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Lionel Messi (FC Barcelona), Mikel Balenziaga (Athletic Club) and Luis Enrique Martínez García(FC Barcelona manager) during the Spanish La Liga match at Camp Nou, Barcelona, Spain, on 13 Sep 2014..................................................................... Final Score - Barcelona(2) : Athletic(0)

This image by Jeff S. PhotoArt is licensed under a Creative Commons Attribution-NonCommercial-NoDerivs 4.0 International License

 

Check out my website: my photos on canvas

 

Feel free to use this image on your blog, for fun and the like but you must:

1. Link the image to Flickr.

2. Give credit to: Jeff S. PhotoArt at HDCanvas.ca.

 

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Photo Inquiry: Click here ................ Buy Art At: FineArtAmerica

 

The Muskegon South Pierhead Light is a steel tapered cylindrical tower located at the west end of the south pier at the entry channel that connects Muskegon Lake with Lake Michigan. The light tower was constructed in 1903 and remains an active navigational light. .

     

On the fringes of an Irish bog. Reptile tongues?

going to be a very weird Christmas this year

 

arachtober 27

Gallileo Tower - Frankfurt am Main, Germany 2015... Gallileo is a 38-storey 136m/446 ft skyscraper in the Bahnhofsviertel district of Frankfurt, currently being used by Commerzbank.

Believed to be in Public Domain From Library of Congress, Prints and Photographs Collections. More on copyright: What does "no known restrictions" mean?

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For information from Creative Commons on proper licensing for images believed to already be in the public domain please-- click here. By using this image from this site, you are acknowledging that you have read all the information in this description and accept responsibility for any use by you or your representatives. You are accepting responsibility for conducting any additional due diligence that may be necessary to ensure your proper use of this image.

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Based on information from the source, this image is believe to be in the public domain. It is up to the user to make their own determination. Additional information is provided below, usually the entire online file, to assist you in doing so. Public domain images SHOULD NOT BE ATTRIBUTED TO PINGNEWS. Please attribute the repository and the originator. If you can add "via pingnews" or a link back to this site it is appreciated. While it may appear with this image, the attribution license does not apply to pingnews in this instance as we are neither the creator of nor the archive for this work.

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Public Domain. Additional source description and credit info from the Library of Congress:

 

TITLE: The war of wealth

 

CALL NUMBER: POS - TH - 1895 .W37, no. 1 (C size) [P&P]

 

REPRODUCTION NUMBER: LC-USZC4-591 (color film copy transparency)

LC-USZ6-380 (b&w film copy neg.)

 

RIGHTS INFORMATION: No known restrictions on publication.

 

MEDIUM: 1 print (poster) : lithograph, color ; 77 x 102 cm.

 

CREATED/PUBLISHED: Cin'ti ; N.Y. : Strobridge Lith. Co., c1895.

 

CREATOR:

 

Strobridge & Co. Lith.

 

RELATED NAMES:

 

Litt, Jacob.

Dazey, Charles Turner, 1855-1938.

 

NOTES:

 

Created and "copyright 1895 by The Strobridge Lith Co, Cin'ti. -- N.Y."

 

Jacob Litt, proprietor.

 

By C.T. Dazey, author of In old Kentucky.

 

Caption: The run on the bank : a crisis in the affairs of the great financial institution. The most animated and realistic scene ever shown on the stage.

 

N.Y. 6312.

 

SUBJECTS:

 

Business panics.

Banks.

Crowds.

Melodramas.

 

FORMAT:

 

Theatrical posters American.

Lithographs Color.

 

PART OF: Theatrical Poster Collection (Library of Congress)

 

REPOSITORY: Library of Congress Prints and Photographs Division Washington, D.C. 20540 USA

 

DIGITAL ID: (digital file from intermediary roll copy film) var 0760 hdl.loc.gov/loc.pnp/var.0760

 

CONTROL #: var1994000815/PP

Olympus XA-2

Expired Store Brand 400 Film

Canoscan 8400f

   

West Coast National Park

Pallas-Athene-Brunnen/Athena Fountain - Austrian Parliament, Vienna, Austria 2014..... At the entrance of Austrian Parliament building, is the 5,5 m high statue of Pallas Athene which stands in the middle of a large fountain. The sculptor Carl Kundmann created the statue according to the plans from architect Hansen.

