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Discovered in 1781 by the French astronomer and comet hunter, Pierre Méchain, the Sombrero galaxy is a lenticular galaxy, which is a classification between full elliptical and spiral, meaning that it has a disc structure but without spiral arms. It’s about 31 million light years away in the constellation of Virgo and about 50 million light years across (one-third of the Milky Way’s diameter). Astronomers have determined that the supermassive black hole at the center of the galaxy is about 1 billion solar masses, making it one of the largest in nearby galaxies. They’ve also determined that there are between 1,200 and 2,000 globular clusters present, more than ten times the estimate for the Milky Way’s population, and they’ve been able to correlate the prevalence of globular clusters with the amount of bulge in the galaxy. Using infrared spectroscopy astronomers have also determined that the bulk of star formation occurs within the highly contrasted dust lane.

This is 2:20 hours of exposure.

Discovered in 1781 by the French astronomer and comet hunter, Pierre Méchain, the Sombrero galaxy is a lenticular galaxy, which is a classification between full elliptical and spiral, meaning that it has a disc structure but without spiral arms. It’s about 31 million light years away in the constellation of Virgo and about 50 million light years across (one-third of the Milky Way’s diameter). Astronomers have determined that the supermassive black hole at the center of the galaxy is about 1 billion solar masses, making it one of the largest in nearby galaxies. They’ve also determined that there are between 1,200 and 2,000 globular clusters present, more than ten times the estimate for the Milky Way’s population, and they’ve been able to correlate the prevalence of globular clusters with the amount of bulge in the galaxy. Using infrared spectroscopy astronomers have also determined that the bulk of star formation occurs within the highly contrasted dust lane. This is 2:20 hours of exposure.

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NGC 4565 – the Needle Galaxy

Located between 30 – 50 million light years away, it’s the most prominent edge-on spiral galaxies we have in our view. Residing near the North Galactic Pole in the constellation Coma Berenices (named for “Berenice's Hair" in Latin and refers to Queen Berenice II of Egypt, who cut off her hair in gratitude to the gods for the safe return of her husband from battle), it has a spatial diameter of 140,000 light-years (Milky Way = 105,000 ly) and is estimated to contain a trillion stars (Milky Way 250-400 billion). With the darkness from a central dust lane obscuring much of the visual core of the galaxy, it’s very similar to our view of the core our Milky Way, and as such is studied extensively by astronomers.

NGC 4565 – the Needle Galaxy Located between 30 – 50 million light years away, it’s the most prominent edge-on spiral galaxies we have in our view. Residing near the North Galactic Pole in the constellation Coma Berenices (named for “Berenice's Hair" in Latin and refers to Queen Berenice II of Egypt, who cut off her hair in gratitude to the gods for the safe return of her husband from battle), it has a spatial diameter of 140,000 light-years (Milky Way = 105,000 ly) and is estimated to contain a trillion stars (Milky Way 250-400 billion). With the darkness from a central dust lane obscuring much of the visual core of the galaxy, it’s very similar to our view of the core our Milky Way, and as such is studied extensively by astronomers.

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M51 through 127mm/952mm FL telescope for 9:55 of total exposure from 8600’ in CO. Located an estimated 23 - 36 million light years from Earth, M51 is approximately 30,000 light years across and home to an estimated 100 billion stars. It’s an interesting target due to its interaction with a dwarf elliptical galaxy, which it appears to be cannibalizing, but with the use of the Hubble astronomers have determined that the dwarf galaxy is actually behind M51. There is still interaction, though, and the dwarf galaxy’s gravitational forces have created areas of great star formation in M51.

M51 through 127mm/952mm FL telescope for 9:55 of total exposure from 8600’ in CO. Located an estimated 23 - 36 million light years from Earth, M51 is approximately 30,000 light years across and home to an estimated 100 billion stars. It’s an interesting target due to its interaction with a dwarf elliptical galaxy, which it appears to be cannibalizing, but with the use of the Hubble astronomers have determined that the dwarf galaxy is actually behind M51. There is still interaction, though, and the dwarf galaxy’s gravitational forces have created areas of great star formation in M51.

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Japanese Word For Astronomy - わが夫、溥儀: ラストエンペラーとの日々 [書籍]

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