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Astronomical Imaging

Archive for July, 2013

M33 – The Triangulum Galaxy Remastered

by on Jul.21, 2013, under Image Gallery

M33-LHaRGB-Hannahoe-Grasso-web-small

Click photo for larger view.

2.4 million light-years from Earth, the Triangulum Galaxy resides in the constellation Triangulum and spans some 50,000 light-years. This galaxy contains roughly 40 billion stars and is the third largest galaxy in the Local Group. M33 contains many star-forming regions, and these regions are represented by the color red.

Image credit: Ryan M. Hannahoe and Salvatore Grasso
Exposure time: 60 hours
Equipment Used: 16″ RC Optical Systems Telescope, Bisque Paramount ME, and STX16803 CCD
Location: Perez Observatory at New Mexico Skies, Mayhill – New Mexico

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NGC6960, the Lacework Nebula Remastered

by on Jul.12, 2013, under Image Gallery

NGC6960-LRGB-Hannahoe-Grasso-web-small.jpg

Click photo for larger view.

1,500 light-years from Earth, the Lacework Nebula resides in the constellation Cygnus and spans 80 light-years. This nebula was created about 10,000 years ago by a rare supernova that occurred in our own galaxy, the Milky Way.

Image credit: Ryan M. Hannahoe and Salvatore Grasso
Exposure time: 42 hours
Equipment Used: 16″ RC Optical Systems Telescope, Bisque Paramount ME, and STX16803 CCD
Location: Perez Observatory at New Mexico Skies, Mayhill – New Mexico

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M104, Sombrero Galaxy as seen through 200″ Hale Telescope

by on Jul.05, 2013, under Image Gallery

The Sombrero Galaxy as seen through 200" Hale Telescope.

The Sombrero Galaxy as seen through 200″ Hale Telescope.

The Sombrero Galaxy is an edge-on spiral galaxy located 28 million light-years from Earth. It resides in the constellation Virgo within a filamentous complex of galaxies known as the Virgo Supercluster. The Sombrero Galaxy has between 1,200 – 2,000 globular clusters in its halo, more than usual for a galaxy of its luminosity.

M104_Gardner_Grasso_Hannahoe-web-small

Click photo for larger view.

A symmetrical dark lane composed of mostly cold dust and molecular hydrogen encapsulates the central bulge of this galaxy. At the center of the galactic disk lies a “low ionization nuclear region” where atoms are weakly ionized by the supermassive black hole that powers M104’s active galactic nucleus.

Composite Image From Several Data Sources

200″ Hale Telescope – Palomar Observatory
Luminance data: Caltech/Palomar Observatory/Paul Gardner

16″ RCOS Telescope – Perez Observatory/New Mexico Skies
Color data: Ryan Hannahoe

Image assembly and processing: Salvatore Grasso

Copyright: Caltech/Palomar Observatory/Paul Gardner, Salvatore Grasso, and Ryan Hannahoe

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