Primordial Light: Deep Sky 2

Primordial Light: DEEP SKY Page 2

M33, The Triangulum Galaxy

M33

September 27, 2009. M33 is a face-on spiral galaxy about 3 million light years (LY) from Earth (very near in cosmic terms) in the undistinguished constellation Triangulum. It is a member of the Local Group, which is a cluster of galaxies, including our own Milky Way, that are close enough to each other to be gravitationally bound together. The largest member of the Local Group is M31, the Andromeda Galaxy. Our galaxy, the Milky Way, is the second largest, and M33 is the third largest. M33 is about 50,000 LY across, which is about half the size of the Milky Way, and it contains perhaps 50 billion stars, compared to about 400 billion in the Milky Way. M33 is rather diffuse and has low surface brightness and it does not seem to photograph well through polluted skies (like mine). All stars that are seen overlaying the galaxy are nearby stars in the Milky Way. Only the largest telescopes are able to resolve individual stars in distant galaxies. The blue haze is the cumulative light of the billions of unresolved stars and the brownish smudges are vast dust clouds that are the birthplaces of new stars. LRGB with an SBIG STL-11000M on a Takahashi TOA-150. Made on a Mac with Nebulosity, PixInsight, and Photoshop CS3.

M51, the Pinwheel Galaxy, and Its Neighbors

April-May, 2008. The famous Pinwheel Galaxy in the northern constellation Canes Venatici. If you place your cursor over the image you will see the names of some of M51’s neighbors. M51 and its companion galaxy NGC 5195 are experiencing a close encounter of the gravitational kind. There appears to be a bridge of stars connecting the two galaxies. This would indicate that M51, with its greater mass, is disrupting NGC 5195 and stripping away its stars. Eventually the two galaxies will merge into a galaxy that will probably not resemble what we see today. The faint light surrounding with both galaxies is actually starlight from regions with a lower density of stars than the central parts of the galaxies. The number of stars in M51 and its companion, numbers in the hundreds of billions. The distance to M51 is believed to be about 30 million light years.

NGC 5198 is a giant elliptical galaxy that is about 150 million light years distant. It must be extremely luminous to appear as bright as it does at that great distance. IC 4263 and NGC 5169 are spiral galaxies.

Takahashi FSQ-106ED, SBIG STL-11000M. LRGB.

Wide View of M16, the Eagle Nebula

May 30, 2008. M16 (NGC 6611,) the Eagle Nebula

The Eagle Nebula was discovered by Jean Phillippe Loys de Cheseaux in 1845. The many columns of dust and gas in M16 have been nicknamed the “Pillars of Creation” because they are regions where new stars are forming. The black spots that stand out against the nebula in the background are also starbirth regions. They are called Bok Globules after the great astronomer Bart Bok. M16 is in our celestial back yard at a distance of only 7,000 light years. Takahashi FSQ-106ED, SBIG STL-11000M, Hydrogen Alpha.

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