
As gently as she could, she picked up the tiny baby and lay him down where he'd be sleeping for a while. The first stable home he'd ever had.
She was crying then, too, looking down at the adorable baby. "Is it crazy that I love him so much already?"
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2,838 notes - Posted February 27, 2022
#2
The Private Side of a Secret Life
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Part 1
Summary: After the ladies of the BAU take Spencer's mystery wife out and learn some... new things about their colleague, the Reids get to work on making their fantasy a reality.
A/n: I just want to say a very quick thank you to all of you amazing people who loved part 1 and inspired me to write a part two. Enjoy  🤍
Pairing: Spencer Reid x Fem!Reader (SMUT 18+)
Content Warning: vomiting | swearing | NSFM (breeding kink, daddy kink, unprotective penetrative sex, slight fingering)
Word Count: 3.1k
MasterlistNavigation
"Spencer, seriously, I'll be fine." Y/n attempted to assure him for the fourth time, trying to wave him out of the bathroom so she could continue to apply her mascara without his watchful gaze.
Despite the reassurance, he grimaced. It wasn't that he didn't trust Y/n because he absolutely did and had for some years or that he didn't have faith the ladies of the BAU would look after her, but Spencer had second-hand nerves about what they would discuss. Mostly because he knew after a few drinks, Y/n was down for anything, which was actually how they ended up buying their very first sex toy. Although, that was beside the point because it brought immense pleasure and not lifelong embarrassment at work.
He still had one more trick up his sleeve, executing his scheme by pressing her against the bathroom vanity, caging her in with his arms on their side of her body as he leaned down to whisper in her ear. "Or, you could just say here." He suggested. "Put Poppy to bed early so I could rip that dress off you." His eyes were all over her figure, admiring the curves the tight dress accentuated.
When he used that tone, she had a hard time focusing on anything that wasn't how the temptation that was the growing bulge in his pants pressed against her ass.
Luckily, before she could drop the mascara wand, another Reid spoke. "Daddy! The iPad isn't working." Poppy complained, no doubt sitting on the couch tapping it harshly.
"Mood killer." Spencer dramatically whined.
Y/n could hear the playful tone in his voice as she shoved his shoulder. "I recall you named her Poppy."
"I don't even know anything about technology." He complained, stepping out of the bathroom.
Pulling him back in, Y/n passionately dove in to kiss him, purposefully teasing. "Spencer?" She asked, earning a nod after a pause from him as if his brain momentarily stopped working. "You were never going to convince me anyway."
Spencer let out another groan, more than a bit sexually frustrated before going to read the iPad instruction manual. Y/n fluffed her hair out again, trying to make sure it looked alright. Although she wouldn't tell him, she was worried about what Spencer's best friends would think of her.
"Okay, I'm going now." She announced, heels that she would end up taking off on as she walked into the living room. Poppy waved, still watching Spencer when Y/n walked over to place a kiss on her forehead. "Mwah." Spencer, sitting on the floor, tilted his chin up as he waited for his kiss. After she giggled, she leaned down to place a soft kiss on his lips. "Love you both!" She announced, walking towards the door.
"No secrets," Spencer instructed, although it came out weaker than he would have liked.
Y/n spun back around, drawing a cross over the fabric of her dress where her heart was. "Promise." She assured him.
She stayed true to her oath to Spencer for most of the enjoyable evening. His friends were great, like how he'd described them so many times, and she had no trouble fitting in. The problems- spilled secrets- came when the shots came. Some tequila and her lips were loose.
"Oh yeah, having Henry changed the game," JJ said in reply to a question about her and Will's sex life. "Not that I don't love him with all my heart, but things were... different when we were still sneaking around."
"So you're trying to convince us that three-hour flights to New Orleans are sexy?" Emily rhetorically asked, making all of them burst into a fit of giggles while JJ tried to defend her statement.
Penelope was next to playfully bad mouth her friend's relationship. "A long-distance booty call." She joked. "I can't believe you thought we didn't know."
JJ laughed at the mistakes of her younger self, burying her head in her hands to avoid the embarrassment. "Even I knew." Y/n chimed in between laughs, making Emily and Penelope double over in giggles.
With the attention back on Y/n, they had the same question to repeat to her. "We know absolutely nothing about Spencer's sex life, so feel free to tell us everything," Emily told her, least drunk and ready to save his secrets for a later day.
"Well, Spencer never changed. Like, at all." Y/n was ready to brag about her husband and the way he could fuck her. "When I was pregnant, oh my gosh, he was insane like wild all day every day."
It made her shiver thinking about it. Spencer had been away on a case when she really popped, and as soon as he saw her pregnant with his child, he went crazy. She lost count of how many times she came that night.
"So when you got together, was he, you know, a virgin?" Penelope steered the conversation back to the question everyone at the BAU had wondered before they learned he had a wife and child.
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2,919 notes - Posted February 5, 2022
My #1 post of 2022
The guaranteed way to get to sleep
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reader having a hard time sleeping and spencer noticing that and that she is touch starved so he lets them cuddle and she finally sleeps and just fluff <3 + reader having a hard time sleeping (either insomnia or just regular trouble sleeping) and spencer realizing that they're touch starved and he lets them sleep with him and they finally sleep?
a/n: i'm not sure if this was the same anon, but either way thank you for this request🤍
Summary: Spencer is the only one who can recognize the signs of needing someone in the new agent
Pairing: Spencer Reid x Fem!Reader (Fluff)
Content Warning: tiny implied mention of Maeve | touch starved reader
Word Count: 1.7k
Masterlist Navigation
There were many things stressful about working at the BAU. Mostly the serial murder, but the effect of seeing what they saw each day had really started getting to Y/n a few months in.
For weeks, she'd been struggling to sleep, waking up with the same recurring nightmares and haunting visions. It had gotten so bad she had become known as the superlative of coffee addicts- a title that was hard to take from Spencer-
For as long as the nightmares had been going on, Y/n had been keeping her feelings bottled up, not telling anyone what was going on in her mind in case they saw it as a sign of weakness. The unit had been her dream since she was first in the academy. It had taken 5 years to get there, and she wasn't about to have anyone thinking she wasn't cut out for it.
It was incurable, and she found herself awake on the jet in the middle of the night journey. It was only three of them, coming back from San Diego where she'd gone along on a prison consult with JJ and Spencer.
JJ was out as soon as they got on the jet, curled up on the double seat, but all Y/n could do was look out the window at the dark sky and let her mind race.
The cold window pressed against her cheek was a constant reminder she was awake, and the tiny flickering of lights across the country should have been enough to put her to sleep. It was as relaxing as it could be without letting her sleep.
"What's wrong?" A voice unmistakably Spencer's made her jump in surprise as he sat on the single-seat across from her. He knew the signs, all of them from only two years ago after he'd been forced to watch someone he loved die.
Y/n flashed him a smile filled with false confidence, trying to brush his concern off. "Nothing."
He tipped his head to the side like he was asking if she seriously thought he'd believe that. "I can't help you if you don't tell me." He reminded her.
Over the three months, she'd worked with the team, they'd grown close. Of course, everyone was welcoming, but she found it easy to get along with Spencer. If her feelings weren't totally unreciprocated and bordering on inappropriate, she would have asked him out, but he'd only ever treated her like a colleague, so her little crush stayed buried.
"What makes you think I want you to help me?" She asked, much snarkier than she wanted to. Immediately, she felt guilty when she realized why she'd taken that tone. "Sorry, I didn't mean to-"
"It's okay," Spencer assured her, reaching out to touch her hand. "How long has it been?"
Frowning, she wondered if he could possibly know, but it seemed unlikely. She'd only seen a side of him that was protective, articulate, and well presented, and while it was unrealistic, it wasn't hard to assume he was perfect. "What do you mean?" She hesitantly asked.
"Since you slept." He clarified, not willing to let her dodge the question.
"Three days." She mumbled, pulling her knees tighter to her chest like it would bring her human comfort. Over the months, she'd become more anxious, stressed, and generally sad, and she knew it wasn't just because of her job. It was dangerously near to a full-scale breakdown, teetering on the edge of a.
The look on Spencer's face was far from the judgment she expected. It was... caring in a way she wasn't sure she could care for herself. "L/n, you know you can't go on like that." He reminded her.
"How do you make it stop?" She asked voice just a whisper from trying not to cry. All the emotions were intense from the hours she'd spent awake, threatening to spill over at any moment. "I can't stop seeing...things when I close my eyes." She explained like he didn't get it, shivering as she envisioned the memories.
One thing Spencer hated about his job was the fact other people had to do it. Especially when they were as pure as Y/n was. The way she gripped his hand like it was her lifeline led him to deduce something else was going on.
