Blogs / Dr.Bob's blog / The end of eclipse

The end of eclipse


Posted by Dr.Bob on May 28, 2011 - 12:20pm

The next few days mark the closest approach of the Sun to epsilon Aurigae, as part of the annual solar motion.  This also makes observations rather difficult, given the lingering twilight and the high airmasses involved.  At last report, epsilon appeared to be between 3.2 and 3.3 mag, visual.  This is behind schedule, relative to predictions based on prior eclipse light curves - epsilon Aurigae was predicted to have reached full brightness, mag 3.0, by mid-May 2011.  The evidence suggests that this portion of the disk may be less transparent than the corresponding ingress portion of the disk.

Relative to mid-eclipse, which occurred in late July 2010, circa JD 2,455,400, we are now ~310 days later.  The start of eclipse began approximately 350 days prior to mid-eclipse, so emergence from eclipse could be as late as late June/early July.  Over the coming weeks, anyone able to make a visual assessment or photometric measurement is encouraged to report their findings here at CitizenSky.org .

Photometry on 23 and 30 May

Using a digital camera and reducing to Johnson V with intermediate spreadsheet, of course including air mass correction, I got during nautical twilight: 2011 May 23.84 UT 3.27mag +/- 0,05mag 2011 May 30.85 UT 3.22mag +/- 0.09mag Here is the scene on one of the images on 30 May: http://flic.kr/p/9P119e Best regards, Wolfgang Vollmann, Vienna, Austria (VOL)

Cool

Very, very cool Wolfgang. The error bars are getting fairly large there, is that estimated from the errors in the coefficients or standard deviation of the data? Brian

Standard deviation

Hello Brian, this is the standard deviation of measuring 8 images. It is usually smaller, around 0.02-0.03mag but now Epsilon Aurigae is low and so it gets bigger. Best regards Wolfgang

Eps Aur 2011-06-02

My latest meassurment was 3.20 on June 2 23:06 UT, 8 images with a SD of 0.033. Before that I got 3.26 on May 20 22:41 UT. Both values seems to agree well with yours Wolfgang. Meassured witha DSLRwith correction for airmass and colorindex.

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