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307 files in 32 albums and 1 categories with 3 comments viewed 365712 times

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North American Nebula1610 viewsNorth American Nebula (NGC 7000) in Cygnus. A 3-minute exposure taken with a Takahashi Epsilon 180 f2.8 and a Canon 20Da DSLR (ISO 800)
Massive Filament on the Sun931 viewsA dark filament of magnetism in the sun's southern hemisphere has curled upon itself to form a circle of gargantuan proportions. The circumference of the ring is almost a million kilometers (600,000 miles)! Magnetic filaments are very often unstable, and have a tendency to collapse. Filaments crashing to the surface of the sun can cause of a type of explosion called a Hyder flare. Any flare from this filament could be extra-energetic as it releases the tension stored in its million-km coil. Image taken from Alamogordo, NM on 11/13/15 at 10:14 AM MST (1714 UTC) using a Meade Instruments Coronado 90mm SolarMax II telescope and Imaging Source 41AU02 camera.
Rosette Nebula878 viewsThe Rosette nebula is large nebula that resembles a a flower. The open cluster in its center, NGC 2244, consist of stars that formed from the nebula's material. The photo consist of 8 X 3 minutes photos and 5 X 5 minutes photos utilizing a Canon 60Da on and Orion 80mm refractor. Images were stacked in Nebulosity with levels and curves adjusted with Photoshop CS6.
The Cave Nebula (Caldwell 9)1020 viewsCaldwell 9 (Cave Nebula) located in the constellation of Cepheus, is a diffuse nebula that forms part of a larger area that contains emission, reflection, and dark nebulosity. The image consist of 68 x 5min exposures with a Canon 60Da and Orion ED80T telescope on a Celestron CGM mount.
IC5070 (Pelican Nebula)909 viewsIC5070 (Pelican Nebula) located in the constellation of Cygnus is part of a large H-II cloud. The hydrogen gas is excited by the energy originating from nearby stars, and then emits its own light in the red wavelength of hydrogen. The image consist of 4 hours of exposures taken with a Canon 60Da camera, ES 127mm refractor with .8 reducer, mounted on a Celestron CGEM mount. The image was stacked with Nebulosity 4 and processed with Pixinsight 1.8.
Leo Triplet with Tidal Trail1070 viewsMessier 65, Messier 66, and NGC 3628 are commonly known as the Leo Triplet. M 65 is a spiral galaxy whose center is comprised of older yellowish stars (bottom left center of image). M 66 (top center) and NGC 3628 (top right center of image; aka the hamburger galaxy) are suggested to have had a past encounter that resulted in a faint tidal trail seen coming off the top of NGC 3628. The image was captured with a modified Canon 40D (ISO 800) and a Takahashi E180 f/2.8 astrograph on a Paramount. Total exposure time was 8 hours (48 X 10 min guided sub-exposures; 13 darks; 64 flats; 64 flat darks). Calibrated and stacked with Images Plus 5.0; processed with PixInsight 1.8 followed by final Levels and Curves adjustment in Adobe Photoshop CS6.
The Rho Ophiuchi Nebulae IC 4604 and IC 46031195 viewsOn the border of Scorpius and Ophiuchus by Antares lies a complex region of dust, molecular clouds, and reflection nebula. In the center of this image is the triple star Rho Ophiuchi, which is surrounded by the blue reflection nebula IC 4604. Throughout the image large dust clouds are seen. To the right of IC 4604 is the smaller reflection nebula IC 4603. Image was acquired using a Takahashi Epsilon 180 f/2.8 astrograph and a modified Canon 40D DSLR camera on a Paramount. Images Plus 5.0 was used for calibration and stacking of the sub images. PixInsight 1.8 Ripley was used to process the image. Image was a total of 2 hours 40 minutes exposure (16 x 10 min lights, 13 darks, 64 flats, 64 flat darks).
