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Naamah, the daughter of Lamech and Stella, working at her loom
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Burney 227 f.3 A member of the Stella family of Verona: the family's arms: azure, an eight-pointed star, from 'Amphitruo, Eight comedies with prologues and arguments' by Titus Maccius Plautus, c.1440 (ink, colour and gold on vellum)
Stella Maris, Mary, Star of the Sea, sgraffito on a villa from 1926, historic uptow..., 2015 (photo)
Porto Ferrajo from the sea: To the Right Hon.ble Earl Spencer This view [...] is with great respect inscribed by his Lordship's obedient Servant James Weir. / Drawn by Capt. James Weir; Engraved by F. Jukes.
View of Portoferraio in the island of Elba from the east, with ship sailing near the lighthouse and Forte Stella at left, Forte Falcone at right, and mountains in the background.
This view of the west side of Porto Ferrajo Bay with the positions of the Captain 74 - Flora, Inconstant, Southampton Frigates: To the Right Hon.ble Earl Spencer This VIEW [...] is with great respect inscribed by his Lordship's obedient Servant James Weir. / Drawn by Capt. James Weir; Engraved by F. Jukes.
Fishing boat, rowing boat and four British ships sailing near the coast of the island of Elba, with bay and mountains at left and Forte Stella at right in the background.
Illustrated page from The Desert of Religion
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Or 16455 f.13r, Animals from the Zodiac, from Phrommachat (parchment)
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Or 16455 f.9r, Animals from the Zodiac, from Phrommachat (parchment)
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Or 16455 f.2r, Animals from the Zodiac, from Phrommachat (parchment)
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Or 16455 f.14r, Animals from the Zodiac, from Phrommachat (parchment)
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Or 16455 f.7r, Animals from the Zodiac, from Phrommachat (parchment)
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Or 16455 f.5r, Animals from the Zodiac, from Phrommachat (parchment)
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June: haymaking, 15th century (vellum)
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Or 16455 f.19r, Lucky and unlucky combinations of couples, from Phrommachat (parchment)
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Or 16455 f.17r, Lucky and unlucky combinations of couples, from Phrommachat (parchment)
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Life on an Exoplanet: View of an alien life artist on the surface of an exoplanet orbiting a class F star. Extraterrestrial life on an exoplanet orbiting a F-type star
Cotton MS Tiberius C I f.28r 'Cicero, Aratea with scholiae; Germano-Roman Pontifical' (ink & colour on vellum)
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Ms 65/1284 f.3v March: peasants at work on a feudal estate, from the 'Tres Riches Heures du Duc de Berry' (vellum) (for facsimile copy see 65835)
Comete Hale - Bopp 08/03/1997 - Comet Hale - Bopp on March 8 1997 - Comet Hale - Bopp (4 min. exposure on Kodak Pro 400 PPF film with 8 inch f/1.5 Schmidt camera
Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. In red, the coldest regions, in blue and green, the warmer regions. SDO (Solar Dynamics Observatory) First Light Image. A full - disk multiwavelength extreme ultraviolet image of the sun taken by SDO on March 30, 2010. False colors trace different gas temperatures. Reds are relatively cool (about 60,000 Kelvin, or 107,540 F); blues and greens are hotter (greater than 1 million Kelvin, or 1,799,540 F)
Psalm 44; Magi follow the star
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Add MS 10302 f.67v Horoscopes from 'The Ordinal of Alchemy' by Thomas Norton, c.1477 (vellum)
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Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Object number 45 in Messier's catalog is the Pleiades, also know as the Seven Sisters for the seven stars that can be easily seen with excellent eyesight.The Pleiades is a relatively nearby open cluster, which according to new data from the Hipparcos satellite is located at a distance of 370 light years. The cluster is surrounded by blue nebulosity illuminated by the light reflected from the nearby stars. Astro - Physic's 130EDT F/8 Triplet Refractor working at f/6 two 20 minute exposures
Tabby's Star
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Dark Nebula Barnard 142 in the Eagle - B142 Dark Nebula B142 and B143 are a pair of dark nebulae in Aquila in the rich summer Milky Way star fields near Tarazed (Gamma Aquilae), the brightest star in this photo at magnitude 2.7. Dark nebula are clouds of non - luminous matter in space that obscure the stars behind them. 500 mm f/4 Nikkor ED lens working at f/4 composite to two 7 minute exposures no filter hypered (8HRS) Kodak Ektapress Multi - speed PJM 9:11, 9:23 pm September 26, 1997 Chatsworth, N
