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Images of 'Reticulum' found, 24

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with Siding Spring's 3.9m telescope. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual galaxy. NGC 1313 is at a distance of about 15 million light years, close enough for some of its brightest stars to be seen as individuals
 
Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with Siding Spring's 3.9m telescope. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual gal

PIX4609773

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with Siding Spring's 3.9m telescope. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual gal

PIX4609773

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual galaxy. NGC 1313 is at a distance of about 15 million light years, close enough for some of its brightest stars to be seen as individuals
 
Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual galaxy. NGC 1313 is at a distance of about 15 milli

R. Gendler

PIX4609785

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual galaxy. NGC 1313 is at a distance of about 15 milli

R. Gendler

PIX4609785

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with Siding Spring's 3.9m telescope. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual galaxy. NGC 1313 is at a distance of about 15 million light years, close enough for some of its brightest stars to be seen as individuals
 
Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with Siding Spring's 3.9m telescope. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual gal

PIX4609776

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with Siding Spring's 3.9m telescope. In visible light, NGC 1313 seems dominated by scattered patches of star formation which give our picture a rather ragged appearance. The clouds of bluish stars seem to have burst into existence at random, without the normal trigger gravitational interaction or even a distinct spiral to prompt them. Star formation seems to have occurred in a series of irregular, self-sustaining bursts. However, a very deep image shows that the outer parts of galaxy are also very disturbed. Seen with a radio telescope, the galaxy is rich in hydrogen, the raw material of stars, and the gas circulates around the centre of the galaxy in a well ordered way, apparently hardly affected by the starburst activity or other irregularities that so colour our visual impression of this unusual gal

PIX4609776

Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way
 
Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way

PIX4593550

Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way

PIX4593550

Model of animal cell, including cell nucleus, golgi body, lysosomes, centrioles, mitochondria, endoplasmic reticulum, ribosomes, cytoplasm, vesicles, thin plasma membrane, and microvilli (projections) at top
 
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Model of animal cell, including cell nucleus, golgi body, lysosomes, centrioles, mitochondria, endoplasmic reticulum, ribosomes, cytoplasm, vesicles, thin plasma membrane, and microvilli (projections) at top

UDK844365

Model of animal cell, including cell nucleus, golgi body, lysosomes, centrioles, mitochondria, endoplasmic reticulum, ribosomes, cytoplasm, vesicles, thin plasma membrane, and microvilli (projections) at top

UDK844365

Large and Small Magellan Clouds - Large and Small Magellanic clouds - These two irregular galaxies are close to our galaxy. Visible in the southern hemisphere, they are located approximately 160,000 (Grand Cloud, right) and 240,000 light years (Small Cloud, left). The Magellanic Clouds are the nearest galaxies to the Milky Way, about 170,000 and 240,000 light years distant respectively. They are in the far southern sky, practically invisible from northern latitudes, and their low surface brightness makes them difficult to see unless they are high in the sky. Both Magellanic Clouds are less than 25 degrees from the South Celestial Pole and are visible at some time on any clear, dark night from Siding Spring, where this picture was taken. To the dark adapted eye the Magellanic Clouds look like detached pieces of the Milky Way, but this apparent detachment is misleading because both are in orbit around it. Although the Magellanic Clouds are separate galaxies they are interacting with each other and with the Milky Way itself. Already the SMC has been substantially disrupted by this process, and the LMC distorted. Eventually the galaxies will merge with each other and with the Milky Way itself
 
Large and Small Magellan Clouds - Large and Small Magellanic clouds - These two irregular galaxies are close to our galaxy. Visible in the southern hemisphere, they are located approximately 160,000 (Grand Cloud, right) and 240,000 light years (Small Cloud, left). The Magellanic Clouds are the nearest galaxies to the Milky Way, about 170,000 and 240,000 light years distant respectively. They are in the far southern sky, practically invisible from northern latitudes, and their low surface brightness makes them difficult to see unless they are high in the sky. Both Magellanic Clouds are less than 25 degrees from the South Celestial Pole and are visible at some time on any clear, dark night from Siding Spring, where this picture was taken. To the dark adapted eye the Magellanic Clouds look like detached pieces of the Milky Way, but this apparent detachment is misleading because both are in orbit around it. Although the Magellanic Clouds are separate galaxies they are interacting with each

