'Sans Terre' images and/or videos results

Type # for projects,to access projects, > for users, and ? for help.

Your ongoing selection

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"UIG5447133","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"wealthy_american_passenger_on_the_titanic_mr_daniel_warner_marvin_19_from_new_york_ny_was_the_son_of","item_variant":"undefined"},{"item_id":"UIG5447092","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"how_the_titanic_survivors_were_picked_up_by_the_carpathia_photograph_taken_by_mr_j_w_barker_of_a_lif","item_variant":"undefined"},{"item_id":"UIG5447095","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"how_the_titanic_survivors_were_picked_up_by_the_carpathia_photograph_taken_by_mr_j_w_barker_of_titan","item_variant":"undefined"},{"item_id":"MMM7340101","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"unknown_artist_19th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"lieutenant_james_wilcox_d_1811_c_1806_09_watercolour_ivory_glass_gilt_human_hair","item_variant":"undefined"},{"item_id":"PFH2635107","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_the_imposing_hue_citadel_walls_and_moat_seen_from_the_southeastern_wall_hue","item_variant":"undefined"},{"item_id":"PIX4609266","item_category2":"no_copyright","item_category3":"standard","item_category4":"d_de_martin","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m33_in_the_triangle_spiral_galaxy_m33_in_triangulum_m33_ngc_598_the_galaxy_of_the_tria","item_variant":"undefined"},{"item_id":"PIX4622329","item_category2":"no_copyright","item_category3":"standard","item_category4":"w_promper","item_category5":"not_balown","item_list_name":"search_results","item_name":"elephant_tube_nebula_vdb_142_in_cephee_the_elephant_trunk_nebula_vdb_142_in_cepheus_ic1396_vdb_142_n","item_variant":"undefined"},{"item_id":"MMM7340699","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"russell_john_1745_1806","item_category5":"not_balown","item_list_name":"search_results","item_name":"nevil_maskelyne_1732_1811_c_1776_chalk_on_paper","item_variant":"undefined"},{"item_id":"PIX4622088","item_category2":"no_copyright","item_category3":"standard","item_category4":"stephane_guisard","item_category5":"not_balown","item_list_name":"search_results","item_name":"horsehead_nebula_ic_434_in_orion_horsehead_nebula_b33_in_orion_the_horse_s_head_nebula_barnard_33_is","item_variant":"undefined"},{"item_id":"PIX4622607","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebulae_ic_2948_and_2944_in_centaur_a_large_southern_emission_nebula_ic_2948_nebula_ic_2948_is_a_vas","item_variant":"undefined"},{"item_id":"PIX4623684","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_helix_ngc_7293_located_in_aquarius_is_one_of_the_closest_to_earth_c_690_light_years","item_variant":"undefined"},{"item_id":"USB1156639","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"dyck_anthony_van_1599_1641_manner_of","item_category5":"not_balown","item_list_name":"search_results","item_name":"henry_jermyn_1st_earl_of_st_albans_d_1684","item_variant":"undefined"},{"item_id":"PFH3277869","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_turtle_on_the_roof_of_the_royal_library_within_the_purple_forbidden_city_the_imperial_city_t","item_variant":"undefined"},{"item_id":"PIX4620228","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"southern_crown_nebula_the_corona_australis_nebula_ngc_6726_27_29_r_coronae_australis_is_a_region_of_","item_variant":"undefined"},{"item_id":"PIX4610440","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_m82_in_the_great_bear_seen_in_x_rays_the_galaxy_m82_seen_in_x_ray_image_obtained_by_chandra_i","item_variant":"undefined"},{"item_id":"PIX4565462","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_group_stephan_s_quintet_in_pegase_stephan_s_quintet_group_of_galaxies_image_obtained_with_t","item_variant":"undefined"},{"item_id":"IMO2122550","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"princess_juliena_airport_on_the_island_of_saint_martin_2007","item_variant":"undefined"},{"item_id":"BL3304990","item_category2":"out_of_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"mudras_inscribed_these_are_many_of_the_attitudes_assumed_by_the_lamas_in_their_devotions_each_of_whi","item_variant":"undefined"},{"item_id":"PFH3277861","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_detail_of_mandarins_and_dragons_on_the_roof_of_the_royal_library_within_the_purple_forbidden","item_variant":"undefined"},{"item_id":"PFH3277867","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_detail_of_mandarins_and_dragons_on_the_roof_of_the_royal_library_within_the_purple_forbidden","item_variant":"undefined"},{"item_id":"PFH2635102","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_cyclos_pass_in_front_of_the_flag_tower_of_the_imperial_city_the_citadel_hue","item_variant":"undefined"},{"item_id":"PIX4622787","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"neptune_voyager_2_neptune_has_an_equatorial_diameter_of_about_49_000_kilometres_its_blue_color_is_du","item_variant":"undefined"},{"item_id":"PIX4581418","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"stars_the_southern_cross_alpha_and_beta_of_centaur_southern_cross_and_pointers_star_trails_because_o","item_variant":"undefined"},{"item_id":"PIX4612202","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_centaurus_a_ngc_5128_x_ray_view_radio_visible_galaxy_centaurus_a_in_different_wavelengths_fal","item_variant":"undefined"},{"item_id":"PIX4609963","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_ngc_1614_interacting_galaxies_ngc_1614_the_galaxy_ngc_1614_is_located_about_200","item_variant":"undefined"},{"item_id":"PIX4610335","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"SRB1202781","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"boeng_yeak_lom_lake_ratanakiri_cambodia_photo","item_variant":"undefined"},{"item_id":"UIG5447100","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"how_the_titanic_survivors_were_picked_up_by_the_carpathia_photograph_taken_by_mr_j_w_barker_of_two_l","item_variant":"undefined"},{"item_id":"UIG5447097","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"how_the_titanic_survivors_were_picked_up_by_the_carpathia_photograph_taken_by_mr_j_w