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Indian pink, Spigelia marilandica. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.
Indian pink, Spigelia marilandica. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.

FLO4607285: Indian pink, Spigelia marilandica. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s. / Bridgeman Images

ID: FLO4607285

Indian pink, Spigelia marilandica. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.

Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away
Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away

PIX4607290: Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away / Bridgeman Images

ID: PIX4607290

Artist's view of the New Horizons probe near Pluto - The New Horizons spacecraft near Pluto - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Artist's concept of the New Horizons spacecraft as it approaches Pluto and its largest moon, Charon, in July 2015. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global geology and geomorphology of Pluto and Charon, map their surface compositions and temperatures, and examine Pluto's atmosphere in detail. The spacecraft's most prominent design feature is a nearly 7 - foot (2.1 - meter) dish antenna, through which it will communicate with Earth from as far as 4.7 billion miles (7.5 billion kilometers) away

The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in November 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, workers begin installing the radioisotope thermoelectric generator (RTG) onto the New Horizons spacecraft for a fit check. The RTG is the baseline power supply for New Horizons, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. It is expected to reach Pluto in July 2015
The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in November 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, workers begin installing the radioisotope thermoelectric generator (RTG) onto the New Horizons spacecraft for a fit check. The RTG is the baseline power supply for New Horizons, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. It is expected to reach Pluto in July 2015

PIX4607332: The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in November 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, workers begin installing the radioisotope thermoelectric generator (RTG) onto the New Horizons spacecraft for a fit check. The RTG is the baseline power supply for New Horizons, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. It is expected to reach Pluto in July 2015 / Bridgeman Images

ID: PIX4607332

The New Horizons probe - The New Horizons spacecraft - The New Horizons probe at Nasa's Kennedy Space Center in November 2005. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it reached in 2015 and Kuiper's objects in 2020. In NASA Kennedy Space Center's Payload Hazardous Servicing Facility, workers begin installing the radioisotope thermoelectric generator (RTG) onto the New Horizons spacecraft for a fit check. The RTG is the baseline power supply for New Horizons, scheduled to launch in January 2006 on a journey to Pluto and its moon, Charon. It is expected to reach Pluto in July 2015

Poor man's orchid, Schizanthus porrigens. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.
Poor man's orchid, Schizanthus porrigens. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.

FLO4607342: Poor man's orchid, Schizanthus porrigens. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s. / Bridgeman Images

ID: FLO4607342

Poor man's orchid, Schizanthus porrigens. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.

The Ulysses probe - View of the Ulysses probe in preparation before launching by the shuttle Discovery. The Ulysses probe was launched on 6 October 1990 to study the Sun
The Ulysses probe - View of the Ulysses probe in preparation before launching by the shuttle Discovery. The Ulysses probe was launched on 6 October 1990 to study the Sun

PIX4607363: The Ulysses probe - View of the Ulysses probe in preparation before launching by the shuttle Discovery. The Ulysses probe was launched on 6 October 1990 to study the Sun / Bridgeman Images

ID: PIX4607363

The Ulysses probe - View of the Ulysses probe in preparation before launching by the shuttle Discovery. The Ulysses probe was launched on 6 October 1990 to study the Sun

New Horizons near Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft flies by dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 11,000 miles from Pluto (lower left), 23,000 miles from its largest moon Charon (upper right) and 2.97 billion miles from the Earth. While little is known about Pluto's appearance, here this Kuiper belt dwarf planet is realized as a frozen world covered with various ices, hosting a thin atmosphere of nitrogen, methane and other hydrocarbons too possibly, with a significantly weathered surface as Pluto's 248 - year orbit alternately brings it closer then further from the warmth of the sun
New Horizons near Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft flies by dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 11,000 miles from Pluto (lower left), 23,000 miles from its largest moon Charon (upper right) and 2.97 billion miles from the Earth. While little is known about Pluto's appearance, here this Kuiper belt dwarf planet is realized as a frozen world covered with various ices, hosting a thin atmosphere of nitrogen, methane and other hydrocarbons too possibly, with a significantly weathered surface as Pluto's 248 - year orbit alternately brings it closer then further from the warmth of the sun

