It just kills me when writers create franchises where like 95% of the speaking roles are male, then get morally offended that all of the popular ships are gay. It’s like, what did they expect?
yo quiero que ustedes sepan que “Alex” es como un AU que he echo de Onceler😭💀 siento que ustedes suponen que es otro Alex o no se por que aún no he explicado nada😭🙏🏻//
I want you to know that “Alex” is like an AU that I made from Onceler😭💀 I feel like you assume it's another Alex or I don't know why I haven't explained anything yet😭🙏🏻
This phenomenon is something I'm sure everyone faces everyday!! Like when I wake up in the morning my mom looks like she is the happiest person to ever exist, laughing, smiling, joking and even does some of my chores!! But as the day progresses, my mom's mood worsens and soon it's time to go to bed, and she looks like me as if I'm the worst criminal on this Earth ToT. Don't be mistaken, I love my mom. BUT SOMEONE PLEASE EXPLAIN THIS PHENONEMON!!
Hi.dr.naomi.i have 2 questions.
1.Can this JAMES WEB T.S able to see Mercury, Venus and certain stars that are close to the sun either. I.
2.Why is the James Webb t.s.mirror yellow?
Any specific reason for this
Will it take pictures of Pluto?
When will we start seeing images from the James Webb telescope??
Does Webb have resolution to look more closely at nearby objects, like Mars or even Earth? Or just far things?
How exactly will it work? And whats the goal of the project?
Do you have any protections against asteroids?
Concerning the new telescope -out of curiosity- what is the maximum distance it can view planets, galaxies, objects, anything up to -in terms of common/metric measurement, and/or years (if applicable) etc.? -Rose
What does “chemical fingerprints” mean? What chemicals indicate possible life on other planets?
Will the James Webb Telescope also be able to spot out signs of life on habitable worlds?
Questions coming up from….
@maybeinanotherworld: JWST IS HAPPENING! How are all of you feeling about this?
@Anonymous: How powerful is this telescope, exactly?
@Anonymous: Why are the mirrors on it yellow?
@foeofcolor: How long is this estimated to last for? Like how long will it be able to function in space by estimates?
See that tiny blob of light, circled in red? Doesn’t look like much, does it? But that blob represents a feast big enough to feed a black hole around 30 million times the mass of our Sun! Scientists call these kinds of stellar meals tidal disruption events, and they’re some of the most dramatic happenings in the cosmos.
Sometimes, an unlucky star strays too close to a black hole. The black hole’s gravity pulls on the star, causing it to stretch in one direction and squeeze in another. Then the star pulls apart into a stream of gas. This is a tidal disruption event. (If you’re worried about this happening to our Sun – don’t. The nearest black hole we know about is over 1,000 light-years away. And black holes aren’t wild space vacuums. They don’t go zipping around sucking up random stars and planets. So we’re pretty safe from tidal disruption events!)
The trailing part of the stream gets flung out of the system. The rest of the gas loops back around the black hole, forming a disk. The material circling in the disk slowly drifts inward toward the black hole’s event horizon, the point at which nothing – not even light – can escape. The black hole consumes the gas and dust in its disk over many years.
Sometimes the black hole only munches on a passing star – we call this a partial tidal disruption event. The star loses some of its gas, but its own gravity pulls it back into shape before it passes the black hole again. Eventually, the black hole will have nibbled away enough material that the star can’t reform and gets destroyed.
We study tidal disruptions, both the full feasts and the partial snacks, using many kinds of telescopes. Usually, these events are spotted by ground-based telescopes like the Zwicky Transient Facility and the All-Sky Automated Survey for Supernovae network.
They alert other ground- and space-based telescopes – like our Neil Gehrels Swift Observatory (illustrated above) and the European Space Agency’s XMM-Newton – to follow up and collect more data using different wavelengths, from visible light to X-rays. Even our planet-hunting Transiting Exoplanet Survey Satellite has observed a few of these destructive wonders!
We’re also studying disruptions using multimessenger astronomy, where scientists use the information carried by light, particles, and space-time ripples to learn more about cosmic objects and occurrences.