_barker_of_one_o","item_variant":"undefined"},{"item_id":"PFH3277863","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_detail_of_mandarins_and_mythical_creatures_on_the_roof_of_the_royal_library_within_the_purpl","item_variant":"undefined"},{"item_id":"PFH3277870","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_detail_of_a_phoenix_and_a_ky_lan_vietnamese_unicorn_on_the_roof_of_the_royal_library_within_","item_variant":"undefined"},{"item_id":"PIX4610399","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4618845","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_formation_in_the_nebula_ngc_2467_star_forming_region_ngc_2467_star_formation_in_the_nebula_ngc_","item_variant":"undefined"},{"item_id":"PIX4609292","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m33_in_the_triangle_spiral_galaxy_m33_in_triangulum_the_galaxy_of_the_triangle_m33_ngc","item_variant":"undefined"},{"item_id":"PIX4574313","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_7098_barred_spiral_galaxy_ngc_7098_the_barree_spiral_galaxy_ngc_7098_is_loc","item_variant":"undefined"},{"item_id":"BOF6323908","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"development_of_communications_from_telegraph_to_t_v","item_variant":"undefined"},{"item_id":"PRX3116836","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"raphael_raffaello_sanzio_of_urbino_1483_1520_after","item_category5":"not_balown","item_list_name":"search_results","item_name":"paul_preaches_in_athens_colour_litho","item_variant":"undefined"},{"item_id":"PFH3277860","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_the_royal_library_within_the_purple_forbidden_city_the_imperial_city_the_citadel_hue","item_variant":"undefined"},{"item_id":"PFH3277872","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"vietnam_roof_detail_at_the_royal_library_within_the_purple_forbidden_city_the_imperial_city_the_cita","item_variant":"undefined"},{"item_id":"PIX4622303","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"elephant_tube_nebula_vdb_142_in_cephee_the_elephant_trunk_nebula_vdb_142_in_cepheus_ic1396_vdb_142_n","item_variant":"undefined"},{"item_id":"PIX4610325","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_jay_gabany","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4620728","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_ngc_7635_in_cassiopee_the_bubble_nebula_this_nebula_is_located_about_8000_light_years_from_ea","item_variant":"undefined"},{"item_id":"PIX4581409","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"stars_the_southern_cross_alpha_and_beta_of_centaur_southern_cross_and_pointers_star_trails_because_o","item_variant":"undefined"},{"item_id":"PIX4613757","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_deep_field_north_hubble_deep_field_north_north_of_the_constellation_of_the_great_bear_the_hub","item_variant":"undefined"},{"item_id":"PIX4612937","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_arp_81_interacting_galaxies_arp_81_arp_81_is_located_about_300_million_light_ye","item_variant":"undefined"},{"item_id":"PIX4613210","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_markarian_533_interacting_galaxies_markarian_533_the_galaxy_ngc_7674_markarian_","item_variant":"undefined"},{"item_id":"GRL6166444","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"byzantine_12th_13th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"apsidal_arch_etymasia_preparation_for_the_throne_with_the_instruments_of_passion_restored_in_1979_by","item_variant":"undefined"},{"item_id":"UIG5447101","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"how_the_titanic_survivors_were_picked_up_by_the_carpathia_photograph_taken_by_mr_j_w_barker_of_someo","item_variant":"undefined"},{"item_id":"UIG5447128","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"herbert_fitzhugh_walter_mcelroy_chief_purser_of_rms_titanic_was_born_28th_october_1874_in_liverpool_","item_variant":"undefined"},{"item_id":"UIG5447091","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"how_the_titanic_survivors_were_picked_up_by_the_carpathia_photographs_taken_by_mr_j_w_barker_a_passe","item_variant":"undefined"},{"item_id":"PIX4613022","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"irregular_galaxy_ngc_6822_in_sagittarius_irregular_galaxy_ngc_6822_in_sagittarius_the_galaxy_ngc_682","item_variant":"undefined"},{"item_id":"PIX4624891","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"saturn_and_satellites_seen_by_the_hubble_space_telescope_saturn_rings_edge_on_with_satellites_saturn","item_variant":"undefined"},{"item_id":"PIX4610471","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_3079_in_the_great_bear_spiral_galaxy_ngc_3079_ngc_3079_is_a_spiral_galaxy_distant_","item_variant":"undefined"},{"item_id":"PIX4619350","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebulae_ngc_6334_and_ngc_6357_in_scorpio_nebulae_ngc_6334_and_ngc_6357_in_scorpius_these_nebulae_are","item_variant":"undefined"},{"item_id":"UIG5447130","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"john_george_jack_phillips_wireless_operator_on_titanic_jack_philips_was_born_in_farncombe_surrey_on_","item_variant":"undefined"},{"item_id":"GRL3743649","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_representing_a_captured_moor_from_the_marble_theatre_monument_to_philip_v_facing_the_royal_pa","item_variant":"undefined"},{"item_id":"CH3504152","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"ryckaert_marten_1587_1631","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_rocky_landscape_with_figures_by_an_iron_foundry_a_river_and_houses_on_the_bank_beyond_oil_on_panel","item_variant":"undefined"},{"item_id":"PIX4613420","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"irregular_galaxy_of_the_little_magellan_cloud_ngc_292_the_small_magellanic_cloud_the_galaxy_of_the_l","item_variant":"undefined"},{"item_id":"PIX4612203","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_centaurus_a_ngc_5128_in_visible_and_infrared_galaxy_centaurus_a_in_visible_and_infrared_the_g","item_variant":"undefined"},{"item_id":"PIX4612910","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"black_hole_collision_in_ngc_6240_black_holes_colliding_in_ngc_6240_the_galaxy_ngc_6240_is_located_ab","item_variant":"undefined"}]}}