James Webb Space Telescope (JWST) - Artist view - The James Webb Space Telescope (JWST) - Artist view: The James Webb Space Telescope (JWST) will replace the Hubble Space Telescope in 2018. The James Webb Space Telescope (JWST) is a large, infrared-optimized space telescope scheduled for launch in 2018. Equipped with a large mirror 6.5 meters (21.3 feet) in diameter, it will find the first galaxies that formed in the early Universe, connecting the Big Bang to our own Milky Way Galaxy and will reside in an orbit about 1.5 million km (1 million miles) from the Earth - The shaded side of the James Webb Space Telescope (JWST) as it may appear later this decade when it is observing from the Earth-Sun L2 point about 930 thousand miles from the Earth. Part of the Milky Way can be seen reflected in the 21-foot diameter mirror assembly. This assembly is composed of 18 hexagonal segments of gold-coated beryllium which combines to create a near-infrared light-collecting area of about 80 square feet (the Hubble Space Telescope has a collecting area of 48 square feet) - The JWST's sensitive optical elements are shaded from the perpetual sunlight via a “” parasol” consisting of multiple spaced layers of polyimide film. These layers act as a passive cooling barrier between the 185* F sunward side and the -388* F shaded side hosting the optics and sensors
Edelweiss
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Sabre in Close Formation with T33 Jet Trainer at 3 (F) Wing, 1954 (oil on board)
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Dark stars and nebulae in Sagittarius and Ophiuchus - Dark Nebulae in Sagittarius and Scorpius - Dark nebulae on the edge of the Pipe nebula. This complex of dust clouds that block the light of the stars is located between the Sagittarius and the Scorpio, near the center of our lactee road. Also visible, the nebulae emitted from the Lagoon, Trifide, and Omega. Image obtained with Canon 20Da, 50 mm f/1.4, 6 x 5 min ISO 1600 poses. This amazing complex of dark nebulae and dust in Sagittarius and Ophiuchus lies near the central bulge of our own galaxy, the Milky Way. Dark nebulae are non - luminous clouds of obscuring matter and dust which block the light from stars behind them. Many of the dark nebulae seen here are listed in E.E. Barnard's catalog of dark nebulae and are given a “” B” designation, such as B72, the Snake Nebula. Almost the entire complex of dark nebulae seen on the right hand side of the image make up the “Dark Horse and Rider””. The Pipe Nebula, Lynds Dark Nebula 1773, comprises the hind quarter and back leg of the Dark Horse, which is seen vertically in this image. B63 is the front leg, B270 is the Horse's head, and B276 is the Rider's head. The area is also filled with star clouds, bright emission nebulae such as M8 - the Lagoon Nebula, M20 - the Trifid Nebula, and M17 - the Omega Nebula. The small Sagittarius star cloud, M24, is at the upper left, and the large Sagittarius star cloud at lower left. The center of our galaxy lies near the bottom edge of the image. Image taken with a Canon 20Da DSLR, 50 mm f/1.4, and 6 x 5 min exposures at ISO 1600
Add. 17367, f.3r Aquarius & Pisces, from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
Eagle Nebula (IC 4703) and Star Cluster M16 in the Snake - M16, The Eagle Nebula 130 EDT f/8 60 minute exposure hypered Fuji Super G 800 1:36 am am May 29, 1995 Sentinel, A
Add. 17367, f.4r Aries & Taurus, from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
The center of our galaxy, the milky way - The center of our galaxy, the milky way - This billion pixel mosaic shows the central region of our galaxy, the Lactee Way. The 52 assembled images cover an area that extends from Sagittarius (with the galactic center and nebulae M8 and M20) on the left, to the Scorpio, with the star Antares and the colored cloud of Rho Ophiuchus on the right. Image obtained with a Takahashi FSQ 106 Ed bezel at Cerro Paranal Observatory in Chile; 200 hours of poses. This image is a 1 billion pixel RGB mosaic of the galactic center region (340 million pixels in each R, V and B color). It shows the region spanning from Sagittarius (with the Milky Way center and M8/M20 area on the left) to Scorpius (with colorful Antares and Rho Ophiuchus region on the right) and cat paw nebula (red nebula at the bottom). This mosaic was assembled from 52 different sky fields made from 1200 individual images and 200 hours total exposure time, final image size is 24000x14000 pixels. The images were taken with a SBIG STL camera+Takahashi FSQ106ed f/3.6 telescope and NJP160 mount from the clear skies of ESO Paranal Observatory in Chile. This mosaic is one of the three parts of the ESO Gigagalaxy Zoom project
