{"id":481,"date":"2026-09-23T06:05:00","date_gmt":"2026-09-23T04:05:00","guid":{"rendered":"https:\/\/hujer.net\/?p=481"},"modified":"2026-09-20T22:13:39","modified_gmt":"2026-09-20T20:13:39","slug":"putovani-za-galaxiemi-iii-leto-2026","status":"publish","type":"post","link":"https:\/\/hujer.net\/?p=481","title":{"rendered":"Putov\u00e1n\u00ed za Galaxiemi III. (L\u00e9to 2026)"},"content":{"rendered":"

Dnes tu pro v\u00e1s m\u00e1m nyn\u00ed ji\u017e t\u0159et\u00ed pokra\u010dov\u00e1n\u00ed m\u00e9ho putov\u00e1n\u00ed za m\u00e9n\u011b zn\u00e1m\u00fdmi galaxiemi z NGC a IC katalogu.<\/p>\n

Po\u010d\u00e1tek l\u00e9ta nen\u00ed z d\u016fvodu velmi kr\u00e1tk\u00fdch noc\u00ed okolo letn\u00edho slunovratu pro pozorov\u00e1n\u00ed hlubok\u00e9ho vesm\u00edru a zejm\u00e9na slab\u00fdch galaxi\u00ed v \u010cR p\u0159\u00edli\u0161 p\u0159\u00edzniv\u00fd. Proto jsem doufal, \u017ee b\u011bhem m\u00e9 cesty do rovn\u00edkov\u00e9 oblasti v Tichomo\u0159\u00ed na Galap\u00e1gy<\/a> zachyt\u00edm pomoc\u00ed \u201eTrpasl\u00edka\u201c (chytr\u00e9ho dalekohledu Dwarf 3) n\u011bjak\u00e9 zaj\u00edmav\u00e9 objekty ji\u017en\u00ed oblohy, kter\u00e9 nejsou z \u010cR dostupn\u00e9. Leto\u0161n\u00ed velmi siln\u00e9 El Ni\u00f1o v\u0161ak na Galap\u00e1gy p\u0159ineslo mnohem v\u00edce obla\u010dnosti, ne\u017e b\u00fdv\u00e1 v tuto ro\u010dn\u00ed dobu obvykl\u00e9. Z focen\u00ed tak bohu\u017eel nic nebylo, a proto jsem si na lov dal\u0161\u00edch galaktick\u00fdch skvost\u016f musel po\u010dkat na n\u00e1vrat zp\u011bt do \u010cesk\u00e9 republiky a dal\u0161\u00ed focen\u00ed zah\u00e1jit a\u017e v pr\u016fb\u011bhu \u010dervence.<\/p>\n

<\/p>\n

\n

<\/p>\n

NGC 6822 (Caldwell 57) \u2013 Barnard’s Galaxy<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 8. 7. 2026
\n\"NGC<\/a><\/p>\n

NGC 6822 je nepravideln\u00e1 trpasli\u010d\u00ed galaxie ve St\u0159elci, zn\u00e1m\u00e1 t\u00e9\u017e jako Barnardova galaxie, pat\u0159\u00edc\u00ed do M\u00edstn\u00ed skupiny galaxi\u00ed. V na\u0161ich zem\u011bpisn\u00fdch \u0161\u00ed\u0159k\u00e1ch vych\u00e1z\u00ed jen pom\u011brn\u011b n\u00edzko nad ji\u017en\u00ed obzor, co\u017e z n\u00ed d\u011bl\u00e1 fotograficky n\u00e1ro\u010dn\u011bj\u0161\u00ed c\u00edl. I p\u0159es n\u00edzkou v\u00fd\u0161ku se v\u0161ak poda\u0159ilo zachytit jej\u00ed strukturu i mlhoviny, ve kter\u00fdch prob\u00edh\u00e1 p\u0159ekotn\u00e1 tvorba nov\u00fdch hv\u011bzd. Galaxie je vzd\u00e1len\u00e1 asi 1,6 milionu sv\u011bteln\u00fdch let, objevil ji Edward Emerson Barnard.<\/p>\n

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<\/p>\n

NGC 7479 (Caldwell 44) \u2013 Superman Galaxy<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 25. 7. a 8. 8. 2026
\n\"NGC<\/a><\/p>\n