The goddess of wisdom Pallas Athene holds in her right hand a small figure of Nike the goddess of victory and in her left hand a spear. www.city-walks.info/Vienna/Parliament.html

Desperately wishing I had cold feet right now, or even to get a cold shoulder would be nice. It's been over a week since my escape to the cold, and it's been too long.

make you wonder if aliens are in control of our shampoo

Just in time for the festive season, this new Picture of the Week from the NASA/ESA Hubble Space Telescope features a glistening scene in holiday red. This image shows a small region of the well-known nebula Westerhout 5, which lies about 7000 light-years from Earth. Suffused with bright red light, this luminous image hosts a variety of interesting features, including a free-floating Evaporating Gaseous Globule (frEGG). The frEGG in this image is the small tadpole-shaped dark region in the upper centre-left. This buoyant-looking bubble is lumbered with two rather uninspiring names — [KAG2008] globule 13 and J025838.6+604259.

 

FrEGGs are a particular class of Evaporating Gaseous Globules (EGGs). Both frEGGs and EGGs are regions of gas that are sufficiently dense that they photoevaporate less easily than the less compact gas surrounding them. Photoevaporation occurs when gas is ionised and dispersed away by an intense source of radiation — typically young, hot stars releasing vast amounts of ultraviolet light. EGGs were only identified fairly recently, most notably at the tips of the Pillars of Creation, which were captured by Hubble in iconic images released in 1995. FrEGGs were classified even more recently, and are distinguished from EGGs by being detached and having a distinct ‘head-tail’ shape. FrEGGs and EGGs are of particular interest because their density makes it more difficult for intense UV radiation, found in regions rich in young stars, to penetrate them. Their relative opacity means that the gas within them is protected from ionisation and photoevaporation. This is thought to be important for the formation of protostars, and it is predicted that many FrEGGs and EGGs will play host to the birth of new stars.

 

The frEGG in this image is a dark spot in the sea of red light. The red colour is caused by a particular type of light emission known as H-alpha emission. This occurs when a very energetic electron within a hydrogen atom loses a set amount of its energy, causing the electron to become less energetic and this distinctive red light to be released.

 

[Image description: The background is filled with bright orange-red clouds of varying density. Towards the top-left several large, pale blue stars with prominent cross-shaped spikes are scattered. A small, tadpole-shaped dark patch floats near one of these stars. More of the same dark, dense gas fills the lower-right, resembling black smoke. A bright yellow star and a smaller blue star shine in front of this.]

 

Credits: ESA/Hubble & NASA, R. Sahai; CC BY 4.0

 

All rights reserved - Tous droits réservés

   

Christine Lebrasseur - Photographe

 

French Website / Site en français

 

Christine Lebrasseur Photo Studio

  

DNA - Ipernity - YouTube - JPGMag - Facebook

 

Ce sont les mots qui existent, ce qui n'a pas de nom n'existe pas. Le mot lumière existe, la lumière n'existe pas.

 

[Francis Picabia] - Peintre et écrivain français

 

The words really exist, which does not have a name does not exist. The word light exists, the light does not exist.

 

Approximative translation

Så er der Kronhjort...

 

Roaring Stag in Dyrehaven

The subject of this image is a group of three galaxies, collectively known as NGC 7764A. They were imaged by the NASA/ESA Hubble Space Telescope, using both its Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). The two galaxies in the upper right of the image appear to be interacting with one another — indeed, the long trails of stars and gas extending from them both give the impression that they have both just been struck at great speed, thrown into disarray by the bowling-ball-shaped galaxy to the lower left of the image. In reality, however, interactions between galaxies happen over very long time periods, and galaxies rarely collide head-on with one another. It is also unclear whether the galaxy to the lower left is actually interacting with the other two, although they are so relatively close in space that it seems possible that they are. By happy coincidence, the collective interaction between these galaxies have caused the two on the upper right to form a shape, which from our Solar System's perspective, ressembles the starship known as the USS Enterprise from Star Trek!

