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AstroOtus

@astrootus.bsky.social

I See All Astronomy Astrophotography Space stuff Lost in Space

121 Followers  |  241 Following  |  23 Posts  |  Joined: 26.11.2024  |  2.4301

Latest posts by astrootus.bsky.social on Bluesky

Post image

πŸ“‘ El gran radiotelescopio de 40 metros del observatorio de Yebes, bajo la mirada de la galaxia de AndrΓ³meda y las mΓ‘s pequeΓ±as, M110 y M32.
Entre tormentas y contaminaciΓ³n lumΓ­nica, lleguΓ© a la localizaciΓ³n sin saber si podrΓ­a capturar la imagen que tenΓ­a en mente.

06.07.2025 15:57 β€” πŸ‘ 5    πŸ” 2    πŸ’¬ 1    πŸ“Œ 0
Preview
The Iris Nebula This is NGC 7023, a reflection nebula located in the constellation of Cepheus. This image was automatically captured in the early hours of the morning using the Vaonis Vespera II telescope, exposing f...

com.xipteras.org/Astroimaging...

11.07.2025 14:34 β€” πŸ‘ 1    πŸ” 1    πŸ’¬ 0    πŸ“Œ 0
An unusual galaxy is shown that appears lens-like in overall shape yet has various rings of stars around the center. Please see the explanation for more detailed information.

An unusual galaxy is shown that appears lens-like in overall shape yet has various rings of stars around the center. Please see the explanation for more detailed information.

πŸ”­ NGC 2685: The Helix Galaxy

Image Credit & Copyright: Stefan Thrun

apod.nasa.gov/apod/ap25071...

14.07.2025 08:00 β€” πŸ‘ 151    πŸ” 36    πŸ’¬ 1    πŸ“Œ 2
Messier 14 – Metal-Poor Globular Cluster in Ophiuchus

Messier 14 (NGC 6402) is a moderately concentrated globular cluster located in the constellation Ophiuchus, approximately 30,300 light-years from Earth. With an estimated age of ~13.25 billion years, it is a representative example of the old, metal-poor stellar populations that inhabit the Galactic halo.

The cluster spans about 100 light-years in diameter and contains several hundred thousand Population II stars. Its low metallicity ([Fe/H] β‰ˆ –1.28) reflects a formation epoch early in the history of the Milky Way. M14 is classified as a Shapley-Sawyer Class VIII cluster and exhibits a relatively diffuse outer halo surrounding a dense core.

More than 70 RR Lyrae variable stars have been identified within the cluster, making it useful for refining distance measurements through the period-luminosity relation. In 1938, a nova event was recorded on photographic plates, one of the few confirmed nova eruptions within a globular cluster.

Imaging Details:

Telescope: Celestron EdgeHD 8"
Camera: ZWO ASI1600MM Pro
Filters: ZWO Red, Green, Blue (36mm)
Exposure:
Red: 96 Γ— 60 sec
Green: 90 Γ— 60 sec
Blue: 90 Γ— 60 sec
Mount: Sky-Watcher EQ6-R Pro
Software: NINA (acquisition), PixInsight (processing)

This image resolves the core and extended halo of M14 in broadband RGB. The cluster’s structure and variable population contribute to studies of globular cluster dynamics, distance calibration, and the early chemical evolution of the Milky Way.

