Recently BAS (Bangalore Astronomy Society) and IIA (Indian Institute of Astrophysics) organized a trip to Hanle, the first dark sky reserve of India. A team of 15 astrophotographers and visual observers (9 from Bangalore, 3 from Coimbatore, 1 from Pune, 1 from Delhi and 1 from Kolkatta) took part in this trip. I, my daughter and a friend and fellow astrophotographer Obulichandran joined this group from Coimbatore. I shipped all the heavy equipment like the mount, tripod and counterweights by air cargo and hand carried the optics and cameras by flight. We had planned for 5 nights in Hanle. But due to the delay in retreat of monsoon, we had 4 nights washed out due to clouds, with only one clear night in Hanle. I did some photography in Leh as well on the way back and salvaged a few more pictures. Out of the 14 planned targets, I could only get 4 in full quality. I managed to salvage a few more with low integration times.
I am writing a detailed travelogue documenting the trip. This should go live in a day or two.
Before posting the pictures and exposure details, below is the list of equipment and software used to shoot and process these targets.
Equipment:
EQ6-R Pro German Equatorial Mount
William Optics GT81 APO triplet refractor telescope
William Optics 50mm guide scope
ZWO ASI2600MC Pro cooled colour camera with an APS-C sensor
ZWO ASI224 guide camera
ZWO EAF – Electronic Auto Focuser
Intel NUC Mini PC controlling the equipment
Software:
N.I.N.A for image acquisition (Image composition, slewing and centering the target, auto focus, plate solving, and exposure control)
PHD2 for guiding (through N.I.N.A)
Pixinsight for calibration, stacking and post-processing.
Lightroom and Windows Photo Editor for final touch-ups
First, let me post the 4 good images I managed followed by the average images that I could salvage with lower integration times.
Jelly Fish Nebula (IC 443)
IC 443 (also known as the Jellyfish Nebula and Sharpless 248 (Sh2-248)) is a galactic supernova remnant in the constellation Gemini. Its distance is roughly 5,000 light years from Earth and it is roughly 70 light years in size. NASA’s latest research estimates the age of this supernova remnant to be tens of thousands of years, which aligns with previous work that estimated IC 443 to be about 30,000 years old. IC 443’s true age remains in question, as other scientists have inferred much younger ages of about 3,000 years.
Exposure (2:25 hours total integration time)
Lights - 29 x 300 seconds
Darks - 25
Flats – 25
North American and Pelican Nebulae:
The Pelican Nebula (also known as IC 5070 and IC 5067) is an H II region associated with the North America Nebula in the constellation Cygnus. The gaseous contortions of this emission nebula bear a resemblance to a pelican, giving rise to its name. The Pelican Nebula is located nearby first magnitude star Deneb, and is divided from its more prominent neighbour, the North America Nebula, by a foreground molecular cloud filled with dark dust.
The North America Nebula (NGC 7000 or Caldwell 20) is an emission nebula in the constellation Cygnus, close to Deneb (the tail of the swan and its brightest star). The shape of the nebula resembles that of the continent of North America, complete with a prominent Gulf of Mexico.
The distances to the North America and Pelican nebulae were controversial, because there are few precise methods for determining how far away an HII region lies. Until 2020, most astronomers accepted a value of 2,000 light years, though estimates ranged from 1,500 to 3,000 light years.[10]
But in 2020, the Gaia astrometry spacecraft measured the distances to 395 stars lying within the HII region, giving the North America and Pelican nebulae a distance of 2,590 light years. The entire HII region Sh2-117 is estimated to be 140 light years across, and the North America nebula stretches 90 light years
Exposure (2:51 hours total integration time)
Lights - 57 x 180 seconds
Darks - 25
Flats – 25
The Triangulum Galaxy (M33 / NGC 598):
The Triangulum Galaxy is a spiral galaxy 2.73 million light-years from Earth in the constellation Triangulum. It is catalogued as Messier 33 or NGC 598. With a diameter of 61,100 light-years, the Triangulum Galaxy is the third-largest member of the Local Group of galaxies, behind the Andromeda Galaxy and the Milky Way. It is one of the most distant permanent objects that can be viewed with the naked eye.
The galaxy is the smallest spiral galaxy in the Local Group, and is believed to be a satellite of the Andromeda Galaxy or on its rebound into the latter due to their interactions, velocities, and proximity to one another in the night sky. It also has an H II nucleus.
Exposure (2:18 hours total integration time)
Lights - 46 x 180 seconds
Darks - 25
Flats – 25
The Eastern Veil Nebula (NGC6992):
The Veil Nebula is a cloud of heated and ionized gas and dust in the constellation Cygnus. It constitutes the visible portions of the Cygnus Loop, a supernova remnant, many portions of which have acquired their own individual names and catalogue identifiers. The portion I have shot is identified as the Eastern Veil or NGC6992.
The source supernova was a star 20 times more massive than the Sun which exploded between 10,000 and 20,000 years ago. At the time of explosion, the supernova would have appeared brighter than Venus in the sky, and visible in daytime. The remnants have since expanded to cover an area of the sky roughly 3 degrees in diameter (about 6 times the diameter, and 36 times the area, of the full Moon). While previous distance estimates have ranged from 1200 to 5800 light-years, a recent determination of 2400 light-years is based on direct astrometric measurements.
The red hues in this image are from ionized hydrogen content of gas clouds that emit light in the H-alpha wavelength, while the cyan hues are from oxygen ions.
Exposure (2:00 hours total integration time)
Lights - 24 x 300 seconds
Darks - 25
Flats – 25
Notice the uncanny resemblance to the creature from the movie "Alien"
