Sunday, April 24, 2022
Mythical Gardens - Adam & Eve in The Garden of Eden at Creation - Illuminated Manuscripts
Saturday, April 23, 2022
Spring 2022 at Longwood Gardens in Pennsylvania
Mythical Gardens - The Garden of Eden at Creation - Illuminated Manuscripts
Friday, April 22, 2022
17C Woman Holding A Fan by Abraham Bosse (French, c 1602-04–1676)
Mythical Gardens - The Garden of Eden at Creation - Illuminated Manuscripts
Genesis, The Creation of the Animals. Oxford MS. Douce 135 fol-017v Here the garden is filled with trees & birds.
Thursday, April 21, 2022
Spring 2022 at Longwood Gardens in Pennsylvania
Mythical Gardens - The Garden of Eden at Creation - Illuminated Manuscripts
French illuminated manuscript, Image du Monde, attributed to Gautier de Metz, portraying God creating animals and birds; Harley 344, folio 1. British Library
Wednesday, April 20, 2022
17C Spring by Wenceslaus Hollar (1607-1677)
Mythical Gardens - The Garden of Eden at Creation - Illuminated Manuscripts
Tuesday, April 19, 2022
Plants & Incense already traveled The Silk Road as China officially began trade with the West in 130 B.C.
Journey of the Magi by Hieronymus Bosch 1500-1510
Stefano Di Giovanni Sassetta (Italian artist, 1394-1450) Journey of the Magi along The Silk Road 1435
The Middle Ages refers to the period of European history from the fall of the Roman Empire in the West (5C) to the fall of Constantinople (1453). In the history of Europe, the Middle Ages (or medieval period) lasted from the 5C to the 15C. The Middle Ages is the middle period of the 3 traditional divisions of Western history: classical antiquity, the medieval period, & the modern period.
The Meeting of the Magi on The Silk Road by Maestro de Saint Bartholomew 1480
The medieval period is subdivided into the Early, High, & Late Middle Ages. During the High Middle Ages, which began after 1000, the population of Europe increased greatly as technological & agricultural innovations allowed trade to flourish. The Crusades, first preached in 1095, were military attempts by Western European Christians to regain control of the Holy Land from Muslims. For Europe as a whole, 1500 is often considered to be the end of the Middle Ages, but there is no firmly agreed upon end date. Events such as the conquest of Constantinople by the Turks in 1453, Christopher Columbus's first voyage to the Americas in 1492, or the Protestant Reformation in 1517 are sometimes used.
Ancient Societies also Stopped to Smell the Flowers
Science News. By Bruce Bower. May 4, 2022
Ramses VI faced a smelly challenge when he became Egypt’s king in 1145 B.C. The new pharaoh’s first job was to rid the land of the stench of fish & birds, denizens of the Nile Delta’s fetid swamps.
That, at any rate, was the instruction in a hymn written to Ramses VI upon his ascension to the throne. Some smells, it seems, were considered far worse than others in the land of the pharaohs.
Surviving written accounts indicate that, perhaps unsurprisingly, residents of ancient Egyptian cities encountered a wide array of nice & nasty odors. Depending on the neighborhood, citizens inhaled smells of sweat, disease, cooking meat, incense, trees & flowers. Egypt’s hot weather heightened demand for perfumed oils & ointments that cloaked bodies in pleasant smells.
“The written sources demonstrate that ancient Egyptians lived in a rich olfactory world,” says Egyptologist Dora Goldsmith of Freie Universität Berlin...
Archaeologists have traditionally studied visible objects. Investigations have reconstructed what ...buildings looked like based on excavated remains & determined how people lived by analyzing their tools, personal ornaments & other tangible finds.
Rare projects have re-created what people may have heard thousands of years ago at sites such as Stonehenge (SN: 8/31/20). Piecing together, much less re-creating, the olfactory landscapes, or smellscapes, of long-ago places has attracted even less scholarly curiosity. Ancient cities in Egypt & elsewhere have been presented as “colorful & monumental, but odorless & sterile,” Goldsmith says.