But tidal disruptions are super rare. They only happen once every 10,000 to 100,000 years in a galaxy the size of our own Milky Way. Astronomers have only observed a few dozen events so far. By comparison, supernovae – the explosive deaths of stars – happen every 100 years or so in a galaxy like ours.
That’s why scientists make their own tidal disruptions using supercomputers, like the ones shown in the video here. Supercomputers allow researchers to build realistic models of stars. They can also include all of the physical effects they’d experience whipping ‘round a black hole, even those from Einstein’s theory of general relativity. They can alter features like how close the stars get and how massive the black holes are to see how it affects what happens to the stars. These simulations will help astronomers build better pictures of the events they observe in the night sky.
Keep up with what’s happening in the universe and how we study it by following NASA Universe on Twitter and Facebook.
Make sure to follow us on Tumblr for your regular dose of space!
They say a picture is worth a thousand words, but no images have left a greater impact on our understanding of the universe quite like the Hubble Space Telescope’s deep fields. Like time machines, these iconic images transport humanity billions of light-years back in time, offering a glimpse into the early universe and insight into galaxy evolution!
You’ve probably seen these images before, but what exactly do we see within them? Deep field images are basically core samples of our universe. By peering into a small portion of the night sky, we embark on a journey through space and time as thousands of galaxies appear before our very eyes.
So, how can a telescope the size of a school bus orbiting 340 miles above Earth uncover these mind-boggling galactic masterpieces? We’re here to break it down. Here’s Hubble’s step-by-step guide to viewing deep fields:
Believe it or not, capturing the light of a thousand galaxies actually begins in the dark. To observe extremely faint galaxies in the farthest corners of the cosmos, we need minimal light interference from nearby stars and other celestial objects. The key is to point Hubble’s camera at a dark patch of sky, away from the outer-edge glow of our own galaxy and removed from the path of our planet, the Sun, or the Moon. This “empty” black canvas of space will eventually transform into a stunning cosmic mosaic of galaxies.
The first deep field image was captured in 1995. In order to see far beyond nearby galaxies, Hubble’s camera focused on a relatively empty patch of sky within the constellation Ursa Major. The results were this step-shaped image, an extraordinary display of nearly 3,000 galaxies spread across billions of light-years, featuring some of the earliest galaxies to emerge shortly after the big bang.
The universe is vast, and peering back billions of years takes time. Compared to Hubble’s typical exposure time of a few hours, deep fields can require hundreds of hours of exposure over several days. Patience is key. Capturing and combining several separate exposures allows astronomers to assemble a comprehensive core slice of our universe, providing key information about galaxy formation and evolution. Plus, by combining exposures from different wavelengths of light, astronomers are able to better understand galaxy distances, ages, and compositions.
The Hubble Ultra Deep Field is the deepest visible-light portrait of our universe. This astonishing display of nearly 10,000 galaxies was imaged over the course of 400 Hubble orbits around Earth, with a total of 800 exposures captured over 11.3 days.
The ability to see across billions of light-years and observe the farthest known galaxies in our universe requires access to wavelengths beyond those visible to the human eye. The universe is expanding and light from distant galaxies is stretched far across space, taking a long time to reach us here on Earth. This phenomenon, known as “redshift,” causes longer wavelengths of light to appear redder the farther they have to travel through space. Far enough away, and the wavelengths will be stretched into infrared light. This is where Hubble’s infrared vision comes in handy. Infrared light allows us to observe light from some of the earliest galaxies in our universe and better understand the history of galaxy formation over time.
In 2009, Hubble observed the Ultra Deep Field in the infrared. Using the Near Infrared Camera and Multi-Object Spectrometer, astronomers gathered one of the deepest core samples of our universe and captured some of the most distant galaxies ever observed.
Apart from their remarkable beauty and impressive imagery, deep field images are packed with information, offering astronomers a cosmic history lesson billions of years back in time within a single portrait. Since light from distant galaxies takes time to reach us, these images allow astronomers to travel through time and observe these galaxies as they appear at various stages in their development. By observing Hubble’s deep field images, we can begin to discover the questions we’ve yet to ask about our universe.