PIX4607366: New Horizons near Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft flies by dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 11,000 miles from Pluto (lower left), 23,000 miles from its largest moon Charon (upper right) and 2.97 billion miles from the Earth. While little is known about Pluto's appearance, here this Kuiper belt dwarf planet is realized as a frozen world covered with various ices, hosting a thin atmosphere of nitrogen, methane and other hydrocarbons too possibly, with a significantly weathered surface as Pluto's 248 - year orbit alternately brings it closer then further from the warmth of the sun / Bridgeman Images

ID: PIX4607366

New Horizons near Pluto and Charon - Artist's view of the New Horizons probe near Pluto and its largest satellite Charon. The New Horizons probe was launched on 19 January 2006 to Jupiter, then Pluto and Charon, which it will reach in 2015 and Kuiper's objects in 2020. Nasa's New Horizons unmanned spacecraft flies by dwarf planet Pluto and its moon Charon. New Horizons has been en route to Pluto since its launch from Earth in 2006 and is scheduled to make its closest approach on 14 July 2015. New Horizons is about the size and shape of a grand piano and weighed 1,054 pounds at launch. The high - gain dish antenna is about 7 feet in diameter and is employed for communication with the Earth. In this image the New Horizons spacecraft is about 11,000 miles from Pluto (lower left), 23,000 miles from its largest moon Charon (upper right) and 2.97 billion miles from the Earth. While little is known about Pluto's appearance, here this Kuiper belt dwarf planet is realized as a frozen world cove

The Ulysses probe observes the Sun - The Ulysses probe observes the Sun - Artist's view
The Ulysses probe observes the Sun - The Ulysses probe observes the Sun - Artist's view

PIX4607369: The Ulysses probe observes the Sun - The Ulysses probe observes the Sun - Artist's view / Bridgeman Images

ID: PIX4607369

The Ulysses probe observes the Sun - The Ulysses probe observes the Sun - Artist's view

Plains coreopsis or calliopsis, Coreopsis tinctoria. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.
Plains coreopsis or calliopsis, Coreopsis tinctoria. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.

FLO4607385: Plains coreopsis or calliopsis, Coreopsis tinctoria. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s. / Bridgeman Images

ID: FLO4607385

Plains coreopsis or calliopsis, Coreopsis tinctoria. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.

Willow gentian, Gentiana asclepiadea. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.
Willow gentian, Gentiana asclepiadea. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.

FLO4607393: Willow gentian, Gentiana asclepiadea. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s. / Bridgeman Images

ID: FLO4607393

Willow gentian, Gentiana asclepiadea. Handcoloured botanical illustration drawn and engraved by William Clark from Richard Morris's “Flora Conspicua” London, Longman, Rees, 1826. William Clark was former draughtsman to the London Horticultural Society and illustrated many botanical books in the 1820s and 1830s.

Phoenix Probe - Artist's View - The American Phoenix Probe will be launched in August 2007. After a 10-month trip, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras
Phoenix Probe - Artist's View - The American Phoenix Probe will be launched in August 2007. After a 10-month trip, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras

PIX4606713: Phoenix Probe - Artist's View - The American Phoenix Probe will be launched in August 2007. After a 10-month trip, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras / Bridgeman Images

ID: PIX4606713

Phoenix Probe - Artist's View - The American Phoenix Probe will be launched in August 2007. After a 10-month trip, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras

Phoenix Probe - Artist's View - The American Phoenix Probe will be launched in August 2007. After a 10-month trip, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras
Phoenix Probe - Artist's View - The American Phoenix Probe will be launched in August 2007. After a 10-month trip, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras

PIX4606724: Phoenix Probe - Artist's View - The American Phoenix Probe will be launched in August 2007. After a 10-month trip, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras / Bridgeman Images

ID: PIX4606724

Phoenix Probe - Artist's View - The American Phoenix Probe will be launched in August 2007. After a 10-month trip, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras

Miss Anne Demerson as Liselle in Le Mari et l'Amant by Jean-Claude Vial, Theatre Francais, 1821. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Miss Anne Demerson as Liselle in Le Mari et l'Amant by Jean-Claude Vial, Theatre Francais, 1821. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4606745: Miss Anne Demerson as Liselle in Le Mari et l'Amant by Jean-Claude Vial, Theatre Francais, 1821. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825., Colin, Alexandre Marie (1798-1875) / Bridgeman Images

