lupuvictor

Compoziţia lui Saturn este similara cu cea al lui Jupiter, dar are o masă mult mai mică si deci un interior cu un nucleu mult mai mic. În acelasi fel ca Jupiter, răcirea interiorului lui Saturn produce condensul de heliu lichid în hidrogen-heliu. Acest proces eliberează căldură ca urmare a schimbării de fază.

In these images the telescope, is presented the East of the Moon. On the Moon seen from Earth, are some features on the edge that are rarely seen because the Moon always remains the same face toward us. These features are large craters or seas.

Videos of the planets are in the forefront in the processing programs. The videos with Moon craters are burned on the DVDs, and I put a dot with a marker, and get back to them later.

Aceasta este "Super Luna" la perigeu din data de 5-6 mai 2012 . In acest articol am postat fotografii cu Luna plina realizate prin telescop cu Nikon DSLR D80, dar si video cu, si fara telescop, prin camera Sony CX 130. Denumirea de "Supermoon" sau "Super Luna" , nu a venit din astronomie, ci de la astrologie.

This is "Super Moon" at perigee from 5 May 2012. In this article I posted photos of full Moon through a telescope made ​​with Nikon D80 DSLR, and videos with no telescope through my Sony CX 130. The name "Super Moon" did not come from astronomy, but astrology.

Aceasta este planeta Venus filmata in data de 30 aprilie 2012, cand aceasta a fost la -4.5 magnitudine, destul pentru a fi vizibila la lumina zilei. Aceasta data este inscrisa in tabelul cu pozitiile speciale ale planetei, ca fiind foarte straucitoare.

Read more: http://astrofotografieluna.blogspot.com/2012/05/planeta-venus-la-magnitudine-mare.html

Snellius (83 km), este un crater aflat la sud-vest de craterul mai mare Petavius (177 km) de pe partea de sud-est a Lunii. Hase (83 km) de 2,5 km adancime,, in aceste fotografii are marginea podelei de vest in umbra, iar Hase D (56 km), este complet in intuneric, avand in lumina doar marginea de sud-est.

Snellius (83 km), a crater is located southwest of the crater Petavius (177 km) on the south-east of the Moon. Hase (83 km) 2.5 km in depth, in these pictures the western edge of the floor is in shadow, and Hase D (56 km), is completely in the dark, the southeast edge being only in the sunlight.

This is Vendelinus crater (147 km), through telescope and video camcorder, and the images in this article are captures.
Details are fine and I applied several edits to photos like brightness and sharpness in FastStone program.

In the images of Mars here, we see only the northern ice cap (as seen in pictures, north is reversed as seen through the telescope).
To see the video in which I made these images visualize: Mars video.