{"id":3293,"date":"2025-08-05T09:52:54","date_gmt":"2025-08-05T07:52:54","guid":{"rendered":"https:\/\/www.astro-novinky.eu\/?p=3293"},"modified":"2025-08-05T09:53:51","modified_gmt":"2025-08-05T07:53:51","slug":"3293","status":"publish","type":"post","link":"https:\/\/www.astro-novinky.eu\/index.php\/2025\/08\/05\/3293\/","title":{"rendered":"Pozoruhodn\u00e9 \u00fakazy na srpnov\u00e9 no\u010dn\u00ed obloze"},"content":{"rendered":"

Leto\u0161n\u00ed srpen nab\u00eddne opravdu pozoruhodn\u00e9 nebesk\u00e9 \u00fakazy. Krom\u011b ka\u017edoro\u010dn\u00edch Perseid, kter\u00e9 tento rok kv\u016fli svitu M\u011bs\u00edce nebudou pozorovateln\u00e9 za nejlep\u0161\u00edch podm\u00ednek, se nab\u00edz\u00ed pohled hned k n\u011bkolika planet\u00e1m. Ty budou v pr\u016fb\u011bhu m\u011bs\u00edce nab\u00edzet nejr\u016fzn\u011bj\u0161\u00ed o\u010dima pozorovateln\u00e9 a nesm\u00edrn\u011b fotogenick\u00e9 konstelace. U\u017e 12. srpna se p\u0159itom do\u010dk\u00e1me \u00fahlov\u011b t\u011bsn\u00e9ho nebesk\u00e9ho setk\u00e1n\u00ed nejjasn\u011bj\u0161\u00edch z nich: Jupiteru a Venu\u0161e.<\/p>\n

12. srpna: Velk\u00e9 setk\u00e1n\u00ed nejjasn\u011bj\u0161\u00edch planet<\/h4>\n
\"Konjunkce<\/a>
Konjunkce Venu\u0161e s Jupiterem na ja\u0159e 2023 nad ostrovem Thoddoo. Foto: petr Hor\u00e1lek\/Fyzik\u00e1ln\u00ed \u00fastav v Opav\u011b.<\/figcaption><\/figure>\n

K velmi vz\u00e1cn\u00e9 nebesk\u00e9 pod\u00edvan\u00e9 se sch\u00fdl\u00ed v\u00a0\u010dasn\u00fdch rann\u00edch hodin\u00e1ch v\u00a0\u00fater\u00fd 12. srpna 2025<\/strong>. Nejjasn\u011bj\u0161\u00ed planety Slune\u010dn\u00ed soustavy \u2013 Venu\u0161e<\/em> a Jupiter<\/em> \u2013 se na rann\u00ed obloze p\u0159ibl\u00ed\u017e\u00ed na \u00fahlovou vzd\u00e1lenost jen 51,6′<\/strong> (m\u00e9n\u011b jak dva m\u011bs\u00ed\u010dn\u00ed \u00fapl\u0148ky vedle sebe). Samotn\u00e9 maxim\u00e1ln\u00ed p\u0159ibl\u00ed\u017een\u00ed nastane a\u017e po rozedn\u011bn\u00ed, ale u\u017e p\u0159ed rozb\u0159eskem planety budou \u00fahlov\u011b dosti bl\u00edzko. Jasn\u00e1 dvojice vyjde nad severov\u00fdchodn\u00edm obzorem okolo 2:30 SEL\u010c<\/strong> (\u010das v\u00fdchodu se bude li\u0161it v z\u00e1vislosti na m\u00edst\u011b pozorov\u00e1n\u00ed \u0159\u00e1dov\u011b v minut\u00e1ch), slab\u0161\u00ed Jupiter bude le\u017eet severn\u011b (vlevo naho\u0159e) od v\u00fdrazn\u011b jasn\u011bj\u0161\u00ed Venu\u0161e. P\u0159i pohledu pouh\u00fdma o\u010dima budou dosti bl\u00edzko sebe a vizu\u00e1ln\u011b nep\u0159ehl\u00e9dnuteln\u00e9 i z\u00a0m\u011bst a\u017e do sv\u00edt\u00e1n\u00ed okolo 5. hodiny rann\u00ed<\/strong>, kdy u\u017e budou le\u017eet vysoko nad v\u00fdchodn\u00edm obzorem (v t\u00e9 dob\u011b se n\u00edzko nad v\u00fdchodo-severov\u00fdchodn\u00edm obzorem bude d\u00e1t vyhledat tak\u00e9 planeta Merkur).<\/p>\n

