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IC443 (Marmoka Nebulosa) supernoba baten hondarrak dira (ingeleraz SNR) Bikiak konstelazioan, Lurretik gutxi gora behera 5.000 argi-urteko distantzian kokatzen dena. Duela 3.000 eta 30.000 urte artean gertatu zen supernoba eztanda baten hondarrak direla uste da. Irudian Messier 35 izar multzoa ikus daiteke, Philippe Loys de Chéseaux-ek aurkitzu zuen 1745an lehenengoz eta John Bevis-ek ere 1750a baino lehenago bere kabuz topatu zuen. Izar multzoa Lurretik 2800 argi-urtera kokatzen da.

IC 443 (Jellyfish Nebula) is a supernova remnant (SNR) in the constellation Gemini at a roughly distance of 5,000 light years from Earth. May be the remains of a supernova that occurred 3,000 - 30,000 years ago. In the field can be seeing Messier 35, an open cluster which was discovered by Philippe Loys de Chéseaux in 1745 and independently discovered by John Bevis before 1750. The cluster lies 2,800 light-years from Earth.


Neguko Esne Bidean, Adarbakarra eta Txakur Handia konstelazioen arteko mugan kokatzen den nebulosa konplexu polit hau Kaio Nebulosa bezala ezagutzen dugu. Eremu zabaleko nebulosa honek distiratsuak diren hainbat izar multzo eta nebulosa biltzen ditu, IC2177, NGC2327, NGC2335, NGC2343, SH2-293 edo LBN1039.

A spectacular nebulae region of the winter Milky Way lies along the border between the constellations Monoceros and Canis Major, is known as Seagull nebula. This nebulous complex encompasses some bright nebulae and star clusters as IC2177, NGC2327, NGC2335, NGC2343, Sh2-293 or LBN1039.


Zefeo konstelazioan, NGC7822 (erdian goian, non izar berriak sortzen ari diren) nebulosak eta CED-214 (erdian behean) nebulosak Sharpless 171 igorle eremua osatzen dute. Izar multzoak, egitura ugariz osatutako nebulosak, nebulosa ilunak eta eremu aberatsak OIIIan ere.

In the Cepheus constellation, the star forming complex NGC 7822 (upper center) and CED-214 (lower center) encompasses the Sharpless emission region 171. Beautiful nebula with plenty structures, star clusters, many dark nebulaes with rich area in OIII.

 

IDA


Barnard B169, B171 eta B174 nebulosa ilunen eremua, Esnebidean kokaturik dagoen Cepheus konstelazioan. Hainbat objektu ikus daitezke, B170, B368, B173 nebulosa ilunak eta baita Sh2-134 eta Sh2-135 nebulosa distiratsuak ere.

Several dark nebula in Cepheus constellation located in the Milky Way. Among of them, dark nebulae B170, B368, B169, B171 and B173 can be seen. Including bright nebulas SH2-134 and SH2-135.


2017ko abuztuak 21, arratsaldeko 16:00ak, autoa gidatzen noa amaigabeko autopilaketa batean, bitartean eklipseak emandako segundu guztiak gogoratzen gabiltz lagun Julen, Freddy eta hirurok. Niretzat bigarren eklipse osoa, aurrekoa 1999an Errumanian ikusi baitnuen, saros berdineko eklipsea. Saros 145ko hurrengo eklipsea 2035ko irailan izango da Japonian. Nork jakin...

August 21 2017, 4:00PM driving to hotel through an endless jam, I am remembering with my friends Julen and Freddy all the seconds of the solar total eclipse. My second total eclipse with Romania 1999 and both from same Saros, a coincidence. Next eclipse from Saros 145 will be in Japan in sep 2035. Who knows...


IC 1318, Sadr izarraren edo Gamma Cygniren inguruan dagoen igortze nebulosa da, Tximeleta nebulosa bezala ezaguna ere. Gamma Cygni izarraren inguruan nebulosa ilun asko daude, igortze nebulosez gain. Sadr izarraren distira 2,2 magnitude ingurukoa da gutxi gorabehera eta inguruko nebulosak ere nahiko distiratsuak dira.

IC 1318, is the diffuse emission nebula surrounding Sadr or Gamma Cygni (the star of the center of Cygnus's cross), known also as Buttefly Nebula. This region contains many dark nebulae in addition to the emission diffuse nebulae. Sadr itself has approximately a magnitude of 2.2 and the nebulous regions around it are also fairly bright.


Barnard 72 nebulosa iluna Ofiuko konstelazioan kokatzen da, Esne-Bidearen gainean S itxura duenez Sugea Nebulosa bezala ezaguna. Eremuan nebulosa beltz ugari daude, irudian Barnard 60, B62, B63, B67, B68, B72, B74, B75 eta B77 ikus daitezke.

Barnard 72 is a dark nebula in the Ophiuchus constellation known as Snake Nebula cause it's S-shaped dust lane over Milky-Way. It's a dark nebulaes region, Barnard 60, B62, B63, B67, B68, B72, B74, B75 and B77 can be find in this image.


Saturno. Oposizioan aurkituko da ekainak 15an.

Saturno. Will be at opposition in June 15.


Jupiter Eguzki-sistemako bosgarren planeta da, dauden gasezko lau erraldoietako bat. Sistemako planetarik handiena da. Lurrak baino 318 aldiz masa handiagoa du, eta diametroan 11 aldiz handiagoa da.

Jupiter. The fifth planet in the Solar System is one of the giants of the four giant gas planets. It's the biggest planet in the system. 318 times greater than Earth's mass and 11 times greater in diameter.


Messier 81 (NGC 3031 or Bode's Galaxy refering to Johann Elert Bode who discovered it) is a spiral galaxy about 12 million light-years away in the constellation Ursa Major while the Messier 82 (NGC 3034, Cigar Galaxy), about five times more luminous than the whole Milky Way, is a starburst galaxy near to M81. NGC 3077 is a small galaxy, also member of the M81 Group. Despite looking much like an elliptical galaxy, shows wispy edges and scattered dust clouds that are probably a result of gravitational interaction with its larger neighbors.

Messier 81 (NGC 3031 edo Boderen Galaxia bezala ezaguna, Johann Elert Bodek lehen aldiz aurkitu zuenez bere oroimenez izendatua) galaxia espirala da gugandik 12 milioi argi-urtera kokatzen delarik Hartz Handia konstelazioan. Messier 82 (NGC 3034 edo Zigarro Galaxia) berriz, Esne Bidea baino bost aldiz distiratsuagoa da, M81 galaxiatik gertu leherketa prozesuan dagoen galaxia da. NGC 3077 galaxia txikia da, M81 galaxia-multzoko kide bat. Nahiz eta galaxia eliptikoa dirudien izar-hodei barreiatuak ditu bere baitan, bere bizilagun handiekiko grabitazio iterezioen ondorioa izan daitekela uste da.

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