{"id":460,"date":"2026-03-22T15:23:57","date_gmt":"2026-03-22T14:23:57","guid":{"rendered":"https:\/\/hujer.net\/?p=460"},"modified":"2026-03-22T16:05:02","modified_gmt":"2026-03-22T15:05:02","slug":"zimni-putovani-za-galaxiemi","status":"publish","type":"post","link":"https:\/\/hujer.net\/?p=460","title":{"rendered":"Zimn\u00ed putov\u00e1n\u00ed za Galaxiemi"},"content":{"rendered":"

Zimn\u00ed putov\u00e1n\u00ed za Galaxiemi z Caldwell a Herschel katalogu<\/em><\/p>\n

P\u0159esto\u017ee hlavn\u00ed sez\u00f3na galaxi\u00ed vrchol\u00ed na ja\u0159e, i zimn\u00ed m\u011bs\u00edce nab\u00edzej\u00ed \u0159adu pozoruhodn\u00fdch c\u00edl\u016f. B\u011bhem zimy 2025\/2026 jsem se zam\u011b\u0159il na fotografov\u00e1n\u00ed galaxi\u00ed z katalog\u016f Caldwell<\/strong> a Herschel<\/strong>, kter\u00e9 jsou dob\u0159e dostupn\u00e9 ze severn\u00ed polokoule a umo\u017e\u0148uj\u00ed mi systematick\u00e9 dopl\u0148ov\u00e1n\u00ed m\u00e9 sb\u00edrky.<\/p>\n

\n

NGC 2403 \u2013 Caldwell 7<\/h3>\n

11.\u201312. 12. 2025<\/strong><\/p>\n

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

Spir\u00e1ln\u00ed galaxie v souhv\u011bzd\u00ed \u017dirafy (Camelopardalis)<\/strong>, vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 9,7 milionu sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena byla Williamem Herschelem v roce 1788<\/strong>.<\/p>\n

\n

NGC 2403 pat\u0159\u00ed mezi nejvd\u011b\u010dn\u011bj\u0161\u00ed spir\u00e1ln\u00ed galaxie severn\u00ed oblohy a pr\u00e1vem je pova\u017eov\u00e1na za jeden z klenot\u016f Caldwellova katalogu. Sv\u00fdm vzhledem \u010dasto p\u0159ipom\u00edn\u00e1 galaxii M33, i kdy\u017e p\u016fsob\u00ed o n\u011bco kompaktn\u011bj\u0161\u00edm dojmem. Na sn\u00edmc\u00edch vynikaj\u00ed jemn\u011b vinut\u00e1 spir\u00e1ln\u00ed ramena poset\u00e1 mno\u017estv\u00edm oblast\u00ed tvorby hv\u011bzd, kter\u00e9 galaxii dod\u00e1vaj\u00ed velmi \u017eiv\u00fd a p\u0159irozen\u00fd vzhled.<\/p>\n<\/div>\n

\n

IC 342 \u2013 Caldwell 5 (Hidden Galaxy)<\/h3>\n

15. 12. 2025<\/strong><\/p>\n

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

Velk\u00e1 spir\u00e1ln\u00ed galaxie v souhv\u011bzd\u00ed \u017dirafy<\/strong>, vzd\u00e1len\u00e1 asi 10\u201311 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Frederickem Denningem v roce 1892<\/strong>.<\/p>\n

\n

IC 342 je jednou z nejzaj\u00edmav\u011bj\u0161\u00edch, ale z\u00e1rove\u0148 nejn\u00e1ro\u010dn\u011bj\u0161\u00edch galaxi\u00ed severn\u00ed oblohy. P\u0159esto\u017ee pat\u0159\u00ed mezi relativn\u011b bl\u00edzk\u00e9 a rozm\u011brov\u011b velk\u00e9 spir\u00e1ln\u00ed galaxie, jej\u00ed skute\u010dn\u00e1 kr\u00e1sa je skryt\u00e1 za z\u00e1vojem mezihv\u011bzdn\u00e9ho prachu Ml\u00e9\u010dn\u00e9 dr\u00e1hy. Pr\u00e1v\u011b proto si vyslou\u017eila p\u0159ezd\u00edvku Hidden Galaxy<\/em> \u2013 Skryt\u00e1 galaxie.<\/p>\n<\/div>\n

