Month: October 2024

NGC 7293 Helix Nebula

October 5, 2024
Planetary nebula
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The Helix Nebula, also known as NGC 7293, is a large planetary nebula located in the constellation Aquarius, about 650 light-years away from Earth. Often called the “Eye of God” due to its striking appearance, it features a bright, donut-shaped ring of gas and dust surrounding a central, faint white dwarf—the remnant core of a dying star. This nebula formed when the star shed its outer layers in the final stages of its life, creating the colorful halo we see today. It spans about 2.5 light-years and is one of the closest planetary nebulae to Earth, making it a popular object of study in astronomy.

TelescopeNewtonian 200/800 mm
Aperture200 mm
Focal length800 mm
MountSkywatcher EQ6R
AutoguidingZWO 174MM, WO 40/200 mm
CameraZWO 071MC @-0°C
CorrectorGPU
FiltersAntlia DualBand
Exposure131x180s, Gain 100, bin 1×1,
Date2024-10-05

NGC 104 Globular Cluster

October 4, 2024
Globular cluster
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NGC 104, also known as 47 Tucanae, is a massive globular cluster located in the constellation Tucana, about 13,000 light-years from Earth. It’s one of the brightest and most massive globular clusters in the Milky Way, containing several million stars densely packed within a roughly spherical shape. With a diameter of around 120 light-years, NGC 104 is easily visible to the naked eye in the southern hemisphere. The cluster is rich in older stars, giving it a golden hue, and is known for its dense core, where stars are packed thousands of times closer together than in our solar neighborhood.

TelescopeNewtonian 200/800 mm
Aperture200 mm
Focal length800 mm
MountSkywatcher EQ6R
AutoguidingZWO 174MM, WO 40/200 mm
CameraZWO 071MC @-10°C
CorrectorGPU
Filters–
Exposure47x180s, Gain 100, bin 1×1,
Date2024-10-04

IC 2177 Seagull Nebula

October 4, 2024
H II nebula
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The Seagull Nebula, designated IC 2177, is a large emission nebula located on the border between the constellations Monoceros and Canis Major, about 3,650 light-years from Earth. Shaped somewhat like a bird in flight, this nebula spans approximately 100 light-years across and consists of a combination of glowing gas and dark dust clouds. The vibrant colors are produced as young, hot stars energize surrounding hydrogen gas, causing it to emit a reddish glow. IC 2177 is part of a larger complex of nebulae and star-forming regions, making it an active area for the birth of new stars and a popular subject for both amateur and professional astrophotographers.

TelescopeSkywatcher Esprit 100ED
Aperture100 mm
Focal length550 mm
MountRainbow Astro RST135
AutoguidingZWO 178MM, QHY Mini Guide Scope
CameraZWO ASI2600MM @0°C
CorrectorSkywatcher flattener
FiltersAntlia Ha OIII SII
Exposure106x300s, Gain 100, bin 1×1,
Date2024-10-04

M78 Nebula

October 3, 2024
Reflection nebula
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The M78 Nebula, also known as Messier 78, is a bright reflection nebula located in the constellation Orion, about 1,350 light-years from Earth. Known for its striking blue color, M78 is illuminated by the light of young, hot stars embedded within it. The nebula’s dust particles reflect this starlight, creating a luminous glow that highlights its wispy clouds and dark lanes of dust. M78 is one of the brightest reflection nebulae in the sky and is a fascinating region of active star formation, where new stars continue to emerge within dense pockets of gas and dust.

TelescopeNewtonian 200/800 mm
Aperture200 mm
Focal length800 mm
MountSkywatcher EQ6R
AutoguidingZWO 174MM, WO 40/200 mm
CameraZWO 071MC @-10°C
CorrectorGPU
Filters–
Exposure200x180s, Gain 100, bin 1×1,
Date2024-10-03

M42 Orion Nebula

October 2, 2024
H II nebula
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The Orion Nebula, also known as M42 or NGC 1976, is a massive and bright emission nebula located in the constellation Orion, about 1,344 light-years away from Earth. It spans roughly 24 light-years across and is one of the most active star-forming regions in our galaxy, making it a vivid nursery for new stars and planetary systems. Its intense, colorful glow is due to ultraviolet radiation from young, hot stars within, which ionizes surrounding gas, causing it to shine. Visible even to the naked eye, M42 is one of the most studied and photographed nebulae, offering insights into the processes of stellar and planetary formation.

TelescopeSkywatcher Esprit 100ED
Aperture100 mm
Focal length550 mm
MountRainbow Astro RST135
AutoguidingZWO 178MM, QHY Mini Guide Scope
CameraZWO ASI2600MM @0°C
CorrectorSkywatcher flattener
FiltersAntlia HaRGB
Exposure232x120s, Gain 100, bin 1×1,
Date2024-10-02

Lagoon Nebula (M8) and Trifid Nebula (M20)

October 1, 2024
H II nebulaReflection nebula
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The Lagoon Nebula (M8) and the Trifid Nebula (M20) are two iconic star-forming regions in the constellation Sagittarius, located approximately 4,100 and 5,200 light-years from Earth, respectively.

The Lagoon Nebula (right) is a vast emission nebula filled with glowing hydrogen gas, creating a reddish hue. Spanning about 110 light-years across, it’s a region rich with young stars and dense, dark clouds of gas and dust, where new stars continue to form. The Lagoon’s large, bright structure and open star cluster make it a prominent and popular sight in the Milky Way.

The Trifid Nebula (left) is known for its unique appearance, where dark dust lanes divide its central region into three distinct lobes, giving it a “trifid” or “three-part” look. The Trifid features a combination of reddish emission nebula, blue reflection nebula, and dark nebula, creating a beautiful, multicolored display. Together, the Lagoon and Trifid nebulae offer a stunning view of diverse nebular activity and star formation.

TelescopeSkywatcher Esprit 100ED
Aperture100 mm
Focal length550 mm
MountRainbow Astro RST135
AutoguidingZWO 178MM, QHY Mini Guide Scope
CameraZWO 2600MM @-10°C
CorrectorSkywatcher flattener
FiltersAntlia HaRGB
Exposure127x180s, Gain 100, bin 1×1,
Date2024-10-01

Comet C/2023 A3 (Tsuchinshan–ATLAS)

October 1, 2024
Solar system
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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