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Showing posts with label Jupiter. Show all posts
Showing posts with label Jupiter. Show all posts

Wednesday, September 4, 2019

Zodiacal Light Bolivia Astrophotography

This Zodiacal Light astrophotography image was captured in the high Andes of Bolivia, approximately two hours after sunset, during a New Moon night. The observation site was near Hotel Jardines De Mallku Cueva, at an elevation of 4,020 meters (13,190 feet), where the atmosphere is exceptionally clear and dry.

The faint triangular glow rising from the western horizon is the zodiacal light, aligned with the ecliptic plane. Jupiter is visible near the top of the frame, providing a natural reference point above the glowing dust column. Despite the camera’s enhanced sensitivity, the zodiacal light was clearly visible to the naked eye, a rare experience even for experienced observers.

For beginners, planets provide one of the easiest ways to locate the zodiacal light. All major planets orbit within the ecliptic plane — the same plane in which the zodiacal dust cloud is distributed. If you remember where the Sun set and can identify at least one bright planet after dusk, that planet effectively marks the path along which the zodiacal light may appear.

When two or more planets are visible, the orientation of the Solar System’s plane becomes even clearer. The same approach works before sunrise: by noting the position of a bright planet and the upcoming direction of sunrise, you can determine where to search for the faint zodiacal glow.

Modern mobile sky-mapping applications can also be helpful, but seeing zodiacal light visually offers something unique — while the plane of our Galaxy is easily traced by the Milky Way, the plane of the Solar System is far more subtle. Observing zodiacal light is one of the few ways to directly perceive that solar plane with the naked eye.

Captured with Canon EOS 60Da and Canon EF 16–35mm f/2.8L, this panorama consists of three stitched exposures, each taken at 25 seconds, f/2.8, ISO 6400.

Zodiacal Light over the Andes in Bolivia with Jupiter visible above the ecliptic, captured at 4020 meters during New Moon
Zodiacal Light over the Andes, Bolivia – New Moon astrophotography at 4,020 meters

Zodiacal light is a faint, diffuse, and roughly triangular glow visible in exceptionally dark skies, appearing along the zodiac and following the ecliptic plane. It is brightest near the horizon and gradually fades upward, tilted according to the seasonal angle of the ecliptic.

This glow is caused by sunlight scattering off microscopic interplanetary dust particles distributed throughout the inner Solar System. Most of this dust is believed to originate from cometary debris and collisions between small rocky bodies.

High-altitude locations such as the Bolivian Andes dramatically enhance zodiacal light visibility due to reduced atmospheric scattering, extremely low humidity, and minimal light pollution.

Below is a color-enhanced variation of the same zodiacal light panorama, revealing subtle gradients and dust-scattering structure that are difficult to perceive visually.

Color-enhanced zodiacal light astrophotography showing interplanetary dust glow along the ecliptic
Zodiacal Light Astrophotography

The black and white version below is the closest representation of what the zodiacal light appeared like to the human eye — a soft, ghostly glow rising from the horizon, barely distinguishable from the natural night sky background.

Black and white zodiacal light astrophotography showing faint triangular glow similar to naked-eye view
Zodiacal Light Astrophotography Black and White
 

Observing zodiacal light from the high Andes of Bolivia was a reminder that not all structures in the night sky are immediately obvious. While the Milky Way clearly traces the plane of our Galaxy, zodiacal light reveals the far subtler plane of our Solar System itself — made visible only under pristine conditions. At high altitude, far from light pollution, this delicate glow becomes one of the most rewarding naked-eye experiences in night-sky observation.

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Thursday, June 12, 2014

Jupiter Moons and Red Spot - Astrophotography - Celestron 4SE

How does Jupiter hold up his trousers?
With an asteroid belt.

--Astronomy Jokes

Jupiter is one of the most exciting objects to observe in the solar system. Even a small telescope reveals its bright cloud belts, the famous Great Red Spot, and the four large Galilean moons — Io, Europa, Ganymede, and Callisto. Watching these moons change position from night to night (and sometimes hour to hour) is one of the highlights of amateur astronomy.