PIX4613338

Large and Small Magellan Clouds - Large and Small Magellanic clouds - These two irregular galaxies are close to our galaxy. Visible in the southern hemisphere, they are located approximately 160,000 (Grand Cloud, right) and 240,000 light years (Small Cloud, left). The Magellanic Clouds are the nearest galaxies to the Milky Way, about 170,000 and 240,000 light years distant respectively. They are in the far southern sky, practically invisible from northern latitudes, and their low surface brightness makes them difficult to see unless they are high in the sky. Both Magellanic Clouds are less than 25 degrees from the South Celestial Pole and are visible at some time on any clear, dark night from Siding Spring, where this picture was taken. To the dark adapted eye the Magellanic Clouds look like detached pieces of the Milky Way, but this apparent detachment is misleading because both are in orbit around it. Although the Magellanic Clouds are separate galaxies they are interacting with each

PIX4613338

Barree spiral galaxy NGC 1559 and supernova - Barred spiral galaxy NGC 1559 with a supernova - The galaxy NGC 1559 is a galaxy of Seyfert located about 50 million years ago - light in the constellation Reticule. In this image obtained in 2005 by the Kueyen European telescope of the VLT in Chile, a bright star is visible just above the galaxy, a supernova of type Ia named SN 2005df. On the night of August 4, 2005, an amateur astronomer and supernovae discoverer Reverend Robert Evans discovered a supernova just North of this galaxy. This supernova is classified as a somewhat unusual type Ia supernova, caught probably 10 days before it reached its maximum brightness. Such a supernova is thought to be the result of the explosion of a small and dense star - a white dwarf - inside a binary system. As its companion was continuously spilling matter onto the white dwarf, the white dwarf reached a critical mass, leading to a fatal instability. NGC 1559 is a SBc (s) - type spiral galaxy located about 50 million light - years away, that weighs the equivalent of about 10,000 million of suns, and is about 7 times smaller than our Milky Way. Receding from us at a speed of about 1,300 km/s, it is a galaxy of the Seyfert type. Such galaxies are characterized by a bright nucleus that radiates strongly in the blue and in the ultraviolet. Astronomers think that about 2 solar masses of gas per year are transformed into stars in this galaxy. Like most galaxies, NGC 1559 probably contains a black hole in its centre, which should have a mass that is equivalent to 300,000 suns. Colour composite image obtained with the multi - mode FORS1 instrument on ESO's 8.2m VLT. The supernova, SN 2005df, is visible as the bright star just above the galaxy
 
Barree spiral galaxy NGC 1559 and supernova - Barred spiral galaxy NGC 1559 with a supernova - The galaxy NGC 1559 is a galaxy of Seyfert located about 50 million years ago - light in the constellation Reticule. In this image obtained in 2005 by the Kueyen European telescope of the VLT in Chile, a bright star is visible just above the galaxy, a supernova of type Ia named SN 2005df. On the night of August 4, 2005, an amateur astronomer and supernovae discoverer Reverend Robert Evans discovered a supernova just North of this galaxy. This supernova is classified as a somewhat unusual type Ia supernova, caught probably 10 days before it reached its maximum brightness. Such a supernova is thought to be the result of the explosion of a small and dense star - a white dwarf - inside a binary system. As its companion was continuously spilling matter onto the white dwarf, the white dwarf reached a critical mass, leading to a fatal instability. NGC 1559 is a SBc (s) - type spiral galaxy located a