ID: FLO4606745

Miss Anne Demerson as Liselle in Le Mari et l'Amant by Jean-Claude Vial, Theatre Francais, 1821. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Colin, Alexandre Marie (1798-1875)

Phoenix probe - View of American Phoenix probe installed in the cap of a Delta II rocket at Kennedy space center in Florida. Launch on 4 August 2007, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras
Phoenix probe - View of American Phoenix probe installed in the cap of a Delta II rocket at Kennedy space center in Florida. Launch on 4 August 2007, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras

PIX4606754: Phoenix probe - View of American Phoenix probe installed in the cap of a Delta II rocket at Kennedy space center in Florida. Launch on 4 August 2007, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras / Bridgeman Images

ID: PIX4606754

Phoenix probe - View of American Phoenix probe installed in the cap of a Delta II rocket at Kennedy space center in Florida. Launch on 4 August 2007, it should land in May 2008 near the northern polar cap of Mars. She will perform analyses of Martian soil by digging at about 50 cm deep. Phoenix will also be equipped with cameras

Model of the Rover MSL - Model Rover MSL - Test at CNES of the model of the Rover MSL in July 2009. This model at scale 1 was made by students of BTS section. Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. Test at CNES (Toulouse) in july 2009 of the animated replica of NASA's martian Rover MSL built by english industrial BTS students. Mars Science Laboratory (MSL) is a rover that will study Mars' habitability. Launch is scheduled in the fall of 2011
Model of the Rover MSL - Model Rover MSL - Test at CNES of the model of the Rover MSL in July 2009. This model at scale 1 was made by students of BTS section. Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. Test at CNES (Toulouse) in july 2009 of the animated replica of NASA's martian Rover MSL built by english industrial BTS students. Mars Science Laboratory (MSL) is a rover that will study Mars' habitability. Launch is scheduled in the fall of 2011

PIX4606828: Model of the Rover MSL - Model Rover MSL - Test at CNES of the model of the Rover MSL in July 2009. This model at scale 1 was made by students of BTS section. Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. Test at CNES (Toulouse) in july 2009 of the animated replica of NASA's martian Rover MSL built by english industrial BTS students. Mars Science Laboratory (MSL) is a rover that will study Mars' habitability. Launch is scheduled in the fall of 2011 / Bridgeman Images

ID: PIX4606828

Model of the Rover MSL - Model Rover MSL - Test at CNES of the model of the Rover MSL in July 2009. This model at scale 1 was made by students of BTS section. Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. Test at CNES (Toulouse) in july 2009 of the animated replica of NASA's martian Rover MSL built by english industrial BTS students. Mars Science Laboratory (MSL) is a rover that will study Mars' habitability. Launch is scheduled in the fall of 2011

Model of the Rover MSL - Model Rover MSL - Test at CNES of the model of the Rover MSL in July 2009. This model at scale 1 was made by students of BTS section. Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. Test at CNES (Toulouse) in july 2009 of the animated replica of NASA's martian Rover MSL built by english industrial BTS students. Mars Science Laboratory (MSL) is a rover that will study Mars' habitability. Launch is scheduled in the fall of 2011
Model of the Rover MSL - Model Rover MSL - Test at CNES of the model of the Rover MSL in July 2009. This model at scale 1 was made by students of BTS section. Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. Test at CNES (Toulouse) in july 2009 of the animated replica of NASA's martian Rover MSL built by english industrial BTS students. Mars Science Laboratory (MSL) is a rover that will study Mars' habitability. Launch is scheduled in the fall of 2011

PIX4606848: Model of the Rover MSL - Model Rover MSL - Test at CNES of the model of the Rover MSL in July 2009. This model at scale 1 was made by students of BTS section. Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. Test at CNES (Toulouse) in july 2009 of the animated replica of NASA's martian Rover MSL built by english industrial BTS students. Mars Science Laboratory (MSL) is a rover that will study Mars' habitability. Launch is scheduled in the fall of 2011 / Bridgeman Images

ID: PIX4606848

Model of the Rover MSL - Model Rover MSL - Test at CNES of the model of the Rover MSL in July 2009. This model at scale 1 was made by students of BTS section. Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. Test at CNES (Toulouse) in july 2009 of the animated replica of NASA's martian Rover MSL built by english industrial BTS students. Mars Science Laboratory (MSL) is a rover that will study Mars' habitability. Launch is scheduled in the fall of 2011