Credit: NASA, ESA, R. Bouwens and G. Illingworth (University of California, Santa Cruz)
Hubble’s deep field images observe galaxies that emerged as far back as the big bang. This image of the Hubble Ultra Deep Field showcases 28 of over 500 early galaxies from when the universe was less than one billion years old. The light from these galaxies represent different stages in their evolution as their light travels through space to reach us.
Hubble’s deep fields have opened a window to a small portion of our vast universe, and future space missions will take this deep field legacy even further. With advancements in technologies and scientific instruments, we will soon have the ability to further uncover the unimaginable.
Slated for launch in late 2021, NASA’s James Webb Space Telescope will offer a new lens to our universe with its impressive infrared capabilities. Relying largely on the telescope’s mid-infrared instrument, Webb will further study portions of the Hubble deep field images in greater detail, pushing the boundaries of the cosmic frontier even further.
And there you have it, Hubble’s guide to unlocking the secrets of the cosmos! To this day, deep field images remain fundamental building blocks for studying galaxy formation and deepening not only our understanding of the universe, but our place within it as well.
Still curious about Hubble Deep Fields? Explore more and follow along on Twitter, Facebook, and Instagram with #DeepFieldWeek!
Make sure to follow us on Tumblr for your regular dose of space!
They say a picture is worth a thousand words, but no images have left a greater impact on our understanding of the universe quite like the Hubble Space Telescope’s deep fields. Like time machines, these iconic images transport humanity billions of light-years back in time, offering a glimpse into the early universe and insight into galaxy evolution!
You’ve probably seen these images before, but what exactly do we see within them? Deep field images are basically core samples of our universe. By peering into a small portion of the night sky, we embark on a journey through space and time as thousands of galaxies appear before our very eyes.
So, how can a telescope the size of a school bus orbiting 340 miles above Earth uncover these mind-boggling galactic masterpieces? We’re here to break it down. Here’s Hubble’s step-by-step guide to viewing deep fields:
Believe it or not, capturing the light of a thousand galaxies actually begins in the dark. To observe extremely faint galaxies in the farthest corners of the cosmos, we need minimal light interference from nearby stars and other celestial objects. The key is to point Hubble’s camera at a dark patch of sky, away from the outer-edge glow of our own galaxy and removed from the path of our planet, the Sun, or the Moon. This “empty” black canvas of space will eventually transform into a stunning cosmic mosaic of galaxies.
The first deep field image was captured in 1995. In order to see far beyond nearby galaxies, Hubble’s camera focused on a relatively empty patch of sky within the constellation Ursa Major. The results were this step-shaped image, an extraordinary display of nearly 3,000 galaxies spread across billions of light-years, featuring some of the earliest galaxies to emerge shortly after the big bang.
The universe is vast, and peering back billions of years takes time. Compared to Hubble’s typical exposure time of a few hours, deep fields can require hundreds of hours of exposure over several days. Patience is key. Capturing and combining several separate exposures allows astronomers to assemble a comprehensive core slice of our universe, providing key information about galaxy formation and evolution. Plus, by combining exposures from different wavelengths of light, astronomers are able to better understand galaxy distances, ages, and compositions.
The Hubble Ultra Deep Field is the deepest visible-light portrait of our universe. This astonishing display of nearly 10,000 galaxies was imaged over the course of 400 Hubble orbits around Earth, with a total of 800 exposures captured over 11.3 days.
The ability to see across billions of light-years and observe the farthest known galaxies in our universe requires access to wavelengths beyond those visible to the human eye. The universe is expanding and light from distant galaxies is stretched far across space, taking a long time to reach us here on Earth. This phenomenon, known as “redshift,” causes longer wavelengths of light to appear redder the farther they have to travel through space. Far enough away, and the wavelengths will be stretched into infrared light. This is where Hubble’s infrared vision comes in handy. Infrared light allows us to observe light from some of the earliest galaxies in our universe and better understand the history of galaxy formation over time.
In 2009, Hubble observed the Ultra Deep Field in the infrared. Using the Near Infrared Camera and Multi-Object Spectrometer, astronomers gathered one of the deepest core samples of our universe and captured some of the most distant galaxies ever observed.
