The north-east of the Moon seen through astronomical telescope.

Moon's north has many interesting features though not as many as other areas. The first things I think about when it comes to this area are Sinus Iridum Bay, crater Plato, Aristarchus, Aristoteles and Mare Frigoris. Of these only Mare Frigoris Sinus Iridum can be distinguished through binoculars, and Plato, in some lighting conditions. In southern Sinus Iridum is the largest basin on the moon, Oceanus Procellarum, which extends over the northwestern part of it.

In these images are not seen all northern craters of the moon. Photographic maps of the area are here.

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.



Magnitude: -11.90
Phase: 0.86
Distance: 400.253 km
Illuminated: 85.8% (0% = new, 100% = full)

Astronomical Instrument: Celestron C8-Newtonian telescope
Eyepiece: Plossl 20mm, 2x Barlow
Mount: CG5 (EQ5)
Camera: Sony CX105
Filter: no
Date: 06.11.2011
Location: Baia Mare, Romania
Processing: FastStone Image Viewer

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HD astronomical telescope video on the Moon: Schickard Phocylides and Nasmith.

In this video of a few minutes, we have an observation on southwest craters of the Moon, such as Schickard (227 km), the largest in center of images, Nasmith and Phocylides located south of it, and Inghirami crater (91 km) which is located on the edge of the Moon, it is seen oval and submerged by darkness.

The impact that formed the crater Schickard, occurred in an area predominantly high. This was followed by an episode of flooding that occurred both inside and outside the crater Schickard, which took place before the impact that formed Mare Orientale.

Another episode of flooding followed, creating a thin layer of material that covered the areas that were affected by the first episode of flooding.

A final episode of flooding occurred within the crater Schickard, creating two spots that can be seen today.
Photo images extracted from this video are here.



Moon Age: 1.00 days
Illuminated: 99.8% (0% = New, 100% = Full)
Magnitude: -12.20
Distance: 398.772 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Video mode: 1080p
Filter: no
Date: 14/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

In the picture below are labeled craters and other lunar features in the region. To better understand this photo, you should note that the label with the name or the letter of larger craters could be found at their center, and on the small craters, you should find them around them, usually above.

Imafe from 2010.

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Video Astronomy Telescope Moon craters Pythagoras, Babbage, J. Herschel in a HD video.

In these video images, you can see on the Moon crater like Babbage (144 km.), J. Herschel (156 km), Philolaus (71 km) and Oenopides (67 km). All these lunar craters are located on the northern Moon.
To view video captures of this clip, press here.

Babbage has a depth of 2 km. It is an old lunar crater located near the northwest edge of the Moon, named after Charles Babbage. It is attached on southeast edge of the prominent crater Pythagoras (130 km). The remnant crater floor called South enters the southeast of Babbage.

Charles Babbage (December 26, 1791 - October 18, 1871) was an English poet, mathematician, philosopher, inventor and mechanical engineer. Babbage is best remembered for originating the concept of programmable computer.



Moon Age: 1.00 days
Illuminated: 99.8% (0% = New, 100% = Full)
Magnitude: -12.20
Distance: 398.772 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Video mode: 1080p
Filter: no
Date: 14/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

This video was also used also for simple video captures.

In the picture below are labeled craters and other lunar features in the region. To better understand this photo, you should note that the label with the name or the letter of larger craters could be found at their center, and on the small craters, you should find them around them, usually above.

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Grimaldi crater HD video through the telescope.

This video was also used for simple video captures. Photo images are here.
Craters that are visible here: Grimaldi (430 km), Hevelius (106 km), Lohrmann (31 km), Damoiseau (37 km) and Hermann (16 km).

Grimaldi (430 km) is rather a basin flooded by lava, not a crater, and has a round not oval shape as seen from Earth because it is located on the edge of the Moon. Its margins has not ordinary walls like other craters, but is so destroyed that was transformed into hills and irregular peaks.

Hevelius (106 km) has a low affected rim, and has a shallow depth of 1.8 km, in contrast with its size.
At the northern edge is a small but prominent crater, Cavalerius. At the south of Hevelius is Lohrmann crater (31 km) and to the south is Grimaldi (430 km). Because of their positions on the Moon, craters are oval when viewed from Earth.

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

In the pictures below are labeled craters and other lunar features in the region. To better understand this photo, you should note that the label with the name or the letter of larger craters could be found at their center, and on the small craters, you should find them around them, usually above.

