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Light curve for TX Dra since Janury 2015


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About this observation
Tracie Heywood
Time of observation
30/09/2017 - 21:00
TX Draconis
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Here is my light curve for the semi-regular variable star TX Draconis since the start of 2015. This is one of the more reliable semi-regular variables. During this interval, it has varied over the whole of its listed magnitude range of 6.8-8.2, pushing the lower limit at times. The catalogued period is 92 days. Being a semi-regular variable, it doesn't necessarily stick to this but the gaps between maxima have been mostly in this region.

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