Ve st\u0159edn\u011b velk\u00e9m dalekohledu (s pr\u016fm\u011brem nad 10 cm) budeme moci Jupiter s Venu\u0161\u00ed sledovat v jednom zorn\u00e9m poli<\/strong>. Venu\u0161e se bude jevit jako velmi n\u00e1padn\u00fd b\u011blav\u00fd ov\u00e1lek s f\u00e1z\u00ed podobnou M\u011bs\u00edci mezi \u00fapl\u0148kem a posledn\u00ed \u010dtvrt\u00ed, Jupiter jako kotou\u010dek s pruhy (atmosf\u00e9rick\u00fdmi p\u00e1sy) a v jeho bl\u00edzkosti se v jedn\u00e9 rovin\u011b uk\u00e1\u017e\u00ed 3 \u201eGalileovsk\u00e9 m\u011bs\u00edce\u201c \u2013 Io<\/em>, Ganymedes<\/em> a Callisto<\/em>. \u010ctvrt\u00fd, Europa<\/em>, se bude prom\u00edtat ve v\u011bt\u0161\u00edch teleskopech p\u0159ed samotnou planetou pobl\u00ed\u017e \u201eVelk\u00e9 \u010derven\u00e9 skvrny\u201c (slavn\u00e1 dlouhotrvaj\u00edc\u00ed Jupiterova bou\u0159e) a od kotou\u010de se vzd\u00e1l\u00ed a\u017e po 4. hodin\u011b rann\u00ed. Dal\u0161\u00edho t\u011bsn\u00e9ho setk\u00e1n\u00ed Jupiteru a Venu\u0161e se do\u010dk\u00e1me u\u017e o necel\u00fd rok pozd\u011bji \u2013 na ve\u010dern\u00ed obloze 9. \u010dervna 2026. Tehdy bude planety d\u011blit \u00fahlov\u00e1 vzd\u00e1lenost o polovinu v\u011bt\u0161\u00ed ne\u017e p\u0159i tomto srpnov\u00e9m \u00fakazu. Nenechte si jej proto uj\u00edt.<\/p>\n

\"Planety<\/a>
Planety Venu\u0161e a Jupiter b\u011bhem sv\u00e9 konjunkce na rann\u00ed obloze 12. srpna 2025. U\u017e v mal\u00e9m dalekohledu pak rozli\u0161\u00edme ov\u00e1lnou f\u00e1zi Venu\u0161e a kotou\u010dek Jupiteru s jeho jasn\u00fdmi m\u011bs\u00edci (obd\u00e9ln\u00edkov\u00fd v\u00fd\u0159ez). Velk\u00fd dalekohled odhal\u00ed dal\u0161\u00ed detaily (kruhov\u00e9 v\u00fd\u0159ezy). Zdroj: Petr Hor\u00e1lek\/Stellarium\/Fyzik\u00e1ln\u00ed \u00fastav v Opav\u011b.<\/figcaption><\/figure>\n

A to nen\u00ed v\u0161echno.<\/strong> Shodou okolnost\u00ed v to r\u00e1no bude pozvolna sp\u011bt k maximu aktivity meteorick\u00fd roj Perseid. Aby toho nebylo m\u00e1lo, v t\u00e9 sam\u00e9 dob\u011b, kdy se naskytne pohled na p\u0159ibl\u00ed\u017een\u00ed obou jasn\u00fdch planet, se nad ji\u017en\u00edm obzorem bude nach\u00e1zet M\u011bs\u00edc<\/em> \u00fahlov\u011b nedaleko planet Saturn<\/em> a Neptun<\/em><\/strong>, kter\u00e9 v\u00a0to r\u00e1no budou rovn\u011b\u017e v\u00a0konjunkci (\u00fahlov\u011b asi 1\u00b0 14\u2019 daleko od sebe). Zat\u00edmco M\u011bs\u00edc a Saturn budou vid\u011bt pohodln\u011b o\u010dima, Neptun je t\u0159eba vyhledat mal\u00fdm dalekohledem, nap\u0159\u00edklad triedrem. Brzk\u00e9 r\u00e1no 12. srpna 2025 tedy nab\u00eddne hned n\u011bkolik vz\u00e1cn\u00fdch nebesk\u00fdch \u00fakaz\u016f najednou!<\/p>\n