Changes are in the air, though. Some archaeologists are sniffing out odor molecules from artifacts found at dig sites & held in museums. Others are poring over ancient texts for references to perfume recipes, & have even cooked up a scent much like one presumably favored by Cleopatra. In studying & reviving scents of the past, these researchers aim to understand how ancient people experienced, & interpreted, their worlds through smell...
Researchers generally assume that Tayma in what’s now Saudi Arabia .was a pit stop on an ancient network of trade routes, known as the Incense Route, that carried frankincense & myrrh from southern Arabia to Mediterranean destinations around 2,300 to 1,900 years ago. Frankincense & myrrh are both spicy-smelling resins extracted from shrubs & trees that grow on the Arabian Peninsula & in northeastern Africa & India. But Tayma was more than just a refueling oasis for trade caravans.
The desert outpost’s residents purchased aromatic plants for their own uses during much of the settlement’s history, a team led by Huber found. Chemical & molecular analyses of charred resins identified frankincense in cube-shaped incense burners previously unearthed in Tayma’s residential quarter, myrrh in cone-shaped incense burners that had been placed in graves outside the town wall, & an aromatic substance from Mediterranean mastic trees in small goblets used as incense burners in a large public building...
Other researchers have gone searching for molecular scent clues in previously excavated pottery. Analytical chemist Jacopo La Nasa of the University of Pisa in Italy & his colleagues used a portable version of a mass spectrometer to study 46 vessels, jars, cups & lumps of organic material.
These artifacts were found more than a century ago in the underground tomb of Kha & his wife Merit, prominent nonroyals who lived during Egypt’s 18th dynasty from about 1450 B.C. to 1400 B.C. The spectrometer can detect the signature chemical makeup of invisible gases emitted during the decay of different fragrant plants & other substances that had been placed inside vessels...
Re-creating Cleopatra’s perfume
A tradition of fragrant remedies & perfumes began as the first Egyptian royal dynasties assumed power around 5,100 years ago, Goldsmith’s research suggests. Ancient Egyptian hieroglyphic & cursive documents describe recipes for several perfumes. But precise ingredients & preparation methods remain unknown...
That didn’t stop Goldsmith & historian of Greco-Roman philosophy & science Sean Coughlin of the Czech Academy of Sciences in Prague from trying to re-create a celebrated Egyptian fragrance known as the Mendesian perfume. Cleopatra, a perfume devotee during her reign as queen from 51 B.C. to 30 B.C., may have doused herself with this scented potion. The perfume took its name from the city where it was made, Mendes.
Excavations conducted since 2009 at Thmouis, a city founded as an extension of Mendes, have uncovered the roughly 2,300-year-old remains of what was probably a fragrance factory, including kilns & clay perfume containers. Archaeologist Robert Littman of the University of Hawaii at Manoa & anthropological archaeologist Jay Silverstein of the University of Tyumen in Russia, who direct the Thmouis dig, asked Goldsmith & Coughlin to try to crack the Mendesian perfume code by consulting ancient writings.
After experimenting with ingredients that included desert date oil, myrrh, cinnamon & pine resin, Goldsmith & Coughlin produced a scent that they suspect approximates what Cleopatra probably wore. It’s a strong but pleasant, long-lasting blend of spiciness & sweetness, they say.
Ingredients of a re-creation of an ancient fragrance called the Mendesian perfume consist of pine resin, cinnamon cassia, true cinnamon, myrrh & moringa oil. Cleopatra herself may have worn the ancient scent. A description of the Thmouis discoveries & efforts to revive the Mendesian scent — dubbed Eau de Cleopatra by the researchers — appeared in the Sept. 2021 Near Eastern Archaeology.
Goldsmith has re-created several more ancient Egyptian perfumes from written recipes for fragrances that were used in everyday life, for temple rituals & in the mummification process...
In the royal palace, for instance, the perfumed smell of rulers & their family members would have overpowered that of court officials & servants. That would perhaps have denoted special ties to the gods among those in charge, Goldsmith wrote in a chapter of The Routledge Handbook of the Senses in the Ancient Near East, published in September of 2021.
In temples, priests anointed images of gods with what was called the 10 sacred oils. Though their ingredients are mostly unknown, each substance apparently had its own pleasing scent & ritual function...
