Photographing Orion – Handheld

It’s interesting to see how far sensor technology has come in the past generation or two. On the night of January 6, the sky was clear (but not photometric) after a very stretch of iffy weather. Walking to the house, I admired the majestic Orion riding high in the southern sky. I wondered, “Have DSLRs become capable of photographing the night sky handheld?” Orion, being full of bright stars would be my test case. Here is the result using a fast lens and ISO 32,000. Can you spot Orion at the upper right and α Canis Majoris (Sirius), at the bottom?

Orion – 28mm f/1.4 @ ISO 32,000, 1/13 second @ f/1.4, handheld

For comparison, here is a 10-second exposure at a lower sensitivity (ISO 3,200 rather than ISO 32,000) with the camera on a tripod without tracking. Most notable to me is that faint wisps of cloud appear here and there, showing that the night was not actually “perfectly” clear (termed “photometric”). The image shows the Great Orion Nebula (M42) in Orion’s sword and also the Rosette Nebula as a diffuse smudge far left of Orion’s sword. Notice the bright red giant star α Orionis (Betelgeuse) in Orion’s upper left armpit. That’s my house at the bottom.

Orion – 28mm f/1.4 @ ISO 3,200, 10 seconds @ f/1.4, on Tripod.

Finally, here is a 15-second exposure, unguided, adjusted to include the Pleiades cluster at the upper right. Look carefully and you will see the Pleiades enveloped in the bluish glow of nebulosity enveloping the cluster and illuminated by its hot B-type stars. Sirius is the bright star near the bottom. The Milky Way is visible stretching vertically, left of Orion. Again, notice the faint reddish patches of cloud near the center and horizontally along the bottom — definitely not a photometric night!

Orion and surroundings – 15-second exposure on a non-photometric night.

20 Jan 2019 Lunar Eclipse

Although the lunar eclipse on the evening of 20 Jan 2019 was seen by countless millions across the Americas, Arizona was not the place to be! Clouds of varying thickness covered the entire state, including my location in south central Arizona.

The image below shows the eclipse during totality with Praesepe (the Beehive Cluster) at bottom. The moon’s aura was caused by the thick cloud cover (which also blocked the stars). Two bright stars of the constellation Cancer are visible near the cluster: To the left is γ Cancri (Asellus Borealis) and lower right is δ Cancri (Asellus Australis).

Eclipsed Moon with Praesepe. Image Details: 04:49:48 UT, 2.5 seconds @ ISO 800, 200 mm f/2.8 lens @ f/3.5.

21 Aug 2017 Solar Eclipse

The photographic sequence below shows 59 images taken 3 minutes apart, from 16:10 to 18:04 UT on 21 August 2017. From beginning to end, follow this sequence left to right and downward. I used a 200 mm f/2.8 lens and north is toward the top. The location was East of Sells, AZ, where the Moon’s maximum coverage was around 65%. In front of the lens, I placed a 12,000x neutral density filter to keep the camera from catching fire.

August in southern Arizona is usually cloudy, as the big surge in July precipitation peaks before introducing another 10 months of dryness. Thus we were fortunate the weather was completely clear for the entire event!

Solar Eclipse, 21 Aug 2017

Getting Ready for the August 21 Solar Eclipse

I was refining my technique today in readiness for the eclipse on August 21. This photo was taken using a 200mm lens. You can see several sunspots near the Sun’s limb, at the upper left. I will not b able to travel to the path of totality so I hope the weather will be clear here in southern Arizona on the morning of August 21.

WARNING: Never look through a camera at the Sun and never point your camera at the sun without proper filtration in front of the lens.

 

First images with SBIG STF-8300M CCD Camera

I unboxed this new CCD Camera today, installed the drivers, and fired it up. Here are my first impressions from test images:

Bias frames (0.09s exposure time) at 0°C temperature are very clean. This is the shortest possible exposure time but is close to the 0s exposure of a true bias frame. The readout noise measured from 2 bias frames is 5.18e-, assuming SBIG’s nominal gain of 0.38e-/ADU is correct. To get a more definitive value, I will have to calculate the gain and re-measure the readout noise. The screenshots below show the images in Mira Pro x64.


A Bias frame taken at 0°C.


Readout Noise Calculation from 2 bias frames.

Orion’s Belt and Sword


This was my first attempt at photographing the central portion of the Orion Complex. This region contains the Orion Giant Molecular Cloud which envelops the constellation Orion but is directly observable only in the millimeter wavelength portion of the spectrum. In the visible regime, the sky from Orion eastward into Monoceros is chock full of diffuse nebulae, some of which are shown in this photo. In Orion’s sword are NGC 1976 (Orion Nebula) and NGC 1973,5,7 (Running Man Nebula). Near the left star in Orion’s belt, ζ Orionis, are NGC 2024 (Flame Nebula) and IC 434 with the less distant dark cloud, Bok 33, which together create the Horsehead Nebula.
This is a 168-second exposure at ISO 4000 using a 200mm lens at f/2.8. It was tracked but not guided, and the sky was clear but not especially dark, with a measured zenith V-mag of 21.5 per square arcsecond. I plan to re-image this region on the next good night using a series of many exposures to go deeper.

Summer Milky Way



The summer Milky Way at Sierrita Observatory is a spectacular sight. These wide angle views show the southern Milky Way setting along the SSW horizon. The left image runs from Cepheus at the top, through the Galactic Bulge in Sagittarius, just above the horizon. About 1/4 the way down from the top is the constellation Cygnus, with NGC7000 (“North America Nebula”) glowing red to the left of the bright star, Alpha Cygni (Deneb). The other two images show the sky below Sagittarius. To the right of the Galactic Bulge, notice the dark region called the “Pipe Nebula” which actually consists of several contiguous galactic dust clouds known as Barnard objects.

In this compass direction, there is no human development all the way to the Gulf of California, but the sky brightness increases toward the horizon as we view a longer optical path length through the upper atmosphere. Emission from the upper atmosphere, or “airglow”, occurs from forbidden transitions of OⅠ λ6300 (red) and NⅡ λ5577 (green), and other species. [ref]. Very close to the horizon, however, the extinction rapidly increases from looking through the low elevation dust layer.

Left: 2016-09-03, Nikon D800e + 12mm fisheye, f/2.8, 156 seconds @ ISO 1600″
Middle: 2016-09-04, Nikon D800e + 14-24mm @ 20mm, f/2.8, 30 seconds @ ISO 2000
Right: 2016-08-27, Nikon D800e + 14-24mm @ 24mm, f/2.8, 95 seconds @ ISO 1600
Not shown above: Comparison with labeled objects in SkyGazer

Sierrita Observatory is a private astronomical observatory established by Dr. Michael Newberry for scientific research and educational purposes.