\"Konjunkce<\/a>
Konjunkce Saturnu a Neptunu pobl\u00ed\u017e jasn\u00e9ho M\u011bs\u00edce 12. srpna 2025. Na nalezen\u00ed Neptunu je zapot\u0159eb\u00ed alespo\u0148 mal\u00fd dalekohled. Zdroj: Petr Hor\u00e1lek\/Stellarium\/Fyzik\u00e1ln\u00ed \u00fastav v Opav\u011b.<\/figcaption><\/figure>\n

12.\/13. srpna: Perseidy za m\u011bs\u00ed\u010dn\u00edho svitu<\/h4>\n
\"Maximum<\/a>
Maximum meteorick\u00e9ho roje Perseidy v roce 2016 z Parku tmav\u00e9 oblohy Ve\u013ek\u00e1 Fatra na Slovensku. Foto: Petr Hor\u00e1lek.<\/figcaption><\/figure>\n

Nejobl\u00edben\u011bj\u0161\u00ed \u201ekosmick\u00fd oh\u0148ostroj\u201c roku \u2013 meteorick\u00fd roj <\/strong>Perseid<\/strong><\/em> \u2013 se v roce 2025 net\u011b\u0161\u00ed p\u0159\u00edzniv\u00fdm podm\u00ednk\u00e1m, ale i tak si jej nenechte uj\u00edt. Pod\u00edvan\u00e1 u\u017e toti\u017e neodmysliteln\u011b pat\u0159\u00ed k letn\u00edmu p\u0159\u00edrodn\u00edmu koloritu. S t\u00edmto obdob\u00edm souvis\u00ed i v\u00edce volna, teplej\u0161\u00ed a \u010dasto p\u0159\u00edzniv\u011bj\u0161\u00ed po\u010das\u00ed, mo\u017enosti v\u00fdlet\u016f do p\u0159\u00edrody a z\u00e1\u017eitk\u016f pod \u201e\u0161ir\u00e1kem\u201c a je mo\u017enost uvid\u011bt opravdu jasn\u00e9 meteory ve v\u011bt\u0161\u00ed \u010detnost\u00ed.<\/p>\n

Maximum roje, za n\u00edm\u017e stoj\u00ed kometa 109P\/Swift-Tuttle<\/em> a kter\u00e9 s\u00a0sebou nese p\u0159ipomenut\u00ed p\u0159es 1760 let star\u00e9 nespravedlnosti<\/a> (nespravedlivou a krutou popravu svat\u00e9ho Vav\u0159ince), vych\u00e1z\u00ed v\u00a0roce 2025 na noc 12.\/13. srpna<\/strong> (z \u00fater\u00fd na st\u0159edu) a m\u011bs\u00ed\u010dn\u00ed f\u00e1ze p\u0159ipad\u00e1 3 dny po \u00fapl\u0148ku<\/strong>. N\u00e1\u0161 soused tedy bude sv\u00fdm svitem v\u00fdrazn\u011b ru\u0161it po v\u011bt\u0161inu noci v\u00a0souhv\u011bzd\u00ed Ryb<\/strong>.<\/strong> Perseidy ov\u0161em nejsou aktivn\u00ed jen v\u00a0noc maxima, jejich aktivita za\u010d\u00edn\u00e1 u\u017e ve t\u0159et\u00ed dek\u00e1d\u011b \u010dervence a kon\u010d\u00ed v\u00a0z\u00e1v\u011bru srpna. Vyplat\u00ed se tedy pozorovat zejm\u00e9na v\u00a0t\u00fddnech p\u0159ed maximem, tedy p\u0159ibli\u017en\u011b<\/strong> od 1. srpna 2025, a to v\u017edy v \u010dasn\u00fdch rann\u00edch hodin\u00e1ch.<\/strong> Nejv\u00edce meteor\u016f je v\u017edy vid\u011bt r\u00e1no mezi p\u016flnoc\u00ed a 5. hodinou rann\u00ed. V noc maxima roje bude mo\u017en\u00e9 za svitu M\u011bs\u00edce spat\u0159it jen ty nejjasn\u011bj\u0161\u00ed meteory, zejm\u00e9na mezi p\u016flnoci a 4. hodinou rann\u00ed by frekvence mohla vystoupat na 20-30 meteor\u016f za hodinu. Vytrval\u00e9 pozorovatele na rann\u00ed obloze p\u0159ed rozb\u0159eskem odm\u011bn\u00ed vz\u00e1cn\u00e1 konjunkce jasn\u00fdch planet Venu\u0161e a Jupiteru (viz p\u0159edchoz\u00ed \u00fakaz).<\/p>\n

