Archive for refractor

M34 Open Cluster at Perseus Constellation

Posted in Astrophotography with tags , , , , , , , , , , , on 2013/10/12 by computerphysicslab

Very close to Tringulum galaxy M33 we may spot a bright open cluster towards Perseus constellation. Its name is M34 and here it is a picture I took today through a remote 6 inch apochromatic refractor on New Mexico that shows colorful stars. Enjoy it!

M34-open-cluster-color-Perseus-constellation

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Celestron NexStar 5SE vs Takahashi FS102

Posted in Astrophotography with tags , , , , , , , , , , , , , , on 2011/02/19 by computerphysicslab

This week I had the chance to test a Takahashi FS102 refractor apochromatic fluorite telescope and also a Celestron NexStar 5SE Schmidt-Cassegrain catadioptric telescope. First one has an aperture of 102mm and second one of 125mm plus a central obstruction. Their light gathering power is similar and also their theoretical resolution. Nevertheless I wanted to check by myself the mythical optical quality of FS102 in contrast to the well-known Celestron.

Tests were made using the same camera to capture video and similar weather conditions both nights. I took in both cases a video of the planet Saturn when reaching the meridian, its maximum altitude. Celestron C5 perform flawlessly because I could get a sharp view of Saturn and its ring at 500x magnification. Takahashi also let me reach that high powers with a crisp result. C5’s focuser is very precise, but Takahashi’s is even more being a rack and pinion system. Focusing the FS 102 was very pleasant due to its smoothness and accuracy. Probably a better contrast in visual images delivered by refractor telescopes also gave it an advantage here.

Trying to resolve fine details, in both telescopes I could see the shadow of Saturn over the rings clearly. Here it is the final picture after applying Registax and Fitswork4 to both videos.

Probably FS102 performs better on wide field astrophotography, but on planetary imaging this picture above is my conclusion.

Sharing raw footage of Jupiter and Saturn

Posted in Astrophotography with tags , , , , , , , , , , , on 2011/02/11 by computerphysicslab

On 2011-02-06 I  took some videos of Jupiter and Saturn through a (4 inch) 102mm apochromatic refractor telescope. Applying Registax I got the results of the picture.

I’d like to share these two videos with anybody interested in playing with them:

http://www.mediafire.com/file/tqkri1z5z4pw8ge/Saturn-Takahashi-FS-102-F40-2011-02-06-divx.avi

http://www.mediafire.com/file/jbu38q5ucq9diwz/Jupiter-Takahashi-FS-102-F40-2011-02-06-divx.avi

Pluto, a dwarf planet

Posted in Astrophotography with tags , , , , , , , on 2010/10/22 by computerphysicslab

This picture is the result of stacking 9 subframes of 120 seconds of exposition each one through a 6-inch refractor telescope.

Pluto is a dwarf planet in the solar system, part of a double planetary system with its satellite Charon. It has a highly eccentric orbit inclined to the ecliptic, which runs until closer at perihelion inside the orbit of Neptune. The Pluto-Charon system has two moons: Nix and Hydra. These are celestial bodies that share the same category.

It was discovered on February 18, 1930 by American astronomer Clyde William Tombaugh (1906-1997) from the Lowell Observatory in Flagstaff, Arizona, and as the ninth and smallest planet in the Solar System by the International Astronomical Union and public opinion from then until 2006, but their group of planets in the solar system was always the subject of controversy among astronomers.

Its great distance from the Sun and the Earth, coupled with its small size, prevents shine below the magnitude 13.8 in its best moments (orbital perihelion and opposition), so it can be spotted only with telescopes bigger than 200 mm aperture (although there are people that says it can be spotted through apertures of 125 mm), photographically or CCD camera. It appears as star-looking, yellow, featureless point of light (apparent diameter of less than 0.1 arcsec).