'New Years' images et/ou videos résultats

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

Votre Sélection en cours

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"MME4736160","item_category2":"no_copyright","item_category3":"standard","item_category4":"marcello_mencarini","item_category5":"not_balown","item_list_name":"search_results","item_name":"savanna_knoop_a_k_a_j_t_leroy_during_a_reading_rome_june_3_2000_photo","item_variant":"undefined"},{"item_id":"MME4736174","item_category2":"no_copyright","item_category3":"standard","item_category4":"marcello_mencarini","item_category5":"not_balown","item_list_name":"search_results","item_name":"rome_june_3_2000_savanna_knoop_a_k_a_j_t_leroy_during_a_reading_knoop_pretends_to_be_writer_j_t_lero","item_variant":"undefined"},{"item_id":"MME4736097","item_category2":"no_copyright","item_category3":"standard","item_category4":"marcello_mencarini","item_category5":"not_balown","item_list_name":"search_results","item_name":"rome_june_3_2000_savanna_knoop_a_k_a_j_t_leroy_knoop_pretends_to_be_writer_j_t_leroy_but_in_2006_the","item_variant":"undefined"},{"item_id":"MME4736139","item_category2":"no_copyright","item_category3":"standard","item_category4":"marcello_mencarini","item_category5":"not_balown","item_list_name":"search_results","item_name":"rome_june_3_2000_savanna_knoop_a_k_a_j_t_leroy_knoop_pretends_to_be_writer_j_t_leroy_but_in_2006_the","item_variant":"undefined"},{"item_id":"MME4736158","item_category2":"no_copyright","item_category3":"standard","item_category4":"marcello_mencarini","item_category5":"not_balown","item_list_name":"search_results","item_name":"rome_june_3_2000_savanna_knoop_a_k_a_j_t_leroy_knoop_pretends_to_be_writer_j_t_leroy_but_in_2006_the","item_variant":"undefined"},{"item_id":"PIX4620256","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_in_the_nebula_omega_m17_part_of_m17_nebula_detail_in_the_nebula_omega_m17_a_region_of_star_fo","item_variant":"undefined"},{"item_id":"ZUM4946652","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"dec_12_1954_laying_the_foundation_stone_for_new_church_of_annunciation_for_nazareth_the_latin_patria","item_variant":"undefined"},{"item_id":"PIX4613594","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_of_the_wheel_of_the_charette_in_the_sculptor_the_cartwheel_galaxy_the_ring_galaxy_of_the_whee","item_variant":"undefined"},{"item_id":"PIX4568831","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"pleiades_open_cluster_the_pleiades_star_cluster_the_pleiades_star_cluster_contains_about_500_stars_f","item_variant":"undefined"},{"item_id":"MME4736182","item_category2":"no_copyright","item_category3":"standard","item_category4":"marcello_mencarini","item_category5":"not_balown","item_list_name":"search_results","item_name":"rome_june_3_2000_savanna_knoop_a_k_a_j_t_leroy_during_a_reading_knoop_pretends_to_be_writer_j_t_lero","item_variant":"undefined"},{"item_id":"MME4736109","item_category2":"no_copyright","item_category3":"standard","item_category4":"marcello_mencarini","item_category5":"not_balown","item_list_name":"search_results","item_name":"rome_june_3_2000_savanna_knoop_a_k_a_j_t_leroy_knoop_pretends_to_be_writer_j_t_leroy_but_in_2006_the","item_variant":"undefined"},{"item_id":"ZUM4864906","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jul_20_1953_coloured_photos_on_stone_professor_kleinschmidt_teacher_at_the_highschool_for_art_in_ber","item_variant":"undefined"},{"item_id":"PIX4608507","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"exoplanete_ross_128_b_ross_128_b_is_an_extrasolar_planet_probably_of_an_earth_type_located_only_11_l","item_variant":"undefined"},{"item_id":"PIX4663009","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"zuniceratops_an_adult_zuniceratops_who_lived_90_million_years_ago_walks_through_a_cretacious_forest_","item_variant":"undefined"},{"item_id":"PIX4621537","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"young_stars_in_rho_ophiuchi_young_stars_in_rho_ophiuchi_image_of_the_central_part_of_rho_ophiuchi_ob","item_variant":"undefined"},{"item_id":"ZUM4913337","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"feb_02_1954_robert_donat_returns_to_the_screen_robert_donat_who_was_last_seen_in_films_as_william_fr","item_variant":"undefined"},{"item_id":"ZUM4836232","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"apr_04_1953_geiselgasteig_takes_colour_3_dimensional_pictures_europe_s_most_up_to_date_and_most_expe","item_variant":"undefined"},{"item_id":"ZUM4838785","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"apr_23_1953_north_korean_children_in_eastern_germany_as_many_iron_curtain_countries_the_german_democ","item_variant":"undefined"},{"item_id":"ZUM4867718","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"aug_08_1953_film_star_ballerina_to_dance_in_london_colette_marchand_the_french_ballerina_who_became_","item_variant":"undefined"},{"item_id":"ZUM4913320","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"feb_02_1954_robert_donat_returns_to_the_screeen_a_welcome_kiss_for_the_parson_robert_donat_who_was_l","item_variant":"undefined"},{"item_id":"PIX4610751","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_ngc_3521_in_the_lion_spiral_galaxy_ngc_3521_in_leo_ngc_3521_is_a_spiral_galaxy_located","item_variant":"undefined"},{"item_id":"ZUM4888533","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"oct_10_1953_africa_s_women_march_to_the_polls_acara_capital_of_the_golad_coast_with_an_estimated_pop","item_variant":"undefined"},{"item_id":"ZUM4900374","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"dec_12_1953_at_the_ganges_the_first_white_lady_met_the_greats_jogi_of_india_swami_sivananda_mrs_char","item_variant":"undefined"},{"item_id":"ZUM4857277","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jul_07_1953_lebanon_s_women_go_the_polls_general_elections_all_over_the_country_for_the_second_time_","item_variant":"undefined"},{"item_id":"PIX4612498","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_m83_in_hydra_spiral_galaxy_m83_in_hydra_the_galaxy_m83_ngc_5236_is_located_about_15_mi","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":"PIX4609655","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1097_in_the_furnace_barred_spiral_galaxy_ngc_1097_in_fornax_located_at_a_di","item_variant":"undefined"},{"item_id":"ZUM4914312","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"feb_02_1954_behind_the_iron_curtain_acclimatization_of_sable_since_1949_sable_this_valuable_fur_bear","item_variant":"undefined"},{"item_id":"PIX4619137","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_nebula_ngc_3372_in_carene_eta_carinae_nebula_detail_detail_of_nebula_ngc_3372_in_the_const","item_variant":"undefined"},{"item_id":"PIX4613572","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_of_the_wheel_of_the_charette_in_the_sculptor_the_cartwheel_galaxy_the_ring_galaxy_of_the_whee","item_variant":"undefined"},{"item_id":"PIX4569009","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"open_cluster_trumpler_5_in_unicorn_open_cluster_trumpler_5_in_monoceros_trumpler_5_is_a_cluster_of_s","item_variant":"undefined"},{"item_id":"NTB8931296","item_category2":"no_copyright","item_category3":"standard","item_category4":"aage_storlokken","item_category5":"not_balown","item_list_name":"search_results","item_name":"oslo_19540821_broadcasting_television_trials_are_lining_towards_the_end_of_the_1954_photo","item_variant":"undefined"},{"item_id":"PIX4590815","item_category2":"no_copyright","item_category3":"standard","item_category4":"jerry_lodriguss","item_category5":"not_balown","item_list_name":"search_results","item_name":"constellations_of_the_great_dog_orion_and_taurus_winter_constellations_on_the_left_the_constellation","item_variant":"undefined"},{"item_id":"PIX4611053","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_ngc_4038_4039_in_the_raven_the_antennae_galaxy_in_corvus_the_galaxy_ngc_4038_39","item_variant":"undefined"},{"item_id":"PIX4569073","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"open_cluster_westerlund_1_in_the_altar_open_cluster_westerlund_1_in_ara_the_open_cluster_westerlund_","item_variant":"undefined"},{"item_id":"PIX4617504","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_cluster_ic_1590_in_ngc_281_cassiopee_open_cluster_and_bok_globules_in_ngc_281_view_of_a_detail_","item_variant":"undefined"},{"item_id":"PIX4609403","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_m74_in_pisces_spiral_galaxy_m74_in_pisces_image_of_the_spiral_galaxy_m74_ngc_628_this_","item_variant":"undefined"},{"item_id":"PIX4612940","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_6503_in_the_dragon_spiral_galaxy_ngc_6503_in_draco_the_dwarf_spiral_galaxy_ngc_650","item_variant":"undefined"},{"item_id":"PIX4623200","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_ngc_6302_in_scorpio_planetary_nebula_ngc_6302_in_scorpius_ngc_6302_is_a_planetary_n","item_variant":"undefined"},{"item_id":"PIX4626466","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"remains_of_the_supernova_of_vails_the_vela_supernova_remnant_nearly_12_000_years_ago_a_massive_star_","item_variant":"undefined"},{"item_id":"PIX4609424","item_category2":"no_copyright","item_category3":"standard","item_category4":"adam_block","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m74_in_pisces_spiral_galaxy_m74_in_pisces_image_of_the_spiral_galaxy_m74_ngc_628_this_","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":"MME4736120","item_category2":"no_copyright","item_category3":"standard","item_category4":"marcello_mencarini","item_category5":"not_balown","item_list_name":"search_results","item_name":"rome_june_3_2000_savanna_knoop_a_k_a_j_t_leroy_and_italian_actress_director_asia_argentina_savannah_","item_variant":"undefined"},{"item_id":"ZUM4911978","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"feb_02_1954_a_wedding_begins_her_day_miss_suzanne_cloutier_the_25_year_old_english_canadian_actress_","item_variant":"undefined"},{"item_id":"PIX4638007","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_gamma_ray_sky_the_gamma_ray_sky_map_of_the_whole_sky_seen_in_gamma_rays_by_the_fermi_gamma_ray_s","item_variant":"undefined"},{"item_id":"PIX4620802","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_n44_in_the_large_magellan_cloud_superbubble_lha_120_n_44_in_the_large_magellanic_cloud_this_i","item_variant":"undefined"},{"item_id":"PIX4608051","item_category2":"no_copyright","item_category3":"standard","item_category4":"miller_ron_b_1947","item_category5":"not_balown","item_list_name":"search_results","item_name":"exoplanete_gliese_1214_b_gliese_1214_b_or_gj_1214_b_is_a_super_earth_exoplanet_orbiting_the_star_gli","item_variant":"undefined"},{"item_id":"PIX4618385","item_category2":"no_copyright","item_category3":"standard","item_category4":"tom_davis","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_ngc_2170_in_unicorn_nebula_ngc_2170_in_monoceros_nebula_by_reflexion_located_in_the_constella","item_variant":"undefined"},{"item_id":"PIX4623735","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_mycn18_dans_la_mouche_hst_this_is_an_image_of_mycn18_a_young_planetary_nebula_locat","item_variant":"undefined"},{"item_id":"NTB8912403","item_category2":"no_copyright","item_category3":"standard","item_category4":"aage_storlokken","item_category5":"not_balown","item_list_name":"search_results","item_name":"oslo_19540821_marienlyst_broadcasting_television_trials_are_lining_towards_the_end_of_the_1954_photo","item_variant":"undefined"},{"item_id":"ZUM4947073","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"dec_12_1954_two_women_murdered_at_old_folks_home_a_woman_who_called_herself_lady_menzies_and_her_dau","item_variant":"undefined"},{"item_id":"ZUM4894597","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nov_11_1953_the_wilds_of_darkest_africa_filmed_in_elstree_studios_under_a_galvanised_iron_roof_at_el","item_variant":"undefined"},{"item_id":"PIX4610976","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_3810_in_the_lion_spiral_galaxy_ngc_3810_in_leo_ngc_3810_is_a_spiral_galaxy_located","item_variant":"undefined"},{"item_id":"PIX4621694","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_birth_in_scorpio_stellar_nursery_in_scorpius_rcw_120_is_a_star_forming_region_about_4200_years_","item_variant":"undefined"},{"item_id":"PIX4623639","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_jay_gabany","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_helix_ngc_7293_in_aquarius_planetary_nebula_helix_ngc_7293_this_nebula_is_located_4","item_variant":"undefined"},{"item_id":"PIX4574069","item_category2":"no_copyright","item_category3":"standard","item_category4":"miller_ron_b_1947","item_category5":"not_balown","item_list_name":"search_results","item_name":"exoplanete_gliese_1214_b_gliese_1214_b_or_gj_1214_b_is_a_super_earth_exoplanet_orbiting_the_star_gli","item_variant":"undefined"},{"item_id":"PIX4608046","item_category2":"no_copyright","item_category3":"standard","item_category4":"miller_ron_b_1947","item_category5":"not_balown","item_list_name":"search_results","item_name":"exoplanete_gliese_1214_b_gliese_1214_b_or_gj_1214_b_is_a_super_earth_exoplanet_orbiting_the_star_gli","item_variant":"undefined"},{"item_id":"PIX4612595","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_arp_240_interacting_galaxies_arp_240_the_galaxy_arp_240_is_located_about_300_mi","item_variant":"undefined"},{"item_id":"PIX4573892","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"exoplanete_gj_1214_b_exoplanet_gj_1214_b_illustration_showing_the_transit_of_the_extrasolar_planet_g","item_variant":"undefined"},{"item_id":"PIX4565683","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_cluster_sdss_j1004_4112_galaxy_cluster_sdss_j1004_4112_view_of_the_cluster_of_sdss_j1004_4112","item_variant":"undefined"}]}}

