Book contents
- Front Matter
- Contents
- Foreword
- Opening thoughts
- Acknowledgments
- Part 1 Getting to know the sky
- Part 2 Getting to know the variables
- 5 Meeting the family
- 6 Getting started with Cepheids
- 7 Algol, the demon of autumn
- 8 How to estimate a variable
- 9 Names and records
- 10 Observing hints
- 11 Stately and wonderful
- 12 Stars of challenge
- 13 Bright, easy, and interesting
- 14 Betelgeuse: easy and hard
- 15 Not too regular
- 16 Nova? What Nova?
- 17 Supernovae
- 18 Three stars for all seasons
- 19 A nova in reverse?
- 20 RU Lupi?
- 21 Orion, the star factory
- 22 Other variable things
- 23 The Sun
- Part 3 Suggested variables for observation throughout the year
- Part 4 A miscellany
- Index
8 - How to estimate a variable
Published online by Cambridge University Press: 22 September 2009
- Front Matter
- Contents
- Foreword
- Opening thoughts
- Acknowledgments
- Part 1 Getting to know the sky
- Part 2 Getting to know the variables
- 5 Meeting the family
- 6 Getting started with Cepheids
- 7 Algol, the demon of autumn
- 8 How to estimate a variable
- 9 Names and records
- 10 Observing hints
- 11 Stately and wonderful
- 12 Stars of challenge
- 13 Bright, easy, and interesting
- 14 Betelgeuse: easy and hard
- 15 Not too regular
- 16 Nova? What Nova?
- 17 Supernovae
- 18 Three stars for all seasons
- 19 A nova in reverse?
- 20 RU Lupi?
- 21 Orion, the star factory
- 22 Other variable things
- 23 The Sun
- Part 3 Suggested variables for observation throughout the year
- Part 4 A miscellany
- Index
Summary
Z Ursae Majoris and the AAVSO method
A huge red giant, Z Ursae Majoris displays some unusual behavior in this late stage of its life. Although it usually ranges from magnitude 6.5 to 8.3, it occasionally surprises us. Once I watched it drop to 9.5 — more than a full magnitude below its normal minimum.
With the earlier starter stars we used a simple method where 1 represents the brightest and 5 the faintest. Now that we have some understanding of what the process means, we need not use it; now we are going to play the variable star game by the rules as outlined by the American Association of Variable Star Observers.
Look closely at the two charts (Figs. 8.1 and 8.2) for Z Ursae Majoris. Fig. 8.1 is designed for binoculars and has north up. Fig. 8.2 is meant for Newtonian viewing where the image is usually inverted. South is up, north down, and east and west are exchanged.
In Fig. 8.1 you recognize the Big Dipper, and near the top of the bowl is the circle-and-dot symbol for the variable star. Near other selected stars are numbers like 66, 54, and 64. These numbers represent magnitudes and tenths, but the decimal point is left out to avoid confusion with the other points that represent stars. Therefore, read “66” as “6.6” and so on. If you look at the area with binoculars, and are able to find Z and see that it is easily visible, then you can use Fig. 8.1.
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- Chapter
- Information
- Observing Variable StarsA Guide for the Beginner, pp. 28 - 32Publisher: Cambridge University PressPrint publication year: 1989