This kind of stuff never gets old! A crisp Sunday morning, a cup of hot coffee, and a glorious sunrise with our friends Venus, who is a morning planet now after passing through inferior conjunction,, and of course a waning crescent moon.
Spring hasn’t quite sprung yet up here on the Hill. This morning the temp didn’t quite break 30 degrees. Strange patch of high humidity came through last night and when I checked the scope after last night’s session there was frost on it! Had to throw out about 75% of the images as a result. But, we did get one hour’s worth of new data on a new imaging project, the galaxy pair M81 and M82. I have never actually imaged these together before. Looking forward to the finished result! Then to top it off I found one of this month’s binocular bright comets, PanSTARRS, making its way through Aquarius now. I caught a glimpse of it about an hour and half before sunrise. Not enough time to do a full imaging sequence but enough to see a tail! Comet Lovejoy, supposedly more impressive is just too low now for me to get a good look at it. We’ll have to revisit these next month perhaps!
Comet PanSTARRS (C/2015 ER61) just passed closest to Earth on April 19 at 109.5 million miles. It should continue to brighten up until May 10 when it reaches perihelion, closest to the Sun. This is just a 1 minute single frame uncalibrated luminance image taken with the 5″ refractor
New project! The galaxy pair M81, M82 are part of the “M81 galaxy group”. There is a third galaxy, NGC 3077 which is interacting with the other 2 gravitationally but not in this field. The interactions have stripped away hydrogen gases from all 3 forming intergalactic filamentary structures called the Integrated Flux Nebula, I hope will be revealed in the final image. This is a single raw uncalibrated 6 minute luminance image taken with the 5″ refractor. Note the vertical lines through some of the stars. This ccd is very sensitive and what is called non-antiblooming, meaning that for these stars the charge in these pixels have exceeded the saturation level and then start to fill adjacent pixels. The sensor is designed to allow for vertical shifting of charge but not horizontal. So yes, this is kind of an “accepted inconvenience” , which has to be processed out of the image at some point, in exchange for higher quantum efficiency and data preservation but perhaps a topic for another day!
Thanks for reading!
Ok, well not so new today, but it was discovered a couple of days ago in the “nearby” galaxy M82. This is a popular target among amateur astronomers. Full details: http://www.universetoday.com/108386/bright-new-supernova-blows-up-in-nearby-m82-the-cigar-galaxy/
Even more remarkable is that several observers have been able to obtain spectra of the supernova with the popular low resolution grating called “Star Analyser” which I happen to own, but haven’t been able to set it up as of yet! Probably even at magnitude 11 it is too dim for my refractor, and my 10″ scope is now tied up with the M1 project. What is now possible with modest amateur equipment regarding spectroscopy is quite remarkable! http://www.insideastronomy.com/index.php?/topic/1520-supernova-in-m82was-cloudy/#entry7607