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

Recherche avancée Astuces de recherche

Images de 'New Years' médias trouvés, 29,634

«
1
…
5
6
7
…
494
»

Savanna Knoop a.k.a. J.T. Leroy during a reading., Rome, June 3, 2000 (photo)

Savanna Knoop a.k.a. J.T. Leroy during a reading., Rome, June 3, 2000 (photo)

Marcello Mencarini

MME4736160

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy during a reading. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy, durante un reading. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, present

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy during a reading. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy, durante un reading. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, present

Marcello Mencarini

MME4736174

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, presentati come autobiografici -

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, presentati come autobiografici -

Marcello Mencarini

MME4736097

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, presentati come autobiografici -

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, presentati come autobiografici -

Marcello Mencarini

MME4736139

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, presentati come autobiografici -

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, presentati come autobiografici -

Marcello Mencarini

MME4736158

Detail in the nebula Omega (M17) - Part of M17 nebula - Detail in the nebula Omega (M17), a region of star formation. Image obtained from the 3.5-metre NTT telescope of the European Observatory of La Silla in Chile. The Omega Nebula (M17) is one of the youngest and most massive star - forming regions in the Milky Way. Active star - birth started a few million years ago and continues through today. The brightly shining gas shown in this picture is just a blister erupting from the side of a much larger dark cloud of molecular gas. The dust that is so prominent in this picture comes from the remains of massive hot stars that have ended their brief lives and ejected material back into space, as well as the cosmic detritus from which future suns form. Three - colour composite image of the Omega Nebula (Messier 17), based on images obtained with the EMMI instrument on the ESO 3.58 - metre New Technology Telescope at the La Silla Observatory. North is down and East is to the right in the imag

Detail in the nebula Omega (M17) - Part of M17 nebula - Detail in the nebula Omega (M17), a region of star formation. Image obtained from the 3.5-metre NTT telescope of the European Observatory of La Silla in Chile. The Omega Nebula (M17) is one of the youngest and most massive star - forming regions in the Milky Way. Active star - birth started a few million years ago and continues through today. The brightly shining gas shown in this picture is just a blister erupting from the side of a much larger dark cloud of molecular gas. The dust that is so prominent in this picture comes from the remains of massive hot stars that have ended their brief lives and ejected material back into space, as well as the cosmic detritus from which future suns form. Three - colour composite image of the Omega Nebula (Messier 17), based on images obtained with the EMMI instrument on the ESO 3.58 - metre New Technology Telescope at the La Silla Observatory. North is down and East is to the right in the imag

PIX4620256

Dec. 12, 1954 - Laying the Foundation Stone for new” Church of Annunciation for Nazareth”... The Latin Patriarch Monsignor Alberto Gori recently visited Israel from the Old City of Jerusalem - for the purpose of laying the Foundation Stone of the Fourth Church of the Annunciation at Nazareth - also to mark the end of the” Marian Year”. The new church will be the largest in the Middle East measuring about 260 ft by 260 ft and about 210 ft in height. The church was designed by the Vatican Architect Signor Barluzzi - will take about three years to complete and will cost about Four Million Dollars - will be built in local stone - with Italian marble for the interior. Keystone Photo Shows: Dr. P. Colbi, representative of the Ministry of Religion of the State of Israel reads the greetings of the Government of Israel. To right (With Mithra) the Latin Patriarch Mrs. A. Gori, the third from left Msgr. Antonio Vergani, Patriarch Vicar of Galileo

Dec. 12, 1954 - Laying the Foundation Stone for new” Church of Annunciation for Nazareth”... The Latin Patriarch Monsignor Alberto Gori recently visited Israel from the Old City of Jerusalem - for the purpose of laying the Foundation Stone of the Fourth Church of the Annunciation at Nazareth - also to mark the end of the” Marian Year”. The new church will be the largest in the Middle East measuring about 260 ft by 260 ft and about 210 ft in height. The church was designed by the Vatican Architect Signor Barluzzi - will take about three years to complete and will cost about Four Million Dollars - will be built in local stone - with Italian marble for the interior. Keystone Photo Shows: Dr. P. Colbi, representative of the Ministry of Religion of the State of Israel reads the greetings of the Government of Israel. To right (With Mithra) the Latin Patriarch Mrs. A. Gori, the third from left Msgr. Antonio Vergani, Patriarch Vicar of Galileo

ZUM4946652

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from the Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars. This particular form is the result of a collision, probably with one of the two galaxies on the right. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two objects to the right of the ring - - that careened through the core of the host

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from the Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars. This particular form is the result of a collision, probably with one of the two galaxies on the right. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two objects to the right of the ring - - that careened through the core of the host

