NASA's Astronomy Picture of the Day
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To find and view past APODs, tap here: t.me/apodQA/3 NASA's APOD presence in Telegram: 🌐apod.nasa.gov Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
Больше📈 Аналитический обзор Telegram-канала NASA's Astronomy Picture of the Day
Канал NASA's Astronomy Picture of the Day (@apod_telegram) языкового сегмента Английский является активным участником. Сейчас сообщество объединяет 34 818 подписчиков, занимая 410 место в категории Факты и 1 010 место в регионе США.
📊 Показатели аудитории и динамика
С момента создания невідомо проект демонстрирует стремительный рост, собрав аудиторию из 34 818 подписчиков.
Согласно последним данным от 17 июля, 2026, канал показывает стабильную активность. За последние 30 дней изменение числа участников составило 87, а за последние 24 часа — -3, при этом общий охват остаётся высоким.
- Статус верификации: Верифицирован (официально подтверждён Telegram)
- Уровень вовлечённости (ER): Средний показатель вовлечённости аудитории составляет 15.66%. В первые 24 часа после публикации контент обычно набирает 7.10% реакций от общего числа подписчиков.
- Охват публикаций: В среднем каждый пост получает 5 453 просмотров. В течение первых суток публикация набирает 2 474 просмотров.
- Реакции и взаимодействия: Аудитория активно поддерживает контент: среднее количество реакций на один пост — 58.
- Тематические интересы: Контент сосредоточен на ключевых темах, таких как copyright, orion, jupiter, dust, nasa.
📝 Описание и контентная политика
Автор описывает ресурс как площадку для выражения субъективного мнения:
“To find and view past APODs, tap here:
t.me/apodQA/3
NASA's APOD presence in Telegram:
🌐apod.nasa.gov
Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astron...”
Благодаря высокой частоте обновлений (последние данные получены 18 июля, 2026) канал поддерживает актуальность и высокий уровень охвата публикаций. Аналитика показывает, что аудитория активно взаимодействует с контентом, что делает его важной точкой влияния в категории Факты.
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Посты канала
| 2 | Why might Tempel 2's dust trail appear narrower and brighter around July 20? | 1 597 |
| 3 |  2026 July 17
The Dust Trail of Comet Tempel 2
Image Credit & Copyright: Dan Bartlett
Comet 10P/Tempel 2 orbits the Sun once every 5.4 years. Currently visible in binoculars or small telescopes toward the constellation Capricornus, the periodic comet is captured in this sharp telescopic image from July 11 sporting a bright nuclear region and pretty greenish coma. Remarkably, a thin dust trail, not a typical dust tail, is also seen extending both east and west of the Tempel 2 nucleus. Unlike a comet dust tail, which tends to temporarily fan out in a direction away from the Sun, this dust trail is due to the residual dust shed during many past orbits along this ancient periodic comet's orbital plane. In fact, Tempel 2's dust trail may get a little narrower and brighter from our perspective as Earth crosses through the comet's orbital plane on July 20. Comet 10P/Tempel 2 will reach a perihelion on August 2, and make its closest approach to Earth on August 3.
🔗Discuss 🎞HD | 2 387 |
| 4 | 🗨️ Tell us what you saw! | 2 537 |
| 5 | What creates the colorful glowing clouds in NGC 300? | 2 788 |
| 6 |  2026 July 16
NGC 300: A Cosmic Gemstone with Stars and Gas Clouds
Image Credit & Copyright: Team Ciel Austral; Team Members: P. Bernhard, L. Bourgon, J. C. Canonne, D. Chaplain, G. Chassaigne, N. Outters, M. Selby, S. Vetter
Text: Cecilia Chirenti (NASA GSFC, UMCP, CRESST II)
This sparkling, colorful gemstone is a spiral galaxy, NGC 300. It is one of the closest spiral galaxies to Earth, only about 6 million light-years away. But does it really look like this? (Here is a more standard portrait of it.) This unusual image combines the light from the stars and dust within the galaxy with the light from ionized clouds of interstellar gas shown in red (Sulphur), green (Hydrogen) and blue (Oxygen). Combining red and green light in different proportions makes yellow or orange light, most visible in the image. Light from ionized gas is also at work in neon signs, fluorescent tubes and street lights. These massive clouds of ionized gas are typically created by young, massive stars that produce high-energy ultraviolet radiation capable of ionizing the gas. Massive stars are short-lived, compared with lighter stars like our sun, and explode as supernovas at the end of their lives. Some of the colorful clouds in the image could be hiding supernova remnants.