Apart from their remarkable beauty and impressive imagery, deep field images are packed with information, offering astronomers a cosmic history lesson billions of years back in time within a single portrait. Since light from distant galaxies takes time to reach us, these images allow astronomers to travel through time and observe these galaxies as they appear at various stages in their development. By observing Hubble’s deep field images, we can begin to discover the questions we’ve yet to ask about our universe.
Credit: NASA, ESA, R. Bouwens and G. Illingworth (University of California, Santa Cruz)
Hubble’s deep field images observe galaxies that emerged as far back as the big bang. This image of the Hubble Ultra Deep Field showcases 28 of over 500 early galaxies from when the universe was less than one billion years old. The light from these galaxies represent different stages in their evolution as their light travels through space to reach us.
Hubble’s deep fields have opened a window to a small portion of our vast universe, and future space missions will take this deep field legacy even further. With advancements in technologies and scientific instruments, we will soon have the ability to further uncover the unimaginable.
Slated for launch in late 2021, NASA’s James Webb Space Telescope will offer a new lens to our universe with its impressive infrared capabilities. Relying largely on the telescope’s mid-infrared instrument, Webb will further study portions of the Hubble deep field images in greater detail, pushing the boundaries of the cosmic frontier even further.
And there you have it, Hubble’s guide to unlocking the secrets of the cosmos! To this day, deep field images remain fundamental building blocks for studying galaxy formation and deepening not only our understanding of the universe, but our place within it as well.
Still curious about Hubble Deep Fields? Explore more and follow along on Twitter, Facebook, and Instagram with #DeepFieldWeek!
Make sure to follow us on Tumblr for your regular dose of space!
Allright Luca fandom, it’s time for the history behind this now famous panel & why it’s out-of -picture. Because I’ve seen wild theories on here, as there should be, that’s why I love Tumblr.
Here’s Mckenna Harris’ caring redraw:
Here’s my original from a couple versions earlier, notice how I only did a goofy reaction shot, and how she went full on HUG, of all story artists on the film, she loved these boys the most, and it shows!
These were part of a longer bit where we had plenty of shots, them speeding down those terraces towards town, exchanging dialogue. -But the dialogue kinda stopped the flow of the energy we had started at the tower.
-Also it’s dramatically more interesting to see humans in town react to sea monsters on a bicycle, then just the 2 alone on the terraces (where there are less spectators)
-A 3rd problem is the line ‘and you thought me how to’; it’s one-the-nose and stating the obvious. We were shown over & over throughout the movie how Alberto gave Luca a push. No need to ram it in there. As always: Show, Don’t Tell.
-Another pro to the cut is that any Alberto/Luca love budget saved in the rest of the race could be spent in Parting Ways, at the train station. You don’t want the movie to end on the hill; you want to let the sweetness all out at the end, because it’ll feel all the more earned.
So on the cutting floor it went. ✂️
When you have a well-defined objective of an exact activity to partake in on this particular 24 period of time and ecstatically wish to include Ferbs Fletcher in the proposed latter
scared shitless but its ok..
THE DIFFERENCE BETWEEN THE VOID STATE AND THE VOID:
tag: @aestheticlizalis
As always, I will love to hear your thoughts! and if you have any questions, I will be more than happy to answer them! If you liked it, leave a comment or reblog (that is always appreciated!). if you are intrested in more method check the masterlist!
Every time I end up talking about the void state, there is a part of me that tends to raise awareness about the void itself. It is a thing the void does not help you manifest, like the void state. In this post, I will try my best to explain how much these two things are truly different.
WARNING: COGNITO HAZARD (For those who do not know, a cognito hazard is a term used to describe an image, pattern, sound, or any other kind of sensory signal that directly causes harmful or undesired physiological or physical effects to one who senses or perceives it. (It is specifically used as a warning when talking about "forced awakening" things like the void.)
