{"id":34121,"date":"2025-03-12T15:08:58","date_gmt":"2025-03-12T14:08:58","guid":{"rendered":"https:\/\/www.ieec.cat\/?p=34121"},"modified":"2025-03-17T11:42:19","modified_gmt":"2025-03-17T10:42:19","slug":"a-super-earth-discovered-in-the-habitable-zone-of-a-nearby-red-dwarf","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/en\/a-super-earth-discovered-in-the-habitable-zone-of-a-nearby-red-dwarf\/","title":{"rendered":"A super-Earth discovered in the habitable zone of a nearby red dwarf"},"content":{"rendered":"<p>[et_pb_section fb_built=&#8221;1&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; background_image=&#8221;https:\/\/www.ieec.cat\/wp-content\/uploads\/2022\/02\/slider-comunicacio.jpg&#8221; max_height=&#8221;130px&#8221; custom_padding=&#8221;0px||0px||false|false&#8221; da_disable_devices=&#8221;off|off|off&#8221; global_colors_info=&#8221;{}&#8221; da_is_popup=&#8221;off&#8221; da_exit_intent=&#8221;off&#8221; da_has_close=&#8221;on&#8221; da_alt_close=&#8221;off&#8221; da_dark_close=&#8221;off&#8221; da_not_modal=&#8221;on&#8221; da_is_singular=&#8221;off&#8221; da_with_loader=&#8221;off&#8221; da_has_shadow=&#8221;on&#8221;][\/et_pb_section][et_pb_section fb_built=&#8221;1&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_padding=&#8221;24px||11px|||&#8221; da_disable_devices=&#8221;off|off|off&#8221; global_colors_info=&#8221;{}&#8221; da_is_popup=&#8221;off&#8221; da_exit_intent=&#8221;off&#8221; da_has_close=&#8221;on&#8221; da_alt_close=&#8221;off&#8221; da_dark_close=&#8221;off&#8221; da_not_modal=&#8221;on&#8221; da_is_singular=&#8221;off&#8221; da_with_loader=&#8221;off&#8221; da_has_shadow=&#8221;on&#8221;][et_pb_row _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_padding=&#8221;||||false|false&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text admin_label=&#8221;Unitats de recerca&#8221; module_class=&#8221;ieec-orgs&#8221; _builder_version=&#8221;4.27.4&#8243; _dynamic_attributes=&#8221;content&#8221; _module_preset=&#8221;default&#8221; text_font=&#8221;|700||on|||||&#8221; text_font_size=&#8221;16px&#8221; header_font=&#8221;|700|||||||&#8221; custom_margin=&#8221;||10px||false|false&#8221; header_font_size_tablet=&#8221;28px&#8221; header_font_size_phone=&#8221;26px&#8221; header_font_size_last_edited=&#8221;on|phone&#8221; global_colors_info=&#8221;{}&#8221;]@ET-DC@eyJkeW5hbWljIjp0cnVlLCJjb250ZW50IjoiY3VzdG9tX21ldGFfb3JnYW5pemFjaW9uZXMiLCJzZXR0aW5ncyI6eyJiZWZvcmUiOiIiLCJhZnRlciI6IiIsImVuYWJsZV9odG1sIjoib2ZmIn19@[\/et_pb_text][et_pb_post_title author=&#8221;off&#8221; categories=&#8221;off&#8221; comments=&#8221;off&#8221; featured_image=&#8221;off&#8221; admin_label=&#8221;T\u00edtol i data&#8221; module_class=&#8221;ieec-title&#8221; _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; title_font=&#8221;Cairo|300|||||||&#8221; title_font_size=&#8221;40px&#8221; meta_font=&#8221;||on||||||&#8221; meta_font_size=&#8221;16px&#8221; title_font_size_tablet=&#8221;35px&#8221; title_font_size_phone=&#8221;30px&#8221; title_font_size_last_edited=&#8221;on|desktop&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_post_title][et_pb_text admin_label=&#8221;Subt\u00edtols&#8221; module_class=&#8221;ieec-summary&#8221; _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; text_font=&#8221;Source Sans Pro||on||||||&#8221; text_font_size=&#8221;24px&#8221; text_line_height=&#8221;1.1em&#8221; hover_enabled=&#8221;0&#8243; text_font_size_tablet=&#8221;22px&#8221; text_font_size_phone=&#8221;20px&#8221; text_font_size_last_edited=&#8221;on|phone&#8221; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<ul>\n<li>GJ 3998 d is the third planet found in the habitable zone of GJ 3998, a nearby red dwarf located 59 light-years away from Earth<\/li>\n<li>The proximity of this system to the Sun makes GJ 3998 d an attractive candidate for atmosphere characterisation<\/li>\n<li>IEEC researchers at the Institute of Space Sciences (ICE-CSIC) have participated in this