Submissions: 2013 September
Submissions: 2013 September
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Please post your images here.
Please see this thread before posting images; posting images demonstrates your agreement with
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Hotlinks to images over 400K slow down the thread too much and will be disabled.
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<- Previous submissions
[c]«« Discuss Anything in Astronomy «» Visit The Asterisk Main Page «» See Introductory Astonomy Lectures »»
«« Introduce Yourself «» Please Read the Rules »»[/c]
Please post your images here.
Please see this thread before posting images; posting images demonstrates your agreement with
the possible uses for your image.
If hotlinking to an image, please ensure it is under 400K.
Hotlinks to images over 400K slow down the thread too much and will be disabled.
Thank you!
_________________________________________________________________________________________________
<- Previous submissions
[c]«« Discuss Anything in Astronomy «» Visit The Asterisk Main Page «» See Introductory Astonomy Lectures »»
«« Introduce Yourself «» Please Read the Rules »»[/c]
A closed mouth gathers no foot.
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NGC7822 in Ha, OIII, NII & SII
http://andersson-design.s3.amazonaws.co ... 048_v1.jpg
[attachment=0]7822.jpg[/attachment]
TEC140 at f/7 plus an FLI ML16803 camera. Astrodon 3nm narrowband filters.
Ha = 8 x 1500 secs
OIII, NII & SII = 18 x 1500 secs
R, G & B = 8 x 200 secs
Bob.
[attachment=0]7822.jpg[/attachment]
- NGC7822
TEC140 at f/7 plus an FLI ML16803 camera. Astrodon 3nm narrowband filters.
Ha = 8 x 1500 secs
OIII, NII & SII = 18 x 1500 secs
R, G & B = 8 x 200 secs
Bob.
Last edited by owlice on Mon Sep 02, 2013 8:34 am, edited 1 time in total.
Reason: Attached smaller image for faster downloading; left link to larger image. Please keep hotlinked images under 400K. Thanks for sharing!
Reason: Attached smaller image for faster downloading; left link to larger image. Please keep hotlinked images under 400K. Thanks for sharing!
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Re: Submissions: 2013 September
Lightning, The Milky Way and the lake.
Cochiti Lake. Central New Mexico
Nikon D600 Samyang 14mm f/2.8
15 second exposure at ISO3200
http://www.facebook.com/bspencerphoto
http://www.brianspencer.com/mwlake.jpg
[attachment=0]bspencer.jpg[/attachment]
Cochiti Lake. Central New Mexico
Nikon D600 Samyang 14mm f/2.8
15 second exposure at ISO3200
http://www.facebook.com/bspencerphoto
http://www.brianspencer.com/mwlake.jpg
[attachment=0]bspencer.jpg[/attachment]
Last edited by owlice on Mon Sep 02, 2013 7:54 pm, edited 1 time in total.
Reason: Attached smaller image for faster downloading; left link to larger image. Thanks for sharing!
Reason: Attached smaller image for faster downloading; left link to larger image. Thanks for sharing!
Re: Submissions: 2013 September
http://www.abrelosojos.nl
WeBo 1 - Planetary Nebula in Cassiopeia
Copyright: Andre van Zegveld (Severe crop)
WeBo 1
Planetary Nebula in Cassiopeia (The small blue oval in quadrant below left)
The small, OIII rich planetary nebula WeBo 1 (PN G135.6+01.0), is an elongated blue oval near the "V" of the heart nebula.
Visibility is greatly enhanced by the OIII filter. This has been called a Barium Star surrounded by a young planetary nebula.
Discovered by Webbink and Bond, It is morphologically extremely similar to SuWt 2, in being an almost mathematically perfect ellipse. Recent observations at KPNO reveal that its central star is also a close binary, with a sinusoidal light curve and a period of approximately 5 days.