Type # for projects,to access projects, > for users, and ? for help.

Advanced Search Search Tips

Images of 'Sans Terre' found, 49,156

«
1
…
814
815
816
…
820
»

Wealthy American passenger on the Titanic, Mr Daniel Warner Marvin, 19, from New York, NY, was the son of Henry Norton Marvin. Henry Norton Marvin was founder of the early motion picture production houses of American Mutoscope and the Biograph Company. Daniel was married to Mary Farquarson. They both boarded the Titanic at Southampton as first class passengers. They were returning to New York City from their honeymoon in Europe. They occupied cabin D-30. On the night of the accident Daniel assisted his wife to a boat with the words 'It's alright, little girl. You go. I will stay.' Daniel died in the sinking, his body, if recovered, was never identified. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911, and sank on 15th April, 1912, after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) Photographi

Wealthy American passenger on the Titanic, Mr Daniel Warner Marvin, 19, from New York, NY, was the son of Henry Norton Marvin. Henry Norton Marvin was founder of the early motion picture production houses of American Mutoscope and the Biograph Company. Daniel was married to Mary Farquarson. They both boarded the Titanic at Southampton as first class passengers. They were returning to New York City from their honeymoon in Europe. They occupied cabin D-30. On the night of the accident Daniel assisted his wife to a boat with the words 'It's alright, little girl. You go. I will stay.' Daniel died in the sinking, his body, if recovered, was never identified. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911, and sank on 15th April, 1912, after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) Photographi

UIG5447133

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of a lifeboat containing passengers from the Titanic, as it approaches the Carpathia. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photographie ©UIG/

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of a lifeboat containing passengers from the Titanic, as it approaches the Carpathia. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photographie ©UIG/

UIG5447092

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of Titanic survivors being waited on by Carpathia passengers. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photographie ©UIG/Leemage

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of Titanic survivors being waited on by Carpathia passengers. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photographie ©UIG/Leemage

UIG5447095

Lieutenant James Wilcox (d. 1811), c.1806-09 (watercolour, ivory, glass, gilt, human hair)

Lieutenant James Wilcox (d. 1811), c.1806-09 (watercolour, ivory, glass, gilt, human hair)

Unknown Artist, (19th century)

MMM7340101

Vietnam: The imposing Hue Citadel walls and moat seen from the southeastern wall, Hue

Vietnam: The imposing Hue Citadel walls and moat seen from the southeastern wall, Hue

David Henley

PFH2635107

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This image is a composite of two black and white images obtained from the 1.2m telescope of Mount Palomar, California. Spiral galaxy M33 is a mid - sized member of our Local Group of Galaxies. M33 is also called the Triangulum Galaxy for the constellation in which it resides. About four times smaller (in radius) than our Milky Way Galaxy and the Andromeda Galaxy (M31), it is much larger than the many of the local dwarf spheroidal galaxies. M33's proximity to M31 causes it to be thought by some to be a satellite galaxy of this more massive galaxy. M33's proximity to our Milky Way Galaxy causes it to appear more than twice the angular size of the Full Moon, and be visible with a good pair of binoculars. <BR>This image is a composite from black and

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This image is a composite of two black and white images obtained from the 1.2m telescope of Mount Palomar, California. Spiral galaxy M33 is a mid - sized member of our Local Group of Galaxies. M33 is also called the Triangulum Galaxy for the constellation in which it resides. About four times smaller (in radius) than our Milky Way Galaxy and the Andromeda Galaxy (M31), it is much larger than the many of the local dwarf spheroidal galaxies. M33's proximity to M31 causes it to be thought by some to be a satellite galaxy of this more massive galaxy. M33's proximity to our Milky Way Galaxy causes it to appear more than twice the angular size of the Full Moon, and be visible with a good pair of binoculars. <BR>This image is a composite from black and

D. De Martin

PIX4609266

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and

W. Promper

PIX4622329

Nevil Maskelyne (1732 -1811), c.1776 (chalk on paper)

Nevil Maskelyne (1732 -1811), c.1776 (chalk on paper)

Russell, John (1745-1806)

MMM7340699

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20

Stephane Guisard

PIX4622088

Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation. There are young stars scattered through the nebula and these stars are responsible for its existence

Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation. There are young stars scattered through the nebula and these stars are responsible for its existence

PIX4622607

Planetary nebula Helix (NGC 7293), located in Aquarius, is one of the closest to Earth (c. 690 light years) Image by the 2.2m Max Planck Society/ESO/MPG telescope of the La Silla Observatory in Chile.

Planetary nebula Helix (NGC 7293), located in Aquarius, is one of the closest to Earth (c. 690 light years) Image by the 2.2m Max Planck Society/ESO/MPG telescope of the La Silla Observatory in Chile.

PIX4623684

Henry Jermyn, 1st Earl of St Albans (d.1684)

Henry Jermyn, 1st Earl of St Albans (d.1684)

Dyck, Anthony van (1599-1641) (manner of)

USB1156639

Vietnam: Turtle on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

Vietnam: Turtle on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

David Henley

PFH3277869

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

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

PIX4620228

Galaxy M82 in the Great Bear seen in X-rays - The galaxy M82 seen in X-ray - Image obtained by Chandra in X-rays, reveals a cloud (in red) of very hot gas of several million degres emitted from the central regions of the galaxy. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Chandra's X - ray image reveals gas that has been heated to millions of degrees by the violent outflow of matter blasting out of the galaxy. The eruption can be traced back to the central regions of the galaxy where stars are forming at a furious rate, some 10 times faster than in the Milky Way Galaxy. Many of these newly formed stars are very massive and race through their evolution to explode as supernovas. Vigorous mass loss f

Galaxy M82 in the Great Bear seen in X-rays - The galaxy M82 seen in X-ray - Image obtained by Chandra in X-rays, reveals a cloud (in red) of very hot gas of several million degres emitted from the central regions of the galaxy. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Chandra's X - ray image reveals gas that has been heated to millions of degrees by the violent outflow of matter blasting out of the galaxy. The eruption can be traced back to the central regions of the galaxy where stars are forming at a furious rate, some 10 times faster than in the Milky Way Galaxy. Many of these newly formed stars are very massive and race through their evolution to explode as supernovas. Vigorous mass loss f

PIX4610440

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

PIX4565462

Princess Juliena Airport on the island of Saint Martin 2007

Princess Juliena Airport on the island of Saint Martin 2007

IMO2122550

Mudras. Inscribed: ' 'These are many of the attitudes assumed by the lamas in their devotions, each of which has a different name'. '1. Sagnon gnyumshak' [sa-gnon-gnam-gzag]. 'Sanon means that one hand is bent towards sa, the earth, and gnumshak contemplation. Shakya is' 'said to have assumed this position when he was only three years of age'. '2'. 'Gnyumshak' [gnam-gzag]. 'Shakya placed his hands in this position when he was reading'. '3. bSumstun' [bsam-stan]' Shakya sat in this position they say night and day for six years' [when he was in the desert]' in the Kingdom of Oudipa on the borders of Naracara'.. '4. bsKyuschin' [bskyabs-sbyin]' Shakya assumed this position after he had done his contemplation and was explaining everything to his disciples'. '5. Chhoschud' [chos-chad]' Shakya explaining passages in his holy works'. '6. Dingzub' [sdin-rdzub]' Shakya is said to have placed his fingers in this position when he reprimanded the Rakhas because they would not obey his orders: and

