Tag: Askar ACL200

Comet C/2023 A3 (Tsuchinshan–ATLAS)

Comet C/2023 A3 (Tsuchinshan–ATLAS) is a long-period comet discovered in early 2023 by the Tsuchinshan Observatory in China and the ATLAS survey project in Hawaii. It has drawn attention for its potential to become a bright object in the sky as it approaches the Sun. The comet’s path took it closest to the Sun (perihelion) in late September 2024, making it visible from Earth, especially in the southern hemisphere, and giving it a spectacular appearance. I was lucky to be in the right place at the right time, and I captured it with two different optical instruments. The comet was very close to the sun, and two tails were visible on this specific day. The primary large tail is made of dust particles, which are frozen in the comet and evaporated by the sun. The secondary tail is on the other hand created by the UV light, which ionizes the gas blown off the comet, and the solar wind carries these ions straight out from the Sun to form the ion tail, which typically glows blue. This is exactly, what is visible on the following picture:

TelescopeAskar ACL200
Aperture50 mm
Focal length200 mm
MountiOptron HEM15
AutoguidingZWO ASI485MC, QHY Mini Guide Scope
CameraZWO 6200MC @0°C
Exposure8x60s, Gain 100, bin 1×1,
Date2024-10-01
LensSigma 40 mm Art
Focal ratio F 1.4
Focal length40 mm
MountTripod
CameraSony A7III astro-modified
ISO1600
Exposure158x5s
Date2024-10-01

Dark Nebula in the constellation Corona Australis

The Dark Nebula in the constellation Corona Australis, also known as the Corona Australis Molecular Cloud, is a dense region of interstellar dust and gas located about 430 light-years from Earth. This dark nebula is notable for its opaque appearance, as it blocks light from stars behind it, creating a stark, shadowy silhouette against the surrounding star field. Within this cloud, young stars are actively forming, and the nebula itself appears to be dotted with faint, reflection nebulae illuminated by these young stars. Its dark, dusty tendrils make it a fascinating example of a star-forming region hidden in shadow, offering a glimpse into the early stages of stellar evolution.

TelescopeAskar ACL200
Aperture50 mm
Focal length200 mm
MountiOptron HEM15
AutoguidingZWO ASI485MC, QHY Mini Guide Scope
CameraZWO 6200MC @0°C
Corrector
Filters
Exposure102x300s, Gain 100, bin 1×1,
Date2024-09-29

Dark nebulae in Taurus

Constellation Taurus is full of deep space gems. Probably everybody knows the Pleiades open cluster. There are many dark nebulae next to it, which I intended to capture during our winter vacation in Flims-Laax. Three and half hours of total exposure revealed 3D structures of the dark clouds floating in space. The darkest cloud on the left side is B 22 Taurus Dark Cloud Complex, the small one on the left B 207 Eagle’s Head, and the central part B 18 Kutner’s Cloud.

TelescopeAskar ACL 200 F4
Aperture50 mm
Focal length200 mm
MountRainbow Astro RST 135
AutoguidingZWO 178MM, QHY Mini Guide Scope
CameraZWO 6200MC @-10°C
Filtersnone
Exposure72x180s, Gain 100, bin 1×1,
Date2024-01-11

IC 2118 Witch Head Nebula IC 2118

The Witch Head Nebula is a striking and eerie interstellar cloud of dust and gas located in the constellation Orion. Its distinct shape, resembling the profile of a witch’s face in profile, is created by the illumination of nearby stars. This nebula spans about 50 light-years across and is primarily composed of hydrogen gas, which glows faintly in the presence of ultraviolet radiation from neighboring stars. The nebula is a site of ongoing star formation, with young, hot stars embedded within its dusty tendrils. Captivating and mysterious, the Witch Head Nebula is a captivating sight in the night sky, sparking the imagination of astronomers and stargazers alike.

TelescopeAskar ACL 200 F4
Aperture50 mm
Focal length200 mm
MountRainbow Astro RST 135
AutoguidingZWO 178MM, QHY Mini Guide Scope
CameraZWO 6200MC @-10°C
Filtersnone
Exposure73x180s, Gain 100, bin 1×1,
Date2024-01-08

Sh2-91 supernova remnant in Cygnus

In my previous project, where I created a mosaic of the Cygnus constellation, I discovered a faint supernova remnant near the star Albireo. Recognizing the significance of this finding, I committed to giving this celestial object more attention. I directed my Askar ACL telescope to these coordinates and gathered additional data over several hours.

Sh2-91, also identified as LBN 147, is a supernova remnant situated close to Albireo. Unlike its more well-known visual neighbor, the Veil Nebula, Sh2-91 is infrequently captured in deep-space photography. According to available literature, this nebula spans 230 light-years in diameter and is approximately 20 thousand years old.

Aware of the complexity of this target, I understood that an extensive integration time was necessary to highlight its intricate structures. Hence, I dedicated seven clear nights to capturing data for this deep-space object, accumulating nearly 14 hours of valuable data.

TelescopeAskar ACL 200 F4
Aperture50 mm
Focal length200 mm
MountRainbow Astro RST 135
AutoguidingZWO 178MM, QHY Mini Guide Scope
CameraZWO 6200MC @-10°C
FiltersAntlia ALP-T Dualband 5nm
Exposure167x300s, Gain 100, bin 1×1,
Date2023-09-15
2023-09-17
2023-09-19
2023-10-04
2023-10-06
2023-10-07
2023-10-08

Cygnus

Cygnus is a prominent constellation in the northern hemisphere’s summer and autumn skies. Known as the “Swan,” it is easily recognizable due to its distinctive shape, which some people interpret as a flying bird with outstretched wings. In Greek mythology, Cygnus is often associated with the story of Zeus and the transformation of his lover, the beautiful mortal named Leda, into a swan.

The constellation Cygnus is home to several interesting celestial objects. One of the most famous is the Northern Cross, a prominent asterism formed by the brightest stars in the constellation. Deneb (upper right corner), is the brightest star in Cygnus.

In addition to stars, Cygnus contains various deep-sky objects. The North America Nebula (NGC 7000) and the Pelican Nebula (IC 5070) are two emission nebulae located in the region of Deneb. These nebulae are often photographed due to their striking shapes, resembling the continent of North America and a pelican, respectively. Moreover, two supernova remnants can be found in this constellation. The Veil Nebula (upper left) knows probably every amateur astrophotographer, but to find out that there is another remnant called LNB 147 (lower left) was a surprise for me. This one deserves more attention, and if the weather allows, I will try to capture more light coming from there.

Cygnus is also traversed by the Milky Way, making it a rich region for observing star clusters, nebulae, and other deep-sky wonders. Overall, the constellation Cygnus holds a special place in both mythology and astronomy, offering stargazers a captivating celestial experience.

The pictures are a mosaic of 3×4 frames. In total, I captured 342 frames, each 5 minutes long (integration time 28 hours 30 minutes), which were taken during 10 nights in August and September. This makes it my biggest astrophotography project so far.

TelescopeAskar ACL 200 F4
Aperture50 mm
Focal length200 mm
MountRainbow Astro RST 135
AutoguidingZWO 178MM, QHY Mini Guide Scope
CameraZWO 6200MC @-10°C
FiltersAntlia ALP-T Dualband 5nm
Exposure342x300s, Gain 100, bin 1×1,
Date2023-09-12
2023-09-15
2023-09-05
2023-09-06
2023-08-23
2023-08-24
2023-08-16
2023-08-21
2023-08-22
2023-08-11
2023-08-22
2023-08-23