NASA's Astronomy Picture of the Day
الذهاب إلى القناة على Telegram
To find and view past APODs, tap here: t.me/apodQA/3 NASA's APOD presence in Telegram: science.nasa.gov/apod Each day a different image of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
إظهار المزيد📈 نظرة تحليلية على قناة تيليجرام NASA's Astronomy Picture of the Day
تُعد قناة NASA's Astronomy Picture of the Day (@apod_telegram) في القطاع اللغوي الإنكليزية لاعباً نشطاً. يضم المجتمع حالياً 35 302 مشتركاً، محتلاً المرتبة 417 في فئة حقائق والمرتبة 1 161 في منطقة الولايات المتحدة.
📊 مؤشرات الجمهور والحراك
منذ تأسيسه في невідомо، حقق المشروع نمواً سريعاً وجمع 35 302 مشتركاً.
بحسب آخر البيانات بتاريخ 14 أكتوبر, 2026، تحافظ القناة على نشاط مستقر. خلال آخر 30 يوماً تغيّر عدد الأعضاء بمقدار 141، وفي آخر 24 ساعة بمقدار 0، مع بقاء الوصول العام مرتفعاً.
- حالة التحقق: موثّقة (مؤكدة رسمياً من تيليجرام)
- معدل التفاعل (ER): يبلغ متوسط تفاعل الجمهور 16.26%. وخلال أول 24 ساعة من النشر يحصد المحتوى عادةً 6.75% من ردود الفعل نسبةً إلى إجمالي المشتركين.
- وصول المنشورات: يحصل كل منشور على متوسط 5 735 مشاهدة. وخلال اليوم الأول يجمع عادةً 2 382 مشاهدة.
- التفاعلات والاستجابة: يتفاعل الجمهور بانتظام؛ متوسط التفاعلات لكل منشور يبلغ 73.
- الاهتمامات الموضوعية: يركز المحتوى على مواضيع رئيسية مثل copyright, orion, jupiter, dust, nasa.
📝 الوصف وسياسة المحتوى
يصف المؤلف القناة بأنها مساحة للتعبير عن الآراء الذاتية:
“To find and view past APODs, tap here:
t.me/apodQA/3
NASA's APOD presence in Telegram:
science.nasa.gov/apod
Each day a different image of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.”
بفضل وتيرة التحديث المرتفعة (أحدث البيانات بتاريخ 15 أكتوبر, 2026) تحافظ القناة على حداثتها ومستوى وصول مرتفع. وتُظهر التحليلات تفاعلاً نشطاً من الجمهور، ما يجعلها نقطة تأثير مهمة ضمن فئة حقائق.
35 302
المشتركون
لا توجد بيانات24 ساعات
+937 أيام
+14130 أيام
جارٍ تحميل البيانات
القنوات المماثلة
سحابة العلامات
الإشارات الواردة والصادرة
---
---
---
---
---
---
جذب المشتركين
أكتوبر '26أكتوبر '26
أكتوبر '26
+236
في 3 قنوات
سبتمبر '26
+572
في 5 قنوات
Get PRO
أغسطس '26
+677
في 7 قنوات
Get PRO
يوليو '26
+525
في 3 قنوات
Get PRO
يونيو '26
+480
في 5 قنوات
Get PRO
مايو '26
+519
في 8 قنوات
Get PRO
أبريل '26
+2 601
في 4 قنوات
Get PRO
مارس '26
+409
في 3 قنوات
Get PRO
فبراير '26
+690
في 3 قنوات
Get PRO
يناير '26
+581
في 2 قنوات
Get PRO
ديسمبر '25
+639
في 5 قنوات
Get PRO
نوفمبر '25
+768
في 2 قنوات
Get PRO
أكتوبر '25
+1 020
في 5 قنوات
Get PRO
سبتمبر '25
+879
في 2 قنوات
Get PRO
أغسطس '25
+1 630
في 9 قنوات
Get PRO
يوليو '25
+791
في 3 قنوات
Get PRO
يونيو '25
+595
في 4 قنوات
Get PRO
مايو '25
+797
في 6 قنوات
Get PRO
أبريل '25
+800
في 5 قنوات
Get PRO
مارس '25
+1 153
في 9 قنوات
Get PRO
فبراير '25
+1 395
في 7 قنوات
Get PRO
يناير '25
+1 685
في 7 قنوات
Get PRO
ديسمبر '24
+1 307
في 7 قنوات
Get PRO
نوفمبر '24
+1 381
في 5 قنوات
Get PRO
أكتوبر '24
+1 270
في 5 قنوات
Get PRO
سبتمبر '24
+1 586
في 4 قنوات
Get PRO
أغسطس '24
+1 565
في 5 قنوات
Get PRO
يوليو '24
+1 283
في 4 قنوات
Get PRO
يونيو '24
+1 756
في 1 قنوات
Get PRO
مايو '24
+2 027
في 5 قنوات
Get PRO
أبريل '24
+2 330
في 6 قنوات
Get PRO
مارس '24
+1 633
في 4 قنوات
Get PRO
فبراير '24
+2 058
في 4 قنوات
Get PRO
يناير '24
+5 383
في 2 قنوات
| التاريخ | نمو المشتركين | الإشارات | القنوات | |
| 15 أكتوبر | +30 | |||
| 14 أكتوبر | 0 | |||
| 13 أكتوبر | +13 | |||
| 12 أكتوبر | +14 | |||