Mudras. Inscribed: ' 'These are many of the attitudes assumed by the lamas in their devotions, each of which has a different name'. '1. Sagnon gnyumshak' [sa-gnon-gnam-gzag]. 'Sanon means that one hand is bent towards sa, the earth, and gnumshak contemplation. Shakya is' 'said to have assumed this position when he was only three years of age'. '2'. 'Gnyumshak' [gnam-gzag]. 'Shakya placed his hands in this position when he was reading'. '3. bSumstun' [bsam-stan]' Shakya sat in this position they say night and day for six years' [when he was in the desert]' in the Kingdom of Oudipa on the borders of Naracara'.. '4. bsKyuschin' [bskyabs-sbyin]' Shakya assumed this position after he had done his contemplation and was explaining everything to his disciples'. '5. Chhoschud' [chos-chad]' Shakya explaining passages in his holy works'. '6. Dingzub' [sdin-rdzub]' Shakya is said to have placed his fingers in this position when he reprimanded the Rakhas because they would not obey his orders: and

BL3304990

Vietnam: Detail of mandarins and dragons on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

Vietnam: Detail of mandarins and dragons on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

David Henley

PFH3277861

Vietnam: Detail of mandarins and dragons on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

Vietnam: Detail of mandarins and dragons on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

David Henley

PFH3277867

Vietnam: Cyclos pass in front of the flag tower of the Imperial City, The Citadel, Hue

Vietnam: Cyclos pass in front of the flag tower of the Imperial City, The Citadel, Hue

David Henley

PFH2635102

Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The brig

Neptune - Voyager 2 - Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Image of Neptune obtained by the Voyager 2 probe on August 16, 1989. During August 16 and 17, 1989, the Voyager 2 narrow - angle camera was used to photograph Neptune almost continuously, recording approximately two and one - half rotations of the planet. These images represent the most complete set of full disk Neptune images that the spacecraft will acquire. This picture from the sequence shows two of the four cloud features which have been tracked by the Voyager cameras during the past two months. The large dark oval near the western limb (the left edge) is at a latitude of 22 degrees south and circuits Neptune every 18.3 hours. The brig

PIX4622787

Stars - The Southern Cross - Alpha and Beta of Centaur - Southern Cross and pointers - Star trails - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here it is the constellation of the Southern Cross (center right) and the Centaurus Alpha and Beta stars, in the center below, that are photographed in this way during a 30-minute pose. Star images are point sources of light of widely varying intensity. Normally, no single photographic exposure on colour film can capture their subtle colours. Those stars whose intensity is just right for their colour to be recorded appear insignificant on the photograph, while anything brighter is overexposed and washed out. By changing the focus of the lens during a star trail exposure, star images are spread out over the film surface. This effectively changes the amount

Stars - The Southern Cross - Alpha and Beta of Centaur - Southern Cross and pointers - Star trails - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here it is the constellation of the Southern Cross (center right) and the Centaurus Alpha and Beta stars, in the center below, that are photographed in this way during a 30-minute pose. Star images are point sources of light of widely varying intensity. Normally, no single photographic exposure on colour film can capture their subtle colours. Those stars whose intensity is just right for their colour to be recorded appear insignificant on the photograph, while anything brighter is overexposed and washed out. By changing the focus of the lens during a star trail exposure, star images are spread out over the film surface. This effectively changes the amount

PIX4581418

Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the out

Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the out

PIX4612202

Interacting galaxies NGC 1614 - Interacting galaxies NGC 1614 - The galaxy NGC 1614 is located about 200 million light years away from Earth in the southern constellation of Eridan. This system is composed of interacting galaxies. Image obtained by the Hubble Space Telescope on August 13, 2002. The galaxy system NGC 1614 has a bright optical center and two clear inner spiral arms that are fairly symmetrical. It also has a spectacular outer structure that consists principally of a large one - sided curved extension of one of these arms to the lower right, and a long, almost straight tail that emerges from the nucleus and crosses the extended arm to the upper right. The galaxy appears to be the result of a tidal interaction and the resulting merger of two predecessor systems. The system has a nuclear region of quasar - like luminosity, but shows no direct evidence for an active nucleus. It is heavily and unevenly reddened across its nucleus, while infrared imaging also shows a ridge of d

Interacting galaxies NGC 1614 - Interacting galaxies NGC 1614 - The galaxy NGC 1614 is located about 200 million light years away from Earth in the southern constellation of Eridan. This system is composed of interacting galaxies. Image obtained by the Hubble Space Telescope on August 13, 2002. The galaxy system NGC 1614 has a bright optical center and two clear inner spiral arms that are fairly symmetrical. It also has a spectacular outer structure that consists principally of a large one - sided curved extension of one of these arms to the lower right, and a long, almost straight tail that emerges from the nucleus and crosses the extended arm to the upper right. The galaxy appears to be the result of a tidal interaction and the resulting merger of two predecessor systems. The system has a nuclear region of quasar - like luminosity, but shows no direct evidence for an active nucleus. It is heavily and unevenly reddened across its nucleus, while infrared imaging also shows a ridge of d

PIX4609963

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. Image obtained with a 50 cm telescope through different filters, total of different poses: 20h. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral gala

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. Image obtained with a 50 cm telescope through different filters, total of different poses: 20h. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral gala

R. Gendler

PIX4610335

Boeng Yeak Lom Lake, Ratanakiri, Cambodia (photo)

Boeng Yeak Lom Lake, Ratanakiri, Cambodia (photo)

Sergi Reboredo

SRB1202781

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of two lifeboats containing passengers from the Titanic, as it approaches the Carpathia. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photographie ©

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of two lifeboats containing passengers from the Titanic, as it approaches the Carpathia. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photographie ©

UIG5447100

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of one of Titanic's collaspible boats containing about 30 people, approaching the Carpathia. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photograph