NGC 4236 \u2013 Caldwell 3<\/h3>\n

18. 12. 2025<\/strong><\/p>\n

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

Prot\u00e1hl\u00e1 galaxie v souhv\u011bzd\u00ed Draka (Draco)<\/strong>, vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 11\u201314 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem roku 1793<\/strong>.<\/p>\n

NGC 4236 je prot\u00e1hl\u00e1 galaxie, kter\u00e1 na prvn\u00ed pohled p\u016fsob\u00ed velmi nen\u00e1padn\u011b, ale p\u0159i del\u0161\u00edm pohledu odhal\u00ed sv\u016fj osobit\u00fd charakter. Jej\u00ed tvar je v\u00fdrazn\u011b podlouhl\u00fd a p\u0159ipom\u00edn\u00e1 tenk\u00fd, lehce rozpt\u00fdlen\u00fd obl\u00e1\u010dek sv\u011btla, bez dominantn\u00edho j\u00e1dra. Pr\u00e1v\u011b tato jemnost a n\u00edzk\u00fd kontrast z n\u00ed d\u011blaj\u00ed zaj\u00edmav\u00fd objekt, kter\u00fd se v\u00fdrazn\u011b li\u0161\u00ed od klasick\u00fdch \u201eu\u010debnicov\u00fdch\u201c spir\u00e1ln\u00edch galaxi\u00ed. NGC 4236 p\u016fsob\u00ed klidn\u00fdm a p\u0159irozen\u00fdm dojmem, jako by \u0161lo o galaxii na pomez\u00ed mezi pravidelnou strukturou a nepravideln\u00fdm syst\u00e9mem, co\u017e j\u00ed dod\u00e1v\u00e1 zvl\u00e1\u0161tn\u00ed estetiku a nen\u00e1padn\u00e9 kouzlo.<\/div>\n
\n

NGC 1275 \u2013 Caldwell 24 (Perseus A)<\/h3>\n

23. 12. 2025<\/strong><\/p>\n

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

Aktivn\u00ed galaxie v souhv\u011bzd\u00ed Persea<\/strong>, le\u017e\u00edc\u00ed ve vzd\u00e1lenosti p\u0159ibli\u017en\u011b 225 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1786<\/strong>.<\/p>\n

NGC 1275 je mimo\u0159\u00e1dn\u011b v\u00fdrazn\u00e1 galaxie, kter\u00e1 tvo\u0159\u00ed samotn\u00e9 srdce kupy galaxi\u00ed v souhv\u011bzd\u00ed Persea. Na rozd\u00edl od klidn\u00fdch spir\u00e1ln\u00edch galaxi\u00ed p\u016fsob\u00ed tento objekt velmi dynamicky a neklidn\u011b \u2013 jej\u00ed j\u00e1dro je extr\u00e9mn\u011b aktivn\u00ed a cel\u00e9 okol\u00ed je protk\u00e1no jemn\u00fdmi filamenty plynu, kter\u00e9 d\u00e1vaj\u00ed galaxii a\u017e dramatick\u00fd vzhled. NGC 1275 nep\u016fsob\u00ed jako izolovan\u00fd ostrov hv\u011bzd, ale sp\u00ed\u0161e jako gravita\u010dn\u00ed centrum rozs\u00e1hl\u00e9ho syst\u00e9mu, kde se setk\u00e1vaj\u00ed a ovliv\u0148uj\u00ed des\u00edtky dal\u0161\u00edch galaxi\u00ed.<\/div>\n
\n

NGC 891 \u2013 Caldwell 23 (Silver Galaxy)<\/h3>\n

24. 12. 2025<\/strong><\/p>\n

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

Ikonick\u00e1 galaxie viditeln\u00e1 zboku v souhv\u011bzd\u00ed Andromedy<\/strong>, vzd\u00e1len\u00e1 asi 27\u201330 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem roku 1784<\/strong>.<\/p>\n

NGC 891 pat\u0159\u00ed mezi nejp\u016fsobiv\u011bj\u0161\u00ed galaxie severn\u00ed oblohy a je \u010dasto pova\u017eov\u00e1na za jeden z nejlep\u0161\u00edch p\u0159\u00edklad\u016f pohledu na spir\u00e1ln\u00ed galaxii zboku. Jej\u00ed dlouh\u00fd, \u00fazk\u00fd disk je v\u00fdrazn\u011b protknut tmav\u00fdm prachov\u00fdm p\u00e1sem, kter\u00fd d\u00e1v\u00e1 galaxii dramatick\u00fd a velmi plastick\u00fd vzhled. Pr\u00e1v\u011b tento pruh p\u0159ipom\u00edn\u00e1 strukturu na\u0161\u00ed vlastn\u00ed Ml\u00e9\u010dn\u00e9 dr\u00e1hy, pokud bychom ji pozorovali z vn\u011bj\u0161\u00ed perspektivy.<\/div>\n
\n