discovery published in the journal Astronomy &amp; Astrophysics<\/li>\n<\/ul>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row column_structure=&#8221;1_2,1_2&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;1_2&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_post_title title=&#8221;off&#8221; meta=&#8221;off&#8221; module_class=&#8221;ieec-img-container&#8221; _builder_version=&#8221;4.27.2&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;||0px||false|false&#8221; border_width_top=&#8221;10px&#8221; border_color_top=&#8221;#406fda&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_post_title][et_pb_text module_class=&#8221;ieec-img-footer&#8221; _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; text_font=&#8221;||||||||&#8221; text_font_size=&#8221;15px&#8221; text_line_height=&#8221;1.1em&#8221; background_color=&#8221;rgba(64,111,218,0.15)&#8221; custom_margin=&#8221;0px||||false|false&#8221; custom_padding=&#8221;30px|20px|30px|20px|true|true&#8221; hover_enabled=&#8221;0&#8243; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<p><span style=\"font-weight: 400;\">Representation of an exoplanet around its red dwarf.<\/span><br \/><span style=\"font-weight: 400;\"><strong>Gabriel P\u00e9rez D\u00edaz (SMM, IAC)<\/strong><br \/><\/span><\/p>\n<p>[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8221;1_2&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; link_font=&#8221;|700|||on||||&#8221; hover_enabled=&#8221;0&#8243; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<p><span style=\"font-weight: 400;\">An international team, led by the <\/span><a href=\"https:\/\/www.iac.es\/\" target=\"_blank\" rel=\"noopener\"><span style=\"font-weight: 400;\">Instituto de Astrof\u00edsica de Canarias<\/span><\/a><span style=\"font-weight: 400;\"> (IAC) and with the participation of researchers from the <\/span><a href=\"https:\/\/www.ieec.cat\/en\/\"><span style=\"font-weight: 400;\">Institute of Space Studies of Catalonia<\/span><\/a><span style=\"font-weight: 400;\"> (IEEC \u2014 Institut d\u2019Estudis Espacials de Catalunya) at the <\/span><a href=\"https:\/\/www.ice.csic.es\/\" target=\"_blank\" rel=\"noopener\"><span style=\"font-weight: 400;\">Institute of Space Sciences<\/span><\/a><span style=\"font-weight: 400;\"> (ICE-CSIC), has detected a super-Earth orbiting in the habitable zone of GJ 3998, a nearby red dwarf located 59 light-years away. The new planet, named GJ 3998 d, is the third planet found in the system.\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">\u201cGJ 3998 d is a welcome addition to the planetary census of our cosmic neighbourhood\u201d, states Atanas Stefanov, La Caixa funded PhD student at IAC and the University of La Laguna (ULL) and main author of the study published in <\/span><i><span style=\"font-weight: 400;\">Astronomy &amp; Astrophysics<\/span><\/i><span style=\"font-weight: 400;\">. \u201c<\/span><b>This super-Earth appears to be in the habitable zone of one of the nearest stars to the Sun.<\/b><span style=\"font-weight: 400;\"> This gives us one more reason to keep searching for habitable planets at our doorstep,\u201d he adds. <\/span><\/p>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; link_font=&#8221;|700|||on||||&#8221; hover_enabled=&#8221;0&#8243; locked=&#8221;off&#8221; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<p><span style=\"font-weight: 400;\">The newly discovered planet, GJ 3998 d, is a super-Earth with a mass 6 times larger than the mass of the Earth. It resides in the optimistic habitable zone of its star and completes an orbit once every 41.8 days. At this distance, GJ 3998 d gets just 20% more stellar insolation compared to what Earth receives by the Sun.\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">\u201cDespite we already know more than 5800 of them, <\/span><b>only a very small number of exoplanets show such characteristics, which are interesting for further studies on the presence of so-called biomarkers in their atmospheres<\/b><span style=\"font-weight: 400;\">,\u201d says Manuel Perger, IEEC researcher at the ICE-CSIC, and co-author of the study.