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img Adjust the brightness and contrast of your monitor until 18 grayscale steps from white to black are seen


Cepheus (Zefeo) konstelazioan eta gugandik 1400 argi-urtera kokatua, Van den Berg 152 islada nebulosa urdina aurkitzen da, hodei molekular baten ertzean murgildurik dagoen BD+69 1231 izarrak kolore urdina ematen dio. LDN1221 eta hauts adarrak eremua zeharkatzen du kometa balitz bezala.

Located in the Cepheus constellation at 1400 lights-years, Van den Berg 152 is a blue reflection nebula near the edge of a large molecular cloud with full of interstellar dust and a star in the embedded region (BD+69 1231) giving to the edge of the molecular cloud the blue color. LDN1221 and a large tail of dust crosses the field like a comet.


Konstelazio honetako izarrik distiratsuenek "teontzia" deritzon ezaguterraza den asterismo bat eratzen dute. Teontzi honen estalkia φ Sagittarii, λ Sagittarii eta δ Sagittariik, gorputza ζ Sagittarii, φ Sagittarii, δ Sagittarii eta ε Sagittariik, muturra δ Sagittarii, ε Sagittarii (konstelazioko izarrik distiratsuena) eta γ Sagittariik osatzen dute, teontzi honen heldulekua berriz, ζ Sagittarii, τ Sagittarii, σ Sagittarii eta φ Sagittarii izarrek osatzen dute.

Sagittarius constellation's brighter stars form an easily recognizable asterism known as "the Teapot". The stars δ Sgr (Kaus Media), ε Sgr (Kaus Australis), ζ Sgr (Ascella), and φ Sgr form the body of the pot; λ Sgr (Kaus Borealis) is the point of the lid; γ Sgr (Alnasl) is the tip of the spout; and σ Sgr (Nunki) and τ Sgr the handle. These same stars originally formed the bow and arrow of Sagittarius. Marking the bottom of the teapot's "handle", is the bright star (2.59 magnitude) Zeta Sagittarii (ζ Sgr), named Ascella, and the fainter Tau Sagittarii (τ Sgr).


Rho Ophiuchi nebulosa konplexua gas eta hauts nebulosa iluna da ρ Ophiuchi izarretik gradu bat hegoaldera, gugandik 427 argi-urtera aurkitzen da eta Eguzki Sistematik izarrak sortzen ari diren eremurik gertuena da. Zeta Ophiuchi (ζ Oph), gutxi gorabehera 366 argi-urteko distantziara kokatzen da eta Sh2-27 "Cobold" nebulosaz inguratuta dago, izarraren talka-uztaia da, Rho Ophiuchi hodei konplexutik gertu dagoen hauts-hodei trinkoetan barrena doan bitartean.

The Rho Ophiuchi cloud complex is a dark nebula of gas and dust that is located 1° south of the star ρ Ophiuchi of the constellation Ophiuchus and at an estimated distance of 427 ligth years is one of the closest star-forming regions to the Solar System. Zeta Ophiuchi (ζ Oph) is a star located in the constellation of Ophiuchus and lies at estimated distance of 366 light-years from the Earth. It is surrounded by the Sh2-27 "Cobold" nebula, the star's bow shock as it ploughs through dense dust clouds near the Rho Ophiuchi cloud complex.

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Zeta Ophiuchi (ζ Oph), Ofiuchus (Ofiuko) konstelazioan aurkitzen den izarra da eta 2,57ko magnitude bisuala du. Lurretik gutxi gorabehera 366 argi-urteko distantziara kokatzen da. Sh2-27 "Cobold" nebulosaz inguratuta dago, izarraren talka-uztaia da Rho Ophiuchi hodei konplexutik gertu dagoen hauts-hodei trinkoetan barrena doan bitartean.

Zeta Ophiuchi (ζ Oph) is a star located in the constellation of Ophiuchus and has an apparent visual magnitude of 2.57. Lies at estimated distance of 366 light-years from the Earth. It is surrounded by the Sh2-27 "Cobold" nebula, the star's bow shock as it ploughs through dense dust clouds near the Rho Ophiuchi cloud complex.


Irudiko eremua Ophiuchus (Ofiuko) konstelazioaren hegoaldean kokatzen da, bertan hainbat nebulosa ilun daude LDN137, LDN162, LDN158 edo LDN190 hauts nebulosa ahulez inguraturik.

This field is located in southern area in Ophiuchus constellation, many dark nebulae such as LDN137, LDN162, LDN158 and LDN190 by surrounding dusty faint nebulae.


2022ko Maiatzak 16ko Ilargi Eklipse Osoa.

Total Lunar Eclipse of 2022 May 16.


Eguzki-Orbanak.

AR2991, AR2993, AR2994, AR2995, AR2996, AR2997, AR2998

Sunspots.


Iparrizarra (Alpha Ursae Minoris) Ursa Minor (Hartz Txikia) konstelazioko izarrik distiratsuena da. Zeruko ipar polotik oso gertu dago eta horregatik gaur egungo iparrizarra da. Eremuan Hauts Fluxus osatutako nebulosak ikus daitezke, galaxiako izarrek argiztatzen dituzten latitude altuko nebulosak dira. NGC3172 galaxia berriz, iparren dagoen galaxia da, gugandik 285 milioi argi-urtera kokatua eta zeruan duen kokapenagatik Polarissima Borealis bezala ezaguna.

Polaris is a star in the constellation Ursa Minor. Designated α Ursae Minoris and commonly called the Pole Star. The star's position is less than one degree from the north celestial pole, making it the current north pole star. The entire field is full of Integrated Flux Nebula, high-latitude galactic nebulae in the Milky Way composed primarily of dust particles, hydrogen, and carbon monoxide and are illuminated by stars in the Milky Way. NGC 3172 is located 285 million light years away, known as Polarissima Borealis, being the closest NGC object to the North Celestial Pole.


Lur planetak, bira bat ematen dio bere ardatzari 23h 56m 04s-tan. Argazkian, 3 orduko bira argazkitu da.

Earth rotates around its axis in 23h 56m 04s. Here the image has 3 hours of rotation.


William Herschelek aurkitu zuen 1784ko urriaren 16an Monoceros (Adarbakarra) konstelazioan dagoen NGC 2170 nebulosa. Izar berriak sortzen ari diren Monoceros hodei molekularraren ertzean kokatzen da, gugandik 2700 argi-urtera. Eremuan hainbat nebulosa daude, LBN 990, VdB 73, VdB 74 eta LBN 1004 adibidez.

Reflection nebula NGC 2170 was discovered on October 16, 1784 by William Herschel in Monoceros constellation. Located at the edge of the giant star- forming molecular cloud Monoceros, lies 2700 light-years way. Many nebulae in this field around NGC 2170 region, LBN 990, VdB 73, VdB 74, LBN 1004...

 

 

 

 

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
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