| 11 أكتوبر | +8 | |||
| 10 أكتوبر | +21 | |||
| 09 أكتوبر | +40 | |||
| 08 أكتوبر | +21 | |||
| 07 أكتوبر | +21 | |||
| 06 أكتوبر | +10 | |||
| 05 أكتوبر | +13 | |||
| 04 أكتوبر | +7 | |||
| 03 أكتوبر | +14 | |||
| 02 أكتوبر | +9 | |||
| 01 أكتوبر | +15 |
منشورات القناة
2026 October 14
Mars and the Beehive Under an Aurora
Image Credit & Copyright: Petr Horálek (Institute of Physics in Opava), Josef Kujal, Vojan Höfer
What a cosmic coincidence! In today’s image, Mars joins the Beehive cluster (M44 or Praesepe) below an auroral curtain and above a horizon of happy little trees near Lansjärv, Sweden. An eruption off the Sun reached Earth on October 10th, 2026 causing strong disturbances in Earth’s magnetic field. Energetic particles from the eruption collide with and energize the molecules in Earth’s atmosphere, which release that extra energy as the colorful aurora captured here. Auroras, or guovssahasat in North Sámi, is traditionally viewed with respect by the Sámi people indigenous to Sweden and other Arctic regions. Coincidentally, Mars appeared closest to the center of the Beehive cluster in the sky at the time. Although bees have been to space, the Beehive cluster is actually a swarm of young stars. Their rotation periods have helped humanity learn about how stars spin slower over time as they lose mass through their stellar winds.
🔗Discuss 🎞HD
| 2 |  2026 October 13
Desert Stairway to Heaven
Image Credit & Copyright: Julien Looten
This stairway in Chile brings you only a little bit closer to heaven. But ooh, the sky above it makes you wonder. For example, you may wonder about the dark lane of our own Milky Way galaxy rising behind the expansive Atacama Desert in Chile, the band of zodiacal light on the upper left, the green and red airglow just above the horizon, the star Spica in the zodiacal light stripe, and, at the very top on the right, the Small Magellanic Cloud galaxy. The Desert Staircase sculpture is in the foreground, and this image was timed to catch the picturesque peering perch just in front of the near-vertical Milky Way band. Upon close inspection of the horizon you can find, left to right, some Andes Mountains, the Licancabur volcano, and the town lights of San Pedro de Atacama. The featured wide-angle composite was captured in July 2025.
🔗Discuss 🎞HD/Annotated | 2 998 |
| 3 | Tomorrow's picture: stairway to heaven | 2 819 |
| 4 |  2026 October 12
Jupiter and the Moons
Image Credit & Copyright: Chirag Upreti
How many moons can you see? The best answer is five: four orbiting Jupiter and Luna orbiting Earth. This multi-moon picture was possible because Earth's Moon moved directly in front of Jupiter last week. The featured image is a series of exposures near alignment taken from Westchester, New York, USA. The sunlit crescent of Earth's Moon, on the lower left, is overexposed, while the Moon's night side, on the upper right, is faintly illuminated by Earthshine. Lined up nearly vertically above our Moon, listed from bottom to top, are Jupiter's bright Galilean satellites: Ganymede, Io, Callisto, and Europa. Callisto, Ganymede, and Io are larger than Earth's Moon, while Europa is only slightly smaller. NASA's robotic spacecraft Juno is currently orbiting Jupiter and has made close passes near three of these moons.