20. srpna: Bohat\u00e1 nebesk\u00e1 konstelace<\/h4>\n

Opravdu velmi bohatou konstelaci nab\u00eddne na rann\u00ed obloze 20. srpna 2025<\/strong> hned \u0161est v\u00fdrazn\u00fdch objekt\u016f oblohy. P\u011bt z\u00a0nich \u2013 jasn\u00e9 planety Venu\u0161e<\/em> a Jupiter<\/em>, M\u011bs\u00edc<\/em> (s popelav\u00fdm svitem) a hv\u011bzdy Castor<\/em> a Pollux<\/em> ze souhv\u011bzd\u00ed Bl\u00ed\u017eenc\u016f<\/strong> \u2013 se uskup\u00ed do \u00fahlov\u00e9 bl\u00edzkosti do tvaru mot\u00fdla, p\u0159i\u010dem\u017e toto nebesk\u00e9 uskupen\u00ed bude pozorovateln\u00e9 u\u017e od 3. hodiny rann\u00ed SEL\u010c n\u00edzko nad severov\u00fdchodn\u00edm obzorem. Jak uskupen\u00ed pozvolna vystoup\u00e1 v\u00fd\u0161 nad v\u00fdchodn\u00ed obzor a za\u010dne pozvolna sv\u00edtat, okolo 4:30 SEL\u010c se je\u0161t\u011b nad obzorem objev\u00ed planeta Merkur<\/em><\/strong>. Tato mimo\u0159\u00e1dn\u011b bohat\u00e1 nebesk\u00e1 konstelace bude snadno pozorovateln\u00e1 i z m\u011bst a jednozna\u010dn\u011b bude pat\u0159it mezi ty nejsn\u00e1ze fotografovateln\u00e9 v pr\u016fb\u011bhu cel\u00e9ho roku 2025. Nebude probl\u00e9m ji zachytit i na fotoapar\u00e1ty pokro\u010dilej\u0161\u00edch chytr\u00fdch telefon\u016f.<\/p>\n

\"Mimo\u0159\u00e1dn\u011b<\/a>
Mimo\u0159\u00e1dn\u011b pestr\u00e1 nebesk\u00e1 konstelace t\u0159\u00ed planet, M\u011bs\u00edce a dvou jasn\u00fdch hv\u011bzd 20. srpna 2025 v \u010dasn\u00fdch rann\u00edch hodin\u00e1ch. Zdroj: Petr Hor\u00e1lek\/Fyzik\u00e1ln\u00ed \u00fastav v Opav\u011b\/Stellarium.<\/figcaption><\/figure>\n

31. srpna \u00a0– 2. z\u00e1\u0159\u00ed: Venu\u0161e u Jesli\u010dek<\/h4>\n
\"P\u0159echod<\/a>
P\u0159echod planety Venu\u0161e okolo hv\u011bzdokupy M44 (Jesli\u010dky) v souhv\u011bzd\u00ed Raka mezi 31. srpnem a 2. z\u00e1\u0159\u00edm 2025. \u00dakaz bude pozorovateln\u00fd v \u010dasn\u00fdch rann\u00edch hodin\u00e1ch. Zdroj: Petr Hor\u00e1lek\/Fyzik\u00e1ln\u00ed \u00fastav v Opav\u011b\/Stellarium.<\/figcaption><\/figure>\n