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of one of Titanic's collaspible boats containing about 30 people, approaching the Carpathia. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photograph

UIG5447097

Vietnam: Detail of mandarins and mythical creatures on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

Vietnam: Detail of mandarins and mythical creatures on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

David Henley

PFH3277863

Vietnam: Detail of a phoenix and a 'ky lan' (Vietnamese unicorn) on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

Vietnam: Detail of a phoenix and a 'ky lan' (Vietnamese unicorn) on the roof of the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

David Henley

PFH3277870

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major: The spiral galaxy M81 is located 12 million light years from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. - M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate much

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major: The spiral galaxy M81 is located 12 million light years from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. - M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate much

PIX4610399

Star formation in the nebula NGC 2467 - Star - forming region NGC 2467 - Star formation in the nebula NGC 2467, located approximately 17,000 years ago - light from Earth in the southern constellation of Stern. Image obtained by the Hubble Space Telescope in 2004. A colourful star - forming region is featured in this stunning new NASA/ESA Hubble Space Telescope image of NGC 2467. Looking like a roiling cauldron of some exotic cosmic brew, huge clouds of gas and dust are sprinkled with bright blue, hot young stars. Strangely shaped dust clouds, resembling spilled liquids, are silhouetted against a colourful background of glowing. Like the familiar Orion Nebula, NGC 2467 is a huge cloud of gas - - mostly hydrogen - - that serves as an incubator for new stars. It is located about 17,000 light years away in the southern constellation of Puppis. This picture was created from images taken with the Wide Field Channel of the Advanced Camera for Surveys through three different filters (F550M, F6

Star formation in the nebula NGC 2467 - Star - forming region NGC 2467 - Star formation in the nebula NGC 2467, located approximately 17,000 years ago - light from Earth in the southern constellation of Stern. Image obtained by the Hubble Space Telescope in 2004. A colourful star - forming region is featured in this stunning new NASA/ESA Hubble Space Telescope image of NGC 2467. Looking like a roiling cauldron of some exotic cosmic brew, huge clouds of gas and dust are sprinkled with bright blue, hot young stars. Strangely shaped dust clouds, resembling spilled liquids, are silhouetted against a colourful background of glowing. Like the familiar Orion Nebula, NGC 2467 is a huge cloud of gas - - mostly hydrogen - - that serves as an incubator for new stars. It is located about 17,000 light years away in the southern constellation of Puppis. This picture was created from images taken with the Wide Field Channel of the Advanced Camera for Surveys through three different filters (F550M, F6

PIX4618845

Spiral Galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - The Galaxy of the Triangle (M33, NGC598) is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red, the star-forming regions appear, especially at the top left NGC 604 one of the largest and most active star-forming regions. It extends over 150 years of light. Image obtained from the Isaac Newton telescope of La Palma. M33 is a large, almost face - on spiral galaxy about 2.5 million light years distant in the northern constellation of Triangulum. It is a member of the 'Local Group' of galaxies, which is dominated by the Milky Way and M31. Like M31, M33 is approaching the Milky Way at a velocity of about 180km/s. Although the total light M33 galaxy is that of a star of magnitude 5.3, its large diameter makes it hard to see. However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by

Spiral Galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - The Galaxy of the Triangle (M33, NGC598) is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red, the star-forming regions appear, especially at the top left NGC 604 one of the largest and most active star-forming regions. It extends over 150 years of light. Image obtained from the Isaac Newton telescope of La Palma. M33 is a large, almost face - on spiral galaxy about 2.5 million light years distant in the northern constellation of Triangulum. It is a member of the 'Local Group' of galaxies, which is dominated by the Milky Way and M31. Like M31, M33 is approaching the Milky Way at a velocity of about 180km/s. Although the total light M33 galaxy is that of a star of magnitude 5.3, its large diameter makes it hard to see. However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by

PIX4609292

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

PIX4574313

Development Of Communications - From Telegraph To T.V.

Development Of Communications - From Telegraph To T.V.

BOF6323908

Paul preaches in Athens (colour litho)

Paul preaches in Athens (colour litho)

Raphael (Raffaello Sanzio of Urbino) (1483-1520) (after)

PRX3116836

Vietnam: The Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

Vietnam: The Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

David Henley

PFH3277860

Vietnam: Roof detail at the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

Vietnam: Roof detail at the Royal Library within the Purple Forbidden City, The Imperial City, The Citadel, Hue

David Henley

PFH3277872

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in d

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight oxygen, hydrogen, and sulfur. The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc - minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H - II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50 - 100 member stars which vary in brightness spanning an area of approximately 50 'in d

PIX4622303

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. Image obtained by an amateur telescope of 50 cm, composting different poses. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. Image obtained by an amateur telescope of 50 cm, composting different poses. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (

R. Jay GaBany

PIX4610325

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to

Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to

PIX4620728

Stars - The Southern Cross - Alpha and Beta of Centaur - Southern Cross and pointers - Star trails - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here, the constellation of the Southern Cross and the Alpha and Beta stars of the Centaurus, on the left, are photographed this way during a 40mn pose. Star images are point sources of light of widely varying intensity. Normally, no single photographic exposure on colour film can capture their subtle colours. Those stars whose intensity is just right for their colour to be recorded appear insignificant on the photograph, while anything brighter is overexposed and washed out. By changing the focus of the lens during a star trail exposure, star images are spread out over the film surface. This effectively changes the amount of light in each star image as wel

Stars - The Southern Cross - Alpha and Beta of Centaur - Southern Cross and pointers - Star trails - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here, the constellation of the Southern Cross and the Alpha and Beta stars of the Centaurus, on the left, are photographed this way during a 40mn pose. Star images are point sources of light of widely varying intensity. Normally, no single photographic exposure on colour film can capture their subtle colours. Those stars whose intensity is just right for their colour to be recorded appear insignificant on the photograph, while anything brighter is overexposed and washed out. By changing the focus of the lens during a star trail exposure, star images are spread out over the film surface. This effectively changes the amount of light in each star image as wel