Messier 14 – Metal-Poor Globular Cluster in Ophiuchus Messier 14 (NGC 6402) is a moderately concentrated globular cluster located in the constellation Ophiuchus, approximately 30,300 light-years from Earth. With an estimated age of ~13.25 billion years, it is a representative example of the old, metal-poor stellar populations that inhabit the Galactic halo. The cluster spans about 100 light-years in diameter and contains several hundred thousand Population II stars. Its low metallicity ([Fe/H] β‰ˆ –1.28) reflects a formation epoch early in the history of the Milky Way. M14 is classified as a Shapley-Sawyer Class VIII cluster and exhibits a relatively diffuse outer halo surrounding a dense core. More than 70 RR Lyrae variable stars have been identified within the cluster, making it useful for refining distance measurements through the period-luminosity relation. In 1938, a nova event was recorded on photographic plates, one of the few confirmed nova eruptions within a globular cluster. Imaging Details: Telescope: Celestron EdgeHD 8" Camera: ZWO ASI1600MM Pro Filters: ZWO Red, Green, Blue (36mm) Exposure: Red: 96 Γ— 60 sec Green: 90 Γ— 60 sec Blue: 90 Γ— 60 sec Mount: Sky-Watcher EQ6-R Pro Software: NINA (acquisition), PixInsight (processing) This image resolves the core and extended halo of M14 in broadband RGB. The cluster’s structure and variable population contribute to studies of globular cluster dynamics, distance calibration, and the early chemical evolution of the Milky Way.

Messier 14 is a moderately concentrated globular cluster located in the constellation Ophiuchus, approximately 30,300 ly from Earth. The cluster spans about 100 light-years in diameter and has an estimated age of 13.25 million years. #astrophotography @kat-astro-bot.bsky.social

14.07.2025 00:09 β€” πŸ‘ 55    πŸ” 7    πŸ’¬ 2    πŸ“Œ 0

Wow! Check out the gorgeous movie that the Parker Solar Probe made on Christmas Day!πŸŽ„β˜ƒοΈπŸŽπŸ€Ά

It was travelling past the Sun at 430,000 mph (i.e London to New York in 30sec) at a distance of only 9.85 Sun-Radii above the solar surface. Temperatures were > 1000℃ πŸ₯΅
πŸ”­πŸ§ͺ

πŸŽ₯: www.youtube.com/watch?v=k1dT...

11.07.2025 14:13 β€” πŸ‘ 88    πŸ” 20    πŸ’¬ 2    πŸ“Œ 1
Image full version:   https://www.astrobin.com/full/gza49l/B/

Description:   https://www.astrobin.com/gza49l/B/

Dates sessions
May 7, 2021
June 10, 2022
March 18 - 19, 2024 

Integration: 5h 1β€² 30β€³ 

Filters Used:
Optolong L-Pro 2"
Radian Triad Ultra 2"

Image full version: https://www.astrobin.com/full/gza49l/B/ Description: https://www.astrobin.com/gza49l/B/ Dates sessions May 7, 2021 June 10, 2022 March 18 - 19, 2024 Integration: 5h 1β€² 30β€³ Filters Used: Optolong L-Pro 2" Radian Triad Ultra 2"

πŸ”­M 51-Whirlpool GalaxyπŸ”­ Is located between 21-31 M l-y from Earth in the constellation Canes Venatici. Overall is about 88% the size of the Milky Way and estimated 400 M y old.
The companion galaxy is NGC 5195, has been interacting for million years.
www.astrobin.com/full/gza49l/B/ #Galaxy #Space

14.07.2025 13:11 β€” πŸ‘ 0    πŸ” 0    πŸ’¬ 0    πŸ“Œ 0
A clumpy galaxy, possibly merging from the Galaxy Zoo: Hubble project, classified by 125 volunteers.

A clumpy galaxy, possibly merging from the Galaxy Zoo: Hubble project, classified by 125 volunteers.

A clumpy galaxy, possibly merging, observed with the Hubble Space Telescope in the AEGIS survey.

It is at redshift 0.75 (lookback time 6.78 billion years) with coordinates (214.56647, 52.68451).

125 volunteers classified this galaxy in Galaxy Zoo: Hubble.

14.07.2025 12:42 β€” πŸ‘ 19    πŸ” 2    πŸ’¬ 0    πŸ“Œ 0
Draco Triplet galactic group.

Draco Triplet galactic group.

