The goal of splitting the double star, Antares, has been tempting me for a while. I never have the sort of seeing conditions that would make it a nice clean observation. So I gave it a try on this less-than-perfect evening, and was successful in spotting the secondary star. Antares’ primary star flickered like a coppery flame in the jumping air currents, so I had to be patient and wait for the ripples of diffracted light to show me the way. The secondary began to coalesce as a consistent lump in the fluttering kidney beans of orange light near the position of the primary star’s second diffraction ring. It’s color was hard to pick up, but gradually, I perceived what looked like a yellow-green tint. I had not checked data on the secondary’s current position angle to help keep me honest, and it looked to be at a PA of about 280 degrees. Checking Brian Workman’s double star calculator a couple days later gave a PA of 277Â° for 2007.5. The separation comes out to 2.18 arcseconds, which is about right for my ‘second diffraction ring’ sighting–that works out to 2.5 arcseconds in my scope.
I wanted to convey what the diffraction pattern looked like, and how the secondary appeared in the midst of it. The digital sketch I prepared was a bit of a learning experience for me, but I think it does a halfway decent job of rendering what I saw. This can be seen in the detail portion of the sketch. Just imagine all of that jumping around and moving from moment to moment. Clicking the sketch will provide a larger image that is easier to see. You’ll notice that I was fortunate enough to have the spider vanes in a position that didn’t interfere with the secondary star. It really was a beautiful and challenging sight. Give it a try sometime and see if you can identify the secondary in that bubbling mass of starlight.
I’d love to see what they look like under near-perfect seeing.
[Edit June 8, 2012]: Updated digital sketch to match current double star style.
|Subject||Alpha Scorpii (Antares / GNT 1)|
|Position (J2000)||Scorpius [RA: 16:29:24.4 / Dec: -26:25:55]*|
|Position Angle*||277Â° (2007.5)|
|Magnitudes*||0.96 / 5.4|
|Spectral Types*||M1.5 IB E / B2.5V|
|Date/Time||MAY 11, 2007 – 11:35 PM MST (MAY 12, 2007 – 06:35 UT)|
|Observing Loc.||Anderson Mesa, AZ|
|Instrument||Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)|
|Eyepieces/Mag.||10 mm + 2X Barlow (240X)|
|Conditions||Mostly clear, calm|
|Transparency||NELM Mag ~6.0|
|References||The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996); 12th General Catalogue of MK Spectral Classification (Buscombe+ 1995); Brian Workman’s Double Star Calculator|
*Based on published data.