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The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in September 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, the New Horizons spacecraft rests on a work stand. New Horizons will make the first recognition of Pluto and Charon - a “double planet”” and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 2007, and reach Pluto and its moon, Charon, in July 2015

PIX4607319

The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in September 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, the New Horizons spacecraft rests on a work stand. New Horizons will make the first recognition of Pluto and Charon - a “double planet”” and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 2007, and reach Pluto and its moon, Charon, in July 2015

PIX4607319

 
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Jul 07, 1953 - Fail Fashions From London: Shown below are fall styles from the collection of three London designers, Telemac, Rembrandt and Arthur Banks: Photo shows (LEFT) Telemac's” Piper” raincoat of rayon trimmed with black braid piping. It is made with a fly-front and can be worn with or without the belt. The coat has deep turn-back cuffs and a matching hat. (CENTER) Rembrandt's cocktail separates in” Frosty,” a high-quality novelty material with surface interest given by a need-run design in glistening white fancy yarn which feels like straw, on a dark ground. A wide, low-out neckline distinguishes the long-sleeved top, and the skirt swings out in wide, stiff folds. (RIGHT) evening ensemble by Arthur Banks of velvet and Duchesse satin in delphinium blue.

ZUM4858900

Jul 07, 1953 - Fail Fashions From London: Shown below are fall styles from the collection of three London designers, Telemac, Rembrandt and Arthur Banks: Photo shows (LEFT) Telemac's” Piper” raincoat of rayon trimmed with black braid piping. It is made with a fly-front and can be worn with or without the belt. The coat has deep turn-back cuffs and a matching hat. (CENTER) Rembrandt's cocktail separates in” Frosty,” a high-quality novelty material with surface interest given by a need-run design in glistening white fancy yarn which feels like straw, on a dark ground. A wide, low-out neckline distinguishes the long-sleeved top, and the skirt swings out in wide, stiff folds. (RIGHT) evening ensemble by Arthur Banks of velvet and Duchesse satin in delphinium blue.

ZUM4858900

 
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Design by Barroin. An evening dress. It is made of black mousseline de soie, the over-skirt draped back in festoons which are caught up at intervals with full rosettes of black velvet. It opens over a petticoat of white satin veiled with pleated mousseline in a shade of green, upon which is painted a cluster of hortensias. The corsage is draped to match the skirt, a belt of blue satin encircling the waist. The head-dress is particularly striking: a mere rien of white velvet, the quills studded with black paillettes and caught together with a large jet ornament.

BL3302233

Design by Barroin. An evening dress. It is made of black mousseline de soie, the over-skirt draped back in festoons which are caught up at intervals with full rosettes of black velvet. It opens over a petticoat of white satin veiled with pleated mousseline in a shade of green, upon which is painted a cluster of hortensias. The corsage is draped to match the skirt, a belt of blue satin encircling the waist. The head-dress is particularly striking: a mere rien of white velvet, the quills studded with black paillettes and caught together with a large jet ornament.

BL3302233

 
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Ring around the Dwarf Planet Haumea - Illustration - Ring around Dwarf Planet Haumea - Artwork - Haumea, (136108 Haumea), is a transneptunian dwarf planet (a plutoid) of the Solar System member of the Kuiper belt. Discovered in 2004, Haumea has two known natural satellites, a very fast rotation (less than 4 h), an ellipsoidal shape and a high albedo caused by water ice crystals on its surface. Haumea would measure between 1,960 and 2,500 km, barely less than Pluto and twice as much as Ceres, the smallest known dwarf planet. Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit. It was discovered in 2004 and was recognized as a dwarf planet in 2008. Haumea's mass is about one-third that of Pluto, it has an elongated shape with a rapid rotation and has two known moons, Hi iaka and Namaka

Miller, Ron (b.1947)

PIX4629567

Ring around the Dwarf Planet Haumea - Illustration - Ring around Dwarf Planet Haumea - Artwork - Haumea, (136108 Haumea), is a transneptunian dwarf planet (a plutoid) of the Solar System member of the Kuiper belt. Discovered in 2004, Haumea has two known natural satellites, a very fast rotation (less than 4 h), an ellipsoidal shape and a high albedo caused by water ice crystals on its surface. Haumea would measure between 1,960 and 2,500 km, barely less than Pluto and twice as much as Ceres, the smallest known dwarf planet. Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit. It was discovered in 2004 and was recognized as a dwarf planet in 2008. Haumea's mass is about one-third that of Pluto, it has an elongated shape with a rapid rotation and has two known moons, Hi iaka and Namaka