"Don't take this the wrong way, but when was the last time someone hugged you?" He asked, rubbing his thumbs in circles.
Y/n had no idea what his question was supposed to mean, but she answered it regardless. "A long time."
"Come on." Spencer knew what he needed to do, pulling her out of her seat and over to the unoccupied couch.
Y/n's confused expression didn't stop as she tried to figure out what he possibly could have wanted. Spencer didn't let her hypothesize for too long, wrapping his arms around her shoulders and pulling her body into his chest.
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6,410 notes - Posted March 2, 2022
Get your Tumblr 2022 Year in Review →
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Webb Rules Out Thick Carbon Dioxide Atmosphere for Rocky Exoplanet An international team of researchers has used NASA's James Webb Space Telescope to calculate the amount of heat energy coming from the rocky exoplanet TRAPPIST-1 c. The result suggests that the planet's atmosphere - if it exists at all - is extremely thin. With a dayside temperature of roughly 380 kelvins (about 225 degrees Fahrenheit), TRAPPIST-1 c is now the coolest rocky exoplanet ever characterized based on thermal emission. The precision necessary for these measurements further demonstrates Webb's utility in characterizing rocky exoplanets similar in size and temperature to those in our own solar system. The result marks another step in determining whether planets orbiting small red dwarfs like TRAPPIST-1 - the most common type of star in the galaxy - can sustain atmospheres needed to support life as we know it. "We want to know if rocky planets have atmospheres or not," said Sebastian Zieba, a graduate student at the Max Planck Institute for Astronomy in Germany and first author on results being published today in Nature. "In the past, we could only really study planets with thick, hydrogen-rich atmospheres. With Webb we can finally start to search for atmospheres dominated by oxygen, nitrogen, and carbon dioxide." "TRAPPIST-1 c is interesting because it's basically a Venus twin: It's about the same size as Venus and receives a similar amount of radiation from its host star as Venus gets from the Sun," explained co-author Laura Kreidberg, also from Max Planck. "We thought it could have a thick carbon dioxide atmosphere like Venus." TRAPPIST-1 c is one of seven rocky planets orbiting an ultracool red dwarf star (or M dwarf) 40 light-years from Earth. Although the planets are similar in size and mass to the inner, rocky planets in our own solar system, it is not clear whether they do in fact have similar atmospheres. During the first billion years of their lives, M dwarfs emit bright X-ray and ultraviolet radiation that can easily strip away a young planetary atmosphere. In addition, there may or may not have been enough water, carbon dioxide, and other volatiles available to make substantial atmospheres when the planets formed. To address these questions, the team used MIRI (Webb's Mid-Infrared Instrument) to observe the TRAPPIST-1 system on four separate occasions as the planet moved behind the star, a phenomenon known as a secondary eclipse. By comparing the brightness when the planet is behind the star (starlight only) to the brightness when the planet is beside the star (light from the star and planet combined) the team was able to calculate the amount of mid-infrared light with wavelengths of 15 microns given off by the dayside of the planet. This method is the same as that used by another research team to determine that TRAPPIST-1 b, the innermost planet in the system, is probably devoid of any atmosphere. The amount of mid-infrared light emitted by a planet is directly related to its temperature, which is in turn influenced by atmosphere. Carbon dioxide gas preferentially absorbs 15-micron light, making the planet appear dimmer at that wavelength. However, clouds can reflect light, making the planet appear brighter and masking the presence of carbon dioxide. In addition, a substantial atmosphere of any composition will redistribute heat from the dayside to the nightside, causing the dayside temperature to be lower than it would be without an atmosphere. (Because TRAPPIST-1 c orbits so close to its star - about 1/50th the distance between Venus and the Sun - it is thought to be tidally locked, with one side in perpetual daylight and the other in endless darkness.) Although these initial measurements do not provide definitive information about the nature of TRAPPIST-1 c, they do help narrow down the likely possibilities. "Our results are consistent with the planet being a bare rock with no atmosphere, or the planet having a really thin CO2 atmosphere (thinner than on Earth or even Mars) with no clouds," said Zieba. "If the planet had a thick CO2 atmosphere, we would have observed a really shallow secondary eclipse, or none at all. This is because the CO2 would be absorbing all of the 15-micron light, so we wouldn't detect any coming from the planet." The data also shows that it is unlikely the planet is a true Venus analog with a thick CO2 atmosphere and sulfuric acid clouds. The absence of a thick atmosphere suggests that the planet may have formed with relatively little water. If the cooler, more temperate TRAPPIST-1 planets formed under similar conditions, they too may have started with little of the water and other components necessary to make a planet habitable. The sensitivity required to distinguish between various atmospheric scenarios on such a small planet so far away is truly remarkable. The decrease in brightness that Webb detected during the secondary eclipse was just 0.04 percent: equivalent to looking at a display of 10,000 tiny light bulbs and noticing that just four have gone out. "It is extraordinary that we can measure this," said Kreidberg. "There have been questions for decades now about whether rocky planets can keep atmospheres. Webb's ability really brings us into a regime where we can start to compare exoplanet systems to our solar system in a way that we never have before." This research was conducted as part of Webb's General Observers (GO) program 2304, which is one of eight programs from Webb's first year of science designed to help fully characterize the TRAPPIST-1 system. This coming year, researchers will conduct a follow-up investigation to observe the full orbits of TRAPPIST-1 b and TRAPPIST-1 c. This will make it possible to see how the temperatures change from the day to the nightsides of the two planets and will provide further constraints on whether they have atmospheres or not.
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itsgerges · 1 year
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Best Greetings
Why Does Mercury Day Period Equal =176 Solar Days?
The answer is summarized in three point
1-Preface
2-The Rate Of Time Definition
3-The Rate Of Time Using
 1-Preface
The rate of time shows 2 major problems in the physics book
 First problem
The rate of time can't be discovered by the planets motions observation- because- while we observe the planets motions we can't conclude that each planet has its own clock and by that the motions be done based on some system we know nothing about
One method only by which the rate of time can be discovered which is the planets data analysis because we can discover each planets uses its own clock by comparison the planets data one another.
Shortly - The planets data analysis neglect causes to hide the most important part of the solar system motion-
 Second problem
The sun rays is created by the planets motions energies- means -  the sun is not doing nuclear fusion to produce its rays- instead- the planets motions energies total be used as the source of energy to produce the sun rays  
Understandable the planet motion energy is so small and isn't sufficient to produce the light beam – for that reason – the rate of time is used to accumulate the motion energy
Means
The planet motion energy is accumulated day after day during a period of time and when this energy is enough to produce the light beam the energy be used  
Shortly
The rate of time is the method by which the planets motions energies be accumulated, that explains the major effect of the rate of time using- it accumulates the energy –
I want to say
The rate of time is the treasure in which the solar system puts its energy -  and by that- all basic actions in the solar system is done to enable the using of the rate of time or to use the energy be stored by the rate of time –  
I explain (why it's so pity) the science didn't use the planets data analysis– because- the rate of  time is solar system backbone – it's the main motor behind the machine and no clear understanding for the solar system motion can be caught without the rate of time understanding.
Briefly
The real machine is so different from that one be explained currently -  the gap is created by the neglect for the planets data analysis.
2-The Rate Of Time Definition
 (1) (The Rate Of Time Meaning)
The rate of time  means – each planet has its own clock –
 The rate of time is defined by the velocities rate –
For  example – Earth velocity (29.8 km/s) = Pluto velocity (4.7 km/s) x 6.3
Based on that – one hour of Earth clock = 6.3 hours of Pluto clock
This is the method by which the rate of time be created
 (2) (The Rate Of Time Reason)
The solar system is created out of  one light beam energy- means- the planets matters and their distances are created from one energy and this one energy is one light beam energy –
Shortly – the planets are geometrical points found on one light beam – and the planets move with this light beam motion.
