05 May 2015

Jupiter 4/5/2015




 Jupiter 4/5/2015

Mount : Skywatcher HEQ5 pro
Telescope : Skywatcher Skymax 127(5")
Camera : ZWO ASI 120mm
Programms : Registax 6 & Photoshop CS5 


13 January 2015

M 42 Orion & Star Adventurer


M 42 Orion & New Star Adventurer from Skywatcher

First test with ultra portable mount from Skywatcher star adventurer and Nikon D-5100 with 55-200mm lens.
50 frames of 45sec at 135mm. 

08 January 2015

Byzantine chapel


 Byzantine chapel and The Great Orion

Αγία Τριάδα Γραμματικού
Είναι το παλαιότερο κτίσμα που βρέθηκε στην περιοχή και χρονολογείται γύρω στον 13ο -14ο αιώνα. Σύμφωνα με πληροφορίες στον προαύλιο χώρο υπήρχε μοναστήρι ενώ αργότερα χρησιμοποιήθηκε ως άσυλο ανιάτων λόγω τη φυσικής δομής της περιοχής



Holy Trinity Grammatiko
It's the oldest building found in the area dates back to the 13th-14th century. According to information in the courtyard there was a monastery and later used as a Hospice due to the physical structure of the region


Byzantine chapel "Agia Triada" and The Great Orion. - See more at: http://www.astropixel.gr/dslr-astrophotography#sthash.9o0bpiBt.dpuf

17 October 2014

Vdb 152 in Lrgb


Vdb 152 LRGB
Telescope: William Optics FLT 110 with F/T focuser 3025 & Starizona usb motor focus
Mount: Skywatcher ΗEQ5 pro
Chip: Atik 314L+ at 0c
Guiding: TS finder 8x50 with Meade DSI I pro
Filter wheel: Starlight Xpress usb 7x1.25
Location: Elikonas
Luminance: 51x420min - 357min
Red: 9x300 - 45min
Green: 9x240 - 36min
Blue: 9x300 - 45min
Total: 483min (8 hours 5 min)
Programs I have used-
Maxim DL ,Pixinsight 1.6, Photoshop CS5, The Sky6 ,Focusmax

Van den Bergh 152, also known as Cederblad 201, is a blue reflection nebula at top left in the image. The large dark nebula stretching through the frame is Barnard 175, a Bok Globule. This complex, also called Wolf's Cave, is located about 1,400 light years away in the direction of the constellation of Cepheus.

Full of very faint dust, this area is part of a large molecular cloud named the Cepheus Flare by Edwin Hubble. The opaque dust blocks most of the starlight behind it, but blue light from a young star is scattered and reflected off some of the particles to illuminate the reflection part of the nebula. Some of the faint dust may be glowing in a dim red color from luminescence, forming an Extended Red Emission nebula (ERE).

14 June 2014

Mare Nubium-Pitatus-Tycho-Clavius






Mare Nubium, Pitatus, Tycho & Clavius
Another one photo with my new setup(ASI 120mm & Skymax 127/1500)
More information about this photo : http://www.astropixel.gr

"Sea of Clouds" redirects here. It is not to be confused with the Chinese poetic term for the surroundings of a mountain's summit, most-notably at Huangshan.
Mare Nubium ("sea of clouds") is a lunar mare in the Nubium basin on the Moon's near side. The mare is located just to the southeast of Oceanus Procellarum.

Tycho is a prominent lunar impact crater located in the southern lunar highlands, named after the Danish astronomer Tycho Brahe (1546–1601).[1] To the south is the crater Street; to the east is Pictet, and to the north-northeast is Sasserides. The surface around Tycho is replete with craters of various sizes, many overlapping still older craters. Some of the smaller craters are secondary craters formed from larger chunks of ejecta from Tycho.

10 June 2014

Copernicus crater

Copernicus crater
with my new telescope Skywatcher Skymax 127/1500 Maksutov and my new camera ZWO ASI 120mm.
More information about this photo : http://www.astropixel.gr
  
Copernicus is a lunar impact crater named after the astronomer Nicolaus Copernicus, located in eastern Oceanus Procellarum .It typifies craters that formed during the Copernican period in that it has a prominent ray system.
Copernicus is visible using binoculars, and is located slightly northwest of the center of the Moon's Earth-facing hemisphere. South of the crater is the Mare Insularum, and to the south-south west is the crater Reinhold. North of Copernicus are the Montes Carpatus, which lie at the south edge of Mare Imbrium. West of Copernicus is a group of dispersed lunar hills. Due to its relative youth, the crater has remained in a relatively pristine shape since it formed