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Images of 'Corona Australis' found, 36

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NGC 6541 in the Southern Crown - Globular cluster NGC 6541 in Corona Australis - This cluster of stars is located about 23,000 years from Earth. Globular cluster located at about 23,000 light years away

NGC 6541 in the Southern Crown - Globular cluster NGC 6541 in Corona Australis - This cluster of stars is located about 23,000 years from Earth. Globular cluster located at about 23,000 light years away

Vincent Toporenko

PIX4564884

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australia

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australia

PIX4593578

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australia

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australia

PIX4593592

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australis - From ancient times the constellation of Sagittarius (the Archer) was represented as a Centaur, half man, half horse, ready to fire his/its bow and arrow at the heart of Scorpius, the Scorpion. The constellation is the 15th largest in the sky and covers about 867 square degrees, including the brightest part of the Milky Way. It contains no fewer than 15 Messier objects. Sagittarius is a zodiacal constellation, so the ecliptic, the apparent path of the Sun, among the stars, pases through it, between M8 and M20. The much smaller constellation of Corona Australis (the Southern Crown) is quite distinctive to the eye though its stars are fainter than those in neighbouring Sagittarius. It is quite ancient having be recognised by Ptolemy, and one legend has it that it represents the coronet worn by Sagittarius. Who knows. It is 80th in size among the 88 constellations and covers 128 squa

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australis - From ancient times the constellation of Sagittarius (the Archer) was represented as a Centaur, half man, half horse, ready to fire his/its bow and arrow at the heart of Scorpius, the Scorpion. The constellation is the 15th largest in the sky and covers about 867 square degrees, including the brightest part of the Milky Way. It contains no fewer than 15 Messier objects. Sagittarius is a zodiacal constellation, so the ecliptic, the apparent path of the Sun, among the stars, pases through it, between M8 and M20. The much smaller constellation of Corona Australis (the Southern Crown) is quite distinctive to the eye though its stars are fainter than those in neighbouring Sagittarius. It is quite ancient having be recognised by Ptolemy, and one legend has it that it represents the coronet worn by Sagittarius. Who knows. It is 80th in size among the 88 constellations and covers 128 squa

PIX4593652

Constellations of Telescope, Altar and Southern Crown - Constellations of Telescopium, Ara and Corona Australis - The Telescope is a small constellation of the southern hemisphere located under the Southern Crown. To his right is the constellation of the Altar. Telescopium is a faint constellation that was named by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It is utterly undistinguished and is best remembered as that unremarkable piece of sky to the west of Ara and between the distinctive circlet of Corona Australis and Peacock (alpha Pavonis), the brightest star in Pavo. Lacaille's original name was Tubus Telescopium, however, in the way of antique telescopes, it was shortened for convenience

Constellations of Telescope, Altar and Southern Crown - Constellations of Telescopium, Ara and Corona Australis - The Telescope is a small constellation of the southern hemisphere located under the Southern Crown. To his right is the constellation of the Altar. Telescopium is a faint constellation that was named by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It is utterly undistinguished and is best remembered as that unremarkable piece of sky to the west of Ara and between the distinctive circlet of Corona Australis and Peacock (alpha Pavonis), the brightest star in Pavo. Lacaille's original name was Tubus Telescopium, however, in the way of antique telescopes, it was shortened for convenience

PIX4594224

Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Othe

Southern Crown Nebula - The CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clouds'), blotting out the background stars. Fainter features can be seen here. Shiny NGC 6726 - 27 near middle of image contains both a visual binary and a variable star. Othe

PIX4620295

Star births in the nebula NGC 6729 - Young stars in the nebula NGC 6729 - Close up on a star-forming region. The new stars are invisible, hidden behind the dust cloud at the top left of the image, but the material they eject at very high speed causes colorful and luminous arcs in contact with the surrounding gas. Image obtained in Chile with the VLT. This very detailed false - colour image from Eso's Very Large Telescope shows the dramatic effects of very young stars on the dust and gas from which they were born in the star - forming region NGC 6729. The baby stars are invisible in this picture, being hidden behind dust clouds at the upper left of the picture, but material they are ejecting is crashing into the surroundings at speeds of that can be as high as one million kilometres per hour. These shocks cause the gas to shine and create the strangely coloured glowing arcs and blobs known as Herbig - Haro objects. In this view the Herbig - Haro objects form two lines marking out the pr

