I began a short observing session last Tuesday morning (12.05.09) by trying to split the well known double star Izar (also known as Epsilon Boötis) in the constellation of Boötes. Despite a hazy mist in the upper atmosphere conditions were fairly decent, but try as I might I just couldn’t separate the orange giant primary, and it’s smaller main sequence companion from each other. I was sure that a power of 166x would be up to the job, but obviously it wasn’t so perhaps someone can offer a little advice on the subject?
After about twenty minutes of fruitless scrutiny I decided to move on from Boötes to bathe in the radiance of my second morning target: Cor Caroli in Canes Venatici. The view through the 6mm plössl was delightful, but unexpectedly, and quite oddly the brighter A class primary shone with a greenish hue rather than the white or pale blue luminosity that I was anticipating. The secondary which is an F class star should have displayed a yellow iridesence, but instead showed no sign of colour.
Regardless of the perculiar spectral colours that I percieved this really was an attractive binary system to study, but I think it will be one that I will return to quite soon for a follow up observation.