Magnitude: -12.03
Phase: 70.5% (0% = new, 100% = full)
Distance: 398.311 km
Sidereal Period: 27.32 days
Illuminated: 92.2%

Optics: Celestron C8-Newtonian astronomical telescope 
Eyepiece: Plossl 20mm, 2x Barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 14/03/2014
Location: Baia Mare, Romania
Processing: FastStone Image Viewer

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Video Astronomy Telescope Moon craters Darwin Sirsalis, Rimae Byrgius in a HD video.

We note here craters like Darwin (130 km), Crüger flooded crater (46 km) of which has remained only its lip on the surface, Byrgius (87 km), Henry (41 km), Henry Freres (42 km), Cavendish (56 km) and Mersenius (84 km).
We also see in the images some deep grooves called Rimae Darwin and Rimae Sirsalis, named after nearby craters or craters which they cross.

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

This video was also used also for simple video captures.

Moon Age: 1.00 days
Illuminated: 99.8% (0% = New, 100% = Full)
Magnitude: -12.20
Distance: 398.772 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Video mode: 1080p
Filter: no
Date: 14/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

In the picture below are labeled craters and other lunar features in the region. To better understand this photo, you should note that the label with the name or the letter of larger craters could be found at their center, and on the small craters, you should find them around them, usually above.

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Heinsius and Wilhelm lunar craters (video through astronomical telescope)

Visible craters in this video are: Wilhelm (107 km), Heinsius (64 km), Wurzelbauer (88 km) and Tycho (85 km).

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

The video was also used also for simple video captures.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Video mode: 1080p
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

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The crater Archimedes - Astronomical Video.

Archimedes crater (83 km) area is one to which we refer in these pictures. The crater has an edge like a thick collar, circular, and from its south are starting mountains with the same name, Montes Archimedes. They are organized into two rows, so noticeable in pictures.

Large area surrounding both crater and mountains, is Mare Imbrium. To the east of these mountains, is a small basin called Palus Putredinis.

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

Images processed in Registax are, here.
Unprocessed images (video captures), are here.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

888 frames of the video in Registax.

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Videos of the Moon by telescope. Center lunar craters.

Craters located in the center of the lunar disc, as seen from Earth, are the most visible, because their whole structure is facing us revealing their floor and details perfectly, even with a modest telescope. In the center there are many features such as mountains, seas and craters.

There are many Moon craters seen passing in these videos, in which we note in their order of appearance: Godin / Agrippa (46/35 km) Triesnecker (26 km), Pallas / Murchison (50/58 km) Mare Insularum, Copernicus (93 km), Hipparchus (150 km), Flammarion (75 km), Ptolemaeus (153 km) Lalande (24 km), Mosting (26 km), Fra Mauro (95 km) and Gambart (25 km).



These videos were made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

These clips were used in Registax program to process images with higher quality, and also for simple video capture.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

Image of February 10, 2011.

Image of April 29, 2012.

Image of March 10, 2014.

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The Moon. North lunar craters Video through telescope.

In these images we can see many craters on the Moon, namely its north. These include features such as mountains and craters as: Vallis Alpes / Montes Alpes, Plato (109 km), Hercules / Atlas (69/87 km), Burg (40 km), Aristoteles / Euxodus (87/67 km)
The video was also used in Registax program to process images with higher quality, but also for simple video captures.

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

Images processed in Registax of crater Plato, here.
Unprocessed images (video captures), of crater Plato are here.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

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Craters filmed by astronomical telescope. Geber, Abenezra and Azophi.

The video was also used in Registax program to process images with higher quality, but also for simple video captures.

It's a bit more light on these images, but here are distinguished craters close to one another like Geber, Abenezra and Azophi (45/42/48 km) .

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Unstable aspect of the image through the telescope is caused by a combination of turbulence in the Earth's atmosphere and increased streams of heat from the ground and buildings.

Images were obtained by attaching a camera directly into the eyepiece of an astronomical telescope of 8 inch Newtonian; For this reason the eyepiece visual field was increased.

Images processed in Registax, here.
Unprocessed images (video captures), of craters Heraclitus / Licetus are here.

250 video frames in Registax.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

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(Video) Craters on the Moon seen clearly through telescope.

The south of the Moon is full of countless craters, where large basins of lava are missing. Craters Heraclitus and Licetus (90/75 km) are some of seen in these images processed also in Registax.

The astronomical telescope is pointed at the Moon's south pole, using motor tracking from Lacerta. Watch here craters as Heraclitus / Licetus (90/75 km) Maginus (163 km), Orontius (122 km), Tycho (85 km), Sasserides (90 km), Saussure (54 km).

