IC1805 - The Heart Nebula
Objects
IC 1795, IC 1805, IC1795, IC1805, Sh2-190

Equipment :
Mount:
SkyWatcher EQ-6R Pro GoTo
Telescope:
Skywatcher Esprit 100/550 with Original SW Flattener
Camera:
ZWO ASI071 MC Pro
Guiding telescope:
Skywatcher ED50 APO
Guiding Camera:
ZWO ASI290 MM Mini
Controller:
ZWO ASIAIR
Image Details
Exp. data :
36 x 900 s
Image capture date  :
16. 04. 2020
Observing Site
Nagybörzsöny - Hungary
E18°49'29" ; N47°55'57"
Short Description
(from wikipedia - the free encyclopedia)
The Heart Nebula, IC 1805, Sharpless 2-190, lies some 7500 light years away from Earth and is located in the Perseus Arm of the Galaxy in the constellation Cassiopeia. It was discovered by William Herschel on 3 November 1787.[1] It is an emission nebula showing glowing ionized hydrogen gas and darker dust lanes.[2] The brightest part of the nebula (a knot at its western edge) is separately classified as NGC 896, because it was the first part of the nebula to be discovered. The nebula's intense red output and its morphology are driven by the radiation emanating from a small group of stars near the nebula's center. This open cluster of stars, known as Collinder 26 or Melotte 15, contains a few bright stars nearly 50 times the mass of our Sun, and many more dim stars that are only a fraction of our Sun's mass.