Na p\u0159elomu srpna a z\u00e1\u0159\u00ed, konkr\u00e9tn\u011b mezi <\/strong>31. srpnem a 2. z\u00e1\u0159\u00edm 2025<\/strong>, budeme moci n\u00edzko nad severov\u00fdchodn\u00edm a\u017e v\u00fdchodn\u00edm obzorem p\u0159ed rozb\u0159eskem o\u010dima a je\u0161t\u011b l\u00e9pe v mal\u00fdch dalekohledech pozorovat vizu\u00e1ln\u011b velmi p\u011bknou <\/strong>pod\u00edvanou: Planeta Venu\u0161e<\/em><\/strong> se bude prom\u00edtat pobl\u00ed\u017e otev\u0159en\u00e9 hv\u011bzdokupy M44<\/a><\/em><\/strong> (lidov\u011b zvanou \u201eJesli\u010dky\u201c nebo \u201eV\u010del\u00ed \u00fal\u201c) v souhv\u011bzd\u00ed Raka. Hv\u011bzdokupa je pozorovateln\u00e1 mimo m\u011bsta i pouh\u00fdma o\u010dima, jej\u00ed plnou kr\u00e1su ov\u0161em ocen\u00edme a\u017e p\u0159i pohledu mal\u00fdm dalekohledem (nap\u0159\u00edklad v triedru). Jej\u00ed nejjasn\u011bj\u0161\u00ed \u010d\u00e1st na obloze zab\u00edr\u00e1 plochu o pr\u016fm\u011bru p\u0159ibli\u017en\u011b 1,5\u00b0, tedy t\u0159\u00ed m\u011bs\u00ed\u010dn\u00edch \u00fapl\u0148k\u016f vedle sebe.<\/p>\n

K\u00a0hv\u011bzdokup\u011b se Venu\u0161e \u00fahlov\u011b p\u0159ibl\u00ed\u017e\u00ed z jihoz\u00e1padu 31. srpna 2025<\/strong>. Nejbl\u00ed\u017ee se \u201eJit\u0159enka\u201c ke st\u0159edu kupy prom\u00edtne 1. z\u00e1\u0159\u00ed 2025, a to ji\u017en\u011b.<\/strong> V t\u00e9 dob\u011b bude m\u00edt planeta jasnost -3,9 magnitudy a bude opravdu jasn\u00fdm objektem viditeln\u00fdm i z m\u011bst. P\u0159i pohledu o\u010dima se bude zd\u00e1t, jako by jasn\u00e1 Venu\u0161e le\u017eela pobl\u00ed\u017e mlhav\u00e9 skvrnky.<\/p>\n

Cel\u00fd zd\u00e1nliv\u00fd pr\u016fchod Venu\u0161e pobl\u00ed\u017e Jesli\u010dek bude mo\u017en\u00e9 vyhl\u00ed\u017eet ka\u017ed\u00fd ze zm\u00edn\u011bn\u00fdch dn\u00ed \u010dasn\u011b r\u00e1no od \u010dtvrt\u00e9 hodiny do rozb\u0159esku<\/strong> n\u00edzko nad v\u00fdchodo-severov\u00fdchodn\u00edm obzorem. Viditeln\u00fd bude i o\u010dima, ale mnohem kr\u00e1sn\u011bj\u0161\u00ed pohled nab\u00eddne mal\u00fd dalekohled. K\u00a0pozorov\u00e1n\u00ed p\u0159itom posta\u010d\u00ed opravdu jen b\u011b\u017en\u00fd triedr. V\u00a0n\u011bm se z\u00e1hy vedle Venu\u0161e objev\u00ed n\u011bkolik des\u00edtek nejjasn\u011bj\u0161\u00edch hv\u011bzd t\u00e9to asi 600 sv\u011bteln\u00fdch let vzd\u00e1len\u00e9 otev\u0159en\u00e9 hv\u011bzdokupy.<\/p>\n

Cel\u00fd m\u011bs\u00edc: Ml\u00e9\u010dn\u00e1 dr\u00e1ha a tenk\u00e9 Saturnovy prstence<\/h4>\n
\"Pohled<\/a>
Pohled do letn\u00ed Ml\u00e9\u010dn\u00e9 dr\u00e1hy nad Se\u010dskou p\u0159ehradou. Foto: Petr Hor\u00e1lek\/Fyzik\u00e1ln\u00ed \u00fastav v Opav\u011b.<\/figcaption><\/figure>\n