PIX4581409

Hubble deep field north - Hubble Deep Field North - North of the constellation of the Great Bear, the Hubble space telescope posed 75h to obtain this image of the distant universe. More than 1500 galaxies distant from 1 to 12 billion years - light are visible in this image. From Earth, the target field is the one “” that one would see through the eye of a needle held at arm's length.” If the distribution of galaxies over the entire Celestial vault were similar to this field, the number of galaxies observable up to magnitude 30 would be 50 billion. Representing a narrow “” keyhole”” view all the way to the visible horizon of the universe, the HDF image covers a speck of sky 1/30th the diameter of the full Moon. This is so narrow, just a few foreground stars in our Milky Way galaxy are visible and are vastly outnumbered by the menagerie of far more distant galaxies, some nearly as faint as 30th magnitude, or nearly four billion times fainter than the limits of human vision. Although the

Hubble deep field north - Hubble Deep Field North - North of the constellation of the Great Bear, the Hubble space telescope posed 75h to obtain this image of the distant universe. More than 1500 galaxies distant from 1 to 12 billion years - light are visible in this image. From Earth, the target field is the one “” that one would see through the eye of a needle held at arm's length.” If the distribution of galaxies over the entire Celestial vault were similar to this field, the number of galaxies observable up to magnitude 30 would be 50 billion. Representing a narrow “” keyhole”” view all the way to the visible horizon of the universe, the HDF image covers a speck of sky 1/30th the diameter of the full Moon. This is so narrow, just a few foreground stars in our Milky Way galaxy are visible and are vastly outnumbered by the menagerie of far more distant galaxies, some nearly as faint as 30th magnitude, or nearly four billion times fainter than the limits of human vision. Although the

PIX4613757

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

PIX4612937

Interacting galaxies Markarian 533 - Interacting galaxies Markarian 533 - The galaxy NGC 7674 (Markarian 533 or Arp 182) is located about 400 million years ago - light from Earth in the constellation Pegase. It is the most important member of a group of galaxies called Hickson 96 (HCG 96). This spiral galaxy seen from the front is in interaction with other companion galaxies. It has an active core. Image obtained by the Hubble Space Telescope on June 9, 2002. NGC 7674 (seen just above the center), also known as Markarian 533, is the brightest and largest member of the so - called Hickson 96 compact group of galaxies, consisting of four galaxies. This stunning Hubble image shows a spiral galaxy nearly face - on. The central bar - shaped structure is made up of stars. The shape of NGC 7674, including the long narrow streamers seen to the left of and below the galaxy can be accounted for by tidal interactions with its companions. NGC 7674 has a powerful active nucleus of the kind known as

Interacting galaxies Markarian 533 - Interacting galaxies Markarian 533 - The galaxy NGC 7674 (Markarian 533 or Arp 182) is located about 400 million years ago - light from Earth in the constellation Pegase. It is the most important member of a group of galaxies called Hickson 96 (HCG 96). This spiral galaxy seen from the front is in interaction with other companion galaxies. It has an active core. Image obtained by the Hubble Space Telescope on June 9, 2002. NGC 7674 (seen just above the center), also known as Markarian 533, is the brightest and largest member of the so - called Hickson 96 compact group of galaxies, consisting of four galaxies. This stunning Hubble image shows a spiral galaxy nearly face - on. The central bar - shaped structure is made up of stars. The shape of NGC 7674, including the long narrow streamers seen to the left of and below the galaxy can be accounted for by tidal interactions with its companions. NGC 7674 has a powerful active nucleus of the kind known as

PIX4613210

Apsidal arch: Etymasia (preparation for the throne) with the instruments of passion, restored in 1979; Byzantine school mosaic with a golden background (mosaic)

Apsidal arch: Etymasia (preparation for the throne) with the instruments of passion, restored in 1979; Byzantine school mosaic with a golden background (mosaic)

Byzantine, (12th-13th century)

Ghigo Roli

GRL6166444

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of someone fixing a rope step ladder from one of Titanic's lifeboats to the Carpathia. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photographie ©UIG

How the Titanic Survivors Were Picked up by the Carpathia. Photograph taken by Mr J W Barker of someone fixing a rope step ladder from one of Titanic's lifeboats to the Carpathia. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group). Photographie ©UIG

UIG5447101

Herbert Fitzhugh Walter McElroy, Chief Purser of RMS Titanic, was born 28th October 1874 in Liverpool. Purser Hugh McElroy had been in White Star's service for some thirteen years and had served for three years on board the troopship ""Britannic"" during the Boar War. He signed on the Titanic on the 9th April 1912 as Chief Purser on a salary of £20 per month. He helped load passengers in to the lifeboats when Titanic was sinking. Purser McElroy was last seen standing on the Boat-Deck near the gymnasium, beside mail clerk Mr William Logan Gwinn, both men died in the sinking of the Titanic. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911, and sank on 15ht April, 1912, after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) Photographie ©UIG/Leemage

Herbert Fitzhugh Walter McElroy, Chief Purser of RMS Titanic, was born 28th October 1874 in Liverpool. Purser Hugh McElroy had been in White Star's service for some thirteen years and had served for three years on board the troopship ""Britannic"" during the Boar War. He signed on the Titanic on the 9th April 1912 as Chief Purser on a salary of £20 per month. He helped load passengers in to the lifeboats when Titanic was sinking. Purser McElroy was last seen standing on the Boat-Deck near the gymnasium, beside mail clerk Mr William Logan Gwinn, both men died in the sinking of the Titanic. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911, and sank on 15ht April, 1912, after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) Photographie ©UIG/Leemage

UIG5447128

How the Titanic Survivors Were Picked up by the Carpathia. Photographs taken by Mr J W Barker, a passenger on Carpathia, as passengers are rescued from the Titanic lifeboats. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) Photographie ©UIG/Leem

How the Titanic Survivors Were Picked up by the Carpathia. Photographs taken by Mr J W Barker, a passenger on Carpathia, as passengers are rescued from the Titanic lifeboats. Carpathia was sailing from New York City to Rijeka on the night of Sunday, 14 April 1912. The captain, Arthur Henry Rostron, was asleep in his cabin when wireless operator Harold Cottam burst in and told him of Titanic's distress signal. Captain Rostron immediately set course to the liner's last known position, over 60 miles away. At 4 o'clock in the morning Carpathia arrived at the scene after working her way through dangerous ice fields and was able to save 705 people. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911 and sank on April 15th, 1912 after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New York, USA, with the loss of 1,522 passengers and crew. (Photo by Titanic Images/Universal Images Group) Photographie ©UIG/Leem