🔗Discuss 🎞HD | 3 466 |
| 5 | Tomorrow's picture: Moons Planet | 3 276 |
| 6 |  2026 October 11
Ice Fishing for Cosmic Neutrinos
Image Credit: NSF, B. Gudbjartsson, IceCube Collaboration
Scientists are melting holes in the bottom of the world. In fact, almost 100 holes melted near the South Pole are now being used as an astronomical observatory. Astronomers with the IceCube Neutrino Observatory lowered a long string knotted with basketball-sized light detectors into each vertical lake. The water in each hole soon refreezes. The detectors attached to the strings are sensitive to blue light emitted in the surrounding clear ice. Such light results from fast-moving secondary particles liberated when high-energy neutrinos emitted by powerful processes out in the universe collide with ice molecules. IceCube has now detected many illuminating neutrinos. Pictured in 2010, one of the last of IceCube's detector strings is lowered into the freezing abyss, making IceCube the largest neutrino detector ever created. In recognition of unprecedented discoveries, it was announced earlier this week that a founding leader of the IceCube Collaboration will be awarded the Nobel Prize in Physics.
🔗Discuss 🎞HD | 3 918 |
| 7 |  2026 October 10
Lunar Farside
Image Credit & Copyright: NASA / GSFC / Arizona State Univ. / Lunar Reconnaissance Orbiter
Tidally locked in synchronous rotation, the Moon always presents its familiar nearside to denizens of planet Earth. From lunar orbit, the Moon's farside can become familiar, though. In fact this sharp picture, a mosaic from the Lunar Reconnaissance Orbiter's wide angle camera, is centered on the lunar farside. Part of a global mosaic of over 15,000 images acquired between November 2009 and February 2011, the highest resolution version shows features at a scale of 100 meters per pixel. Surprisingly, the rough and battered surface of the farside looks very different from the nearside covered with smooth dark lunar maria. A likely explanation is that the farside crust is thicker, making it harder for molten material from the interior to flow to the surface and form dark, smooth maria.
🔗Discuss 🎞HD | 4 164 |
| 8 | Tomorrow's picture: farside | 4 054 |
| 9 |  2026 October 9
Stickney Crater
Image Credit & Copyright: HiRISE, MRO, LPL (U. Arizona), NASA
Stickney Crater, the largest crater on the martian moon Phobos, is named for Chloe Angeline Stickney Hall, mathematician and wife of astronomer Asaph Hall. Asaph Hall discovered both the Red Planet's moons in 1877. Over 9 kilometers across, Stickney is nearly half the diameter of Phobos itself, so large that the impact that blasted out the crater likely came close to shattering the tiny moon. This enhanced-color image of Stickney and surroundings was recorded by the HiRISE camera onboard the Mars Reconnaissance Orbiter as it passed within some six thousand kilometers of Phobos in March of 2008. Even though the surface gravity of asteroid-like Phobos is less than 1/1000th Earth's gravity, streaks suggest loose material slid down inside the crater walls over time. Light bluish regions near the crater's rim could indicate a relatively freshly exposed surface. The origin of the curious grooves along the surface is mysterious but may be related to tidal stresses experienced by close-orbiting Phobos or the crater-forming impact itself.
🔗Discuss 🎞HD | 4 885 |
| 10 | Tomorrow's picture: bumpy | 4 203 |
| 11 |  2026 October 8
The Saturn System Smörgåsbord
Image Credit & Copyright: Tom Williams
How was the Saturn system imaged so clearly? Astrophotographer Tom Williams was able to capture such exquisite details due to near-perfect atmospheric conditions. This means more than a cloudless sky. Pockets of air at different temperatures and densities move around and bend light as it travels through Earth’s atmosphere, distorting astronomy images. This is called “seeing”. Less air motion means clearer images. Distortions from seeing are more obvious for Solar System objects like Saturn. These objects appear smaller in the sky compared to nebulas and galaxies. The higher magnification used to observe them in detail also magnifies the effects of seeing. The astrophotographer reduced the impact of seeing using the lucky imaging technique: take many short-exposure images very quickly with a high-speed camera and add up the clearest images. Which object in this smörgåsbord interests you? Perhaps the lakes on Titan or the icy stripes of Enceladus? Maybe the gaps and spokes in Saturn’s rings?
