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EverythingScience

EverythingScience

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Discover the best, human-curated science facts, news, discoveries, videos, and more! Chat with us: @EverythingScienceChat Contact: @DigitisedRealitySupport

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El país no está especificadoHechos666

📈 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 21 250 suscriptores, ocupando la posición 666 en la categoría Hechos.

📊 Métricas de audiencia y dinámica

Desde su creación el невідомо, el proyecto ha mostrado un crecimiento acelerado, reuniendo a 21 250 suscriptores.

Según los últimos datos del 01 noviembre, 2026, el canal mantiene una actividad estable. En los últimos 30 días la variación de miembros fue de -635, y en las últimas 24 horas de -38, conservando un alto alcance.

  • Estado de verificación: No verificado
  • Tasa de interacción (ER): El promedio de interacción de la audiencia es 3.43%. Durante las primeras 24 horas tras publicar, el contenido suele obtener 1.81% de reacciones respecto al total de suscriptores.
  • Alcance de las publicaciones: Cada publicación recibe en promedio 732 visualizaciones. En el primer día suele acumular 386 visualizaciones.
  • Reacciones e interacción: La audiencia responde de forma activa: el promedio de reacciones por publicación es 5.

📝 Descripción y política de contenido

El autor describe el recurso como un espacio para expresar opiniones subjetivas:
“Discover the best, human-curated science facts, news, discoveries, videos, and more! Chat with us: @EverythingScienceChat Contact: @DigitisedRealitySupport”

Gracias a la alta frecuencia de actualizaciones (últimos datos recibidos el 02 noviembre, 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.

21 250
Suscriptores
-3824 horas
-4577 días
-63530 días
Archivo de publicaciones
There's Growing Evidence That Insects Feel Pain, Just Like Us Article @EverythingScience

Engineers Have Grown a Major Piece of The Human Heart in Miniature, And It Beats Article @EverythingScience

Where in the night sky exactly are the "cosmic cliffs" from the JWST Carina Nebula images? (4K) In order to give some context to the amazing images from the James Webb Space Telescope, we wanted to show where exactly the image belongs in the night sky. The scale is truly immense. Further explanation 1080p Video @EverythingScience

As part of Webb’s prep for science, we tested how the telescope tracks solar system objects like Jupiter. Webb worked better
As part of Webb’s prep for science, we tested how the telescope tracks solar system objects like Jupiter. Webb worked better than expected, and even caught Jupiter’s moon Europa These images are designed for engineering purposes, so they aren’t processed in the same way as our first images this week. Like some earlier calibration images, these are processed to emphasize certain features. https://blogs.nasa.gov/webb/2022/07/14/webb-images-of-jupiter-and-more-now-available-in-commissioning-data Source: @NASAWebb

Webb's First Deep Field (NIRISS Emission Spectra) At far left is a near-infrared image of galaxy cluster SMACS 0723. A group
Webb's First Deep Field (NIRISS Emission Spectra) At far left is a near-infrared image of galaxy cluster SMACS 0723. A group of massive galaxies below and to the right of the bright central star have distorted, magnified, and mirrored many galaxies in this field. By quickly examining the image at left by eye, it becomes clearer that one arc may be made up of two similar-looking galaxies. Their bright central regions match, despite their stretched appearances. These may be lensed galaxies – one galaxy that is mirrored in a second location. Are they the same? Researchers can’t be sure from the image alone – more data are needed to confirm a match. Scientists do this by gathering spectra, which spread light out so they can fully examine an object’s makeup. Webb’s Near-Infrared Imager and Slitless Spectrograph (NIRISS), which gathers spectra of every object in any field it observes, was pointed at the galaxy cluster to gather more detail. A segment of the NIRISS grism image (an instrument that has a grating, or stair steps, on a prism), at center, shows how ionized oxygen and atomic hydrogen emission lines are distributed along the arc. Next, the spectra from each of these two galaxies were plotted as graphs, shown at right, to reveal their compositions. The graphs, known as spectra, match, which indicates that these arcs are mirror images of the same galaxy. Webb’s spectra from NIRISS also quickly proved that light from both galaxies was emitted 9.3 billion years ago, further confirming they are one and the same. Using Webb’s NIRISS is like opening a treasure chest overflowing with spectra. For example, this instrument can disperse the spectra along the image vertically and horizontally. Researchers can use both modes to untangle which lines match each source. Every object’s image can be transformed into spectra like the two shown above. So even if researchers aren’t intending to study a particular galaxy in the field, they may make a surprise discovery. Source @EverythingScience

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SMACS 0723 Thousands of galaxies flood this near-infrared image of galaxy cluster SMACS 0723. High-resolution imaging from NASA’s James Webb Space Telescope combined with a natural effect known as gravitational lensing made this finely detailed image possible. Low-res Read More

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SMACS 0723 Thousands of galaxies flood this near-infrared image of galaxy cluster SMACS 0723. High-resolution imaging from NASA’s James Webb Space Telescope combined with a natural effect known as gravitational lensing made this finely detailed image possible. Read More