The atmospheric quality has helped me quite a lot to shoot clear images of the area. The land in sunlight is white as milk. This color stops at the terminator at the large crater Clavius, where we encounter a hard penetrating dark.

The video was also used in Registax program to process images with higher quality, but also for simple video captures.

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable.

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Images processed in Registax, here.
Unprocessed images (video captures), of craters Heraclitus / Licetus are here.

170 frames, in Registax.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

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Telescope video of Maginus and Clavius lunar craters.

Atmosphere quality was satisfactory during video recording. Some turbulence are observed, but there are moments of great clarity.
Craters seen here are  Maginus (163 km) și Clavius (225 km).

Video captures images are in this article.
Registax images are in this article.

The video was also used in Registax program to process images with higher quality, but also for simple video captures.

The video was made with the camera mounted on the telescope, to be more exact on the telescope eyepiece. To protect the telescope from vibrations, I used a tracking motor from Lacerta, and thus the image was more stable. 

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

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Video and astrophotography by telescope Moretus crater.

I always liked to shoot the edge of the Moon, to observe closely the characteristics of vertices outside the lunar disk out. These shapes always fascinated me, because the edge of the Moon is the only area where you can enjoy a "3D" view of its relief, and the south is best suited for this.

Atmosphere quality was satisfactory during video recording. Some turbulence are observed, but there are moments of great clarity. Craters seen here are Moretus, Gruemberger/Cysatus, Zach.

The video was also used in Registax program to process images with higher quality, but also for simple video captures.
Simple video capture Images are here, and here.

The video was done with the camera mounted on the telescope, specifically on the telescope eyepiece. To protect telescope of vibrations, I used a guide motor from Lacerta, and thus the image was more stable. 

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

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Craters on the surface of the Moon Eratosthenes, Sinus Aestuum, Gambart.

These images include a larger area of the center area of the Moon.
Craters and other areas of relief observed while watching the clip, are: Manilius, Mare Vaporum, Sinus Aestuum, Eratosthenes, Stadius, and Gambart.

This video was also used in Registax program to process images with higher quality, but also for simple video captures.
Registax Photo Images are here.

The video was done with the camera mounted on the telescope, specifically on the telescope eyepiece. To protect telescope of vibrations, I used a guide motor from Lacerta, and thus the image was more stable. 

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.

Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

228 frames, in Registax.

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Images by astronomical telescope Moon craters Pitatus and Wurzelbauer (video).

In this video, the telescope was stopped over the western part of the Moon. We see some craters that I have not considered so large on other occasions, but at this stage, the shadow's edge of Wurzelbauer (88 km) and Pitatus (97 km), make them out to be more obvious. The two craters are located at the southern Mare Nubium.
The video was also used in Registax program to process images with higher quality, but also for simple video captures.
Registax Photo Images are here.

The video was done with the camera mounted on the telescope, specifically on the telescope eyepiece. To protect telescope of vibrations, I used a guide motor from Lacerta, and thus the image was more stable. 

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.


Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

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Copernicus Moon Crater filmed by astronomical telescope.

This is a video I have captured crater Copernicus (93 km) in unique circumstances for me in a light that I have never seen it. Observing this area through the telescope, is also subject to other articles, in which as usual, I presented simple video captures, but also Registax processings.

Copernicus's beauty is magnified because of its position on the center of the Moon, and in this way we see the round shape, as being above it. Here we can admire its dark inside and the outside in sunlight.

This video was also used in Registax program to process images with higher quality, but also for simple video captures.
Registax Photo Images are here.

The video was done with the camera mounted on the telescope, specifically on the telescope eyepiece. To protect telescope of vibrations, I used a guide motor from Lacerta, and thus the image was more stable. 

However, even with this tracking device for celestial bodies, there were vibrations of the telescope tube, causing the image to be slightly unstable. For this, I used the video stabilization option in Sony Vegas editing software, so the video was 100% correct on this issue.


Moon Age: 9.05 days
Phase: 70.5% (0% = New, 100% = Full)
Distance: 399.221 km

Optics (telescope or lenses): Celestron C8-Newtonian telescope, eyepiece 20mm Plossl, 2x barlow
Mount: CG5 (EQ5)
Camera: Sony CX130
Filter: no
Date: 10/03/2014
Location: Baia Mare, Romania
Processing: Sony Vegas HD Platinum 10.0

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