PIX4613594

Pleiades open cluster - The Pleiades star cluster - The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located about 400 light years from Earth, in the constellation Taurus. This field corresponds to that of a small telescope or a pair of binoculars. Object number 45 in Messier's catalog is the Pleiades, also know as the Seven Sisters for the seven stars that can be easily seen with excellent eyesight.The Pleiades is a relatively nearby open cluster, which according to new data from the Hipparcos satellite is located at a distance of 370 light years. The cluster is surrounded by blue nebulosity illuminated by the light reflected from the nearby stars. This skyview is corresponding to binoculars and small telescopes

Pleiades open cluster - The Pleiades star cluster - The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located about 400 light years from Earth, in the constellation Taurus. This field corresponds to that of a small telescope or a pair of binoculars. Object number 45 in Messier's catalog is the Pleiades, also know as the Seven Sisters for the seven stars that can be easily seen with excellent eyesight.The Pleiades is a relatively nearby open cluster, which according to new data from the Hipparcos satellite is located at a distance of 370 light years. The cluster is surrounded by blue nebulosity illuminated by the light reflected from the nearby stars. This skyview is corresponding to binoculars and small telescopes

PIX4568831

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy during a reading. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy, durante un reading. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, present

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy during a reading. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy, durante un reading. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, present

Marcello Mencarini

MME4736182

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, presentati come autobiografici -

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy. Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times reveals that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical/Roma, 3 June 2000. Savannah Knoop, a.k.a. lo scrittore J.T. Leroy. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parrucca bionda e grandi occhiali da sole, per creare un personaggio problematico e rendere pi credibili quei racconti di prostituzione e maltrattamenti, presentati come autobiografici -

Marcello Mencarini

MME4736109

Jul. 20, 1953 - Coloured Photos on Stone.: Professor Kleinschmidt, teacher at the highschool for art in Berlin, brought out an invention which took him and his co-operators 5 years and which is quite a senstaion on the field of photo- and publicity tecnhnics. Huge photos on stone! The photos do not react to heat, cold, snow or rain. They are made the following way: eternit-plate sensitive to light a size 120 to 150 centimeters are exposed to the light in the dark room as with normal enlarging. The stone photos may be produced in black and white or in colours. It is quite obvious that this process bears quite new possibilities for publicity

Jul. 20, 1953 - Coloured Photos on Stone.: Professor Kleinschmidt, teacher at the highschool for art in Berlin, brought out an invention which took him and his co-operators 5 years and which is quite a senstaion on the field of photo- and publicity tecnhnics. Huge photos on stone! The photos do not react to heat, cold, snow or rain. They are made the following way: eternit-plate sensitive to light a size 120 to 150 centimeters are exposed to the light in the dark room as with normal enlarging. The stone photos may be produced in black and white or in colours. It is quite obvious that this process bears quite new possibilities for publicity

ZUM4864906

Exoplanete Ross 128 b: Ross 128 b is an extrasolar planet probably of an Earth type, located only 11 light years from Earth in the constellation of the Virgin. Planet Ross 128 b, with its red dwarf parent star in the background. This planet, which lies only 11 light-years from Earth, was found by a team using Eso's unique planet-hunting HARPS instrument. The new world is now the second-closest temperate planet to be detected after Proxima b. It is also the closest planet to be discovered orbiting an inactive red dwarf star, which may increase the likelihood that this planet could potentially sustain life. Ross 128 b will be a prime target for Eso's Extremely Large Telescope, which will be able to search for biomarkers in the planet's atmosphere

Exoplanete Ross 128 b: Ross 128 b is an extrasolar planet probably of an Earth type, located only 11 light years from Earth in the constellation of the Virgin. Planet Ross 128 b, with its red dwarf parent star in the background. This planet, which lies only 11 light-years from Earth, was found by a team using Eso's unique planet-hunting HARPS instrument. The new world is now the second-closest temperate planet to be detected after Proxima b. It is also the closest planet to be discovered orbiting an inactive red dwarf star, which may increase the likelihood that this planet could potentially sustain life. Ross 128 b will be a prime target for Eso's Extremely Large Telescope, which will be able to search for biomarkers in the planet's atmosphere

PIX4608507

Zuniceratops - An adult Zuniceratops who lived 90 million years ago walks through a cretacious forest. The Zuniceratops was 90 centimetres high at the withers and weighed 110 kilograms. A 10 football long, 250 pound Zuniceratops wonders a Cretaceous forest 90 million years ago in what is today New Mexico. Like the better known and larger Triceratops, Zuniceratops was a Ceratopsid, a family of four-legged plant-eating dinosaurs characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that they may have served a purpose other than protecting against a brute force attack. One possibility is that the frills were employed as visual displays in order to intimidate rivals and attract the opposite sex

Zuniceratops - An adult Zuniceratops who lived 90 million years ago walks through a cretacious forest. The Zuniceratops was 90 centimetres high at the withers and weighed 110 kilograms. A 10 football long, 250 pound Zuniceratops wonders a Cretaceous forest 90 million years ago in what is today New Mexico. Like the better known and larger Triceratops, Zuniceratops was a Ceratopsid, a family of four-legged plant-eating dinosaurs characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that they may have served a purpose other than protecting against a brute force attack. One possibility is that the frills were employed as visual displays in order to intimidate rivals and attract the opposite sex

Walter B Myers

PIX4663009

Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new

Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new

PIX4621537

Feb. 02, 1954 - Robert Donat Returns to the screen. Robert Donat who was last seen in films as William Friese-Greene” The Magic Box” nearly three years ago - now takes on the role of a country parson - vicar of a South takes on the role of a country parson - vicar of a South Yorkshire Parish in the new film” Leas ~ of Life” which is being made at Ealing Studios. His wife is being played by Kay Walsh - and technical advice is being given by Canon Edward Carpenter of Westminster Abbey - who took part in the procession of regalia Coronation

Feb. 02, 1954 - Robert Donat Returns to the screen. Robert Donat who was last seen in films as William Friese-Greene” The Magic Box” nearly three years ago - now takes on the role of a country parson - vicar of a South takes on the role of a country parson - vicar of a South Yorkshire Parish in the new film” Leas ~ of Life” which is being made at Ealing Studios. His wife is being played by Kay Walsh - and technical advice is being given by Canon Edward Carpenter of Westminster Abbey - who took part in the procession of regalia Coronation

ZUM4913337

Apr. 04, 1953 - Geiselgasteig takes colour 3 dimensional pictures. Europe's most up to date and most expensive camera is presently to be seen on the Geiselgasteig film grounds. The new” stereo camera” a Zeiss Icon, was developed by scientist in more than 20 years of research. Kurt Gewissen, the experienced man from Hamburg will practise a colour 3 dimensional film, in order to take advantage of this camera. Margot Mielscher and Wastl Witt play the dominate role in connection with the famous October Festival. Out Picture shows: Left: Kurt Gewisson working on the plastic Zeiss Nikon camera. Right: A close up of one of the most important details of the camera, the adjustable sectors.

Apr. 04, 1953 - Geiselgasteig takes colour 3 dimensional pictures. Europe's most up to date and most expensive camera is presently to be seen on the Geiselgasteig film grounds. The new” stereo camera” a Zeiss Icon, was developed by scientist in more than 20 years of research. Kurt Gewissen, the experienced man from Hamburg will practise a colour 3 dimensional film, in order to take advantage of this camera. Margot Mielscher and Wastl Witt play the dominate role in connection with the famous October Festival. Out Picture shows: Left: Kurt Gewisson working on the plastic Zeiss Nikon camera. Right: A close up of one of the most important details of the camera, the adjustable sectors.

ZUM4836232

Apr. 23, 1953 - North Korean children in Eastern Germany: As many iron Curtain countries, the” German Democratic Republic” (Germany's Soviet occupied territory) has welcomed North Korean children, ranging in age from 6 to 16 years. These children have lost their parents during the Korean campaign, and it happened in the first days of March when the children arrived in Mortizburg, near Dresden, East Germany. This picture has been taken from the” New Berliner Illustrierte”, a government sponsored weekly in East Germany. The East German People's Police presented the children uniforms and air rifles of many of them according to the paper have already passed proficiency in “Successful Partnership” and other military or para military training, when they were in their native country.

Apr. 23, 1953 - North Korean children in Eastern Germany: As many iron Curtain countries, the” German Democratic Republic” (Germany's Soviet occupied territory) has welcomed North Korean children, ranging in age from 6 to 16 years. These children have lost their parents during the Korean campaign, and it happened in the first days of March when the children arrived in Mortizburg, near Dresden, East Germany. This picture has been taken from the” New Berliner Illustrierte”, a government sponsored weekly in East Germany. The East German People's Police presented the children uniforms and air rifles of many of them according to the paper have already passed proficiency in “Successful Partnership” and other military or para military training, when they were in their native country.