\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">Researchers at the ICE-CSIC and the IEEC contributed with the analysis of the complex data of both the planetary companions and the magnetic activity of the host star, manifested in dark spots on the stellar surface. <\/span><span style=\"font-weight: 400;\">\u00a0<\/span><span style=\"font-weight: 400;\">\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">\u201cGJ 3998 is significantly smaller and cooler than the Sun, and this moves the habitable zone closer to the star,\u201d explains Alejandro Su\u00e1rez Mascare\u00f1o, a researcher in the IAC and co-author of the study. \u201cWhile it is certainly different from the Earth, if the planet is rocky, it might be able to host liquid water on its surface, one of the main requirements for life,\u201d noted Jonay I. Gonz\u00e1lez Hern\u00e1ndez, a researcher at the IAC and a co-author.\u00a0<\/span><\/p>\n<p><span style=\"font-weight: 400;\">The proximity of this system to the Sun makes GJ 3998 d an attractive candidate for atmosphere characterisation. \u201c<\/span><b>It should be possible to check for the presence of an atmosphere and probe for oxygen <\/b><span style=\"font-weight: 400;\">using the future ANDES spectrograph at ESO\u2019s Extremely Large Telescope (ELT). GJ 3998 d would also be a good target for the future 50m Exo Life Finder (ELF) telescope, led by the IAC, which will be looking for biosignatures in exoplanet atmospheres,\u201d adds Rafael Rebolo, researcher at the IAC and co-author of the study.<\/span><\/p>\n<p><span style=\"font-weight: 400;\">The discovery is part of the HADES programme, an international effort to explore planetary systems around red dwarfs through the Telescopio Nazionale Galileo (TNG) telescope at <\/span><a href=\"https:\/\/www.iac.es\/es\/observatorios-de-canarias\/observatorio-del-roque-de-los-muchachos\" target=\"_blank\" rel=\"noopener\"><span style=\"font-weight: 400;\">Roque de los Muchachos Observatory<\/span><\/a><span style=\"font-weight: 400;\">, La Palma. Red dwarfs are smaller, cooler stars than our own, and make up nearly three quarters of the stellar population in our galaxy. Their low masses and their abundance make them prime targets in the search of low-mass planets. GJ 3998, one such red dwarf, has been attractive to the community for its proximity (59 light years) and for its rather tame stellar activity. Using the HARPS-N spectrograph at the TNG telescope, the team was able to detect minute wobbles in the star\u2019s motion, caused by the gravitational tug of orbiting planets.<\/span><\/p>\n<p><span style=\"font-weight: 400;\">A previous study conducted in 2016 by the same team had already detected two planets. The presence of an additional signal in the data prompted the continuation of the observations and the reanalysis of the dataset. With three known planets now detected in the system, GJ 3998 highlights once again how common multi-planetary systems are. \u201cPlanets, in particular low-mass ones, are rarely on their own\u2014they prefer to have company. Often, when we revisit a system with new measurements and new methods, we find new planets that had been overlooked before\u201d, concludes Atanas Stefanov.\u00a0<\/span><\/p>\n<p>&nbsp;<\/p>\n<p><i><span style=\"font-weight: 400;\">Press release prepared in collaboration with the Instituto de Astrof\u00edsica de Canarias and the Institute of Space Sciences.