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Author: Tracie Heywood

T Cephei is near maximum

Tracie Heywood Variable Star news 15th May 20167th December 2017 0 Comment

The Mira type variable star T Cephei is currently near its peak brightness and is readily visible in binoculars.

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Eclipsing Binary Predictions : 2016 Apr-May

Tracie Heywood Variable Star news 3rd April 20167th December 2017 0 Comment

Here are predictions for eclipses that are reasonably favourable from the UK during April and May:

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Mira (Omicron Ceti) is brightening rapidly

Tracie Heywood Variable Star news 16th February 20167th December 2017 0 Comment

Omicron Ceti (Mira) has been brightening rapidly in recent weeks.

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Mira on the rise

Tracie Heywood Variable Star news 7th February 20167th December 2017 0 Comment

Omicron Ceti (Mira), having passed through minimum in late 2015, is now brightening towards its spring maximum.

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Eclipsing Binary predictions 2016 Feb-Mar

Tracie Heywood Variable Star news 24th January 20167th December 2017 0 Comment

Here are predictions, up to late March, for eclipses that are reasonably favourable from the UK:

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Z UMa and T UMa approaching maximum

Tracie Heywood Variable Star news 9th January 20167th December 2017 0 Comment

Two variable stars located near the ‘bowl’ of the Plough are currently approaching maximum.

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Catch R Leonis near maximum

Tracie Heywood Variable Star news 17th September 20157th December 2017 0 Comment

Alongside the sight of Venus, Mars and Jupiter in the pre-dawn sky, the constellation of Leo is also emerging from the morning twilight.

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Chi Cygni : heading for a bright maximum

Tracie Heywood Variable Star news 17th July 20157th December 2017 0 Comment

2014 was a disappointing year for observers of the variable star chi Cygni,… but 2015 is already much better!

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R Scuti is fading

Tracie Heywood Variable Star news 4th July 20157th December 2017 0 Comment

Recent observations indicate that the star R Scuti is fading into a minimum.

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R Serpentis heading for maximum

Tracie Heywood Variable Star news 1st July 20157th December 2017 0 Comment

The Mira type variable R Serpentis is now readily visible in binoculars as it closes in on its 2015 maximum.

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