Scent is a powerful part of the human experience. Today, scientists know that smells, which humans might discriminate surprisingly well, can instantly trigger memories of past experiences...
People in modern settings probably perceive the same smells as nice or nasty as folks in ancient Egypt or other past societies did, says psychologist Asifa Majid of the University of Oxford. In line with that possibility, members of nine non-Western cultures, including hunter-gatherers in Thailand & farming villagers in highland Ecuador, closely agreed with Western city dwellers when ranking the pleasantness of 10 odors, Majid & her colleagues report April 4 in Current Biology.
Smells of vanilla, citrus & floral sweetness — dispensed by pen-sized devices — got high marks...
So, even if the ancients tagged the same odors as pleasurable or offensive as people do today, culture & context probably profoundly shaped responses to those smells.
Working-class Romans living in Pompeii around 2,000 years ago — before Mount Vesuvius’ catastrophic eruption in A.D. 79 — provide one example. Archaeological evidence & written sources indicate that patrons of small taverns throughout the city were bombarded with strong smells, says archaeologist Erica Rowan of Royal Holloway, University of London. Diners standing or sitting in small rooms & at outdoor counters whiffed smoky, greasy food being cooked, body odors of other customers who had been toiling all day & pungent aromas wafting out of nearby latrines.
The smells & noises that filled Pompeii’s taverns provided a familiar & comforting experience for everyday Romans, who made these establishments successful, Rowan suspects. Excavations have uncovered 158 of these informal eating & drinking spots throughout Pompeii.
Roman cities generally smelled of human waste, decaying animal carcasses, garbage, smoke, incense, cooked meat & boiled cabbage, Classical historian Neville Morley of the University of Exeter in England wrote in 2014 in a chapter of Smell & the Ancient Senses. That potent mix “must have been the smell of home to its inhabitants & perhaps even the smell of civilization,” he concluded.
Ramses VI undoubtedly regarded the perfumed world of his palace as the epitome of civilized life. But at the end of a long day, Egyptian sandal-makers & smiths, like Pompeii’s working stiffs, may well have smelled home as the air of city streets filled their nostrils.
See:
A. Arshamian et al. The perception of odor pleasantness is shared across cultures. Current Biology. Published April 4, 2022.
D. Goldsmith. Smellscapes in ancient Egypt. In K. Neumann & A. Thomason, eds., The Routledge Handbook of the Senses in the Ancient Near East. New York, September 2021.
D. Goldsmith. Fish, fowl & stench in ancient Egypt. In A. Schellenberg & T. Krüger, eds., Sounding Sensory Profiles in the Ancient Near East. SBL Press, 2019.
B. Huber et al. How to use modern science to reconstruct ancient scents. Nature Human Behavior. Published March 28, 2022.
B. Huber et al. An archaeology of odors: Chemical evidence of ancient aromatics at the oasis of Tayma, NW Arabia. 11th International Conference on the Archaeology of the Ancient Near East. Munich, April 3–7, 2018.
R.J. Littman et al. Eau de Cleopatra: Mendesian perfume & Tell Timai. Near Eastern Archaeology. Vol. 84, September 2021.
N. Morley. Urban smells & Roman noses. In M. Bradley, ed., Smell & the Ancient Senses. New York, December 2014.
J. La Nasa et al. Archaeology of the invisible: The scent of Kha & Merit. Journal of Archaeological Science. Vol. 141, May 2022.
E. Rowan. The sensory experiences of food consumption. In R. Skeates & J. Day, eds., The Routledge Handbook of Sensory Archaeology. New York, November 2019.
The Woman who Figured Out what Mankind is Made of after Thousands of Years Passed
The answer to this fundamental question of astrophysics was discovered in 1925 by Cecilia Payne (1900-1979) & explained in her Ph.D. thesis. Payne showed how to decode the complicated spectra of starlight in order to learn the relative amounts of the chemical elements in the stars. In 1960 the distinguished astronomer Otto Struve referred to this work as “the most brilliant Ph.D. thesis ever written in astronomy.”
Cecilia Payne was born in Wendover, England. After entering Cambridge University she soon knew she wanted to study a science but was not sure which one. She then chanced to hear the astronomer Arthur Stanley Eddington (1882-1944) give a public lecture on his recent expedition to observe the 1919 solar eclipse, an observation that proved Einstein’s Theory of General Relativity.
