Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  HD14817  ·  HD15069  ·  HD15238  ·  HD15239  ·  HD15250  ·  HD15382  ·  HD15522  ·  HD15557  ·  HD15558  ·  HD15570  ·  HD15629  ·  HD15665  ·  HD15785  ·  HD15851  ·  HD16183  ·  HD16429  ·  HD236966  ·  IC 1795  ·  IC 1805  ·  LBN 645  ·  LBN 646  ·  LBN 647  ·  LBN 648  ·  LBN 650  ·  LBN 654  ·  LBN 655  ·  LBN 656  ·  LBN 657  ·  LBN 658  ·  LDN 1359  ·  And 16 more.
Getting plate-solving status, please wait...
IC 1805 The Heart Nebula, George  Yendrey
Powered byPixInsight

IC 1805 The Heart Nebula

Getting plate-solving status, please wait...
IC 1805 The Heart Nebula, George  Yendrey
Powered byPixInsight

IC 1805 The Heart Nebula

Equipment

Loading...

Acquisition details

Loading...

Description

This is my 3rd targeting of The Heart Nebula and the first time as a monochromej/Narrowband imaging session.  This is a fitting target for personal reasons (for me) - it is soon to be my wife's birthday and this Nebula symbolizes what she means to me -  she is my Heart and my Light...

This was captured for three nights of imaging; the first being a bit short as I worked through the sensor tilt adjustment of my ZWO ASI2600MM-P.

Lum: 52 x 120s
Ha:    50 x 300s
Sii:     40 x 300s
Oiii:    34 x 300s

Post processing was in PixInsight with the Hubble/SHO palette.  After cropping and DBE, I split the narrow band images into a Starless version, and Stars, for separate post processing.  This allows processing to go after Nebula details relatively aggressively without having to be concerned about star bloating.


The Heart NebulaIC 1805Sharpless 2-190, is 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.=10.5px  It is an emission nebula showing glowing ionized hydrogen gas and darker dust lanes.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.

More information on this object can be found here: Heart Nebula - Wikipedia

Comments

Sky plot

Sky plot

Histogram

IC 1805 The Heart Nebula, George  Yendrey