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Frontispiece of Elnava o L'assedio di Leida by Errico Petrella, 1856
Frontispiece of Elnava o L'assedio di Leida by Errico Petrella, 1856

LRI4567299: Frontispiece of Elnava o L'assedio di Leida by Errico Petrella, 1856, Anonymous / Bridgeman Images

ID: LRI4567299

Frontispiece of Elnava o L'assedio di Leida by Errico Petrella, 1856

Anonymous

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses
Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

PIX4567320: Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses / Bridgeman Images

ID: PIX4567320

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses
Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

PIX4567349: Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses / Bridgeman Images

ID: PIX4567349

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

Eclipse de Soleil observee par projection - Solar eclipse observation - Total eclipse of Sun of 29 March 2006. Partial phase of the projected eclipse using a pair of binoculars. Total solar eclipse, March 29, 2006, Turkey. Partial phase projected by binoculars
Eclipse de Soleil observee par projection - Solar eclipse observation - Total eclipse of Sun of 29 March 2006. Partial phase of the projected eclipse using a pair of binoculars. Total solar eclipse, March 29, 2006, Turkey. Partial phase projected by binoculars

PIX4567359: Eclipse de Soleil observee par projection - Solar eclipse observation - Total eclipse of Sun of 29 March 2006. Partial phase of the projected eclipse using a pair of binoculars. Total solar eclipse, March 29, 2006, Turkey. Partial phase projected by binoculars / Bridgeman Images

ID: PIX4567359

Eclipse de Soleil observee par projection - Solar eclipse observation - Total eclipse of Sun of 29 March 2006. Partial phase of the projected eclipse using a pair of binoculars. Total solar eclipse, March 29, 2006, Turkey. Partial phase projected by binoculars

Cite de l'espace - Toulouse - The Cite de l'Espace is a theme park located in Toulouse, inaugurated in June 1997
Cite de l'espace - Toulouse - The Cite de l'Espace is a theme park located in Toulouse, inaugurated in June 1997

PIX4567395: Cite de l'espace - Toulouse - The Cite de l'Espace is a theme park located in Toulouse, inaugurated in June 1997 / Bridgeman Images

ID: PIX4567395

Cite de l'espace - Toulouse - The Cite de l'Espace is a theme park located in Toulouse, inaugurated in June 1997

First page of musical score of a Symphony in D major by Pleyel
First page of musical score of a Symphony in D major by Pleyel

LRI4567426: First page of musical score of a Symphony in D major by Pleyel, Pleyel, Joseph Ignace (1757-1831) / Bridgeman Images

ID: LRI4567426

First page of musical score of a Symphony in D major by Pleyel

Pleyel, Joseph Ignace (1757-1831)

Cubic houses in Rotterdam (Netherlands). Construction 1984, architect Piet Blom.
Cubic houses in Rotterdam (Netherlands). Construction 1984, architect Piet Blom.

TEC4568376: Cubic houses in Rotterdam (Netherlands). Construction 1984, architect Piet Blom., Blom, Piet (1934-1999) / Bridgeman Images

ID: TEC4568376

Cubic houses in Rotterdam (Netherlands). Construction 1984, architect Piet Blom.

Blom, Piet (1934-1999)

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.
The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

TEC4568398: The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine. / Bridgeman Images

ID: TEC4568398

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

Gallo, Roman art: bronze statuettes of naked man and dancer, from the Tresor of Neuvy, en, Sullias (Loiret), 3rd century (bronze)
Gallo, Roman art: bronze statuettes of naked man and dancer, from the Tresor of Neuvy, en, Sullias (Loiret), 3rd century (bronze)

JLJ4568406: Gallo, Roman art: bronze statuettes of naked man and dancer, from the Tresor of Neuvy, en, Sullias (Loiret), 3rd century (bronze), Gallo-Roman (3rd century) / Bridgeman Images

ID: JLJ4568406

Gallo, Roman art: bronze statuettes of naked man and dancer, from the Tresor of Neuvy, en, Sullias (Loiret), 3rd century (bronze)

Gallo-Roman (3rd century)

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.
The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

TEC4568435: The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine. / Bridgeman Images

ID: TEC4568435

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

Chess players Engraving by Henry Monnier (1805-1877), 19th century (engraving)
Chess players Engraving by Henry Monnier (1805-1877), 19th century (engraving)