 

NGC 7764A, which lies about 425 million light years from Earth in the constellation Phoenix, is a fascinating example of just how awkward astronomical nomenclature can be. The three galaxies are individually referred to as NGC 7764A1, NGC 7764A2 and NGC 7764A3, and just to be really difficult, an entirely separate galaxy, named NGC 7764, sits in the skies about a Moon’s distance (as seen from Earth) away. This rather haphazard naming makes more sense when we consider that many of the catalogues for keeping track of celestial bodies were compiled well over 100 years ago, long before modern technology made standardising scientific terminology much easier. As it is, many astronomical objects have several different names, or might have names that are so similar to other objects’ names that they cause confusion.

 

Credits: ESA/Hubble & NASA, J. Dalcanton, Dark Energy Survey, DOE, FNAL, DECam, CTIO, NOIRLab/NSF/AURA, ESO; CC BY 4.0

Acknowledgement: J. Schmidt

Bleu ciel, bleu marine. C’est cette couleur qui va à la Bretagne comme un gant, qui s’associe à elle si naturellement que la question ne se pose même pas.

Je vous laisse regarder ce bleu qui se marie à merveille avec la pierre bretonne.

 

www.breizh-info.com/2015/08/22/30157/le-bleu-bretagne-un-...

 

Merci pour vos visites et vos commentaires.

Ce(tte) œuvre est mise à disposition selon les termes de la Licence Creative Commons Attribution 4.0 International.

Crunchy wouldn't let me use the bathroom sink, much to my amusement.

Rather than shoo her off, I took out my carry along pocket camera and shot a series of her modeling in the sink. 😸📷

 

Here we see JO204, a ‘jellyfish galaxy’ so named for the bright tendrils of gas that appear in this image to be drifting lazily below JO204’s bright central bulk. The galaxy lies almost 600 million light-years away in the constellation Sextans. This image was captured by the NASA/ESA Hubble Space Telescope, and it is the third of a series of Pictures of the Week featuring jellyfish galaxies. This series of images is possible thanks to a survey in which observations were made of six of these fascinating galaxies, including JO204. This survey was performed with the intention of better understanding star formation under extreme conditions.

 

Given the dreamy appearance of this image, it would be understandable to wonder why jellyfish galaxies should be such a crucible for star formation. The answer is that — as is often the case with astronomy — first appearances can be deceiving. Whilst the delicate ribbons of gas beneath JO204 may look like floating jellyfish tentacles, they are in fact the outcome of an intense astronomical process known as ram pressure stripping.

 

Ram pressure is a particular type of pressure exerted on a body when it moves relative to a fluid. An intuitive example is the sensation of pressure you experience when you are standing in an intense gust of wind — the wind is a moving fluid, and your body feels pressure from it. An extension of this analogy is that your body will remain whole and coherent, but the more loosely bound things — like your hair and your clothes — will flap in the wind. The same is true for jellyfish galaxies. They experience ram pressure because of their movement against the intergalactic medium that fills the spaces between galaxies in a galaxy cluster. The galaxies experience intense pressure from that movement, and as a result their more loosely bound gas is stripped away. This gas is mostly the colder and denser gas in the galaxy — gas which, when stirred and compressed by the ram pressure, collapses and forms new stars in the jellyfish’s beautiful tendrils.

 

[Image Description: A spiral galaxy in the centre is tilted almost edge-on. The bright core and spiral arms can just be seen from the top. A slight glow surrounds it. Below, strands made of bright blue patches trail down like tentacles. On the left it is just touched by a second, faint and dim galaxy. The background is very dark, with only a few other stars and tiny galaxies visible.]

 

Credits: ESA/Hubble & NASA, M. Gullieuszik and the GASP team; CC BY 4.0

 

The mass of dust and bright swirls of stars in this image are the distant galaxy merger IC 2431, which lies 681 million light-years from Earth in the constellation Cancer. The NASA/ESA Hubble Space Telescope has captured what appears to be a triple galaxy merger in progress, as well as a tumultuous mixture of star formation and tidal distortions caused by the gravitational interactions of this galactic trio. The centre of this image is obscured by a thick cloud of dust — though light from a background galaxy can be seen piercing its outer extremities.