PIX4609916

Barree spiral galaxy NGC 1559 and supernova - Barred spiral galaxy NGC 1559 with a supernova - The galaxy NGC 1559 is a galaxy of Seyfert located about 50 million years ago - light in the constellation Reticule. In this image obtained in 2005 by the Kueyen European telescope of the VLT in Chile, a bright star is visible just above the galaxy, a supernova of type Ia named SN 2005df. On the night of August 4, 2005, an amateur astronomer and supernovae discoverer Reverend Robert Evans discovered a supernova just North of this galaxy. This supernova is classified as a somewhat unusual type Ia supernova, caught probably 10 days before it reached its maximum brightness. Such a supernova is thought to be the result of the explosion of a small and dense star - a white dwarf - inside a binary system. As its companion was continuously spilling matter onto the white dwarf, the white dwarf reached a critical mass, leading to a fatal instability. NGC 1559 is a SBc (s) - type spiral galaxy located a

PIX4609916

Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way
 
Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way

PIX4593553

Constellations of Reticulum and Dorado - Constellations of Reticulum and Dorado - Constellations of Reticulum and Bream (top) near the galaxy of the Great Magellan Cloud. Reticulum is another small and insignificant southern constellation introduced by Lacaille in the 1750s. It commemorates a reticle, the cross hairs in an eyepiece used for measuring star positions, from the Latin for 'net' (hence reticulation, network). It is best found by looking for the Large Magellanic Cloud in the adjoining constellation of Dorado. Dorado, the Goldfish or Swordfish (Xiphias), is a constellation introduced by Johann Bayer, best known for his 1603 star atlas Uranometria, which was the first to cover the entire sky. It is notable mainly for containing most of the Large Magellanic Cloud (LMC), the nearest galaxy to the Milky Way

PIX4593553

Constellation of Carene and other constellations of the southern hemisphere - Southern constellations with Large and Small Magellanic clouds - Carene, cameleon, flying fish, painter, seam, table, reticule, bird of paradise, octant, male hydra, Toucan and part of the horlog
 
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Constellation of Carene and other constellations of the southern hemisphere - Southern constellations with Large and Small Magellanic clouds - Carene, cameleon, flying fish, painter, seam, table, reticule, bird of paradise, octant, male hydra, Toucan and part of the horlog

S. Numazawa

PIX4589536

Constellation of Carene and other constellations of the southern hemisphere - Southern constellations with Large and Small Magellanic clouds - Carene, cameleon, flying fish, painter, seam, table, reticule, bird of paradise, octant, male hydra, Toucan and part of the horlog

S. Numazawa

PIX4589536

Cross-section of a cell (colour litho)
 
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Cross-section of a cell (colour litho)

Italian School, (20th century)

DGA441118

Cross-section of a cell (colour litho)

Italian School, (20th century)

DGA441118

Constellations near the south pole - Constellations near southern celestial pole - Image obtained from New Zealand
 
Constellations near the south pole - Constellations near southern celestial pole - Image obtained from New Zealand

Christopher Picking

PIX4594573

Constellations near the south pole - Constellations near southern celestial pole - Image obtained from New Zealand

Christopher Picking

PIX4594573

Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination
 
Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination

PIX4590607

Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination

PIX4590607

Southern constellations around the Clock - Southern constellations around Horologium - Southern constellations around the Clock. The two bright stars are Canopus (bottom) and Achernar. This wide angle image includes Horologium, Phoenix and Pictor, insignificant constellations roughly centred on an arc of delination 50* south, but at a scale too small to show the star identifications and stick figures. Horologium, the Pendulum Clock (originally l'Horloge and then Horologium Oscillitorium), was a constellation introduced by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It was named to honor Christian Huygens as the inventor of this type of clock, but the idea for such a method of regulating time came from Galileo. Lacaille's constellation drawing shows a remarkably detailed dial, weights and a pendulum that has little apparent connection with the scattering of faint stars in this part of the sky. There are no named stars and little else in Horologium to attract the eye of the casual observer. Phoenix, the Phoenix, is a long - lived mythological, eagle - like bird with vivid plumage. The word has entered the language as an entity that is able to resurrect itself after a firey death in its nest. The cycle of death and rebirth may have symbolised the rising and setting of the Sun. On the sky Phoenix is hemmed in on two sides by other birds in Grus and Tucana and a large snake in the form of Eridanus. The constellation was invented by the Dutch navigators Pieter Dirkszoon Keyser and Frederick de Houtman, and first appeared in Johan Beyer's altas of 1603. The only named star in Phoenix is Ankaa. Pictor was also named by Lacaille during his sojourn at the Cape of Good Hope. He originally called it le Easel et la Palette, the easel and palette and later Equuleus Pictorius, soon shortened to Pictor. It requires the imagination of an artist to find anything like an easle here. The constellation runs between Ca
 