By that –
The planets be similar to carriages in one train and the light beam is this train engine – this idea explains perfectly the real motion of the solar planets
Now –
The light moves (one motion) and passes (one distance) in (one period of time)
And
Because the light moves with all planets – for that –
The planets have to move (this same motion) and pass (this same distance) in (this same period of time)
Shortly- the planets move (equal distances) in (equal periods of time)
And – because the planets velocities are different that necessitates to use rates of time for the planets motions –
 (3) (The Rate Of Time Geometrical Effect)
Let's consider a river of water
The engineer creates some tool to control the passed amount of water from a point to another – they control the rate of passing water by this tool
Similar to that –
The solar system is a continuum of energy– means -  the planets matters and distances are created from the same one energy (light beam energy) and this one energy is in motion – the rate of time defines the amount and direction of the passed energy from a point to another –
(4) (The Useful Result Of The Rate Of Time Using)
The rate of time helps to accumulate the motion energy
The planet moves and produces motion energy daily, the rate of time causes to store this motion energy daily – by that the energy can be accumulated day after day
(5) (The Rate Of Time Real Effect)
Let's summarize this effect in following
(a)
The space has mechanical features
In details - The space is similar to the sea of water and the planet motion energy creates a wave in the space, this wave is similar to the water wave and it moves far from  its source and can be reflected typically as the water wave –
(b)
Because the planets revolve around the sun in the same one direction the motion energies create waves  move in the same direction (toward Pluto) perpendicular  on the revolution direction-    
In Pluto orbit the energies be unified together into one unified energy  
And
(c)
The unified energy wave is reflected from Pluto toward Venus -  means-  the wave is reflected from Pluto to Neptune then to  Uranus and reach to Saturn (but) – in  Saturn the wave is reflected one more time inside the planet body (as if the planet body be similar to two mirrors and the energy is reflected between them) – then the wave  left Saturn moves in the same original direction toward Venus – and the wave reach Venus – then – Venus reflected the wave to Mars and the wave energy is stored in the Earth moon orbit between Venus and Mars    
(d)
Shortly
The planets motions energies total is stored in the moon orbit in (moving wave form)
Means
There's one wave moves around the sun and this wave moves through the Earth moon orbit – and – this wave velocity = The Planets Velocities Total  
This is the wave in which the energy will be stored and the rate  of time will have effect on this wave to cause to accumulate the energy
Let's see how that can be done
(e)
The energy is stored in (a moving wave form) and this wave revolves around the sun moves by velocity (= the planets velocities total)
Then – let's ask (How Can We Increase The Energy Of This Wave?)
By increasing its relative motion velocity- what does that mean??
 The wave revolves around the sun point- The revolution motion causes to create 2 velocities on the 2 sides of the sun point – these 2 velocities are equal in value and opposite in direction –then the total is Zero – means- the revolution motion creates a stationary point in the center –
Based on that - We have a relative motion between 2 points
The unified wave motion moves by the planets velocities total and the sun point of space its velocity is (Zero) relative to this wave motion      
Shortly
The wave moves by velocity 176 km/s (The 9 Planets Velocities Total)
The sun point of space velocity (Zero)
This is the relative motion
How can we increase the energy of this relative motion?
If we can increase the different velocity between the two points– as much the different velocity be increased much energy be added
 The rate of time does a great effect because it uses this wave its velocity 176 km/s and causes to increase its velocity to be (300000 km/s)
We should discuss that in the next point
 Now we understand how the rate of time works and what's its effect on the solar system motion.
 Notice
The creation of the moving wave around the sun – this idea I have proved and discussed in details in my previous paper- please review it for all details because here I can't analyze the planet motion energy because I try to explain in details how the rate of time works in the solar system
My previous paper
The Mass Gravity Force Can't Cause Any Motion (Newton Definition Is Wrong)
 In following I explain how the rate of time works – and – I use this energy wave which revolves around the sun – this wave its velocity 176 km/s and the sun point velocity Zero
This is the basic tool  to explain how the rate of time works and be used
Let's do that in the next point
 3- The Rate Of Time Using
(i)
Let's refer to the basic rates of time in the solar  system before to discuss how the rate of time works
There are 3 basic rates of time we should know
 First rate is (One Second Of Light Clock = One Solar Day Of A Planet Clock)
This rate is produced by the planet creation from the light beam energy
 Second rate is (One Second Of Mercury Clock = 24 Seconds Of Any Planet Clock)
This is the solar system general rate
 Third rate is (One Second Of Any Planet Clock = 24 Seconds Of Saturn Clock) and by that (One Second Of Mercury Clock = 576 Seconds Of Saturn Clock)
Later I should explain and prove how these rates are created.
Now let's see how the rate of time works in following
(ii)
We know – the planets motions energies are unified together into one wave revolving around the sun- this wave motion creates a relative motion with the sun point of space  Means- we have a relative motion between the wave motion (its velocity =176  km/s) and the sun point of space (its velocity Zero) and by that the different velocity is 176 km/s.
Where (V1)= 176 km/s = The 9 Planets Velocities Total   and
(V2) = Zero = The Sun Point Of Space Velocity
 (iii)
We know the rate of velocities creates the rate of time – and we have 2 velocities
V1= 176 km/s and V2= Zero
Based on that – a rate of time will be created – which is (1 second = 176 seconds)
Means
One Second Of The Wave Clock = 176 Seconds Of The Sun Clock
But
The wave is reflected as I have explained and proved before
The reflection of energy causes to reflect the players and as a result  
One Second Of The Sun Clock = 176 Seconds Of The Wave Clock
And
One Solar Day Of The Sun Clock = 176 Solar Days Of The Wave Clock
 This rate is very effective in our discussion for two reasons -  
First reason because– the sun obliquity is 7.25 degrees where the inclination and obliquity is considered as a rate of  time means this value (7.25) causes a rate of time between the sun and Mercury
Shortly
One second of the sun clock = 7.25 seconds of Mercury clock
And
One second of Mercury clock = 24 seconds of any planet clock
By that
One second of the sun clock = 176 seconds of any planet clock – that causes
One second of the sun clock = 176 seconds of the wave clock
 (iii)
Second reason
(One Solar Day Of The Sun Clock = 176 Solar Days Of The Wave Clock)
We know that – 176 solar days = Mercury Day Period
Also – the sun has no a day by definition
Because – the planet days is created by its rotation around its axis in front of the sun- the sun itself has no day period
For that -  the sun uses Mercury day period in place of its own day because Mercury is the most near planet to the sun
 That means- Mercury day period =176 solar days because the 9 planets velocities total =176 km/s
Here we have no any confusion with Mercury rate of time (1=24) -  Mercury day (176 days) is defined for the sun rate and not for Mercury rate.
 (iv)
As we know the rate of time is created by the velocities rates-  for that we have to ask – how can Mercury have one rate of time with all planets?
The answer is understandable by the data -  because the rate depends on the velocity 176 km/s which is the 9 planets velocities total – means – mercury depends on the velocities total to create one rate of time with all planets –as we have seen
The rate is (1 =176) and the sun obliquity (7.25 deg) causes (176 =24 x 7.25)  and by that Mercury rate of time be (one second on Mercury clock = 24 seconds of and planet clock)
That tells (because of the interaction between the sun and Mercury) – Mercury has this chance to have one rate of time with all planets
Notice
The reflection of energy (inside Saturn) caused to double its rate and by that the rate (1=24) is doubled to be (1=576)
This relationship is done between Saturn and Mercury and by that Saturn depends on Mercury to create one rate of time for  himself with all planets which is
(one second of any planet clock = 24 seconds of Saturn clock)    
 (v)
Why does Mercury move in its day  period (176 solar days)  a distance =720 million km = Mercury Jupiter distance?
This behavior is similar to Venus and earth behaviors- because –
Venus Jupiter distance= 671 mkm and Venus orbital circumference =680 mkm (1.2%)  
And
Earth Jupiter distance= 929 mkm and Earth orbital circumference =940 mkm (1.2%)  
We have to discuss this data later with other questions as
Why does Mercury day period = 2 its orbital period =3 its rotation period?
Where
Mercury moves in its rotation period a distance 240 million km  
Mercury moves in its orbital period a distance 360 million km  
More data
(1.6)^3 x 2 x 176 days = 1461 days
176= 24 x 7.25 = 7 x 25.2  
But (58.66/88) = cos (41.8)
Notice
We understand that Mercury day period causes Mercury to rotate around its axis through the same ancient point – means -  Mercury doesn't change its starting point of rotation in each day period – means – Mercury depends on the ancient design of the solar system.