She later recalled her exhilaration: “The result was a complete transformation of my world picture. When I returned to my room I found that I could write down the lecture word for word.” She realized that physics was for her.
Later, at Cambridge Observatory Cecilia told Professor Eddington, that she wanted to be an astronomer. He suggested a number of books for her to read, but she had already read them. Eddington then invited her to use the Observatory’s library, with access to all the latest astronomical journals.
"There is no joy more intense than that of coming upon a fact that cannot be understood in terms of currently accepted ideas." declared Cecilia Payne
Payne realized early during her Cambridge years, that a woman had little chance of advancing beyond a teaching role, & no chance at all of getting an advanced degree in England.
Women in the USA had only won the right to vote in national elections in 1920, just 3 years before Payne left England in 1923 for the United States. Here she met Professor Harlow Shapley (1885-1952), the new director of the Harvard College Observatory, who offered her a graduate fellowship.
Cecilia Payne became the 1st person to earn a PhD in astronomy from Harvard University. Her 1925 graduate thesis proposed that the Sun & other stars were made predominantly of hydrogen, & described as "the most brilliant PhD thesis ever written in astronomy." (Payne received the 1st Ph.D. in astronomy from Radcliffe College for her thesis, since Harvard did not grant doctoral degrees to women.)
But Harvard did have the world’s largest archive of stellar spectra on photographic plates. Astronomers obtain such spectra by attaching a spectroscope to a telescope. This instrument spreads starlight out into its “rainbow” of colors, spanning all the wavelengths of visible light. The wavelength increases from the violet to the red end of the spectrum, as the energy of the light decreases. A typical stellar spectrum has many narrow dark gaps where the light at particular wavelengths (or energies) is missing. These gaps are called absorption “lines,” & are due to various chemical elements in the star’s atmosphere that absorb the light coming from hotter regions below.
The study of spectra had led to the science of astrophysics. In 1859, Gustav Kirchoff & Robert Bunsen in Germany heated various chemical elements & observed the spectra of the light given off by the incandescent gas. They found that each element has its own characteristic set of spectral lines—its uniquely identifying “fingerprint.” In 1863, William Huggins in England observed many of these same lines in the spectra of the stars. The visible universe, it turned out, is made of the same chemical elements as those found on Earth.
Beginning in the 1880s, astronomers at Harvard College such as Edward Pickering, Annie Jump Cannon, Williamina Fleming, & Antonia Maury had succeeded in classifying stars according to their spectra into seven types: O, B, A, F, G, K, & M. It was believed that this sequence corresponded to the surface temperature of the stars, with O being the hottest & M the coolest. In her Ph.D. thesis (published as Stellar Atmospheres [1925]), Payne used the spectral lines of many different elements & the work of Indian astrophysicist Meghnad Saha, who had discovered an equation relating the ionization states of an element in a star to the temperature to definitively establish that the spectral sequence did correspond to quantifiable stellar temperatures. Payne also determined that stars are composed mostly of hydrogen & helium. However, she was dissuaded from this conclusion by Princeton astronomer Henry Norris Russell (1877-1957), who thought that stars surely would have the same composition as Earth. (Russell conceded in 1929 that Payne was correct.)
In principle, it seemed that one might obtain the composition of the stars by comparing their spectral lines to those of known chemical elements observed in laboratory spectra. Astronomers had identified elements like calcium & iron as responsible for some of the most prominent lines, so they naturally assumed that such heavy elements were among the major constituents of the stars. In fact, Princeton's Henry Norris Russell at Princeton had concluded that if the Earth’s crust were heated to the temperature of the Sun, its spectrum would look nearly the same.
When Cecilia Payne arrived at Harvard, a comprehensive study of stellar spectra had long been underway. Annie Jump Cannon (1863-1941) whose cataloging work was instrumental in the development of contemporary stellar classification. Annie was nearly deaf throughout her career. She was a suffragist & a member of the National Women's Party.