The Draco Triplet, in the constellation (you guessed it) Draco! The spiral galaxy at the top (NGC 5986) is about a third larger than our Milky Way and 140 million light years distant! Image details on my Astrobin page at app.astrobin.com/i/jccmmy #astrophotography #astronomy

08.06.2025 22:38 β€” πŸ‘ 112    πŸ” 15    πŸ’¬ 2    πŸ“Œ 1
NGC 6752 – Globular Cluster in Pavo

One of the brightest and nearest globular clusters in our galaxy, NGC 6752 lies roughly 13,000 light-years away in the constellation Pavo. This dense sphere of ancient stars is estimated to be over 11 billion years old and contains multiple stellar populations, including blue stragglers and millisecond pulsarsβ€”signposts of complex internal dynamics and stellar evolution.

Captured using RGB filters, this image reveals the dense core and surrounding halo of stars, tightly packed into a cluster only ~100 light-years across. NGC 6752 is a post-core-collapse cluster, and its high central concentration is evident even at modest image scale.

Acquisition Details
πŸ”΄ Red: 33 Γ— 180s
🟒 Green: 31 Γ— 180s
πŸ”΅ Blue: 28 Γ— 180s
Total Integration: 5 hours

Equipment
β€’ Telescope: Celestron EdgeHD 8"
β€’ Camera: ZWO ASI1600MM Pro
β€’ Mount: Sky-Watcher EQ6-R Pro
β€’ Filters: ZWO 36mm RGB
β€’ Accessories: Primaluce Lab EAGLE5S, ECCO 2, ESATTO 2", ZWO EFW 7Γ—36mm, ZWO OAG-L
β€’ Software: NINA, PixInsight

Visible from the Southern Hemisphere during winter months, NGC 6752 sits near the bright star Peacock and is a rewarding target for both visual observation and resolved stellar imaging.

NGC 6752 – Globular Cluster in Pavo One of the brightest and nearest globular clusters in our galaxy, NGC 6752 lies roughly 13,000 light-years away in the constellation Pavo. This dense sphere of ancient stars is estimated to be over 11 billion years old and contains multiple stellar populations, including blue stragglers and millisecond pulsarsβ€”signposts of complex internal dynamics and stellar evolution. Captured using RGB filters, this image reveals the dense core and surrounding halo of stars, tightly packed into a cluster only ~100 light-years across. NGC 6752 is a post-core-collapse cluster, and its high central concentration is evident even at modest image scale. Acquisition Details πŸ”΄ Red: 33 Γ— 180s 🟒 Green: 31 Γ— 180s πŸ”΅ Blue: 28 Γ— 180s Total Integration: 5 hours Equipment β€’ Telescope: Celestron EdgeHD 8" β€’ Camera: ZWO ASI1600MM Pro β€’ Mount: Sky-Watcher EQ6-R Pro β€’ Filters: ZWO 36mm RGB β€’ Accessories: Primaluce Lab EAGLE5S, ECCO 2, ESATTO 2", ZWO EFW 7Γ—36mm, ZWO OAG-L β€’ Software: NINA, PixInsight Visible from the Southern Hemisphere during winter months, NGC 6752 sits near the bright star Peacock and is a rewarding target for both visual observation and resolved stellar imaging.

This is NGC6752, one of the brightest and nearest globular clusters to us at 13,000ly away. Working on RCW58 that sets at 11:30pm local, so I hopped over to this nice cluster for the second half of the night and got about 4.5 hours on it. #astrophotography
@kat-astro-bot.bsky.social

09.06.2025 10:32 β€” πŸ‘ 58    πŸ” 8    πŸ’¬ 1    πŸ“Œ 0
A starfield is shown with many stars and several faint light brown dust clouds. In the center is a large cloud with brown dust and gas shells lined in blue. Please see the explanation for more detailed information.

A starfield is shown with many stars and several faint light brown dust clouds. In the center is a large cloud with brown dust and gas shells lined in blue. Please see the explanation for more detailed information.

πŸ”­ Between Scylla and Charybdis: A Double Cosmic Discovery

Image Credit: M. Drechsler, Y. Sainty, A. Soto, N. Martino, L. Leroux-Gere, S. Khallouqui, & A. Kaeouach; Text: Ogetay Kayali (Michigan Tech U.)

apod.nasa.gov/apod/ap25060...