ZUM4838785

Aug. 08, 1953 - Film Star Ballerina To Dance In London: Colette Marchand, the French Ballerina who became an International film star in” Moulin Rouge”, is to dabbed in London this month at twn times the salary she craned here as a small name in Roland Petite's Company four years ago. That is the price M. Petite has had to pay for the screen fame of Colette, who has been hailed in New York as” Les Legs” and her own Paris as France's favorite ballet dancer. In the latest Petite ballet,” Cine-Bijou”, Roland Petite and Colette Marchand as a Parisian worker and a little typist sitting side by in their suburban cinema watching an American gangster film

Aug. 08, 1953 - Film Star Ballerina To Dance In London: Colette Marchand, the French Ballerina who became an International film star in” Moulin Rouge”, is to dabbed in London this month at twn times the salary she craned here as a small name in Roland Petite's Company four years ago. That is the price M. Petite has had to pay for the screen fame of Colette, who has been hailed in New York as” Les Legs” and her own Paris as France's favorite ballet dancer. In the latest Petite ballet,” Cine-Bijou”, Roland Petite and Colette Marchand as a Parisian worker and a little typist sitting side by in their suburban cinema watching an American gangster film

ZUM4867718

Feb. 02, 1954 - Robert Donat Returns to the screeen. A welcome kiss for the Parson: Robert Donat who was lasts seen in films as William Friese-Greene nearly three years ago - now takes on the role of a country parson - vicar of a South takes on the role of a country pason - vicar of a South Yorkshire Parish in the new film” Leas ~ of Life” which is being made at Ealing Studios. His wife is played by Kay Walsh - and technical advice on wearing the clerical clothes come from Canon Edward Carpenter of Westminster Abbey - who take part in the procession of regalia at the Coronation

Feb. 02, 1954 - Robert Donat Returns to the screeen. A welcome kiss for the Parson: Robert Donat who was lasts seen in films as William Friese-Greene nearly three years ago - now takes on the role of a country parson - vicar of a South takes on the role of a country pason - vicar of a South Yorkshire Parish in the new film” Leas ~ of Life” which is being made at Ealing Studios. His wife is played by Kay Walsh - and technical advice on wearing the clerical clothes come from Canon Edward Carpenter of Westminster Abbey - who take part in the procession of regalia at the Coronation

ZUM4913320

Spiral Galaxy NGC 3521 in the Lion - Spiral galaxy NGC 3521 in Leo - NGC 3521 is a spiral galaxy located about 35 million years ago - light from Earth. NGC 3521 is located about 35 million light years in the distance towards the northern constellation of Leo. This new deep image depicts multiple debris shells that evidence previous mergers with one or more satellite galaxies. NGC 3521 is an example of a flocculent galaxy. Galaxies are assigned this classification because they exhibit short, fragmented and somewhat disorganized spiral arms. Almost one third of all spiral galaxies display this characteristic to some extent. The cause of this condition remains elusive but recent observations have revealed that this galaxy has experienced a merger with one or more satellite galaxies

Spiral Galaxy NGC 3521 in the Lion - Spiral galaxy NGC 3521 in Leo - NGC 3521 is a spiral galaxy located about 35 million years ago - light from Earth. NGC 3521 is located about 35 million light years in the distance towards the northern constellation of Leo. This new deep image depicts multiple debris shells that evidence previous mergers with one or more satellite galaxies. NGC 3521 is an example of a flocculent galaxy. Galaxies are assigned this classification because they exhibit short, fragmented and somewhat disorganized spiral arms. Almost one third of all spiral galaxies display this characteristic to some extent. The cause of this condition remains elusive but recent observations have revealed that this galaxy has experienced a merger with one or more satellite galaxies

R. Jay GaBany

PIX4610751

Oct. 10, 1953 - Africa's women march to the Polls: Acara, capital of the Golad Coast with an estimated population of 150,000. recently elected a new Municipal Council. Women were predominent at the 23 polling booths from which the returns showed the city was to be governed by an All-African council for the next three years. It was another example of how the Gold Coast, with the cooperation of the British Government, is moving toward self-government in a democratic manner

Oct. 10, 1953 - Africa's women march to the Polls: Acara, capital of the Golad Coast with an estimated population of 150,000. recently elected a new Municipal Council. Women were predominent at the 23 polling booths from which the returns showed the city was to be governed by an All-African council for the next three years. It was another example of how the Gold Coast, with the cooperation of the British Government, is moving toward self-government in a democratic manner

ZUM4888533

Dec. 12, 1953 - At the Ganges... the first white lady met the greats Jogi of India, Swami Sivananda. Mrs. Charlotte Walinski Heller from Nuremberg is a good mediating woman and already since many months she has a spiritual contact with Sivananadsa who had been unknown to her and she had been able to accept the far spiritual religious injunctions coming from the interpretation well known Jogi. By his invitation Mrs. Walinski started on Nov 30th to the India were she had been welcomed by the great Jogi by the words “my mind is your mind and your Ming is my mind”. On strip through India and later through all the world Mrs. Walinski should be prepared for her further tasks. Father Walinski and his sons raced the Christians and New Years of the mother

Dec. 12, 1953 - At the Ganges... the first white lady met the greats Jogi of India, Swami Sivananda. Mrs. Charlotte Walinski Heller from Nuremberg is a good mediating woman and already since many months she has a spiritual contact with Sivananadsa who had been unknown to her and she had been able to accept the far spiritual religious injunctions coming from the interpretation well known Jogi. By his invitation Mrs. Walinski started on Nov 30th to the India were she had been welcomed by the great Jogi by the words “my mind is your mind and your Ming is my mind”. On strip through India and later through all the world Mrs. Walinski should be prepared for her further tasks. Father Walinski and his sons raced the Christians and New Years of the mother

ZUM4900374

Jul 07, 1953 - Lebanon's women go the polls. General elections all over the country: For the second time since the foundation of the Republic of Lebanon, the indigenous population elects its legal diet. And it happened for the first time that women were given the privilege to vote. The elections were necessary because three ministers had resigned, within a three years period. Camille Chamoun, the” new strong man of the Lebanon” is said to be much like man and politician. When he dissolved the parliament, he declared the war to corruption and pseudo Parliamentarism.

Jul 07, 1953 - Lebanon's women go the polls. General elections all over the country: For the second time since the foundation of the Republic of Lebanon, the indigenous population elects its legal diet. And it happened for the first time that women were given the privilege to vote. The elections were necessary because three ministers had resigned, within a three years period. Camille Chamoun, the” new strong man of the Lebanon” is said to be much like man and politician. When he dissolved the parliament, he declared the war to corruption and pseudo Parliamentarism.

ZUM4857277

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million light years away from Earth in the constellation Hydra. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained in 2006 and 2007 in several combined long poses, with a large amateur instrument, a 50 cm telescope. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. The image was taken through a remote controlled 20 inch Ritchey - Chretien telescope using an eleven mega - pixel camera. Fourteen hour exposure between May and June of 2006 with additional exposures taken in April 2007 from over seven thousand feet above sea level in the mountains of south central New Mexico

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million light years away from Earth in the constellation Hydra. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained in 2006 and 2007 in several combined long poses, with a large amateur instrument, a 50 cm telescope. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. The image was taken through a remote controlled 20 inch Ritchey - Chretien telescope using an eleven mega - pixel camera. Fourteen hour exposure between May and June of 2006 with additional exposures taken in April 2007 from over seven thousand feet above sea level in the mountains of south central New Mexico

R. Jay GaBany

PIX4612498

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

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope provides us with a spectacular image of the bright star - forming ring that surrounds the heart of the barred spiral galaxy NGC 1097. In this image, the larger - scale structure of the galaxy is barely visible: its comparatively dim spiral arms, which surround its heart in a loose embrace, reach out beyond the edges of this frame. This face - on galaxy, lying 45 million light - years away from Earth in the southern constellation of Fornax (The Furnace), is particularly attractive for astronomers. NGC 1097 is a Seyfert galaxy. Lurking at the very centre of the galaxy, a supermassive black hole 100 million times the mass of our Sun is gr

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope provides us with a spectacular image of the bright star - forming ring that surrounds the heart of the barred spiral galaxy NGC 1097. In this image, the larger - scale structure of the galaxy is barely visible: its comparatively dim spiral arms, which surround its heart in a loose embrace, reach out beyond the edges of this frame. This face - on galaxy, lying 45 million light - years away from Earth in the southern constellation of Fornax (The Furnace), is particularly attractive for astronomers. NGC 1097 is a Seyfert galaxy. Lurking at the very centre of the galaxy, a supermassive black hole 100 million times the mass of our Sun is gr

PIX4609655

Feb. 02, 1954 - Behind the iron Curtain acclimatization of sable; Since 1949, sable, this valuable fur-bearing animal, has been systematically introduced on a large scale into all suitable hunting grounds in the far eastern taiga of soviet Russia. As an experiment the animals were brought to paled in which they has never vied before. chesessavtion carried out bu scientists for four years has led them to the conclusion that sable are successful acclimatizing and multiplying. valuable fur is obtained from those reared in the far east and in the forests of the Verkhne-bureisky, selemdzhisky, Badhalsky and dusse slinsky mountain ranges. Many more sable are being introduced into these area by plane - lorries - on horseback and even - by redder drawn carts

