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Veil_3-min_exp_n=3_E180_.jpg
Veil Nebula844 viewsThree 3-minute exposures stacked of the Veil Nebula in Cygnus (NGC 6960) taken with a Takahashi Epsilon 180 and a Canon 20Da DSLR
Barnard_86-NGC_6520_n_=_4_3-minute_exposures_Stacked_and_Processed.jpg
Barnard 86 and NGC 6520840 viewsBarnard 86, which is a dark nebula, and the open cluster NGC 6520 in a Milky Way star field in Sagittarius. Four 3-minute exposures stacked taken with a Takahashi FSQ 106 and a Canon 20Da DSLR (ISO 400)
Sun_2012_03_11_first_light_5_2x_reduced.jpg
Sun Spot 1429839 viewsThis is an Ha image of sunspot 1429 on 3-11-12.
Crescent_Nebula.jpg
The Crescent Nebula and surrounding nebulosity837 viewsThe Crescent Nebula (NGC 6888) is in the constellation Cygnus. The brighter portion of the surrounding nebulosity in the upper left is IC 1318, which is part of the gamma Cygnus nebulae complex. The bright star in the center of the Crescent Nebula is a Wolf-Rayet star, which are extremely luminous and hot stars that loose mass at very high rates, designated as HD 192163. The image is a total exposure of 1 hr 45 min (21 X 300 sec) taken with a Takahashi E-180 f/2.8 astrograph and Canon 20Da DSLR camera.
M31_30-min_exposure_E180_.jpg
Andromeda Galaxy835 viewsTwo 30-minute exposures stacked of the Andromeda Galaxy (M31) taken with a Takahashi Epsilon 180 f2.8 and a Canon 20Da DSLR.
M31-b.jpg
M31834 viewsTaken from my backyard - corrected
103P_Hartley_2_10_11_10_DSLR_1min.jpg
103P/Comet Hartley 2833 viewsComet Hartley 2, officially designated 103P/Hartley, is a small periodic comet with an orbital period of 6.46 years. It was discovered in 1986. It will be the subject of a flyby by the NASA Deep Impact (EPOXI) spacecraft on November 4, 2010. This image was taken with the C9.25 @ f6.3 with a Canon T2i DSLR (2 ea. 30sec images at ISO 1600) on 10/10/10 at 8:50 PM MT (284:02:50 UT) from Alamogordo NM.
2012_05_11_AR1476_Solar_Wedge_90mm_f30_LRdecon_532nm.jpg
Super Sunspot AR1746831 viewsSunpots are cooler regions in the photosphere where the magnetic field pops through and cools the surrounding plasma. The latest large sunspot rotated into view on May 5 and is the largest since 2003. Active Region (AR) 1476 spans about 160,000 km (100,000 miles) in this image. Image taken on 5/11/2012 using a 90mm refractor at f30, Lunt solar wedge and 532nm filter with a DMK41AU02 camera. See live images of the Sun on our "PLANETS" page.
Jupiter_6_21_09.jpg
Jumpin' Jupiter!831 viewsJupiter is nearing its 2009 opposition - so I thought I'd go out and practice. Shot with the Celestron C9.25/CGE at f/25 (5875mm) with the NexImage/Televue Powermate (2.5x) from the backyard. I shot at 20 fps to get the most amount of images (1800). Stacked with Registax 2.0, Processed with Photoshop 7.0.1.
Messier_27.jpg
Messier 27826 viewsM 27 , aka the dumbbell nebula, in the constellation Vulpecula was discovered by Charles Messier in 1764. M27 is a large cloud of expanding gas, which is the remains of a star that expelled its outer atmosphere near the end of its lifetime. M27 is a bright object that can be seen in binoculars and is a favorite telescopic object in the Spring and early Fall. Total exposure of 1 hr 40 minutes (20 x 5 min lights;30 darks; 66 flats; AP 178 f/9 refractor; Modified Canon 50D; AP 1200 mount; guided exposures)
2011_10_03_Whitelight_CaK_composite.jpg
What a diiference a filter makes!824 viewsHere is the Sun taken on 10/3/11 at 11:15 AM first in White light (left) and Calcium K (right) using a Stellarvue 80ED. The white light image shows a few sunspot groups while the CaK image shows much more detail and areas of increased magnetic activity. AR1302 is on the far right, nearly rotating out of view. The white light image was taken using an Orion glass filter and single snapshot from a Canon T2i. The CaK image was taken with an Imaging Source camera and Lunt B1200 CaK filter.
Horse-color-scaled.jpg
Horse Head Reworked815 viewsThis was taken at Steve's on Nov 2, 2007 this is 7x10 minute images. with TakFS102 and SBig ST2000XCM. I reworked the image to pull out more of the sutle areas.
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