NGC 7479 je v\u00fdrazn\u00e1 spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou v souhv\u011bzd\u00ed Pegase. Sv\u016fj neofici\u00e1ln\u00ed n\u00e1zev \u201eSuperman Galaxy\u201c z\u00edskala d\u00edky asymetrick\u00fdm, jasn\u00fdm spir\u00e1ln\u00edm ramen\u016fm, je\u017e p\u0159i pohledu v teleskopu p\u0159ipom\u00ednaj\u00ed ikonick\u00e9 logo Supermana. Je pozoruhodn\u00e1 tak\u00e9 t\u00edm, \u017ee jej\u00ed ramena v radiov\u00e9m spektru rotuj\u00ed v opa\u010dn\u00e9m sm\u011bru ne\u017e hv\u011bzdy v disku, co\u017e nazna\u010duje ned\u00e1vnou galaktickou f\u00fazi. Galaxie je vzd\u00e1len\u00e1 cca 105 milionu sv\u011bteln\u00fdch let, objevil ji William Herschel.<\/p>\n

\n

<\/p>\n

NGC 7814 (Caldwell 43) \u2013 Little Sombrero<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 22. 8. 2026
\n\"NGC<\/a><\/p>\n

Tato spir\u00e1ln\u00ed galaxie v Pegasovi b\u00fdv\u00e1 p\u0159ezd\u00edv\u00e1na jako Mal\u00e9 Sombrero, proto\u017ee se n\u00e1m prom\u00edt\u00e1 p\u0159\u00edmo ze strany (edge-on). V\u00fdrazn\u00fd potem\u0148uj\u00edc\u00ed prachov\u00fd p\u00e1s prot\u00edn\u00e1 centr\u00e1ln\u00ed galaktick\u00e9 j\u00e1dro a vytv\u00e1\u0159\u00ed tak pozoruhodnou analogii ke zn\u00e1m\u00e9 galaxii M104 v Pann\u011b. Je vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 40 milion\u016f sv\u011bteln\u00fdch let, objevil ji rovn\u011b\u017e William Herschel.<\/p>\n

\n

<\/p>\n

IC 1613 (Caldwell 51)<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 22. 8. 2026
\n\"IC<\/a><\/p>\n

Toto je nen\u00e1padn\u00e1, ale astronomicky nesm\u00edrn\u011b d\u016fle\u017eit\u00e1 nepravideln\u00e1 trpasli\u010d\u00ed galaxie v souhv\u011bzd\u00ed Velryby. Nach\u00e1z\u00ed se v M\u00edstn\u00ed skupin\u011b galaxi\u00ed a obsahuje velmi m\u00e1lo mezihv\u011bzdn\u00e9ho prachu, co\u017e z n\u00ed d\u011bl\u00e1 ide\u00e1ln\u00ed kalibra\u010dn\u00ed standard pro m\u011b\u0159en\u00ed vesm\u00edrn\u00fdch vzd\u00e1lenost\u00ed pomoc\u00ed prom\u011bnn\u00fdch hv\u011bzd Cepheid a RR Lyrae. Je zhruba 2,3 milionu sv\u011bteln\u00fdch let daleko a objevil ji pro zm\u011bnu Max Wolf.<\/p>\n

\n

<\/p>\n

NGC 7640<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 23. 8. 2026
\n\"NGC<\/a><\/p>\n

P\u011bkn\u00e1 spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou v souhv\u011bzd\u00ed Je\u0161t\u011brky (Lacerta). Z na\u0161eho pohledu je zna\u010dn\u011b naklon\u011bn\u00e1, d\u00edky \u010demu\u017e je jej\u00ed p\u0159\u00ed\u010dka pom\u011brn\u011b \u00fazk\u00e1 a ramena se jev\u00ed jako propleten\u00e9 prachov\u00e9 p\u00e1sy protkan\u00e9 slab\u00fdmi H-II oblastmi. Galaxie je vzd\u00e1len\u00e1 okolo 30 milion\u016f sv\u011bteln\u00fdch let, objevil ji op\u011bt William Herschel.<\/p>\n

