Astrophotography - Iñaki Lizaso

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Equipment:

Takahashi FCT-100

Takahashi FSQ-106ED

Takahashi Mewlon-210

Takahashi FS-102

Takahashi EM-200 Temma2M

ZAO & eyepieces / okularrak

Lunt LS-80THa

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 objects 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.

Barnard's Loop (Sh 2-276) is an emission nebula in the constellation of Orion. The loop takes the form of a large arc centered approximately on the Orion Nebula (M42) and it's part of the Orion Molecular Cloud Complex. The stars within the Orion Nebula are believed to be ionizing the Barnard's loop. M78 (at lower right) is a diffuse reflection nebula and belongs to the Orion Molecular Cloud Complex, lies about 1600 light years distant. The dark nebulae LDN1622 can be seen at upper left in the image.

Barnard begizta (Sh2-276) Orion konstelazioan dagoen igortze nebulosa da. Begiztak arku itxura dauka, gutxi gorabehera Orion nebulosan (M42) du bere erdigunea eta Orion Hodei Molekularraren zati bat da. Orion nebulosan zehar dauden izarrek Barnard begizta ionizatzen dutela uste da. M78 (behean eskuin aldean) islada-nebulosa hedatsua da, Orion Hodei Molekularraren zati bat osatzen duelarik gugandik 1600 argi urtera dago. LDN1622 hodei iluna goian eskuin aldean ikus daiteke argazkian.

Witch Head Nebula (IC 2118) is a faint reflection nebula in the Eridanus constellation at about 900 light years. Still to be determined, its believed to be an ancient supernova remnant or gas cloud illuminated by nearby supergiant star Rigel in Orion. Blue color is determined by the nature of the dust particles contained in the nebula by reflecting better blue than red. Radio observations confirmed substantial carbon monoxide emission throughout parts of the nebula, an indicator of the presence of molecular clouds where stars are forming.

Sorgin Buru nebulosa (IC 2118) Eridano konstelazioan 900 argi-urtera dagoen distira ahuleko islada-nebulosa da. Oraindik argitzeke dagoen arren gertu dagoen Orion konstelazioko Rigel izar erraldoiak argiztatzen duen, aintzinako supernoba baten hondarrak edo izar hodeia dela uste da. Kolore urdina nebulosaren partikulen izaerak ematen dio, kolore urdina gorria baino hobeto islatuz. Irrati uhin bidezko behaketek karbono-monoxidozko emisio nabarmena baieztatu dute nebulosaren gune zehatzetan, non izarrak sortzen ari diren hodei molekularren presentziaren adierazle.

Remaining in the Taurus Molecular Cloud, this image covers the west part of this big complex. Many dark nebulae can be seen there, B22 (center left), the Little Flame IC2087, B18 at lower right and B128 upper right.

Taurus Hodei Molekularran jarraituz, irudiak konplexuaren mendebaldeko nebulosa ilunak argazkitzen ditu, B22 (erdian ezker aldean), IC2087 nebulosa txikia, B18 behean eskuin aldean eta B18 goian eskuin aldean.

All the images in this site are © copyright by Iñaki Lizaso. Any use of these images without the prior written consent of the autor is strictly prohibited. Contact Iñaki Lizaso at edif300@yahoo.es

Web gune honetako irudi guztiek Iñaki Lizasoren © copyright dute. Irudi hauen edozein motako erabiliera egilearen idatzizko baimenik gabe zorrozki debekatua dago. Jar zaitez Iñaki Lizasorekin harremanetan edif300@yahoo.es