09.06.2025 08:00 β€” πŸ‘ 152    πŸ” 38    πŸ’¬ 2    πŸ“Œ 3
Post image Post image

First light under the Sun with the solar filter on my new Vespera 2! β˜€οΈπŸ”­ A few tiny #sunspots are visible on the Earth-facing sideβ€”but they’re really small. #SolarImaging #smarttelescope #Vespera2

09.06.2025 12:54 β€” πŸ‘ 14    πŸ” 2    πŸ’¬ 3    πŸ“Œ 0
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Helix Nebula.
Reprocesado en Siril de Γ©sta imagen obtenida el aΓ±o pasado con el Seestar s50 de 30' de exposiciΓ³n. Editada en Gimp.
El ojo de Sauron en el cielo...
#Astronomy #Astrophotography #Astronomia #Astrofotografia

09.06.2025 13:32 β€” πŸ‘ 7    πŸ” 4    πŸ’¬ 1    πŸ“Œ 0

there’s just something so magical about the universe… πŸ₯Ήβœ¨

09.06.2025 00:10 β€” πŸ‘ 140    πŸ” 19    πŸ’¬ 2    πŸ“Œ 1
A barred spiral galaxy from the Galaxy Zoo 2 project, classified by 39 volunteers.

A barred spiral galaxy from the Galaxy Zoo 2 project, classified by 39 volunteers.

A barred spiral galaxy, observed with the Apache Point 2.5m Telescope in the SDSS survey.

It is at redshift 0.039 (lookback time 549.7 million years) with coordinates (237.74329, 33.86752).

39 volunteers classified this galaxy in Galaxy Zoo 2.

09.06.2025 08:28 β€” πŸ‘ 81    πŸ” 9    πŸ’¬ 0    πŸ“Œ 0
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The Eagle Nebula! This is one of the most imaged objects in the night sky. In the center is the pillars of creation. I hope you enjoy! #science #space #universe #astronomy #astrophotography @kat-astro-bot.bsky.social

09.06.2025 04:50 β€” πŸ‘ 131    πŸ” 17    πŸ’¬ 4    πŸ“Œ 0
Preview
Did our local supermassive black hole recently eat its little sibling? Indirect evidence suggests a smaller black hole orbited the much, much larger one

So, did our local supermassive monster black hole eat a slightly smaller but still quite huge black hole some time in the cosmically recent past?

Actually, yeah, maybe!

badastronomy.beehiiv.com/p/did-our-lo...

πŸ”­ πŸ§ͺ

09.06.2025 14:33 β€” πŸ‘ 264    πŸ” 36    πŸ’¬ 11    πŸ“Œ 4
COSMOS-Web NIRCam mosaic (upper left) with zoom-ins to the region surrounding the COSMOS-Web Ring (upper right). This image covers more than 800,000 galaxies across the universe.

COSMOS-Web NIRCam mosaic (upper left) with zoom-ins to the region surrounding the COSMOS-Web Ring (upper right). This image covers more than 800,000 galaxies across the universe.

The new COSMOS-Web survey provides an unprecedented view of the universe, combing both breadth and depth.

It includes detailed information about 800,000 galaxies spanning more than 75% of cosmic history. And you can browse through it yourself online. πŸ§ͺπŸ”­

cosmos.astro.caltech.edu/news/87

09.06.2025 15:04 β€” πŸ‘ 31    πŸ” 7    πŸ’¬ 1    πŸ“Œ 0
The comet sessions was done between October 31 and November 2, 2024.
This image comes from the last day session.