🔗Discuss 🎞HD | 3 323 |
| 7 | What causes the red glow of a red sprite? | 2 790 |
| 8 | Tomorrow's picture: a galaxy bursting with excitement | 2 837 |
| 9 | 🗨️ Tell us what you think! | 2 973 |
| 10 |  2026 July 15
Red Sprites in the Tatacoa Desert
Image Credit & Copyright: Mario Vargas
Text: Keighley Rockcliffe (NASA GSFC, UMBC CSST, CRESST II)
Is there an angry Sith using force lightning in the Tatacoa Desert? This is not science fiction, but a red sprite with multiple streamers! Ordinary lightning occurs when thundercloud particles collide, lose their electrons, and build up negative charge at the cloud bottom. The cloud’s negative charge repels negative charge deeper into the Earth, leaving Earth’s surface positively charged. The opposite charges attract, reaching towards each other and superheating the air into a white strike of plasma. Red sprites are millisecond events triggered by positive cloud-to-ground lightning. They extend up into the mesosphere where the air is too thin for thunder. Their red glow comes from heated molecular nitrogen. There are several potential causes for red sprites, including that the preceding positive lightning exposes the negatively charged cloud core to the positively charged upper atmosphere, allowing those charges to connect. NASA’s Juno has observed sprites on Jupiter, indicating that sprites occur on other planets!
🔗Discuss 🎞HD | 3 434 |
| 11 | Why do scientists think Torifune has two lobes? | 3 235 |
| 12 |  2026 July 14
Double Lobed Asteroid Torifune
Image Credit & Copyright: JAXA, U. of Tokyo, Chiba Tech, Tokyo U. of Science, AIST, Paris Obs., IAC
Why is this asteroid a double? Earlier this month the Japanese robotic spacecraft Hayabusa2 shot past asteroid 98943 Torifune and captured pictures. Although previous observations from distant Earth indicated that Torifune was oblong, Hayabusa2 found that Torifune actually has two joined lobes. With a length of about four soccer fields, this space rock frequently comes near the Earth as it orbits the Sun, although it is not a threat. Besides the two lobes, Torifune shows many large boulders, but, surprisingly, no obvious craters, likely because its surface is a pile of rubble. Like asteroid Arrokoth, it appears that each lobe formed separately before colliding and becoming stuck together. Hayabusa2 famously encountered asteroid Ryugu in 2018, and now heads for an encounter in 2031 with 1998 KY26, a smaller asteroid that rotates unusually fast and might have reservoirs of ice.
🔗Discuss 🎞HD | 3 716 |
| 13 | How often does the International Space Station orbit Earth? | 3 533 |
| 14 | Tomorrow's picture: asteroid double | 3 659 |
| 15 | If you could watch an aurora from one place, which would you choose? | 4 049 |
| 16 |  2026 July 13
Auroras from Space
Image Credit: ESA, NASA, ISS Expedition 74; Capture: Sophie Adenot;
Music: Circle of Light (Patrick Hawes & Grace Davidson)
What do auroras look like from above? Behold! From the ground, auroras dance high above clouds, frequently causing spectacular displays. From space, they look a bit different. As the International Space Station (ISS) circles the Earth every 90 minutes, it sometimes sees auroras below that are active on the night side. A one-hour time-lapse video showing auroras from above was captured about two weeks ago from the orbiting ISS. The ISS -- and all objects in low Earth orbit -- will pass well above green auroras but just a bit above red glowing auroras. The auroras' electron and proton streams are too thin to be a danger to the ISS, just as clouds pose little danger to airplanes. From orbit, as magnetic fields change, auroras can appear to squiggle and crawl like giant snakes. The featured one-minute video was captured by French astronaut Sophie Adenot of the ISS Expedition 74 crew.
🔗Discuss | 4 390 |
| 17 | Tomorrow's picture: aurora below | 4 054 |
| 18 |  2026 July 12
Galaxy NGC 474: Shells and Star Streams
Image Credit & License: CFHT, Coelum, MegaCam, J.-C. Cuillandre (CFHT) & G. A. Anselmi (Coelum)
What's happening to galaxy NGC 474? The multiple layers of emission appear strangely complex given the relatively featureless appearance of the elliptical galaxy in less deep images. The cause of the shells is a topic of research, but they are possibly tidal tails related to debris left over from absorbing numerous small galaxies in the past billion years. Alternatively, the shells may be like ripples in a pond, where the ongoing collision with the spiral galaxy just to the right of NGC 474 is causing density waves to ripple through the galactic giant. Regardless of the actual cause, the featured image dramatically highlights the increasing evidence that the halos of some elliptical galaxies are surprisingly complicated. Similarly, the halo of our own Milky Way Galaxy is one example of such unexpected intricacies. NGC 474 spans about 250,000 light years and lies about 100 million light years distant toward the constellation of the Fish (Pisces).
🔗Discuss 🎞HD | 5 085 |
| 19 | What is Messier 24 actually showing us? | 4 207 |
| 20 | Tomorrow's picture: shells and streams | 4 107 |
