NASA's Astronomy Picture of the Day
Kanalga Telegram’da o‘tish
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.
Ko'proq ko'rsatish📈 Telegram kanali NASA's Astronomy Picture of the Day analitikasi
NASA's Astronomy Picture of the Day (@apod_telegram) Ingliz til segmentidagi kanali faol ishtirokchi. Hozirda hamjamiyat 34 827 obunachidan iborat bo'lib, Maʼlumotlar toifasida 409-o'rinni va AQSH mintaqasida 1 013-o'rinni egallagan.
📊 Auditoriya ko‘rsatkichlari va dinamika
невідомо sanasidan buyon loyiha tez o‘sib, 34 827 obunachiga ega bo‘ldi.
18 Iyul, 2026 dagi oxirgi ma’lumotlarga ko‘ra kanal barqaror faollikka ega. Oxirgi 30 kunda obunachilar soni 87 ga, so‘nggi 24 soatda esa 1 ga o‘zgardi va umumiy qamrov yuqori darajada qolmoqda.
- Tasdiqlash holati: Tasdiqlangan (Telegram tomonidan rasmiy tasdiq)
- Jalb etish (ER): Auditoriya o‘rtacha 15.60% darajada jalb etiladi. Nashrdan keyingi dastlabki 24 soatda kontent odatda umumiy obunachilar sonining 7.08% ini tashkil etuvchi reaksiyalarni to‘playdi.
- Post qamrovi: Har bir post o‘rtacha 5 433 marta ko‘riladi; birinchi sutkada odatda 2 466 ta ko‘rish yig‘iladi.
- Reaksiyalar va o‘zaro ta’sir: Auditoriya faol: har bir postga o‘rtacha 56 ta reaksiya keladi.
- Tematik yo‘nalishlar: Kontent copyright, orion, jupiter, dust, nasa kabi asosiy mavzularga jamlangan.
📝 Tavsif va kontent siyosati
Muallif resursni shaxsiy fikrni ifoda etish maydoni sifatida ta’riflaydi:
“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...”
Yuqori yangilanish chastotasi (oxirgi ma’lumot 19 Iyul, 2026 da olingan) sababli kanal doimo dolzarb va katta qamrovli bo‘lib qoladi. Analitika auditoriya kontent bilan faol hamkorlik qilishini, uni Maʼlumotlar toifasidagi muhim ta’sir nuqtasiga aylantirishini ko‘rsatadi.
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Kanal postlari
Why couldn't scientists simply collect the same solar wind samples on Earth?
| 2 |  2026 July 19
Flying Saucer Crash Lands in Utah Desert
Image Credit: USAF 388th Range Sqd., Genesis Mission, NASA
A flying saucer from outer space crash-landed in the Utah desert after being tracked by radar and chased by helicopters. The year was 2004, and no space aliens were involved. The saucer, pictured here, was the Genesis sample return capsule, part of a human-made robot Genesis spaceship launched in 2001 by NASA itself to study the Sun. The unexpectedly hard landing at over 300 kilometers per hour occurred because the parachutes did not open as planned. The Genesis mission had been orbiting the Sun collecting solar wind particles that are usually deflected away by Earth's magnetic field. Despite the crash landing, many return samples remained in good enough condition to analyze. Genesis-related discoveries included new details about the composition of the Sun and how the abundance of some types of elements differ across the Solar System. These results have provided intriguing clues into details of how the Sun and planets formed billions of years ago.
🔗Discuss 🎞HD | 2 007 |
| 3 | Tomorrow's picture: it came from space | 2 192 |
| 4 |  2026 July 18
Shadow and Rainbow
Image Credit & License: Dave Loschiavo
At sunset, an alignment of rainbow and mountain shadow was captured in this remarkable snapshot. The stunning view was recorded from a fire lookout on Smith Peak in the Plumas National Forest near Portola, California on July 13. Still, near sunset it's no accident that the majestic mountain shadow seems to point to the center of the graceful rainbow arc. Due to perspective and the long line of sight the mountain shadow naturally forms a tapering triangular shape, its apex positioned at the point opposite the Sun on the horizon. Following thunderstorms across the region, the rainbow arcs across the early evening sky, with its colorful and characteristic 42 degree arc formed as sunlight is refracted and reflected by the atmospheric water droplets. The geometric center of a rainbow arc lies at the antisolar point. And in this scene from the golden hour on planet Earth, that's also oposite the setting Sun along the distant horizon.
🔗Discuss 🎞HD | 2 982 |
| 5 | Tomorrow's picture: the antisolar horizon | 2 800 |
| 6 | Why might Tempel 2's dust trail appear narrower and brighter around July 20? | 2 984 |
| 7 |  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 | 3 234 |
| 8 | 🗨️ Tell us what you saw! | 3 214 |
| 9 | What creates the colorful glowing clouds in NGC 300? | 3 264 |
| 10 |  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 | 4 994 |
| 11 | What causes the red glow of a red sprite? | 3 220 |
| 12 | Tomorrow's picture: a galaxy bursting with excitement | 3 264 |
| 13 | 🗨️ Tell us what you think! | 3 701 |
| 14 |  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 | 4 040 |
| 15 | Why do scientists think Torifune has two lobes? | 3 919 |
| 16 |  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 | 4 350 |
| 17 | How often does the International Space Station orbit Earth? | 4 125 |
| 18 | Tomorrow's picture: asteroid double | 4 223 |
| 19 | If you could watch an aurora from one place, which would you choose? | 4 551 |
| 20 |  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 | 4 750 |