Southern constellations around the Clock - Southern constellations around Horologium - Southern constellations around the Clock. The two bright stars are Canopus (bottom) and Achernar. This wide angle image includes Horologium, Phoenix and Pictor, insignificant constellations roughly centred on an arc of delination 50* south, but at a scale too small to show the star identifications and stick figures. Horologium, the Pendulum Clock (originally l'Horloge and then Horologium Oscillitorium), was a constellation introduced by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It was named to honor Christian Huygens as the inventor of this type of clock, but the idea for such a method of regulating time came from Galileo. Lacaille's constellation drawing shows a remarkably detailed dial, weights and a pendulum that has little apparent connection with the scattering of faint stars in this part of the sky. There are no named stars and little else in

PIX4594625

Southern constellations around the Clock - Southern constellations around Horologium - Southern constellations around the Clock. The two bright stars are Canopus (bottom) and Achernar. This wide angle image includes Horologium, Phoenix and Pictor, insignificant constellations roughly centred on an arc of delination 50* south, but at a scale too small to show the star identifications and stick figures. Horologium, the Pendulum Clock (originally l'Horloge and then Horologium Oscillitorium), was a constellation introduced by Abbe Nicolas Louis de Lacaille during his stay at the Cape of Good Hope between 1751 and 1752. It was named to honor Christian Huygens as the inventor of this type of clock, but the idea for such a method of regulating time came from Galileo. Lacaille's constellation drawing shows a remarkably detailed dial, weights and a pendulum that has little apparent connection with the scattering of faint stars in this part of the sky. There are no named stars and little else in

PIX4594625

Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination
 
Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination

PIX4590625

Constellation of Eridan - Constellation of Eridanus - View from the Hyadas to the Hydra Male. In the center is the great constellation of Eridan. The brightest stars visible here are Rigel, Sirius, Canopus and Achernar. In the center of image is the Eridanus constellation. Brightest stars visible are Rigel (top in Orion); Sirius (top left); Canopus (below) and Achernar (bottom center). Eridanus (the Celestial River) is very well named; since it winds its way over an enormous area of the sky. It is the 6th largest constellation (almost 1140 square degrees) and wanders over a huge range of Declination. The river runs from close to the celestial equator (which runs through Orion's Belt) to its brightest star Achernar (a Eri; from the English for 'river's end'); which is at 57* south declination

PIX4590625

Sea mat, Conopeum reticulum (Reticulated millepore, Millepora reticulata). Illustration drawn and engraved by Richard Polydore Nodder. Handcoloured copperplate engraving from George Shaw and Frederick Nodder's “” The Naturalist's Miscellany,”” London, 1810.
 
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Sea mat, Conopeum reticulum (Reticulated millepore, Millepora reticulata). Illustration drawn and engraved by Richard Polydore Nodder. Handcoloured copperplate engraving from George Shaw and Frederick Nodder's “” The Naturalist's Miscellany,”” London, 1810.

FLO4683751

Sea mat, Conopeum reticulum (Reticulated millepore, Millepora reticulata). Illustration drawn and engraved by Richard Polydore Nodder. Handcoloured copperplate engraving from George Shaw and Frederick Nodder's “” The Naturalist's Miscellany,”” London, 1810.

FLO4683751

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