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Hello all,
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<div>The estimates of brightness for this object - visual and CCD - between 3rd and 6th July are very interesting. Erik Bryssinck, whose 4th July CCD data you can see on his image via the BAA archive, is very similar to mine - across the range of aperture sizes.
Basically we determined the comet to be just shy of mag 11, which is closer to trend. Let’s hope more data comes out.</div>
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<div>David Swan<br>
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On 3 Jul 2018, at 22:07, Shanklin, Jonathan D. <<a href="mailto:jdsh@bas.ac.uk">jdsh@bas.ac.uk</a>> wrote:<br>
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<p style="margin-top:0;margin-bottom:0">Although there is talk of 2017 S3 being bright because of an outburst, it may just be brightening a little more rapidly than expected. Observers are suggesting that it is diffuse, yet for a recent outburst it should
be well condensed. I'll need some more observations before making any predictions, but I might be prepared to get up early at the beginning of August. The comet is not well placed at perihelion or afterwards.</p>
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<div class="PlainText">Regards,<br>
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Jonathan Shanklin</div>
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