Lunar Eclipse of Sept 2015790 viewsThe 9/27/15 Lunar Eclipse in Mayhill, New Mexico (9/28/15 02:59:14 UT) taken with an Astro-Physics 178mm f/9 refractor with field flattener and SBIG STF8300c camera on an Astro-Physics 1200 mount; processed in PixInsight

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“37” Open Cluster in Orion33 viewsThe open cluster 2169, often called the 37 cluster or Shopping Cart cluster, is found in the constellation Orion. It was arguably discovered by Giovanni Batista Hodierna before 1694 and was independently discovered by William Herschel in 1784. Combined exposure was 2.7 hr through an Takahashi Epsilon-180ED f/2.8 astrograph with a SBIG STC-7 camera mounted on a Paramount ME on the night 16 March 2022 in Mayhill, NM (20 x 160 sec B, 20 X160 sec G, 20 X 160 sec R, Medium Gain, sub-exposure 10 sec, MaxIm DL Stack ProTM). All images calibrated, registered, and integrated with PixInsight 1.8.8-9 Ripley (x64).Apr 16, 2022
Arp 270 in Leo Minor41 viewsArp 270, a pair of galaxies with connected arm NGC 3395 and NCC 3396, lies in the constellation Leo Minor. The image of NGC 3395 appears disturbed and a bridge extends from it to NGC 3396. The image is a total of 3 hours exposure with a 12.5 inch RCOS f/9 operating at f/6 (Astro-Physics CCDT67) with a SBIG STF8300m mounted on a Paramount taken on the nights of 26 Feb and 5 Mar 2019 in Mayhill, NM (9 x 1200 sec Lights, 128 Bias, 128 Flats, 22 Darks all @ -15 degrees C). Processed with PixInsight 1.8.8-12 Ripley (x64).Feb 11, 2022
A Spiral Galaxy in Leo155 viewsMessier 66, aka M66 or NGC 3627, is a spiral galaxy (semi-barred) found in the constellation Leo. M66 belongs to a group of galaxies including M65 and NGC 3628 known as the Leo Triplet. In the past, it is likely that M66 that encountered NGC 3628. M66 lies around 31 to 33.5 million light-years from us. Image is a total of 10 hr 40 min combined exposure taken with a Takahashi CCA-250 f/5 astrograph with a QSI683wsg CCD camera mounted on a Paramount ME on the nights of 28, 29 March, 3, 29 May 2019 and 15, 26 April 2020 in Mayhill, NM (19 x 1200 sec Lum; 4 x 1200 sec R; 5 x 1200 sec G; 4 x 1200 sec B all at -20 degrees C.; 128 Bias; 22 Darks; 128 Flats for LRGB, respectively). Processed in PixInsight 1.8.8-7 Ripley (x64).Apr 10, 2021
The Ring Nebula in the Constellation Lyra175 viewsM57, the ring nebula, is found in the constellation Lyra. M57 is a planetary nebula, which is an expanding shell of gas ejected from a star in the later stages of its evolution. The image captured the outer halo structure of M57 as well as the galaxy IC 1296 (see annotated image on the Facebook page). Image is a total of 9 hr 20 min exposure taken through a 12.5” RCOS f/9 astrograph at f/6 (Astro-Physics CCDT67 reducer) with a SBIG STF8300m CCD camera on a Paramount ME on the nights of 18, 19, 22 May 17, 19 June 2020 in Mayhill, NM (13 x 1200 s lights, 5 x 1200 s blue, 5 x 1200 s red, 5 x 1200 s green all at -15 degrees C). Processed in PixInsight 1.8.8-6 Ripley (x64).
Mar 17, 2021
Jan 2019 lunar eclipse642 viewsJanuary 20, 2019 lunar eclipse taken with Borg 71FL refractor and Canon 1000D DSLR on a Vixen alt-az mount. Single exposure 0.8 sec, ISO 400Jan 22, 2019
The Perseus Cluster of Galaxies685 viewsThis image of the Perseus cluster of galaxies, also known as Abell 426, is centered on NGC 1275. NGC 1275 is a giant elliptical galaxy, which is a radio source and x-ray emitter. Abell 426 is part of the Pisces-Perseus supercluster, which contains over a thousand galaxies. The image is a total of 9 hrs exposure with a Takahashi CCA-250 f/5 astrograph and a QSI683wsg camera (Astrodon Gen2 filters) on a Paramount ME taken on the nights of 7 Nov, 3, 13 Dec 2018 in Mayhill, NM (18 x 1200 sec lights; 3 x 1200 sec R, G, and B at -20 degrees; 24 darks; 128 flats; 128 bias). Processed with PixInsight Ripley (x64).Jan 18, 2019
Open Cluster in Cassiopeia 632 viewsThe open cluster NGC 663 is found in the constellation Cassiopeia. NGC 663 contains a significant number of Be stars (spectral class B stars showing emission lines in their spectra). The distance from us is on the order of 2,100 parsecs (6850 light years). The image is a total of 5 hrs 20 min exposure taken with a 12.5” RCOS f/9 @ f/6 (Astro-Physics CCDT67) and SBIG STF8300m camera on a Paramount ME in Mayhill, NM on the nights of 28 Nov and 3 Dec, 2018 (6 x 1200 sec R; 5 x 1200 sec G & B; 24 darks; 128 bias; 128 flats). Processed in PixInsight Ripley (x64).Jan 18, 2019
A Large Emission Nebula in Cassiopeia671 viewsNGC 281 is a H II emission nebula in Cassiopeia containing the open cluster IC 1590, which powers the ionization of the hydrogen gas. Large dust filaments as well as Bok globules, which may be the site of future star formation, can be seen. The image is a total of 5 hrs 20 min exposure in H alpha light. Image taken with a Takahashi CCA250 astrograph and QSI683wsg camera on a Paramount ME on the nights of 13, 15 Dec, 16 Nov 2018 in Mayhill, NM (16 x 1200 sec lights @ -20 degrees C. Astrodon H alpha filter 5 nm bandwidth; 24 darks; 128 bias; 128 flats). Processed with PixInsight Ripley (x64). Oct 19, 2018