JLJ4568450: Chess players Engraving by Henry Monnier (1805-1877), 19th century (engraving), Monnier, Henri Bonaventure (1799-1877) / Bridgeman Images

ID: JLJ4568450

Chess players Engraving by Henry Monnier (1805-1877), 19th century (engraving)

Monnier, Henri Bonaventure (1799-1877)

The Ice Scene de rue in Paris during the winter, a clerk slides on the floorboard because of the ice, as well as a horse pulling a carriage, 20th century (chromolithograph)
The Ice Scene de rue in Paris during the winter, a clerk slides on the floorboard because of the ice, as well as a horse pulling a carriage, 20th century (chromolithograph)

JLJ4568483: The Ice Scene de rue in Paris during the winter, a clerk slides on the floorboard because of the ice, as well as a horse pulling a carriage, 20th century (chromolithograph), French School, (20th century) / Bridgeman Images

ID: JLJ4568483

The Ice Scene de rue in Paris during the winter, a clerk slides on the floorboard because of the ice, as well as a horse pulling a carriage, 20th century (chromolithograph)

French School, (20th century)

Page of musical score of Psalm 23, op 132, D 706 by Franz Schubert
Page of musical score of Psalm 23, op 132, D 706 by Franz Schubert

LRI4568506: Page of musical score of Psalm 23, op 132, D 706 by Franz Schubert / Bridgeman Images

ID: LRI4568506

Page of musical score of Psalm 23, op 132, D 706 by Franz Schubert

Feminism: 'Speech for Women's Empowerment in the United States' A young woman standing on a barrel claim women's rights, 19th century (engraving)
Feminism: 'Speech for Women's Empowerment in the United States' A young woman standing on a barrel claim women's rights, 19th century (engraving)

JLJ4568521: Feminism: 'Speech for Women's Empowerment in the United States' A young woman standing on a barrel claim women's rights, 19th century (engraving), Anonymous / Bridgeman Images

ID: JLJ4568521

Feminism: 'Speech for Women's Empowerment in the United States' A young woman standing on a barrel claim women's rights, 19th century (engraving)

Anonymous

Open cluster NGC 6939 and galaxy NGC 6946 - Spiral galaxy NGC 6946 and open cluster NGC 6939 - The spiral galaxy NGC 6946 is located about 10 million years ago - light in Cephee. Many star formations are observed here. The cluster of stars NGC 6939, on the right, belongs to our galaxy. Spiral Galaxy NGC 6946 and Open Cluster NGC 6939 are located about 2 degrees southwest of Eta Cepheus. 6946 is a 9.7 magnitude spiral galaxy that was discovered by William Herschel on September 9, 1798 and is about 10 arc minutes in diameter. It is a relatively close galaxy at a distance of about 10 million light years, and was once suspected by Edwin Hubble of being a member of the Local Group of galaxies that includes the Milky Way, but today it is not believed to be a member. Because we are looking at it through the plane of our own galaxy, it is highly obscured by dust. NGC 6946 is sometimes called the Fireworks galaxy because of the number of supernovae that have been discovered there and the galaxy's prodigious rate of star formation. By contrast, open cluster NGC 6939, seen about 40 arc minutes northwest of NGC 6946, is located inside of our own galaxy at a distance of approximately 36 light years. It is just by coincidence that these two objects lie close to each other in the same line of sight
Open cluster NGC 6939 and galaxy NGC 6946 - Spiral galaxy NGC 6946 and open cluster NGC 6939 - The spiral galaxy NGC 6946 is located about 10 million years ago - light in Cephee. Many star formations are observed here. The cluster of stars NGC 6939, on the right, belongs to our galaxy. Spiral Galaxy NGC 6946 and Open Cluster NGC 6939 are located about 2 degrees southwest of Eta Cepheus. 6946 is a 9.7 magnitude spiral galaxy that was discovered by William Herschel on September 9, 1798 and is about 10 arc minutes in diameter. It is a relatively close galaxy at a distance of about 10 million light years, and was once suspected by Edwin Hubble of being a member of the Local Group of galaxies that includes the Milky Way, but today it is not believed to be a member. Because we are looking at it through the plane of our own galaxy, it is highly obscured by dust. NGC 6946 is sometimes called the Fireworks galaxy because of the number of supernovae that have been discovered there and the galaxy's prodigious rate of star formation. By contrast, open cluster NGC 6939, seen about 40 arc minutes northwest of NGC 6946, is located inside of our own galaxy at a distance of approximately 36 light years. It is just by coincidence that these two objects lie close to each other in the same line of sight