NGC 4244 \u2013 Caldwell 26 (Silver Needle Galaxy)<\/h3>\n

25. 12. 2025<\/strong><\/p>\n

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

Velmi tenk\u00e1 galaxie v souhv\u011bzd\u00ed Honic\u00edch ps\u016f (Canes Venatici)<\/strong>, vzd\u00e1len\u00e1 asi 14 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1787<\/strong>.<\/p>\n

NGC 4244 je velmi tenk\u00e1, prot\u00e1hl\u00e1 galaxie. Jej\u00ed \u00fazk\u00fd disk p\u0159ipom\u00edn\u00e1 jemnou sv\u011btelnou jehlu, d\u00edky \u010demu\u017e si vyslou\u017eila p\u0159ezd\u00edvku Silver Needle Galaxy<\/em>. Na rozd\u00edl od v\u00fdrazn\u011bj\u0161\u00edch podobn\u011b k n\u00e1m nato\u010den\u00fdm galaxi\u00edm zde chyb\u00ed dominantn\u00ed prachov\u00fd p\u00e1s a celkov\u00fd dojem je mnohem subtiln\u011bj\u0161\u00ed a klidn\u011bj\u0161\u00ed.<\/div>\n
\n

NGC 2775 \u2013 Caldwell 48<\/h3>\n

26. 12. 2025<\/strong>
\n<\/a><\/p>\n

Spir\u00e1ln\u00ed galaxie v souhv\u011bzd\u00ed Raka (Cancer)<\/strong>, vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 67 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem roku 1783<\/strong>.<\/p>\n

NGC 2775 p\u016fsob\u00ed velmi klidn\u00fdm a vyv\u00e1\u017een\u00fdm dojmem, kter\u00fd ji odli\u0161uje od v\u00fdrazn\u011bj\u0161\u00edch a kontrastn\u011bj\u0161\u00edch spir\u00e1ln\u00edch galaxi\u00ed. Dominantn\u00ed centr\u00e1ln\u00ed oblast p\u0159ech\u00e1z\u00ed do jemn\u011b nazna\u010den\u00fdch spir\u00e1ln\u00edch ramen, kter\u00e1 nejsou na prvn\u00ed pohled agresivn\u00ed, ale sp\u00ed\u0161e uhlazen\u00e1 a decentn\u00ed. Celkov\u011b galaxie p\u0159ipom\u00edn\u00e1 star\u0161\u00ed, vyzr\u00e1l\u00fd syst\u00e9m, kde nep\u0159eva\u017euje dramatick\u00e1 struktura, ale harmonie a symetrie.<\/div>\n
\n

NGC 3115 \u2013 Caldwell 53 (Spindle Galaxy)<\/h3>\n

15. 2. 2026<\/strong>
\n<\/a><\/p>\n

\u010co\u010dkovit\u00e1 galaxie v souhv\u011bzd\u00ed Sextantu<\/strong>, vzd\u00e1len\u00e1 asi 32 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1787<\/strong>.<\/p>\n

\n

NGC 3115 p\u016fsob\u00ed na prvn\u00ed pohled velmi stroze a elegantn\u011b, t\u00e9m\u011b\u0159 geometricky. Jej\u00ed v\u00fdrazn\u011b prot\u00e1hl\u00fd tvar p\u0159ipom\u00edn\u00e1 \u0161t\u00edhl\u00e9 v\u0159eteno, podle kter\u00e9ho z\u00edskala p\u0159ezd\u00edvku Spindle Galaxy<\/em>. Na rozd\u00edl od spir\u00e1ln\u00edch galaxi\u00ed zde chyb\u00ed v\u00fdrazn\u00e1 ramena. Dominantn\u00ed centr\u00e1ln\u00ed oblast plynule p\u0159ech\u00e1z\u00ed do hladk\u00e9ho disku bez ru\u0161iv\u00fdch detail\u016f, co\u017e d\u00e1v\u00e1 galaxii velmi \u010dist\u00fd a vyzr\u00e1l\u00fd vzhled.<\/p>\n<\/div>\n

