EverythingScience
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The best science facts, news, discoveries, videos and more! Official Chat: @EverythingScienceChat Contact: @DigitisedRealitySupport Links: @DigitisedRealityHub
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📈 Análisis del canal de Telegram EverythingScience
El canal EverythingScience (@everythingscience) en el segmento lingüístico de Inglés es un actor destacado. Actualmente la comunidad reúne a 13 575 suscriptores, ocupando la posición 1 000 en la categoría Hechos.
📊 Métricas de audiencia y dinámica
Desde su creación el невідомо, el proyecto ha mostrado un crecimiento acelerado, reuniendo a 13 575 suscriptores.
Según los últimos datos del 28 julio, 2026, el canal mantiene una actividad estable. En los últimos 30 días la variación de miembros fue de 0, y en las últimas 24 horas de 0, conservando un alto alcance.
- Estado de verificación: No verificado
- Tasa de interacción (ER): El promedio de interacción de la audiencia es 0%. Durante las primeras 24 horas tras publicar, el contenido suele obtener N/A% de reacciones respecto al total de suscriptores.
- Alcance de las publicaciones: Cada publicación recibe en promedio 0 visualizaciones. En el primer día suele acumular 0 visualizaciones.
- Reacciones e interacción: La audiencia responde de forma activa: el promedio de reacciones por publicación es 0.
📝 Descripción y política de contenido
El autor describe el recurso como un espacio para expresar opiniones subjetivas:
“The best science facts, news, discoveries, videos and more!
Official Chat: @EverythingScienceChat
Contact: @DigitisedRealitySupport
Links: @DigitisedRealityHub”
Gracias a la alta frecuencia de actualizaciones (últimos datos recibidos el 29 julio, 2026), el canal mantiene la vigencia y un amplio alcance. La analítica demuestra que la audiencia interactúa activamente con el contenido, lo que lo convierte en un punto de referencia dentro de la categoría Hechos.
13 575
Suscriptores
Sin datos24 horas
Sin datos7 días
Sin datos30 días
Archivo de publicaciones
13 575
Atmosphere of excitement as Europe’s JWST astronomers study climate on other planets
Article
@EverythingScience
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New technique for decoding people's thoughts can now be done from a distance
Past mind-reading techniques relied on implanting electrodes deep in peoples' brains. The new method, described in a report posted 29 Sept. to the preprint database bioRxiv, instead relies on a noninvasive brain scanning technique called functional magnetic resonance imaging (fMRI).
fMRI tracks the flow of oxygenated blood through the brain, and because active brain cells need more energy and oxygen, this information provides an indirect measure of brain activity.
By its nature, this scanning method cannot capture real-time brain activity, since the electrical signals released by brain cells move much more quickly than blood moves through the brain.
But remarkably, the study authors found that they could still use this imperfect proxy measure to decode the semantic meaning of people's thoughts, although they couldn't produce word-for-word translations.
Article
@EverythingScience
13 575
During sleep, one brain region teaches another, converting novel data into enduring memories
Article
@EverythingScience
13 575
The International Space Station had to burn thrusters for more than 5 minutes on Monday night to avoid a chunk of debris from the satellite Russia shot down in November.
Article
@EverythingScience
13 575
Pillars of Creation (NIRCam)
The Pillars of Creation are set off in a kaleidoscope of color in NASA’s James Webb Space Telescope’s near-infrared-light view. The pillars look like arches and spires rising out of a desert landscape, but are filled with semi-transparent gas and dust, and ever changing. This is a region where young stars are forming – or have barely burst from their dusty cocoons as they continue to form.
Newly formed stars are the scene-stealers in this Near-Infrared Camera (NIRCam) image. These are the bright red orbs that sometimes appear with eight diffraction spikes. When knots with sufficient mass form within the pillars, they begin to collapse under their own gravity, slowly heat up, and eventually begin shining brightly.
Along the edges of the pillars are wavy lines that look like lava. These are ejections from stars that are still forming. Young stars periodically shoot out supersonic jets that can interact within clouds of material, like these thick pillars of gas and dust. This sometimes also results in bow shocks, which can form wavy patterns like a boat does as it moves through water. These young stars are estimated to be only a few hundred thousand years old, and will continue to form for millions of years.
Low-res
Source
#Webb
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If this majestic landscape looks familiar, you may recognize the original. Here, Hubbles’s iconic view, taken in visible light, is on the left. Webb “sees” in infrared light invisible to our eyes, allowing it to pierce through the dust and reveal stars galore (right).
Why go back to where we’ve been before? Webb’s new look identifies far more precise counts of newborn stars, along with the quantities of gas and dust. This will help us build a clearer understanding of how stars form and burst out of these dusty clouds over millions of years.
#Webb
Source: @NASAWebb
@EverythingScience
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This is what you’ve waited for.
Journey with us through Webb’s breathtaking view of the Pillars of Creation, where scores of newly formed stars glisten like dewdrops among floating, translucent columns of gas and dust.
First, direct your attention to the tips of the pillars, many of which appear tinged with fiery “lava.” Here, young stars periodically shoot out jets of material that collide with the pillars, which can then form wavy patterns. Energetic hydrogen molecules create that red glow.
Also near the edges of the pillars are tiny red orbs. These are the baby stars of the show, only a few hundred thousand years old!
#Webb
Source: @NASAWebb
@EverythingScience
13 575
Success! NASA Knocked an Asteroid Off Course (And Now It Has a Tail)
Article
@EverythingScience
13 575
A Pair of Supermassive Black Holes Could Be Fated to Collide Within 3 Years
Article
@EverythingScience