For details follow the links below

Session October 31, 2024
https://www.astrobin.com/bxcdab/

Session November 1, 2024
https://www.astrobin.com/3lx1pa/D/

Session November 2, 2024
https://www.astrobin.com/6egucs/D/

The comet sessions was done between October 31 and November 2, 2024. This image comes from the last day session. For details follow the links below Session October 31, 2024 https://www.astrobin.com/bxcdab/ Session November 1, 2024 https://www.astrobin.com/3lx1pa/D/ Session November 2, 2024 https://www.astrobin.com/6egucs/D/

β˜„οΈComet/2023 A3 Tsuchinshan-ATLASβ˜„οΈ
November 2, 2024 18:43pm-19:22pm
Session 34 frames x 60 sec.
Comet originating from the Oort Cloud.
Closest approach to Earth was on October 12, 2024.
astrobin.com/full/6egucs/D/
#Astrophotography #Space #Astronomy #Comet

09.06.2025 15:19 β€” πŸ‘ 1    πŸ” 0    πŸ’¬ 0    πŸ“Œ 0
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Streamlined Shapes

The objective of this observation is to observe streamlined forms. This scene is also avaiable in Context Camera imagery data.

ID: ESP_076000_2115
date: 13 October 2022
altitude: 290 km

uahirise.org/hipod/ESP_07...
NASA/JPL-Caltech/University of Arizona
#Mars #science

10.05.2025 14:10 β€” πŸ‘ 60    πŸ” 9    πŸ’¬ 0    πŸ“Œ 2
looking out over a natural flat rock shell towards a small hill. There are some clouds that are being silouetted against the bright red and green aurora

looking out over a natural flat rock shell towards a small hill. There are some clouds that are being silouetted against the bright red and green aurora

If you remember, there was loads of places around the world - even at higher latitudes (reported as high as Sydney) that saw the night sky dazzle in reds, green, soft purples and pinks.

That's our magnetosphere protecting us from the jerk Sun.

Sean O'Riordan took this awesome image from Tasmania.

09.05.2025 23:23 β€” πŸ‘ 59    πŸ” 9    πŸ’¬ 2    πŸ“Œ 0
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#Lines of stars and meteors as the Earth rotates under them for the #BlueSkyArtShow. I discovered later that the planet was passing through three meteor showers at the time.

#StormHour #PhotoHour #PhotographersOfBluesky #PhotographersUnited #EastCoastKin #photography #longexposure

10.05.2025 15:08 β€” πŸ‘ 95    πŸ” 11    πŸ’¬ 3    πŸ“Œ 1
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Good fun yesterday reintroducing legendary visual astronomy observer Stephen O'Meara to Harvard's Alvan Clark refractor telescope

09.05.2025 21:31 β€” πŸ‘ 160    πŸ” 5    πŸ’¬ 7    πŸ“Œ 1
Two images of the sun in hydrogen alpha.  The left image was taken at 11:00 and the right at 16:00.  Both disks show prominences at the edge of the disk and filaments on the solar disk.  Comparison of the two images shows changes in the prominences over 5 hours.

Two images of the sun in hydrogen alpha. The left image was taken at 11:00 and the right at 16:00. Both disks show prominences at the edge of the disk and filaments on the solar disk. Comparison of the two images shows changes in the prominences over 5 hours.

Two h-alpha images of the Sun taken today 5 hours apart, showing changes in the prominences. Coronado SolarMax πŸ”­, Touptek 585M camera, stacked in AstroSurface, coloured, prominences boosted and solar disks inverted using Solar Toolbox in PixInsight. #astrophotography

10.05.2025 15:41 β€” πŸ‘ 30    πŸ” 2    πŸ’¬ 3    πŸ“Œ 0
This release features two composite images of a long, thin, cosmic structure. With the structure's vertical orientation, seemingly fragile dimensions, and pale grey color against the blackness of space, the images resemble medical X-rays of a long, thin, bone. The main image shows the structure in its entirety. The inset image is an annotated close-up highlighting an apparent fracture in the bone-like structure.

The structure, called G359.13, or "The Snake", is a Galactic Center Filament. These filament formations are threaded by parallel magnetic fields, and spiraling, energized particles. The particles cause radio waves, which can be detected by radio arrays, in this case by the MeerKAT array in South Africa.

In the first composite image, the largely straight filament stretches from the top to the bottom of the vertical frame. At each end of the grey filament is a hazy grey cloud. The only color in the image is neon blue, found in a few specks which dot the blackness surrounding the structure. The blue represents X-rays seen by NASA's Chandra X-ray Observatory. 