Star births in the nebula NGC 6729 - Young stars in the nebula NGC 6729 - Close up on a star-forming region. The new stars are invisible, hidden behind the dust cloud at the top left of the image, but the material they eject at very high speed causes colorful and luminous arcs in contact with the surrounding gas. Image obtained in Chile with the VLT. This very detailed false - colour image from Eso's Very Large Telescope shows the dramatic effects of very young stars on the dust and gas from which they were born in the star - forming region NGC 6729. The baby stars are invisible in this picture, being hidden behind dust clouds at the upper left of the picture, but material they are ejecting is crashing into the surroundings at speeds of that can be as high as one million kilometres per hour. These shocks cause the gas to shine and create the strangely coloured glowing arcs and blobs known as Herbig - Haro objects. In this view the Herbig - Haro objects form two lines marking out the pr

PIX4620300

Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clou

Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clou

PIX4620260

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 ne

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 ne

PIX4620317

Constellations of Sagittarius, Southern Crown, Microscope and Telescope - Constellation of Sagittarius - Plate extracted from the Mirror of Urania by Jehoshaphat Aspin - 1825 Represented with constellations of Corona Australis, Telescopium and Microscopium. Urania's Mirror, by Jehoshaphat Aspin, 1825

Constellations of Sagittarius, Southern Crown, Microscope and Telescope - Constellation of Sagittarius - Plate extracted from the Mirror of Urania by Jehoshaphat Aspin - 1825 Represented with constellations of Corona Australis, Telescopium and Microscopium. Urania's Mirror, by Jehoshaphat Aspin, 1825

PIX4593666

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australia

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australia

PIX4593590

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australis - From ancient times the constellation of Sagittarius (the Archer) was represented as a Centaur, half man, half horse, ready to fire his/its bow and arrow at the heart of Scorpius, the Scorpion. The constellation is the 15th largest in the sky and covers about 867 square degrees, including the brightest part of the Milky Way. It contains no fewer than 15 Messier objects. Sagittarius is a zodiacal constellation, so the ecliptic, the apparent path of the Sun, among the stars, pases through it, between M8 and M20. The much smaller constellation of Corona Australis (the Southern Crown) is quite distinctive to the eye though its stars are fainter than those in neighbouring Sagittarius. It is quite ancient having be recognised by Ptolemy, and one legend has it that it represents the coronet worn by Sagittarius. Who knows. It is 80th in size among the 88 constellations and covers 128 squa

Constellations of Sagittarius and the Southern Crown - Constellations of Sagittarius and Corona Australis - From ancient times the constellation of Sagittarius (the Archer) was represented as a Centaur, half man, half horse, ready to fire his/its bow and arrow at the heart of Scorpius, the Scorpion. The constellation is the 15th largest in the sky and covers about 867 square degrees, including the brightest part of the Milky Way. It contains no fewer than 15 Messier objects. Sagittarius is a zodiacal constellation, so the ecliptic, the apparent path of the Sun, among the stars, pases through it, between M8 and M20. The much smaller constellation of Corona Australis (the Southern Crown) is quite distinctive to the eye though its stars are fainter than those in neighbouring Sagittarius. It is quite ancient having be recognised by Ptolemy, and one legend has it that it represents the coronet worn by Sagittarius. Who knows. It is 80th in size among the 88 constellations and covers 128 squa

PIX4593659

Southern Crown Nebula - The Corona Australis nebula (NGC 6726 - 27 - 29) - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. Image made with Siding Spring's 3.9m telescope. This spectacular reflection nebula is the result of a few bright stars caught up in a large, dusty cloud. If that is all there was here, this region would be considered to be like the Pleiades, an accidental association of dust and stars. However, there are features here that show the dark cloud to be an active star forming nebula, though most of the action is hidden from view. The peculiar yellowish curved streak near the two bright reflection nebulae surround an intriguing object best seen in infrared light, R CRA, a young star still accreting interstellar material on to its surface. It seems to be the source of two compact but distinctly red patches which are Herbig - Haro objects, often the first visible signs of star forma

