PIX4615663: March - Spirit - View from the top of Husband Hill - Panorama of 240 degres obtained by Spirit from 24 to 26 August 2005. The Rover Spirit landed on Mars in the Gusev crater area, July 4, 2004 / Bridgeman Images

FLO4615707: Madagascar giant swallowtail, Pharmacophagus antenor (Papilio antenor) 1, hairstreak butterfly, Thecla sylvanus 2,3, and white-banded babul blue, Azanus isis (Polyommatus isis) 4,5, ventral and dorsal views. Handcoloured lithograph from John O. Westwood's new edition of Dru Drury's “” Illustrations of Exotic Entomology,”” Bohn, London, 1837. / Bridgeman Images

FLO4615728: Large emerald pearl, Stemorrhages sericea (Botys Desmia? sericea) 1, ailanthus silkmoth, Samia cynthia (Saturnia cynthia) 2, Crotalaria pod borer, Argina astrea (Deiopeia astrea) 3, and Pidorus glaucopis (Callimorpha? glaucopis) 4. Handcoloured lithograph from John O. Westwood's new edition of Dru Drury's “” Illustrations of Exotic Entomology,”” Bohn, London, 1837. / Bridgeman Images

PIX4615736: March - Spirit - Panorama McMurdo - Detail - 10 - 2006 - March: McMurdo panorama - Spirit - Detail 10 - 2006 - Detail of the panorama “” Mac Murdo”” obtained by the Spirit rover from April to October 2006. Spirit stayed in the same place directing its solar panels towards the Sun to recharge its batteries. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. “McMurdo” panorama detail. From April through October 2006, Spirit has stayed on a small hill known as “Low Ridge.”” There, the rover's solar panels are tilted towards the sun to maintain enough solar power for Spirit to keep making scientific observations throughout the winter on southern Mars. This view of the surroundings from Spirit's “Winter Haven”” is presented in approximately true color / Bridgeman Images

FLO4615759: Wavy common palmfly, Elymnias hypermnestra undularis (Biblis undularis) 1,2, white admiral, Limenitis arthemis (Nymphalis Limenitis arthemis) 3,4, and common jezebel, Delias eucharis (Pieris eucharis) 5,6, ventral and dorsal. Handcoloured lithograph from John O. Westwood's new edition of Dru Drury's “” Illustrations of Exotic Entomology,”” Bohn, London, 1837. / Bridgeman Images

PIX4615764: Martian surface seen by Spirit in 2008 - Martian surface seen from the rover Spirit in 2008 - 360 degres panorama obtained by the Martian rover Spirit from February 28 to October 5, 2008. The 246 images that make up this panorama were taken from a tray called the Home Plate. The hill has the horizon on the right is Husband Hill. The hill on the left is McCool Hill. The Rover Spirit landed on Mars in the Gusev crater area on July 4, 2004. This 360 - degree panorama shows the vista from the location where Nasa's Mars Exploration Rover Spirit has spent its third Martian southern - hemisphere winter inside Mars' Gusev Crater. The rover's overwintering location is on the northern edge of a low plateau informally called “Home Plate,””” which is about 80 meters or 260 feet in diameter. This view combines 246 different exposures taken with Spirit's panoramic camera (Pancam) - - 82 pointings, with three filters at each pointing. Spirit took the first of these frames during the mission's 1,477th Martian day, or sol, (February 28, 2008) two weeks after the rover made its last move to reach the location where it would stop driving for the winter. Solar energy at Gusev Crater is so limited during the Martian winter that Spirit does not generate enough electricity to drive, nor even enough to take many images per day. The last frame for this mosaic was taken on Sol 1691 (October 5, 2008). Spirit began moving again on Sol 1709 (October 23, 2008), inching uphill to adjust the angle of its solar panels for the last portion of the winter. The hill on the horizon at far right is Husband Hill, to the north. Spirit acquired a 360 - degree panorama from the summit of Husband Hill during August 2005. The hill dominating the left portion of the image is McCool Hill. Husband and McCool hills are two of the seven principal hills in the Columbia Hills range within Gusev Crater. Home Plate is in the inner basin of the range. The northwestern edge of Home Plate is visible in th / Bridgeman Images

TEC4615786: Quai de Valmy in Paris 10th. Photography 25/08/07. / Bridgeman Images

PIX4615799: March - Opportunity - Cratere Endurance. 05/2004 - Martian crater Endurance seen by Opportunity. 05/2004 - Panorama of 360 degres obtained by Opportunity from 22 to 28 May 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows “” Endurance Crater”” and the surrounding plains of Meridiani Planum on Mars. It took seven sols to complete this panorama (sols 117 - 123), using 81 separate camera positions. The composite shown here is an approximate true - color rendering / Bridgeman Images

TEC4613812: The countryside district in Paris, 19th arrondissement. / Bridgeman Images

TEC4613816: Cinema MK2, 14 quai de la Seine Paris 19th arrondissement. / Bridgeman Images

