{"id":468,"date":"2026-06-20T13:37:07","date_gmt":"2026-06-20T11:37:07","guid":{"rendered":"https:\/\/hujer.net\/?p=468"},"modified":"2026-06-20T13:39:24","modified_gmt":"2026-06-20T11:39:24","slug":"putovani-za-galaxiemi-ii-jaro-2026","status":"publish","type":"post","link":"https:\/\/hujer.net\/?p=468","title":{"rendered":"Putov\u00e1n\u00ed za Galaxiemi II. (Jaro 2026)"},"content":{"rendered":"

Dnes tu pro v\u00e1s m\u00e1m druh\u00e9 pokra\u010dov\u00e1n\u00ed m\u00e9ho putov\u00e1n\u00ed za m\u00e9n\u011b zn\u00e1m\u00fdmi galaxiemi z katalogu NGC. N\u011bkter\u00e9 z nich jsou z\u00e1rove\u0148 za\u0159azen\u00e9 v Caldwellov\u011b \u010di Herschelov\u011b katalogu, p\u0159\u00edpadn\u011b v Arpov\u011b katalogu podivn\u00fdch galaxi\u00ed (Arp). Tento \u010dl\u00e1nek p\u0159\u00edmo navazuje na prvn\u00ed \u010d\u00e1st z b\u0159ezna 2026, kterou si m\u016f\u017eete p\u0159e\u010d\u00edst zde: Zimn\u00ed putov\u00e1n\u00ed za Galaxiemi<\/a>.<\/p>\n

Jarn\u00ed obloha roku 2026 mi p\u0159inesla \u0159adu jasn\u00fdch noc\u00ed, kter\u00e9 jsem pln\u011b vyu\u017eil k zachycen\u00ed t\u011bchto fascinuj\u00edc\u00edch vzd\u00e1len\u00fdch vesm\u00edrn\u00fdch ostrov\u016f. Poj\u010fme se na n\u011b pod\u00edvat podrobn\u011bji.<\/p>\n

\n

1. NGC 5248 (Caldwell 45)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 21. 3. 2026<\/p>\n

\"NGC<\/a><\/p>\n

Tato n\u00e1dhern\u00e1 spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou se nach\u00e1z\u00ed v souhv\u011bzd\u00ed Past\u00fd\u0159e. Pat\u0159\u00ed do rodiny Caldwellova katalogu jako C45. Na sn\u00edmku jsou kr\u00e1sn\u011b patrn\u00e1 jej\u00ed v\u00fdrazn\u00e1, pevn\u011b zavinut\u00e1 spir\u00e1ln\u00ed ramena, kter\u00e1 se t\u00e1hnou daleko od jasn\u00e9ho, hork\u00e9ho j\u00e1dra. V tomto j\u00e1dru prob\u00edh\u00e1 intenzivn\u00ed p\u0159ekotn\u00e1 tvorba nov\u00fdch hv\u011bzd (tzv. starburst region), co\u017e z n\u00ed d\u011bl\u00e1 velmi vd\u011b\u010dn\u00fd c\u00edl pro astrofotografii.<\/p>\n

\n

2. NGC 4889 (Caldwell 35)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 22. 3. 2026<\/p>\n

\"NGC<\/a><\/p>\n

V srdci zn\u00e1m\u00e9 kupy galaxi\u00ed ve Vlasu Bereniky (Coma Cluster) le\u017e\u00ed ob\u0159\u00ed eliptick\u00e1 galaxie NGC 4889. Je domovem jedn\u00e9 z nejv\u011bt\u0161\u00edch dosud objeven\u00fdch supermasivn\u00edch \u010dern\u00fdch d\u011br ve vesm\u00edru. Na sn\u00edmku se sice jev\u00ed jako nen\u00e1padn\u00fd mlhav\u00fd obl\u00e1\u010dek, ale nenechte se m\u00fdlit \u2013 obklopuje ji obrovsk\u00e9 mno\u017estv\u00ed men\u0161\u00edch galaxi\u00ed a samotn\u00fd objekt svou hmotnost\u00ed i rozm\u011bry naprosto zasti\u0148uje na\u0161i Ml\u00e9\u010dnou dr\u00e1hu.<\/p>\n