V srpnu se lze nejsn\u00e1ze kochat nejkr\u00e1sn\u011bj\u0161\u00edm \u00fasekem Ml\u00e9\u010dn\u00e9 dr\u00e1hy<\/em><\/strong>. Ten v druh\u00e9 polovin\u011b l\u00e9ta nach\u00e1z\u00edme n\u00edzko nad ji\u017en\u00edm obzorem v m\u00edstech, kde v tomto sm\u011bru neru\u0161\u00ed sv\u011btla ze vzd\u00e1len\u00fdch m\u011bst. N\u00e1dhern\u00e9 je vyhl\u00ed\u017eet Ml\u00e9\u010dnou dr\u00e1hu v\u017edy, kdy\u017e v\u016fbec neru\u0161\u00ed sv\u00fdm svitem M\u011bs\u00edc. Letn\u00ed \u00fasek Ml\u00e9\u010dn\u00e9 dr\u00e1hy je pozorovateln\u00fd v pr\u016fb\u011bhu letn\u00edch m\u011bs\u00edc\u016f celou noc, v srpnu je nad hlavou u\u017e po setm\u011bn\u00ed<\/strong>. Pokud budete daleko od m\u011bst, kde neru\u0161\u00ed sv\u011bteln\u00e9 zne\u010di\u0161t\u011bn\u00ed (nap\u0159\u00edklad v jedn\u00e9 z oblast\u00ed tmav\u00e9 oblohu v \u010cesku \u010di na Slovensku \u2013 v Man\u011bt\u00edn\u011b, Jizersk\u00fdch hor\u00e1ch, Beskydech), uvid\u00edte st\u0159\u00edb\u0159it\u00fd p\u00e1s hv\u011bzd s bohat\u00fdmi strukturami a\u017e k ji\u017en\u00edmu obzoru, kde se v souhv\u011bzd\u00edch \u0160t\u00edra a St\u0159elce Ml\u00e9\u010dn\u00e1 dr\u00e1ha opticky roz\u0161i\u0159uje. T\u00edm sm\u011brem se d\u00edv\u00e1me do centra na\u0161\u00ed Galaxie.<\/p>\n

T\u00e9m\u011b\u0159 celou noc je tak\u00e9 pozorovateln\u00e1 planeta Saturn<\/em><\/strong>. Najdeme ji pouh\u00fdma o\u010dima v souhv\u011bzd\u00ed Ryb jako pon\u011bkud v\u00fdrazn\u011bj\u0161\u00ed objekt v t\u00e9to oblasti. Jist\u011b ale pot\u011b\u0161\u00ed ka\u017ed\u00e9ho majitele u\u017e men\u0161\u00edho hv\u011bzd\u00e1\u0159sk\u00e9ho dalekohledu nebo n\u00e1v\u0161t\u011bvn\u00edka nejbli\u017e\u0161\u00ed lidov\u00e9 hv\u011bzd\u00e1rny, nebo\u0165 pr\u00e1v\u011b dalekohled nam\u00ed\u0159en\u00fd k t\u00e9to planet\u011b nab\u00edz\u00ed pohled i na jej\u00ed prstence. Prstence jsou p\u0159itom tak rozs\u00e1hl\u00e9, \u017ee a\u010dkoliv je planeta Saturn od n\u00e1s fyzicky okolo sv\u00e9 opozice p\u0159es 1 miliardu kilometr\u016f daleko, jsou jako sv\u011btl\u00fd krou\u017eek obep\u00ednaj\u00edc\u00ed kotou\u010dek planety viditeln\u00e9 u\u017e ve v\u011bt\u0161\u00edm binokul\u00e1ru ustaven\u00e9m na pevn\u00e9m stativu. Proto je spat\u0159il u\u017e Galileo Galilei sv\u00fdm primitivn\u00edm dalekohledem na po\u010d\u00e1tku 17. stolet\u00ed a nazval Saturn \u201eplanetou s u\u0161ima\u201c.<\/p>\n

\"V<\/a>
V roce 2025 se rovina Saturnov\u00fdch prstenc\u016f bude prom\u00edtat p\u0159i pozorov\u00e1n\u00ed ze Zem\u011b pod nejmen\u0161\u00edm \u00fahlem. Znovu takov\u00e1 situace nastane a\u017e v roce 2038. Zdroj: NASA.<\/figcaption><\/figure>\n