PIX4568549: Open cluster NGC 6939 and galaxy NGC 6946 - Spiral galaxy NGC 6946 and open cluster NGC 6939 - The spiral galaxy NGC 6946 is located about 10 million years ago - light in Cephee. Many star formations are observed here. The cluster of stars NGC 6939, on the right, belongs to our galaxy. Spiral Galaxy NGC 6946 and Open Cluster NGC 6939 are located about 2 degrees southwest of Eta Cepheus. 6946 is a 9.7 magnitude spiral galaxy that was discovered by William Herschel on September 9, 1798 and is about 10 arc minutes in diameter. It is a relatively close galaxy at a distance of about 10 million light years, and was once suspected by Edwin Hubble of being a member of the Local Group of galaxies that includes the Milky Way, but today it is not believed to be a member. Because we are looking at it through the plane of our own galaxy, it is highly obscured by dust. NGC 6946 is sometimes called the Fireworks galaxy because of the number of supernovae that have been discovered there and the galaxy's prodigious rate of star formation. By contrast, open cluster NGC 6939, seen about 40 arc minutes northwest of NGC 6946, is located inside of our own galaxy at a distance of approximately 36 light years. It is just by coincidence that these two objects lie close to each other in the same line of sight / Bridgeman Images

ID: PIX4568549

Open cluster NGC 6939 and galaxy NGC 6946 - Spiral galaxy NGC 6946 and open cluster NGC 6939 - The spiral galaxy NGC 6946 is located about 10 million years ago - light in Cephee. Many star formations are observed here. The cluster of stars NGC 6939, on the right, belongs to our galaxy. Spiral Galaxy NGC 6946 and Open Cluster NGC 6939 are located about 2 degrees southwest of Eta Cepheus. 6946 is a 9.7 magnitude spiral galaxy that was discovered by William Herschel on September 9, 1798 and is about 10 arc minutes in diameter. It is a relatively close galaxy at a distance of about 10 million light years, and was once suspected by Edwin Hubble of being a member of the Local Group of galaxies that includes the Milky Way, but today it is not believed to be a member. Because we are looking at it through the plane of our own galaxy, it is highly obscured by dust. NGC 6946 is sometimes called the Fireworks galaxy because of the number of supernovae that have been discovered there and the galaxy

Sheet music of Suite for piano (Opus 90) by Camille Saint-Saens (print)
Sheet music of Suite for piano (Opus 90) by Camille Saint-Saens (print)

LRI4568361: Sheet music of Suite for piano (Opus 90) by Camille Saint-Saens (print), Anonymous / Bridgeman Images

ID: LRI4568361

Sheet music of Suite for piano (Opus 90) by Camille Saint-Saens (print)

Anonymous

Open cluster M26 in the ECU of Sobieski - Open cluster M26 in Scutum - M26 (NGC 6694) is located about 5000 years - light from Earth and is about 90 million years old. M26 is an open cluster in the constellation Scutum. A fairly tight cluster, in this deep image it has to compete with a very populous background of Milky Way stars. It is about 5000 light - years away and around 90 million years old
Open cluster M26 in the ECU of Sobieski - Open cluster M26 in Scutum - M26 (NGC 6694) is located about 5000 years - light from Earth and is about 90 million years old. M26 is an open cluster in the constellation Scutum. A fairly tight cluster, in this deep image it has to compete with a very populous background of Milky Way stars. It is about 5000 light - years away and around 90 million years old

PIX4568402: Open cluster M26 in the ECU of Sobieski - Open cluster M26 in Scutum - M26 (NGC 6694) is located about 5000 years - light from Earth and is about 90 million years old. M26 is an open cluster in the constellation Scutum. A fairly tight cluster, in this deep image it has to compete with a very populous background of Milky Way stars. It is about 5000 light - years away and around 90 million years old / Bridgeman Images

ID: PIX4568402

Open cluster M26 in the ECU of Sobieski - Open cluster M26 in Scutum - M26 (NGC 6694) is located about 5000 years - light from Earth and is about 90 million years old. M26 is an open cluster in the constellation Scutum. A fairly tight cluster, in this deep image it has to compete with a very populous background of Milky Way stars. It is about 5000 light - years away and around 90 million years old

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.
The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

TEC4568449: The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine. / Bridgeman Images

ID: TEC4568449

The port of Rotterdam, Netherlands (Netherlands) is the first European port and is located at the mouth of the Meuse and the Rhine.

Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, with an overall brightness of magnitude 5.8, contains as many as 500 stars ranging from 8th magnitude down to 14th magnitude
Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, with an overall brightness of magnitude 5.8, contains as many as 500 stars ranging from 8th magnitude down to 14th magnitude

PIX4568454: Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, with an overall brightness of magnitude 5.8, contains as many as 500 stars ranging from 8th magnitude down to 14th magnitude / Bridgeman Images

ID: PIX4568454

Open cluster M11 in the ECU of Sobieski - M11 open cluster in Scutum - M11 (NGC 6705) is a cluster of about 3000 stars. Image obtained by Siding Spring Clusters of bright blue stars like M11 are found scattered among the spiral arms of the Milky Way and other galaxies like it. They are a clear sign that star formation is active, because such clusters are usually very young and short lived. The stars in M11 all formed from the same material and at about the same time, a few million years ago. In 100 million years or so, all the brightest stars in the group will have evolved into cool supergiants and exploded as supernovae, leaving behind large numbers of low mass, relatively faint stars whose lives will be much longer and whose end will be much less dramatic. Located in the constellation of Scutum, it is sometimes mistaken for a loose globular cluster. M11 is also called the “” Wild Duck Cluster”” because of it's resemblance to a flight of wild ducks when viewed in a telescope. M11, wit

The Erasmus bridge in Rotterdam (Netherlands). Construction 1990-1996, Arcchitecte Van Berkel and Bos Architecten.
The Erasmus bridge in Rotterdam (Netherlands). Construction 1990-1996, Arcchitecte Van Berkel and Bos Architecten.

TEC4568481: The Erasmus bridge in Rotterdam (Netherlands). Construction 1990-1996, Arcchitecte Van Berkel and Bos Architecten. / Bridgeman Images

ID: TEC4568481

The Erasmus bridge in Rotterdam (Netherlands). Construction 1990-1996, Arcchitecte Van Berkel and Bos Architecten.

The house of the bridge guard in Wilhemminakade, Rotterdam (Netherlands). Construction 1994-1996, architect Bolles Wilson.
The house of the bridge guard in Wilhemminakade, Rotterdam (Netherlands). Construction 1994-1996, architect Bolles Wilson.

MDA4568503: The house of the bridge guard in Wilhemminakade, Rotterdam (Netherlands). Construction 1994-1996, architect Bolles Wilson., Bolles+Wilson / Bridgeman Images

ID: MDA4568503

The house of the bridge guard in Wilhemminakade, Rotterdam (Netherlands). Construction 1994-1996, architect Bolles Wilson.

Bolles+Wilson

Frontispiece of I due Figaro, opera by Alessandro Speranza
Frontispiece of I due Figaro, opera by Alessandro Speranza

LRI4568538: Frontispiece of I due Figaro, opera by Alessandro Speranza, Anonymous / Bridgeman Images

ID: LRI4568538

Frontispiece of I due Figaro, opera by Alessandro Speranza

Anonymous

Vegetalised roof in Geneva (Switzerland).
Vegetalised roof in Geneva (Switzerland).

RCT4568588: Vegetalised roof in Geneva (Switzerland)., Castan, Remy / Bridgeman Images

ID: RCT4568588

Vegetalised roof in Geneva (Switzerland).

Castan, Remy

Confluence of the Arve and the Rhones. General view, Geneva (Switzerland).
Confluence of the Arve and the Rhones. General view, Geneva (Switzerland).

RCT4568607: Confluence of the Arve and the Rhones. General view, Geneva (Switzerland)., Castan, Remy / Bridgeman Images

ID: RCT4568607

Confluence of the Arve and the Rhones. General view, Geneva (Switzerland).