Thanks a lot - Kind regards
Speed Of Light Has An Effect On Matter Creation Process
https://www.academia.edu/s/053a0a794e
or
https://www.academia.edu/98508585/Speed_Of_Light_Has_An_Effect_On_Matter_Creation_Process
or
https://app.box.com/s/tpl1shsi2m28dqo6rq6x6j7ncid0zl4g
or
https://app.box.com/s/x52am353v74fwieeodg4a73yv9c31l2r
Gerges Francis Tawdrous +201022532292
Physics Department- Physics & Mathematics Faculty  
Peoples' Friendship university of Russia – Moscow   (2010-2013)
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kissingdeadgirls · 2 years
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this weekend i watched iwtv, the terror (first half very beautiful and comprehendable, second half i have some questions), the bear (everything tumblr said it was), and the expanse (almost done the second season)
some thots on the expanse so far
i wasn’t sure i liked most of the first season, but was stuck in bed, so i powered through it. and i miss shitty cable sci-fi. it’s the first space show i’ve seen since sgu, lmao.
the first season very much Feels Like A Book. that way books are so particular about all the threads connecting, where television (esp kinda b sci-fi shows) are more lax. this is especially charming.
the expanse has a very small amount of fanfic? i am avoiding spoilers, i just wanted to see!, but it’s f/f is the biggest category? and the top ship is the hot milf? god is good? i love chrisjen. holy shit.
i also do not know anyones name and spoiled myself trying to look some up. you should not pay for streaming services ever, and esp not pr*me who gives you a fucking ad in between each eps, but on the other hand if you want to know characters names without looking them up on the database where you will learn the number of eps they’re in, or a wiki which will spoil everything in a single sentence, the nightmare x-ray gimmick is actually pretty useful. sorry.
i just wanted to know drummer’s name so i could more adequately imagine her and naomi getting married in the mormon chapel (slow burn, 200k, au) (racket ball after game, 5k, explicit) (anarchist book club coffee shop au, 20k, archive locked).
took a lil break because i am currently frustrated with naomi’s characterization, where it doesn’t feel like she’s being given the room to be the moral centrepiece but actually just a wet blanket. like. this truncated version of her is making me want to scream. she’s not that!!!! and it’s so close to being a good continuation of her arc but fails to be and it’s driving me to violence.
trying to imagine changes that would have taken up the same amount of screen time but would have been more effective:
having the crew bust in to the aid ship in 2x09 the weeping somnambulist, being like: i am holden, saver of worlds, instead of mars cosplay. using this to really lead in to naomi’s distaste for Causes and jim’s newfound expediency through violence. having the pirates only go for the 10% (20% if you want to give a bone to jim, which i don’t) and not be especially murderous, (which also reaffirms the mundanity of this kind of violence, it’s structural) and then still having jim choose to be the hero to deleterious effect. those scenes dragged for a thousand years and blew chunks, and they seriously undercut naomi’s character and politics (and the politics of the show).
like. wrt the vulture preying on families looking to get reunited with stolen security access. is that the best example of violence as expediency and holden’s impaired judgement coming to align with amos (my belovéd)? i would personally break his legs for free. which again leaves…. wet blanket :(
idk i just think that would be a more useful base to cut from. idk!!! just really truncated her!!! the 10 second scene of her and pax mentioning her lost son in the hallway. like. the narrative about state experimentation on children doesn’t care about these kids at all huh.
a final note: having miller and julie die naked while being consumed by the alien life force, embracing a nuclear bomb is so comically close to being My Shit™ but i do not condone heterosexuality like that. also having an ingenue and not having her be gay about it is simply bad writing. and finally having her naked in her final scene (which is also the only one where we see her in real time) be naked (literal male gaze) is just so fucking boring. if they weren’t going to put her in the razorback gear (and then transforming to her dead self as they embraced etc) they should have just used the consumed state. i also hated that her solar plexus was exposed. we deserve so much better than that.
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jcmarchi · 4 months
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NASA’s Fermi Detects Surprise Gamma-Ray Feature Beyond Our Galaxy - Technology Org
New Post has been published on https://thedigitalinsider.com/nasas-fermi-detects-surprise-gamma-ray-feature-beyond-our-galaxy-technology-org/
NASA’s Fermi Detects Surprise Gamma-Ray Feature Beyond Our Galaxy - Technology Org
Astronomers analyzing 13 years of data from NASA’s Fermi Gamma-ray Space Telescope have found an unexpected and unexplained feature outside our galaxy.
This artist’s concept shows the entire sky in gamma rays with magenta circles, illustrating the uncertainty in the direction from which more high-energy gamma rays than average seem to be arriving. In this view, the plane of our galaxy runs across the middle of the map. The circles enclose regions with a 68% (inner) and a 95% chance of containing the origin of these gamma rays. Image credit: NASA’s Goddard Space Flight Center
Intriguingly, the gamma-ray signal is found in a similar direction and with a nearly identical magnitude as another unexplained feature, one produced by some of the most energetic cosmic particles ever detected.
A paper describing the findings was published in The Astrophysical Journal Letters.
The team was searching for a gamma-ray feature related to the CMB (cosmic microwave background), the oldest light in the universe. Scientists say the CMB originated when the hot, expanding universe had cooled enough to form the first atoms, an event that released a burst of light that, for the first time, could permeate the cosmos. Stretched by the subsequent expansion of space over the past 13 billion years, this light was first detected in the form of faint microwaves all over the sky in 1965.
In the 1970s, astronomers realized that the CMB had a so-called dipole structure, which was later measured at high precision by NASA’s COBE (Cosmic Background Explorer) mission. The CMB is about 0.12% hotter, with more microwaves than average, toward the constellation Leo, and colder by the same amount, with fewer microwaves than average, in the opposite direction. In order to study the tiny temperature variations within the CMB, this signal must be removed. Astronomers generally regard the pattern as a result of the motion of our own solar system relative to the CMB at about 230 miles (370 kilometers) per second.
This motion will give rise to a dipole signal in the light coming from any astrophysical source, but so far the CMB is the only one that has been precisely measured. By looking for the pattern in other forms of light, astronomers could confirm or challenge the idea that the dipole is due entirely to our solar system’s motion.
“Such a measurement is important because a disagreement with the size and direction of the CMB dipole could provide us with a glimpse into physical processes operating in the very early universe, potentially back to when it was less than a trillionth of a second old,” said co-author Fernando Atrio-Barandela, a professor of theoretical physics at the University of Salamanca in Spain.
The team reasoned that by adding together many years of data from Fermi’s LAT (Large Area Telescope), which scans the entire sky many times a day, a related dipole emission pattern could be detected in gamma rays. Thanks to the effects of relativity, the gamma-ray dipole should be amplified by as much as five times over the currently detected CMB’s.     
The scientists combined 13 years of Fermi LAT observations of gamma rays above about 3 billion electron volts (GeV); for comparison, visible light has energies between about 2 and 3 electron volts. They removed all resolved and identified sources and stripped out the central plane of our Milky Way galaxy in order to analyze the extragalactic gamma-ray background.
“We found a gamma-ray dipole, but its peak is located in the southern sky, far from the CMB’s, and its magnitude is 10 times greater than what we would expect from our motion,” said co-author Chris Shrader, an astrophysicist at the Catholic University of America in Washington and at Goddard. “While it is not what we were looking for, we suspect it may be related to a similar feature reported for the highest-energy cosmic rays.”
Cosmic rays are accelerated charged particles – mostly protons and atomic nuclei. The rarest and most energetic particles, called UHECRs (ultrahigh-energy cosmic rays), carry more than a billion times the energy of 3 GeV gamma rays, and their origins remain one of the biggest mysteries in astrophysics.
Since 2017, the Pierre Auger Observatory in Argentina has reported a dipole in the arrival direction of UHECRs. Being electrically charged, cosmic rays are diverted by the galaxy’s magnetic field by different amounts depending on their energies, but the UHECR dipole peaks in a sky location similar to what Kashlinsky’s team finds in gamma rays. And both have strikingly similar magnitudes – about 7% more gamma rays or particles than average coming from one direction and correspondingly smaller amounts arriving from the opposite direction.
The scientists think it’s likely the two phenomena are linked – that as yet unidentified sources are producing both the gamma rays and the ultrahigh-energy particles. To solve this cosmic conundrum, astronomers must either locate these mysterious sources or propose alternative explanations for both features.
The Fermi Gamma-ray Space Telescope is an astrophysics and particle physics partnership managed by Goddard. Fermi was developed in collaboration with the U.S. Department of Energy, with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the United States.
Source: National Aeronautics and Space Administration
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solarpanelsau · 5 months
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Why Choosing Premier Solar Panels Installation is Crucial for Sustainability?
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Source: Why Choosing Premier Solar Panels Installation is Crucial for Sustainability?