30 hours on TEC-140 + Astrodon 3nm Ha, SII, OIII filters
Full size image: http://www.abrelosojos.nl/gallery/nebul ... t-full.jpg
WeBo 1 - Planetary Nebula in Cassiopeia
Copyright: Andre van Zegveld (Severe crop)
WeBo 1
Planetary Nebula in Cassiopeia (The small blue oval in quadrant below left)
The small, OIII rich planetary nebula WeBo 1 (PN G135.6+01.0), is an elongated blue oval near the "V" of the heart nebula.
Visibility is greatly enhanced by the OIII filter. This has been called a Barium Star surrounded by a young planetary nebula.
Discovered by Webbink and Bond, It is morphologically extremely similar to SuWt 2, in being an almost mathematically perfect ellipse. Recent observations at KPNO reveal that its central star is also a close binary, with a sinusoidal light curve and a period of approximately 5 days.
30 hours on TEC-140 + Astrodon 3nm Ha, SII, OIII filters
Full size image: http://www.abrelosojos.nl/gallery/nebul ... t-full.jpg
Re: Submissions: 2013 September
NGC 6902 / NGC 6902B / IC 4946 - Galaxy Group in Sagittarius
http://www.rolfolsenastrophotography.com
Copyright: Rolf Wahl Olsen Link to large image
In the far south-eastern corner of Sagittarius, a constellation otherwise known for its spectacular highlights near the crowded Milky Way centre, lies the very rarely imaged galaxy NGC 6902 and a couple of its neighbours. Despite its beautiful and elegant appearance there is very little information about this galaxy to be found anywhere.
It contains a bright central ring and possibly also an elusive inner bar. The spiral arms are quite faint despite almost 17 hours of exposure, which is indicative of a rather weak population of O type stars. The arms also have a knotted appearance, perhaps due to the presence of brighter HII regions located within them.
The galaxy lies approximately 33 million light years away and was discovered by John Herschel.
A number of other galaxies can be seen scattered across the field of view, including the smaller face-on spiral NGC 6902B to the upper left. At the top of the frame lies edge-on galaxy IC 4649 with some traces of obscuring dust and a hint of a bar structure surrounding its core.
And far in the background countless distant galaxy groupings can be seen as small fuzzy yellowish dots throughout the image.
Image details:
Date: 29th July, 5th, 6th, 7th, 8th and 9th August 2013
Exposure: LRGB: 645:152:122:93 mins, total 16 hours 52 mins @ -30C
Telescope: 10" Serrurier Truss Newtonian f/5
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from my observatory in Auckland, New Zealand
http://www.rolfolsenastrophotography.com
Copyright: Rolf Wahl Olsen Link to large image
In the far south-eastern corner of Sagittarius, a constellation otherwise known for its spectacular highlights near the crowded Milky Way centre, lies the very rarely imaged galaxy NGC 6902 and a couple of its neighbours. Despite its beautiful and elegant appearance there is very little information about this galaxy to be found anywhere.
It contains a bright central ring and possibly also an elusive inner bar. The spiral arms are quite faint despite almost 17 hours of exposure, which is indicative of a rather weak population of O type stars. The arms also have a knotted appearance, perhaps due to the presence of brighter HII regions located within them.
The galaxy lies approximately 33 million light years away and was discovered by John Herschel.
A number of other galaxies can be seen scattered across the field of view, including the smaller face-on spiral NGC 6902B to the upper left. At the top of the frame lies edge-on galaxy IC 4649 with some traces of obscuring dust and a hint of a bar structure surrounding its core.
And far in the background countless distant galaxy groupings can be seen as small fuzzy yellowish dots throughout the image.
Image details:
Date: 29th July, 5th, 6th, 7th, 8th and 9th August 2013
Exposure: LRGB: 645:152:122:93 mins, total 16 hours 52 mins @ -30C
Telescope: 10" Serrurier Truss Newtonian f/5
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from my observatory in Auckland, New Zealand
Re: Submissions: 2013 September
RS Puppis
http://www.flickr.com/photos/stephen63/ ... otostream/
RS Puppis (or RS Pup) is a Cepheid variable star in the constellation of Puppis.