\n

NGC 2903 \u2013 Herschel 137<\/h3>\n

20. 2. 2026<\/strong>
\n<\/a><\/p>\n

Jasn\u00e1 spir\u00e1ln\u00ed galaxie v souhv\u011bzd\u00ed Lva (Leo)<\/strong>, vzd\u00e1len\u00e1 asi 30 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1784<\/strong>.<\/p>\n

NGC 2903 je v\u00fdrazn\u00e1 a vizu\u00e1ln\u011b velmi atraktivn\u00ed spir\u00e1ln\u00ed galaxie. Jej\u00ed spir\u00e1ln\u00ed ramena jsou jasn\u011b patrn\u00e1 a bohat\u011b strukturovan\u00e1, co\u017e galaxii dod\u00e1v\u00e1 dynamick\u00fd vzhled a pocit pohybu. Na rozd\u00edl od klidn\u011bj\u0161\u00edch spir\u00e1l p\u016fsob\u00ed NGC 2903 v\u00fdrazn\u011b \u201eaktivn\u011b\u201c, s patrn\u00fdm kontrastem mezi centr\u00e1ln\u00ed oblast\u00ed a vn\u011bj\u0161\u00edmi \u010d\u00e1stmi disku. Celkov\u011b jde o galaxii, kter\u00e1 na sn\u00edmku okam\u017eit\u011b upout\u00e1 pozornost a pr\u00e1vem b\u00fdv\u00e1 pova\u017eov\u00e1na za jeden z nejhez\u010d\u00edch objekt\u016f t\u00e9to \u010d\u00e1sti oblohy, p\u0159esto\u017ee nepat\u0159\u00ed mezi klasick\u00e9 Messierovy c\u00edle.<\/div>\n
\n

NGC 3626 \u2013 Caldwell 40<\/h3>\n

25. 2. 2026<\/strong>
\n<\/a><\/p>\n

Galaxie v souhv\u011bzd\u00ed Lva<\/strong>, vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 70 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1784<\/strong>.<\/p>\n

NGC 3626 je galaxie, kter\u00e1 na prvn\u00ed pohled nep\u016fsob\u00ed nijak n\u00e1padn\u011b, ale p\u0159i bli\u017e\u0161\u00edm pohledu m\u00e1 kompaktn\u00ed, v\u00fdrazn\u011bj\u0161\u00ed centr\u00e1ln\u00ed oblast a jemn\u011b nazna\u010den\u00fd disk, kter\u00fd nep\u016fsob\u00ed tak otev\u0159en\u011b jako u klasick\u00fdch spir\u00e1l.<\/div>\n
\n

NGC 4449 \u2013 Caldwell 21 (Box Galaxy)<\/h2>\n

27. 2. a 10. 3. 2026<\/strong>
\n<\/a><\/p>\n

Nepravideln\u00e1 galaxie v souhv\u011bzd\u00ed Honic\u00edch ps\u016f<\/strong>, vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 12 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem roku 1788<\/strong>.<\/p>\n

NGC 4449 pat\u0159\u00ed mezi nejzaj\u00edmav\u011bj\u0161\u00ed nepravideln\u00e9 galaxie severn\u00ed oblohy. Na prvn\u00ed pohled p\u016fsob\u00ed chaoticky, ale p\u0159i hlub\u0161\u00edm pohledu je z\u0159ejm\u00e9, \u017ee jde o velmi aktivn\u00ed syst\u00e9m s intenzivn\u00ed tvorbou hv\u011bzd. Galaxie je bohat\u00e1 na oblasti ionizovan\u00e9ho vod\u00edku a p\u0159ipom\u00edn\u00e1 sp\u00ed\u0161e zv\u011bt\u0161enou obdobu Magellanov\u00fdch mra\u010den. D\u00edky sv\u00e9 aktivit\u011b a \u010dlenit\u00e9 struktu\u0159e je velmi fotogenick\u00e1 a nab\u00edz\u00ed mno\u017estv\u00ed detail\u016f i p\u0159i del\u0161\u00edch ohnisc\u00edch.<\/p>\n

Sn\u00edmek t\u00e9to galaxie z\u00edskal ocen\u011bn\u00ed Top Pick Nomination na AstroBinu.<\/p>\n

\n

NGC 4559 \u2013 Caldwell 36 (Koi Fish Galaxy)<\/h3>\n

6. 3. 2026<\/strong>
\n<\/a>
\nSpir\u00e1ln\u00ed galaxie Kap\u0159\u00edk v souhv\u011bzd\u00ed Honic\u00edch ps\u016f<\/strong>, vzd\u00e1len\u00e1 asi 29 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1784<\/strong>.<\/p>\n

