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Inspired from
Ustad Rashid Khan singing Raag Desh [Nadaan Jiya Re Gum Gayo Re]
www.youtube.com/watch?NR=1&v=6sT3DJsUIzo&feature=...
Thank you, Val, for introducing me to such a wonderful music!
www.flickr.com/photos/ma85/6386099389/in/set-721576226493...
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A diary-like experiment of life-sized emaki scroll on 1350mmx30m Kent paper roll. Planning 1850mm a day. Acrylic and charcoal.
1350mmx30mのケント紙ロールによる等身大絵巻の日記的実験。
制作可能な日に、幅1850mm制作予定。アクリル絵具、木炭を使用。
Emaki
Beware!! I’m landing! Walking around my home through fields and gardens looking for some nice subjects for my macro photography studies.
Pretty much what I have to do cuz I have to raise my Social studies grade~Hw..Not my thing~ by the end of the quarter or I might not be allowed on the computer for a long time so yeah~
see the rest here www.laurencephilomene.com/blog/color-studies-lavender
and you can buy prints of this image here : society6.com/product/color-study-2-rne_print#1=45
:)
Another study in advance of working on a commission. The building has been demolished but I hope to add a small version of it to the reconstruction drawing I have been commissioned to make. It stood near the entrance of an extensive goods yard, some indication of which will be part of the work o am doing. Drawn with a Pentel P205 0.5mm pencil in an A4 sketchbook.
Excerpt from uwaterloo.ca:
Description of the District
St. Clair Boulevard Heritage Conservation District runs along St. Clair Boulevard between Delaware Avenue and Cumberland Avenue. The district consists of 38 residential properties.
Cultural Heritage Value of the District
The Heritage Conservation District Planning Background Study and Plan discuss the value of the district:
“The St. Clair Park survey, registered in 1911, was one of a number of residential surveys laid out in Hamilton’s east end just after the turn of the century, a boom period for residential construction throughout the City. The St. Clair Park Survey formed part of a middle to upper class residential area comprising a number of surveys, which extended from King Street East to the foot of the escarpment and from Wentworth Street South to Gage Park.
As was common practice in Hamilton at the time, the St. Clair Park Survey has building restrictions in the form of restrictive covenants registered on deed to the lots. Restrictions on the cost, construction and setback of the house account to a large extent for the cohesive character of St. Clair Boulevard’s urban streetscape.
While the restrictive covenants associated with the St. Clair Park Survey has building restrictions on its social make-up, the social composition of St. Clair Boulevard was nevertheless very homogenous, comprising middle to upper-middle income families of Anglo-Saxon origins. In the course of its history the boulevard has attracted some of Hamilton’s most prominent citizens; notably, he well-known and highly-respected judge, William F Schwenger and the successful construction company manager, Ralph W. Cooper. The Boulevard is also noteworthy for its social stability, owning to the long-term residence of most of the homeowners and
continuous use of the houses as single-family dwellings”.
Designation of the District
The designation of St. Clair Boulevard was initiated by local residents following the designation of the adjacent St. Clair Avenue district. According to the Background Study and Plan, “a petition requesting designation of the area...signed by all 37 homeowners, was presented to LACAC at its December meeting
and was supported by this committee”.
The St. Clair Boulevard Heritage Conservation District is protected by By-law 92-140, passed in 1992.
I love the colours of Boston Ivy in the fall, and Sunday while out and about it was no exception ... I took some time to do a photographic study of the vines clinging to some limestone walls and wooden trellis'.
blogged here: djenglandphotography.blogspot.ca/2017/10/photo-of-week-20...
A new image from the NASA/ESA/CSA James Webb Space Telescope reveals a remarkable cosmic sight: at least 17 concentric dust rings emanating from a pair of stars. Located just over 5000 light-years from Earth, the duo is collectively known as Wolf-Rayet 140. Each ring was created when the two stars came close together and their stellar winds (streams of gas they blow into space) met, compressing the gas and forming dust. The stars’ orbits bring them together about once every eight years; like the rings of a tree’s trunk, the dust loops mark the passage of time.
In addition to Webb’s overall sensitivity, its Mid-Infrared Instrument (MIRI) is uniquely qualified to study the dust rings. These rings are also called shells by astronomers because they are thicker and wider than they appear in the image. Webb’s science instruments detect infrared light, a range of wavelengths invisible to the human eye.
Contributed under both ESA and NASA leadership, Webb’s MIRI instrument detects the longest infrared wavelengths. This means that it can often see cooler objects – including the dust rings – than Webb’s other instruments can. MIRI’s spectrometer also revealed the composition of the dust, formed mostly from material ejected by a type of star known as a Wolf-Rayet star. A Wolf-Rayet star is born with at least 25 times more mass than our Sun and is nearing the end of its life, when it will likely explode as a supernova and then collapse into a black hole. Burning hotter than in its youth, a Wolf-Rayet star generates powerful winds that push huge amounts of gas into space. The Wolf-Rayet star in this particular pair may have shed more than half its original mass via this process.
Transforming gas into dust is somewhat like turning flour into bread. It requires specific conditions and ingredients. Hydrogen, the most common element found in stars, can’t form dust on its own. But because Wolf-Rayet stars shed so much mass, they also eject more complex elements typically found deep in a star’s interior, including carbon. The heavy elements in the wind cool as they travel into space and are then compressed where the winds from both stars meet, like when two hands knead dough.
Some other Wolf-Rayet systems form dust, but none is known to make rings like Wolf-Rayet 140 does. The unique ring pattern forms because the orbit of the Wolf-Rayet star in WR 140 is elongated, not circular. Only when the stars come close together – about the same distance between Earth and the Sun – and their winds collide is the gas under sufficient pressure to form dust. With circular orbits, Wolf-Rayet binaries can produce dust continuously.
The science team thinks WR 140’s winds also swept the surrounding area clear of residual material they might otherwise collide with, which may be why the rings remain so pristine rather than smeared or dispersed. There are likely even more rings that have become so faint and dispersed, not even Webb can see them in the data.
Wolf-Rayet stars may seem exotic compared to our Sun, but they may have played a role in star and planet formation. When a Wolf-Rayet star clears an area, the swept-up material can pile up at the outskirts and become dense enough for new stars to form. There is some evidence the Sun formed in such a scenario.
Using data from MIRI’s Medium Resolution Spectroscopy mode, the new study provides the best evidence yet that Wolf-Rayet stars produce carbon-rich dust molecules. What’s more, the preservation of the dust shells indicates that this dust can survive in the hostile environment between stars, going on to supply material for future stars and planets. The catch is that while astronomers estimate that there should be at least a few thousand Wolf-Rayet stars in our galaxy, only about 600 have been found to date.
These results have been published today in Nature Astronomy.
MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (the MIRI European Consortium) in partnership with JPL and the University of Arizona.
[Image Description: The background of this Webb image of star Wolf-Rayet 140 is black. A pair of bright stars dominates the centre of the image, with at least 17 pink-orange concentric dust rings emanating from them. Throughout the scene are a range of distant galaxies, the majority of which are very tiny and red, appearing as splotches.]
Credits: NASA/ESA/CSA/STScI/JPL-Caltech; CC BY 4.0
"Slow down and enjoy life.
It's not only the scenery you miss by going to fast -
you also miss the sense of where you are going and why."
-- Eddie Cantor --
a cobweb white with frost...
Photo published in 2010 as a New Year's message by Max Planck Institute for the Study of Societies in Cologne, a research institution in social sciences.