<\/span><\/i><\/p>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;30px||||false|false&#8221; locked=&#8221;off&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_divider color=&#8221;#406fda&#8221; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;||10px||false|false&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_divider][et_pb_text admin_label=&#8221;M\u00e9s informaci\u00f3&#8221; module_class=&#8221;ieec-sub-title&#8221; _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; text_font=&#8221;Cairo|700|||||||&#8221; text_text_color=&#8221;#406fda&#8221; text_font_size=&#8221;20px&#8221; custom_margin=&#8221;||10px||false|false&#8221; hover_enabled=&#8221;0&#8243; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<p>More information<\/p>\n<p>[\/et_pb_text][et_pb_text module_class=&#8221;ieec-sub-text&#8221; _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; text_font_size=&#8221;16px&#8221; text_line_height=&#8221;1.1em&#8221; link_font=&#8221;|700|||on||||&#8221; custom_margin=&#8221;20px||||false|false&#8221; hover_enabled=&#8221;0&#8243; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<p><span style=\"font-weight: 400;\">This research is presented in a paper entitled \u201c<\/span><a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/202452630\" target=\"_blank\" rel=\"noopener\"><span style=\"font-weight: 400;\">HADES RV Programme with HARPS-N at TNG. XVI. A super-Earth in the habitable zone of the GJ 3998 multi-planet system<\/span><\/a><span style=\"font-weight: 400;\">\u201d, by <\/span><span style=\"font-weight: 400;\">Stefanov, A. K. <\/span><i><span style=\"font-weight: 400;\">et al.<\/span><\/i><span style=\"font-weight: 400;\">, incl. Ribas, I., Perger, M.<\/span><span style=\"font-weight: 400;\">, to appear in the journal Astronomy &amp; Astrophysics on 11 March 2025.<\/span><\/p>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;||||false|false&#8221; locked=&#8221;off&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_divider color=&#8221;#406fda&#8221; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;||10px||false|false&#8221; global_colors_info=&#8221;{}&#8221;][\/et_pb_divider][et_pb_text admin_label=&#8221;Enlla\u00e7os&#8221; module_class=&#8221;ieec-sub-title&#8221; _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; text_font=&#8221;Cairo|700|||||||&#8221; text_text_color=&#8221;#406fda&#8221; text_font_size=&#8221;20px&#8221; custom_margin=&#8221;||10px||false|false&#8221; hover_enabled=&#8221;0&#8243; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<p>Links<\/p>\n<p>[\/et_pb_text][et_pb_text module_class=&#8221;ieec-sub-text&#8221; _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; text_font_size=&#8221;16px&#8221; text_line_height=&#8221;1.1em&#8221; link_font=&#8221;|700|||on|||#1a1140|&#8221; link_text_color=&#8221;#1a1140&#8243; link_line_height=&#8221;1.4em&#8221; custom_margin=&#8221;20px||||false|false&#8221; hover_enabled=&#8221;0&#8243; global_colors_info=&#8221;{}&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<ul>\n<li><a href=\"http:\/\/www.ieec.cat\/\"><span style=\"font-weight: 400;\">IEEC<\/span><\/a><\/li>\n<li><a href=\"https:\/\/www.ice.csic.es\/\" target=\"_blank\" rel=\"noopener\"><span style=\"font-weight: 400;\">ICE-CSIC<\/span><\/a><\/li>\n<li><a href=\"https:\/\/www.iac.es\/\" target=\"_blank\" rel=\"noopener\"><span style=\"font-weight: 400;\">Instituto de Astrof\u00edsica de Canarias<\/span><\/a><\/li>\n<\/ul>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row _builder_version=&#8221;4.16&#8243; 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admin_label=&#8221;Row&#8221; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_margin=&#8221;0px||||false|false&#8221; custom_padding=&#8221;0px||||false|false&#8221; global_colors_info=&#8221;{}&#8221; theme_builder_area=&#8221;post_content&#8221;][et_pb_column type=&#8221;2_5&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_padding=&#8221;|||20px|false|false&#8221; border_width_left=&#8221;1px&#8221; border_color_left=&#8221;#406fda&#8221; global_colors_info=&#8221;{}&#8221; theme_builder_area=&#8221;post_content&#8221;][et_pb_text _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; text_font_size=&#8221;16px&#8221; text_line_height=&#8221;1.1em&#8221; link_font=&#8221;|700|||on|||#1a1140|&#8221; link_text_color=&#8221;#1a1140&#8243; link_line_height=&#8221;1.4em&#8221; header_4_font=&#8221;|700|||||||&#8221; header_4_text_color=&#8221;#1a1140&#8243; custom_margin=&#8221;||||false|false&#8221; locked=&#8221;off&#8221; global_colors_info=&#8221;{}&#8221; theme_builder_area=&#8221;post_content&#8221;]<\/p>\n<h4>IEEC Communication Office<\/h4>\n<p>Castelldefels, Barcelona<br \/>E-mail: <a href=\"mailto:comunicacio@ieec.cat\">comunicacio@ieec.cat<\/a><\/p>\n<p>[\/et_pb_text][\/et_pb_column][et_pb_column type=&#8221;3_5&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_padding=&#8221;|||20px|false|false&#8221; border_width_left=&#8221;1px&#8221; border_color_left=&#8221;#406fda&#8221; global_colors_info=&#8221;{}&#8221; theme_builder_area=&#8221;post_content&#8221;][et_pb_text _builder_version=&#8221;4.27.4&#8243; _module_preset=&#8221;default&#8221; text_font_size=&#8221;16px&#8221; text_line_height=&#8221;1em&#8221; link_font=&#8221;|700|||on||||&#8221; link_text_color=&#8221;#1a1140&#8243; header_4_font=&#8221;|700|||||||&#8221; header_4_text_color=&#8221;#1a1140&#8243; hover_enabled=&#8221;0&#8243; global_colors_info=&#8221;{}&#8221; theme_builder_area=&#8221;post_content&#8221; sticky_enabled=&#8221;0&#8243;]<\/p>\n<h4>Lead Researcher at the IEEC<\/h4>\n<h4>Manuel Perger<\/h4>\n<p>Institute of Space Studies of Catalonia (IEEC)<br \/>Institute of Space Sciences (ICE-CSIC)<br \/>E-mail: <a href=\"mailto:perger@ieec.cat,\">perger@ieec.cat,<\/a> <a href=\"mailto:perger@ice.csic.es\">perger@ice.csic.es<\/a><\/p>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][et_pb_row module_class=&#8221;ieec-about&#8221; _builder_version=&#8221;4.14.8&#8243; _module_preset=&#8221;default&#8221; background_color=&#8221;rgba(64,111,218,0.15)&#8221; global_module=&#8221;17324&#8243; global_colors_info=&#8221;{}&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; custom_padding=&#8221;20px|50px|20px|50px|true|true&#8221; global_colors_info=&#8221;{}&#8221;][et_pb_text admin_label=&#8221;Sobre l&#8217;IEEC&#8221; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; header_2_font=&#8221;|700|||||||&#8221; header_2_font_size=&#8221;25px&#8221; custom_margin=&#8221;||10px||false|false&#8221; header_2_font_size_tablet=&#8221;23px&#8221; header_2_font_size_phone=&#8221;23px&#8221; header_2_font_size_last_edited=&#8221;on|phone&#8221; locked=&#8221;off&#8221; global_colors_info=&#8221;{}&#8221;]<\/p>\n<h2>About the IEEC<\/h2>\n<p>[\/et_pb_text][et_pb_text admin_label=&#8221;Text&#8221; _builder_version=&#8221;4.16&#8243; _module_preset=&#8221;default&#8221; text_font=&#8221;||on||||||&#8221; link_font=&#8221;|700|||on||||&#8221; locked=&#8221;off&#8221; global_colors_info=&#8221;{}&#8221;]<\/p>\n<p>The Institute of Space Studies of Catalonia (IEEC \u2014 Institut d\u2019Estudis Espacials de Catalunya) promotes and coordinates space research and technology development in Catalonia for the benefit of society. IEEC fosters collaborations both locally and worldwide and is an efficient agent of knowledge, innovation and technology transfer. As a result of more than 25 years of high-quality research, done in collaboration with major international organisations, IEEC ranks among the best international research centres, focusing on areas such as: astrophysics, cosmology, planetary science, and Earth Observation. IEEC\u2019s engineering division develops instrumentation for ground- and space-based projects, and has extensive experience in working with private or public organisations from the aerospace and other innovation sectors.<\/p>\n<p>The IEEC is a non-profit public sector foundation that was established in February 1996. It has a Board of Trustees composed of the Generalitat de Catalunya, Universitat de Barcelona (UB), Universitat Aut\u00f2noma de Barcelona (UAB), Universitat Polit\u00e8cnica de Catalunya \u00b7 BarcelonaTech (UPC), and the Spanish Research Council (CSIC). 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