\n

3. NGC 4490 (The Cocoon Galaxy)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 23. 3. 2026<\/p>\n

\"NGC<\/a><\/p>\n

Galaxie Z\u00e1motek (Cocoon Galaxy) v souhv\u011bzd\u00ed Honic\u00edch ps\u016f je uk\u00e1zkov\u00fdm p\u0159\u00edkladem kosmick\u00e9 kolize. NGC 4490 je gravita\u010dn\u011b siln\u011b deformov\u00e1na interakc\u00ed se sv\u00fdm men\u0161\u00edm sousedem NGC 4485 (kter\u00fd se nach\u00e1z\u00ed t\u011bsn\u011b mimo hlavn\u00ed z\u00e1b\u011br nebo na jeho okraji). Tento gravita\u010dn\u00ed tanec naru\u0161il p\u016fvodn\u00ed spir\u00e1ln\u00ed strukturu a za\u017eehl masivn\u00ed vlnu hv\u011bzdotvorby, d\u00edky n\u00ed\u017e galaxie z\u00e1\u0159\u00ed v mnoha spektrech.<\/p>\n

\n

4. NGC 4656 (Herschel 280 – Hockey Stick Galaxy)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 27. 3. 2026<\/p>\n

\"NGC<\/a><\/p>\n

Hokejka, neboli NGC 4656, je dal\u0161\u00ed velmi pok\u0159iven\u00e1 galaxie z Honic\u00edch ps\u016f. Sv\u016fj charakteristick\u00fd zahnut\u00fd tvar z\u00edskala kv\u016fli ned\u00e1vn\u00e9mu bl\u00edzk\u00e9mu pr\u016fletu kolem sousedn\u00ed ob\u0159\u00ed galaxie NGC 4631 (Velryba). Na konci jej\u00edho dlouh\u00e9ho ramene je patrn\u00fd jasn\u00fd uzel (ozna\u010dovan\u00fd n\u011bkdy jako NGC 4657), kter\u00fd tvo\u0159\u00ed pr\u00e1v\u011b onu pomyslnou \u010depel hokejky.<\/p>\n

\n

5. NGC 4697 (Caldwell 52)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 6. 4. 2026<\/p>\n

\"NGC<\/a><\/p>\n

Tato eliptick\u00e1 galaxie se nach\u00e1z\u00ed v souhv\u011bzd\u00ed Panny. P\u0159esto\u017ee eliptick\u00e9 galaxie \u010dasto postr\u00e1daj\u00ed divok\u00e9 prachov\u00e9 struktury a mlad\u00e9 otev\u0159en\u00e9 hv\u011bzdokupy, NGC 4697 zaujme sv\u00fdm symetrick\u00fdm, jasn\u00fdm profilem, kter\u00fd plynule sl\u00e1bne do okoln\u00edho temn\u00e9ho prostoru. Je nejjasn\u011bj\u0161\u00edm \u010dlenem mal\u00e9 skupiny galaxi\u00ed le\u017e\u00edc\u00ed kousek od hlavn\u00ed kupy v Pann\u011b.<\/p>\n

\n

6. NGC 4753<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 7. 4. 2026<\/p>\n

\"NGC<\/a><\/p>\n

NGC 4753 v Pann\u011b je naprosto fascinuj\u00edc\u00ed \u010do\u010dkovit\u00e1 galaxie, zn\u00e1m\u00e1 svou neuv\u011b\u0159iteln\u011b slo\u017eitou s\u00edt\u00ed temn\u00fdch prachov\u00fdch p\u00e1s\u016f obep\u00ednaj\u00edc\u00edch jej\u00ed j\u00e1dro. Tyto prachov\u00e9 struktury jsou pravd\u011bpodobn\u011b poz\u016fstatkem men\u0161\u00ed galaxie bohat\u00e9 na plyn, kterou NGC 4753 pohltila zhruba p\u0159ed miliardou let. Pro astrofotografy p\u0159edstavuje skv\u011blou v\u00fdzvu pro vykreslen\u00ed jemn\u00fdch kontrast\u016f.<\/p>\n