You are free to believe or not believe every word I will say in this post, and you are free to not believe every word I say. If, while reading this, you start to feel a negative emotion or a sensation as if you are lost or bodily or emotionally sick, DO NOT CONTINUE READING.
i will talk breefly about the void state and then i will get in a more detailed way into what the void is, just because i aready explained the void state many times.
is a state of deep meditation where you feel like floating and feel nothingness embodies you, making you feel one with the universe helping you to manifest. (Click the name if you actually want to know more.)
The void is nothing and everything at the same time. Let me explain better: the void is a place where everything is possible and exists, but at the same time is impossible and does not exist. The thing is, the void in itself is a pass to every other dimension because every dimension resides in the void, even the cursed ones or the ones that never will be or never were timelines. As a person with a lot of experience in the void itself, I will tell you that it is not a nice place. Every kind of entity can catch you, good or evil, whatever they might be. As mere humans in the void, we are exposed to a lot of deep-rooted energy that corrupts our bodies in the long run.
As humans, in the void, we can only "survive" in the backrooms.
One thing that is definitely more popular than the void itself are the backrooms that reside in the void. The backrooms became popular around 2012 as a SCP thing as images of liminal spaces. But I assure you, they are pretty much real, and they have many levels, not in a specific order. On every level, we can find different things and different entities, as mentioned before. We can find the good ones that will try to keep you safe and the bad ones that will literally try to kill you.
I will also add that the backroom exists because we are the front room, so for every timeline in existence, there is a backroom, and much like the universe, the void is pretty much endless, so there are infinite possibilities for the frontroom and the backroom.
because I talk from experience, and let me tell you some of them were not fun. Still to this day, when I go to sleep, I find myself in the void. Bruh, I don't know how it simply happens. And that's been my life since I was 14 years old. I had my time to understand and learn a few rules to exit the backrooms fast enough or not to be killed.
I will put them at the end, but first, a little check on the main differences that we found out about the void state and the void itself:
The void state is a meditation; the void is an "endless place.".
The void can be a dangerous place, but the void state is harmless.
The void state helps us connect with the universe; the void is not used to manifest.
The void is a constant state of rooted energy, which means, in more basic words, that the energy in the void is dirty, and on the long run, a normal human will not "survaive.". In the void state, it is your energy.
In the void state, we find only ourselves; in the void, we can find an endless amount of dimensions, timelines, frontrooms and backrooms, entities, and liminal spaces. Some are all put together.
If you decide to go into the void state, it is a conscious decision. You can mistakenly enter the void by just falling asleep.
Those are the main differences, just because I can't say much more about the void itself because, as said before, it is a forced awakening, and I don't want people to feel sick with too much information.
if by mystake you enter the backrooms here some rules that will help you get out faster:
Don't scream; you will give off your location to any type of entity. In whatever level you enter, you will find the exit in the same level.
Not every level is scary. Some have flowers and are pretty; others are simple rooms. Those levels are safe as long as you don't hurt yourself. Be careful.
Don't take stairs, and don't jump in holes or on poles. Again, you will find the exit on the same level as you entered.
If you see fluffy entities, look at their eyes first. If the eyes are blue, they are friendly; any other color is to be avoided.
There is only one entity that is 100% friendly and will help you. It looks like a shadow with no features; it does not talk, but you will understand her.
If you hear a sound, go in the opposite direction; if you feel like a sound surrounds you, hide and stay still no matter what; some entities don't have eyes.
If you can't find the exit, pray to whatever god you believe in, and good entities will find you and help you.
On rare occasions, you might find other humans; don't trust them; they are no longer humans.
and I think that I said everything that has to be said. If you have any questions, I will be more than happy to answer them, and I hope you did not feel sick or do any negative things from this post.
I have heard few voices in the community against ai generated art, this is my personal perspective on the topic. But I also invite you to a dialogue - everyone who hates/loves/neutral to ai art in general and particularly on tumblr... Please explain your point of view, I want to understand you better😉
Carmen part 3 -
Benefits of ai for an artist in hardest days of disability - I can keep fulfilling my imagination even in days of very low ability to move. Of course when I paint I express something more authentic, but with time I compose prompts that give results that are very close to my imagination - which deeply satisfy and comfort me.