\n

<\/p>\n

NGC 147 (Caldwell 17) a NGC 185 (Caldwell 18)<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 29. 8. 2026
\n\"NGC<\/a><\/p>\n

Dvojice trpasli\u010d\u00edch eliptick\u00fdch (resp. sf\u00e9roidn\u00edch) galaxi\u00ed v Kasiopeji. Ob\u011b jsou ob\u011b\u017en\u00fdmi pr\u016fvodci Velk\u00e9 galaxie v Andromed\u011b (M31). Zat\u00edmco NGC 185 obsahuje mal\u00e9 mno\u017estv\u00ed prachu a plynu a vykazuje stopy ned\u00e1vn\u00e9 tvorby hv\u011bzd, sousedn\u00ed NGC 147 je tvo\u0159ena p\u0159ev\u00e1\u017en\u011b star\u00fdmi hv\u011bzdami bez mezihv\u011bzdn\u00e9 hmoty.
\nNGC 147 je vzd\u00e1len\u00e1 asi 2,5 milionu sv\u011bteln\u00fdch let a NGC 185 je daleko p\u0159ibli\u017en\u011b 2,6 milionu sv\u011bteln\u00fdch let, objevil je ob\u011b William Herschel.<\/p>\n

\n

<\/p>\n

NGC 7217<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 31. 8. 2026
\n\"NGC<\/a><\/p>\n

Izolovan\u00e1 spir\u00e1ln\u00ed galaxie v Pegasovi charakteristick\u00e1 sv\u00fdmi soust\u0159edn\u00fdmi kruhov\u00fdmi prstenci hv\u011bzd a prachu. Na rozd\u00edl od v\u011bt\u0161iny spir\u00e1ln\u00edch galaxi\u00ed m\u00e1 velmi m\u00e1lo plynu a v\u00fdznamn\u00e1 \u010d\u00e1st jej\u00edch hv\u011bzd rotuje v opa\u010dn\u00e9m sm\u011bru, ne\u017e je obvykl\u00e9, co\u017e sv\u011bd\u010d\u00ed o jej\u00ed pohnut\u00e9 minulosti spojen\u00e9 s pohlcen\u00edm men\u0161\u00edho galaktick\u00e9ho souseda. Galaxie je vzd\u00e1len\u00e1 okolo 50 milion\u016f sv\u011bteln\u00fdch let, objevil ji zase William Herschel.<\/p>\n

\n

<\/p>\n

NGC 7741<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 1. 9. 2026
\n\"NGC<\/a><\/p>\n

Typick\u00e1 spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou le\u017e\u00edc\u00ed v Pegasovi. M\u00e1 velmi jasnou centr\u00e1ln\u00ed p\u0159\u00ed\u010dku, z n\u00ed\u017e se odv\u00edjej\u00ed kropenat\u00e1, nepravideln\u00e1 spir\u00e1ln\u00ed ramena pln\u00e1 mlad\u00fdch modr\u00fdch hv\u011bzdokup a p\u0159ekotn\u00fdch H-II region\u016f. Tento objekt je vzd\u00e1len\u00fd cca 40 milion\u016f sv\u011bteln\u00fdch let a objevil ho William Herschel.<\/p>\n

\n

<\/p>\n

NGC 7332 a NGC 7339<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 6. 9. 2026
\n\"NGC<\/a><\/p>\n

Vizu\u00e1ln\u011b atraktivn\u00ed fyzick\u00e1 dvojice galaxi\u00ed v Pegasovi le\u017e\u00edc\u00edch t\u00e9m\u011b\u0159 pravouhle v\u016f\u010di sob\u011b. NGC 7332 je jasn\u011bj\u0161\u00ed \u010do\u010dkov\u00e1 galaxie s netypick\u00fdm tvarem j\u00e1dra, zat\u00edmco NGC 7339 je slab\u0161\u00ed spir\u00e1ln\u00ed galaxie viditeln\u00e1 z boku. Galaxie jsou vzd\u00e1len\u00e9 n\u011bjak\u00fdch 67 milion\u016f sv\u011bteln\u00fdch let, objevil je kdo jin\u00fd ne\u017e William Herschel.<\/p>\n

\n

<\/p>\n

NGC 247 (Caldwell 62)<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 7. 9. 2026
\n\"NGC<\/a><\/p>\n