\n

7. NGC 4618 (Herschel 273) a NGC 4625<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 8. 4. 2026<\/p>\n

\"NGC<\/a><\/p>\n

Tato dvojice asymetrick\u00fdch trpasli\u010d\u00edch galaxi\u00ed v Honic\u00edch psech je v astronomii velmi popul\u00e1rn\u00ed. Zvl\u00e1\u0161tnost\u00ed NGC 4618 je, \u017ee m\u00e1 pouze jedno jedin\u00e9, siln\u011b vyvinut\u00e9 spir\u00e1ln\u00ed rameno, co\u017e ji \u0159ad\u00ed mezi tzv. Magellanovy spir\u00e1ln\u00ed galaxie. Jej\u00ed men\u0161\u00ed sousedka NGC 4625 vykazuje podobn\u00e9 anom\u00e1lie, co\u017e jasn\u011b ukazuje na vz\u00e1jemnou gravita\u010dn\u00ed interakci.<\/p>\n

\n

8. NGC 4725 (Arp 159, NGC 4747 a NGC 4712)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 9. 4. 2026<\/p>\n

\"Arp<\/a><\/p>\n

Tento n\u00e1dhern\u00fd \u0161iroko\u00fahl\u00fd z\u00e1b\u011br n\u00e1s zav\u00e1d\u00ed do souhv\u011bzd\u00ed Vlas\u016f Bereniky. Dominantou pole je velk\u00e1, netradi\u010dn\u00ed jednoramenn\u00e1 spir\u00e1ln\u00ed galaxie NGC 4725. V jej\u00edm t\u011bsn\u00e9m sousedstv\u00ed se nach\u00e1z\u00ed siln\u011b naru\u0161en\u00e1 galaxie NGC 4747 (kter\u00e1 kv\u016fli slapov\u00fdm sil\u00e1m p\u0159ich\u00e1z\u00ed o sv\u00e1 ramena) a v pozad\u00ed klidn\u011b odpo\u010d\u00edv\u00e1 vzd\u00e1len\u011bj\u0161\u00ed spir\u00e1la NGC 4712. Cel\u00e1 skupina je zanesena v Arpov\u011b katalogu jako Arp 159.<\/p>\n

\n

9. NGC 5364 (Skupina galaxi\u00ed v Pann\u011b)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 16. a 17. 4. 2026<\/p>\n

\"Skupina<\/a><\/p>\n

NGC 5364 je uk\u00e1zkovou spir\u00e1ln\u00ed galaxi\u00ed s designem \u201egrand design\u201c v souhv\u011bzd\u00ed Panny. Jej\u00ed ramena jsou v\u0161ak m\u00edrn\u011b asymetrick\u00e1, co\u017e zp\u016fsobuje gravita\u010dn\u00ed vliv bl\u00edzk\u00e9 \u010do\u010dkovit\u00e9 galaxie NGC 5363, kter\u00e1 na sn\u00edmku dominuje svou vysokou povrchovou jasnost\u00ed. Spole\u010dn\u011b s dal\u0161\u00edmi drobn\u00fdmi galaxiemi v poli tvo\u0159\u00ed kr\u00e1snou prostorovou kompozici.<\/p>\n

\n

10. NGC 5322 (Herschel 308)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 18. 4. 2026<\/p>\n

\"NGC<\/a><\/p>\n

V severn\u00edm souhv\u011bzd\u00ed Velk\u00e9 medv\u011bdice najdeme \u010distou eliptickou galaxii NGC 5322, kterou poprv\u00e9 pozoroval William Herschel pod ozna\u010den\u00edm H I.308. Galaxie skr\u00fdv\u00e1 vnit\u0159n\u00ed hv\u011bzdn\u00fd disk rotuj\u00edc\u00ed opa\u010dn\u00fdm sm\u011brem ne\u017e jej\u00ed vn\u011bj\u0161\u00ed ob\u00e1lka, co\u017e nazna\u010duje, \u017ee v minulosti vznikla splynut\u00edm dvou velk\u00fdch galaxi\u00ed.<\/p>\n