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spacenutspod · 5 months
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In 2023, researchers made plenty of discoveries for the record books — and the history books. This year’s scientific superlatives shed new light on our ancient ancestors, our planet and the animals we share it with. Least sleep among mammals However sleep-deprived you may be, you’re probably still better rested than a northern elephant seal. During monthslong hunting trips at sea, these seals nap less than 20 minutes at a time and average just two hours of total sleep per day. That rivals African elephants for the title of mammal that sleeps the least (SN: 4/20/23). Earliest equestrians The Yamnaya people may have been the world’s earliest horseback riders, mounting steeds as far back as 3000 B.C., centuries before the earliest known depictions of horseback riding (SN: 4/8/23, p. 12). Yamnaya skeletons unearthed in Romania, Bulgaria and Hungary show telltale signs of horsemanship, including marks on the femur and pelvis that could come from sitting astride and vertebral damage from falling off. Several skeletons from the ancient Yamnaya people, including the one shown here, bear signs that they may have ridden horses around 5,000 years ago. That would make them the earliest known horseback riders.MICHAŁ PODSIADŁO Sunniest place on Earth Visitors to the Altiplano plateau in Chile’s Atacama Desert should be sure to pack sunscreen. This high-altitude region gets hit with an average of 308 watts of sunshine per square meter — the most intense sunlight anywhere on Earth (SN: 8/26/23, p. 5). Sometimes, solar radiation exceeds 2,000 watts per square meter, rivaling the amount of sunshine expected to beat down on Venus, which is much closer to the sun than Earth is. A researcher working high in the Chilean Andes sets up an instrument to measure solar radiation. The region’s Altiplano plateau gets the most intense sunlight on Earth. Raúl Cordero Oldest back hole A supermassive black hole some 13.2 billion light-years from Earth is the most distant, most ancient supermassive black hole ever observed. The monster dates to when the universe was just 470 million years old, making it about 200 million years older than a record breaker announced in 2021 and 100 million years older than a black hole that claimed the title in July (SN: 12/18/21 & 1/1/22, p. 29). Because the newfound black hole boasts about the same heft as its surrounding galaxy, researchers think the black hole could have formed only through the collapse of a massive gas cloud. The finding could help shed light on how the universe’s first generation of juggernaut black holes were born. This composite image, made with data from NASA’s Chandra X-ray Observatory and James Webb Space Telescope, shows the most distant, most ancient supermassive black hole ever observed (left inset) and its host galaxy (right inset).X-ray: NASA/CXC/SAO/Ákos Bogdán; Infrared: NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/L. Frattare & K. Arcand Snappiest claws Famously fast adult snapping shrimp have nothing on their young. High-speed video reveals that youngsters can snap their claws up to about 600 kilometers per second per second — an acceleration 20 times as fast as their elders achieve. A 1-month-old shrimp’s claw acceleration is on the same order of magnitude as a 9-millimeter bullet blasting out of a gun and is the highest acceleration for a reusable body part underwater (SN: 4/8/23, p. 5). It takes less than a millisecond for a juvenile snapping shrimp (Alpheus heterochaelis) to slam its claw shut. But thanks to footage taken at 300,000 frames per second and then slowed down by 10,000 times, the human eye can capture this extreme acceleration and the imploding bubble it creates. Oldest wooden structure Despite what happened to the second little pig’s house, wood has long proved a sturdy, reliable construction material — for perhaps as long as half a million years. Carved, interlocking logs uncovered in Zambia date to nearly 480,000 years ago, making them the oldest known wooden structure (SN: 9/20/23). The structure — possibly a remnant of a walkway, seating area or storage unit — hints that some human relatives may have led a less nomadic lifestyle than previously thought. Since wood decays quickly, ancient wooden artifacts are rare. But two interlocked logs found in Zambia may have been part of a hominid-built structure 476,000 years ago. LARRY BARHAM/UNIV. OF LIVERPOOL Heaviest animal ever The animal kingdom appears to have a new heavyweight champion. An extinct whale aptly named Perucetus colossus might have weighed up to 340 metric tons, about twice as much as the heaviest blue whales, an analysis of fossils found in Peru suggests (SN: 9/9/23, p. 5). The mighty mammal is thought to have prowled shallow waters 39 million years ago — but what it could have eaten to maintain its size remains a mystery. The ancient whale Perucetus colossus (illustrated) might have edged out blue whales for the title of heaviest known animal, possibly weighing up to 340 metric tons.ALBERTO GENNARI
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dzthenerd490 · 5 months
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File: Infamous - The Beast
SCP#: ATV
Code Name: The Beast
Object Class: Keter
Special Containment Procedures: SCP-ATV's essence has been transferred to an updated Q/A-CC device mark 42. This one is designed to not only contain SCP-ATV's Ray Field Radiation but also siphon the atomic energy produced from its essence. This is done to help fuel the entirety of Site-AN where SCP-ATV is contained. It should be noted that the original Artificial Star Core Reactor (ASCR) was not discharged but instead used as an emergency source of energy should SCP-ATV ever break containment or if it someday runs out of energy. 
The Q/A-CC-42 device is locked within a cooling room connected to the main power station and emergency energy storage unit of Site-AN. The Cooling room is outfitted with 200 canisters of Nitrogenic Gas placed all around and outside the room. The canisters will fill the room and everywhere around the room with the gas should a containment breach occur preventing SCP-ATV from taking advantage and escaping. 
Should this fail Mobile Task Force Zeus-1 "Conduits" Division "Ice" is to be deployed at Site-AN with the sole purpose of containing SCP-ATV. If they fail, then MTF Zues-1 Division "Destruction" is to be deployed with the experimental Q/A/R-FG-50 device. 
Description: SCP-ATV is an extremely unique member of the artificially created Species of Interest: Conduits. What makes SCP-ATV unique is that he never needs to recharge his energy by absorbing his designated element. Instead, SCP-ATV can produce an infinite amount of heat, fire, and atomic energy any time he desires. Though this process is sped up when his body is exposed to some form of energy, the most useful being the solar rays of the sun. 
Despite SCP-ATV being sentient, it's quite difficult for him to control his powers all the time and often needs to expel a majority of it to control it. Otherwise, his energy controls him and builds him up into a Large-Scale Anomaly with the size of 200 feet tall and a body made of radioactive molten magma as well as atomic energy. In this form SCP-ATV will find every human with the ability to evolve into a SoI: Conduit and fill them with RF Radiation while also unintentionally filling everyone he comes across with the same radiation. 
Most who get exposed to RF Radiation during a birth of a Conduit get killed by being transformed into energy that infuses into the newly birthed Conduit becoming the foundation for their new body and powers. This process is quite similar to how SCP-ATQ can turn any human that uses it when surrounded by other humans into Conduits. Though unlike SCP-ATQ, SCP-ATV can only do this to those that are compatible enough to become Conduits. Furthermore, anyone who is not compatible but doesn't get transformed into energy suffers from RF Radiation poisoning. 
RF Radiation poisoning is a result of exposure to SCP-ATV and its massive amount of atomic energy. The symptoms include slow but painful cellular decay, organ failure, and eventual death. The terrifying aspect of RF Radiation is that its highly infectious, only modern Foundation medicine was able to find a vaccine and cure from the plague. Regardless, SCP-ATV's ability to find humans and turn them into conduits as well as create an infectious RF Radiation plague has made it an obvious SK Class Dominance Shift Scenario Hazard, with the end result being humanities extinction. It is for this reason that SCP-ATV has been contained at Site-AN and not at Site-AO despite technically being an LSA. Because of SCP-ATV's hazardous radiation it is unknown as to why SCP-ABQ never bothered to attack SCP-ATV or at the very least, use it as some kind of food source. 
“Guess we can’t rely on the big guy forever; guess he was trying to tell us that we need to be at least strong enough to save ourselves every so often. You might think I’m stretching by that lizard is a lot smarter than most give it credit.” MTF High Commander Riker
SCP-ATV was discovered in 2011 within the secluded and now destroyed Empire City. It was filled with great power and close to destroying the city, so the Foundation and Global Occult Coalition mobilized their space fleets and launched an orbital bombardment. This was believed to be the end of SCP-ATV but in reality, it was still alive. Unfortunately, that wasn't all that was discovered later in the year. 
A Splinter Cell within the Horizon Initiative was discovered to secretly be trying to create living weapons from Species of Interest: The Conduits. They did this to sell them to terrorists and warlords to scare and build hate in the hearts of the people of the world against the anomalous and the godless. Though they failed and were all either executed or prosecuted as D Class personnel within the Foundation. After their intel was recovered it was discovered that SCP-ATV was alive and within the waters of the Atlantic Ocean. It was swimming towards the secluded small city of New Marais while spreading its RF Radiation off the East Coast of the United States. Though thankfully the Foundation was not only able to make a cure in the same year but also found SCP-ATV and contained it with Mobile Task Force Alpha-1 "Red Right Hand". Please see Tales: Formation of Mobile Task Force Zeus-1 “Conduits” for details. 
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SCP: Horror Movie Files Hub
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theexpertsnotebook · 1 year
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Gravitational Lensing & the Cosmos: Quasars, Galaxies, Mass
Exploring the Fascinating World of Gravitational Lensing, Mass, Quasar, and Galaxy
Introduction
The universe is a vast and mysterious place that has captivated human curiosity for ages. Its secrets have been slowly unravelled over time through the scientific method, observation, and experimentation. One of the most intriguing phenomena in our universe is gravitational lensing. Gravitational lensing is an optical phenomenon that occurs when light from a distant object is bent by a massive object such as a galaxy or cluster of galaxies. This bending of light can create multiple images or distortions of the original source, resulting in impressive visual effects.