Because it is located in a large nebula, astronomers using the ESO’s New Technology Telescope at La Silla Observatory, Chile have been able to measure its distance by strictly geometric analysis of light echos from particles in the nebula, determining it to be 6500 ± 90 light years from Earth, the most accurate measurement achieved for any Cepheid as of early 2008-Wiki
Hubble Legacy Archive Data set:
ACS/WFC 435W/606W Single exposure
Synthetic Green
http://www.flickr.com/photos/stephen63/ ... otostream/
RS Puppis (or RS Pup) is a Cepheid variable star in the constellation of Puppis.
Because it is located in a large nebula, astronomers using the ESO’s New Technology Telescope at La Silla Observatory, Chile have been able to measure its distance by strictly geometric analysis of light echos from particles in the nebula, determining it to be 6500 ± 90 light years from Earth, the most accurate measurement achieved for any Cepheid as of early 2008-Wiki
Hubble Legacy Archive Data set:
ACS/WFC 435W/606W Single exposure
Synthetic Green
Last edited by stephen63 on Mon Sep 02, 2013 7:48 pm, edited 1 time in total.
Re: Submissions: 2013 September
NGC 6357 & Pismis 24 in Scorpius
http://www.astropilar.com.ar/nebulosas/NGC6357_1.html
Copyright: Ezequiel Bellocchio Best regards,
Ezequiel.
http://www.astropilar.com.ar/nebulosas/NGC6357_1.html
Copyright: Ezequiel Bellocchio Best regards,
Ezequiel.
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Re: Submissions: 2013 September
Bright Green Meteor - I caught this on 9-1 while shooting timelapse. I also caught it on a second camera with a 14mm wide angle lens.
http://www.facebook.com/dakotalapse
http://www.facebook.com/dakotalapse
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Re: Submissions: 2013 September
Soap bubble nebula - PN G75.5+1.7
http://www.stefanofocosi.altervista.org ... _2013.html
Copyright: Stefano Focosi
http://www.stefanofocosi.altervista.org ... _2013.html
Copyright: Stefano Focosi
Re: Submissions: 2013 September
Last edited by orion69 on Tue Sep 03, 2013 1:22 pm, edited 1 time in total.
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Re: Submissions: 2013 September
M27 - The Dumbbell Nebula in Vulpecula
Hybrid Composition of Natural Colours (LRGB) and Narrow Bands (SII-Ha-OIII) of M27. This mix of different spectral contributions allows a better perception and visibility of the nebula's details and of its gases distribution.
Authors: M.Angelini - F.Antonucci - F.Tagliani ADARA-ASTROBRALLO
http://www.astrobrallo.com
Image details: http://www.astrobrallo.com/gallery/inde ... N-Finale-M
Full-Res: http://www.astrobrallo.com/gallery/var/ ... 1378161523
Hybrid Composition of Natural Colours (LRGB) and Narrow Bands (SII-Ha-OIII) of M27. This mix of different spectral contributions allows a better perception and visibility of the nebula's details and of its gases distribution.