Miss Rose Dupuis as Madame Dorval in La Mere Rivale by Casimir Bonjour, Theatre Français. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Miss Rose Dupuis as Madame Dorval in La Mere Rivale by Casimir Bonjour, Theatre Français. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4606892: Miss Rose Dupuis as Madame Dorval in La Mere Rivale by Casimir Bonjour, Theatre Français. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4606892

Miss Rose Dupuis as Madame Dorval in La Mere Rivale by Casimir Bonjour, Theatre Français. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Joseph David as Idamore in Le Paria by Casimir Delavigne, Theatre Royal de l'Odeon, 1821. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Joseph David as Idamore in Le Paria by Casimir Delavigne, Theatre Royal de l'Odeon, 1821. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4606898: Joseph David as Idamore in Le Paria by Casimir Delavigne, Theatre Royal de l'Odeon, 1821. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4606898

Joseph David as Idamore in Le Paria by Casimir Delavigne, Theatre Royal de l'Odeon, 1821. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Miss Anais or Anais-Pauline-Nathalie Aubert as Misael in Les Macchabees by Alexandre Guiraud, Theatre Royal de l'Odeon, 1822. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Miss Anais or Anais-Pauline-Nathalie Aubert as Misael in Les Macchabees by Alexandre Guiraud, Theatre Royal de l'Odeon, 1822. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4606918: Miss Anais or Anais-Pauline-Nathalie Aubert as Misael in Les Macchabees by Alexandre Guiraud, Theatre Royal de l'Odeon, 1822. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4606918

Miss Anais or Anais-Pauline-Nathalie Aubert as Misael in Les Macchabees by Alexandre Guiraud, Theatre Royal de l'Odeon, 1822. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Mission ExoMars - Rover Pasteur - Artist view - Artist view of the Rover Pasteur on Martian soil. European ExoMars Mission
Mission ExoMars - Rover Pasteur - Artist view - Artist view of the Rover Pasteur on Martian soil. European ExoMars Mission

PIX4606925: Mission ExoMars - Rover Pasteur - Artist view - Artist view of the Rover Pasteur on Martian soil. European ExoMars Mission / Bridgeman Images

ID: PIX4606925

Mission ExoMars - Rover Pasteur - Artist view - Artist view of the Rover Pasteur on Martian soil. European ExoMars Mission

Soprano opera singer Miss Grassari as Amazili in Fernand Cortez by Gaspare Spontini, Royal Academy of Music. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Soprano opera singer Miss Grassari as Amazili in Fernand Cortez by Gaspare Spontini, Royal Academy of Music. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4606934: Soprano opera singer Miss Grassari as Amazili in Fernand Cortez by Gaspare Spontini, Royal Academy of Music. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4606934

Soprano opera singer Miss Grassari as Amazili in Fernand Cortez by Gaspare Spontini, Royal Academy of Music. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

English soprano opera singer Caroline Branchu as Dido, Queen of Carthage, in Didon by Nicolo Piccinni, Royal Academy of Music, 1824. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
English soprano opera singer Caroline Branchu as Dido, Queen of Carthage, in Didon by Nicolo Piccinni, Royal Academy of Music, 1824. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4606955: English soprano opera singer Caroline Branchu as Dido, Queen of Carthage, in Didon by Nicolo Piccinni, Royal Academy of Music, 1824. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4606955

English soprano opera singer Caroline Branchu as Dido, Queen of Carthage, in Didon by Nicolo Piccinni, Royal Academy of Music, 1824. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Contralto singer Madame Montano as Rosine in the opera Le Barbier de Seville by Gioachino Rossini, Theatre Royal de l'Odeon, 1823. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Contralto singer Madame Montano as Rosine in the opera Le Barbier de Seville by Gioachino Rossini, Theatre Royal de l'Odeon, 1823. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4606959: Contralto singer Madame Montano as Rosine in the opera Le Barbier de Seville by Gioachino Rossini, Theatre Royal de l'Odeon, 1823. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4606959