Feb. 02, 1954 - Behind the iron Curtain acclimatization of sable; Since 1949, sable, this valuable fur-bearing animal, has been systematically introduced on a large scale into all suitable hunting grounds in the far eastern taiga of soviet Russia. As an experiment the animals were brought to paled in which they has never vied before. chesessavtion carried out bu scientists for four years has led them to the conclusion that sable are successful acclimatizing and multiplying. valuable fur is obtained from those reared in the far east and in the forests of the Verkhne-bureisky, selemdzhisky, Badhalsky and dusse slinsky mountain ranges. Many more sable are being introduced into these area by plane - lorries - on horseback and even - by redder drawn carts

ZUM4914312

Detail of nebula NGC 3372 in Carene - Eta Carinae nebula detail - Detail of nebula NGC 3372 in the constellation Carene. Within the dark structures visible in this image, stars will be born. Image obtained by the Hubble Space Telescope in 2005 and 2010. These one - light - year - tall pillars of cold hydrogen and dust, imaged by the Hubble Space Telescope, are located in the Carina Nebula. Violent stellar winds and powerful radiation from massive stars are sculpting the surrounding nebula. Inside the dense structures, new stars may be born. This image of dust pillars in the Carina Nebula is a composite of 2005 observations taken of the region in hydrogen light (light emitted by hydrogen atoms) along with 2010 observations taken in oxygen light (light emitted by oxygen atoms), both times with Hubble's Advanced Camera for Surveys. The immense Carina Nebula is an estimated 7,500 light - years away in the southern constellation Carina

Detail of nebula NGC 3372 in Carene - Eta Carinae nebula detail - Detail of nebula NGC 3372 in the constellation Carene. Within the dark structures visible in this image, stars will be born. Image obtained by the Hubble Space Telescope in 2005 and 2010. These one - light - year - tall pillars of cold hydrogen and dust, imaged by the Hubble Space Telescope, are located in the Carina Nebula. Violent stellar winds and powerful radiation from massive stars are sculpting the surrounding nebula. Inside the dense structures, new stars may be born. This image of dust pillars in the Carina Nebula is a composite of 2005 observations taken of the region in hydrogen light (light emitted by hydrogen atoms) along with 2010 observations taken in oxygen light (light emitted by oxygen atoms), both times with Hubble's Advanced Camera for Surveys. The immense Carina Nebula is an estimated 7,500 light - years away in the southern constellation Carina

PIX4619137

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars (detail at the top left). This particular form is the result of a collision, probably with one of the two galaxies on the right. Bottom left, close-up on the nucleus of the galaxy. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two object

Galaxy of the Wheel of the Charette in the Sculptor - The Cartwheel Galaxy - The ring galaxy of the Wheel of the Charette is about 500 million years away - light from Earth. It is surrounded by a ring of 150,000 years - light of diameter composed of young and very bright stars (detail at the top left). This particular form is the result of a collision, probably with one of the two galaxies on the right. Bottom left, close-up on the nucleus of the galaxy. Image obtained by the Hubble Space Telescope in October 1994. A rare and spectacular head - on collision between two galaxies appears in this NASA Hubble Space Telescope true - color image of the Cartwheel Galaxy, located 500 million light - years away in the constellation Sculptor. The details of star birth resolved by Hubble provide an opportunity to study how extremely massive stars are born in large fragmented gas clouds. The striking ring - like feature is a direct result of a smaller intruder galaxy - - possibly one of two object

PIX4613572

Open cluster Trumpler 5 in Unicorn - Open cluster Trumpler 5 in Monoceros - Trumpler 5 is a cluster of stars aged 125 million years. Image obtained by Siding Spring's 3.9m telescope As they age, open clusters of stars begin to lose their identity. This is partly because the brighter members tend to self - destruct as supernovae, and, though the group members share a common motion through space, they are only loosely bound. Thus stars drift away from the cluster in a process that accelerates with time. However, some clusters are big enough to retain their identity much longer than usual, and Trumpler 5 is one such. Its age is estimated to be 125 million years, and it must have been a spectacular sight in its youth. It seems to be at the edge of the Monoceros molecular cloud, where star formation is continuing new generations of young clusters

Open cluster Trumpler 5 in Unicorn - Open cluster Trumpler 5 in Monoceros - Trumpler 5 is a cluster of stars aged 125 million years. Image obtained by Siding Spring's 3.9m telescope As they age, open clusters of stars begin to lose their identity. This is partly because the brighter members tend to self - destruct as supernovae, and, though the group members share a common motion through space, they are only loosely bound. Thus stars drift away from the cluster in a process that accelerates with time. However, some clusters are big enough to retain their identity much longer than usual, and Trumpler 5 is one such. Its age is estimated to be 125 million years, and it must have been a spectacular sight in its youth. It seems to be at the edge of the Monoceros molecular cloud, where star formation is continuing new generations of young clusters

PIX4569009

Oslo 19540821. Broadcasting television trials are lining towards the end of the …, 1954 (photo)

Oslo 19540821. Broadcasting television trials are lining towards the end of the …, 1954 (photo)

Aage Storløkken

NTB8931296

Constellations of the Great Dog, Orion and Taurus - Winter constellations. On the left the constellation of the Great Dog with the star Sirius, in the center the constellation Orion, on the right the constellation of the Taurus with the cluster of the Hyades and the cluster of the Pleiades. Image obtained on November 3, 2005 in New Jersey - USA. The constellations of Canis Major (the Big Dog), Orion (the Hunter), and Taurus (the Bull) stretch across the winter sky just before the start of dawn in the beginning of November. Sirius, the brightest star in the night sky, dominates the left side of the frame. Sirius is the alpha star in the constellation of Canis Major and is located only 9 light years away. Orion, the most distinctive of the winter constellations, is in the middle of the frame. The Hyades and Pleiades (the 7 Sisters), two beautiful open clusters in Taurus, are on the right side of the image

Constellations of the Great Dog, Orion and Taurus - Winter constellations. On the left the constellation of the Great Dog with the star Sirius, in the center the constellation Orion, on the right the constellation of the Taurus with the cluster of the Hyades and the cluster of the Pleiades. Image obtained on November 3, 2005 in New Jersey - USA. The constellations of Canis Major (the Big Dog), Orion (the Hunter), and Taurus (the Bull) stretch across the winter sky just before the start of dawn in the beginning of November. Sirius, the brightest star in the night sky, dominates the left side of the frame. Sirius is the alpha star in the constellation of Canis Major and is located only 9 light years away. Orion, the most distinctive of the winter constellations, is in the middle of the frame. The Hyades and Pleiades (the 7 Sisters), two beautiful open clusters in Taurus, are on the right side of the image

Jerry Lodriguss

PIX4590815

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - The galaxy NGC 4038 - 39 (antenna galaxy) is located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. These images made by the Hubble space telescope on 20 January 1996 show in detail the nuclei of these two twin galaxies (right) as well as clusters of blue stars, consisting of young and massive stars (left). The scale bar at the top of each image represents 1500 years - light. These four close - up views are taken from a head - on collision between two spiral galaxies, called the Antennae galaxies, seen at image center. The scale bar at the top of each image is 1,500 light - years across. Left: the collision triggers the birth of new stars in brilliant blue star clusters, the brightest of which contains roughly a million stars. The star clusters are blue because they are very young, the youngest b

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - The galaxy NGC 4038 - 39 (antenna galaxy) is located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. These images made by the Hubble space telescope on 20 January 1996 show in detail the nuclei of these two twin galaxies (right) as well as clusters of blue stars, consisting of young and massive stars (left). The scale bar at the top of each image represents 1500 years - light. These four close - up views are taken from a head - on collision between two spiral galaxies, called the Antennae galaxies, seen at image center. The scale bar at the top of each image is 1,500 light - years across. Left: the collision triggers the birth of new stars in brilliant blue star clusters, the brightest of which contains roughly a million stars. The star clusters are blue because they are very young, the youngest b

PIX4611053

Open cluster Westerlund 1 in the Altar - Open cluster Westerlund 1 in Ara - The open cluster Westerlund 1 is located about 16,000 years - light in the southern constellation of the Altar. It contains hundreds of very young massive stars as well as the supergiant red star W26. Image obtained by the VST telescope in Chile. This exceptionally bright cluster lies about 16 000 light - years from Earth in the southern constellation of Ara (The Altar). It contains hundreds of very massive and brilliant stars, all of which are just a few million years old - - babies by stellar standards. But our view of this cluster is hampered by gas and dust that prevents most of the visible light from the cluster's stars from getting to Earth. Around one of the stars - - known as W26, a red supergiant and possibly the biggest star known - - astronomers have discovered clouds of glowing hydrogen gas, shown as green features in this new image. Such glowing clouds around massive stars are very rare, and are ev

Open cluster Westerlund 1 in the Altar - Open cluster Westerlund 1 in Ara - The open cluster Westerlund 1 is located about 16,000 years - light in the southern constellation of the Altar. It contains hundreds of very young massive stars as well as the supergiant red star W26. Image obtained by the VST telescope in Chile. This exceptionally bright cluster lies about 16 000 light - years from Earth in the southern constellation of Ara (The Altar). It contains hundreds of very massive and brilliant stars, all of which are just a few million years old - - babies by stellar standards. But our view of this cluster is hampered by gas and dust that prevents most of the visible light from the cluster's stars from getting to Earth. Around one of the stars - - known as W26, a red supergiant and possibly the biggest star known - - astronomers have discovered clouds of glowing hydrogen gas, shown as green features in this new image. Such glowing clouds around massive stars are very rare, and are ev