Castan, Remy

First page of musical score of Symphony in F major by Johann Franz Sterkel
First page of musical score of Symphony in F major by Johann Franz Sterkel

LRI4568641: First page of musical score of Symphony in F major by Johann Franz Sterkel, Sterkel, Johann Franz (1750-1817) / Bridgeman Images

ID: LRI4568641

First page of musical score of Symphony in F major by Johann Franz Sterkel

Sterkel, Johann Franz (1750-1817)

Portrait of Nicolas Boileau, 18th century (oil on canvas)
Portrait of Nicolas Boileau, 18th century (oil on canvas)

JLJ4567464: Portrait of Nicolas Boileau, 18th century (oil on canvas), Gresly, Gabriel (1712-56) / Bridgeman Images

ID: JLJ4567464

Portrait of Nicolas Boileau, 18th century (oil on canvas)

Gresly, Gabriel (1712-56)

The Winter Canal separating the Old Hermitage from the Theatre from the Hermitage in St. Petersburg (Russia).
The Winter Canal separating the Old Hermitage from the Theatre from the Hermitage in St. Petersburg (Russia).

TEC4567593: The Winter Canal separating the Old Hermitage from the Theatre from the Hermitage in St. Petersburg (Russia). / Bridgeman Images

ID: TEC4567593

The Winter Canal separating the Old Hermitage from the Theatre from the Hermitage in St. Petersburg (Russia).

The Bank Bridge with the Cathedral of the Resurrection of Christ behind, Griboiedov Canal, St. Petersburg (Russia).
The Bank Bridge with the Cathedral of the Resurrection of Christ behind, Griboiedov Canal, St. Petersburg (Russia).

TEC4567612: The Bank Bridge with the Cathedral of the Resurrection of Christ behind, Griboiedov Canal, St. Petersburg (Russia). / Bridgeman Images

ID: TEC4567612

The Bank Bridge with the Cathedral of the Resurrection of Christ behind, Griboiedov Canal, St. Petersburg (Russia).

Poster for painting 'Valentine' showing the silhouette of a man with a brush, 1929 (oil on canvas)
Poster for painting 'Valentine' showing the silhouette of a man with a brush, 1929 (oil on canvas)

JLJ4567646: Poster for painting 'Valentine' showing the silhouette of a man with a brush, 1929 (oil on canvas), Loupot, Charles (1892-1962) / Bridgeman Images

ID: JLJ4567646

Poster for painting 'Valentine' showing the silhouette of a man with a brush, 1929 (oil on canvas)

Loupot, Charles (1892-1962)

The Cathedral of Our Lady of Kazan in St. Petersburg (Russia). Construction 1801-1811, architect Andrei Voronikhine (1759-1814).
The Cathedral of Our Lady of Kazan in St. Petersburg (Russia). Construction 1801-1811, architect Andrei Voronikhine (1759-1814).

TEC4567697: The Cathedral of Our Lady of Kazan in St. Petersburg (Russia). Construction 1801-1811, architect Andrei Voronikhine (1759-1814). / Bridgeman Images

ID: TEC4567697

The Cathedral of Our Lady of Kazan in St. Petersburg (Russia). Construction 1801-1811, architect Andrei Voronikhine (1759-1814).

French Revolution: poster on law no. 407 on the marriage of canonesses of 19/01/1791 (print)
French Revolution: poster on law no. 407 on the marriage of canonesses of 19/01/1791 (print)

JLJ4567734: French Revolution: poster on law no. 407 on the marriage of canonesses of 19/01/1791 (print), French School, (18th century) / Bridgeman Images

ID: JLJ4567734

French Revolution: poster on law no. 407 on the marriage of canonesses of 19/01/1791 (print)

French School, (18th century)

First page of musical score of Symphony in c major by Johann Franz Sterkel
First page of musical score of Symphony in c major by Johann Franz Sterkel

LRI4568653: First page of musical score of Symphony in c major by Johann Franz Sterkel, Sterkel, Johann Franz (1750-1817) / Bridgeman Images

ID: LRI4568653

First page of musical score of Symphony in c major by Johann Franz Sterkel

Sterkel, Johann Franz (1750-1817)

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus.Seven of the brightest stars are quite easy to see with the unaided eye.The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space
Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus.Seven of the brightest stars are quite easy to see with the unaided eye.The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

PIX4568736: Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus.Seven of the brightest stars are quite easy to see with the unaided eye.The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space / Bridgeman Images