 

This image is from a series of Hubble observations investigating weird and wonderful galaxies found by the Galaxy Zoo citizen science project. Using Hubble’s powerful Advanced Camera for Surveys (ACS), astronomers took a closer look at some of the more unusual galaxies that volunteers had identified. The original Galaxy Zoo project was the largest galaxy census ever carried out, and relied on crowdsourcing time from more than 100 000 volunteers to classify 900 000 unexamined galaxies. The project achieved what would have been years of work for a professional astronomer in only 175 days, and has led to a steady stream of similar astronomical citizen science projects. Later Galaxy Zoo projects have included the largest ever studies of galaxy mergers and tidal dwarf galaxies, as well as the discovery of entirely new types of compact star-forming galaxies.

 

Credits: ESA/Hubble & NASA, W. Keel, Dark Energy Survey, DOE, FNAL, DECam, CTIO, NOIRLab/NSF/AURA, SDSS; CC BY 4.0

Acknowledgement: J. Schmidt

A stream on the side of Mount Hood. From our trip in Oregon.

Arachtober 23rd

 

a tower of potential scatterscape pictures

 

Shonen Knife - Tower Of The Sun

www.youtube.com/watch?v=Xgcv9kP-nCI

Driving in the Driving rain, what else are you going to go with it? One of my favorite stretches of road that remains oddly quiet most days, even though it's just a couple of miles from the Golden Gate Bridge. Looking southwest towards New Zealand.

For Asteroid Day, the Copernicus Sentinel-2 mission takes us over the Shoemaker Impact Structure (formerly known as Teague Ring) in Western Australia.

 

Located around 100 km northeast of the small town Wiluna, the Shoemaker Impact Structure was renamed in honour of Eugene Shoemaker, a planetary geologist and pioneer in impact crater studies.

 

The almost circular shape of the Shoemaker impact site, visible in the bottom-right of the image, is approximately 30 km in diameter and is defined by concentric rings formed in sedimentary rocks (seen in dark brown). The precise age of the impact is unknown, but is estimated to be between 1000 and 600 million years ago – making it Australia’s oldest impact crater.

 

This false-colour image was processed by selecting spectral bands that can be used for classifying geological features, allowing us to clearly identify the concentric rings in the image. The light blue areas are saline and ephemeral lakes including Nabberu, Teague, Shoemaker and other smaller ponds.

 

Asteroid Day, the UN-endorsed global awareness campaign is back on 30 June with an exciting 5-hour live broadcast from 18:00 CET. With the help of leading experts, Asteroid Day Co-founder Dr. Brian May and the most engaging voices in science communications from around the world, the five hour programme will bring the solar system’s smallest worlds to vivid life for audiences of all ages and backgrounds. For more information, visit ESA joins Asteroid Day for rocky live broadcast.

 

Credits: contains modified Copernicus Sentinel data (2021), processed by ESA, CC BY-SA 3.0 IGO

 

Dodging buses which run fast to make time ...

This is a Blue Dasher, I think I read somewhere, the most common dragonfly in North America. They love slow moving water and so, no surprise they were in abundance on the bayous of Louisiana.

 

One for Macro Monday.

Stag roaring in the last rays of sunlight...

Traitement Façon Polaroid . . .

 

www.pcastuces.com/pratique/multimedia/polaroid/page2.htm

www.rollip.com/

 

Merci pour vos visites et vos commentaires.

Ce(tte) œuvre est mise à disposition selon les termes de la Licence Creative Commons Attribution 4.0 International.

As all the pictures in my gallery, this is a FREE picture. You can download it and do whatever you want with it: share it, adapt it and/or combine it with other material and distribute the resulting works.

 

I’d very much appreciate if you give photo credits to “Carlos ZGZ” when you use this picture. This would help me find it and add it to my photoset “Used elsewhere”.

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Como todas las imágenes de mi galería, esta es una imagen LIBRE. Puedes descargarla y hacer lo que quieras con ella: compartirla tal cual, modificarla y/o combinarla con otro material y distribuir el resultado.

 

Por favor, si utilizas esta imagen, dale el crédito a “Carlos ZGZ”. De esta manera podré encontrarla fácilmente y añadirla a mi álbum “Used elsewhere”.

Stables in Owens Valley, California.

This photo is licensed under a Creative Commons Attribution

Non-Commercial Share-Alike license.

For information on the license see this link.

 

The required attribution should read:

" Erica Marshall of muddyboots.org "

 

If you'd like information on using my photos commercially, see this link.

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