[et_pb_section fb_built=\u00bb1″ fullwidth=\u00bbon\u00bb theme_builder_area=\u00bbpost_content\u00bb _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb height=\u00bb114px\u00bb background_color=\u00bb\u00bb hover_enabled=\u00bb0″ sticky_enabled=\u00bb0″ title_text=\u00bb\u00bb background_image=\u00bb\/wp-content\/uploads\/2022\/04\/slider-corpo2.jpg\u00bb][\/et_pb_section][et_pb_section fb_built=\u00bb1″ theme_builder_area=\u00bbpost_content\u00bb _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb custom_padding=\u00bb||0px||false|false\u00bb custom_margin=\u00bb||0px||false|false\u00bb hover_enabled=\u00bb0″ sticky_enabled=\u00bb0″][et_pb_row _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb theme_builder_area=\u00bbpost_content\u00bb][et_pb_column _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb type=\u00bb4_4″ theme_builder_area=\u00bbpost_content\u00bb][et_pb_text _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb theme_builder_area=\u00bbpost_content\u00bb _dynamic_attributes=\u00bbcontent\u00bb hover_enabled=\u00bb0″ sticky_enabled=\u00bb0″ custom_margin=\u00bb0px||0px||false|false\u00bb custom_padding=\u00bb0px||0px||false|false\u00bb]@ET-DC@eyJkeW5hbWljIjp0cnVlLCJjb250ZW50IjoicG9zdF90aXRsZSIsInNldHRpbmdzIjp7ImJlZm9yZSI6IjxoMSBjbGFzcz1cImVudHJ5X3RpdGxlXCI+IiwiYWZ0ZXIiOiI8L2gxPiJ9fQ==@[\/et_pb_text][et_pb_text _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb theme_builder_area=\u00bbpost_content\u00bb _dynamic_attributes=\u00bbcontent\u00bb custom_padding=\u00bb0px||0px||false|false\u00bb custom_margin=\u00bb0px||0px||false|false\u00bb hover_enabled=\u00bb0″ sticky_enabled=\u00bb0″]@ET-DC@eyJkeW5hbWljIjp0cnVlLCJjb250ZW50IjoicG9zdF9kYXRlIiwic2V0dGluZ3MiOnsiYmVmb3JlIjoiIiwiYWZ0ZXIiOiIiLCJkYXRlX2Zvcm1hdCI6ImN1c3RvbSIsImN1c3RvbV9kYXRlX2Zvcm1hdCI6IlktbS1kIEg6aTpzIn19@[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section][et_pb_section fb_built=\u00bb1″ _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb custom_margin=\u00bb0px||||false|false\u00bb custom_padding=\u00bb0px||||false|false\u00bb top_divider_color=\u00bbRGBA(255,255,255,0)\u00bb top_divider_height=\u00bb0px\u00bb hover_enabled=\u00bb0″ global_colors_info=\u00bb{}\u00bb sticky_enabled=\u00bb0″][et_pb_row column_structure=\u00bb4_4″ _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_column type=\u00bb4_4″ _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_image src=\u00bbhttps:\/\/www.ieec.cat\/wp-content\/uploads\/2022\/12\/1543421896_5549ce274b13b5da9d996ebde545114b_foto1_entrada_bolido_asko_aikkila.jpg\u00bb alt=\u00bbIEEC researchers determine the origin of Annama meteorite\u00bb _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb title_text=\u00bbPR_Image1.png\u00bb hover_enabled=\u00bb0″ sticky_enabled=\u00bb0″ width=\u00bb600px\u00bb module_alignment=\u00bbcenter\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00bb4.14.8″ _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb]An international team led by the Institute of Space Sciences (CSIC-IEEC) has determined the orbit of Annama, a new characterized meteorite from a fireball occurred on April 19th 2014 at the Kola Peninsula (Russia). Researchers highlight the importance of this finding because only the orbit of another 22 meteorites is known so far.<\/p>\n
The characterization of Annama indicates that this is an ordinary H5 chondrite, a group of meteorites with high strength that constitutes 31% of meteorite falls. Researchers have also searched for the existence of some asteroid, among all known, that may have been fragmented and resulted in the meteorite. According to the paper published in Monthly Notices of the Royal Astronomical Society journal, the orbital evolution of Annama shows some similarity to the 2014 UR116, a potentially dangerous asteroid (i.e. an object that might collide the Earth) of about 400 meters in diameter that was discovered last year.<\/p>\n
The reconstruction of the orbit<\/p>\n
IEEC-CSIC researchers compared the orbit of Annama with the evolution of a dozen orbits of near-Earth asteroids, reconstructing how their orbits evolved in the solar system over the past 10,000 years. Through this method, they explain, the degree of orbital similarity is determined and, in the most favourable cases, it can be established if both objects have a common origin.<\/p>\n
Members of several research centres from Finland and Russia reconstructed the trajectory of the fireball and calculated the location of the fall using the data from three stations of the Finnish Fireball Network and the filming of a security camera from the Kola Peninsula. One month later, meteor rocks were recovered in this peninsula. Meanwhile, Josep Maria Trigo, CSIC-IEEC, and his team determined its orbit and reconstructed the orbital evolution of Annama in the Solar System in order to compare it with a dozen asteroids with which, a priori, showed orbital similarity at the present time. Most of them are similar by chance, so an orbital integration in the past of the objects is required to decipher if the dynamic link is possible.<\/p>\n
The analysis of the orbital evolution of the meteorite has showed, according to researchers, a “disturbing similarity” with the evolution of 2014 UR116 which, given its size and minimum distance of intersection with the orbit of the Earth, has been classified as a potentially dangerous asteroid. Currently, 1,573 asteroids of this type are known so researchers are investigating to what extent they can pose a danger.<\/p>\n
Origin of meteorites<\/p>\n
Trigo states: “While it is true that many of these dangerous projectiles come from the main belt of asteroids after being gravitationally scattered towards the Earth by the so-called planetary resonances, in 2007 we proposed other physical mechanisms that enable these rocks to be detached from asteroids or comets as they undergo close approaches to our planet”. He also adds: “The tidal effect on an asteroid, which rapidly rotates under the gravitational field of a planet, can fragment these objects or release large rocks from its surface, which could then become such dangerous projectiles at a local scale as the one fell in Cheliábinsk (Russia) on February 15th 2013”.<\/p>\n
Manuel Moreno-Ibáñez, CSIC-IEEC researcher that participated in the study, explains: “The data we have obtained provided new clues about the origin of the rocks with a few meters in diameter that produce meteorite falls. So far, we only know the orbits of other 22 meteorites, and not always with the sought accuracy”. Trigo adds: “In addition, Annama is a fascinating meteorite because it reveals the processes taken place during the formation of the Solar System, as well as more details about the thermal processing suffered by the asteroid it comes from”.<\/p>\n
– J. M. Trigo-Rodríguez, et al. Orbit and dynamic origin of the recently recovered Annama’s H5 chondrite. MNRAS, DOI: 10.1093\/mnras\/stv37<\/p>\n
A picture taken from the Kola Peninsula (Russia) of the fireball at the time of entry to Earth (Credit: Asko Aikkila)<\/p>\n
A section of the meteorite Annama (Credit: Jakub Haloda)<\/p>\n
IEEC in the media<\/p>\n