\n

11. NGC 5395 (Arp 84 – The Heron Galaxy a NGC 5394)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 21. 4. 2026<\/p>\n

\"Arp<\/a><\/p>\n

Galaxie Volavka (Heron Galaxy) v souhv\u011bzd\u00ed Honic\u00edch ps\u016f je \u00fachvatn\u00fdm interaktivn\u00edm p\u00e1rem galaxi\u00ed. V\u011bt\u0161\u00ed spir\u00e1la NGC 5395 p\u0159edstavuje \u201et\u011blo\u201c volavky, zat\u00edmco men\u0161\u00ed NGC 5394 s dlouh\u00fdmi otev\u0159en\u00fdmi rameny tvo\u0159\u00ed \u201ekrk a hlavu\u201c. Gravita\u010dn\u00ed s\u00edly mezi nimi vytvo\u0159ily dlouh\u00e9 slapov\u00e9 ohony pln\u00e9 nov\u011b vznikaj\u00edc\u00edch hv\u011bzdokup.<\/p>\n

\n

12. NGC 5216 (Arp 104 – Galactic Yo-Yo a NGC 5218)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 22. a 23. 4. 2026<\/p>\n

\"Arp<\/a><\/p>\n

Tento p\u00e1r, zn\u00e1m\u00fd jako Galaktick\u00e9 jojo, le\u017e\u00ed v souhv\u011bzd\u00ed Velk\u00e9 medv\u011bdice. Ob\u011b galaxie (kulat\u011bj\u0161\u00ed eliptick\u00e1 NGC 5216 a spir\u00e1ln\u00ed NGC 5218) jsou navz\u00e1jem propojeny velmi tenk\u00fdm, ale dlouh\u00fdm hv\u011bzdn\u00fdm mostem, kter\u00fd se t\u00e1hne temnotou jako prov\u00e1zek od joja. Zachytit tento jemn\u00fd most vy\u017eaduje vynikaj\u00edc\u00ed pr\u016fzra\u010dnost oblohy a dostatek expozi\u010dn\u00edho \u010dasu.<\/p>\n

\n

13. NGC 2655 (Arp 225)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 28. 4. 2026<\/p>\n

\"Arp<\/a><\/p>\n

NGC 2655 v souhv\u011bzd\u00ed \u017dirafy je jasn\u00e1 \u010do\u010dkovit\u00e1 galaxie s aktivn\u00edm galaktick\u00fdm j\u00e1drem (Seyfertova galaxie). Na hlubok\u00fdch sn\u00edmc\u00edch odhaluje komplexn\u00ed strukturu vn\u011bj\u0161\u00edch prachov\u00fdch a hv\u011bzdn\u00fdch slupek, kter\u00e9 jsou p\u0159\u00edm\u00fdm d\u016fsledkem pohlcen\u00ed men\u0161\u00edho galaktick\u00e9ho souseda v ned\u00e1vn\u00e9 minulosti.<\/p>\n

\n

14. NGC 3147 (Herschel 146)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 29. 4. 2026<\/p>\n

<\/a><\/p>\n

Tato \u010dist\u00e1, symetrick\u00e1 spir\u00e1ln\u00ed galaxie se nach\u00e1z\u00ed bl\u00edzko severn\u00edho nebesk\u00e9ho p\u00f3lu v souhv\u011bzd\u00ed Draka. NGC 3147 je klasifikov\u00e1na jako Seyfertova galaxie typu II s velmi kompaktn\u00edm aktivn\u00edm j\u00e1drem, kter\u00e9 ukr\u00fdv\u00e1 supermasivn\u00ed \u010dernou d\u00edru. Jej\u00ed spir\u00e1ln\u00ed ramena jsou hust\u011b poseta modrav\u00fdmi oblastmi zrodu nov\u00fdch hv\u011bzd.<\/p>\n