Miller, Ron (b.1947)

PIX4629567

 
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SOUTH KOREANS LEARN TO SING IN SEOUL, 1999-01-08 (photo)

REU8160718

SOUTH KOREANS LEARN TO SING IN SEOUL, 1999-01-08 (photo)

REU8160718

 
The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in September 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, workers begin checking out the New Horizons spacecraft, which rests on a work stand. New Horizons will make the first recognition of Pluto and Charon - a “double planet”” and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 2007, and reach Pluto and its moon, Charon, in July 2015

PIX4607322

The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in September 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, workers begin checking out the New Horizons spacecraft, which rests on a work stand. New Horizons will make the first recognition of Pluto and Charon - a “double planet”” and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 2007, and reach Pluto and its moon, Charon, in July 2015

PIX4607322

 
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Charles Bedingfeld, 1833 (oil on canvas)

Austrian School, (19th century)

USB1157748

Charles Bedingfeld, 1833 (oil on canvas)

Austrian School, (19th century)

USB1157748

 
Gold ring gifted by Oscar Wilde to William Ward, 1876 (photo)

MCO8701858

Gold ring gifted by Oscar Wilde to William Ward, 1876 (photo)

MCO8701858

 
The Rosetta probe and the Steins asteroid - Rosetta spacecraft near asteroid Steins - Artist's view of the passage of the Rosetta probe near the Steins asteroid (2867) on September 5, 2008. The Rosetta probe was launched on 2 March 2004 in order to study comet 67P/Churyumov - Gerasimenko, which it should meet around May 2014. She will put a lander on her surface. Esa's Rosetta spacecraft flew by asteroid (2867) Steins on 5 September 2008 at 20:58 CEST, ground received time (= spacecraft time CEST+20 minutes), with a closest approach distance of 800 km. Steins is Rosetta's first nominal scientific target. The spacecraft encountered the asteroid in the course of its first incursion into the main asteroid belt located between the orbits of Mars and Jupiter, while on its way to Comet 67P/Churyumov - Gerasimenko

C. Carreau

PIX4607105

The Rosetta probe and the Steins asteroid - Rosetta spacecraft near asteroid Steins - Artist's view of the passage of the Rosetta probe near the Steins asteroid (2867) on September 5, 2008. The Rosetta probe was launched on 2 March 2004 in order to study comet 67P/Churyumov - Gerasimenko, which it should meet around May 2014. She will put a lander on her surface. Esa's Rosetta spacecraft flew by asteroid (2867) Steins on 5 September 2008 at 20:58 CEST, ground received time (= spacecraft time CEST+20 minutes), with a closest approach distance of 800 km. Steins is Rosetta's first nominal scientific target. The spacecraft encountered the asteroid in the course of its first incursion into the main asteroid belt located between the orbits of Mars and Jupiter, while on its way to Comet 67P/Churyumov - Gerasimenko

C. Carreau

PIX4607105

 
The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in September 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, the New Horizons spacecraft is moved toward a work stand (behind it) for a checkout. New Horizons will make the first recognition of Pluto and Charon - a “double planet”” and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 2007, and reach Pluto and its moon, Charon, in July 2015

PIX4607343

The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in September 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, the New Horizons spacecraft is moved toward a work stand (behind it) for a checkout. New Horizons will make the first recognition of Pluto and Charon - a “double planet”” and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 2007, and reach Pluto and its moon, Charon, in July 2015

PIX4607343

 
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A design by Doucet for the Princess Lazareff. Soft blue velvet spotted with white is the material for the skirt; it has a narrow edging of chinchilla. Over this is worn a bolero of the same fur, cut out across the chest, and turned back with large revers of black fox. The high upstanding collar of chinchilla is caught round the throat with a neckband embroidered in silver to match the belt. Huge of chinchilla and a hat by Caroline Reboux of soft black felt trimmed with two large feathers starting sideways from a great bow of tulle which is clasped in the centre by a buckle in old sliver.