PIX4613853: Sagittarius dwarf irregular galaxy - SagDig - Sagittarius dwarf irregular galaxy - Image of the irregular dwarf galaxy ESO 594 - 4 located 3.5 million years ago - light seen by the Hubble space telescope on August 18, 2003. The Sagittarius dwarf irregular galaxy (SagDig, ESO 594 - 4) lies some 3.5 million light - years (1.1 Megaparsecs) from us. Background galaxies (reddish/brown extended objects with spiral arms and halos) are located even further beyond SagDig at several tens of millions parsecs away. This dwarf irregular galaxy was observed by the Advanced Camera for Surveys on - board the Hubble Space Telescope on 18 August 2003. Fifty-minute exposures were taken in blue, green and red filters / Bridgeman Images

PIX4613873: Irregular dwarf galaxy I Zwicky 18 - Irregular dwarf galaxy I Zwicky 18 - The irregular dwarf galaxy I Zwicky 18 is located 59 million years - light in the Great Bear and extends over about 3000 years - light. The two bright white spots are star-forming regions. At the top left, another galaxy is visible. This galaxy could be interacting with I Zwicky 18. This image is the result of observations made by the Hubble Space Telescope in 2005 and 2006. Called I Zwicky 18, this galaxy has a youthful appearance that resembles galaxies typically found only in the early universe. Hubble has now found faint, older stars within this galaxy, suggesting that the galaxy may have formed at the same time as most other galaxies. I Zwicky 18 is classified as a dwarf irregular galaxy and is much smaller than our Milky Way Galaxy. The concentrated bluish - white knots embedded in the heart of the galaxy are two major starburst regions where stars are forming at a furious rate. The wispy blue filaments surrounding the central starburst regions are bubbles of gas that have been blown away by stellar winds and supernovae explosions from a previous generation of hot, young stars. This gas is now heated by intense ultraviolet radiation unleashed by hot, young stars. A companion galaxy lies just above and to the left of I Zwicky 18. The companion may be interacting with I Zwicky 18 by gravitationally tugging on the galaxy. The interaction may have triggered the galaxy's recent star formation that is responsible for the youthful appearance. Besides the bluish - white young stars, white - reddish stars also are visible in both I Zwicky 18 and its companion. These stars may be as old as 10 billion years. The reddish extended objects surrounding I Zwicky 18 and its companion are ancient, fully formed galaxies of different shapes that are much farther away. Hubble data also allowed astronomers for the first time to identify Cephe / Bridgeman Images

PIX4613904: The dwarf galaxy of the furnace - Fornax dwarf galaxy - The dwarf galaxy of the furnace belongs to the local group, just like our galaxy or the galaxy of Andromede. The Fornax dwarf galaxy is one of our Milky Way's neighbouring dwarf galaxies. The Milky Way is, like all large galaxies, thought to have formed from smaller galaxies in the early days of the Universe. These small galaxies should also contain many very old stars, just as the Milky Way does, and a team of astronomers has now shown that this is indeed the case. This image was composed from data from the Digitized Sky Survey 2 / Bridgeman Images

FLO4613908: Wild common carp, Cyprinus carpio. Vulnerable. Handcoloured copperplate drawn and engraved by Edward Donovan from his Natural History of British Fishes, Donovan and F.C. and J. Rivington, London, 1802-1808., Donovan, Edward (1768-1837) / Bridgeman Images

TEC4613947: Marche, Boulevard de Belleville in Paris 19th. / Bridgeman Images

PIX4614013: Classification of galaxies. The Hubble sequence - Edwin Hubble's galaxy classification - The Hubble sequence is a classification of galaxy types based on morphological criteria developed by astronomer Edwin Hubble in 1936. Artist's view. The Hubble sequence is a morphological classification scheme for galaxies created by the astronomer Edwin Hubble in 1936. Artwork / Bridgeman Images

LBY4614087: Les Entrepots les Magasins generaux, Bassin de la Vilette, Paris 19th. Photography 1989. / Bridgeman Images

FLO4614091: Stone loach, Barbatula barbatula (Bearded loche, Cobitis barbatula). Handcoloured copperplate drawn and engraved by Edward Donovan from his Natural History of British Fishes, Donovan and F.C. and J. Rivington, London, 1802-1808., Donovan, Edward (1768-1837) / Bridgeman Images

LRI4615813: Nude bent over, 20th century (drawing), Kokoschka, Oskar (1886-1980) / Bridgeman Images

LRI4615827: Sitting Woman. 20th century (Drawing), Kokoschka, Oskar (1886-1980) / Bridgeman Images

FLO4615925: Delta beetle, Trigonopeltastes delta 1, magnified 2, Antichira virens 3, Chlorocala smaragdina 4, Golofa aegeon 5, and Dipelicus geryon 6. Handcoloured lithograph from John O. Westwood's new edition of Dru Drury's “” Illustrations of Exotic Entomology,”” Bohn, London, 1837. / Bridgeman Images

TEC4615946: Gare de l'Est in Paris 75010. Architecture by Francois Alexandre Duquesney, 1852. Photography 17/04/09 / Bridgeman Images

