A small documentary style image showing the newly enlarging split of
Porrima A-B (gam Vir) now at around 1". Porrima B is now again
becoming accessible by small telescopes. This binary split is
discussed in Alan MacRobert's S&T note on page 68 of the June 2008
issue.
http://gallery.utahastronomy.com/main.php?g2_itemId=11377
Porrima was only at 38 degs alt at my op and seeing was Pickering 1 or
2. Because of this, an asthetic image was not possible. 83 short
0.125" exposures where taken of the atmospheric speckle pattern. The
two best images showing the split and the two components are included
in the posted image.
Visually, at 564x with a 16" apeture, Porrima AB, in moments of still
air, appeared as figure-8 pattern or a just-touching kiss split, using
Haas's 2006 split nomenclature.
My computed split of 1.4" has a high degree of uncertainty and, due to
observation error, is not in consistent with the S&T article predicted
separations of 1.0" on April 20th, 2008, increasing to 1.1" on Sept.
15th. It is not consistent with the 6th Orbit Catalogue ephemeris
split (rho) values of 0.91" for 2008 increasing to 1.168" in 2009.