BL3302235

A design by Doucet for the Princess Lazareff. Soft blue velvet spotted with white is the material for the skirt; it has a narrow edging of chinchilla. Over this is worn a bolero of the same fur, cut out across the chest, and turned back with large revers of black fox. The high upstanding collar of chinchilla is caught round the throat with a neckband embroidered in silver to match the belt. Huge of chinchilla and a hat by Caroline Reboux of soft black felt trimmed with two large feathers starting sideways from a great bow of tulle which is clasped in the centre by a buckle in old sliver.

BL3302235

 
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Lieut General Sir S J Browne and Staff

UIS5080249

Lieut General Sir S J Browne and Staff

UIS5080249

 
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643771

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643771

 
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statue of Montuemhat

Egyptian School

Sandro Vannini

SVA660289

statue of Montuemhat

Egyptian School

Sandro Vannini

SVA660289

 
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643784

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643784

 
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643799

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643799

 
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Robert Chaumberleyn

Smith, Charles Hamilton (1776-1859) (after)

BL3266251

Robert Chaumberleyn

Smith, Charles Hamilton (1776-1859) (after)

BL3266251

 
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643791

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (single) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens (as here). Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643791

 
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643748

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643748

 
Planetary Nebula of the Red Rectangle in the Unicorn - The Red Rectangle, AFGL 915 - This planetary nebula is located about 2300 years ago - light. Image from Siding Spring 3.9m Telescope This surprising object is one of an unusual class of nebulae surrounding mature, sun - like stars that are about to turn into planetary nebulae. Not all pre - planetary nebulae have outbursts like this, and in those that do, the nebula lasts only a few thousand years, hence the rarity. The central star has a thick belt of dust like a girdle around its equator which restricts outflow in that direction. Instead, the star ejects material in a kind of cone from each of its poles. The spectrum of the nebula shows unusual, strong red lines from hydrogen bonded to grains of carbon, however there is sufficient light reflected from the embedded star to dilute the strong red spectrum to the deep yellow we see here

PIX4623779

Planetary Nebula of the Red Rectangle in the Unicorn - The Red Rectangle, AFGL 915 - This planetary nebula is located about 2300 years ago - light. Image from Siding Spring 3.9m Telescope This surprising object is one of an unusual class of nebulae surrounding mature, sun - like stars that are about to turn into planetary nebulae. Not all pre - planetary nebulae have outbursts like this, and in those that do, the nebula lasts only a few thousand years, hence the rarity. The central star has a thick belt of dust like a girdle around its equator which restricts outflow in that direction. Instead, the star ejects material in a kind of cone from each of its poles. The spectrum of the nebula shows unusual, strong red lines from hydrogen bonded to grains of carbon, however there is sufficient light reflected from the embedded star to dilute the strong red spectrum to the deep yellow we see here

PIX4623779

 
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643730

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643730

 
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643732

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643732

 
The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643767

The New Horizons probe near 2014 MU69 - Artist's View - New Horizons and 2014 MU69 (binary) - Artwork: Artist's view of the New Horizons probe near the small object of Kuiper 2014 MU69. Observations in 2017 show that 2014 MU69 would be either a binary object (model favors), in contact or not, or a single object lengthens. Speculative illustration of Nasa's New Horizons interplanetary probe flying by classical Kuiper belt object (486958) 2014 MU69, about 3 billion miles from the Earth, on 1 January 2019. 2014 MU69 is either a single elongated object about 30 miles long, or two smaller objects orbiting very closely together, maybe even touching; this image illustrates the latter. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high-gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth

Walter B Myers

PIX4643767

 
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Raja Jai Singh of Amber (reg. c.1621-1667), aged about 60, dressed in a green jama and gold embroidered paijama, seated on a gilt and painted chair, his bare feet on a purple cushion, one hand held out to a young man standing before him. The latter is dressed in a plain muslin jama over gold paijama, with a 'tulvar' in a red velvet scabbard hanging from his jewelled belt, and holds out his hands respectfully, palms together. The plain green ground merges into blue sky streaked with gold at the top.