D\u00edky sklonu osy Saturnovy rotace v\u016f\u010di rovin\u011b ekliptiky se ale i prstence jev\u00ed r\u016fzn\u011b naklon\u011bn\u00e9, a pr\u00e1v\u011b v roce 2025 jsou velmi tenk\u00e9 \u2013 d\u00edv\u00e1me se na n\u011b t\u00e9m\u011b\u0159 z boku<\/strong>. Saturn tedy vypad\u00e1 jako kotou\u010dek s tenkou gymnastickou obru\u010d\u00ed. Takto tenk\u00fdch prstenc\u016f se p\u0159itom znovu do\u010dk\u00e1me a\u017e na podzim roku 2038.<\/strong><\/p>\n

Kontakty a dal\u0161\u00ed informace:<\/h3>\n

Mgr. Petr Hor\u00e1lek<\/strong>
\nPR v\u00fdstup\u016f evropsk\u00fdch projekt\u016f F\u00da SU v\u00a0Opav\u011b<\/em>
\n<\/em>Email:\u00a0petr.horalek@slu.cz
\n<\/a>Telefon: +420\u00a0732\u00a0826\u00a0853<\/p>\n

RNDr. Tom\u00e1\u0161 Gr\u00e1f,\u00a0Ph.D.<\/strong>
\nFyzik\u00e1ln\u00ed \u00fastav SU v\u202fOpav\u011b,\u00a0vedouc\u00ed\u00a0observato\u0159e WHOO! a Unisf\u00e9ry<\/em>
\nEmail:\u00a0tomas.graf@fpf.slu.cz<\/a>
\nTelefon: +420 553 684\u202f548<\/p>\n","protected":false},"excerpt":{"rendered":"

Leto\u0161n\u00ed srpen nab\u00eddne opravdu pozoruhodn\u00e9 nebesk\u00e9 \u00fakazy. Krom\u011b ka\u017edoro\u010dn\u00edch Perseid, kter\u00e9 tento rok kv\u016fli svitu M\u011bs\u00edce nebudou pozorovateln\u00e9 za nejlep\u0161\u00edch podm\u00ednek, se nab\u00edz\u00ed pohled hned k n\u011bkolika planet\u00e1m. Ty budou v pr\u016fb\u011bhu m\u011bs\u00edce nab\u00edzet nejr\u016fzn\u011bj\u0161\u00ed o\u010dima pozorovateln\u00e9 a nesm\u00edrn\u011b fotogenick\u00e9 konstelace. U\u017e 12. srpna se p\u0159itom do\u010dk\u00e1me \u00fahlov\u011b t\u011bsn\u00e9ho nebesk\u00e9ho setk\u00e1n\u00ed nejjasn\u011bj\u0161\u00edch z nich: Jupiteru a Venu\u0161e.<\/p>\n","protected":false},"author":7,"featured_media":3294,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"colormag_page_container_layout":"default_layout","colormag_page_sidebar_layout":"default_layout","footnotes":""},"categories":[26,27,30],"tags":[],"class_list":["post-3293","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-aktuality","category-clanky","category-ukazy"],"yoast_head":"\nPozoruhodn\u00e9 \u00fakazy na srpnov\u00e9 no\u010dn\u00ed obloze - Astro-novinky.eu<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/www.astro-novinky.eu\/index.php\/2025\/08\/05\/3293\/\" \/>\n<meta property=\"og:locale\" content=\"sk_SK\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Pozoruhodn\u00e9 \u00fakazy na srpnov\u00e9 no\u010dn\u00ed obloze - Astro-novinky.eu\" \/>\n<meta property=\"og:description\" content=\"Leto\u0161n\u00ed srpen nab\u00eddne opravdu pozoruhodn\u00e9 nebesk\u00e9 \u00fakazy. Krom\u011b ka\u017edoro\u010dn\u00edch Perseid, kter\u00e9 tento rok kv\u016fli svitu M\u011bs\u00edce nebudou pozorovateln\u00e9 za nejlep\u0161\u00edch podm\u00ednek, se nab\u00edz\u00ed pohled hned k n\u011bkolika planet\u00e1m. Ty budou v pr\u016fb\u011bhu m\u011bs\u00edce nab\u00edzet nejr\u016fzn\u011bj\u0161\u00ed o\u010dima pozorovateln\u00e9 a nesm\u00edrn\u011b fotogenick\u00e9 konstelace. 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