Authors: M.Angelini - F.Antonucci - F.Tagliani ADARA-ASTROBRALLO
http://www.astrobrallo.com
Image details: http://www.astrobrallo.com/gallery/inde ... N-Finale-M
Full-Res: http://www.astrobrallo.com/gallery/var/ ... 1378161523
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Re: Submissions: 2013 September
NGC 6992 - The Eastern Part of the Cygnus Loop
Hybrid Composition of the Eastern Part of the Veil Nebula, a beautiful supernova remnant in the Cygnus constellation
Authors: F.Antonucci - M.Angelini - F.Tagliani ADARA ASTROBRALLO
http://www.astrobrallo.com
Image Details: http://www.astrobrallo.com/gallery/inde ... /S2HaO3-14
Full-Res: http://www.astrobrallo.com/gallery/var/ ... 1378161523
Hybrid Composition of the Eastern Part of the Veil Nebula, a beautiful supernova remnant in the Cygnus constellation
Authors: F.Antonucci - M.Angelini - F.Tagliani ADARA ASTROBRALLO
http://www.astrobrallo.com
Image Details: http://www.astrobrallo.com/gallery/inde ... /S2HaO3-14
Full-Res: http://www.astrobrallo.com/gallery/var/ ... 1378161523
Re: Submissions: 2013 Sept
Subject: IC5146 Cocoon Nebula (LRGB image)
Copyrights: James Collins
Larger image URL http://jimstar11.com/IC5146cc.jpg
Web Site: Meadow View Observatory
http://jimstar11.com/
Copyrights: James Collins
Larger image URL http://jimstar11.com/IC5146cc.jpg
Web Site: Meadow View Observatory
http://jimstar11.com/
Re: Submissions: 2013 September
NGC 2070 (30 Doradus, The Tarantula Nebula) in Dorado
http://www.irida-observatory.org
Copyright: [url=mailto://info@irida-observatory.org]Velimir Popov, Emil Ivanov[/url]
The Tarantula Nebula (also known as 30 Doradus, or NGC 2070) is an H II region in the Large Magellanic Cloud (LMC). The Tarantula Nebula has an apparent magnitude of 8. Considering its distance of about 49 kpc (160 000 light years), this is an extremely luminous non-stellar object. Its luminosity is so great that if it were as close to Earth as the Orion Nebula, the Tarantula Nebula would cast shadows. In fact, it is the most active starburst region known in the Local Group of galaxies. It is also the largest such region in the Local Group with an estimated diameter of 200 pc. The nebula resides on the leading edge of the LMC, where ram pressure stripping, and the compression of the interstellar medium likely resulting from this, is at a maximum. At its core lies the compact star cluster R136 (approximate diameter 35 light years) that produces most of the energy that makes the nebula visible. The estimated mass of the cluster is 450 000 solar masses, suggesting it will likely become a globular cluster in the future.
The images was taken in Namibia on May 2013 during our Southern Sky expedition.
NGC 2070 - HaLRGB: Annotated image: Mousehover image NGC 2070 - Ha: Higher resolution, and more images and information is avaliable NGC 2070 ...
Thank you for looking ...
http://www.irida-observatory.org
Copyright: [url=mailto://info@irida-observatory.org]Velimir Popov, Emil Ivanov[/url]
http://www.irida-observatory.org
Copyright: [url=mailto://info@irida-observatory.org]Velimir Popov, Emil Ivanov[/url]
The Tarantula Nebula (also known as 30 Doradus, or NGC 2070) is an H II region in the Large Magellanic Cloud (LMC). The Tarantula Nebula has an apparent magnitude of 8. Considering its distance of about 49 kpc (160 000 light years), this is an extremely luminous non-stellar object. Its luminosity is so great that if it were as close to Earth as the Orion Nebula, the Tarantula Nebula would cast shadows. In fact, it is the most active starburst region known in the Local Group of galaxies. It is also the largest such region in the Local Group with an estimated diameter of 200 pc. The nebula resides on the leading edge of the LMC, where ram pressure stripping, and the compression of the interstellar medium likely resulting from this, is at a maximum. At its core lies the compact star cluster R136 (approximate diameter 35 light years) that produces most of the energy that makes the nebula visible. The estimated mass of the cluster is 450 000 solar masses, suggesting it will likely become a globular cluster in the future.
The images was taken in Namibia on May 2013 during our Southern Sky expedition.
NGC 2070 - HaLRGB: Annotated image: Mousehover image NGC 2070 - Ha: Higher resolution, and more images and information is avaliable NGC 2070 ...
Thank you for looking ...
http://www.irida-observatory.org
Copyright: [url=mailto://info@irida-observatory.org]Velimir Popov, Emil Ivanov[/url]
Re: Submissions: 2013 September
Starry cloudy night over urban light
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Re: Submissions: 2013 September
Wow it's rare to see a closeup of this planetary nebula that was discovered in 1996! It is visible in many widefields of the Heart Nebula.Zegveld wrote:http://www.abrelosojos.nl
WeBo 1 - Planetary Nebula in Cassiopeia
Copyright: Andre van Zegveld
http://www.abrelosojos.nl/gallery/nebul ... Nebula.jpg
(Severe crop)
WeBo 1
Planetary Nebula in Cassiopeia (The small blue oval in quadrant below left)
The small, OIII rich planetary nebula WeBo 1 (PN G135.6+01.0), is an elongated blue oval near the "V" of the heart nebula.