Definition of Gravitational Lensing
Gravitational lensing was first predicted by Albert Einstein's theory of general relativity in 1915. According to Einstein's theory, mass warps space-time around it, causing light to bend as it travels through that curved space-time. In other words, massive objects such as galaxies and clusters act like lenses that bend and magnify the light coming from behind them. This effect can be likened to looking through a windowpane that has been distorted due to irregularities. Gravitational lensing can be categorized into three types: strong gravitational lensing occurs when multiple images are produced around the massive object; weak gravitational lensing occurs when slight distortions are created but no multiple images are formed; microlensing happens when small-scale objects like stars produce temporary brightenings in background sources.
Importance of Mass in Gravitational Lensing
The key factor affecting gravitational lensing is mass; specifically, the amount of mass present between an observer on earth and a distant source behind it will determine how much bending will occur. Therefore, astronomers use gravitational lensing as an indirect way to measure invisible dark matter since it affects the bending of light in the same way as visible matter. Gravitational lensing is a powerful tool for studying dark matter as it allows astronomers to map its distribution and study its properties.
Brief Overview of Quasars and Galaxies
Quasars are incredibly bright objects in space that emit vast amounts of energy. They are located in the center of galaxies and are powered by supermassive black holes that consume material from surrounding gas and dust. Quasars emit light at different wavelengths, including radio, infrared, visible, ultraviolet, X-ray, and gamma rays. On the other hand, galaxies are massive structures in space comprising stars, gas clouds, dust particles, and dark matter. They come in various shapes - spiral galaxies like our Milky Way have arms that emerge from a central disk while elliptical galaxies appear round or oval-shaped. These structures play an essential role in gravitational lensing as they can act as lenses themselves due to their mass. Understanding gravitational lensing is crucial to understand some of the most profound mysteries of our universe such as dark matter and dark energy. In this article series exploring gravitational lensing with mass using quasars and galaxies will provide insights for readers into scientific discoveries enabled by these fields' integration toward better scientific understanding about universe's composition.
The Wonders of Gravitational Lensing
Gravitational lensing is a fascinating phenomenon that occurs due to the bending of light caused by the mass of an object. This bending effect creates a distortion in the image of a background object, such as a galaxy or quasar, allowing scientists to study distant objects that would otherwise be impossible to observe. The first observation of gravitational lensing was made in 1919 during a solar eclipse by Arthur Eddington, testing Einstein's general theory of relativity.Read more
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myfeeds · 1 year
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An X-ray look at the heart of powerful quasars
Hosted by a galaxy 9.6 billion light years away from the Earth, between the constellations of Centaurus and Hydra, J1144 is extremely powerful, shining 100,000 billion times brighter than the Sun. J1144 is much closer to Earth than other sources of the same luminosity, allowing astronomers to gain insight into the black hole powering the quasar and its surrounding environment. The study was led by Dr Elias Kammoun, a postdoctoral researcher at the Research Institute in Astrophysics and Planetology (IRAP), and Zsofi Igo, a PhD candidate at the Max Planck Institute for Extraterrestrial Physics (MPE). Quasars are among the brightest and most distant objects in the known universe, powered by the fall of gas into a supermassive black hole. They can be described as active galactic nuclei (AGN) of very high luminosity that emit vast amounts of electromagnetic radiation observable in radio, infrared, visible, ultraviolet and X-ray wavelengths. J1144 was initially observed in visible wavelengths in 2022 by the SkyMapper Southern Survey (SMSS). For this study, researchers combined observations from several space-based observatories: the eROSITA instrument on board the Spectrum-Roentgen-Gamma (SRG) observatory, the ESA XMM-Newton observatory, NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR), and NASA’s Neil Gehrels Swift observatory. The team used the data from the four observatories to measure the temperature of the X-rays being emitted from the quasar. They found this temperature to be around 350 million Kelvin, more than 60,000 times the temperature at the surface of the Sun. The team also found that the mass of the black hole at the quasar’s centre is around 10 billion times the mass of the Sun, and the rate at which it is growing to be of the order of 100 solar masses per year. The X-ray light from this source varied on a time scale of a few days, which is not usually seen in quasars with black holes as large as the one residing in J1144. The typical timescale of variability for a black hole of this size would be on the order of months or even years. The observations also showed that while a portion of the gas is swallowed by the black hole, some gas is ejected in the form of extremely powerful winds, injecting large amounts of energy into the host galaxy. Dr. Kammoun, lead author of the paper, says “We were very surprised that no prior X-ray observatory has ever observed this source despite its extreme power.” He adds, “Similar quasars are usually found at much larger distances, so they appear much fainter, and we see them as they were when the Universe was only 2-3 billion years old. J1144 is a very rare source as it is so luminous and much closer to Earth (although still at a huge distance!), giving us a unique glimpse of what such powerful quasars look like.” “A new monitoring campaign of this source will start in June this year, which may reveal more surprises from this unique source.”
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5 reasons to go for louvered aluminum patio roof
Patio roofs are a valued addition to modern homes. Having a shaded patio is great for creating a comfortable and relaxing outdoor living space. The patio roof makes your outdoors a year-round seating space. In summer, the patio covers are helpful in blocking harmful UV rays and improving energy efficiency. Spring season drizzle can be prevented by having a patio roof. Besides, you can extend the life of your furniture. 
From the conventional choice of wood to innovative solutions of aluminum and fiber, the options are endless. However, the aluminum patio has become the talk of the town. Here are the top 5 reasons that advocate investing in aluminum patios.
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Superior heat blocking capabilities
If you live in an area with high summer sun, investing in an aluminum patio roof is highly beneficial. The material efficiently blocks sun rays and reduces heat while it still maintains ventilation. Besides, if you opt for a louvered patio roof, you get the option to regulate the amount of sunlight and temperature under the roof.
All year protection 
Aluminum is a versatile material that protects your patio from harsh climatic conditions. Whether it is raining or snowing outside, you can enjoy quality time with your loved ones under the patio roof. Aluminum works efficiently and offers optimum protection in every weather.
Amazing durability
Wood can rot or warp, fiberglass can also damage under harsh sun, but aluminum is a robust material that stands the test of time. Aluminum shade structures come with a long lasting finish, hence the color remains the same. From the rainy season to the harsh summer, the roof will look like new forever. Unlike a rotting wood structure or conventional metal roof, you don’t have to worry about pests or rust. Aluminum is a rust-resistant material that offers superior value for money performance.
Low maintenance 
Invest in extruded aluminum patio covers and rest assured. There is no need to repair, repaint or maintain the aluminum patio roof every year. Annual maintenance is a big concern when you invest in wooden structures. On the other hand, aluminum roofs are like a set it and forget it option due to their weatherproof performance.
Customization 
Another reason that makes aluminum the unrivaled hero for patio roofing is the provision for customization. You don’t have to compromise on the aesthetics because the latest innovation has made it possible to get a style that seamlessly integrates into your existing architectural style. There are tons of colors and finish options to choose from. 
Which are the best-selling aluminum patio covers near me?
Now that you know that investing in an aluminum patio cover is a worthy investment. You might want to learn more about the best seller in the industry. If you want to transform the outdoor seating area, invest in an Equinox louvered roof. It is made from precision engineered extruded aluminum and has become the ultimate shading solution.
Equinox louvered roof can go from fully open to fully shut with the touch of a button. The motorized operation offers the benefit of user friendliness and optimum functionality. Equinox louvered roof can be customized according to style and aesthetic preferences. Besides, the options of remote control and solar battery have made these roofing structures the conversation starters at house parties.
Conclusion
Aluminum is rust resistant, durable, and offers superior weather protection. In popular options, Equinox louvered roof is the best choice to create a relaxing outdoor environment. Those who are thinking about where to buy the Equinox aluminum patio cover near me can get a quote from Bluebonnet Patio Covers. They are Equinox certified and authorized dealers for installation and maintenance services.