Southern Crown Nebula - The Corona Australis nebula (NGC 6726 - 27 - 29) - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. Image made with Siding Spring's 3.9m telescope. This spectacular reflection nebula is the result of a few bright stars caught up in a large, dusty cloud. If that is all there was here, this region would be considered to be like the Pleiades, an accidental association of dust and stars. However, there are features here that show the dark cloud to be an active star forming nebula, though most of the action is hidden from view. The peculiar yellowish curved streak near the two bright reflection nebulae surround an intriguing object best seen in infrared light, R CRA, a young star still accreting interstellar material on to its surface. It seems to be the source of two compact but distinctly red patches which are Herbig - Haro objects, often the first visible signs of star forma

PIX4620228

Constellations of Telescope, Altar and Southern Crown - Constellations of Telescopium, Ara and Corona Australis - The Telescope is a small constellation of the southern hemisphere located between the Southern Crown (at the top) and the constellation of the Altar (at the bottom of the picture). Telescopium is a faint constellation that was named by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It is utterly undistinguished and is best remembered as that unremarkable piece of sky to the west of Ara and between the distinctive circlet of Corona Australis and Peacock (alpha Pavonis), the brightest star in Pavo. Lacaille's original name was Tubus Telescopium, however, in the way of antique telescopes, it was shortened for convenience

Constellations of Telescope, Altar and Southern Crown - Constellations of Telescopium, Ara and Corona Australis - The Telescope is a small constellation of the southern hemisphere located between the Southern Crown (at the top) and the constellation of the Altar (at the bottom of the picture). Telescopium is a faint constellation that was named by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It is utterly undistinguished and is best remembered as that unremarkable piece of sky to the west of Ara and between the distinctive circlet of Corona Australis and Peacock (alpha Pavonis), the brightest star in Pavo. Lacaille's original name was Tubus Telescopium, however, in the way of antique telescopes, it was shortened for convenience

PIX4594226

Corona Australis, constellation, Hemisphere 1559, Dele Stelle Fisse by A. Piccolomini, 1559 (engraving)

Corona Australis, constellation, Hemisphere 1559, Dele Stelle Fisse by A. Piccolomini, 1559 (engraving)

TRK2598008

This image from NASA's WISE is a view of an area of the sky over 12 times the size of the full Moon on the border of the constellations Sagittarius and Corona Australis. Two types of star clusters are visible in the image.

This image from NASA's WISE is a view of an area of the sky over 12 times the size of the full Moon on the border of the constellations Sagittarius and Corona Australis. Two types of star clusters are visible in the image.

UIG867158

This image from NASA's WISE is a view of an area of the sky over 12 times the size of the full Moon on the border of the constellations Sagittarius and Corona Australis. Two types of star clusters are visible in the image.

This image from NASA's WISE is a view of an area of the sky over 12 times the size of the full Moon on the border of the constellations Sagittarius and Corona Australis. Two types of star clusters are visible in the image.

UIG867157

Corona Australis Dust Complex, 2017 (digital photo)

Corona Australis Dust Complex, 2017 (digital photo)

Cogo, Mario (21st century)

MMM7340922

Leo, Ara and Corona Australis. Illustrations to a treatise on astrology

Leo, Ara and Corona Australis. Illustrations to a treatise on astrology

BL3286288

Sagittarius and Corona Australis. Microscopium and Telescopium., c.1825 (card, paper, tissue)

Sagittarius and Corona Australis. Microscopium and Telescopium., c.1825 (card, paper, tissue)

Hall, Sydney (fl.1826)

MMM7340083

Sagittarius and Corona Australis, Microscopium, and Telescopium, Illustration from 'Urania's Mirror', 1825 (etching)

Sagittarius and Corona Australis, Microscopium, and Telescopium, Illustration from 'Urania's Mirror', 1825 (etching)

Hall, Sydney (fl.1826)

