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The Milky Way: November-December

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Astronomy of the Milky Way

Part of the book series: Patrick Moore’s Practical Astronomy Series ((PATRICKMOORE))

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Abstract

As autumn turns to winter for northern observers we are still in those parts of the sky that are rich in Milky Way objects. However, some of the constellations are getting very low during the southern summer months and may prove difficult for southern telescopes (see Figure 4.1).

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Notes

  1. See Appendix 1 for details on astronomical coordinate systems.

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  2. The bright stars that extend from Perseus, Taurus and Orion, and down to Centaurus and Scorpius, including the Orion and Scorpius-Centaurus associations, He at an angle of about 1.5° to the Milky Way, and thus to the equatorial plane of the Galaxy. This group or band of stars is often called Gould’s Belt.

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  3. Not forgetting that it is perfect for observation!

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  4. It is, however, the only galaxy that can be seen in small telescopes.

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  5. Astronomically speaking, of course!

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  6. It is ironic that the most famous nebula is also probably the most difficult to observe. Such is the life of an astronomer.

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  7. A full description of M45 and many other celestial objects can be found in my book, Field Guide to the Deep Sky Objects, Springer-Verlag.

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  8. The photographic magnitude change has been measured to be some 4.49 magnitudes.

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  9. It is always a problem knowing what to include in the book, and what to leave out, but as I mentioned in the first chapter, I try to stick rigidly to the premise that an object can be included if it lies within the boundaries of the Milky Way as defined by the Dutch Astronomer Antonie Pannakoek (as used in the star atlas Sky Atlas 2000.0), who measured the approximate brightness levels of the Milky Way. Anything outside of this is not mentioned. This does leave out a lot of famous and bright objects, but if I were to include them, this book would run to several volumes, and possibly a few bank overdrafts.

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  10. But not completely so. I eventually found it on a clear transparent night. Try it for yourselves.

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  11. If you have to use a star which does not lie on or close to the celestial equator, then the formula 15t cos δ where δ is the declination of the star, can be used to find the apparent field diameter of the eyepiece in minutes and seconds of arc.

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© 2004 Springer-Verlag London

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Inglis, M.D. (2004). The Milky Way: November-December. In: Astronomy of the Milky Way. Patrick Moore’s Practical Astronomy Series. Springer, London. https://doi.org/10.1007/978-0-85729-368-8_4

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  • DOI: https://doi.org/10.1007/978-0-85729-368-8_4

  • Publisher Name: Springer, London

  • Print ISBN: 978-1-85233-709-4

  • Online ISBN: 978-0-85729-368-8

  • eBook Packages: Springer Book Archive

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