Studiuesit kan\u00eb zbuluar shkakun e shp\u00ebrthimit m\u00eb t\u00eb ndritsh\u00ebm t\u00eb drit\u00ebs t\u00eb regjistruar ndonj\u00ebher\u00eb, sipas BBC.<\/p>\n\n\n\n
Por, duke e b\u00ebr\u00eb k\u00ebt\u00eb ata jan\u00eb p\u00ebrballur me dy mistere t\u00eb m\u00ebdha, duke p\u00ebrfshir\u00eb nj\u00eb q\u00eb hedh dyshime se nga vijn\u00eb element\u00ebt tan\u00eb t\u00eb r\u00ebnd\u00eb \u2013 si ari.<\/p>\n\n\n\n
\u201cShp\u00ebrthimi i drit\u00ebs, i studiuar n\u00eb vitin 2022, tani dihet se kishte nj\u00eb yll shp\u00ebrthyes n\u00eb zemr\u00ebn e tij\u201d, than\u00eb studiuesit.<\/p>\n\n\n\n
Por ai shp\u00ebrthim, n\u00eb vetvete, nuk do t\u00eb kishte qen\u00eb i mjaftuesh\u00ebm p\u00ebr t\u00eb ndri\u00e7uar kaq shum\u00eb.<\/p>\n\n\n\n
\u201cTeoria jon\u00eb aktuale thot\u00eb se yje t\u00eb till\u00eb shp\u00ebrthyes, t\u00eb njohur si supernova, prodhojn\u00eb gjithashtu t\u00eb gjith\u00eb element\u00ebt e r\u00ebnd\u00eb n\u00eb univers si ari dhe platini\u201d, sipas studiuesve.<\/p>\n\n\n\n
Por ekipi nuk gjeti asnj\u00eb nga k\u00ebta element\u00eb, duke ngritur pyetje t\u00eb reja se si prodhohen metalet e \u00e7muara.<\/p>\n\n\n\n
Profesoresha, Catherine Heymans e Universitetit t\u00eb Edinburgut dhe Astronomi Royal i Skocis\u00eb, i cili \u00ebsht\u00eb i pavarur nga ekipi hulumtues, tha se rezultatet si k\u00ebto ndihmojn\u00eb p\u00ebr t\u00eb \u00e7uar shkenc\u00ebn p\u00ebrpara.<\/p>\n\n\n\n
Shp\u00ebrthimi u zbulua nga teleskop\u00ebt n\u00eb tetor 2022. Ai erdhi nga nj\u00eb galaktik\u00eb e larg\u00ebt 2,4 miliard\u00eb vite drit\u00eb larg, duke l\u00ebshuar drit\u00eb n\u00eb t\u00eb gjitha frekuencat. Por ishte ve\u00e7an\u00ebrisht intensiv n\u00eb rrezet e tij gama, t\u00eb cilat jan\u00eb nj\u00eb form\u00eb m\u00eb dep\u00ebrtuese e rrezeve X.<\/p>\n\n\n\n
Shp\u00ebrthimi i rrezeve gama zgjati shtat\u00eb minuta dhe ishte aq i fuqish\u00ebm saq\u00eb ishte jasht\u00eb shkall\u00ebs, duke mposhtur instrumentet q\u00eb mund\u00ebsuan zbulimin e tyre.<\/p>\n\n\n\n
T\u00eb dh\u00ebnat treguan se shp\u00ebrthimi ishte 100 her\u00eb m\u00eb i ndritsh\u00ebm se \u00e7do gj\u00eb q\u00eb ishte regjistruar ndonj\u00ebher\u00eb m\u00eb par\u00eb, duke u quajtur n\u00eb mesin e astronom\u00ebve si \u201cBrightest Of All Time\u201d ose B.O.A.T.<\/p>\n\n\n\n
Shp\u00ebrthimet e rrezeve gama lidhen me shp\u00ebrthimin e supernovave, por kjo ishte aq e ndritshme sa nuk mund t\u00eb shpjegohej leht\u00eb.<\/p>\n\n\n\n
\u201cN\u00ebse do t\u00eb ishte nj\u00eb supernova, do t\u00eb duhej t\u00eb kishte qen\u00eb absolutisht e madhe\u201d, sipas teoris\u00eb aktuale.<\/p>\n\n\n\n
Shp\u00ebrthimi ishte aq i ndritsh\u00ebm sa fillimisht i mahniti instrumentet n\u00eb teleskopin hap\u00ebsinor James Webb t\u00eb NASA-s (JWST).<\/p>\n\n\n\n
Shp\u00ebrthime t\u00eb tilla t\u00eb fuqishme llogariten t\u00eb ndodhin nj\u00eb her\u00eb n\u00eb 10,000 vjet.<\/p>\n\n\n\n