BL3298401

Raja Jai Singh of Amber (reg. c.1621-1667), aged about 60, dressed in a green jama and gold embroidered paijama, seated on a gilt and painted chair, his bare feet on a purple cushion, one hand held out to a young man standing before him. The latter is dressed in a plain muslin jama over gold paijama, with a 'tulvar' in a red velvet scabbard hanging from his jewelled belt, and holds out his hands respectfully, palms together. The plain green ground merges into blue sky streaked with gold at the top.

BL3298401

 
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Figure 170: Royal dress. As worn at the late procession to St. Paul's.Chiffenet of gold net, ornamented with gold chain, cords and tassels; five ostrich feathers placed at the top of the head, and a diamond anchor in the front. Petticoat of rich point lace, bordered with white satin and scarlet velvet, and trimmed with a deep gold fringe. Robe of purple satin, short close sleeves, trimmed with narrow point ruffles; the whole bordered with scarlet velvet and a rich gold fringe. Tucker of point lace. Belt of solid gold. Diamond ear-rings and necklace, with a medallion. White gloves and shoes, embroidered in gold.

BL3294782

Figure 170: Royal dress. As worn at the late procession to St. Paul's.Chiffenet of gold net, ornamented with gold chain, cords and tassels; five ostrich feathers placed at the top of the head, and a diamond anchor in the front. Petticoat of rich point lace, bordered with white satin and scarlet velvet, and trimmed with a deep gold fringe. Robe of purple satin, short close sleeves, trimmed with narrow point ruffles; the whole bordered with scarlet velvet and a rich gold fringe. Tucker of point lace. Belt of solid gold. Diamond ear-rings and necklace, with a medallion. White gloves and shoes, embroidered in gold.

BL3294782

 
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Fashion plates of woman wearing yellow, chiffon walking dress, with white fichu and gilet, and hat adorned with flowers, holding parasol, and red, ratine walking dress

DGA5187386

Fashion plates of woman wearing yellow, chiffon walking dress, with white fichu and gilet, and hat adorned with flowers, holding parasol, and red, ratine walking dress

DGA5187386

 
Horse's Head Nebula and IC 434 in Orion - The Horsehead nebula in Orion - The Horse's Head Nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - Earth light in the constellation Orion. Lower left is the reflexion nebula, NGC 2023. The Horsehead nebula is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. Here, we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel. The bright complex of dust and gas below the Horsehead reflects the light given off by the bright star near it's center and is one of the brightest examples of reflection nebulae in the northern sky. The central star is surrounded with a thin shell of hydrogen that glows red by emitting it's own light in a rare examp

R. Jay GaBany

PIX4622130

Horse's Head Nebula and IC 434 in Orion - The Horsehead nebula in Orion - The Horse's Head Nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - Earth light in the constellation Orion. Lower left is the reflexion nebula, NGC 2023. The Horsehead nebula is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. Here, we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel. The bright complex of dust and gas below the Horsehead reflects the light given off by the bright star near it's center and is one of the brightest examples of reflection nebulae in the northern sky. The central star is surrounded with a thin shell of hydrogen that glows red by emitting it's own light in a rare examp

R. Jay GaBany

PIX4622130

 
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Fashion plates of woman wearing blue cashmere skirt, fancy silk blouse and hat adorned with flowers, holding parasol, and orange, rep and guipure lace walking dress and black plumed hat

DGA5187387

Fashion plates of woman wearing blue cashmere skirt, fancy silk blouse and hat adorned with flowers, holding parasol, and orange, rep and guipure lace walking dress and black plumed hat

DGA5187387

 
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An Unknown Gentleman, called Lionel Tollemache, 3rd Earl of Dysart (1649-1727)

Lely, Peter (1618-80)

USB1155876

An Unknown Gentleman, called Lionel Tollemache, 3rd Earl of Dysart (1649-1727)

Lely, Peter (1618-80)

USB1155876

 
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standing statue of Tuthmosis III

