👋🏻 Durov "USERNAME"lar haqida!
"Yaqin vaqtgacha Telegram’dagi barcha foydalanuvchi nomlarining 70 foizi Erondan kelgan kibersquatterlar tomonidan faol bo‘lmagan kanallarda saqlangan. Bu qidiruv natijalarini chalkashtirib yuboradigan o'lik foydalanuvchi nomlari qabristonini yaratdi va millionlab Telegram foydalanuvchilariga o'z akkauntlari, guruhlari va kanallari uchun tegishli umumiy manzillarni tanlashiga to'sqinlik qildi.
Ushbu zaxiralangan foydalanuvchi nomlarini olishni istagan foydalanuvchilar ko'pincha hech qanday javob olmagan yoki aldanib qolishgan.
Yaxshiyamki, bu vaziyat o'zgara boshladi. Avgust oyi oʻrtalarida biz oʻtgan yil davomida boʻsh yoki faol boʻlmagan kanallarga bogʻlangan barcha ochiq Telegram manzillarini olib tashladik. Biz bu manzillarning 99 foizini asta-sekin qaytadan umumiy foydalanishga kiritamiz, bu safar algoritmik va geolokatsiya cheklovlari bilan faqat bir nechta foydalanuvchilar emas, balki ko‘proq foydalanuvchilar foyda ko‘rishi mumkin.
Eng yuqori baholangan qisqa foydalanuvchi nomlariga kelsak, ularni tarqatishning eng samarali va adolatli usuli men avvalgi postimda aytib o'tgan auktsion bo'lib tuyuladi. Shunday qilib, ushbu jozibali havolalarni qo'lga kiritganlar ularni yaxshi foydalanishga va taniqli t.me manzillarida joylashtirilgan original kontent bilan foydalanuvchilarimiz uchun qadrlashga undaydi.
Telegram foydalanuvchi nomlarini yig‘ib olganlar hafsalasi pir bo‘lganiga shubha qilmayman, lekin bu o‘zgarish foydalanuvchilarning katta qismiga foyda keltiradi. Men millionlab ajoyib Telegram manzillari qanday qayta tiklanishini va nihoyat bizning hamjamiyatimizga xizmat qila boshlashini intiqlik bilan kutaman.
P.S. Kelgusi voqealarni kutgan holda, bugun biz Telegramdagi har bir foydalanuvchi nomi uchun sindor.t.me kabi maxsus havolalarni qo'llab-quvvatlashni boshlaymiz. Ushbu veb-saytlar allaqachon istalgan brauzerda ishlaydi." - Pavel Durov
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💚@TGraphUz | YouTube
🪐 The mysterious "dark flow" observed in the movement of galaxy clusters like Abell 3627 suggests that something unseen—possibly related to dark matter or dark energy—is pulling vast regions of the universe in the same direction. This large-scale motion, detected using X-rays from hot gas in clusters, remains unexplained by normal gravity and hints at the hidden forces shaping the cosmos beyond what we can directly observe. ✨
#darkmatter⚡#universe⚡#galaxyclusters⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#cosmos⚡#space
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🪐 Deep in the Coma Cluster, a packed group of over 1,000 galaxies, astronomers have measured how dark energy—a mysterious force causing the universe to expand faster over time—stretches the space between galaxies. Observations show that the distance between massive galaxies in the Coma Cluster grows not just from their own motion, but because dark energy is steadily pushing the entire cosmic structure apart. ✨
#darkenergy⚡#galaxyclusters⚡#cosmology⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The Bullet Cluster, found in the constellation Carina, provides some of the clearest real-world evidence for dark matter—a mysterious, invisible substance making up most of the universe’s mass. When two galaxy clusters crashed together, X-ray images showed that most of the visible matter stayed at the center, but gravity maps revealed most of the mass had moved ahead, proving something unseen—dark matter—was driving the collision's aftermath. ✨
#darkmatter⚡#galaxyclusters⚡#carina⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The cosmic microwave background holds a hidden fingerprint—tiny temperature fluctuations mapped in exquisite detail by satellites like Planck reveal how the first stars and galaxies, such as those in the ancient cluster Abell 2744, grew from initial small ripples in the early universe. These faint variations, just millionths of a degree, became the seeds around which all the cosmic structures we see today first assembled. ✨
#cosmicmicrowavebackground⚡#earlyuniverse⚡#galaxyclusters⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The cosmic microwave background contains faint "Sunyaev-Zel’dovich effects," which happen when the ancient microwave light passes through hot gas in galaxy clusters like the Bullet Cluster. This process boosts the energy of some photons (light particles), leaving tiny shadows in the background glow—allowing astronomers to map both distant galaxy clusters and the hot plasma between galaxies by studying these subtle marks in the oldest light in the universe. ✨
#microwave⚡#background⚡#galaxyclusters⚡#plasma⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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