🔗Discuss 🎞HD | 5 131 |
| 12 | Tomorrow's picture: smörgåsbord | 4 441 |
| 13 | Why is Pa 30's central star especially important for understanding the 1181 explosion? | 4 981 |
| 14 |  2026 October 7
Supernova Remnant Pa 30
Image Credit & Copyright: International Gemini Observatory/NOIRLab/NSF/AURA. Acknowledgment: PI: T. Cunningham (Center for Astrophysics - Harvard & Smithsonian). Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab), T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab).
"Happy New Year!" No, wait, this is not a fireworks display. This image shows Nebula Pa 30, observed with the Gemini North Telescope in Hawai'i. It is likely the remnant of an old supernova explosion: separate historical records by Chinese, Japanese and Arabic astronomers tell of a "guest star" that appeared in the sky for 185 days in the year 1181. It is believed that this bright new point of light came from the supernova that caused the fireworks in Pa 30. Astronomers don't know exactly what happened in this unusual explosion, classified as a Type Iax supernova, but it is thought to be caused by the merger of two white dwarfs. The mysterious central star in the image is extremely hot and produces a strong wind, possibly forming the radial filaments. Look closely at them: those pearl-like knots stringing the filaments are 4 light-days in diameter. Understanding how a supernova created this amazing nebula continues an 845-year old mystery (and counting).
🔗Discuss 🎞HD | 5 173 |
| 15 | 2026 October 7
The Saturn System Smörgåsbord
Image Credit & Copyright: Tom Williams
How was the Saturn system imaged so clearly? Astrophotographer Tom Williams was able to capture such exquisite details due to near-perfect atmospheric conditions. This means more than a cloudless sky. Pockets of air at different temperatures and densities move around and bend light as it travels through Earth’s atmosphere, distorting astronomy images. This is called “seeing”. Less air motion means clearer images. Distortions from seeing are more obvious for Solar System objects like Saturn. These objects appear smaller in the sky compared to nebulas and galaxies. The higher magnification used to observe them in detail also magnifies the effects of seeing. The astrophotographer reduced the impact of seeing using the lucky imaging technique: take many short-exposure images very quickly with a high-speed camera and add up the clearest images. Which object in this smörgåsbord interests you? Perhaps the lakes on Titan or the icy stripes of Enceladus? Maybe the gaps and spokes in Saturn’s rings?
🔗Discuss 🎞HD | 837 |
| 16 | Tomorrow's picture: a spokey image | 4 796 |
| 17 |  2026 October 6
A Complete Auroral Oval from SMILE
Video Credit: ESA, CAS, SMILE, UVI
Have you ever seen a complete auroral oval? You can't see one from the ground because it makes too large a circle around one of Earth's magnetic poles. But spacecraft high above the Earth can see them. The featured video from ESA and CAS's robotic SMILE spacecraft shows not only a full auroral oval, but using ultraviolet light, one that occurred during the day. The time-lapse covers about an hour in late July and shows visually how variable and turbulent auroras really are. The points of light on the sides are distant stars that appear to move only because SMILE's camera view shifts as the spacecraft orbits the Earth. A goal of SMILE is to better understand how the Sun's wind interacts with the Earth's magnetosphere -- and so better understand how to protect astronauts, spacecraft, and ground-based electrical grids from solar storms.
🔗Discuss 🎞HD | 6 073 |
| 18 | Tomorrow's picture: a smile | 5 027 |
| 19 |  2026 October 5
M104: The Sombrero Galaxy's Tidal Streams
Image Credit & Copyright: Engelbert Vollmer
A deep image of the Sombrero galaxy reveals surprises. M104 is named the Sombrero galaxy because, on shorter exposures, it looks like a hat. A key defining feature of this huge galaxy is a dark brim of dust that circles the disk galaxy's center. A much longer exposure, however, brings up a hairy past where a bright, hazy halo is revealed that extends well past the central disk and contains many unresolved stars. Surprisingly, in this stellar haze, structures can be seen that include a diagonal ring. These structures and tidal streams provide fresh evidence that M104 had a violent past and is surely the result of collisions and mergers of smaller galaxies. Light takes about 30 million years to reach us from the Sombrero galaxy, which fully spans about 150 thousand light years across. The featured image was taken over seven days in mid-2026 from Namibia.
🔗Discuss 🎞HD | 6 341 |
| 20 | Tomorrow's picture: hat stream | 5 098 |
