Ursa Minor

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Observation Notes: I wasn't planning on a naked eye constellation sketch this evening. But the sky was so fantastically clear, and my new astronomy glasses were doing such a great job, that I decided to see how deep I could go with Ursa Minor. When I began the sketch, I was picking up a lot of granularity throughout the constellation. By the time I had finished sketching the stars you see in the sketch, a fine gauze of cirrus had moved in, cutting off that granular appearance. The faintest I got was magnitude 6.8 with HIP 81757 (See rollover labels in the sketch).

One feature of Ursa Minor I find interesting is the close star pairing at the first joint in the handle. I find it analogous to the Mizar/Alcor pairing in Ursa Major, but much more difficult to resolve. Mizar and Alcor are 2nd and 4th magnitude stars that are separated by 11 arc minutes, and something I can separate with or without the glasses. The 2 Ursa Minor stars Delta- and 24-Ursa Minoris are 4.3 and 5.8 magnitude stars that are separated by 23 arc minutes. Although the separation is larger, they are both about 2 magnitudes fainter. Without the stargazing glasses, I only get the foggiest hint that there is more to Delta than just a single star. With the glasses, the two stars are distinct. If you get to a 6th magnitude observing site, give those stars a try and see what you can make out.

SubjectUrsa Minor
Date/TimeApril 20, 2006 - 10:00 PM MST (April 21, 2006 - 05:00 UT)
Observing Loc.Anderson Mesa, AZ
InstrumentNaked eye
ConditionsClear at first, then high cirrus, calm
TransparencyMag 6.8 (Based on HIP 81757)

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This page contains a single entry by Jeremy Perez published on April 20, 2006 10:00 PM.

73P/Schwassmann-Wachmann 3-B and -C - April 19, 2006 was the previous entry in this blog.

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