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[vsnet-chat 258] Re: observing season of Mira (omicron Cet)
- Date: Thr, 24 Apr 1997 23:30:52 +2200
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Fraser Farrell <fraserf@dove.net.au>
- Subject: [vsnet-chat 258] Re: observing season of Mira (omicron Cet)
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
On 1997-04-19 b.h.granslo@astro.uio.no said:
>The longest Mira season (349 days) occurs at lat. 54.5 deg. S.
Not much land at that latitude, or clear nights. A friend of mine who
has worked extensively on sub-Antarctic islands says you can wait weeks
to get a glimpse of the Sun, never mind stars!
>In order to observe Mira for as long as possible it is of course
>necessary to have a transparent atmosphere and an unobstructed
>view in the appropriate direction.
Late March and April skies here are typically either: (a) cloudy & wet,
due to approaching winter, or (b) hazy, due to dust blowing from
drought-stricken farms. May is effectively the start of winter too.
>In addition, it is important to correct brightness
>estimates for extinction when the star is very low in the sky.
Now _that_ is the hard part. Cloud coming off open ocean at night is
hard to detect, and it can move in within minutes around here.
This reminds me of a Sky & Telescope article I read some time ago,
concerning the number of bright stars visible from various latitudes.
Has anyone done the same calculation for GCVS objects?
cheers,
Fraser Farrell
http://vsnet.dove.net.au/~fraserf/ email: fraserf@dove.net.au
traditional: PO Box 332, Christies Beach, SA 5165, Australia
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