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Webb rules out thick carbon dioxide atmosphere for rocky exoplanet Infrared measurements of TRAPPIST-1 c indicate that it is probably not as Venus-like as once imagined. NASA's James Webb Space Telescope has successfully measured the heat radiating from TRAPPIST-1 c, an exoplanet orbiting a red dwarf star 40 light-years from Earth. With a dayside temperature of about 225 degrees Fahrenheit, it is the coolest rocky planet ever characterized using this method. Unfortunately for those hoping that the TRAPPIST-1 system is a true analog to our own, the results are a bit disappointing. While TRAPPIST-1 c is roughly the same size and mass as Venus and receives the same amount of radiation from its star, it appears unlikely to have the same thick carbon dioxide atmosphere. This indicates that the planet, and perhaps the system as a whole, may have formed with very little water. The result is the latest in the quest to determine whether planetary atmospheres can survive the violent environs of a red dwarf star. An international team of researchers has used NASA's James Webb Space Telescope to calculate the amount of heat energy coming from the rocky exoplanet TRAPPIST-1 c. The result suggests that the planet's atmosphere—if it exists at all—is extremely thin. With a dayside temperature of roughly 380 Kelvin (about 225 degrees Fahrenheit), TRAPPIST-1 c is now the coolest rocky exoplanet ever characterized based on thermal emission. The precision necessary for these measurements further demonstrates Webb's utility in characterizing rocky exoplanets similar in size and temperature to those in our own solar system. The result marks another step in determining whether planets orbiting small red dwarfs like TRAPPIST-1—the most common type of star in the galaxy—can sustain atmospheres needed to support life as we know it. "We want to know if rocky planets have atmospheres or not," said Sebastian Zieba, a graduate student at the Max Planck Institute for Astronomy in Germany and first author on results being published today in Nature. "In the past, we could only really study planets with thick, hydrogen-rich atmospheres. With Webb we can finally start to search for atmospheres dominated by oxygen, nitrogen, and carbon dioxide." "TRAPPIST-1 c is interesting because it's basically a Venus twin: It's about the same size as Venus and receives a similar amount of radiation from its host star as Venus gets from the sun," explained co-author Laura Kreidberg, also from Max Planck. "We thought it could have a thick carbon dioxide atmosphere like Venus." TRAPPIST-1 c is one of seven rocky planets orbiting an ultracool red dwarf star (or M dwarf) 40 light-years from Earth. Although the planets are similar in size and mass to the inner, rocky planets in our own solar system, it is not clear whether they do in fact have similar atmospheres. During the first billion years of their lives, M dwarfs emit bright X-ray and ultraviolet radiation that can easily strip away a young planetary atmosphere. In addition, there may or may not have been enough water, carbon dioxide, and other volatiles available to make substantial atmospheres when the planets formed. To address these questions, the team used MIRI (Webb's Mid-Infrared Instrument) to observe the TRAPPIST-1 system on four separate occasions as the planet moved behind the star, a phenomenon known as a secondary eclipse. By comparing the brightness when the planet is behind the star (starlight only) to the brightness when the planet is beside the star (light from the star and planet combined) the team was able to calculate the amount of mid-infrared light with wavelengths of 15 microns given off by the dayside of the planet. This method is the same as that used by another research team to determine that TRAPPIST-1 b, the innermost planet in the system, is probably devoid of any atmosphere. The amount of mid-infrared light emitted by a planet is directly related to its temperature, which is in turn influenced by atmosphere. Carbon dioxide gas preferentially absorbs 15-micron light, making the planet appear dimmer at that wavelength. However, clouds can reflect light, making the planet appear brighter and masking the presence of carbon dioxide. In addition, a substantial atmosphere of any composition will redistribute heat from the dayside to the nightside, causing the dayside temperature to be lower than it would be without an atmosphere. (Because TRAPPIST-1 c orbits so close to its star—about 1/50th the distance between Venus and the sun—it is thought to be tidally locked, with one side in perpetual daylight and the other in endless darkness.) Although these initial measurements do not provide definitive information about the nature of TRAPPIST-1 c, they do help narrow down the likely possibilities. "Our results are consistent with the planet being a bare rock with no atmosphere, or the planet having a really thin CO2 atmosphere (thinner than on Earth or even Mars) with no clouds," said Zieba. "If the planet had a thick CO2 atmosphere, we would have observed a really shallow secondary eclipse, or none at all. This is because the CO2 would be absorbing all of the 15-micron light, so we wouldn't detect any coming from the planet." The data also show that it is unlikely the planet is a true Venus analog with a thick CO2 atmosphere and sulfuric acid clouds. The absence of a thick atmosphere suggests that the planet may have formed with relatively little water. If the cooler, more temperate TRAPPIST-1 planets formed under similar conditions, they too may have started with little of the water and other components necessary to make a planet habitable. The sensitivity required to distinguish between various atmospheric scenarios on such a small planet so far away is truly remarkable. The decrease in brightness that Webb detected during the secondary eclipse was just 0.04 percent: equivalent to looking at a display of 10,000 tiny light bulbs and noticing that just four have gone out. "It is extraordinary that we can measure this," said Kreidberg. "There have been questions for decades now about whether rocky planets can keep atmospheres. Webb's ability really brings us into a regime where we can start to compare exoplanet systems to our solar system in a way that we never have before." This research was conducted as part of Webb's General Observers (GO) program 2304, which is one of eight programs from Webb's first year of science designed to help fully characterize the TRAPPIST-1 system. This coming year, researchers will conduct a follow-up investigation to observe the full orbits of TRAPPIST-1 b and TRAPPIST-1 c. This will make it possible to see how the temperatures change from the day to the night sides of the two planets and will provide further constraints on whether they have atmospheres or not. The research is published in Nature. IMAGE....This artist's concept shows what the hot rocky exoplanet TRAPPIST-1 c could look like based on this work. TRAPPIST-1 c, the second of seven known planets in the TRAPPIST-1 system, orbits its star at a distance of 0.016 AU (about 1.5 million miles), completing one circuit in just 2.42 Earth-days. TRAPPIST-1 c is slightly larger than Earth, but has around the same density, which indicates that it must have a rocky composition. Webb's measurement of 15-micron mid-infrared light emitted by TRAPPIST-1 c suggests that the planet has either a bare rocky surface or a very thin carbon dioxide atmosphere. Illustrated in the background is TRAPPIST-1 b, the innermost planet in the TRAPPIST-1 system. TRAPPIST-1 b is also rocky and appears to have no substantial atmosphere. The star, TRAPPIST-1, is an ultracool red dwarf (M dwarf) with a temperature of only 2,550 Kelvin (about 4,150 degrees Fahrenheit) and a mass just 0.09 times the mass of the sun. This illustration is based on new data gathered by Webb's Mid-Infrared Instrument (MIRI) as well as previous observations from other ground- and space-based telescopes. Webb has not captured any images of the planet. Credit: Illustration: NASA, ESA, CSA, Joseph Olmsted (STScI); Science: Sebastian Zieba (MPI-A), Laura Kreidberg (MPI-A)
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sealtech5 · 1 year
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Window Replacement Chilliwack:The Latest Trends in Window Replacement
Thermal Windows
Thermal windows are one of the latest trends in new window replacement Fraser valley. Thermal windows are made to pass a high percentage of the infrared rays in the sun. This makes your home to feel warm and inviting. Currently, there are two main types of thermal windows. The first type is the dual pane thermal window. This type is made of two panes of glass, and one layer is made of a low-E glass. This type of thermal window is perfect for reducing the heat loss in your house and keeping your home warm in the winter. The second type of thermal window is the single pane thermal window. This is also made of two panes of glass, but it is made from just one layer of glass. This type of thermal window is great for reducing the heat loss in your house and keeping your home cool in the summertime.
Low-E Glass & Shatter Resistant Glass
Low-E glass and shatter resistant glass are also very common in window replacements. Low-E glass is specially designed to allow more light to enter the room and reduce the amount of blue light that is present. Blue light has been found to negatively affect the brain. This is especially true for those who suffer from issues like insomnia. Shatter resistant glass is ideal for anyone with kids or pets because it won’t shatter like regular glass will. Therefore, you won’t have to clean up a broken window and risk injuring your family or pets.
Vinyl Window Replacements
Vinyl window replacements are another big trend in window replacement. While they are not necessarily more durable than regular window materials, they are cheaper to maintain and come in a variety of colors and styles. In addition, they don’t require any special care. This means that you don’t have to worry about damaging them in the same way that you do for wood or metal windows. When it comes to choosing a vinyl replacement for your windows, you don’t want to just pick one based on price. Make sure that you consider the look and feel of the material before you commit to a certain brand.
Solar Energy Panels
Solar energy panels are becoming more and more popular. This is because they are an efficient way of generating power. What many homeowners don’t realize is that solar energy panels can be very cost-effective. This is because they don’t require an enormous initial investment. Instead, they can be paid for over time through monthly payments. In fact, this can be true even if you only use solar energy panels on your roof. This is because they are able to generate a large amount of electricity when the sun is out. This means you can use the electricity generated by the panels to power anything that you want. When it comes to choosing a solar energy panel, you want to make sure you go with a reputable brand. This is because you want to make sure that the panel you choose will generate the electricity you need while also remaining efficient.
