|Help and Advice|
|Transit of Mercury 2016|
|Giving long exposures on a digital camera|
|Photographing star trails|
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|Choosing a Telescope|
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|Photographing a partial eclipse|
A Cepheid variable star that varies in a very predictable way, going up and down in brightness every 10.15 days.
Zeta Geminorum is a yellow supergiant star whose variations are due to very regular pulsations in the star's outer layers.
This light curve combines all of the brightness estimates of Zeta Gem made by SPA VSS members during 2016.
For each observation, the phase (i.e. the fraction of the 10.15 day cycle) completed was calculated.
As can be seen, the light curve is fairly sinusoidal - the brightness rises to maximum at the same rate as that with which it fades back down afterwards.
In some ways, Zeta Geminorum is very similar to Delta Cephei. However, the shape of the above light curve is somewhat different from that of Delta Cephei. For Delta Cephei, the rise in brightness is steeper than the subsequent fall. The difference occurs because Zeta Gem pulsates in a different way from that with which Delta Cephei pulsates.
|Extreme brightness range||3.7 - 4.3|
|More typical range||Always the same brightness range|
|Period of variation||10.15 days|
|Frequency of observation||Worth checking on every clear night when Zeta Gem is well clear of the horizon and any haze|
Naked eye if you have a reasonably dark observing site
Otherwise, use 40mm or 50mm binoculars
|Visibility||Can be observed from late August to early May|
Here is a finder chart that will allow you to locate Zeta Geminorum:
As is the case for Delta Cephei, the brightness changes of this star can be followed with the naked eye if you have a reasonably dark observing site.
However, you may find it easier to use 40mm or 50mm binoculars if light pollution is a significant problem.
At maximum, Zeta Gem will be almost as bright as comparison star E.
At minimum, it becomes fainter than comparison star G.
Take extra care with your brightness estimates when Zeta Gem is low in the sky - try as far as is possible to use comparison stars that are at the same altitude above the horizon as Zeta Gem (otherwise, haze may dim the stars and thus introduce errors).