PIX4569073

Star cluster IC 1590 in NGC 281 (Cassiopee) - Open cluster and Bok globules in NGC 281 - View of a detail in the center of the nebula NGC 281 in Cassiopee. The brightest stars of the open cluster IC 1590 are visible, accompanied by Bok's blood cells, dark interstellar clouds consisting of gas and dust that absorb light. Image obtained by the Hubble Space Telescope (HST). Astronomers have used the NASA/ESA Hubble Space Telescope to study the young open star cluster IC 1590, which is found within the star formation region NGC 281 - - nicknamed the Pacman Nebula due to its resemblance to the famous arcade game character. This image only shows the central part of the nebula, where the brightest stars at the core of the cluster are found, with part of the Pacman's hungry mouth visible as the dark region below. But Pacman isn't gobbling up these stars. Instead, the nebula's gas and dust are being used as raw ingredients to make new stars. However, the stars in IC 1590 are still plotting thei

Star cluster IC 1590 in NGC 281 (Cassiopee) - Open cluster and Bok globules in NGC 281 - View of a detail in the center of the nebula NGC 281 in Cassiopee. The brightest stars of the open cluster IC 1590 are visible, accompanied by Bok's blood cells, dark interstellar clouds consisting of gas and dust that absorb light. Image obtained by the Hubble Space Telescope (HST). Astronomers have used the NASA/ESA Hubble Space Telescope to study the young open star cluster IC 1590, which is found within the star formation region NGC 281 - - nicknamed the Pacman Nebula due to its resemblance to the famous arcade game character. This image only shows the central part of the nebula, where the brightest stars at the core of the cluster are found, with part of the Pacman's hungry mouth visible as the dark region below. But Pacman isn't gobbling up these stars. Instead, the nebula's gas and dust are being used as raw ingredients to make new stars. However, the stars in IC 1590 are still plotting thei

PIX4617504

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a

R. Jay GaBany

PIX4609403

Spiral galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The dwarf spiral galaxy NGC 6503 is located about 17 million years ago - light from Earth. It spans 30,000 light years and shows many star-forming regions. Image obtained by the Hubble Space Telescope. Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside. This new image from Hubble's Advanced Camera for Surveys displays, with particular clarity, the pink - colored puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light - years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy. NGC 6503 lies approximately 17 million light - years away in the co

Spiral galaxy NGC 6503 in the Dragon - Spiral galaxy NGC 6503 in Draco - The dwarf spiral galaxy NGC 6503 is located about 17 million years ago - light from Earth. It spans 30,000 light years and shows many star-forming regions. Image obtained by the Hubble Space Telescope. Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside. This new image from Hubble's Advanced Camera for Surveys displays, with particular clarity, the pink - colored puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light - years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy. NGC 6503 lies approximately 17 million light - years away in the co

PIX4612940

Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the

Planetary nebula NGC 6302 in Scorpio - Planetary nebula NGC 6302 in Scorpius - NGC 6302 is a planetary nebula located about 4000 years from Earth. In the center of the nebula, an extremely hot dying star. Image obtained by the Hubble Space Telescope with the new WFC 3 (Wide Field Camera 3) camera, July 27, 2009. A dying star that was once about five times the mass of the Sun is at the center of this nebula. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast - off material glow. This object is an example of a planetary nebula, so - named because many of them have a round appearance resembling that of a planet when viewed through a small telescope. The Wide Field Camera 3 (WFC3), a new camera aboard Nasa's Hubble Space Telescope, snapped this image of the planetary nebula, catalogued as NGC 6302, but more popularly called the Bug Nebula or the Butterfly Nebula. WFC3 was installed by NASA astronauts in May 2009, during the

PIX4623200

Remains of the Supernova of Vails - The Vela supernova remnant: Nearly 12,000 years ago, a massive star exploded in the constellation of Vails. The star reaches the end of life and expels its material to become a small star only a few kilometres in diameter. This stellar corpse is a neutron star, the pulsar of Voiles, barely visible in the image. The gas shell that surrounds it today extends over more than 100 light years. Mosaic of 117 images - Approximately 11,000 to 12,000 years ago a massive star exploded in the southern constellation of Vela. The matter ejected by the supernova scattered the contents of the star into the surrounding interstellar medium creating shock fronts of multimillion degree gas and high energy particles. The heated matter produces brilliant visible light as well as radio and x-ray emission which will continue for thousands of years until the entire remnant of the dying star completely dissipates into space. Supernovas enrich the surrounding interstellar medi

Remains of the Supernova of Vails - The Vela supernova remnant: Nearly 12,000 years ago, a massive star exploded in the constellation of Vails. The star reaches the end of life and expels its material to become a small star only a few kilometres in diameter. This stellar corpse is a neutron star, the pulsar of Voiles, barely visible in the image. The gas shell that surrounds it today extends over more than 100 light years. Mosaic of 117 images - Approximately 11,000 to 12,000 years ago a massive star exploded in the southern constellation of Vela. The matter ejected by the supernova scattered the contents of the star into the surrounding interstellar medium creating shock fronts of multimillion degree gas and high energy particles. The heated matter produces brilliant visible light as well as radio and x-ray emission which will continue for thousands of years until the entire remnant of the dying star completely dissipates into space. Supernovas enrich the surrounding interstellar medi

R. Gendler

PIX4626466

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns

Adam Block

PIX4609424

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

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy and Italian actress-director Asia Argentina. Savannah Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times will reveal that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical. From the book The Heart Is Deceitful Above All Things, Asia Argento in 2004 will take a movie/Roma, 3 December 2000. Savannah Knoop a.k.a. lo scrittore J.T. Leroy, with the attrick-regista Asia Argento. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parr

Rome, June 3, 2000. Savanna Knoop a.k.a. J.T. Leroy and Italian actress-director Asia Argentina. Savannah Knoop pretends to be writer J.T. Leroy, but in 2006, the New York Times will reveal that J.T. Leroy does not exist: the true author of his books is writer Laura Albert. Savannah Knoop, the half sister of Albert mate, played this part for years around the world wearing a blonde wig and big sunglasses, to create a problematic character and make believable those tales of prostitution and ill-treatment, presented as autobiographical. From the book The Heart Is Deceitful Above All Things, Asia Argento in 2004 will take a movie/Roma, 3 December 2000. Savannah Knoop a.k.a. lo scrittore J.T. Leroy, with the attrick-regista Asia Argento. Nel 2006 il New York Times riveler che J.T. Leroy in realt non esiste: la vera auteur dei suoi libri et la scrittrice Laura Albert. Savannah Knoop, sorellastra del compagno della Albert, ha recitato la parte per anni in giro per il mondo indossando una parr

Marcello Mencarini

MME4736120

Feb. 02, 1954 - A Wedding Begins Her Day. Miss Suzanne Cloutier, the 25-year old English Canadian actress who had a one-word part last December in Mr. Peter Ustinov's ten-night play “No sign of the Dove”, became Mrs. Ustinov yesterday. The couple, who met three years ago while the 32 -ear old actor-author was starring in his own success” The Love of Four Colonels”, had an early morning wedding at Chelsea Register Office, so that the bridegroom should miss no more than an hour's work on the Elstree film” Beau Brummel”. The wedding lasted only ten minutes. Within the hour, Mr. Ustinov was at Elstree to resume his role of the Prince Regent. The couple will fly to New York tomorrow. Keystone Photo Shows: - Yesterday's picture of Mrs. Ustinov, with models of characters played by her husband in” The Love of Four Colonels'

Feb. 02, 1954 - A Wedding Begins Her Day. Miss Suzanne Cloutier, the 25-year old English Canadian actress who had a one-word part last December in Mr. Peter Ustinov's ten-night play “No sign of the Dove”, became Mrs. Ustinov yesterday. The couple, who met three years ago while the 32 -ear old actor-author was starring in his own success” The Love of Four Colonels”, had an early morning wedding at Chelsea Register Office, so that the bridegroom should miss no more than an hour's work on the Elstree film” Beau Brummel”. The wedding lasted only ten minutes. Within the hour, Mr. Ustinov was at Elstree to resume his role of the Prince Regent. The couple will fly to New York tomorrow. Keystone Photo Shows: - Yesterday's picture of Mrs. Ustinov, with models of characters played by her husband in” The Love of Four Colonels'

ZUM4911978

The Gamma ray sky - The Gamma ray sky - Map of the whole sky seen in gamma rays by the Fermi Gamma-Ray Space Telescope (FGST) satellite from August 4 to October 30, 2008. The strongest sources of gamma radiation are legendeed here. All-sky image seen in gamma ray showing the glowing gas of the Milky Way, blinking pulsars, and galaxies billions of light-years away. The all-sky image released today shows us how the cosmos would look if our eyes could detect radiation 150 million times more energetic than visible light. The view merges Large Area Telescope (LAT) on Fermi Gamma-ray Space Telescope (FGST) observations spanning 87 days, from August 4 to October 30, 2008. The top five sources within our galaxy are: The sun. Now near the minimum of its activity cycle, the sun would not be a particularly notable source except for one thing: It's the only one that moves across the sky. The sun's annual motion against the background sky is a reflection of Earth's orbit around the sun. LSI+61 303.