\n

15. NGC 4410 (Arp 324 a NGC 4411)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 25. 4., 2. 5., 8. 5. a 9. 5. 2026<\/p>\n

\"Arp<\/a><\/p>\n

Tento projekt si vy\u017e\u00e1dal hned n\u011bkolik kv\u011btnov\u00fdch a dubnov\u00fdch noc\u00ed. V poli se nach\u00e1z\u00ed spir\u00e1ln\u00ed galaxie NGC 4411 a extr\u00e9mn\u011b zaj\u00edmav\u00e1 skupina interaguj\u00edc\u00edch galaxi\u00ed zanesen\u00e1 jako Arp 324 (j\u00e1drem je pr\u00e1v\u011b NGC 4410). Tyto objekty vykazuj\u00ed siln\u00e9 gravita\u010dn\u00ed mosty a radiov\u00e9 emise, co\u017e sv\u011bd\u010d\u00ed o velmi divok\u00fdch procesech prob\u00edhaj\u00edc\u00edch uvnit\u0159 t\u00e9to t\u011bsn\u00e9 kupy v Pann\u011b.<\/p>\n

\n

16. NGC 4157<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 30. 4. 2026<\/p>\n

\"NGC<\/a><\/p>\n

NGC 4157 v souhv\u011bzd\u00ed Velk\u00e9 medv\u011bdice je n\u00e1dhern\u00e1 spir\u00e1ln\u00ed galaxie, kterou vid\u00edme t\u00e9m\u011b\u0159 p\u0159esn\u011b z profilu (edge-on). Cel\u00fdm jej\u00edm diskem se t\u00e1hne v\u00fdrazn\u00fd, ost\u0159e ohrani\u010den\u00fd prachov\u00fd p\u00e1s, kter\u00fd d\u00e1v\u00e1 galaxii dramatick\u00fd vzhled. V minul\u00fdch letech v n\u00ed bylo zaznamen\u00e1no n\u011bkolik jasn\u00fdch supernov.<\/p>\n

\n

17. NGC 4151 (a NGC 4156)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 1. a 21. 5. 2026<\/p>\n

\"NGC<\/a><\/p>\n

Galaxie NGC 4151 v Honic\u00edch psech je v astronomick\u00e9 komunit\u011b zn\u00e1m\u00e1 jako \u201eSauronovo oko\u201c kv\u016fli sv\u00e9mu neobvykl\u00e9mu vzhledu v n\u011bkter\u00fdch spektrech a extr\u00e9mn\u011b aktivn\u00edmu j\u00e1dru. Jedn\u00e1 se o jednu z nejbli\u017e\u0161\u00edch a nejl\u00e9pe prostudovan\u00fdch Seyfertov\u00fdch galaxi\u00ed v\u016fbec. T\u011bsn\u011b vedle n\u00ed se nach\u00e1z\u00ed men\u0161\u00ed a klidn\u011bj\u0161\u00ed spir\u00e1ln\u00ed spole\u010dnice NGC 4156.<\/p>\n

\n

18. Abell 2151 (Kupa galaxi\u00ed v Herkulovi)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 16. a 17. 5. 2026<\/p>\n

\"Abell<\/a><\/p>\n

Abell 2151 je neuv\u011b\u0159iteln\u011b bohat\u00e1 kupa galaxi\u00ed v souhv\u011bzd\u00ed Herkula, vzd\u00e1len\u00e1 od n\u00e1s p\u0159ibli\u017en\u011b 500 milion\u016f sv\u011bteln\u00fdch let. Na rozd\u00edl od jin\u00fdch kup zde najdeme obrovsk\u00e9 mno\u017estv\u00ed spir\u00e1ln\u00edch galaxi\u00ed, z nich\u017e mnoh\u00e9 spolu prokazateln\u011b koliduj\u00ed. Sn\u00edmek nab\u00edz\u00ed fascinuj\u00edc\u00ed pohled do hlubok\u00e9ho vesm\u00edru, kde je doslova ka\u017ed\u00fd druh\u00fd fl\u00ed\u010dek samostatn\u00fdm galaktick\u00fdm ostrovem.<\/p>\n