Southern Crown Nebula - The Corona Australis nebula (NGC 6726 - 27 - 29) - R Coronae Australis is one of the closest and most intense star-forming regions; visible in the southern hemisphere, it is located about 500 years from Earth. R Coronae Australis is the star in the center of the image that illuminates a reddish nebula around it. Image obtained in Chile at the observatory of La Silla with the 2.2 meter MPG/ESO telescope. Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - called “” T Tauri””” class, a type that is quite common in star - forming regions. T Tauri stars are in the early stages of stellar evolution and display various observable characteristics of this phase, e.g. emission at visible and infrared wavelengths due to the accretion of matter left over from their formation, as well as X - ray emission. The nebulosity seen in this picture is mostly due to reflection of the stellar light by small dust particles. The stars in the R Coronae Australis complex do not emit sufficient ultraviolet light to ionize a substantial fraction of the surrounding hydrogen, and thus cause this gas to glow. Also visible are so - called Herbig - Haro objects, dense clumps of gas ejected f
Add. 17367, f.7r Libra & Scorpio, from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
The Hanger and Nebula SH2 - 83 - Coathanger and nebula SH2 - 83 in Vulpecula - The Hanger cluster or Brocchi cluster (left) is not a true cluster of stars but an asterism located in the constellation of Little Fox. Towards the center of the image, a small nebula emitted, Sh2 - 83. Little Fox Constellation. Brocchi's Cluster (also known as the Coathanger or Collinder 399) is an asterism located in the constellation Vulpecula. It was first described by the Persian astronomer Al Sufi in his Book of Fixed Stars in 964 and was independently rediscovered by Giovanni Hodierna in the seventeenth century. In the 1920s, D. F. Brocchi, an amateur astronomer and chart maker for the American Association of Variable Star Observers, created a map of this object for use in calibrating photometers. The asterism is made up of ten stars ranging from fifth to seventh magnitude which form the conspicuous Coathanger, a straight line of six stars with a “” hook””” of four stars on the south side. An additional thirty or so fainter stars are sometimes considered to be associated as well. Under a dark sky, Brocchi's Cluster can be seen with the naked eye as an unresolved patch of light; binoculars or a telescope at very low power are usually needed in order to view the “” coathanger””” asterism. It is best found by slowly sweeping across the Milky Way along an imaginary line from the bright star Altair towards the even brighter star Vega. About one third of the way toward Vega, the Coathanger should be spotted easily against a darker region of the Milky Way. The status of this group as a star cluster has changed in recent years. The main stars were cataloged as an open cluster by Per Collinder in 1931, and the group was considered to be a cluster for most of the twentieth century. Looking at a variety of criteria, however, a study in 1970 concluded that only six of the brightest stars formed an actual cluster. Several independent studies since 1998 have now determined that t
Comete Hale - Bopp and clusters open M34 - 04/1997 - Comet Hale - Bopp with open cluster M34 - This is the beautiful Comet Hale - Bopp as it as it passed by (from our point of view) the star cluster M34 in April of 1997. The solid portion or nucleus of the comet is made up of ice, frozen gases, dust and small rock. Compared to most comets Hale - Bopp is very large - about 35 kilometers in diameter. As its orbit brought it closer to the sun, the frozen mass began to melt and a coma, which is a gaseous cloud, developed around the nucleus. This coma has grown to be hundreds of thousands of miles in diameter. Finally the tail developed which became millions of miles long. (4 min. exposure on Kodak Pro 400 PPF film with 8 inch f/1.5 Schmidt camera
Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained with a bezel Astro - Physics 130 EDT, 12x6min of poses. M20, The Trifid Nebula, in the constellation of Sagittarius, is a remarkable object - large, bright and beautiful. It is a complex of red emission, blue reflection, and dark nebulae about the size of the full moon. It was shot at 1,000 mm of focal length with 130 mm of aperture at f/8 (Astro - Physics 130EDT apochromatic refractor) with a Canon 20Da DSLR and only 12 x 6 minutes of exposure at ISO 1600
The Swan Lace - The Veil Nebula - The rest of supernova lies about 1500 years - light in the constellation Swan. The supernova would have exploded less than 10,000 years ago. The Veil Nebula is the remnant of a supernova explosion that occurred about 10,000 years ago. It is located 1,500 light years away in the constellation of Cygnus. NGC 6992/95 is the brighter eastern half of the nebula at left. NGC 6960 is the portion of the SNR that appears close to the star 52 Cygnus on the right half arc. Pickering's Triangular Wisp, above and to the left of the NGC 6960 portion of the nebula is designated as Simeis 3 - 188. At the top center of the photo is a small patch of the Veil designated as NGC 6974/79. Canon 300 mm f/2.8. Exposure: 96 x 2 mi
