IC1805 Heart Nebula, update to 11 hours of exposure time.
The Heart Nebula is an emission nebula with an open star cluster inside and is located in the constellation Cassiopeia in the northern starry sky.
The object is about 6,500 light-years away from us in the Perseus Arm of the Milky Way. The emission nebula, made up of gas clouds and dark dust regions, consists of plasma from ionized hydrogen and free electrons.
The reddish, nebulous areas are illuminated by the stars of the open star cluster. This group consists of several stars with a total mass about 50 times that of the Sun, along with smaller and less bright stars. The cluster included a microquasar that was ejected millions of years ago. (Wiki)IC1805 Heart Nebula, update to 11 hours of exposure time.
The Heart Nebula is an emission nebula with an open star cluster inside and is located in the constellation Cassiopeia in the northern starry sky.
The object is about 6,500 light-years away from us in the Perseus Arm of the Milky Way. The emission nebula, made up of gas clouds and dark dust regions, consists of plasma from ionized hydrogen and free electrons.
The reddish, nebulous areas are illuminated by the stars of the open star cluster. This group consists of several stars with a total mass about 50 times that of the Sun, along with smaller and less bright stars. The cluster included a microquasar that was ejected millions of years ago. (Wiki)IC1805 Herznebel, update auf 11 Stunden Belichtungszeit.
Der Herznebel ist ein Emissionsnebel mit einem offenen Sternhaufen im Inneren und befindet sich im Sternbild Kassiopeia am Nordsternhimmel.
Das Objekt befindet sich etwa 6500 Lichtjahre von uns entfernt im Perseus-Arm der Milchstraße. Der Emissionsnebel aus Gaswolken und dunklen Staubbereichen besteht aus Plasma von ionisiertem Wasserstoff und freien Elektronen.
Die rötlichen, nebeligen Partien werden von den Sternen des offenen Sternhaufens beleuchtet. Diese Gruppe besteht aus mehreren Sternen mit insgesamt etwa 50-facher Masse der Sonne und weiteren kleineren und weniger hellen Sternen. Der Haufen schloss einen Mikroquasar ein, welcher vor Millionen von Jahren ausgestoßen wurde. (Wiki)
IC1805 Heart NebulaIC1805 Heart NebulaIC1805 Herznebel
IC1805 Heart Nebula, update to 11 hours of exposure time.The Heart Nebula is an emission nebula with an open star cluster inside and is located in the constellation Cassiopeia in the northern starry sky.
The object is about 6,500 light-years away from us in the Perseus Arm of the Milky Way. The emission nebula, made up of gas clouds and dark dust regions, consists of plasma from ionized hydrogen and free electrons.
The reddish, nebulous areas are illuminated by the stars of the open star cluster. This group consists of several stars with a total mass about 50 times that of the Sun, along with smaller and less bright stars. The cluster included a microquasar that was ejected millions of years ago. (Wiki)IC1805 Heart Nebula, update to 11 hours of exposure time.
The Heart Nebula is an emission nebula with an open star cluster inside and is located in the constellation Cassiopeia in the northern starry sky.
The object is about 6,500 light-years away from us in the Perseus Arm of the Milky Way. The emission nebula, made up of gas clouds and dark dust regions, consists of plasma from ionized hydrogen and free electrons.
The reddish, nebulous areas are illuminated by the stars of the open star cluster. This group consists of several stars with a total mass about 50 times that of the Sun, along with smaller and less bright stars. The cluster included a microquasar that was ejected millions of years ago. (Wiki)IC1805 Herznebel, update auf 11 Stunden Belichtungszeit.
Der Herznebel ist ein Emissionsnebel mit einem offenen Sternhaufen im Inneren und befindet sich im Sternbild Kassiopeia am Nordsternhimmel.
Das Objekt befindet sich etwa 6500 Lichtjahre von uns entfernt im Perseus-Arm der Milchstraße. Der Emissionsnebel aus Gaswolken und dunklen Staubbereichen besteht aus Plasma von ionisiertem Wasserstoff und freien Elektronen.
Die rötlichen, nebeligen Partien werden von den Sternen des offenen Sternhaufens beleuchtet. Diese Gruppe besteht aus mehreren Sternen mit insgesamt etwa 50-facher Masse der Sonne und weiteren kleineren und weniger hellen Sternen. Der Haufen schloss einen Mikroquasar ein, welcher vor Millionen von Jahren ausgestoßen wurde. (Wiki)