UIG5447091

Irregular galaxy NGC 6822 in Sagittarius - Irregular galaxy NGC 6822 in Sagittarius - The galaxy NGC 6822 is about 1.6 million years away - light from Earth. She belongs to our local group. Image obtained with a telescope of 35 cm, 12 hours of poses. The irregular dwarf galaxy NGC 6822 is located at only 1,6 million light year. It is a member of our local group and the third nearest galaxy to the Milky Way after the Sagittarius Dwarf Elliptical and the Magellanic Clouds. The galaxy was discovered by Barnard in 1881 using a 6 inch refractor. It is very similar to the LMC with its weak bar and its irregular distribution of bright OB associations and HII regions. In 1925 in a classic paper, Edwin Hubble reported on several bright objects in NGC 6822, later found to represent a grouping of bright star clusters and HII regions. The galaxy is rich in neutral hydrogen gas, the essential fuel of star formation. NGC 6822 started forming stars some 10 billion years ago. Similar to the LMC it has

Irregular galaxy NGC 6822 in Sagittarius - Irregular galaxy NGC 6822 in Sagittarius - The galaxy NGC 6822 is about 1.6 million years away - light from Earth. She belongs to our local group. Image obtained with a telescope of 35 cm, 12 hours of poses. The irregular dwarf galaxy NGC 6822 is located at only 1,6 million light year. It is a member of our local group and the third nearest galaxy to the Milky Way after the Sagittarius Dwarf Elliptical and the Magellanic Clouds. The galaxy was discovered by Barnard in 1881 using a 6 inch refractor. It is very similar to the LMC with its weak bar and its irregular distribution of bright OB associations and HII regions. In 1925 in a classic paper, Edwin Hubble reported on several bright objects in NGC 6822, later found to represent a grouping of bright star clusters and HII regions. The galaxy is rich in neutral hydrogen gas, the essential fuel of star formation. NGC 6822 started forming stars some 10 billion years ago. Similar to the LMC it has

R. Gendler

PIX4613022

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

PIX4624891

Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. This false-colored image obtained by the Hubble Space Telescope in 1998 shows that a huge gas bubble escapes from the galaxy. This bubble rises more than 3500 years ago - light above the disk of the galaxy. It is a wind from hot stars and blends with very hot gas from supernovae explosions that would cause this bubble. The picture shows the bubble in the center of the NGC 3079 galaxy's disk. The structure is more than 3,000 light - years wide and rises 3,500 light - years above the galaxy's disk. Astronomers suspect that the bubble is being blown by “” winds”” (high - speed streams of particles) released during a burst of star formation. Eventually, this gas will rain down upon the galaxy's disk where it may collide with gas clouds, compress them, and form a new generation of stars. The two white

Spiral Galaxy NGC 3079 in the Great Bear - Spiral galaxy NGC 3079 - NGC 3079 is a spiral galaxy distant about 50 million years - light from Earth. His disc measures about 70,000 years - light. This false-colored image obtained by the Hubble Space Telescope in 1998 shows that a huge gas bubble escapes from the galaxy. This bubble rises more than 3500 years ago - light above the disk of the galaxy. It is a wind from hot stars and blends with very hot gas from supernovae explosions that would cause this bubble. The picture shows the bubble in the center of the NGC 3079 galaxy's disk. The structure is more than 3,000 light - years wide and rises 3,500 light - years above the galaxy's disk. Astronomers suspect that the bubble is being blown by “” winds”” (high - speed streams of particles) released during a burst of star formation. Eventually, this gas will rain down upon the galaxy's disk where it may collide with gas clouds, compress them, and form a new generation of stars. The two white

PIX4610471

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius - These nebulae are located approximately 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebulae NGC 6334 and NGC 6357 show no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. These nebulae are quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Ca

Nebulae NGC 6334 and NGC 6357 in Scorpio - Nebulae NGC 6334 and NGC 6357 in Scorpius - These nebulae are located approximately 5500 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. The star - forming nebulae NGC 6334 and NGC 6357 show no evidence of a blue component in their colour - indeed, the blue - light plate used in these 3 - colour pictures had no nebulous image at all - nor is there any obvious sign of the bright blue stars normally found in these objects. They are excellent examples of the phenomenon known as 'interstellar reddening', the selective removal of blue light by minute particles of dust in the line of sight. This accounts for both the ruddy hue and apparent absence of blue stars. The hot stars are present but only some of the red part of their light is seen so they are not conspicuous. These nebulae are quite nearby (5500 light years) but located close to the Galactic plane and are buried in the dust of the Milky Way. Ca

PIX4619350

John George 'Jack' Phillips Wireless Operator on Titanic. Jack Philips was born in Farncombe, Surrey, on 11th April 1887. Phillips was educated locally and, after learning telegraphy, at a post office, he began working for the Marconi company. He was serving as senior wireless operator on board Titanic, which sank on 15th April 1912. As Titanic was sinking, Phillips worked tirelessly to send wireless messages to nearby ships for help. While Phillips has borne criticism for having told the radio operator of the Californian 'Shut up! I am busy, I am working Cape Race!' when interrupted on-air by his counterpart telling him that his ship was surrounded by ice, similar warning messages earlier that day had been delivered to the captain and a lookout had been posted. He did not survive. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911, and sank after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New Yor

John George 'Jack' Phillips Wireless Operator on Titanic. Jack Philips was born in Farncombe, Surrey, on 11th April 1887. Phillips was educated locally and, after learning telegraphy, at a post office, he began working for the Marconi company. He was serving as senior wireless operator on board Titanic, which sank on 15th April 1912. As Titanic was sinking, Phillips worked tirelessly to send wireless messages to nearby ships for help. While Phillips has borne criticism for having told the radio operator of the Californian 'Shut up! I am busy, I am working Cape Race!' when interrupted on-air by his counterpart telling him that his ship was surrounded by ice, similar warning messages earlier that day had been delivered to the captain and a lookout had been posted. He did not survive. Titanic was built by Harland & Wolff in Belfast Ireland during 1910 - 1911, and sank after striking an iceberg off the coast of New Foundland during her maiden voyage from Southampton, England to New Yor