Annie Jump Cannon (1863-1941)
Annie had sorted the spectra of several hundred thousand stars into seven distinct classes. She had devised & ordered the classification scheme, based on differences in the spectral features. Astronomers assumed that the spectral classes represented a sequence of decreasing surface temperatures of the stars, but no one was able to demonstrate this quantitatively.
Cecilia Payne, who studied the new science of quantum physics, knew that the pattern of features in the spectrum of any atom was determined by the configuration of its electrons. She also knew that at high temperatures, one or more electrons are stripped from the atoms, which are then called ions. The Indian physicist M. N. Saha had recently shown how the temperature & pressure in the atmosphere of a star determine the extent to which various atoms are ionized.
Payne began a long project to measure the absorption lines in stellar spectra, & within two years produced a thesis for her doctoral degree, the first awarded for work at Harvard College Observatory. In it, she showed that the wide variation in stellar spectra is due mainly to the different ionization states of the atoms & hence different surface temperatures of the stars, not to different amounts of the elements. She calculated the relative amounts of eighteen elements & showed that the compositions were nearly the same among the different kinds of stars. She discovered, surprisingly, that the Sun & the other stars are composed almost entirely of hydrogen & helium, the two lightest elements. All the heavier elements, like those making up the bulk of the Earth, account for less than two percent of the mass of the stars.
Most of the mass of the visible universe is hydrogen, the lightest element, & not the heavier elements that are more prominent in the spectra of the stars! This was indeed a revolutionary discovery. Harlow Shapley sent Payne’s thesis to Professor Russell at Princeton, who informed her that the result was “clearly impossible.” To protect her career, Payne inserted a statement in her thesis that the calculated abundances of hydrogen & helium were “almost certainly not real.”
She then converted her thesis into the book Stellar Atmospheres, which was well-received by astronomers. Within a few years it was clear to everyone that her results were both fundamental & correct. Cecilia Payne had showed for the first time how to “read” the surface temperature of any star from its spectrum. She showed that Cannon’s ordering of the stellar spectral classes was indeed a sequence of decreasing temperatures & she was able to calculate the temperatures. The so-called Princeton Hertzsprung-Russell diagram, a plot of luminosity versus spectral class of the stars, could now be properly interpreted, & it became by far the most powerful analytical tool in stellar astrophysics.
From the time she finished her Ph.D. through the 1930s, Payne advised students, conducted research, & lectured—all the usual duties of a professor. Yet, because she was a woman, her only title at Harvard was “technical assistant” to Professor Harlow Shapley.
In 1933, Payne traveled to Europe to meet Russian astronomer Boris Gerasimovich, who had previously worked at the Harvard College Observatory & with whom she planned to write a book about variable stars. In Göttingen, Ger., she met Sergey Gaposchkin, a Russian astronomer who could not return to the Soviet Union because of his politics. Payne was able to find a position at Harvard for him. They married in 1934 & often collaborated on studies of variable stars. She was named a lecturer in astronomy in 1938, but even though she taught courses, they were not listed in the Harvard catalog until after World War II.
Despite being indisputably one of the most brilliant & creative astronomers of the 20C, Cecilia Payne was never elected to the elite National Academy of Sciences. But times were beginning to change. In 1956, she was finally made a full professor (the 1st woman so recognized at Harvard) & chair of the Astronomy Department.
Her fellow astronomers certainly came to appreciate her genius. In 1976, the American Astronomical Society awarded her the prestigious Henry Norris Russell Prize. In her acceptance lecture, she said, “The reward of the young scientist is the emotional thrill of being the 1st person in the history of the world to see something or to understand something.”
See:
American Museum of Natural History: Cecilia Payne & the Composition of the Stars
Encyclopedia Britannica: Cecilia Payne-Gaposchkin
Archival Collections:
Collections of Cecilia Payne- & Sergei Gaposchkin. Wolbach Library, Harvard & Smithsonian Center for Astrophysics, Cambridge, Mass.
Papers of Harlow Shapley, 1906-1966; HUG 4773.10 Box 89. Harvard University Archives, Harvard University, Cambridge, Mass.
Papers of Cecilia Helena Payne-Gaposchkin, 1924, circa 1950s-1990s, 2000; HUGB P182.5, P182.50. Harvard University Archives, Harvard University, Cambridge, Mass. Link.
