Fine Art Print : First photo of ultraheavy primary cosmic ray
Fine Art Prints from Science Photo Library
First photo of ultraheavy primary cosmic ray
First picture of an ultraheavy cosmic ray primary, compared with a cosmic ray iron nucleus. The tracks of both nuclei are recorded in photographic emulsion exposed during balloon flights high in the atmosphere over Texas in 1966. Iron has atomic number 26: it has 26 protons. The ultraheavy nucleus had about 90 protons - the number of thorium. The more protons in a nucleus, the greater its electric charge & its ability to ionise; the more it ionises, the denser the track it produces in emulsion. The wispy side-shoots are " delta rays" - electrons knocked out of atoms by the passage of the nuclei
Science Photo Library features Science and Medical images including photos and illustrations
Media ID 6284257
© PROFESSOR PETER FOWLER/SCIENCE PHOTO LIBRARY
Cosmic Ray Emulsion Photo High Energy Image Iron Nucleus Particle Physics Rays
20"x16" (+3" Border) Fine Art Print
Discover the awe-inspiring mysteries of the universe with Media Storehouse's Fine Art Prints. Feast your eyes on this breathtaking image of the first recorded evidence of an ultraheavy cosmic ray primary, captured by Science Photo Library. Witness the astonishing contrast between this elusive particle and a cosmic ray iron nucleus, both leaving their indelible marks on photographic emulsion during high-altitude balloon flights. Bring the wonders of science into your home or office with this stunning, museum-quality print.
20x16 image printed on 26x22 Fine Art Rag Paper with 3" (76mm) white border. Our Fine Art Prints are printed on 300gsm 100% acid free, PH neutral paper with archival properties. This printing method is used by museums and art collections to exhibit photographs and art reproductions.
Our fine art prints are high-quality prints made using a paper called Photo Rag. This 100% cotton rag fibre paper is known for its exceptional image sharpness, rich colors, and high level of detail, making it a popular choice for professional photographers and artists. Photo rag paper is our clear recommendation for a fine art paper print. If you can afford to spend more on a higher quality paper, then Photo Rag is our clear recommendation for a fine art paper print.
Estimated Image Size (if not cropped) is 40.6cm x 50.2cm (16" x 19.8")
Estimated Product Size is 55.9cm x 66cm (22" x 26")
These are individually made so all sizes are approximate
Artwork printed orientated as per the preview above, with portrait (vertical) orientation to match the source image.
EDITORS COMMENTS
This print captures a groundbreaking moment in particle physics - the first-ever image of an ultraheavy primary cosmic ray. The photograph showcases a remarkable comparison between the cosmic ray iron nucleus and this enigmatic ultraheavy nucleus. Taken during balloon flights high above the Texan atmosphere in 1966, both nuclei's tracks are meticulously recorded on photographic emulsion. Iron, with its atomic number 26 and 26 protons, serves as our reference point for understanding the sheer magnitude of this newly discovered ultraheavy nucleus. With approximately 90 protons - equivalent to thorium's atomic number - this mysterious entity possesses an astonishing electric charge and ionizing ability far beyond anything previously observed. The density of each track within the emulsion reveals fascinating insights into their behavior. As expected, the greater number of protons results in more intense ionization by the ultraheavy nucleus, leaving behind a dense track compared to that of iron. Delicately branching out from these tracks are wispy side-shoots known as "delta rays" which represent electrons dislodged from atoms due to the passage of these powerful nuclei. This extraordinary image not only sheds light on fundamental aspects of particle physics but also highlights humanity's relentless pursuit to unravel nature's deepest mysteries. Courtesy of Science Photo Library, it stands as a testament to scientific progress and serves as an inspiration for future discoveries yet to come.
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