Spir\u00e1ln\u00ed galaxie v souhv\u011bzd\u00ed Velryby pat\u0159\u00ed do bl\u00edzk\u00e9 skupiny galaxi\u00ed v Socha\u0159i (Sculptor Group). Je zn\u00e1m\u00e1 svou neobvyklou asymetri\u00ed \u2013 na jedn\u00e9 stran\u011b disku se nach\u00e1z\u00ed rozs\u00e1hl\u00e1 \u201ed\u00edra\u201c t\u00e9m\u011b\u0159 bez hv\u011bzd a prachu, pravd\u011bpodobn\u011b v\u00fdsledek prav\u011bk\u00e9 sr\u00e1\u017eky s jinou trpasli\u010d\u00ed galaxi\u00ed. Galaxie je od n\u00e1s 67 milion\u016f sv\u011bteln\u00fdch let a objevil ji William Herschel.<\/p>\n

\n

<\/p>\n

IC 10<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed: 8. 9. 2026<\/strong>
\n\"IC<\/a><\/p>\n

Jedin\u00e1 zn\u00e1m\u00e1 \u201estarburst\u201c galaxie v M\u00edstn\u00ed skupin\u011b galaxi\u00ed, situovan\u00e1 v Kasiopeji. Proch\u00e1z\u00ed extr\u00e9mn\u011b p\u0159ekotnou tvorbou nov\u00fdch hv\u011bzd. Jej\u00ed pozorov\u00e1n\u00ed i fotografov\u00e1n\u00ed je zkomplikov\u00e1no t\u00edm, \u017ee le\u017e\u00ed bl\u00edzko roviny Ml\u00e9\u010dn\u00e9 dr\u00e1hy a jej\u00ed sv\u011btlo je zna\u010dn\u011b zeslabov\u00e1no mezihv\u011bzdn\u00fdm prachem. Galaxie je vzd\u00e1len\u00e1 cca 2,2 milionu sv\u011bteln\u00fdch let, objevil ji Lewis Swift v roce 1887.<\/p>\n

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<\/p>\n

NGC 1097 (Caldwell 67)<\/h2>\n

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

Dal\u0161\u00ed v\u00fdrazn\u00e1 spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou le\u017e\u00edc\u00ed v souhv\u011bzd\u00ed Pece (Fornax). Nach\u00e1z\u00ed se ve vzd\u00e1lenosti p\u0159ibli\u017en\u011b 45 milion\u016f sv\u011bteln\u00fdch let a je zn\u00e1m\u00e1 sv\u00fdm aktivn\u00edm galaktick\u00fdm j\u00e1drem a komplexn\u00ed strukturou ram\u00ednek spojenou s pohlcov\u00e1n\u00edm men\u0161\u00edch satelitn\u00edch galaxi\u00ed.
\nObjevena byla jako u\u017e tradi\u010dn\u011b Williamem Herschelem.<\/p>\n

Jej\u00edm zachycen\u00edm jsem \u00fasp\u011b\u0161n\u011b zkompletoval m\u016fj katalog Caldwellov\u00fdch objekt\u016f<\/a> dostupn\u00fdch z \u00fazem\u00ed \u010cesk\u00e9 republiky. Zb\u00fdvaj\u00edc\u00ed objekty z tohoto katalogu se toti\u017e nach\u00e1zej\u00ed v\u00fdhradn\u011b na ji\u017en\u00ed obloze, p\u0159\u00edpadn\u011b u n\u00e1s nevystupuj\u00ed v\u00fd\u0161e ne\u017e 5 \u00b0 nad obzor.<\/p>\n

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<\/p>\n

NGC 7331 (Caldwell 30) \u2013 Supernovy SN 2025rbs a SN 2026aaiv<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 11. 9. 2026, 23. 7. 2025 a 27.\u201329. 8. 2024
\n\"NGC<\/a><\/p>\n