PIX4615979: Mars - The crater that smiles - The Galle crater is 230 km in diameter and is located in the Argyre basin. Assembly of five images obtained by the Mars Express probe from 2004 to 2006 / Bridgeman Images

FLO4615832: Jamaican banner butterfly, Lucinia cadma 1,2, soldier pansy or soldier commodore, Junonia terea 3,4, and brilliant nymph, Acraea circeis 5,6. Handcoloured lithograph from John O. Westwood's new edition of Dru Drury's “” Illustrations of Exotic Entomology,”” Bohn, London, 1837. / Bridgeman Images

LRI4615864: Tale of pistils and etamines Painting by Franck (Frantisek) Kupka (1871-1957), 1919-1920 Oil on canvas Dim: 100x110 cm Prague, Narodni Gallery, Kupka, Frantisek (1871-1957) / Bridgeman Images

TEC4615882: Showcase of a real estate agency in Paris. Photography 25/08/07. / Bridgeman Images

FLO4615889: Yam hawk moth, Theretra nessus 1, Trichura druryi, female 2, Horama plumipes 3, and Levant hawk-moth, theretra alecto 4. Handcoloured lithograph from John O. Westwood's new edition of Dru Drury's “” Illustrations of Exotic Entomology,”” Bohn, London, 1837. / Bridgeman Images

TEC4615947: Gare de l'Est in Paris 75010. Architecture by Francois Alexandre Duquesney, 1852. Photography 17/04/09 / Bridgeman Images

FLO4615965: Cicada killer wasp, Sphecius grandis 1, pigeon tremex horntail, Tremex columba 2, harvester ant, Messor barbarus 3, shield beetle, Raphigaster validus 4, black and scarlet cicada, Huechys sanguinea 5,6, and fish hook ant, Polyrhachis bihamata 7,8. Handcoloured lithograph from John O. Westwood's new edition of Dru Drury's “” Illustrations of Exotic Entomology,”” Bohn, London, 1837. / Bridgeman Images

PIX4616015: March: Caldera of the volcano Apollinaris Patera - This Martian volcano is 180 to 280 km from its base and rises at about 5000 m altitude. Its caldera seen here by the Mars Express probe on October 26, 2004 measures 80 km in diameter and a depth of 1 km / Bridgeman Images

FLO4616099: Description has different stages of maturation of venous fungi: Amanite phalloides (left) and Amanite citrine variete mappa. Chromolithography in Atlas of edible and venenous mushrooms, 1891, by Leon Marie Dufour (1862-1942), French mycologist. / Bridgeman Images

PIX4616118: March: Promethei Planum - Mars: Promethei Planum - Promethei Planum is a region located near the southern pole of Mars. This region is seasonally covered with a thick layer of ice up to 3500 metres thick. On this image obtained by the Mars Express probe on September 22, 2005, an impact crater about 100 km wide and 800 metres deep is visible to the right (north). It is partially covered with ice. In the center of the image, structures formed by lava flows; on the left of the image, ice, which is an extension of the southern polar cap. Promethei Planum, an area seasonally covered with layer of ice more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera's focus on 22 September 2005 as Mars Express was in orbit above the Red Planet. Promethei Planum lies at approximately 76* south and 105* east. An approximately 100 km - large and 800 m - deep impact crater is visible in the northern part of the image. The crater's interior is partly covered in ice. In the centre of the image are structures that may have been created by basaltic lava flow from a volcano. This area is covered in ice. The dark dunes towards the bottom of the image are most likely made up of dust originating from this lava flow or volcanic ash. A broad sheet of ice, which is an extension of the south polar ice cap is located south of the lava flow, to the left in the (nadir) image. The steep flanks clearly show white, clean ice. The thickness of the ice is between 900 and 1100 m / Bridgeman Images

LRI4616199: Painting 0528 (oil on canvas, 1915), Magnelli, Alberto (1888-1971) / Bridgeman Images

FLO4611726: Fencers in outside guard/thrust positions, tierce and carte positions, tierce and second positions. Copperplate engraving by Robert Benard from the Fencing fencing section of Denis Diderot's Encyclopedia, Pellet, Geneva, 1779. / Bridgeman Images

PIX4611740: Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281 / Bridgeman Images

PIX4611764: Galaxies NGC 4631 and NGC 4656 - 57 in Hunting Dogs - Galaxies NGC 4631 and NGC 4656 - 57 - The spiral galaxy NGC 4631 (upper right) is a galaxy seen by the slice that is located at a distance of 30 million years - light. His small companion, the elliptical galaxy NGC 4627, is visible just above it. Below the irregular galaxies NGC 4656 and NGC 4657. Galaxies NGC 4631 (top right) and NGC 4656 (bottom left) are two unusual galaxies in Canes Venatici. A small companion galaxy, NGC 4627, can be seen next to NGC 4631. The galaxies, which are located about 30 million lights years away, get their unusual shapes from gravitational interactions with each other. NGC 6431 and NGC 4627 are also listed in ARP's Atlas of Peculiar Galaxies as Arp 281 / Bridgeman Images