In the annotated close-up, one such speck appears to be interacting with the structure itself. This is a fast-moving, rapidly spinning neutron star, otherwise known as a pulsar. Astronomers believe that this pulsar has struck the filament halfway down its length, distorting the magnetic field and radio signal. 

In both images, this distortion resembles a small break, or spur, in the bone-like filament.

This release features two composite images of a long, thin, cosmic structure. With the structure's vertical orientation, seemingly fragile dimensions, and pale grey color against the blackness of space, the images resemble medical X-rays of a long, thin, bone. The main image shows the structure in its entirety. The inset image is an annotated close-up highlighting an apparent fracture in the bone-like structure. The structure, called G359.13, or "The Snake", is a Galactic Center Filament. These filament formations are threaded by parallel magnetic fields, and spiraling, energized particles. The particles cause radio waves, which can be detected by radio arrays, in this case by the MeerKAT array in South Africa. In the first composite image, the largely straight filament stretches from the top to the bottom of the vertical frame. At each end of the grey filament is a hazy grey cloud. The only color in the image is neon blue, found in a few specks which dot the blackness surrounding the structure. The blue represents X-rays seen by NASA's Chandra X-ray Observatory. In the annotated close-up, one such speck appears to be interacting with the structure itself. This is a fast-moving, rapidly spinning neutron star, otherwise known as a pulsar. Astronomers believe that this pulsar has struck the filament halfway down its length, distorting the magnetic field and radio signal. In both images, this distortion resembles a small break, or spur, in the bone-like filament.

Something punched a celestial snake in the gut.

Radio images show the center of our galaxy is full of long, puzzling magnetic "snakes." This one has an unusual kink in it--apparently from where it was smacked by a pulsar racing by at nearly 1000 km/sec. πŸ§ͺπŸ”­

chandra.harvard.edu/photo/2025/b...

09.05.2025 17:46 β€” πŸ‘ 429    πŸ” 64    πŸ’¬ 22    πŸ“Œ 8
Description:  https://www.astrobin.com/9f7315/0/
Full resolution; https://www.astrobin.com/full/9f7315/0/
Dates:  Aug. 22 - 23, 2023  Sept. 7, 2023 
Frames: Optolong L-Pro 2": 307Γ—35β€³(2h 59β€² 5β€³) ISO2000 
Integration: 2h 59β€² 5β€³

Description: https://www.astrobin.com/9f7315/0/ Full resolution; https://www.astrobin.com/full/9f7315/0/ Dates: Aug. 22 - 23, 2023 Sept. 7, 2023 Frames: Optolong L-Pro 2": 307Γ—35β€³(2h 59β€² 5β€³) ISO2000 Integration: 2h 59β€² 5β€³

πŸ”­NGC7023-Iris NebulaπŸ”­Is a bright reflection nebula illuminated by a +7.4 star HD 200775, located in the constellation Cepheus. The bluish light from the star is scattered off dust grains in the nebula, giving its distinctive color.
www.astrobin.com/full/9f7315/0/
#Astrophotography #ReflectionNebula

10.05.2025 15:42 β€” πŸ‘ 4    πŸ” 0    πŸ’¬ 0    πŸ“Œ 0
Preview
M 97 - M 108 The Owl Nebula and Surfboard Galaxy - AstroBin M 97 - M 108Β  Owl Nebula and Surfboard Galaxy Messier 97, also known as the Owl Nebula, is a famous planetary nebula located in Ursa Major constellation. The nebula lies at a distance of 2,030 light ...

www.astrobin.com/full/fze5lr/...

