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Dumbbell_Nebula_(M27).jpg
Dumbbell Nebula (M27)302 viewsThe Dumbbell Nebula (M27) is a planetary nebula in the constellation of Vulpecula. It is the second brightest planetary nebula in the night sky and easy to spot with binoculars or a small telescope. Taken September 5, 2016 with a Canon 60Da camera, Orion ED80T telescope on a Celestron CGEM mount. Stacked with Nebulosity 4.0 and processed with PixInsight 1.8Sep 30, 2016
Moon_9Sep16.jpg
First Quarter Moon346 viewsThe moon on September 9, 2016. During this phase 50% of the moon disc is illuminated. Taken with ES 127mm, Canon 60Da, Celestron CGE Pro. Processed with RegiStax 6 and Photoshop CS 6.Sep 26, 2016
M56normalsize.jpg
A GLOBULAR CLUSTER IN LYRA357 viewsThe globular cluster Messier 56 is found in the part of Milky Way that runs through the constellation Lyra. Admiral Smyth describes M 56 as “a globular cluster in a splendid field” in his “A Cycle of Celestial Objects” (2nd Ed, 1881). The image was taken on 15 June 2016 in Mayhill, NM with a 12.5” RCOS f/9 telescope operating at f/5.95 (Astro-Physics CCDT67 reducer) and a SBIG STF8300c camera mounted on a Paramount ME. Exposure was a total of 1 hr 40 min (5 x 20 min lights @ -15 degrees C; 40 darks; 128 flats; 128 bias). Calibrated, registered, integrated, and processed in PixInsight 1.8.4.1195 Ripley (x64).Sep 19, 2016
NGC2903PixInsightfinal.jpg
Barred Spiral Galaxy in Leo347 viewsNGC 2903 is a intermediate weak-barred spiral galaxy (SABbc) found in the constellation Leo. Discovered by W. Herschel in 1784, NGC 2903 is approximately 20 to 30 million light years away. Image was taken with a 12.5” f/9 RCOS telescope and a SBIG STF8300c camera with an OAG (ST-i) on a Paramount ME. Image a total of 15 hr 20 min of combined exposures taken on 12, 13 Jan and 8,9,12 Feb 2016 in Mayhill, NM (46 x 1200 sec lights @ -15 degrees C, dithered; 30 darks; 128 bias; 128 flats). Processed in PixInsight 1.8.4.1195.Jul 27, 2016
Messier_13_in_Hercules.jpg
The Great Globular Cluster in Hercules372 viewsMessier 13, or the Great Globular Cluster in Hercules, was discovered by Edmond Halley in 1714. The cluster is estimated to contain from 300,000 to a half-million stars and is about 26,000 lights years distant from our solar system. The image was taken with a 12.5” RCOS f/9 telescope operating at f/5.94 (Astro-Physics CCDT67 telecompressor) and a SBIG STF8300c camera on a Paramount ME in Mayhill, NM on 28 May 2016 (6 x 20 min lights @ -20 degrees C; 40 darks; 128 bias; 128 flats). Processed with PixInsight 1.8.4.1195.Jun 20, 2016
Messier78final.jpg
The Messier 78 region361 viewsMessier 78 is a blue reflection nebula (larger nebula near the center of the image) that is found in the constellation Orion. Several other reflection nebulae can be seen in the image along with extensive clouds of dust (dark molecular cloud Orion B). The red emission nebula in the lower right-hand corner is part of Barnard's loop. Image is a total of 11 hr 30min exposure (46 x 15 min lights, dithered; 12 darks; 128 flats; 128 bias) taken on the nights of Nov 6, 2015; Jan 12, 13, 2016; Feb 8, 9, 12, 2016 with a Takahashi FSQ106ED with reducer @ f/3.6; Canon 60Da @ ISO 800; Astro-Physics 1200 mount; and Astro-Physics/Baader 60 mm guider (SBIG ST-i); Processed with PixInsight 1.8.4.1195 (with Bayer drizzle algorithm).Jun 06, 2016
Mercury_Transit_0818MT_SV80ED_CaK_41AU02.jpg