UIG5447130

Detail representing a captured Moor from "The Marble Theatre", Monument to Philip V facing The royal Palace or Palace of the Normans, the Parliament Square, Palermo, Sicily, Italy (photo)

Detail representing a captured Moor from "The Marble Theatre", Monument to Philip V facing The royal Palace or Palace of the Normans, the Parliament Square, Palermo, Sicily, Italy (photo)

GRL3743649

A rocky landscape with figures by an iron foundry, a river and houses on the bank beyond (oil on panel)

A rocky landscape with figures by an iron foundry, a river and houses on the bank beyond (oil on panel)

Ryckaert, Marten (1587-1631)

CH3504152

Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Little Magellan Cloud is about 240,000 light years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Infrared image obtained by Spitzer space telescope. This infrared portrait of the Small Magellanic Cloud, taken by Nasa's Spitzer Space Telescope, reveals the stars and dust in this galaxy as never seen before. The Small Magellanic Cloud is a nearby satellite galaxy to our Milky Way galaxy, approximately 200,000 light - years away. The image shows the main body of the Small Magellanic Cloud, which is comprised of the “” bar”” on the left and a “” wing”” extending to the right. The bar contains both old stars (in blue) and young stars lighting up their natal dust (green/red). The wing mainly contains young stars. In addition, the image contains a galactic globular cluster in the lower left (blue cluster of stars) and emission from

Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Little Magellan Cloud is about 240,000 light years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Infrared image obtained by Spitzer space telescope. This infrared portrait of the Small Magellanic Cloud, taken by Nasa's Spitzer Space Telescope, reveals the stars and dust in this galaxy as never seen before. The Small Magellanic Cloud is a nearby satellite galaxy to our Milky Way galaxy, approximately 200,000 light - years away. The image shows the main body of the Small Magellanic Cloud, which is comprised of the “” bar”” on the left and a “” wing”” extending to the right. The bar contains both old stars (in blue) and young stars lighting up their natal dust (green/red). The wing mainly contains young stars. In addition, the image contains a galactic globular cluster in the lower left (blue cluster of stars) and emission from

PIX4613420

Galaxy Centaurus A (NGC 5128) in visible and infrared - Galaxy Centaurus A in visible and infrared - The galaxy NGC 5128 is about 13 million years away - light from Earth. This an elliptical galaxy that cannibalized a small spiral galaxy. The infrared image, on the right, reveals the complex structure of the central dust strip. Images obtained on the left by Cerro Tololo's 4m telescope and on the right by the Spitzer space telescope. Centaurus A (NGC 5128) is the nearest active galaxy to Earth. Located 13 million light - years away in the southern constellation Centaurus, 'Cen A' appears to be the result of a merger - collision between a large elliptical galaxy (which has a black hole at its center) and a smaller spiral galaxy that veered too close to the larger one, resulting in the cannabalization of the small galaxy. The visible image (left) from the National Science Foundation's Blanco 4 - meter telescope at Cerro Tololo Inter - American Observatory in Chile is dominated by a brigh

Galaxy Centaurus A (NGC 5128) in visible and infrared - Galaxy Centaurus A in visible and infrared - The galaxy NGC 5128 is about 13 million years away - light from Earth. This an elliptical galaxy that cannibalized a small spiral galaxy. The infrared image, on the right, reveals the complex structure of the central dust strip. Images obtained on the left by Cerro Tololo's 4m telescope and on the right by the Spitzer space telescope. Centaurus A (NGC 5128) is the nearest active galaxy to Earth. Located 13 million light - years away in the southern constellation Centaurus, 'Cen A' appears to be the result of a merger - collision between a large elliptical galaxy (which has a black hole at its center) and a smaller spiral galaxy that veered too close to the larger one, resulting in the cannabalization of the small galaxy. The visible image (left) from the National Science Foundation's Blanco 4 - meter telescope at Cerro Tololo Inter - American Observatory in Chile is dominated by a brigh

PIX4612203

Black hole collision in NGC 6240 - Black holes colliding in NGC 6240 - The galaxy NGC 6240, is located about 400 million light years away from Earth in the constellation Ophiuchus. This system consists of two colliding galaxies each with a central black hole; in several millions of years, they will form only one galaxy. A composite X-ray image (red, orange and yellow) and visible from the space telescopes Chandra and Hubble. This image of NGC 6240 contains X - ray data from Chandra (shown in red, orange, and yellow) that has been combined with an optical image from the Hubble Space Telescope. In 2002, the discovery of two merging black holes was announced based on Chandra data in this galaxy. The two black holes are a mere 3,000 light years apart and are seen as the bright point - like sources in the middle of the image. Scientists think these black holes are in such close proximity because they are in the midst of spiraling toward each other - a process that began about 30 million yea

Black hole collision in NGC 6240 - Black holes colliding in NGC 6240 - The galaxy NGC 6240, is located about 400 million light years away from Earth in the constellation Ophiuchus. This system consists of two colliding galaxies each with a central black hole; in several millions of years, they will form only one galaxy. A composite X-ray image (red, orange and yellow) and visible from the space telescopes Chandra and Hubble. This image of NGC 6240 contains X - ray data from Chandra (shown in red, orange, and yellow) that has been combined with an optical image from the Hubble Space Telescope. In 2002, the discovery of two merging black holes was announced based on Chandra data in this galaxy. The two black holes are a mere 3,000 light years apart and are seen as the bright point - like sources in the middle of the image. Scientists think these black holes are in such close proximity because they are in the midst of spiraling toward each other - a process that began about 30 million yea

PIX4612910

«
1
…
814
815
816
…
820
»

Why choose Bridgeman Images

Art. Culture. History.

We partner with the world's leading museums, galleries and artists, so you have access to the highest-quality imagery.

Discover our collection Browse FAQs

Simple. Fast. Reliable.

Our teams can help you find the perfect content and take care of all of the copyright and licensing requirements.

Contact us

Discover millions of images and videos for your creative projects.

Start your search

© Copyright 2024 Bridgeman Art Library Limited. Registered in England and Wales as company number 01056394.