Egyptian School

Sandro Vannini

SVA660250

standing statue of Tuthmosis III

Egyptian School

Sandro Vannini

SVA660250

 
The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in September 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. At NASA Kennedy Space Center's Payload Hazardous Servicing Facility, technicians from the Applied Physics Laboratory work on the New Horizons spacecraft. They have been installing side panels on the spacecraft. A series of interconnecting panels will enclose the spacecraft beneath the antenna to maintain safe operating temperatures in space. New Horizons will make the first recognition of Pluto and Charon - a “double planet”” and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 20

PIX4607326

The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in September 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. At NASA Kennedy Space Center's Payload Hazardous Servicing Facility, technicians from the Applied Physics Laboratory work on the New Horizons spacecraft. They have been installing side panels on the spacecraft. A series of interconnecting panels will enclose the spacecraft beneath the antenna to maintain safe operating temperatures in space. New Horizons will make the first recognition of Pluto and Charon - a “double planet”” and the last planet in our solar system to be visited by spacecraft. The mission will then visit one or more objects in the Kuiper Belt region beyond Neptune. New Horizons is scheduled to launch in January 2006, swing past Jupiter for a gravity boost and scientific studies in February or March 20

PIX4607326

 
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Design by Fred. A bolero and skirt; an autumn walking dress. It is made of fine faced cloth in a new tint which he has called "fauvette" The skirt has two flounces cut en forme. The bolero has a collar and double revers of white.: it ends in rounded points above the waist, each one cut a little shorter than its fellow and overlaid. It is fastened by three large turquoise buttons down the left side. The belt, the vest and the cravate are all of turquoise blue. The three-cornered black felt hat is edged with a line of felt in white and trimmed on one side with a large chou of ribbon.

BL3302217

Design by Fred. A bolero and skirt; an autumn walking dress. It is made of fine faced cloth in a new tint which he has called "fauvette" The skirt has two flounces cut en forme. The bolero has a collar and double revers of white.: it ends in rounded points above the waist, each one cut a little shorter than its fellow and overlaid. It is fastened by three large turquoise buttons down the left side. The belt, the vest and the cravate are all of turquoise blue. The three-cornered black felt hat is edged with a line of felt in white and trimmed on one side with a large chou of ribbon.

BL3302217

 
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Antiquaries at Pola: Sir Henry Mainwaring Bt (1726-1797), Jacob Houblon (b.1736), George Harry Grey, 5th Earl of Stamford (1737-1819) and the Reverend Jonan Lipyeatt

Patch, Thomas (1720-82)

USB1162605

Antiquaries at Pola: Sir Henry Mainwaring Bt (1726-1797), Jacob Houblon (b.1736), George Harry Grey, 5th Earl of Stamford (1737-1819) and the Reverend Jonan Lipyeatt

Patch, Thomas (1720-82)

USB1162605

 
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Sir Thomas Hervey (c.1515/20 - 1575)

English School, (18th century)

USB1156594

Sir Thomas Hervey (c.1515/20 - 1575)

English School, (18th century)

USB1156594

 
The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in December 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In the Payload Hazardous Servicing Facility, the New Horizons spacecraft waits for encapsulation within the fairing sections waiting nearby. The fairing protects the spacecraft during launch and flight through the atmosphere. Once out of the atmosphere, the fairing is jettisoned. The compact 1,060 - pound New Horizons probe carries seven scientific instruments that will characterize the global geology and geomorphology of Pluto and its moon Charon, map their surface compositions and temperatures, and examine Pluto's complex atmosphere. After that, flybys of Kuiper Belt objects from even farther in the solar system may be undertaken in an extended mission. New Horizons is the first mission in Nasa's New Frontiers progra

PIX4607348

The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in December 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In the Payload Hazardous Servicing Facility, the New Horizons spacecraft waits for encapsulation within the fairing sections waiting nearby. The fairing protects the spacecraft during launch and flight through the atmosphere. Once out of the atmosphere, the fairing is jettisoned. The compact 1,060 - pound New Horizons probe carries seven scientific instruments that will characterize the global geology and geomorphology of Pluto and its moon Charon, map their surface compositions and temperatures, and examine Pluto's complex atmosphere. After that, flybys of Kuiper Belt objects from even farther in the solar system may be undertaken in an extended mission. New Horizons is the first mission in Nasa's New Frontiers progra

PIX4607348

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