The Gamma ray sky - The Gamma ray sky - Map of the whole sky seen in gamma rays by the Fermi Gamma-Ray Space Telescope (FGST) satellite from August 4 to October 30, 2008. The strongest sources of gamma radiation are legendeed here. All-sky image seen in gamma ray showing the glowing gas of the Milky Way, blinking pulsars, and galaxies billions of light-years away. The all-sky image released today shows us how the cosmos would look if our eyes could detect radiation 150 million times more energetic than visible light. The view merges Large Area Telescope (LAT) on Fermi Gamma-ray Space Telescope (FGST) observations spanning 87 days, from August 4 to October 30, 2008. The top five sources within our galaxy are: The sun. Now near the minimum of its activity cycle, the sun would not be a particularly notable source except for one thing: It's the only one that moves across the sky. The sun's annual motion against the background sky is a reflection of Earth's orbit around the sun. LSI+61 303.

PIX4638007

Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

PIX4620802

Exoplanete Gliese 1214 b -: Gliese 1214 b (or GJ 1214 b) is a super-earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on December 16, 2009. It is located about 40 light years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light-years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a Super-earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After Corot-7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low de

Exoplanete Gliese 1214 b -: Gliese 1214 b (or GJ 1214 b) is a super-earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on December 16, 2009. It is located about 40 light years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light-years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a Super-earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After Corot-7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low de

Miller, Ron (b.1947)

PIX4608051

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this regio

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this regio

Tom Davis

PIX4618385

Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a

Planetary nebula myCN18 dans la Mouche/HST - This is an image of MyCN18, a young planetary nebula located about 8,000 light - years away, taken with the Wide Field and Planetary Camera 2 (WFPC2) aboard Nasa's Hubble Space Telescope (HST). This picture has been composed from three separate images taken in the light of ionized nitrogen (represented by red), hydrogen (green), and doubly - ionized oxygen (blue). The results are of great interest because they shed new light on the poorly understood ejection of stellar matter which accompanies the slow death of Sun - like stars. According to one theory for the formation of planetary nebulae, the hourglass shape is produced by the expansion of a fast stellar wind within a slowly expanding cloud which is more dense near its equator than near its poles. What appears as a bright elliptical ring in the center, and at first sight might be mistaken for an equatorially dense region, is seen on closer inspection to be a potato shaped structure with a

PIX4623735

Oslo 19540821, Marienlyst. Broadcasting television trials are lining towards the end of the …, 1954 (photo)

Oslo 19540821, Marienlyst. Broadcasting television trials are lining towards the end of the …, 1954 (photo)

Aage Storløkken

NTB8912403

Dec. 12, 1954 - Two Women Murdered at 'Old Folks' Home. A woman who called herself Lady Menzies, and her daughter, Mrs. Isobel Veronica Chesney, were found murdered yesterday in the” Home for elderly Gentlefolk” which they ran at Montpelier Road, Ealing. Mrs. Chesney, who was 48, was half clothed in a bath on the top floor of the home. She appeared to have been attacked from behind while undressing, and left to lie as she fell. Her mother, wearing a red cardigan and fully clothed, was found in front of the fire in a ground floor sitting room. Her injuries suggest that she was struck from behind. The mother had for years used a title which though claimed by her husband when he was alive was never established

Dec. 12, 1954 - Two Women Murdered at 'Old Folks' Home. A woman who called herself Lady Menzies, and her daughter, Mrs. Isobel Veronica Chesney, were found murdered yesterday in the” Home for elderly Gentlefolk” which they ran at Montpelier Road, Ealing. Mrs. Chesney, who was 48, was half clothed in a bath on the top floor of the home. She appeared to have been attacked from behind while undressing, and left to lie as she fell. Her mother, wearing a red cardigan and fully clothed, was found in front of the fire in a ground floor sitting room. Her injuries suggest that she was struck from behind. The mother had for years used a title which though claimed by her husband when he was alive was never established

ZUM4947073

Nov. 11, 1953 - The Wilds Of Darkest Africa Filmed In Elstree Studios: Under a galvanised iron roof at Elstree Studios yesterday 140 feet of Africa's mighty Zambesi River roared and swirled while two Hollywood stars fought to keep their cance afloat. No one knows how many thousands of years it took the real Zambesi to develop, but Elstree technicians did the job in seven days for new film,” Duel In The Jungle” starring Jeanne Crain And Dana Andrews. The result is an ugly stretch of muddy water bordered on one side by tangled jungle with two 16 ft. electric paddles at one end of the 150 ft. long tank to keep the water racing and submerged hoses boil it up into dangerous cross currents. The water was heated to 70 degree in case either of the stars should fall in

Nov. 11, 1953 - The Wilds Of Darkest Africa Filmed In Elstree Studios: Under a galvanised iron roof at Elstree Studios yesterday 140 feet of Africa's mighty Zambesi River roared and swirled while two Hollywood stars fought to keep their cance afloat. No one knows how many thousands of years it took the real Zambesi to develop, but Elstree technicians did the job in seven days for new film,” Duel In The Jungle” starring Jeanne Crain And Dana Andrews. The result is an ugly stretch of muddy water bordered on one side by tangled jungle with two 16 ft. electric paddles at one end of the 150 ft. long tank to keep the water racing and submerged hoses boil it up into dangerous cross currents. The water was heated to 70 degree in case either of the stars should fall in

ZUM4894597

Spiral Galaxy NGC 3810 in the Lion - Spiral galaxy NGC 3810 in Leo - NGC 3810 is a spiral galaxy located at a distance of about 50 million light years in the constellation Lion. Image obtained by the Hubble Space Telescope. The bright galaxy NGC 3810 demonstrates classical spiral structure in this very detailed image from Hubble. The bright central region is thought to be forming many new stars and is outshining the outer areas of the galaxy by some margin. Further out the galaxy displays strikingly rich dust clouds along its spiral arms. A close look shows that Hubble's sharp vision also allows many individual stars to be seen. Hot young blue stars show up in giant clusters far from the center and the arms are also littered with bright red giant stars. NGC 3810 is located about 50 million light - years from Earth in the constellation of Leo (the lion). It was discovered by William Herschel in 1784 and is easily seen as a faint smudge in small telescopes

Spiral Galaxy NGC 3810 in the Lion - Spiral galaxy NGC 3810 in Leo - NGC 3810 is a spiral galaxy located at a distance of about 50 million light years in the constellation Lion. Image obtained by the Hubble Space Telescope. The bright galaxy NGC 3810 demonstrates classical spiral structure in this very detailed image from Hubble. The bright central region is thought to be forming many new stars and is outshining the outer areas of the galaxy by some margin. Further out the galaxy displays strikingly rich dust clouds along its spiral arms. A close look shows that Hubble's sharp vision also allows many individual stars to be seen. Hot young blue stars show up in giant clusters far from the center and the arms are also littered with bright red giant stars. NGC 3810 is located about 50 million light - years from Earth in the constellation of Leo (the lion). It was discovered by William Herschel in 1784 and is easily seen as a faint smudge in small telescopes

PIX4610976

Star Birth in Scorpio - Stellar nursery in Scorpius - RCW 120 is a star-forming region about 4200 years from Earth in the constellation Scorpio. In the center a hot and massive star emits powerful ultraviolet radiation, which ionize the surrounding gas, tearing off electrons from the hydrogen atoms and producing the characteristic red glow of H - alpha emissions. As this ionized region extends into space, the associated shock wave meets the surrounding cold interstellar gas and cosmic dust. This gas becomes unstable and collapses under its own gravite forming dense, cold clouds or new stars will be born. These very cold clouds (- 250 degres Celsius) can only be detected in submillimetre wavelength; they appear here in blue thanks to the data obtained by the APEX telescope which observes this radiation. Illustrating the power of submillimetre - wavelength astronomy, an APEX image reveals how an expanding bubble of ionised gas about ten light - years across is causing the surrounding mat

Star Birth in Scorpio - Stellar nursery in Scorpius - RCW 120 is a star-forming region about 4200 years from Earth in the constellation Scorpio. In the center a hot and massive star emits powerful ultraviolet radiation, which ionize the surrounding gas, tearing off electrons from the hydrogen atoms and producing the characteristic red glow of H - alpha emissions. As this ionized region extends into space, the associated shock wave meets the surrounding cold interstellar gas and cosmic dust. This gas becomes unstable and collapses under its own gravite forming dense, cold clouds or new stars will be born. These very cold clouds (- 250 degres Celsius) can only be detected in submillimetre wavelength; they appear here in blue thanks to the data obtained by the APEX telescope which observes this radiation. Illustrating the power of submillimetre - wavelength astronomy, an APEX image reveals how an expanding bubble of ionised gas about ten light - years across is causing the surrounding mat