Contralto singer Madame Montano as Rosine in the opera Le Barbier de Seville by Gioachino Rossini, Theatre Royal de l'Odeon, 1823. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Soprano singer Madame Valere as Anna in the Romantic opera Robin des Bois by Carl Maria von Weber, Theatre Royal de l'Odeon, 1824. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Soprano singer Madame Valere as Anna in the Romantic opera Robin des Bois by Carl Maria von Weber, Theatre Royal de l'Odeon, 1824. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4606977: Soprano singer Madame Valere as Anna in the Romantic opera Robin des Bois by Carl Maria von Weber, Theatre Royal de l'Odeon, 1824. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4606977

Soprano singer Madame Valere as Anna in the Romantic opera Robin des Bois by Carl Maria von Weber, Theatre Royal de l'Odeon, 1824. Handcoloured lithograph by F. Noel after an illustration by Lavigne Marin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Giotto probe meets Halley's comet - Giotto probe meets Halley's comet - Artist's view
Giotto probe meets Halley's comet - Giotto probe meets Halley's comet - Artist's view

PIX4607001: Giotto probe meets Halley's comet - Giotto probe meets Halley's comet - Artist's view, Dixon, Don (b.1951) / Bridgeman Images

ID: PIX4607001

Giotto probe meets Halley's comet - Giotto probe meets Halley's comet - Artist's view

Dixon, Don (b.1951)

The solar panels of the Rosetta probe being tested. - View of the Rosetta probe in preparation at ESTEC. The Rosetta probe was launched on 2 March 2004 to study the comet Churyumov - Gerasimenko, which it is expected to meet around May 2014. It will put a landing on its surface.
The solar panels of the Rosetta probe being tested. - View of the Rosetta probe in preparation at ESTEC. The Rosetta probe was launched on 2 March 2004 to study the comet Churyumov - Gerasimenko, which it is expected to meet around May 2014. It will put a landing on its surface.

PIX4607013: The solar panels of the Rosetta probe being tested. - View of the Rosetta probe in preparation at ESTEC. The Rosetta probe was launched on 2 March 2004 to study the comet Churyumov - Gerasimenko, which it is expected to meet around May 2014. It will put a landing on its surface. / Bridgeman Images

ID: PIX4607013

The solar panels of the Rosetta probe being tested. - View of the Rosetta probe in preparation at ESTEC. The Rosetta probe was launched on 2 March 2004 to study the comet Churyumov - Gerasimenko, which it is expected to meet around May 2014. It will put a landing on its surface.

Charles-Edme Vernet and Dominique in La Famille du Porter d'Eau by Allarde, Gabriel de Lurieu, Theatre des Varietes, 1824. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Charles-Edme Vernet and Dominique in La Famille du Porter d'Eau by Allarde, Gabriel de Lurieu, Theatre des Varietes, 1824. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4607025: Charles-Edme Vernet and Dominique in La Famille du Porter d'Eau by Allarde, Gabriel de Lurieu, Theatre des Varietes, 1824. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4607025

Charles-Edme Vernet and Dominique in La Famille du Porter d'Eau by Allarde, Gabriel de Lurieu, Theatre des Varietes, 1824. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Miss Pauline as Jeanny in the vaudeville piece Trilby by Theaulon, Lafontaine and Jouslin, Theatre des Varietes, 1823. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.
Miss Pauline as Jeanny in the vaudeville piece Trilby by Theaulon, Lafontaine and Jouslin, Theatre des Varietes, 1823. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

FLO4607042: Miss Pauline as Jeanny in the vaudeville piece Trilby by Theaulon, Lafontaine and Jouslin, Theatre des Varietes, 1823. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825. / Bridgeman Images

ID: FLO4607042

Miss Pauline as Jeanny in the vaudeville piece Trilby by Theaulon, Lafontaine and Jouslin, Theatre des Varietes, 1823. Handcoloured lithograph by F. Noel after an illustration by Alexandre-Marie Colin from Portraits d'Acteurs et d'Actrices dans different roles, F. Noel, Paris, 1825.

Linear acacias. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.
Linear acacias. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.

FLO4609495: Linear acacias. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England. / Bridgeman Images

ID: FLO4609495

Linear acacias. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.

Digital. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.
Digital. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.

FLO4609505: Digital. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England. / Bridgeman Images

ID: FLO4609505

Digital. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.

Psoralier stinks. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.
Psoralier stinks. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.

