| 50°N | 30°N | 10°N | 10°S | 30°S | |
| 2013 March - 2014 May |
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| 2013 June - 2014 August |
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Ephemerides for 2012 S1 (ISON) at
50°N ,
40°N ,
30°N ,
10°N ,
10°S ,
30°S and
50°S which give 1950 and J2000 positions and approximate observing windows for the period
2013 February 23 until 2014 August 31.
The light curve is a complex function of the comet's composition, shape, active area, rotation
rate and season. I have chosen to approximate the
magnitudes using the equation m = 5.3 + 5 log d + 7.5 log r. The comet may brighten
more slowly or more quickly than indicated here and the true light curve can only be
determined
after observations confirm the comet's behaviour.
Projected light curve. Note:
a) The error bars are huge. The perihelion brightness can take just about any
value.
b) On any reasonable projection of brightness increase the light curve will be
fairly flat at the moment. It is therefore not possible to make definitive
statements about the comet's current performance.
c) The fitted curve appears above the observed points as it has been corrected for
aperture in order to predict the naked eye brightness.
There was a joint Asteroids and Remote Planets Section and Comet Section meeting on 2012 October 6. This was held in Milton Keynes and included discussion of Rosetta. For the meeting notes see The Comet's Tale for 2012
There is a Comet Section meeting on 2013 May 18 to discuss observing techniques.
We hope to obtain EU funding to support a pro-am European meeting prior to the Rosetta encounter.