Security Grilles
Security grilles are another common trend in New window replacement Chilliwack. These work in a similar way to the security grilles found on garage doors. This is because they are designed to prevent burglars from gaining access to your home through your windows. This is especially important if you have young children or pets. This is because it is very dangerous for these people to be exposed to these hazards. The most important thing to consider when choosing a security grille for your windows is the strength of the material. Make sure that the security grille you choose has a high enough wire gauge so that it is able to withstand attempts at window-jacking.
Smart Shades & Blinds
Smart Shades and Blinds are also a common trend in window replacement. This is because they are an efficient way of controlling the amount of natural light entering your home. This means that you can control this amount to make your home feel brighter when it is sunny outside or darker when it rains or is cloudy. This is especially important if you have young children or pets because you don’t want them to be exposed to too much natural light. When it comes to choosing a smart shade or blind, you want to make sure that you go with a reputable brand. This is because you want to make sure these items are made of a durable material that can withstand wear and tear over time.
Solar Energy Panels
Finally, we would be remiss if we didn’t talk about the most popular trend in window replacement chilliwack British Columbia. That is the use of solar energy panels. These are ideal for anyone who wants to reduce their utility bills while also generating their own electricity.
What Are the Advantages of Replacement Windows?
Easy Cleaning: Replacing windows is one of the best ways to make your home easier to clean. All you have to do is a quick wipe-down with a damp cloth, or a mixture of bleach and water, and your windows will be as good as new.
Replacing windows is one of the best ways to make your home easier to clean. All you have to do is a quick wipe-down with a damp cloth, or a mixture of bleach and water, and your windows will be as good as new. Durable: Another advantage of replacing your windows is that they are much more durable than standard windows. That means that they will last much longer, reducing the amount of time you will have to spend on maintenance.
Another advantage of replacing your windows is that they are much more durable than standard windows. That means that they will last much longer, reducing the amount of time you will have to spend on maintenance. Better Soundproofing: Finally, replacing your windows is a great way to improve soundproofing in your home. That is because they allow much less air to pass through them than standard windows do.
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itsgerges · 1 year
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The energy distribution proves the solar system creation depend on one light beam energy
Best Greetings
 The energy distribution proves the solar system creation depend on one light beam energy
  Here we analyze the energy distribution through the solar system – this distribution can help to see clearly how the machine works
(1)
We accept the space is energy – and – I claim that the energy be reflected in the solar system – in fact – the reflection of energy is the most strong point of my paper proves – it's simply the point of the paper fighting – the energy reflection proves the space has mechanical features
 Now – the simple analysis can refer to the dilemma – because – the outer planets have great distances (energy) and if this energy be reflected toward the inner planets it will be as a flood of water moves toward a city and houses.  
It's not very clear – how the inner planets can store this huge energy because their distances are so short and can't store such massive energy
The fact is that – the data is reflected on both sides – that means- thousands of the planets data be reflected on one another – this reflection of data should depend on a geometrical reason –
(2)
As example for the data reflection
The inner planets original order (Mercury – Mars – Venus – Earth) shows the planets order in their diameters, masses and orbital distances – Because Mars had migrated from its original orbit (between Mercury and Venus), Mars deformed this good order
 The order shows clearly (Greater Diameter Necessitates Greater Orbital Distance)
The outer planets order is reflected clearly (Jupiter- Saturn- Uranus –Neptune – Pluto) the order shows that greater diameter necessitates shorter orbital distance – this is a clear reflection of data
The question again - if the outer planets energy be reflected how the inner planets short distances can store this massive energy?      
The inner planets don't store the energy – instead – The Energy Be Used To Produce The Sun Rays.
(3)
The sun rays creation theory is discussed in details in the theory – let's summarize the idea in following…
The solar system is one light beam – the light minimum velocity is 300000 km/s- the planets are ships sail over the sea and the sea is the light beam
By that the sea water and the ship move by the same velocity – by that – the solar system moves by the velocity (300000 km/s) – the sun is a stationary point has no motion relative to the sea water velocity –
How can this stationary point be created?  it's the vortex in the sea water
The planets revolve around a point in space – their revolutions cause to create 2 velocities on both sides of this point – the two velocities are equal and opposite in direction – the total velocity on this point be Zero- the revolution wave moves by the sea wave velocity and by that the point be stationary relative to the planets revolution velocity and to the sea water velocity – by that – the revolution causes to create a different velocity equal the sea water velocity (300000 km/s) and we see the sun as a light beam – why??
Because the creature brain uses light velocity (300000 km/s) in thinking – that means- when the creature looks at a light beam it be similar to a light beam looks at another light beam – the special theory of relativity tells (if one light looks at another light beam) they will see each other as matters (Particles)- why? because no difference in velocities    
For that we see all motions with velocity (300000 km/s) as matters around us– the sun motion velocity is (Zero) that creates the different velocity (300000 km/s) and caused to see the sun rays as light beams
(4)
Shortly
The planets motions energies be stored in the outer planets massive distances to store massive amounts of energy (because the light beam be produced based on quantum) and the energy be reflected from the outer planets to the inner planets – and the inner planets use the energy to produce the sun rays by that the energy is not stored in the inner planets distances but be used immediately
Also – that means- the sun is not doing nuclear fusion to create its rays but the planets motions energies total be used as a source for the sun rays production
Notice
The Earth mass equal the rest inner planets masses total (error 1%) – if we imagine that – from a great gamma ray the inner planets be created – and – the Earth be the great electron and the other inner planets be the great positron –
Where– the great electron means (its atom has a positive charge and electrons revolve around) and the great positron means (its atom has a negative charge and positrons revolve around)-
This idea has a advantage because it creates an electric field between the inner planets – this electric field can be so useful to create the sun rays because the sun rays creation depends on a geometrical design and the electric field can provide the accuracy by which the geometrical design can be produced – here we have important notice – because the outer planets store massive amounts of energy (the accuracy here isn't necessary) but the inner planets use this energy to produce the sun rays (or the stationary point) where this process needs accurate geometrical effects which can be supported simply by the electric fields – also – the creation of electron and positron  by gamma ray is experiment be proved empirically – only – I suppose – after the inner planets matters creation the original light beam is not finished but created also the outer planets from the same one light beam energy.
 (5)
Why Is The Data Reflected Between The 2 Sides?
The energy be reflected from Pluto to Venus and then from Venus to Mars –
There's another reflection be done inside Saturn for the wave be sent from Pluto to Venus
The reflection of energy caused to reflect the data- but – in details – the reflection caused (the distance) to be used as (a period of time) and another reflection causes (the period of time) be used as (a distance) one more time – by that- the planets which have many reflections can put their data in ordinary order but the planets which have one reflection only have to put their data in reflected form – that shows how the data be reflected on both sides –
Let's use one example
(a)
Jupiter orbital circumference =4900 million km
Uranus orbital period = 4900 days x 2π  
This data depend on the reflection be done inside Saturn, that makes the data before Saturn be reflected on the data after Saturn  
We need to follow the rate (2π) because this is the key of the data understanding
(b)
Another reflection be done between Venus and Mars for that
680 million km       = Venus orbital circumference  
687 days               = Mars orbital period - And
 224.7 days             = Venus orbital period
227.9 million km = Mars orbital distance
The data shows clearly that the rate (2π) be found between Mars and Venus
(c)
Pluto orbital distance 5906 million km = Earth orbital distance 149.6 million km x 4π2
We see the data clearly
The two rates (2π) be balanced by (4π2) between the Earth and Pluto
But
The rates (2π) be used between (A Distance On One Side And A Period On Another)  
For the Earth case – the rate (4π2) be used between 2 Distances
 The data which is reflected in the outer planets, be reflected one more time in the inner planets and by that the inner planets show ordinary order of the data but the outer planets data still be reflected.  
Notice
There's one more (2π) between Mars and Saturn because Saturn orbital distance = Mars orbital circumference and this (2π) be used also between two distances.
 Kind regards – please read my paper
 The Solar System Origin Theory (The Proves Discussion)
https://www.academia.edu/s/66e37e694d
or
https://www.academia.edu/96290192/The_Solar_System_Origin_Theory_The_Proves_Discussion_
or
https://app.box.com/s/p03ga5q7un313ighc2cbgxa73q0w6gu8
or
https://app.box.com/s/saihd2atjn9kpzkqgagb14snzo50wu9w
 Gerges Francis Tawdrous +201022532292
Physics Department-  Physics & Mathematics  Faculty
Peoples' Friendship university of Russia – Moscow   (2010-2013)
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