Visibility is greatly enhanced by the OIII filter. This has been called a Barium Star surrounded by a young planetary nebula.
Discovered by Webbink and Bond, It is morphologically extremely similar to SuWt 2, in being an almost mathematically perfect ellipse. Recent observations at KPNO reveal that its central star is also a close binary, with a sinusoidal light curve and a period of approximately 5 days.
30 hours on TEC-140 + Astrodon 3nm Ha, SII, OIII filters
Full size image: http://www.abrelosojos.nl/gallery/nebul ... t-full.jpg
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- Posts: 5409
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Re: Submissions: 2013 September
Amazing image of an equally amazing galaxy! I don't know how there was never an AAO image of this one. Sagittarius has everything, it is home to cometary globules, a Wolf Rayet nebula, a few supernova remnants as well as ultra obscure globular clusters. More to it then the common stuff.SkyViking wrote:NGC 6902 / NGC 6902B / IC 4946 - Galaxy Group in Sagittarius
http://www.rolfolsenastrophotography.com
Copyright: Rolf Wahl Olsen
http://www.rolfolsenastrophotography.co ... 454-X2.jpg
Link to large image
In the far south-eastern corner of Sagittarius, a constellation otherwise known for its spectacular highlights near the crowded Milky Way centre, lies the very rarely imaged galaxy NGC 6902 and a couple of its neighbours. Despite its beautiful and elegant appearance there is very little information about this galaxy to be found anywhere.
It contains a bright central ring and possibly also an elusive inner bar. The spiral arms are quite faint despite almost 17 hours of exposure, which is indicative of a rather weak population of O type stars. The arms also have a knotted appearance, perhaps due to the presence of brighter HII regions located within them.
The galaxy lies approximately 33 million light years away and was discovered by John Herschel.
A number of other galaxies can be seen scattered across the field of view, including the smaller face-on spiral NGC 6902B to the upper left. At the top of the frame lies edge-on galaxy IC 4649 with some traces of obscuring dust and a hint of a bar structure surrounding its core.
And far in the background countless distant galaxy groupings can be seen as small fuzzy yellowish dots throughout the image.
Image details:
Date: 29th July, 5th, 6th, 7th, 8th and 9th August 2013
Exposure: LRGB: 645:152:122:93 mins, total 16 hours 52 mins @ -30C
Telescope: 10" Serrurier Truss Newtonian f/5
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from my observatory in Auckland, New Zealand
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Re: Submissions: 2013 September
Wow that looks epic!! The nebula is also catalogued as vdBH6, the only reflection nebula associated with a Cepheid variable. Lots of many interesting deep sky objects in the southern sky.stephen63 wrote:RS Puppis
http://www.flickr.com/photos/stephen63/ ... otostream/
RS Puppis (or RS Pup) is a Cepheid variable star in the constellation of Puppis.