Brown dwarf star Teide 1 - Brown dwarf Teide 1 - Artist view of the brown dwarf star Teide 1. Discovered in 1995 in the Pleiades cluster, about 55 times the mass of Jupiter, this brown dwarf is represented here in the sky of a young exoplanet lit by the star. This is how Teide 1 might appear from the surface of a hypothetical, March - like planet. Discovered in 1995, Teide 1 is a type of mysterious object called a brown dwarf (failed star or super planet). Bigger than a planet, but smaller than a star, this brown dwarf is about 400 light years from the Earth in the Pleiades star cluster. It is thought that Teide 1 has the mass equivalent of about 55 Jupiters, which is considered large for a brown dwarf. Teide 1 is massive enough, and hence hot enough, to sustain lithium fusion in its core, but is unable to initiate hydrogen fusion like our sun. Teide 1 is probably only about 120 million years old (compared to our sun's age of 4.5 billion years) and shines at a temperature of 4,000o F, less than half as hot as the surface of our sun. In this image a young planet orbits Teide 1 from distance of about four million miles. The planet has acquired enough atmosphere to host clouds and put a lower limit on size of meteors that reach its surface (the smaller ones burn up before reaching the ground), but it is still very early in its evolution. Teide 1 looms large in this planet's sky, but in fact Teide 1's diameter is only about twice that of Jupiter's. All brown dwarfs are roughly the size of Jupiter - - the more massive brown dwarfs are simply more dense. As for this planet, it is very unlikely that life will ever evolve here due to its host's relatively short life span; in just another billion years Teide 1 will have cooled to a modest 1,700o F
Harley 2506, f.40, Drawing of an arrow, and of an eagle, with the constellations marked as red dots, from 'Aratea, or Phaenomena' (vellum)
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Orion Nebula M42 in Orion - The Orion Nebula - Located 1500 years - light, Orion Nebula (M42) is the closest region of formation of stars of the Sun. Above these are the NGC nebulae 1973-75-77. The Orion Nebula complex is easily visible to the unaided eye from a dark location as a patch of brightness surrounding Theta Orionis, the middle star in the sword of Orion the Hunter, the constellation which dominates the winter night sky.Located about 1500 light years away, the nebula glows red predominantly from the light of hydrogen gas excited by energetic newly formed stars in the heart of the nebula. It is the nearest star forming region to our own star, the Sun. NGC 1975, just above M42, is a complex of blue reflection nebulae mixed with dark lanes and a touch of red emission nebulae. The blue color comes from reflected starlight scattered by dust. North is up in this image. Composite of a 50 minute exposure and a 5 minute exposure on gas - hypersensitized Kodak Ektapress Multispeed PJM - 2 color negative film. Taken with an Astro - Physic's 130 EDT refractor at f/8 from Chatsworth NJ, USA on November 12, 1996 at 6:17 UT and 7:00 UT
Add. 17367, f.8v from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
Add. 17367, f.7v from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
Add. 17367, f.2r from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
Add. 17367, f.6v from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
Add. 17367, f.10v from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
Add. 17367, f.1r from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)
Brown dwarf star Gliese 229 b - Brown dwarf Gliese 229 b - Artist view of the brown dwarf star Gliese 229B. Discovered in 1995 in the constellation Lievre at 18 years - light from Earth, this brown dwarf is 30 to 40 times more massive than Jupiter and is estimated to be 2 to 4 billion years old. Top left is the red dwarf star Gliese 229A. This is how the brown dwarf Gliese 229b might appear from a distance of about a half million miles. Glowing like a charcoal ember, Gliese 229 b was discovered in 1995 and is 19 light years from the Earth. This brown dwarf orbits the red dwarf Gliese 229A in the constellation Lepus. Gliese A can be seen shining dimly on the upper left. These two dwarfs are about four billion miles apart, about the same distance between Pluto and our sun. Gliese 229 b is believed to be 30 to 40 times more massive than the planet Jupiter, which is massive enough for Gliese 229 b to sustain deuterium fusion, but not enough mass to initiate hydrogen fusion like our Sun. As a result, Gliese 229 b radiates a temperature of only 1,300o F. It is believed to be two to four billion years old. Despite being so much more massive than the planet Jupiter, the diameter of this brown dwarf is believed to be actually slightly less than Jupiter's; Gliese 229 b's greater mass results in its overcoming the internal pressures that sustain Jupiter's greater volume
Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a 20 inch Ritchey - Chretien telescope and an eleven mega - pixel camera at f/8 from high in the south central mountains of New Mexico