Project PHaEDRA. Wolbach Library, Harvard & Smithsonian Center for Astrophysics, Cambridge, Mass. Link.
Radcliffe College Alumnae Association Records, ca.1894-2004; RG IX, Series 2, box 241. Schlesinger Library, Radcliffe Institute, Harvard University, Cambridge, Mass.
Wilbur Kitchener Jordan Records of the President of Radcliffe College, 1943-1960; RG II, Series 3, boxes 27, 60. Radcliffe College Archives, Schlesinger Library, Radcliffe Institute, Harvard University, Cambridge, Mass.
Bibliography:
Bartusiak, Marcia. 1993. “The Stuff of Stars.” The Sciences, no. September/October: 34–39.
Boyd, Sylvia. 2014. Portrait of a Binary : The Lives of Cecilia Payne & Sergei Gaposchkin. Penobscot Press.
DeVorkin, David. 2010. “Extraordinary Claims Require Extraordinary Evidence: C.H. Payne, H.N. Russell & Standards of Evidence in Early Quantitative Stellar Spectroscopy.” Journal Of Astronomical History & Heritage 13 (2): 139–44.
Gaposchkin, Cecilia Helena Payne. 1984. Cecilia Payne-Gaposchkin: An Autobiography (“The Dyer’s Hand”) & Other Recollections. Cambridge ; New York: Cambridge University Press.
Gaposchkin, Sergei. 1970. The Divine Scramble. Self-Published.
Gingerich, Owen, Katherine Haramundanis, & Dorrit Hoffleit. 2001. The Starry Universe: The Cecilia Payne-Gaposchkin Centenary. L. Davis Press.
Popova, Maria. 2017. “Stitching a Supernova: A Needlepoint Celebration of Science by Pioneering Astronomer Cecilia Payne.” Brain Pickings (blog). May 10, 2017.
Russell, Henry Norris. 1929. “On the Composition of the Sun’s Atmosphere.” The Astrophysical Journal 70 (July): 11.
Spiller, James. 2015. Frontiers for the American Century: Outer Space, Antarctica, & Cold War Nationalism. First edition. Palgrave Studies in the History of Science & Technology. New York, NY: Palgrave Macmillan.
Woodman, Jennifer. 2016. “Stellar Works: Searching for the Lives of Women in Science.” Dissertations & Theses, June.
"We Are Made of Starstuff.”
Dear old Hubble & the new James Webb Telescope, the largest space observatory to date, & thousands of scientists around the world will lead us into countless universes & 100 billion galaxies of composed of dying stars expelling dust & gas - elements & gases interchangeable with ours. We are part of infinity living on a tiny blue dot in space. “The nitrogen in our DNA, the calcium in our teeth, the iron in our blood, the carbon in our apple pies were made in the interiors of collapsing stars. We are made of starstuff.”
“Look again at that dot. That's here. That's home. That's us. On it everyone you love, everyone you know, everyone you ever heard of, every human being who ever was, lived out their lives. The aggregate of our joy and suffering, thousands of confident religions, ideologies, and economic doctrines, every hunter and forager, every hero and coward, every creator and destroyer of civilization, every king and peasant, every young couple in love, every mother and father, hopeful child, inventor and explorer, every teacher of morals, every corrupt politician, every "superstar," every "supreme leader," every saint and sinner in the history of our species lived there-on a mote of dust suspended in a sunbeam.
"The Earth is a very small stage in a vast cosmic arena. Think of the endless cruelties visited by the inhabitants of one corner of this pixel on the scarcely distinguishable inhabitants of some other corner, how frequent their misunderstandings, how eager they are to kill one another, how fervent their hatreds. Think of the rivers of blood spilled by all those generals and emperors so that, in glory and triumph, they could become the momentary masters of a fraction of a dot.
"Our posturings, our imagined self-importance, the delusion that we have some privileged position in the Universe, are challenged by this point of pale light. Our planet is a lonely speck in the great enveloping cosmic dark. In our obscurity, in all this vastness, there is no hint that help will come from elsewhere to save us from ourselves.
"The Earth is the only world known so far to harbor life. There is nowhere else, at least in the near future, to which our species could migrate. Visit, yes. Settle, not yet. Like it or not, for the moment the Earth is where we make our stand.