XOS7075939

Constellation of the Southern Crown - Constellation of Corona Australis - Constellation of the Southern Crown extracted from the Hevelius Uranographia. Recolorised image. Map showing the constellation of corona australis with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

Constellation of the Southern Crown - Constellation of Corona Australis - Constellation of the Southern Crown extracted from the Hevelius Uranographia. Recolorised image. Map showing the constellation of corona australis with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

Sebastien Beaucourt

PIX4590107

Southern Crown Nebula - NGC 6726 dust cloud region in Corona Australis - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, a more distant globular cluster, NGC 6723 in Sagittarius is about 30,000 light years away from Earth. The reflection nebulosity NGC 6726/6727/6729 is a star forming region in Corona Australis. To the northeast the globular cluster NGC 6723 in Sagittarius. North is up

Southern Crown Nebula - NGC 6726 dust cloud region in Corona Australis - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, a more distant globular cluster, NGC 6723 in Sagittarius is about 30,000 light years away from Earth. The reflection nebulosity NGC 6726/6727/6729 is a star forming region in Corona Australis. To the northeast the globular cluster NGC 6723 in Sagittarius. North is up

Stephane Guisard

PIX4620287

Sagittarius and Corona Australis, from 'Urania's Mirror; or, a View of the heavens. [A box of 32 cards.]' by Jehoshaphat Aspin, 1834 (colour litho)

Sagittarius and Corona Australis, from 'Urania's Mirror; or, a View of the heavens. [A box of 32 cards.]' by Jehoshaphat Aspin, 1834 (colour litho)

English School, (19th century)

BL3666643

Southern Crown Nebula - NGC 6726, Galactic Dust Cloud in Corona Australis - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, a more distant globular cluster, NGC 6723 in Sagittarius is about 30,000 light years away from Earth. The reflection nebulosity NGC 6726/6727/6729 is a star forming region in Corona Australis. To the northeast the globular cluster NGC 6723 in Sagittarius. North is up. Total Exposure 60 Hour

Southern Crown Nebula - NGC 6726, Galactic Dust Cloud in Corona Australis - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, a more distant globular cluster, NGC 6723 in Sagittarius is about 30,000 light years away from Earth. The reflection nebulosity NGC 6726/6727/6729 is a star forming region in Corona Australis. To the northeast the globular cluster NGC 6723 in Sagittarius. North is up. Total Exposure 60 Hour

PIX4620333

Globular cluster NGC 6723 in Sagittarius - Globular cluster NGC 6723 in Sagittarius - This cluster of stars is located about 30,000 years ago - light from Earth

Globular cluster NGC 6723 in Sagittarius - Globular cluster NGC 6723 in Sagittarius - This cluster of stars is located about 30,000 years ago - light from Earth

PIX4565034

Star Formation in the Southern Crown - A cluster of stars in the constellation of the Southern Crown seen in infrared by the Spitzer space telescope. R Coronae Australis is one of the closest and most intense star-forming regions; visible in the southern hemisphere, it is located about 500 light years away from Earth. The Corona Australis region (containing, at its heart, the Coronet cluster) is one of the nearest and most active regions of ongoing star formation. The infrared Spitzer image shows young stars more diffuse emission from dust

Star Formation in the Southern Crown - A cluster of stars in the constellation of the Southern Crown seen in infrared by the Spitzer space telescope. R Coronae Australis is one of the closest and most intense star-forming regions; visible in the southern hemisphere, it is located about 500 light years away from Earth. The Corona Australis region (containing, at its heart, the Coronet cluster) is one of the nearest and most active regions of ongoing star formation. The infrared Spitzer image shows young stars more diffuse emission from dust

PIX4620236

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) 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 sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). 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 - calle

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) 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 sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). 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 - calle

PIX4620222

Peacock Constellation - Constellation of Pavo - Pavo, the Peacock, lies south of Sagittarius and Corona Australis, and is one of Johann Bayer's twelve constellations, introduced in 1603. It is one of several birds in the southern sky, including Apus, Grus, Phoenix and Tucanae. The legends say that the goddess of the heavens, Juno (the Greek Hera) ordered a hundred - eyed giant, Argos Panoptes, to keep his eyes on her wandering husband, Jupiter. He ordered Argos slain and Juno transformed the 100 eyes into the Peacock's tail. These eyes are also meant to represent the starry sky