FLO4609516: Psoralier stinks. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England. / Bridgeman Images

ID: FLO4609516

Psoralier stinks. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.

Spiral galaxy NGC 1055 in the Whale - Spiral galaxy NGC 1055 in Cetus - NGC 1055 is about 40 million years away - light from Earth. It appears to belong to the small group of M77 galaxies in the Whale. NGC 1055 is a striking disk galaxy seen almost edge - on a distance of about 40 million light years. It seems to be a member of the small NGC 1068 (M77) group of galaxies in the southern constellation of Cetus
Spiral galaxy NGC 1055 in the Whale - Spiral galaxy NGC 1055 in Cetus - NGC 1055 is about 40 million years away - light from Earth. It appears to belong to the small group of M77 galaxies in the Whale. NGC 1055 is a striking disk galaxy seen almost edge - on a distance of about 40 million light years. It seems to be a member of the small NGC 1068 (M77) group of galaxies in the southern constellation of Cetus

PIX4609550: Spiral galaxy NGC 1055 in the Whale - Spiral galaxy NGC 1055 in Cetus - NGC 1055 is about 40 million years away - light from Earth. It appears to belong to the small group of M77 galaxies in the Whale. NGC 1055 is a striking disk galaxy seen almost edge - on a distance of about 40 million light years. It seems to be a member of the small NGC 1068 (M77) group of galaxies in the southern constellation of Cetus / Bridgeman Images

ID: PIX4609550

Spiral galaxy NGC 1055 in the Whale - Spiral galaxy NGC 1055 in Cetus - NGC 1055 is about 40 million years away - light from Earth. It appears to belong to the small group of M77 galaxies in the Whale. NGC 1055 is a striking disk galaxy seen almost edge - on a distance of about 40 million light years. It seems to be a member of the small NGC 1068 (M77) group of galaxies in the southern constellation of Cetus

Spiral galaxy M77 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - M77 (NGC 1068). This active galaxy is the typical example of a Seyfert II galaxy. It has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. Image obtained by Siding Spring's 3.9m telescope. M77 is a Seyfert galaxy, a class of galaxy named for Karl Seyfert who first identified galaxies with emission lines superimposed on the normal radiation from their nuclei in 1943. Such galaxies are a subset of an ill - defined species generally known as 'active galaxies' whose nuclei emit radio - and X - radiation as well as visible light. The least active of the active galaxies are the Seyferts, the most active are the quasars which are mostly so distant that they can only be distinguished from stars by their spectrum. <BR>The common feature of these galaxy types is a small, very bright nucleus thought to host a massive black hole. In Seyferts we see this black hole (or more likely its surrounding shroud of ultra - luminous gas) more or less pole - on. In other active galaxy types at different inclinations the spectrum of the nucleus changes as we see other manifestations of the black hole's influence on its surroundings. M77 is a member of a small group of galaxies at a distance of about 40 million light years
Spiral galaxy M77 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - M77 (NGC 1068). This active galaxy is the typical example of a Seyfert II galaxy. It has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. Image obtained by Siding Spring's 3.9m telescope. M77 is a Seyfert galaxy, a class of galaxy named for Karl Seyfert who first identified galaxies with emission lines superimposed on the normal radiation from their nuclei in 1943. Such galaxies are a subset of an ill - defined species generally known as 'active galaxies' whose nuclei emit radio - and X - radiation as well as visible light. The least active of the active galaxies are the Seyferts, the most active are the quasars which are mostly so distant that they can only be distinguished from stars by their spectrum. <BR>The common feature of these galaxy types is a small, very bright nucleus thought to host a massive black hole. In Seyferts we see this black hole (or more likely its surrounding shroud of ultra - luminous gas) more or less pole - on. In other active galaxy types at different inclinations the spectrum of the nucleus changes as we see other manifestations of the black hole's influence on its surroundings. M77 is a member of a small group of galaxies at a distance of about 40 million light years