"It has been said that astronomy is a humbling and character-building experience. There is perhaps no better demonstration of the folly of human conceits than this distant image of our tiny world. To me, it underscores our responsibility to deal more kindly with one another, and to preserve and cherish the pale blue dot, the only home we've ever known.”
―American astronomer Carl Sagan (1934-1996), Pale Blue Dot: A Vision of the Human Future in Space
Spring 2022 at Longwood Gardens in Pennsylvania
Mythical Gardens - The Garden of Eden at Creation - Illuminated Manuscripts
Animals & Humans Emerging from the Earth Together; from an illustrated manuscript version of Augustine's City of God, c. 1475 (The Hague, RMMW, 10 A 11, fol. 300v) This garden seems to ha a natural curved road with trees evenly planted on both sides
Monday, April 18, 2022
17C Spring - Flowers, Fertility, Sensuality, & Delight.
Mythical Gardens - The Garden of Eden at Creation - Illuminated Manuscripts
Saturday, April 16, 2022
The Angel said Fear not...He is Risen
And the angel...said Fear not ye: for I know that ye seek Jesus, which was crucified. He is not here: for he is risen, as he said. Matthew 28:5–6
Music-making Angel by Melozzo da Forli (Italian Renaissance artist, 1438-1494) from fresco paintings of the Basilica dei Santi Apostoli, the Vault of the Sacristy of Saint Mark. Vatican Museums.
Music-making Angel by Melozzo da Forli (Italian Renaissance artist, 1438-1494) from fresco paintings of the Basilica dei Santi Apostoli, the Vault of the Sacristy of Saint Mark. Vatican Museums.
Music-making Angel by Melozzo da Forli (Italian Renaissance artist, 1438-1494) from fresco paintings of the Basilica dei Santi Apostoli, the Vault of the Sacristy of Saint Mark. Vatican Museums.
Music-making Angel by Melozzo da Forli (Italian Renaissance artist, 1438-1494) from fresco paintings of the Basilica dei Santi Apostoli, the Vault of the Sacristy of Saint Mark. Vatican Museums.
Music-making Angel by Melozzo da Forli (Italian Renaissance artist, 1438-1494) from fresco paintings of the Basilica dei Santi Apostoli, the Vault of the Sacristy of Saint Mark. Vatican Museums.
Music-making Angel by Melozzo da Forli (Italian Renaissance artist, 1438-1494) from fresco paintings of the Basilica dei Santi Apostoli, the Vault of the Sacristy of Saint Mark. Vatican Museums.
Music-making Angel by Melozzo da Forli (Italian Renaissance artist, 1438-1494) from fresco paintings of the Basilica dei Santi Apostoli, the Vault of the Sacristy of Saint Mark. Vatican Museums.
Angel by Melozzo da Forli (Italian Renaissance artist, 1438-1494). Vatican Museums.
Sunday, April 10, 2022
Friday, March 25, 2022
The Annunciation of the coming Birth of Jesus to Mary in Spring Gardens - Illuminated Manuscripts
The Annunciation to Mary by the Archangel Gabriel, with Anne Boleyn's note in the lower margin (London, British Library, MS King's 9, f. 66v).
The Annunciation in a Garden, about 1469
Tuesday, March 1, 2022
In 875 AD Imagining the origin of the Gospels
A gospel is an account describing the life of Jesus of Nazareth. The most widely-known gospels are Matthew, Mark, Luke, & John. Some Christians use the term "gospel," otherwise known as the "good news," in reference to the general message of the biblical New Testament. Here Matthew, Mark, Luke, & John are portrayed with a few of their fierce friends writing about the life of Jesus.
Illuminated Manuscript, Gospels of Freising, Evangelist Portrait of Mark, Walters Art Museum Ms. W.4, fol. 90v Freising, Germany c 875.
Illuminated Manuscript, Gospels of Freising, Evangelist Portrait of Luke, Walters Art Museum Ms. W.4, fol. 126v Freising, Germany c 875.
Illuminated Manuscript, Gospels of Freising, Evangelist Portrait of John, Walters Art Museum Ms. W.4, fol. 178v Freising, Germany c 875.