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 34 860 подписчиков, занимая 410 место в категории Факты и 1 016 место в регионе США.
📊 Показатели аудитории и динамика
С момента создания невідомо проект демонстрирует стремительный рост, собрав аудиторию из 34 860 подписчиков.
Согласно последним данным от 12 июля, 2026, канал показывает стабильную активность. За последние 30 дней изменение числа участников составило 139, а за последние 24 часа — 8, при этом общий охват остаётся высоким.
- Статус верификации: Верифицирован (официально подтверждён Telegram)
- Уровень вовлечённости (ER): Средний показатель вовлечённости аудитории составляет 16.08%. В первые 24 часа после публикации контент обычно набирает 7.21% реакций от общего числа подписчиков.
- Охват публикаций: В среднем каждый пост получает 5 605 просмотров. В течение первых суток публикация набирает 2 513 просмотров.
- Реакции и взаимодействия: Аудитория активно поддерживает контент: среднее количество реакций на один пост — 56.
- 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 13 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 |  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 | 2 003 |
| 3 | What is Messier 24 actually showing us? | 2 246 |
| 4 | Tomorrow's picture: shells and streams | 2 265 |
| 5 |  2026 July 11
Messier 24: Sagittarius Star Cloud
Image Credit & Copyright: Chuck Ayoub
Unlike most entries in Charles Messier's famous catalog of deep sky objects, M24 is not a bright galaxy, star cluster, or nebula. It's a gap in nearby, obscuring interstellar dust clouds that allows a view of the distant stars in the Sagittarius spiral arm of our Milky Way galaxy. Direct your gaze through this gap with binoculars or a small telescope and you are looking through a window over 300 light-years wide at stars some 10,000 light-years or more from Earth. Sometimes called the Small Sagittarius Star Cloud, M24's luminous stars stretch across this gorgeous interstellar scene. Spanning over four full moons on the sky toward the constellation Sagittarius, the telescopic field of view includes dark markings B92 and B93 near the center of M24, along with other clouds of dust and glowing nebulae toward the center of the Milky Way.
🔗Discuss 🎞HD | 3 078 |
| 6 | Why is Mare Orientale (the Eastern Sea) located on the Moon's western edge? | 3 035 |
| 7 | Tomorrow's Picture:
Up in the sky,
A gap among the clouds
Window to the stars | 2 969 |
| 8 |  2026 July 10
Western Moon, Eastern Sea
Image Credit & Copyright: Guy Bardon
The Mare Orientale, Latin for Eastern Sea, is one of the most striking large scale lunar features. The youngest of the large lunar impact basins it's very difficult to see from an earthbound perspective. Still, captured on July 7 during a period of favorable tilt, or libration of the lunar nearside, the Eastern Sea can be found at the upper right in this sharp telescopic view. In the image, the large lunar mare is extremely foreshortened and stretches along the Moon's western edge. Formed by the impact of an asteroid over 3 billion years ago and nearly 1000 kilometers across, the impact basin's concentric circular features are ripples in the lunar crust. But they are a little easier to spot in more direct images of the region taken from lunar orbit. So why is the Eastern Sea at the Moon's western edge? The Mare Orientale lunar feature was named before 1961. That's when the convention labeling east and west on lunar maps was reversed.
🔗Discuss 🎞HD | 3 505 |
| 9 | What makes the Cosmic Bat Nebula glow red? | 3 256 |
| 10 | Tomorrow's picture: western Moon, eastern sea | 3 207 |
| 11 |  2026 July 9
The Red Glow of the Cosmic Bat Nebula
Image Credit & Copyright: Humbert Cédric
Text: Keighley Rockcliffe (NASA GSFC, UMBC CSST, CRESST II)
This Cosmic Bat wishes you a happy Summerween! This mid-year celebration of Halloween transcends hemispheres, even though summer in the Northern hemisphere is winter in the South. Contrary to its eery aura, the Cosmic Bat Nebula (LDN 43), not to be confused with the Bat Nebula (NGC 6995), is a vibrant birthplace for stars. A bit of young starlight peeks through the dense clouds of gas and dust that make up the Cosmic Bat’s 12 lightyear wingspan. The ultraviolet light from the young stars energizes the nebula’s hydrogen gas, causing it to glow an ominous red. The jet of glowing hydrogen gas emerging from the bat’s head hints at the star formation hidden within.
🔗Discuss 🎞HD/Hα | 4 026 |
| 12 | Tomorrow's picture: Cosmic bat 🦇 | 3 655 |
| 13 | If you could save one historic space mission by extending its lifetime, what would it be? | 3 839 |
| 14 |  2026 July 8
Swift Boost Mission
Image Credit: Katalyst Space
Text: Cecilia Chirenti (NASA GSFC, UMCP, CRESST II)
Sometimes we can all use a little help from a friend. NASA's Neil Gehrels Swift Observatory needs a boost to stay in orbit after almost 22 years of service. This video shows an artist's visualization of the Swift Boost Mission: The Katalyst's LINK spacecraft was launched aboard a Northrop Grumman Pegasus XL rocket on July 3 and it is now en route to rendezvous with Swift and boost it to a higher orbit over the course of the next several months. This type of maneuver has never been attempted before. If successful, it will be the technology demonstration of a new key capability to extended the lifetime of spacecraft in low Earth orbit, whose orbits decay over time. Swift has an array of instruments that observe the most energetic explosions in the Universe in gamma-rays, X-rays and ultraviolet, and the unique ability to repoint in their direction within tens of seconds. Astronomers around the world, and indeed all fans of cosmic explosions, are anxiously hoping for a successful mission!
🔗Discuss | 4 443 |
| 15 | Tomorrow's picture: helping Swift | 3 869 |
| 16 |  2026 July 7
NGC 6188: Dragons of Ara
Image Credit & Copyright: Rod Prazeres
Where can you find dragons fighting in the night sky? In the southern constellation of the Altar: Ara. The dragons are, of course, actually made of suggestively shaped gas and dust. The celestial home of the mythological battling beasts is cataloged as NGC 6188 and located about 4,000 light years away near the edge of a large molecular cloud. Massive, young stars of the embedded Ara OB1 association were formed there only a few million years ago, sculpting the dark shapes and powering the nebular glow with stellar winds and intense ultraviolet radiation. Joining NGC 6188 on this cosmic canvas, visible toward the lower right, is unusual emission nebula NGC 6164, also created by one of the region's massive stars. This impressively wide field picture, captured from Queensland, Australia, spans over 2 degrees (four full Moons).
🔗Discuss 🎞HD | 5 129 |
| 17 | Tomorrow's picture: dueling space dragons 🐉 | 4 396 |
| 18 | What causes zodiacal light? | 4 890 |
| 19 |  2026 July 6
Dueling Bands over the Atacama Desert
Image Credit & Copyright: Julien Looten
What are these two bands in the sky? The more commonly seen band is on the left and is the central band of our Milky Way galaxy. Our Sun orbits in the disk of this spiral galaxy so that from inside, it appears as a band of comparable brightness all the way around the sky. The less commonly seen band, on the right, is zodiacal light -- sunlight reflected from dust orbiting the Sun in our Solar System. Zodiacal light is brightest near the Sun and so is best seen just before sunrise or just after sunset. On some evenings, this ribbon of zodiacal light can appear quite prominent. It was discovered only in this century that zodiacal dust was mostly expelled by comets that have passed near Jupiter. The featured image was captured about a year ago from the Atacama Desert in Chile.
🔗Discuss 🎞HD/Annotated | 5 254 |
| 20 | Tomorrow's picture: dueling space bands | 4 423 |