Galaxie NGC 7331 v Pegasovi je sama o sob\u011b n\u00e1dhern\u00fdm c\u00edlem, av\u0161ak v posledn\u00edch dvou letech se stala neuv\u011b\u0159iteln\u011b dynamick\u00fdm m\u00edstem. B\u011bhem jedin\u00e9ho roku a \u010dtvrt se v n\u00ed poda\u0159ilo zachytit hned dv\u011b vzplanut\u00ed supernov: SN 2025rbs<\/strong> a SN 2026aaiv<\/strong>. Na animaci m\u016f\u017eete porovnat m\u00edsta vzplanut\u00ed obou t\u011bchto masivn\u00edch hv\u011bzdn\u00fdch exploz\u00ed a porovnat s refere\u010dn\u00edm sn\u00edmkem z roku 2024. Galaxie je vzd\u00e1len\u00e1 zhruba 45 milion\u016f sv\u011bteln\u00fdch let, objevil ji William Herschel.<\/p>\n

\n

<\/p>\n

NGC 7317, 7318, 7319, 7320 \u2013 Stephan’s Quintet (Arp 319)<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 5. a 14.\u201319. 8. 2025, 3. a 4. 8. 2022<\/p>\n

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

Kdy\u017e jsme si na p\u0159edchoz\u00edm sn\u00edmku uk\u00e1zali supernovy v NGC 7331, nesm\u00edme opomenout tuto ikonickou skupinu galaxi\u00ed v Pegasovi. A\u010dkoliv jsem ji fotografoval ji\u017e v p\u0159edchoz\u00edch letech, v p\u0159ehledu t\u011bchto letn\u00edch skvost\u016f jednodu\u0161e nesm\u00ed chyb\u011bt. \u010cty\u0159i z t\u011bchto galaxi\u00ed spolu sv\u00e1d\u011bj\u00ed t\u011bsn\u00fd gravita\u010dn\u00ed tanec vytv\u00e1\u0159ej\u00edc\u00ed dlouh\u00e9 slapov\u00e9 chvosty, zat\u00edmco p\u00e1t\u00e1 (NGC 7320) se do skupiny pouze opticky prom\u00edt\u00e1 z pop\u0159ed\u00ed. Tuto slavnou skupinu objevil \u00c9douard Stephan v roce 1877. Fyzicky sv\u00e1zan\u00e9 galaxie od n\u00e1s le\u017e\u00ed ve vzd\u00e1lenosti p\u0159ibli\u017en\u011b 210 a\u017e 340 milion\u016f sv\u011bteln\u00fdch let, s v\u00fdjimkou NGC 7320, kter\u00e1 je vzd\u00e1len\u00e1 pouze 39 milion\u016f sv\u011bteln\u00fdch let.<\/p>\n

\n

<\/p>\n

NGC 925<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 14. 9. 2026
\n\"NGC<\/a><\/p>\n

Spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou le\u017e\u00edc\u00ed v souhv\u011bzd\u00ed Troj\u00faheln\u00edku. M\u00e1 pom\u011brn\u011b jasn\u00e9 j\u00e1dro, ale slab\u0161\u00ed, nepravideln\u00e1 spir\u00e1ln\u00ed ramena pln\u00e1 H-II oblast\u00ed, co\u017e zna\u010d\u00ed prob\u00edhaj\u00edc\u00ed formov\u00e1n\u00ed hv\u011bzd. Galaxie je vzd\u00e1len\u00e1 asi 28 milionu sv\u011bteln\u00fdch let, objevil ji William Herschel<\/p>\n

\n

<\/p>\n

NGC 2146 \u2013 Dusty Hand Galaxy<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 15. 9. 2026
\n\"NGC<\/a><\/p>\n

Nepochybn\u011b fascinuj\u00edc\u00ed spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou v souhv\u011bzd\u00ed \u017dirafy (Camelopardalis). Je zn\u00e1m\u00e1 sv\u00fdm v\u00fdrazn\u011b deformovan\u00fdm (\u201eohnut\u00fdm\u201c) tvarem a hust\u00fdmi prachov\u00fdmi p\u00e1sy prot\u00ednaj\u00edc\u00edmi jej\u00ed j\u00e1dro, co\u017e je d\u016fsledek gravita\u010dn\u00edho p\u0159ibl\u00ed\u017een\u00ed se sousedn\u00ed galaxi\u00ed NGC 2146A v minulosti. Pat\u0159\u00ed mezi tzv. \u201estarburst\u201c galaxie s velmi intenz\u00edvn\u00ed tvorbou nov\u00fdch hv\u011bzd. Galaxie je vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 70 milion\u016f sv\u011bteln\u00fdch let a objevitelem je Friedrich August Theodor Winnecke.<\/p>\n

