October 9, 2006: To help provide a consistent style for my double star sketches, the above sketch is a digital update to the original sketch.
This doubly was very close to a brilliant star. The primary is orange. The secondary is white. PA appears to be 240Â° with a separation of 1′. The bright star to the east is yellow orange and about 8′ away. After checking the listed data, I have to say ‘oops’. It looks like the brilliant star to the east is actually the primary. With that being the case, PA in my sketch looks to be about 265Â° which is a lot closer to the listed value of 291Â°. Separation of 480″ in my estimate is a lot closer to the listed value of 378″. Still a pretty ugly estimate though. :-/
|Subject||Double/Multiple Star: Alpha Capricornii (STF 51)|
|Position||Capricornus [RA: 20:18:06 / Dec: -12:33]*|
|Date/Time||09/13/05 – 12:30 AM|
|Observing Loc.||Flagstaff, AZ – Home|
|Instrument||Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)|
|Eyepieces/Mag.||10 mm + 2X Barlow (240X)|
|Conditions||Clear, breezy, 55Â°F|
|Transparency||NELM Mag 4.8|
*Based on published data.