\n

19. NGC 5746 (Skupina kolem NGC 5740 a NGC 5738)<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 18. 5. 2026<\/p>\n

\"NGC<\/a><\/p>\n

V t\u00e9to oblasti v souhv\u011bzd\u00ed Panny dominuje masivn\u00ed spir\u00e1ln\u00ed galaxie vid\u011bn\u00e1 zboku (NGC 5746), kter\u00e1 vykazuje jasnou st\u0159edovou p\u0159\u00ed\u010dku a propracovan\u00fd prachov\u00fd prstenec. V jej\u00edm okol\u00ed se nach\u00e1z\u00ed men\u0161\u00ed, vizu\u00e1ln\u011b velmi zaj\u00edmav\u00e9 galaxie NGC 5740 a drobn\u00e1 NGC 5738, kter\u00e9 spole\u010dn\u011b vytv\u00e1\u0159ej\u00ed \u00fachvatnou jarn\u00ed kompozici.<\/p>\n

\n

20. NGC 6015<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 22. a 23. 5. 2026<\/p>\n

\"NGC<\/a><\/p>\n

P\u0159esouv\u00e1me se do souhv\u011bzd\u00ed Draka, kde le\u017e\u00ed izolovan\u00e1 spir\u00e1ln\u00ed galaxie NGC 6015. Jejich ramena jsou pom\u011brn\u011b voln\u011b rozev\u0159en\u00e1 a protkan\u00e1 jemn\u00fdmi prachov\u00fdmi strukturami a drobn\u00fdmi r\u016f\u017eov\u00fdmi H-II oblastmi p\u0159ekotn\u00e9 tvorby hv\u011bzd. Na tmav\u00e9 obloze p\u016fsob\u00ed velmi elegantn\u00edm dojmem.<\/p>\n

\n

21. NGC 6384<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 7. a 11. 6. 2026<\/p>\n

\"NGC<\/a><\/p>\n

S bl\u00ed\u017e\u00edc\u00edm se l\u00e9tem se focen\u00ed p\u0159esouv\u00e1 do souhv\u011bzd\u00ed Hadono\u0161e. NGC 6384 je p\u0159ekr\u00e1sn\u00e1, jasn\u00e1 spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou. Jej\u00ed \u0161irok\u00e1 ramena se rozb\u00edhaj\u00ed do okoln\u00edho prostoru pln\u00e9ho pop\u0159edov\u00fdch hv\u011bzd na\u0161\u00ed Ml\u00e9\u010dn\u00e9 dr\u00e1hy, co\u017e vytv\u00e1\u0159\u00ed skv\u011bl\u00fd prostorov\u00fd kontrast mezi na\u0161\u00edm galaktick\u00fdm sousedstv\u00edm a vzd\u00e1len\u00fdm vesm\u00edrem.<\/p>\n

\n

22. NGC 6503<\/h3>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 18. 6. 2026<\/p>\n

<\/a><\/p>\n

Na z\u00e1v\u011br jarn\u00edho putov\u00e1n\u00ed tu m\u00e1me galaxii NGC 6503 nach\u00e1zej\u00edc\u00ed se na samotn\u00e9m okraji ob\u0159\u00ed pr\u00e1zdnoty zvan\u00e9 M\u00edstn\u00ed pr\u00e1zdnota (Local Void) v souhv\u011bzd\u00ed Draka. Tato osamocen\u00e1 spir\u00e1ln\u00ed galaxie vynik\u00e1 kr\u00e1sn\u00fdm modrav\u00fdm lemem mlad\u00fdch hv\u011bzdokup a jasn\u00fdm, kompaktn\u00edm j\u00e1drem. Symbolicky tak uzav\u00edr\u00e1 mou jarn\u00ed galaktickou sez\u00f3nu p\u0159ed n\u00e1stupem kr\u00e1tk\u00fdch letn\u00edch noc\u00ed.<\/p>\n