PIX4609570: Spiral galaxy M77 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - M77 (NGC 1068). This active galaxy is the typical example of a Seyfert II galaxy. It has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. Image obtained by Siding Spring's 3.9m telescope. M77 is a Seyfert galaxy, a class of galaxy named for Karl Seyfert who first identified galaxies with emission lines superimposed on the normal radiation from their nuclei in 1943. Such galaxies are a subset of an ill - defined species generally known as 'active galaxies' whose nuclei emit radio - and X - radiation as well as visible light. The least active of the active galaxies are the Seyferts, the most active are the quasars which are mostly so distant that they can only be distinguished from stars by their spectrum.
The common feature of these galaxy types is a small, very bright nucleus thought to host a massive black hole. In Seyferts we see this black hole (or more likely its surrounding shroud of ultra - luminous gas) more or less pole - on. In other active galaxy types at different inclinations the spectrum of the nucleus changes as we see other manifestations of the black hole's influence on its surroundings. M77 is a member of a small group of galaxies at a distance of about 40 million light years / Bridgeman Images

ID: PIX4609570

Spiral galaxy M77 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - M77 (NGC 1068). This active galaxy is the typical example of a Seyfert II galaxy. It has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. Image obtained by Siding Spring's 3.9m telescope. M77 is a Seyfert galaxy, a class of galaxy named for Karl Seyfert who first identified galaxies with emission lines superimposed on the normal radiation from their nuclei in 1943. Such galaxies are a subset of an ill - defined species generally known as 'active galaxies' whose nuclei emit radio - and X - radiation as well as visible light. The least active of the active galaxies are the Seyferts, the most active are the quasars which are mostly so distant that they can only be distinguished from stars by their spectrum.
The common feature of these galaxy types is a small, very bright nucleus thought to host

Fabagelle has sessile leaves. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.
Fabagelle has sessile leaves. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.

FLO4609611: Fabagelle has sessile leaves. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England. / Bridgeman Images

ID: FLO4609611

Fabagelle has sessile leaves. Copper engraving, painted by John Curtis and grave by Weddell, published in the “Curtis Botanical Magazine”, 1820, by Samuel Curtis, London, England.

Crossandre with wavy leaves or petard flower Copper engraving, starring John Curtis and grave by Weddell, published in Samuel Curtis's “” Botanical Magazine” in 1820, London, England.
Crossandre with wavy leaves or petard flower Copper engraving, starring John Curtis and grave by Weddell, published in Samuel Curtis's “” Botanical Magazine” in 1820, London, England.

FLO4609630: Crossandre with wavy leaves or petard flower Copper engraving, starring John Curtis and grave by Weddell, published in Samuel Curtis's “” Botanical Magazine” in 1820, London, England. / Bridgeman Images

ID: FLO4609630

Crossandre with wavy leaves or petard flower Copper engraving, starring John Curtis and grave by Weddell, published in Samuel Curtis's “” Botanical Magazine” in 1820, London, England.

Gomesa orchid, Gomesa flexuosa (Oncidium flexuosus). Handcoloured copperplate engraving by Weddell after an illustration by John Curtis from Samuel Curtis' Botanical Magazine, London, 1821.
Gomesa orchid, Gomesa flexuosa (Oncidium flexuosus). Handcoloured copperplate engraving by Weddell after an illustration by John Curtis from Samuel Curtis' Botanical Magazine, London, 1821.

FLO4609697: Gomesa orchid, Gomesa flexuosa (Oncidium flexuosus). Handcoloured copperplate engraving by Weddell after an illustration by John Curtis from Samuel Curtis' Botanical Magazine, London, 1821. / Bridgeman Images

ID: FLO4609697

Gomesa orchid, Gomesa flexuosa (Oncidium flexuosus). Handcoloured copperplate engraving by Weddell after an illustration by John Curtis from Samuel Curtis' Botanical Magazine, London, 1821.

Castorbean or castor-oil-plant, Ricinus communis. Handcoloured copperplate engraving by Weddell from Samuel Curtis' Botanical Magazine, London, 1821.
Castorbean or castor-oil-plant, Ricinus communis. Handcoloured copperplate engraving by Weddell from Samuel Curtis' Botanical Magazine, London, 1821.

FLO4609701: Castorbean or castor-oil-plant, Ricinus communis. Handcoloured copperplate engraving by Weddell from Samuel Curtis' Botanical Magazine, London, 1821. / Bridgeman Images

ID: FLO4609701

Castorbean or castor-oil-plant, Ricinus communis. Handcoloured copperplate engraving by Weddell from Samuel Curtis' Botanical Magazine, London, 1821.


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