23.04.2025 10:23 β€” πŸ‘ 2    πŸ” 0    πŸ’¬ 0    πŸ“Œ 0
Dates: Feb. 10, 2021   April 1, 2021  May 25 - 27, 2021 May 31, 2021 
Filters: Optolong L-Pro 2"  Optolong L-eNhance 2" Optolong L-eXtreme 2"
Integration: 10h 12β€² 30β€³

Dates: Feb. 10, 2021 April 1, 2021 May 25 - 27, 2021 May 31, 2021 Filters: Optolong L-Pro 2" Optolong L-eNhance 2" Optolong L-eXtreme 2" Integration: 10h 12β€² 30β€³

πŸ”­M 97-The Owl NebulaπŸ”­Is located in Ursa Major constellation. Lies at a 2,030 l-y from Earth. The nebula formed when a dying Sun-like star ran out of hydrogen fuel, collapsed and ejected its outer envelope producing the nebula’s glow.
astrobin.com/full/fze5lr/B
#PlanetaryNebula

23.04.2025 10:23 β€” πŸ‘ 3    πŸ” 0    πŸ’¬ 1    πŸ“Œ 0
Post image

πŸ”­NGC4490 Cocoon GalaxyπŸ”­Is the closest interacting/merging galactic system located 24MM ly from Earth in the constellation of Canes Venatici, had made their closest approach and now are rushing away from each other.
astrobin.com/full/intcxi/B/
#Astrophotography #Space #Astronomy #Galaxy

06.04.2025 09:09 β€” πŸ‘ 9    πŸ” 1    πŸ’¬ 0    πŸ“Œ 0
The Seagull Nebula in the Hubble SHO palette just over 6 hours of total integration. Scope - William Optics RedCat 71. Camera - Atikone 6.0. Filters - Antlia 3nm Ha, Oiii & Sii.

The Seagull Nebula in the Hubble SHO palette just over 6 hours of total integration. Scope - William Optics RedCat 71. Camera - Atikone 6.0. Filters - Antlia 3nm Ha, Oiii & Sii.

Latest #Astrophotography adventure, The Seagull Nebula. This was a difficult one, it’s very low from here, doesn’t get much above 20Β°, skirting the trees. And with the clocks going forward I was only able to about 1.5 hours a night. This it’s just over 6 hours and is very noisy. Details in AltText

06.04.2025 08:52 β€” πŸ‘ 857    πŸ” 81    πŸ’¬ 19    πŸ“Œ 2
Description: https://www.astrobin.com/qb8blw/D/

NGC7000 horizontal https://www.astrobin.com/full/qb8blw/D/

Dates: June 5, 2022 June 10 - 12, 2022 July 15, 2022 Aug. 3, 2022 Aug. 8, 2022 
Filters: Optolong L-Pro 2", Radian Triad Ultra 2"
Integration: 15h 39β€² 40β€³

Description: https://www.astrobin.com/qb8blw/D/ NGC7000 horizontal https://www.astrobin.com/full/qb8blw/D/ Dates: June 5, 2022 June 10 - 12, 2022 July 15, 2022 Aug. 3, 2022 Aug. 8, 2022 Filters: Optolong L-Pro 2", Radian Triad Ultra 2" Integration: 15h 39β€² 40β€³


Description: https://www.astrobin.com/qb8blw/D/

NGC7000 vertical   https://www.astrobin.com/full/qb8blw/0/

Dates: June 5, 2022 June 10 - 12, 2022 July 15, 2022 Aug. 3, 2022 Aug. 8, 2022 
Filters: Optolong L-Pro 2", Radian Triad Ultra 2"
Integration: 15h 39β€² 40β€³

Description: https://www.astrobin.com/qb8blw/D/ NGC7000 vertical https://www.astrobin.com/full/qb8blw/0/ Dates: June 5, 2022 June 10 - 12, 2022 July 15, 2022 Aug. 3, 2022 Aug. 8, 2022 Filters: Optolong L-Pro 2", Radian Triad Ultra 2" Integration: 15h 39β€² 40β€³

πŸ”­NGC7000-North America Nebula πŸ”­ An emission nebula in the Cygnus constellation at 1,700 ly away and 100 ly across, glowing due to the ionization of interstellar gas caused by radiation emitted by hot stars.
astrobin.com/full/qb8blw/D/
#Astrophotography #Space #Astronomy #Nebulae

22.03.2025 16:36 β€” πŸ‘ 13    πŸ” 1    πŸ’¬ 0    πŸ“Œ 0

@astrootus is following 20 prominent accounts