\n

<\/p>\n

NGC 2146A<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 17. 9. 2026
\n\"NGC<\/a><\/p>\n

Je spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou v souhv\u011bzd\u00ed \u017dirafy. Na obloze se sice prom\u00edt\u00e1 jen kousek od v\u00fdrazn\u011bj\u0161\u00ed NGC 2146, ale ve skute\u010dnosti le\u017e\u00ed je\u0161t\u011b o n\u011bkolik milion\u016f sv\u011bteln\u00fdch let d\u00e1le v pozad\u00ed. Jde o \u00fahlov\u011b men\u0161\u00ed a plo\u0161n\u011b slab\u0161\u00ed objekt, spir\u00e1ln\u00ed ramena odhaluj\u00ed jemnou strukturu a prob\u00edhaj\u00edc\u00ed formov\u00e1n\u00ed hv\u011bzd.
\nGalaxie je vzd\u00e1len\u00e1 okolo 80 milion\u016f sv\u011bteln\u00fdch let, objevil ji Edward Swift.<\/p>\n

\n

<\/p>\n

NGC 1003<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 18. 9. 2026
\n\"NGC<\/a><\/p>\n

P\u011bkn\u00e1 spir\u00e1ln\u00ed galaxie v souhv\u011bzd\u00ed Persea, nahl\u00ed\u017een\u00e1 pod zna\u010dn\u00fdm \u00fahlem. Vyzna\u010duje se rozs\u00e1hl\u00fdm diskem s ni\u017e\u0161\u00ed plo\u0161nou jasnost\u00ed, asymetrick\u00fdmi prachov\u00fdmi p\u00e1sy a uzl\u00edky mlad\u00fdch hv\u011bzdokup, kter\u00e9 sv\u011bd\u010d\u00ed o prob\u00edhaj\u00edc\u00ed tvorb\u011b hv\u011bzd. Pat\u0159\u00ed do bl\u00edzko le\u017e\u00edc\u00ed skupiny galaxi\u00ed okolo NGC 1023. Galaxii objevil William Herschel a od Zem\u011b je vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 34 milion\u016f sv\u011bteln\u00fdch let.<\/p>\n

\n

<\/p>\n

ARP 99 (NGC 7547, NGC 7549, NGC7550)<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 19. 9. 2026
\n\"NGC<\/a><\/p>\n

Arp 99 p\u0159edstavuje v\u00fdraznou trojici vz\u00e1jemn\u011b se ovliv\u0148uj\u00edc\u00edch galaxi\u00ed v souhv\u011bzd\u00ed Pegase, vzd\u00e1lenou od n\u00e1s p\u0159ibli\u017en\u011b 210 a\u017e 220 milion\u016f sv\u011bteln\u00fdch let. Dominantn\u00edm \u010dlenem tohoto syst\u00e9mu je \u010deln\u011b nato\u010den\u00e1 lentikul\u00e1rn\u00ed galaxie NGC 7550 (jasnost ~12,2 mag), kterou v roce 1784 objevil William Herschel. V t\u011bsn\u00e9 bl\u00edzkosti se nach\u00e1z\u00ed deformovan\u00e1 spir\u00e1ln\u00ed galaxie s p\u0159\u00ed\u010dkou NGC 7549 s v\u00fdrazn\u011b rozta\u017een\u00fdmi rameny a slapov\u00fdmi proudy, a rovn\u011b\u017e galaxie NGC 7547. Halton Arp za\u0159adil tento syst\u00e9m do sv\u00e9ho katalogu zvl\u00e1\u0161tn\u00edch galaxi\u00ed pod \u010d\u00edslem 99 v kategorii spir\u00e1ln\u00edch galaxi\u00ed s eliptick\u00fdm pr\u016fvodcem. Skupina je z\u00e1rove\u0148 sou\u010d\u00e1st\u00ed kompaktn\u00ed skupiny Hickson 93 (HCG 93).<\/p>\n