PIX4621694

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 450 years - light from Earth. Image obtained by a 50 cm telescope, 42 poses of 15 minutes accumulated. Located in the constellation of Aquarius, the Helix is our closest planetary nebula at only 450 light years distance. It is so close that it can be telescopically seen shifting one side to the other in front of the more distant background stars as the earth moves around the sun - a phenomenon called parallax. Parallax measurements are used to trigonometrically deduce distance between an object in space and the earth. A planetary nebula results when a red giant star, near the ends of it's productive life, sheds its outer layers into space and creates a breathtaking shell of surrounding gas that early visual astronomers likened to the disks of planets. This planetary spans approximately 1.5 light years and is still expanding. The name associated with the Helix is derived from the c

Planetary nebula Helix (NGC 7293) in Aquarius - Planetary nebula Helix (NGC 7293) - This nebula is located 450 years - light from Earth. Image obtained by a 50 cm telescope, 42 poses of 15 minutes accumulated. Located in the constellation of Aquarius, the Helix is our closest planetary nebula at only 450 light years distance. It is so close that it can be telescopically seen shifting one side to the other in front of the more distant background stars as the earth moves around the sun - a phenomenon called parallax. Parallax measurements are used to trigonometrically deduce distance between an object in space and the earth. A planetary nebula results when a red giant star, near the ends of it's productive life, sheds its outer layers into space and creates a breathtaking shell of surrounding gas that early visual astronomers likened to the disks of planets. This planetary spans approximately 1.5 light years and is still expanding. The name associated with the Helix is derived from the c

R. Jay GaBany

PIX4623639

Exoplanete Gliese 1214 b - Gliese 1214 b (or GJ 1214 b) is a super-Earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on 16 December 2009. It is located about 40 years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light - years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a super - Earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After COROT - 7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low dens

Exoplanete Gliese 1214 b - Gliese 1214 b (or GJ 1214 b) is a super-Earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on 16 December 2009. It is located about 40 years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light - years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a super - Earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After COROT - 7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low dens

Miller, Ron (b.1947)

PIX4574069

Exoplanete Gliese 1214 b -: Gliese 1214 b (or GJ 1214 b) is a super-earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on December 16, 2009. It is located about 40 light years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light-years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a Super-earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After Corot-7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low de

Exoplanete Gliese 1214 b -: Gliese 1214 b (or GJ 1214 b) is a super-earth exoplanet orbiting the star Gliese 1214 in the constellation Ophiuchus, whose discovery was announced on December 16, 2009. It is located about 40 light years from the Sun. It is the third discovered exoplanet whose size is smaller than that of a gas giant and the first on which water could be present in large quantities given its size and estimated mass. It could be the first ocean planet discovered. Gliese 1214 b is an extrasolar planet that orbits the star Gliese 1214. The parent star is 13 parsecs (approximately 40 light-years) from the Sun, in the constellation Ophiuchus. The planet was discovered in December 2009. It is classified as a Super-earth because it is larger than Earth but has a mass and radius significantly less than those of the gas giants in the Solar System. After Corot-7b, it is the second such planet to be known and is the first of a new class of planets with small size and relatively low de

Miller, Ron (b.1947)

PIX4608046

Interacting Galaxies Arp 240 - Interacting galaxies Arp 240 - The galaxy Arp 240 is located about 300 million light years away from Earth in the constellation of the Virgin. Composed of spiral galaxies NGC 5257 and NGC 5258, this interacting system presents important star formations. The two galaxies contain a supermassive black hole in the centre. Image obtained by the Hubble Space Telescope on 20 December 2001. NGC 5257/8 (Arp 240) is an astonishing galaxy pair, composed of spiral galaxies of similar mass and size, NGC 5257 and NGC 5258. The galaxies are visibly interacting with each other via a bridge of dim stars connecting the two galaxies, almost like two dancers holding hands while performing a pirouette. Both galaxies harbor supermassive black holes in their centers and are actively forming new stars in their disks. Arp 240 is located in the constellation Virgo, approximately 300 million light - years away, and is the 240th galaxy in ARP's Atlas of Peculiar Galaxies. With the e

Interacting Galaxies Arp 240 - Interacting galaxies Arp 240 - The galaxy Arp 240 is located about 300 million light years away from Earth in the constellation of the Virgin. Composed of spiral galaxies NGC 5257 and NGC 5258, this interacting system presents important star formations. The two galaxies contain a supermassive black hole in the centre. Image obtained by the Hubble Space Telescope on 20 December 2001. NGC 5257/8 (Arp 240) is an astonishing galaxy pair, composed of spiral galaxies of similar mass and size, NGC 5257 and NGC 5258. The galaxies are visibly interacting with each other via a bridge of dim stars connecting the two galaxies, almost like two dancers holding hands while performing a pirouette. Both galaxies harbor supermassive black holes in their centers and are actively forming new stars in their disks. Arp 240 is located in the constellation Virgo, approximately 300 million light - years away, and is the 240th galaxy in ARP's Atlas of Peculiar Galaxies. With the e

PIX4612595

Exoplanete GJ 1214 b - Exoplanet GJ 1214 b - Illustration showing the transit of the extrasolar planet GJ 1214 b in front of its star, the red dwarf GJ 1214, in the constellation Ophiuchus. GJ 1214 b is a super Earth, six times the mass of the Earth, which has an atmosphere but is too inhospitable to shelter life as we know it. This artist's impression shows how the super - Earth surrounding the nearby star GJ1214 may look. Discovered by the Mearth project and investigated further by the HARPS spectrograph on ESO's 3.6 - metre telescope at La Silla, GJ1214b is the second super - Earth exoplanet for which astronomers have determined the mass and radius, giving vital clues about its structure. It is also the first super - Earth around which an atmosphere has been found. The exoplanet, orbiting a small star only 40 light - years away from us, thus opens dramatic new perspectives in the quest for habitable worlds. The planet, GJ1214b, has a mass about six times that of Earth and its interi

Exoplanete GJ 1214 b - Exoplanet GJ 1214 b - Illustration showing the transit of the extrasolar planet GJ 1214 b in front of its star, the red dwarf GJ 1214, in the constellation Ophiuchus. GJ 1214 b is a super Earth, six times the mass of the Earth, which has an atmosphere but is too inhospitable to shelter life as we know it. This artist's impression shows how the super - Earth surrounding the nearby star GJ1214 may look. Discovered by the Mearth project and investigated further by the HARPS spectrograph on ESO's 3.6 - metre telescope at La Silla, GJ1214b is the second super - Earth exoplanet for which astronomers have determined the mass and radius, giving vital clues about its structure. It is also the first super - Earth around which an atmosphere has been found. The exoplanet, orbiting a small star only 40 light - years away from us, thus opens dramatic new perspectives in the quest for habitable worlds. The planet, GJ1214b, has a mass about six times that of Earth and its interi

PIX4573892

Galaxy cluster SDSS J1004+4112 - Galaxy Cluster SDSS J1004+4112 - View of the cluster of SDSS J1004+4112 by the Hubble space telescope; located in the Little Lion about 7 billion years ago - light, this cluster reveals us by a gravitational mirage effect, the deformed image of a quasar, located behind the cluster has a distance of 10 billion years - light. The most unique feature in a new image taken with the NASA/ESA Hubble Space Telescope is a group of five quasar images produced by a process called gravitational lensing, in which the gravitational field of a massive object - in this case, a cluster of galaxies - bends and amplifies light from an object - in this case, a quasar farther behind it. The background quasar is the brilliant core of a galaxy. It is powered by a black hole, which is devouring gas and dust and creating a gusher of light in the process. When the quasar's light passes through the gravity field of the galaxy cluster that lies between us and the quasar, the light

Galaxy cluster SDSS J1004+4112 - Galaxy Cluster SDSS J1004+4112 - View of the cluster of SDSS J1004+4112 by the Hubble space telescope; located in the Little Lion about 7 billion years ago - light, this cluster reveals us by a gravitational mirage effect, the deformed image of a quasar, located behind the cluster has a distance of 10 billion years - light. The most unique feature in a new image taken with the NASA/ESA Hubble Space Telescope is a group of five quasar images produced by a process called gravitational lensing, in which the gravitational field of a massive object - in this case, a cluster of galaxies - bends and amplifies light from an object - in this case, a quasar farther behind it. The background quasar is the brilliant core of a galaxy. It is powered by a black hole, which is devouring gas and dust and creating a gusher of light in the process. When the quasar's light passes through the gravity field of the galaxy cluster that lies between us and the quasar, the light

PIX4565683

«
1
…
5
6
7
…
494
»

Pourquoi choisir Bridgeman Images

Art. Culture. Histoire.

Nous travaillons en partenariat avec les plus grands musées, galeries et artistes du monde entier, ce qui vous permet d'avoir accès à des images de la plus haute qualité.

Découvrez notre collection Consultez nos FAQs

Simple. Rapide. Fiable.

Nos équipes peuvent vous aider à trouver le contenu idéal et s'occuper de toutes les exigences en matière de droits d'auteur et de licences.

Contactez-nous

Découvrez des millions d'images et de vidéos pour vos projets.

Commencez votre recherche

© Droits d'auteur 2024 Bridgeman Art Library Limited. Enregistrée en Angleterre et au Pays de Galles sous le numéro d'entreprise 01056394.