Two cameras are better than one, as seen in this combined view from Webb’s NIRCam & MIRI! In the near-infrared, we see hundre
Two cameras are better than one, as seen in this combined view from Webb’s NIRCam & MIRI! In the near-infrared, we see hundreds of stars and background galaxies. Meanwhile, the mid-infrared shows us dusty planet-forming disks (in red and pink) around young stars. Source: @NASAWebb

The “Cosmic Cliffs” build on the legacy of Hubble’s imagery of the Carina Nebula, seen here. Webb’s new view gives us a rare
The “Cosmic Cliffs” build on the legacy of Hubble’s imagery of the Carina Nebula, seen here. Webb’s new view gives us a rare peek into stars in their earliest, rapid stages of formation. For an individual star, this period only lasts about 50,000 to 100,000 years. Source: @NASAWebb

🌟 A star is born! Behind the curtain of dust and gas in these “Cosmic Cliffs” are previously hidden baby stars, now uncovere
🌟 A star is born! Behind the curtain of dust and gas in these “Cosmic Cliffs” are previously hidden baby stars, now uncovered by Webb. We know — this is a show-stopper. Just take a second to admire the Carina Nebula in all its glory http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse Source: @NASAWebb

Galaxies collide in Stephan’s Quintet, pulling and stretching each other in a gravitational dance. In the mid-infrared view h
Galaxies collide in Stephan’s Quintet, pulling and stretching each other in a gravitational dance. In the mid-infrared view here, see how Webb pierces through dust, giving new insight into how interactions like these may have driven galaxy evolution in the early universe. Source: @NASAWebb

In Webb’s image of Stephan’s Quintet, we see 5 galaxies, 4 of which interact. (The left galaxy is in the foreground!) Webb wi
In Webb’s image of Stephan’s Quintet, we see 5 galaxies, 4 of which interact. (The left galaxy is in the foreground!) Webb will revolutionize our knowledge of star formation & gas interactions in these galaxies http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse Source: @NASAWebb

Put a ring on it! 💍 Compare views of the Southern Ring nebula and its pair of stars by Webb’s NIRCam (L) & MIRI (R) instrume
Put a ring on it! 💍 Compare views of the Southern Ring nebula and its pair of stars by Webb’s NIRCam (L) & MIRI (R) instruments. The dimmer, dying star is expelling gas and dust that Webb sees through in unprecedented detail: http://nasa.gov/webbfirstimages/ #UnfoldTheUniverse Source: @NASAWebb

Why do some of the galaxies in this image appear bent? The combined mass of this galaxy cluster acts as a “gravitational lens
Why do some of the galaxies in this image appear bent? The combined mass of this galaxy cluster acts as a “gravitational lens,” bending light rays from more distant galaxies behind it, magnifying them. The light from the farthest galaxy here traveled 13.1 billion years to us. Source: @NASAWebb

Canada’s instrument NIRISS on #Webb reveals the distinct signature of water 💧 in the atmosphere of a hot, puffy gas giant pl
Canada’s instrument NIRISS on #Webb reveals the distinct signature of water 💧 in the atmosphere of a hot, puffy gas giant planet orbiting a distant Sun-like star. It also shows evidence of haze and clouds that previous studies of this planet did not detect. ☁ Source: @csa_asc

James Webb vs Hubble comparison overlayed. More details @EverythingScience

NASA, in partnership with ESA (European Space Agency) and CSA (Canadian Space Agency), will release the James Webb Space Telescope’s first full-color images and spectroscopic data during a live broadcast beginning at 14:30 UTC Tuesday, July 12, from NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Released one by one, these first images from the world’s largest and most powerful space telescope will demonstrate Webb at its full power as it begins its mission to unfold the infrared universe. Each image will simultaneously be made available on social media, as well as on the agency’s website at: http://www.nasa.gov/webbfirstimages 📺 Join us for the stream and comment on the live broadcast here

The image taken by the JWST compared to one taken by Hubble, of the galaxy cluster SMACS 0723. It's s a gravitational lens, s
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The image taken by the JWST compared to one taken by Hubble, of the galaxy cluster SMACS 0723. It's s a gravitational lens, showing us the light of galaxies that are far behind the cluster in arcs around it. I tried to orient them the same. LOOK AT THE DIFFERENCE. 12.5 hours of exposure for Webb and 2 weeks for Hubble! Source: @Astropartigirl

‍If you held a grain of sand up to the sky at arm’s length, that tiny speck is the size of Webb’s view in this image. Imagine — galaxies galore within a grain, including light from galaxies that traveled billions of years to us! Source: @NASAWebb

This isn’t the farthest back we’ve observed. Non-infrared missions like COBE & WMAP saw the universe closer to the Big Bang (
This isn’t the farthest back we’ve observed. Non-infrared missions like COBE & WMAP saw the universe closer to the Big Bang (~380,000 years after), when there was only microwave background radiation, but no stars or galaxies. Webb sees a few 100 million years after the Big Bang. Source: @NASAWebb