ID: PIX4568736

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. The Pleiades are a reflection nebula associated with a cluster of young stars. The cluster itself is a group of many hundreds of stars about 400 light years from Earth in the northern constellation of Taurus.Seven of the brightest stars are quite easy to see with the unaided eye.The nebulosity seen here is light reflected from the particles in a cloud of cold gas and dust into which the cluster has drifted. It appears blue because these tiny interstellar particles scatter blue light more efficiently than the longer wavelengths of red light and it is streaky because of the distribution of dust particles in space

The Assumption of the Virgin Altarpiece, 1300-25 (painting)
The Assumption of the Virgin Altarpiece, 1300-25 (painting)

JLJ4568780: The Assumption of the Virgin Altarpiece, 1300-25 (painting), Vanni, Turino (1348-1438) / Bridgeman Images

ID: JLJ4568780

The Assumption of the Virgin Altarpiece, 1300-25 (painting)

Vanni, Turino (1348-1438)

The Los Angeles periphery with Mount Cahuenga in the background above Hollywood (California, USA). In the background, the Hollywood sign was a historic monument. Visible has miles from many points of Los Angeles, it is not accessible to the general public. Built in 1923, the letters are 23 metres high and at that time advertised a real estate program.
The Los Angeles periphery with Mount Cahuenga in the background above Hollywood (California, USA). In the background, the Hollywood sign was a historic monument. Visible has miles from many points of Los Angeles, it is not accessible to the general public. Built in 1923, the letters are 23 metres high and at that time advertised a real estate program.

TEC4568793: The Los Angeles periphery with Mount Cahuenga in the background above Hollywood (California, USA). In the background, the Hollywood sign was a historic monument. Visible has miles from many points of Los Angeles, it is not accessible to the general public. Built in 1923, the letters are 23 metres high and at that time advertised a real estate program. / Bridgeman Images

ID: TEC4568793

The Los Angeles periphery with Mount Cahuenga in the background above Hollywood (California, USA). In the background, the Hollywood sign was a historic monument. Visible has miles from many points of Los Angeles, it is not accessible to the general public. Built in 1923, the letters are 23 metres high and at that time advertised a real estate program.

Hyad cluster - Mel 25 - The Hyades cluster in Taurus - Mel 25, the Hyades, is an open cluster visible to the naked eye in the constellation Taurus. The red giant star Aldebaran is the brightest star in the image. On the left, the small open cluster NGC 1647. The Hyades is a beautiful open cluster in Taurus that is easily visible to the unaided - eye. Brilliant Aldeberan, a 0.9 magnitude red giant star, dominates the cluster which is located about 153 light years away. Smaller open cluster NGC 1647 is on the left in the image, some 45 acr minutes in diameter at magnitude 6.4
Hyad cluster - Mel 25 - The Hyades cluster in Taurus - Mel 25, the Hyades, is an open cluster visible to the naked eye in the constellation Taurus. The red giant star Aldebaran is the brightest star in the image. On the left, the small open cluster NGC 1647. The Hyades is a beautiful open cluster in Taurus that is easily visible to the unaided - eye. Brilliant Aldeberan, a 0.9 magnitude red giant star, dominates the cluster which is located about 153 light years away. Smaller open cluster NGC 1647 is on the left in the image, some 45 acr minutes in diameter at magnitude 6.4

PIX4568904: Hyad cluster - Mel 25 - The Hyades cluster in Taurus - Mel 25, the Hyades, is an open cluster visible to the naked eye in the constellation Taurus. The red giant star Aldebaran is the brightest star in the image. On the left, the small open cluster NGC 1647. The Hyades is a beautiful open cluster in Taurus that is easily visible to the unaided - eye. Brilliant Aldeberan, a 0.9 magnitude red giant star, dominates the cluster which is located about 153 light years away. Smaller open cluster NGC 1647 is on the left in the image, some 45 acr minutes in diameter at magnitude 6.4 / Bridgeman Images

ID: PIX4568904

Hyad cluster - Mel 25 - The Hyades cluster in Taurus - Mel 25, the Hyades, is an open cluster visible to the naked eye in the constellation Taurus. The red giant star Aldebaran is the brightest star in the image. On the left, the small open cluster NGC 1647. The Hyades is a beautiful open cluster in Taurus that is easily visible to the unaided - eye. Brilliant Aldeberan, a 0.9 magnitude red giant star, dominates the cluster which is located about 153 light years away. Smaller open cluster NGC 1647 is on the left in the image, some 45 acr minutes in diameter at magnitude 6.4


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