S p\u0159ich\u00e1zej\u00edc\u00edm slunovratem sice hlavn\u00ed jarn\u00ed sez\u00f3na galaxi\u00ed v Pann\u011b a Vlasech Bereniky definitivn\u011b skon\u010dila a oblohu ovl\u00e1dnou mlhoviny Ml\u00e9\u010dn\u00e9 dr\u00e1hy, ale astronomick\u00fd podzim klepe na dve\u0159e d\u0159\u00edv, ne\u017e by se mohlo zd\u00e1t. U\u017e v srpnu n\u00e1s toti\u017e \u010dekaj\u00ed dal\u0161\u00ed nesm\u00edrn\u011b zaj\u00edmav\u00e9 galaxie, kter\u00e9 se za\u010dnou zvedat nad obzor v souhv\u011bzd\u00edch Andromedy a Pegasa.<\/p>\n

Velice se t\u011b\u0161\u00edm nap\u0159\u00edklad na focen\u00ed Caldwell 44 \u2013 \u00fachvatn\u00e9 spir\u00e1ln\u00ed galaxie NGC 7479 v Pegasovi, kter\u00e9 se pro jej\u00ed dynamick\u00fd tvar trefn\u011b p\u0159ezd\u00edv\u00e1 Superman Galaxy<\/em>. Dal\u0161\u00ed velkou srpnovou v\u00fdzvou bude NGC 6822 (Caldwell 57) v St\u0159elci, zn\u00e1m\u00e1 jako Barnardova galaxie. Ta je sice v na\u0161ich zem\u011bpisn\u00fdch \u0161\u00ed\u0159k\u00e1ch kv\u016fli sv\u00e9 n\u00edzk\u00e9 deklinaci obt\u00ed\u017en\u011b fotiteln\u00e1, ale o to v\u011bt\u0161\u00ed radost z jej\u00edho \u00fasp\u011b\u0161n\u00e9ho zachycen\u00ed bude.<\/p>\n

Douf\u00e1m, \u017ee se v\u00e1m druh\u00e9 pokra\u010dov\u00e1n\u00ed m\u00e9ho putov\u00e1n\u00ed l\u00edbilo. U\u017eijte si nadch\u00e1zej\u00edc\u00ed letn\u00ed slunovrat, tepl\u00e9 noci pod hv\u011bzdami a v srpnu tak\u00e9 zatm\u011bn\u00ed Slunce na na\u0161\u00ed spole\u010dn\u00e9 v\u00fdprav\u011b do \u0160pan\u011blska.
\nJasnou oblohu v\u0161em!<\/p>\n

Zpracoval Roman<\/p>\n","protected":false},"excerpt":{"rendered":"

Dnes tu pro v\u00e1s m\u00e1m druh\u00e9 pokra\u010dov\u00e1n\u00ed m\u00e9ho putov\u00e1n\u00ed za m\u00e9n\u011b zn\u00e1m\u00fdmi galaxiemi z katalogu NGC. N\u011bkter\u00e9 z nich jsou z\u00e1rove\u0148 za\u0159azen\u00e9 v Caldwellov\u011b \u010di Herschelov\u011b katalogu, p\u0159\u00edpadn\u011b v Arpov\u011b katalogu podivn\u00fdch galaxi\u00ed (Arp). Tento \u010dl\u00e1nek p\u0159\u00edmo navazuje na prvn\u00ed \u010d\u00e1st z b\u0159ezna 2026, kterou si m\u016f\u017eete p\u0159e\u010d\u00edst zde: Zimn\u00ed putov\u00e1n\u00ed za Galaxiemi. Jarn\u00ed obloha […]<\/p>\n","protected":false},"author":1,"featured_media":471,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7,9],"tags":[15],"class_list":["post-468","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-astronomie","category-deepsky","tag-galaxie"],"_links":{"self":[{"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts\/468","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=468"}],"version-history":[{"count":2,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts\/468\/revisions"}],"predecessor-version":[{"id":472,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts\/468\/revisions\/472"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/media\/471"}],"wp:attachment":[{"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=468"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=468"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=468"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}