Brza kretanja zvijezda dokazala postojanje crne rupe u obližnjoj galaksiji
Izvor:Reuters
Autor:Ivan Šaravanja
SPACE SCIENCE RESEARCH
epa08381592 An undated handout photo made available by the European Space Agency (ESA) on 24 April 2020 shows giant nebula NGC 2014 and its neighbour NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud (issued 24 April 2020). This image is one of the most photogenic examples of the many turbulent stellar nurseries the NASA/ESA Hubble Space Telescope has observed during its 30-year lifetime. The portrait features the giant nebula NGC 2014 and its neighbour NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way, approximately 163 000 light-years away. EPA/NASA, ESA, and STScI / HANDOUT HANDOUT EDITORIAL USE ONLY/NO SALES
foto NASA, ESA, and STScI / HANDOUT
FotoID: HN:20200424547111
Samo prijavljeni korisnici mogu preuzeti fotografiju u punoj kvaliteti.
WASHINGTON, 7. ožujka 2025. (Hina/Reuters) – Veliki Magellanov oblak patuljasta je galaksija u susjedstvu naše Mliječne staze, vidljiva golim okom s južne hemisfere kao mrlja svjetlosti, a novo istraživanje sada je omogućilo njezino bolje razumijevanje i dokaz da se u njezinom središtu nalazi crna rupa.
Samo prijavljeni korisnici mogu pregledati cijeli sadržaj.