Messier 106 or NGC 4258 is a barred spiral galaxy of the Hubble type SBbc in the constellation Canes Venatici. It is estimated to be 23 million light-years away from the Milky Way and has a diameter of about 125,000 light-years.
At this distance, the galaxy is located near several galaxy groups, and depending on the author, it is listed as a member of groups such as the Ursa Major group, the Coma-Sculptor group, the Canes Venatici I group, or the Canes Venatici II group. (Wiki)Messier 106 or NGC 4258 is a barred spiral galaxy of the Hubble type SBbc in the constellation Canes Venatici. It is estimated to be 23 million light-years away from the Milky Way and has a diameter of about 125,000 light-years.
At this distance, the galaxy is located near several galaxy groups, and depending on the author, it is listed as a member of groups such as the Ursa Major group, the Coma-Sculptor group, the Canes Venatici I group, or the Canes Venatici II group. (Wiki)Messier 106 oder NGC 4258 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBbc im Sternbild Canes Venatici. Sie ist schätzungsweise 23 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 125.000 Lichtjahren.
Mit dieser Entfernung liegt die Galaxie in der Umgebung mehrerer Galaxiengruppen, als deren Mitglied die Galaxie je nach Autor gelistet wird, zum Beispiel die Ursa-Major-Gruppe, die Coma-Sculptor-Gruppe, die Canes-Venatici-I-Gruppe oder die Canes-Venatici-II-Gruppe. (Wiki)
M106 GalaxyM106 GalaxyM106 Galaxie
Messier 106 or NGC 4258 is a barred spiral galaxy of the Hubble type SBbc in the constellation Canes Venatici. It is estimated to be 23 million light-years away from the Milky Way and has a diameter of about 125,000 light-years.At this distance, the galaxy is located near several galaxy groups, and depending on the author, it is listed as a member of groups such as the Ursa Major group, the Coma-Sculptor group, the Canes Venatici I group, or the Canes Venatici II group. (Wiki)Messier 106 or NGC 4258 is a barred spiral galaxy of the Hubble type SBbc in the constellation Canes Venatici. It is estimated to be 23 million light-years away from the Milky Way and has a diameter of about 125,000 light-years.
At this distance, the galaxy is located near several galaxy groups, and depending on the author, it is listed as a member of groups such as the Ursa Major group, the Coma-Sculptor group, the Canes Venatici I group, or the Canes Venatici II group. (Wiki)Messier 106 oder NGC 4258 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBbc im Sternbild Canes Venatici. Sie ist schätzungsweise 23 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 125.000 Lichtjahren.
Mit dieser Entfernung liegt die Galaxie in der Umgebung mehrerer Galaxiengruppen, als deren Mitglied die Galaxie je nach Autor gelistet wird, zum Beispiel die Ursa-Major-Gruppe, die Coma-Sculptor-Gruppe, die Canes-Venatici-I-Gruppe oder die Canes-Venatici-II-Gruppe. (Wiki)