Tato spir\u00e1ln\u00ed galaxie je zn\u00e1m\u00e1 sv\u00fdm nepravideln\u00fdm, t\u00e9m\u011b\u0159 \u201erozvln\u011bn\u00fdm\u201c vzhledem spir\u00e1ln\u00edch ramen, d\u00edky kter\u00e9mu z\u00edskala p\u0159ezd\u00edvku Koi Fish Galaxy<\/em>. Ramena galaxie jsou bohat\u00e1 na oblasti tvorby hv\u011bzd a tmav\u00e9 prachov\u00e9 struktury, kter\u00e9 j\u00ed dod\u00e1vaj\u00ed v\u00fdraznou plasticitu. P\u0159esto\u017ee nejde o extr\u00e9mn\u011b jasn\u00fd objekt, p\u0159i dobr\u00fdch podm\u00ednk\u00e1ch dok\u00e1\u017ee nab\u00eddnout velmi estetick\u00fd v\u00fdsledek s v\u00fdrazn\u00fdm kontrastem mezi rameny a okoln\u00edm pozad\u00edm.<\/div>\n
\n

NGC 4631 \u2013 Caldwell 32 (Whale Galaxy)<\/h3>\n

7. 3. 2026<\/strong>
\n<\/a><\/p>\n

Zn\u00e1m\u00e1 \u201eVelryba\u201c v souhv\u011bzd\u00ed Honic\u00edch ps\u016f<\/strong>, vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 30 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1787<\/strong>.<\/p>\n

NGC 4631 je velmi charakteristick\u00e1 galaxie, kter\u00e1 sv\u00fdm tvarem skute\u010dn\u011b p\u0159ipom\u00edn\u00e1 siluetu velryby, podle n\u00ed\u017e z\u00edskala svou p\u0159ezd\u00edvku. Jej\u00ed prot\u00e1hl\u00fd disk p\u016fsob\u00ed robustn\u011b a \u017eiv\u011b, s mno\u017estv\u00edm jemn\u00fdch nerovnost\u00ed a struktur, kter\u00e9 d\u00e1vaj\u00ed galaxii dynamick\u00fd vzhled. NGC 4631 pat\u0159\u00ed mezi vizu\u00e1ln\u011b velmi siln\u00e9 a zapamatovateln\u00e9 objekty zimn\u00ed oblohy.<\/div>\n
\n

NGC 3356<\/h3>\n

12.\u201313. 3. 2026<\/strong>
\n<\/a><\/p>\n

Galaxie v souhv\u011bzd\u00ed Lva<\/strong>, vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 33 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1784<\/strong>.<\/p>\n

NGC 3356 pat\u0159\u00ed mezi m\u00e9n\u011b zn\u00e1m\u00e9 galaxie a \u010dasto z\u016fst\u00e1v\u00e1 ve st\u00ednu v\u00fdrazn\u011bj\u0161\u00edch objekt\u016f v dan\u00e9 oblasti oblohy. Fotografov\u00e1n\u00ed t\u00e9to galaxie prob\u00edhalo za nep\u0159\u00edzniv\u00fdch podm\u00ednek, p\u0159esto se poda\u0159ilo zachytit jej\u00ed z\u00e1kladn\u00ed strukturu a charakteristick\u00fd tvar. Pr\u00e1v\u011b takov\u00e9 sn\u00edmky \u010dasto nejl\u00e9pe dokumentuj\u00ed realitu astronomick\u00e9 praxe, kdy ne ka\u017ed\u00e1 noc nab\u00edz\u00ed ide\u00e1ln\u00ed seeing a pr\u016fzra\u010dnost, ale i p\u0159esto m\u00e1 smysl data sb\u00edrat a zpracovat.<\/div>\n
\n

NGC 5005 \u2013 Caldwell 29<\/h3>\n

17. 3. 2026<\/strong>
\n<\/a><\/p>\n

Spir\u00e1ln\u00ed galaxie v souhv\u011bzd\u00ed Honic\u00edch ps\u016f<\/strong>, vzd\u00e1len\u00e1 p\u0159ibli\u017en\u011b 41 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem roku 1785<\/strong>.<\/p>\n