This photo was taken with my Celestron NexStar 4SE Maksutov telescope from Brooklyn, NYC. For bright planets like Jupiter, Mars, Venus, or Saturn, light pollution is not a problem at all. These planets are extremely bright, and the telescope’s tiny field of view blocks almost all city glow. Light pollution mainly affects faint stars and the Milky Way, but not planets — they remain sharp and clear even in a heavily light-polluted city like New York.

Capturing both Jupiter’s atmospheric details and all four moons in a single frame is not easy. The planet needs a very short exposure to reveal the belts and the Great Red Spot, while the moons require a much brighter setting. For the final image, I combined two photos — one optimized for Jupiter itself and another for the moons. I checked the ephemeris for that night so I could label each moon correctly. The positions of Jupiter’s moons can be easily found using online tools — for example, the Sky & Telescope Jupiter’s Moons calculator.

The Image


Jupiter with the Great Red Spot and Galilean moons captured through a Celestron 4SE telescope from Brooklyn NYC – astrophotography image
Jupiter Moons and Red Spot Astrophotography Celestron 4SE - Brooklyn NYC

What You Can See in the Image

  • Jupiter’s two main cloud belts
  • The Great Red Spot on the disk
  • All four Galilean moons correctly positioned for that night
  • Labeled moons based on calculated ephemeris

For a compact 4-inch telescope, this is a very satisfying result. The combination of sharp planetary details and the full set of moons gives a realistic view of the dynamic Jupiter system.

Gear & Technique

  • Telescope: Celestron NexStar 4SE Maksutov
  • Mount: GoTo Alt-Az
  • Method: Two-photo composite — short exposure for Jupiter, brighter exposure for moons
  • Main challenge: Huge difference in brightness between planet and moons

This image shows what a small telescope can do even in the middle of a major city. Planets are bright enough to cut through light pollution, and their details are visible whenever the atmosphere is steady.

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Sunday, January 26, 2014

Astrophotography Equipment DSLR Webcam Collage

This astrophotography collage shows a small collection of images representing different types of astronomical photography: solar and lunar eclipses, planetary imaging, deep sky objects, the Milky Way, aurora borealis, and astrophotography equipment.

The collage also illustrates some of the equipment used for capturing these images, including a Celestron NexStar 4SE telescope, Canon EOS DSLR cameras, astronomy webcams, and large astronomical binoculars. Different astronomical targets require different techniques — from long-exposure DSLR photography for wide-field night landscapes to high-frame-rate webcam imaging for planets like Saturn, Jupiter, and Mars.

Over the years I have experimented with multiple astrophotography methods: planetary imaging using RegiStax stacking, solar imaging with a Coronado SolarMax telescope, wide-field Milky Way photography, and eclipse photography. This collage represents some of those early experiments and observations.

Astrophotography collage showing Saturn, Jupiter, Mars, solar eclipse, aurora borealis, Milky Way and amateur telescope equipment
Astrophotography Equipment DSLR Webcam Collage – Planetary, Solar and Night Sky Astrophotography


Most of these images were captured from New York City or nearby locations, demonstrating that interesting astrophotography is possible even under light-polluted skies. Other images were taken from darker locations such as national parks and remote observing sites.


Astrophotography Posts Featured in This Collage

This collage shows how different branches of astrophotography — planetary, solar, deep-sky, night landscape, and atmospheric phenomena — can all be captured with relatively modest amateur equipment. From photographing the rings of Saturn and the cloud belts of Jupiter to capturing the Milky Way over dark landscapes, astrophotography allows us to explore the universe from our own planet.

Saturday, April 9, 2011

RegiStax 6 vs. 5 comparison - Jupiter Celestron 4SE

Here is an example of the difference between Registax v5 and v6 for Jupiter (Jupiter with Ganymede Moon and Ganymede Shadow Transit, September 18, 2010 - Celestron 4SE)

Registax v6 - Wavelet - Gaussian Initial Layer 3 Used Linked Wavelets with denoise 1 and 2 layers, RGB shift
Jupiter with Ganymede and shadow transit processed in Registax 6 using linked wavelets, Celestron 4SE astronomy
Registax 6, Celestron 4SE, Jupiter
Jupiter with Ganymede and shadow transit processed in Registax 5, Celestron 4SE backyard planetary astrophotography
Registax 5, Celestron 4SE, Jupiter
Some clouds are more visible in Registax v6, the shadow and Ganymede moon looks better. So my opinion Registax 6 gives better result with Used Linked Wavelets.

