Other Names: Heart Nebula, IC 1805, LBN 654, Collinder 26, Melotte 15, Raab 11, OCL 352
Optics: Borg Astrograph 101ED at f/4.1
Mount: Atlas EQG using The Sky6,
EQMOD,
& MaxPilote Camera: QSI 583WS
Filters: Astrodon Ha 3nm
Exposure: 60 Mins, [6 x 600s] Ha
Accessories: Auto guided with Borg 45ED and Orion Starshoot Auto Guider using Maxim DL guiding
Location: Rodeo, NM
Date: November 15th, 2012
Notes: Processing: Image acquisition with
Maxim DL Pro using
MaxPilote automation
. Image calibration, align, and combine in Maxim DL Pro. Levels, curves, crop and resize in Photoshop.
Calibrated w/30 Darks, 93 Bias, 100 Flats using light box,
CCD temperature was -20C. Image was taken near the Arizona Sky Village near Portal, AZ.
High Res Version:
http://astromarina.zenfolio.com/img/s2/v53/p1385540944-6.jpgHaRGB Version:
http://astromarina.zenfolio.com/p178350886/h52958ab0#h52958ab0Original RGB Version:
http://astromarina.zenfolio.com/p14536770/h5295B386#h5295b386The
Heart Nebula,
IC 1805,
Sh2-190, lies some 7500
light years away from
Earth and is located in the
Perseus Arm of the
Galaxy in the constellation
Cassiopeia. This is an
emission nebula showing glowing gas and darker dust lanes. The nebula is formed by
plasma of ionized
hydrogen and free
electrons.
The very brightest part of this nebula (the knot at the right) is separately classified as
NGC 896, because it was the first part of this nebula to be discovered.
The nebula's intense
red output and its configuration are driven by the radiation emanating from a small group of stars near the nebula's center. This
open cluster of stars known as
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. The cluster used to contain a microquasar that was expelled millions of years ago.