Peacock Constellation - Constellation of Pavo - Pavo, the Peacock, lies south of Sagittarius and Corona Australis, and is one of Johann Bayer's twelve constellations, introduced in 1603. It is one of several birds in the southern sky, including Apus, Grus, Phoenix and Tucanae. The legends say that the goddess of the heavens, Juno (the Greek Hera) ordered a hundred - eyed giant, Argos Panoptes, to keep his eyes on her wandering husband, Jupiter. He ordered Argos slain and Juno transformed the 100 eyes into the Peacock's tail. These eyes are also meant to represent the starry sky

PIX4593100

Peacock Constellation - Constellation of Pavo - Pavo, the Peacock, lies south of Sagittarius and Corona Australis, and is one of Johann Bayer's twelve constellations, introduced in 1603. It is one of several birds in the southern sky, including Apus, Grus, Phoenix and Tucanae. The legends say that the goddess of the heavens, Juno (the Greek Hera) ordered a hundred - eyed giant, Argos Panoptes, to keep his eyes on her wandering husband, Jupiter. He ordered Argos slain and Juno transformed the 100 eyes into the Peacock's tail. These eyes are also meant to represent the starry sky

Peacock Constellation - Constellation of Pavo - Pavo, the Peacock, lies south of Sagittarius and Corona Australis, and is one of Johann Bayer's twelve constellations, introduced in 1603. It is one of several birds in the southern sky, including Apus, Grus, Phoenix and Tucanae. The legends say that the goddess of the heavens, Juno (the Greek Hera) ordered a hundred - eyed giant, Argos Panoptes, to keep his eyes on her wandering husband, Jupiter. He ordered Argos slain and Juno transformed the 100 eyes into the Peacock's tail. These eyes are also meant to represent the starry sky

PIX4593107

Vini australis

NHM1459794

Southern Crown Nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, a more distant globular cluster, NGC 6723 cluster in Sagittarius is about 30,000 light years away from Earth

Southern Crown Nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, a more distant globular cluster, NGC 6723 cluster in Sagittarius is about 30,000 light years away from Earth

W. Promper

PIX4620263

Southern Crown Nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, a more distant globular cluster, NGC 6723 in Sagittarius is about 30,000 light years away from Earth. Image obtained at Mount Palomar and recolorized

Southern Crown Nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, a more distant globular cluster, NGC 6723 in Sagittarius is about 30,000 light years away from Earth. Image obtained at Mount Palomar and recolorized

Vincent Toporenko

PIX4620258

f.13 Blue-crowned Lory (Vini australis) painted while accompanying Captain James Cook on his third voyage 1776-78 (w/c)

f.13 Blue-crowned Lory (Vini australis) painted while accompanying Captain James Cook on his third voyage 1776-78 (w/c)

Ellis, William (18th century)

NHM87728

Southern Crown Nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Schmidt UK Telescope by Siding Spring

Southern Crown Nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Schmidt UK Telescope by Siding Spring

PIX4620237

Lori craving. Copper engraving, coloured, signed N for Frederick Polydor Nodder (1751-1801) for the naturalist collection, published in 1790 by George Shaw. Purple headed parakeet, with purple head, crimson cheeks and legs, green wings and body. Blue crowned lorikeet, Vini australis (Psittacus porphyrocephalus). Handcolored copperplate engraving, illustration signed N (Frederick Polydor Nodder (1751-1801), artist and engraver) from George Shaw's “” Naturalist's Miscellany”” (1790).

Lori craving. Copper engraving, coloured, signed N for Frederick Polydor Nodder (1751-1801) for the naturalist collection, published in 1790 by George Shaw. Purple headed parakeet, with purple head, crimson cheeks and legs, green wings and body. Blue crowned lorikeet, Vini australis (Psittacus porphyrocephalus). Handcolored copperplate engraving, illustration signed N (Frederick Polydor Nodder (1751-1801), artist and engraver) from George Shaw's “” Naturalist's Miscellany”” (1790).

FLO4684122

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