\n

<\/p>\n

M31 \u2013 Velk\u00e1 galaxie v Andromed\u011b<\/h2>\n

Datum sn\u00edm\u00e1n\u00ed:<\/strong> 28. 8. 2022
\n\"M31\"<\/a><\/p>\n

Vl\u00e1du nyn\u00ed ji\u017e p\u0159eb\u00edr\u00e1 podzimn\u00ed obloha, kde je absolutn\u00edm kr\u00e1lem n\u00e1\u0161 nejbli\u017e\u0161\u00ed velk\u00fd galaktick\u00fd soused \u2013 Velk\u00e1 mlhovina (galaxie) v Andromed\u011b (M31). Tato galaxie je vzd\u00e1len\u00e1 cca 2,5 milionu sv\u011bteln\u00fdch let a poprv\u00e9 ji popsal persk\u00fd astronom Abd ar-Rahm\u00e1n as-S\u00faf\u00ed ji\u017e v roce 964.<\/p>\n

Douf\u00e1m, \u017ee se v\u00e1m dne\u0161n\u00ed d\u00edl m\u00e9ho putov\u00e1n\u00ed l\u00edbil. Pokud v\u00e1m unikly p\u0159edchoz\u00ed \u010d\u00e1sti, m\u016f\u017eete nahl\u00e9dnout do I. d\u00edlu (Zimn\u00ed putov\u00e1n\u00ed za Galaxiemi)<\/a> a II. d\u00edlu (Putov\u00e1n\u00ed za galaxiemi II \u2013 Jaro 2026)<\/a>.<\/p>\n

Na p\u0159\u00ed\u0161t\u00ed pokra\u010dov\u00e1n\u00ed tohoto seri\u00e1lu, pokud podzimn\u00ed sychrav\u00e9 po\u010das\u00ed dovol\u00ed, se m\u016f\u017eete t\u011b\u0161it okolo V\u00e1noc. Krom\u011b dal\u0161\u00edch zaj\u00edmav\u00fdch galaxi\u00ed z NGC, IC nebo Arp katalogu se zam\u011b\u0159\u00edm tak\u00e9 na Saturn. Jeho sez\u00f3na pr\u00e1v\u011b za\u010d\u00edn\u00e1 a po cca deseti letech, kdy se plazil n\u00edzko nad obzorem ve St\u0159elci a Vodn\u00e1\u0159i, se nyn\u00ed p\u0159esunul do Velryby a kulminuje pro fotografov\u00e1n\u00ed v mnohem zaj\u00edmav\u011bj\u0161\u00ed v\u00fd\u0161ce, tj. v\u00edce ne\u017e 40\u00b0 nad obzorem.<\/p>\n

Jasnou oblohu v\u0161em!<\/p>\n

Vyfotil a zpracoval Roman<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"

Dnes tu pro v\u00e1s m\u00e1m nyn\u00ed ji\u017e t\u0159et\u00ed pokra\u010dov\u00e1n\u00ed m\u00e9ho putov\u00e1n\u00ed za m\u00e9n\u011b zn\u00e1m\u00fdmi galaxiemi z NGC a IC katalogu. Po\u010d\u00e1tek l\u00e9ta nen\u00ed z d\u016fvodu velmi kr\u00e1tk\u00fdch noc\u00ed okolo letn\u00edho slunovratu pro pozorov\u00e1n\u00ed hlubok\u00e9ho vesm\u00edru a zejm\u00e9na slab\u00fdch galaxi\u00ed v \u010cR p\u0159\u00edli\u0161 p\u0159\u00edzniv\u00fd. Proto jsem doufal, \u017ee b\u011bhem m\u00e9 cesty do rovn\u00edkov\u00e9 oblasti v Tichomo\u0159\u00ed […]<\/p>\n","protected":false},"author":1,"featured_media":485,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7,9],"tags":[],"class_list":["post-481","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-astronomie","category-deepsky"],"_links":{"self":[{"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts\/481","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=481"}],"version-history":[{"count":4,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts\/481\/revisions"}],"predecessor-version":[{"id":486,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts\/481\/revisions\/486"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/media\/485"}],"wp:attachment":[{"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=481"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=481"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=481"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}