Because it is located in a large nebula, astronomers using the ESO’s New Technology Telescope at La Silla Observatory, Chile have been able to measure its distance by strictly geometric analysis of light echos from particles in the nebula, determining it to be 6500 ± 90 light years from Earth, the most accurate measurement achieved for any Cepheid as of early 2008-Wiki
Hubble Legacy Archive Data set:
ACS/WFC 435W/606W Single exposure
Synthetic Green
http://farm4.staticflickr.com/3778/9642 ... e859_b.jpg
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Re: Submissions: 2013 September
That is an excellent image of a very strange nebula, it also has lots of OIII emission.elettrorider wrote:Soap bubble nebula - PN G75.5+1.7
http://www.stefanofocosi.altervista.org ... _2013.html
Copyright: Stefano Focosi
http://stefanofocosi.altervista.org/ast ... ap400K.jpg
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Re: Submissions: 2013 September
Although this region has been imaged to death, I never tire of seeing this crazy complex of nebulae and clusters all entangled together.ViliMax wrote:NGC 2070 (30 Doradus, The Tarantula Nebula) in Dorado
http://www.irida-observatory.org
Copyright: [url=mailto://info@irida-observatory.org]Velimir Popov, Emil Ivanov[/url]
The Tarantula Nebula (also known as 30 Doradus, or NGC 2070) is an H II region in the Large Magellanic Cloud (LMC). The Tarantula Nebula has an apparent magnitude of 8. Considering its distance of about 49 kpc (160 000 light years), this is an extremely luminous non-stellar object. Its luminosity is so great that if it were as close to Earth as the Orion Nebula, the Tarantula Nebula would cast shadows. In fact, it is the most active starburst region known in the Local Group of galaxies. It is also the largest such region in the Local Group with an estimated diameter of 200 pc. The nebula resides on the leading edge of the LMC, where ram pressure stripping, and the compression of the interstellar medium likely resulting from this, is at a maximum. At its core lies the compact star cluster R136 (approximate diameter 35 light years) that produces most of the energy that makes the nebula visible. The estimated mass of the cluster is 450 000 solar masses, suggesting it will likely become a globular cluster in the future.
The images was taken in Namibia on May 2013 during our Southern Sky expedition.
NGC 2070 - HaLRGB:
http://www.irida-observatory.org/Namibi ... terisk.jpg
Annotated image:
http://www.irida-observatory.org/Namibi ... terisk.jpg
Mousehover image
http://www.irida-observatory.org/Namibi ... terisk.jpg
http://www.irida-observatory.org/Namibi ... terisk.jpg
NGC 2070 - Ha:
http://www.irida-observatory.org/Namibi ... terisk.jpg
Higher resolution, and more images and information is avaliable NGC 2070 ...
Thank you for looking ...
http://www.irida-observatory.org
Copyright: [url=mailto://info@irida-observatory.org]Velimir Popov, Emil Ivanov[/url]
Re: Submissions: 2013 September
Animation Nova Delphinus 2013
17 August - 2 September
We see the decline of the band Blue August 17 to September 2 in that it almost disappeared and there is only the red and infrared
Data capture and large size
http://www.astromodelismo.es/Web%20Astr ... /index.htm
Copyright: Máximo Ruiz
http://www.astromodelismo.es/index.htm
17 August - 2 September
We see the decline of the band Blue August 17 to September 2 in that it almost disappeared and there is only the red and infrared
Data capture and large size
http://www.astromodelismo.es/Web%20Astr ... /index.htm
Copyright: Máximo Ruiz
http://www.astromodelismo.es/index.htm
- geckzilla
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Re: Submissions: 2013 September
Cross-posting a batch of the better ones I've submitted at Flickr recently. More information on individual works is available at the Flickr page by clicking on them.
NGC 1999
Credit: Hubble Legacy Archive, processing by Judy Schmidt
NGC 1999 by geckzilla, on Flickr
Transforming Galaxy
Credit: Hubble Legacy Archive, processing by Judy Schmidt
Transforming Galaxy Redo by geckzilla, on Flickr
Blinking Eye Nebula
Credit: Hubble Legacy Archive, processing by Judy Schmidt
Blinking Eye Nebula by geckzilla, on Flickr
NGC 1999
Credit: Hubble Legacy Archive, processing by Judy Schmidt
NGC 1999 by geckzilla, on Flickr
Transforming Galaxy
Credit: Hubble Legacy Archive, processing by Judy Schmidt
Transforming Galaxy Redo by geckzilla, on Flickr
Blinking Eye Nebula
Credit: Hubble Legacy Archive, processing by Judy Schmidt
Blinking Eye Nebula by geckzilla, on Flickr
Just call me "geck" because "zilla" is like a last name.