Mercury Transit 2016270 viewsThe Mercury transit was well underway when this image was taken at 8:17 AM MT on 5/9/2016 from the AAG outreach event at Imago Dei Academy in Alamogordo, NM. The image was taken using a Stellaruve 80ED refractor with a Lunt B1200 Calcium-K module and Imaging Source 41AU02 camera. The Calcium K-line (393.4 nm) shows supergranulation in the lower chromosphere (~1200 km) along with lighter regions indicating magnetic activity. Sunspot AR2542 along with the small disk of Mercury are also visible.May 12, 2016
Messier82_sRGB.jpg
The starburst galaxy Messier 82246 viewsThis HaLRGB image portrays the turbulent starburst galaxy Messier 82 in Ursa Major with its filamentary outflows of ionized hydrogen. This emission is suggested to be due to stellar winds caused by massive energetic young stars (as well as supernovae resulting from their death) being born at a high rate within the galaxy. Total of 18 hrs exposure with a Takahashi CCA-250 f/5 astrograph; Nights of 15, 24, 28 March 2015; 12, 13 Jan 2016; 8, 9 Feb 2016: 2015 Paramount ME, QSI683wsg, Astrodon Gen2 filters (Ha 5 nm); (Lum 16 x 20 min; Ha 17 x 20 min; R 7 x 20 min; G 7 x 20 min; B 7 x 29 min all @ - 20 degrees C), calibrated, registered, integrated, and processed in PixInsight 1.8.4.1195 (x 64).Mar 26, 2016
MultiscaleHaLumFinal.jpg
Messier 82249 viewsThis combined Ha and Luminance image shows the starburst galaxy Messier 82 in Ursa Major with its filamentary outflows of ionized hydrogen. This emission is suggested to be due to stellar winds caused by massive energetic young stars (as well as supernova resulting from their death) being born at a high rate within the galaxy. Total of 9 hr 20 min exposure with a Takahashi CCA-250 f/5 astrograph; Nights of 15, 28 March 2015, 12, 13 Jan 2016, 8, 9 Feb 2016; 2015 Paramount ME, QSI 683wsg, 5 nm Astrodon Ha filter (Lum 11 x 20 min @ - 20 degrees C; Ha 17 x 20 min @ - 20 degrees C), calibrated, registered, integrated, and processed in PixInsight 1.8.4.1195.Mar 16, 2016
Conen_Nebula.jpg
NGC 2264327 viewsNGC 2264 in the constellation of Monoceros consists of the Cone Nebula and the Christmas Tree Cluster. The Cone Nebula is an H II region and a dark absorption nebula. The Christmas Tree cluster (upside down) is the open cluster above the nebula. The bright star towards the top center (S Mon) represents the center of the trunk while HD 47887 above the cone nebula, represents the top. Not officially part of NGC 2264 is the Fox Fur Nebula, the blue and red furry like area next to S Mon. 200 min total exposure.Feb 23, 2016
Crab_Nebula.jpg
Crab Nebula (M1)344 viewsThe Crab Nebula (M1) is a supernova remnant in the constellation of Taurus. In 1731 John Bevis found that M1 corresponded with the bright supernova recorded by Chinese astronomers in 1054 AD as a star bright enough to be seen during the day. The image consists of 47 exposures taken with a Canon 60Da camera, a TPO RC telescope and a Celestron CGEM mount. Exposures were stacked with Nebulosity and processed with PixInsight 1.8.Feb 23, 2016
M76_2016_02_12_130EDT_f7_314L+_130min.jpg
M76 - The Little Dumbbell314 viewsMessier 76 was discovered in 1780 by Pierre Méchain and cataloged by Charles Messier that same year. It wasn't until 1918 that M76's true nature as a planetary nebula was discovered by Herber Curtis. Located some 2,500 light years away in the constellation Perseus, M76 it is one of the faintest objects in the Messier catalog at magnitude 10.1. This image was taken from Alamogordo NM using an Astro-tech 130EDT f7 refractor and Atik 314L+ monochrome camera (130 min) using Ha, Hb and OIII signals.Feb 14, 2016
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