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Monday, January 31, 2011

Backyard Astronomy - Astrophotography Celestron NexStar 4se

Backyard Astronomy - Astrophotography Celestron
NexStar 4se telescope
Canon EOS 40D and T-Adapter-C90 and Barlow T-Adapter 1 1/4 inches and T-ring for Canon EOS
Celestron 4se telescope with T-Adapter-C90 (93635-A) and Canon EOS 40D
Celestron 4se telescope with Barlow t-Adapter 1 1/4 inches (93640) and Canon EOS 40D
Celestron 4se with Barlow t-Adapter 1 1/4 inches (93640), Erect Image Diagonal (94116) and Canon EOS 40D
Photos of the Moon and the Sun
Celestron NexStar 4se telescope NexImage CCD
Jupiter photos
Piggy-Back Camera Mount for Celestron NexStar 4 telescope (Item# BRKTPIG4)
The Green Comet 103P/Hartley 2 (2010)
 


Moon Celestron 4SE Canon 40D Astronomy Brooklyn Astrophotography

Sunday, January 30, 2011

Jupiter 2010 Opposition - Celestron 4SE NexImage Registax

These images and video capture Jupiter during its 2010 opposition, photographed on September 20 and September 21, 2010 from my backyard in Brooklyn, New York. Planetary opposition is one of the best times to observe Jupiter, as the planet is closest to Earth, appears brighter, and shows its largest apparent disk.

All video data was recorded using a Celestron NexStar 4SE telescope with a 2× Barlow lens and the original Celestron NexImage CCD camera. Despite heavy urban light pollution, Jupiter’s cloud bands and the Great Red Spot were clearly resolved using high-frame-rate video capture and stacking techniques.

Capture & Processing Details

  • Telescope: Celestron NexStar 4SE
  • Camera: Celestron NexImage CCD
  • Barlow Lens: 2×
  • Frame Rate: 10 frames per second
  • Exposure: 1/10 second
  • Video Length: ~4 minutes per capture
  • Total Frames: ~2400
  • Resolution: 640 × 480 (AVI)
  • Stacking Software: RegiStax v5
  • Final Processing: Adobe Photoshop

The AVI video files were stacked in RegiStax v5, where the best frames were aligned and combined to reduce atmospheric turbulence. Wavelet sharpening was applied to enhance fine details, followed by final contrast and color adjustments in Photoshop.



The video demonstrates the complete planetary imaging workflow: the physical backyard telescope setup, live Jupiter capture using AmCap, raw CCD footage, RegiStax stacking and wavelet processing, and the final sharpened planetary images.

Three Jupiter images taken about one hour apart showing rotation and Great Red Spot movement
Jupiter Celestron 4SE NexImage Brooklyn Backyard astronomy

Image 1 shows three photographs of Jupiter arranged vertically, taken approximately one hour apart. The planet’s rotation is clearly visible through the changing position of the Great Red Spot. In the top image the Red Spot appears on the left side of Jupiter’s disk, in the middle image it is near the center, and in the bottom image it has moved toward the right side. From this sequence, Jupiter’s rapid rotation can be visually estimated directly from the photographs.


Second Jupiter rotation sequence showing Great Red Spot motion
Celestron 4 SE Jupiter Astrophoto Brooklyn

Image 2 shows the same three Jupiter photographs, again arranged vertically for comparison. This layout makes the motion of the Great Red Spot even easier to follow and highlights how much Jupiter rotates over a short period of time. Since Jupiter completes one full rotation in roughly 10 hours, significant surface movement can be observed within a single night of planetary imaging.



Comparison of raw single frame and final RegiStax stacked Jupiter image
Comparison original one frame and Registax final Image, Celestron 4 SE, Brooklyn

This project demonstrates how effective planetary imaging can be even from a light-polluted city when using high-frame-rate video capture and stacking techniques. Jupiter’s cloud belts, polar shading, and the Great Red Spot are clearly visible thanks to careful capture timing and RegiStax processing during opposition.

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