NGC 5005 je v\u00fdrazn\u00e1 spir\u00e1ln\u00ed galaxie s jasn\u00fdm centr\u00e1ln\u00edm j\u00e1drem a jemn\u011b strukturovan\u00fdmi rameny. Vizu\u00e1ln\u011b i fotograficky zaujme kontrastem mezi sv\u011btl\u00fdm st\u0159edem a tmav\u0161\u00edmi oblastmi prachu v disku. Galaxie je \u010dasto fotografov\u00e1na spole\u010dn\u011b se sv\u00fdm men\u0161\u00edm pr\u016fvodcem NGC 5033, co\u017e umo\u017e\u0148uje zaj\u00edmav\u00e9 srovn\u00e1n\u00ed dvou rozd\u00edln\u00fdch spir\u00e1ln\u00edch syst\u00e9m\u016f.<\/div>\n
\n

NGC 5033 \u2013 Herschel 302<\/h3>\n

18.\u201319. 3. 2026<\/strong>
\n<\/a><\/p>\n

Spir\u00e1ln\u00ed galaxie v souhv\u011bzd\u00ed Honic\u00edch ps\u016f<\/strong>, vzd\u00e1len\u00e1 asi 45 milion\u016f sv\u011bteln\u00fdch let<\/strong>.<\/p>\n

Objevena Williamem Herschelem v roce 1785<\/strong>.<\/p>\n

NGC 5033 je klasick\u00e1 spir\u00e1ln\u00ed galaxie, kter\u00e1 na sn\u00edmc\u00edch p\u016fsob\u00ed velmi vyv\u00e1\u017een\u00fdm dojmem. M\u00e1 dob\u0159e definovan\u00e9 j\u00e1dro a jemn\u00e1 spir\u00e1ln\u00ed ramena, kter\u00e1 nejsou na prvn\u00ed pohled p\u0159\u00edli\u0161 kontrastn\u00ed, ale p\u0159i pe\u010dliv\u00e9m zpracov\u00e1n\u00ed dat vyniknou. Fotografov\u00e1n\u00ed prob\u00edhalo b\u011bhem dvou noc\u00ed. V\u00fdsledn\u00fd sn\u00edmek tak symbolicky uzav\u00edr\u00e1 celou moj\u00ed zimn\u00ed s\u00e9rii galaxi\u00ed.<\/div>\n
\n

Z\u00e1v\u011br<\/h3>\n

S p\u0159\u00edchodem astronomick\u00e9ho jara sez\u00f3na galaxi\u00ed zdaleka nekon\u010d\u00ed. Pokud po\u010das\u00ed dovol\u00ed, budu pokra\u010dovat ve focen\u00ed dal\u0161\u00edch objekt\u016f, kter\u00e9 mi chyb\u00ed do kompletace Caldwellova katalogu<\/a>\u00a0a p\u0159\u00edpadn\u011b i\u00a0Herschelova katalogu<\/a>.<\/p>\n

Velk\u00fdm pomocn\u00edkem je mi i m\u00e1 aplikace DSO dnes<\/a>,\u00a0 kter\u00e1 mi umo\u017e\u0148uje v\u00fdb\u011br nejvhodn\u011bj\u0161\u00edch deep-sky objekt\u016f pro celono\u010dn\u00ed focen\u00ed.<\/p>\n

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

P\u0159esto\u017ee hlavn\u00ed sez\u00f3na galaxi\u00ed vrchol\u00ed na ja\u0159e, i zimn\u00ed m\u011bs\u00edce nab\u00edzej\u00ed \u0159adu pozoruhodn\u00fdch c\u00edl\u016f. B\u011bhem zimy 2025\/2026 jsem se zam\u011b\u0159il na fotografov\u00e1n\u00ed galaxi\u00ed z katalog\u016f Caldwell a Herschel, kter\u00e9 jsou dob\u0159e dostupn\u00e9 ze severn\u00ed polokoule a umo\u017e\u0148uj\u00ed mi systematick\u00e9 dopl\u0148ov\u00e1n\u00ed m\u00e9 sb\u00edrky.<\/p>\n","protected":false},"author":1,"featured_media":466,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7,9],"tags":[],"class_list":["post-460","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\/460","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=460"}],"version-history":[{"count":6,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts\/460\/revisions"}],"predecessor-version":[{"id":467,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/posts\/460\/revisions\/467"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=\/wp\/v2\/media\/466"}],"wp:attachment":[{"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=460"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=460"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/hujer.net\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=460"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}